n Ъ5CE2сј€џђ; Ў/+ s€џџџџџџџ47 Ursae Majoris is 47 [G/light year]s away and is 1.7 times more [G/luminous] than the Sun. The [G/planet] in orbit around this [G/star] is believed to be 2.4 times more massive than [G/Jupiter] and it circles the star once every 3 years. The planet lies approximately 2.1 [G/a.u.] from its star, which would put it just past [G/Mars] in our [G/solar system]. џ16 Cygni B is 72 [G/light year]s away and is 1.4 times more [G/luminous] than the Sun. The [G/planet] in orbit around this [G/star] is believed to be 1.7 times more massive than [G/Jupiter] and it circles the star once every 2.2 years. The planet lies approximately 1.7 [G/a.u.] from its star, which would put it just past [G/Mars] in our [G/solar system]. џ70 Virginis is 59 [G/light year]s away and is 3 times more [G/luminous] than the [G/Sun]. The [G/planet] in orbit around this [G/star] is believed to be 6.8 times more massive than [G/Jupiter] and it circles the star once every 117 days. The planet lies approximately 0.5 [G/a.u.] from its star, which would put it just past [G/Mercury] in our [G/solar system]. џRho Coronae Borealis is 57 [G/light year]s away and is 1.8 times more [G/luminous] than the [G/Sun]. The [G/planet] in orbit around this [G/star] is believed to be almost equal to the mass of [G/Jupiter] and it circles the star once every 40 days. The planet lies approximately 0.2 [G/a.u.] from its star, which would put it much closer to its star that [G/Mercury] is to our Sun. џRho Cancri is 44 [G/light year]s away and is 0.6 times more [G/luminous] than the [G/Sun]. The [G/planet] in orbit around this [G/star] is believed to be 0.9 times as massive as [G/Jupiter] and it circles the star once every 15 days. The planet lies approximately 0.1 [G/a.u.] from its star, which would put it much closer to its star that [G/Mercury] is to our Sun. џUpsilon Andromedae is 57 [G/light year]s away and is 5.5 times more [G/luminous] than the [G/Sun]. The [G/planet] in orbit around this [G/star] is believed to be a little over half the mass of [G/Jupiter] and it circles the star once every 5 days. The planet lies extremely close to its star, at a distance of only 0.05 [G/a.u.]. For comparison, [G/Mercury] lies 0.39 a.u. from the Sun. џ51 Pegasi is 50 [G/light year]s away and is 1.3 times more [G/luminous] than the [G/Sun]. The [G/planet] in orbit around this [G/star] is believed to be about half as massive as [G/Jupiter] and it circles the star once every 4 days. The planet lies extremely close to its star, at a distance of only 0.05 [G/a.u.]. For comparison, [G/Mercury] lies 0.39 a.u. from the Sun. џTau Bootis is 49 [G/light year]s away and is 4.0 times more [G/luminous] than the [G/Sun]. The [G/planet] in orbit around this [G/star] is believed to be over 3.5 times more massive than [G/Jupiter] and it circles the star once every 3 days. The planet lies extremely close to its star, at a distance of only 0.05 [G/a.u.]. For comparison, [G/Mercury] lies 0.39 a.u. from the Sun. џHD 217107 is 13 [G/light year]s away. It has been shown to have a planet that is 1.3 times more massive than Jupiter. This planet orbits the star every 7.1 days. It's orbit is only 0.07 [G/a.u.], this is one tenth the distance to Mercury. џHD 13445 is 36 [G/light year]s away. It has been shown to have a plenat orbiting it that is 5 times as massive as Jupiter. This planet orbits the star ever 15.83 days at a distance of 0.11 [G/a.u.]. џBeta Pictoris: Through a telescope, this [G/star] appears as a typical pinpoint of light. It is slightly larger than our [G/Sun], 58 times more [G/luminous], and 140 [G/light year]s away. The interesting part about Beta Pictoris showed up during an observing session with the [G/IRAS] satellite. [G/Infra-red] images revealed a clump of cool matter in orbit around this star, possibly the beginnings of a planetary system. This cool mass is only visible using infra-red imaging. Through a small telescope, look for a pinpoint of light. џAlpheratz represents the head of [X/Andromeda]. It is approximately 100 [G/light year]s distant and 160 times more [G/luminous] than our [G/Sun]. Alpha CV 2.02 - 2.06V, 0.9636 or 0.966222d. Some spectral lines vary same period, others half period, some nonvariable џALPHERATZџAlp AndџDelta Sct, amp. 0.03V, 0.10101d. џCaphџBet CasџBeta C 2.80 - 2.87V, 0.1517495d. џALGENIB.џGam PegџLb 4.26 - 4.46V. џAE CetџComponent B, 12.87v at 63", optical. 3.46 - 3.56V. џDeneb Kaitos Sheџ2.75 - 2.81V. џANKAAџCPM with HR 127 of which both are close binaries. Also CPM with HR 136. Faint companion at 14". џAlpha Cyg, 4.22 - 4.30B, 0.09028d. џKap Casџ3.59 - 3.68V. џAB CPM. Component C, 15.2v at 48" optical. џD is 8.5v K2IV-V, vsini <54k/s. All components probably optical. Cst 2.20 - 2.27V. џSHEDIRџAlp CasџDiphda is a slightly reddish star a little over 50 [G/light year]s away. I is approximately 40 times more [G/luminous] than our [G/Sun] 1.96 - 2.11V. џDIPHDAџAB CPM. Companions probably optical. Component A of visual system, EB 3.92 - 4.14V, 17.7695d. џZet AndџAB 3.45 G3V, 7.51 K4Ve, 480y, a = 11.994". Combined mag., colors. Component B, vsini =<25k/s. Companions C-H optical A possible invisible companion with period about 40y. Component B, 7.51V, +1.39(B-V), +1.03(U-B). џAchird, accordinџAB CPM. IRAS observations confirm IR excess and yield simple blackbody temperature of 6750 +/- 100K. ADS 782A, Gamma Cas 1.6 - 3.0v. Spectrum and color vary. Expanding circumstellar shell. High-velocity variable mass loss. Variable hydrogen emission, 0.7d. Variable SiIV, CIV, polarization. Variable X-ray source. H alpha indicates rotating disk-like envelope. џGam CasџAll components optical. џPossible periodicities: 19.4, 16.7, 0.95, 0.49d. џSuspected occultation double, 5.2, 5.2v, sep. 0.25". џA* 5.15 G5Vp, 21.43y, a = 0.186", mag. diff 2V, sep. 1.4". Subdwarf with five visual and one astrometric components. џMarfak. Name shџDhenebџinterferometry 1983.93, sep. 0.64". џMIRACHџPrimary component of visual system. EA 3.92 - 4.42V, 1.6697664d, i 84.7d. џZet PheџDelta Sct? џMarfak. Name shџCPM with HR 362 at 24". ADS 996A is close occultation double, 6.3, 6.3v, 0.05":. Component B, HR 362 is SB; C, 12.2 i 1" from B. џProbably optical. џUnresolved by speckle interferometry 1981.69. EA? 2.68 - 2.76V, 759d. џRuchbahџDel CasџA* 2.0 var. F8Ib, 30.46y, a = 0.038". AB physical; B, 8.20V, +0.49(B-V), +0.16(U-B), F3V, 0.0 color excess, vsini =<60k/s; C, 13v at 43"; D, 14v at 83". Polaris is the star currently aligned with Earth's north [G/Celestial Pole] It is only the 49th brightest star in the sky. Polaris is actually a doubl star system, made up of two faint stars that are 465 [G/light year]s away CDelta 1.92 - 2.07V, 3.969778d. Period increases 53 sec./century. Probably unreddened. џPOLARISџAlp UMiџ3.39 - 3.49V. џGam PheџCPM. ADS 1199B, 8.0 - 11.5v? џBoth visual companions probably optical. џAchernar is hot, blue giant star that ranks as the 9th brightest star in the sky. It is approximately 125 [G/light year]s distant and 650 times more [G/luminous] than our [G/Sun]. EB or Ell, amp. 0.02V. H alpha var. emission and possible high-velocity mass loss. Expanding circumstellar shell. џACHERNAR.џBinary with HR 487, q.v. џK1V, K1.5V. џGamma Cas 4.03 - 4.11V, 19.5d. Amp. varies in per. 127d. Possible mass loss. Expanding circumstellar shell. џPhi PerџTorcularis SepteџSecond visual component optical. џBaten Kaitos.џMetallahџDelta Sct? џSharatanџSR 4.3 - 4.5V, 30d. џPsi PheџCPM. џBinary with HR 596, q.v. Alpha CV? џAlpha CV?, 3.79 - 3.83V. Although the NSV identifies the variable as HR 596, the magnitudes given are for the blend o HR 595/6; uncertain which component is the variable. џAlrishaџCPM with HR 604. џALMAAKџHamal, the brightest star in [X/Aries], lies 67 [G/light year]s away and i 70 times more [G/luminous] than our [G/Sun] џHAMALџSuspected occultation double, sep. 0.012". E?, 4.35 - 4.38V. џCompanion G2V? џMira is a pulsating, variable, red giant star which changes in brightness fro [G/magnitude] 3 to magnitude 9 over the course of 331 days. It i approximately 135 [G/light year]s distant AP var. M7IIIe, var. dBe, 400y, a = 0.85". The faint companion was first predicted in 1920 by Joy on the basis of a slightly displaced blue secondary spectrum. First seen by Aitken in 1923. Visible only when Mira is faint. Light variations on scale of hours superimposed by variations of 10-15 min. and rare flares of 2 min. duration. Components B 13v at 73" and C, optical. Two variables: Mira and VZ Cet. Mira, ADS 1778A, M 2.0 - 10.1v, 331.96d; var. CO emission from circumstellar envelope. Speckle interferometry indicates large abrupt variation of diameter as a function of wavelength. Hydrogen lines vary o time scale of 1-2 days. Mira was discovered to be variable by Fabricius in 1596, the first such variable discovered. ADS 1778P, Ne "Novoides" class, VZ Cet, 9.5 - 12.0v, dBe. џMIRA.џOmi CetџVisual companion 11.7v dM6 at 165", CPM. A* 5.84 K3V, 60y, a = 0.257".. Mass of invisible companion 0.12 solar. Companion at 2" probably about 5v fainter. Unresolved by speckle interferometry. џBeta C 4.05 - 4.10V, 0.16113668d. Per. changed 1965, then increased about 0.7 sec./century. џDel CetџAB 4.13 F7V, 9.87 M1V, 2720y, a = 22.289". C probably optical. џAB binary, combined mag., colors. CPM with BD+2d418, 10.2v M6 at 840". џKaffaljidhmaџOccultation binary. Combined mag., color. Delta Sct? џComponent B, B9V, CPM, vsini 149k/s. џMiram in BecvarџOptical system. џDelta Sct? џA* 4.06 G4III+A4V, 4.150y, a = 0.050". Speckle interferometric sep. 0.080" 1981.67. Circumstellar material surroundin the pair? Visual companions 10.7v at 51" possibly physical; 11.8v at 4" possibly optical. EA, 3.94 - 4.07V. џTau PerџM 4.7 - 14.3v, 401.5d, JD2412800-28900; later 407.6d. џR HorџAzha.џBinary with HR 898. Uncertain which component var. Combined mag. HR 897/8, 2.91V; combined colors, +0.125(B-V), +0.13(U-B). џACAMAR.џLb? 2.45 - 2.54V. Spectrum var. џMENKARџAlp CetџSKYLAB observations indicate cool star with hot companion. Components Aa, 14.65y, a = 0.159". Physical nature of B, 11m at 57", uncertain. Close to error box of X-ray source 3U0305+53. џSRb 3.30 - 4.0V, about 50d with possibly slow var. in mean brightness in 1100d period. џGorgonea Tertia.џRho PerџAlgol is an eclipsing variable star, meaning the light from this star appears to brighten and fade as its companion star passes in front of the star and behind it. The star's [G/magnitude] changes in brightness from mag. 2.1 to mag. 3.4, over the course of 2.8 days. Algol is approximately 100 [G/light year]s distant. A* var. B8V, 1.858y, a = 0.011" or 1.862y, a = 0.104". Apparent apsidal period 28.4y or 32y. Resolved by speckle interferometry: sep. 0.086", 2-3v fainter than primary. This may be Algol C. Four visual companions all optical: B, 12.7v at 59"; C, 12.5 at 67"; D, 10.5 at 82"; BC sep. 15"; E, 12.5v at 11" from D. One of the few known galactic radio sources in which the dominant star is normal. 21cm radio source. ADS 2362A is the prototype Algol star, first discovered as variable by Montanari in 1669. The first period determined b Goodricke in 1783, who also interpreted the variations as due to eclipses. The prototype star proves to be a more a complicated system than most of the Algol-type stars, i.e., compact triple system with separation of the components well under 0.1". The components usually designated Algol A, B, C, sometimes A, a, P. Two formerly additionally desig nated components D and E, inferred on the basis of an apparent 32 year apsidal motion, are now considered spurious. The various Algol components must not be confused with the visual components ADS 2362 B-E, optical companions at much greater distances from A. ADS 2362A, EA 2.12 - 3.40V, 2.86732442d, abrupt period changes. Orbital and rotation period synchronized. Rotational velocity 65k/s. Radio flares extending to about 1 A.U., not associated with X-ray activity. Radio flare activity appears correlated with period discontinuities, attributed to "starquakes." Mass flow from K to B component at rate of 1.8x10E-08 solar masses/year. Possible circumstellar material associated with radio or H alpha emission. џALGOLџBet PerџCompanion optical. џBotein.џ3.9 F8IV, 6.5 G7V, 314y, a = 4.367". Combined mag., colors. ADS 2402B, 7.0 - 9.03v. џFornacisџAB binary, B is K0V. C, 11v at 40" optical. Lb? 3.57 - 3.72V. џTau4 EriџMIRPHAKџH alpha profile var. џAstrometric binary, 25y. Unresolved by speckle interferometry. џAmp. 0.04V, 0.5d. Hydrogen emission variable. Expanding circumstellar shell. џPsi PerџCPM? Position angles disagree by about 40d. џAlpha CV? 2.98 - 3.03V, about 1d. Strong variable emission at 1650A, CaII? џDel PerџBinary. Combined mag., colors. Rotational velocity B, 150:k/s. Unresolved by speckle interferometry 1982.16. In interstellar ultraviolet radiation field. Ell 3.79 - 3.85V, 4.419171d, possibly half. џAtikџOmi PerџRana in Becvar. But see HR 188. RS:, 3.51 - 3.56V, about 10d. џDel EriџSep. 0.062". Occultation of 1972 Mar. 19 indicated mag. diff 3.4, sep. 0.010". џElectra.џPrimary is SB, 4.6, 6.1v, sep. 0.012". Visual pair 4.4, 8.1v, sep. 69". џTaygetaџSep. 0.003". Unresolved by speckle interferometry 1981.69. Duplicity questioned. Probably cst. Var. helium lines. џMaia.џLc 4.35 - 4.48V, amp. 0.12p. џBE CamџVariable hydrogen emission. џMerope.џV971 TauџLb? 4.38 - 4.44V. џPi EriџComponent A is occultation double, sep. 0.031". B, C, D, 8.1 A0V, 8.1 Am(A5/F0/F2) and 8.7v F2V at 117" to 190". Possibly second occultation companion at 0.001", unresolved by speckle interferometry. vsini of B 155k/s. Numerous photometric determinations yield 6.3 for B component. The HD gives 8.1 for 23629 and the IDS indicates 8.1. Burnham, Double Stars, gave 7.0 vis. џALCYONE. The briџComponent A SB, 4.1, 5.6, sep. 0.006" and 0.019". B, 6.8v at 0.4". џAtlas.џAB CPM, B 9.16V B8IV; C, 9.12V at 33" optical; D, 10.35V, +0.713(B-V), +0.20(U-B), at 92" optical; E, 9.90V, A2V, +0.33(B-V), +0.17(U-B), at 120" physical. 2.80 - 2.93V. џAB CPM. B, 7.39V, -0.03(B-V), -0.52(U-B), B9.5V, vsini 300:k/s. Beta C, 2.88 - 3.00V, 0.216:d. Brightest component on visual triple. Photoelectric and spectroscopic resonant period found are submultiples of 26.9 hrs or 1.12d. џEps PerџSlightly variable, possibly same period as SB. џMenkibџXi Perџ2.88 - 2.96V. џZaurakџGam EriџEA 3.3 - 3.80p, B3V+A, 3.952955d, i 86d. џLam TauџGamma Cas 4.00 - 4.10V, 55?d. Slow var. possibly associated with emission spectrum. џMX PerџDelta Sct 4.00 - 4.05V, 0.0815d. Secondary per. 0.1291d. џBeid.џOmi1 EriџA* 4.13 G0Ib, 0.778y, a = 0.019". AB CPM; B, 11.8v at 15". C , 10.25V, +0.47(B-V), +0.06(U-B), B8. ADS 3071A, 4.1 - 4.24V. џBC 9.51 A2, 11.18 M4Ve, 252.1y, a = 6.943". Component B is white dwarf. Component A, CPM. ADS 3093C; UV, min. 11.18V, +1.50 (B-V), 12.16 - 13.85U. X-ray source. џKeidџDY EriџEW? or Delta Sct? 4.23 - 4.27V, per. between 0.33 and 1.0d. џGam DorџAmp. 0.1V. џHyadum I.џSmall amp., possible periods 0.96, 1.93, 8.5, 0.89d, with 8.5 slightly favored (Manfroid and Mathys 1985, A&AS, 59, 429). џAmp. 0.1V. џHyadum II.џKappa1 Tau is occultation double. Together with Kappa2 = HR 1388 they form a multiple system of at least 6 components. Delta Sct? џAB binary; C, 11v at 77" CPM. A blue straggler. Amp. 0.02U, 57.25d. Also magnetic field period. џV776 TauџThe visual primary is SB, 4.6, 6.5v, sep. 0.020". Component B, 12.5v at 110". џSome sources calџUps TauџV777 TauџAinџCPM with HR 1412. Not clear if there are one or two occultation companions: mag. diff 3.8v, sep. 0.082", another possible mag. diff 8v, sep. 0.2". џDelta Sct, amp. 0.03V (variable), 0.080d. Possibly also eclipsing. џThe2 TauџA* 4.27 G8II+B, 28.67y, a = 0.054"(not confirmed). џKnown as the "red eye of the Bull'" Aldebaran is a red giant star, 40 times Larger than our Sun. It is approximately 68 [G/light year]s distant and ranks as the 13th brightest star in the sky. AB binary. B is 13.5v, dM2 at 31". CD, 122" from A is 11.2, 13.6v sep. 2" also binary but independent of AB. Lb 0.75 - 0.95V. Var. H and K emission. џALDEBARANџAlp TauџADS 3317A, E?, 4.23 - 4.30V. џBeta C 3.4 - 3.60p, 0.17790414d, changing. Probable interference periods 0.1779 and 0.1735d with beat period of 7.0256d. Possibly also E, 103.9d. џNu EriџEri, or HR 1143,џAlpha CV 3.26 - 3.30V, amp. 0.10u, 2.943d. џAlp DorџSceptrum.џSeen as double only in 1877 and 1923. SRb 4.28 - 4.36V, 30d. џDM Eriџ4.9, 6.4 sep. 0.0005". џCPM. Comp. A of double, Delta Sct? џDelta Sct? Amp. 0.05V. џEll 3.66 - 3.73V, 3.700363d. џPi5 Oriџ4.0 - 4.15p. џHassaleh in BecvџADS 3605A. A* 2.98 var. A8Iap. Five visual and one astrometric components. AB visual binary, B, 14v at 29"; C, 11.26V, +1.83(B-V), +1.31(U-B), at 43"; D, 12.0v at 46". ADS 3605A, EA 2.94 - 3.83V, 9892d. Spectrum var. even outside eclipse. RV and light fluctuations about 110d. џAl AnzџEps AurџEA 3.70 - 3.97V, 972.164d, i 90d. Variable duration of min. Amp. depends on wavelength, 0.55B, 1.97U. K component amp. 0.05V. џHaediџZet AurџBeta C? џHoedus II. One oџCursaџCandidate for becoming a Be star. Beta C 4.22 - 4.34V, 0.701538d. Both spectroscopic and new photometric data suggest period 0.70177d. Small changes i mean brightness (<0.1mag). џLam EriџCPM companion G8Ve, strong lithium. џAlpha CV 2.97 - 3.41V, per. about 2d. џMu LepџCapella is a bright binary star system whose two stars, only 70 million mile (116 million km) apart, are too close together to be seen as individual point of light with a small telescope. This star system is approximately 4 [G/light year]s distant AP 0.6 G5III, 1.1 G0III, sep. 0.04", 0.285y, a = 0.054", masses 2.67 and 2.55 solar. Combined mag., colors. Capella i first star for which an orbit was determined from interferometer measures, by Anderson at Mt. Wilson in 1920. Speckle sep. 0.040" 1981.24 and 1981.68; 0.055" 1982.16. CPM with component H, a close binary, 10.0 dM1, 13.7 dM5 sep. 2" at 723" from A, probably physical with A. Other components all faint and distant from A. Amp. 0.03V. Variable helium and X-ray emission. џCAPELLAџThe bright blue giant star, Rigel, represents one of [X/Orion]'s feet. I is an extremely hot star, with a surface temperature over 7,000 degrees hotte than that of our [G/Sun]. As a result, it is over 57,000 times mor [G/luminous] than our star AxBC, CPM. BC binary, 7.6 B8II, 7.6v sep. 0.12". D, 15.4v at 44". BC also classified B5V+B5V. For B, vsini =<39k/s. 0.03 - 0.30V, 25d. Amp. at 0.58 micrometers about 0.06m. џRIGELџADS 4002A is SB triple system, abc with periods 9.2y and 7.989d. Speckle interferometry gives 9.219y, a = 0.036" for for ab x c. Visual components AB, binary, 3.8, 4.8v, sep. 1.650"; C, 9.4v at 115". The total mass of the quintuple system exceeds 50 solar masses, the most massive component being about 17 solar masses. EA + Beta C 3.31 - 3.60V, 3.14 - 3.35B, 7.989268d. Also sinusoidal pulsation period, amp. 0.05V, 0.30197 or 0.30145d. џEta OriџBELLATRIXџALNATHџAB binary; C, 12.0v at 64"; D, 10.5 at 206"; E, 10.5 at 241". ADS 4066B, 7.0 - 11.0v. џNIHALџ4.49 B5IV, 5.82 B7V, 586y, a = 1.293". Combined mag. and colors. џSRc 6.1 - 6.5p, 165d. џCE TauџBinary with C = HR 1851. Component B, 14.0v at 33". ADS 4134A, EA 2.14 - 2.26V, 1.94 - 2.13B, 5.732476d. Intrinsic variability also possible. џMINTAKAџDel OriџARNEB.џA,B,C fixed. B is HR 1880. Colors for combined light. Blended mag., 3.39V. C is 11.2v at 29", optical; D, 11.2 at 78". Uncertain which of HR 1879 or 1880 is the variable suspect. џMeissaџAB fixed. B is B7IV; vsini 50k/s. Component B is NSV 2334, 7.4V. џNair al SaifџAlpha Cyg 1.64 - 1.74V. џALNILAMџEps OriџGamma Cas 2.90 - 3.03V. Var. shell Sp. Widths H-lines vary in about 10 min. Polarization at H beta changes in tens of minutes, probably due to circumstellar matter. џZet TauџCDelta 3.46 - 4.08V, 9.84200d. Period varies. џBet DorџAB 4.1 O9.5V, 5.1 B0.5V, 170y, a = 0.247". Combined mag. and colors. C, 8.79V, A2V at 11" may be physical; D, 6.62V, -0.20(B-V), B2V, at 13" and E = HR 1932, at 42" CPM with A. A multiple system similar to trapezium. ADS 4241 possibl the most massive visual binary known, 35 solar masses. џAB 1.88 O9.5Ib, 4.02 B2III, 1508.6y, a = 2.728". Colors for combined light. Blended magnitude 1.76V, 18 and 6 solar masses. B is HR 1949. C is 9v at 58", possibly physical. In line of sight of high-velocity interstellar cloud. ADS 4263. Uncertain which component, HR 1948 or 1949, is the variable suspect. џALNITAKџIn line of sight of high-velocity interstellar cloud. џGamma Cas?, 2.62 - 2.66V. H alpha variable. Rapid variations in H beta profile. џPhaetџCPM with HR 1983. C, 11.0v at 45". џSAIPH.џCompanion optical. џWeznџPossibly triple system. Magnitudes of separate components unknown. A*, 14.25y, a = 0.095". Probably low-mass companion. џThis huge star, possibly the largest known today, is a irregularly pulsating red supergiant. Its size changes from 550 to 920 times the diameter of our [G/Sun] over the course of 5 1/2 years. At its largest, this star would completely fill our inner solar system and its surface would be extremely close to Jupiter! Betelguese is 650 [G/light year]s distant. Components B-E all 11 to 14.5v at sep. 40" to 174" from A. D 13.5 at 77", optical. Speckle interferometric observation in 1983 November (Karovska et al. 1986, ApJ, 308, 360) show A to be a triple system with closer companion at 0.06" (mag. diff. 3.4 at H alpha) and more distant companion at 0.51" (mag. diff. 4.6 at H alpha). Radio star. Circumstellar shell of gas and dust. The gas shell detached from photosphere at about 5 stellar radii. Dia of optically thin dust shell possibly 1".5. Surrounded by reflection nebula. Gas shell up to 100 R, dust shell from 12 to 250 R. Highly limb darkened. ADS 4506A, SRc 0.40 - 1.3V, 2335d. Also superimposed waves 200-400d. џBETELGEUSEџAlp OriџAB binary. C, 14.1v at 13". ADS 4556A, EA 1.89 - 1.98V, 1.93 - 2.02B, A2+A2, 3.9600421d, i 78.5d. џMenkalinanџBet AurџRadio star. Lc 4.24 - 4.34V. Radio emission at 2.85cm indicates mass loss. џPi AurџAB binary , combined mag., colors. B is 7.2v G2V. C, 11v at 49" optical. ADS 4566B. Alpha CV 2.62 - 2.70V. Amp. 0.43m at 1400A, 1.3735d. Magnetic field varies 3.618d. џThe AurџAB 4.4 A2V, 6.0 F3V, 17.5d, a = 0.276"; ABxP, 18.25y, a = 0.089". Magnitude and colors for combined light. A is alpha CVn var., SB1, 4.45d; B is SB2, 4.78d. Component C, 14v at 18" probably optical. ADS 4617A, Alpha CV 4.10 - 4.18V. џAB 4.7 G6III, 5.1 G8III, 13.17y, a = 0.19". Combined mag., colors. Component A is SB, 4.9, 6.9v, sep. 0.0013". Speckle interferometric sep. 0.128" 1982.17, 0.086" 1983.93. Component C, 13.0v at 101". џPropus, a name mџAB, 473.7y, a = 1.08". B is 8.8v at 1.4". A is suspected occultation double, 3.4, 5.4v, sep. 0.03". Masses A, 12.4; B, 5.5 solar. The three components are surrounded by a gaseous envelope. ADS 4841A, SRa + EA 3.15 - 3.9v, 232.9d. Deepest min. satisfy SB period 2984d. џPropusџEta GemџE: + Delta Sct: 4.43 - 4.73V. Line widths vary 0.3d. џUZ Lynџ5.4 - 5.47B. џBeta C? џFurudџLb 2.76 - 3.02V. џTejat PosteriorџMu GemџBeta C 1.93 - 2.00V. Prototype star. Multi-periodic: 0.25002246, 0.2513003, 49.17 and 0.23904d, others reported. Bea periods 49.198, 5.442 and 4.900d. Sp. also var. over 0.25d. џMurzimџBet CMaџCanopus is the second brightest star in the sky. It is 116 [G/light year] away, 30 times the diameter of our [G/Sun] and 1,400 times more [G/luminous] џCANOPUSџAA' probably combined light and color. This may be the SB pair, 4.3, 6.0v, sep. 0.2". B, 8.5V A1V at 113", vsini 141k/s, is binary with C, 8.9v, sep. 0.2". Component P, 15.1V at 24" optical. Other components faint at 54" to 92". џTriple system with HR 2357 and 2358. Combined mag., color 3.74V, -0.15(B-V), all Be stars. AB, 17000y; AC, sep. 10", 29000y. Component D, 12.2v at 26" from A. Uncertain which of components A,B,C, HR 2356,7,8 is the light variable NSV 2977, for which the mag. 3.75V is a blend of all three. Hydrogen lines var. K 30k/s. Shell line velocities do not correspond to orbital elements; may be due to gaseous ring. џBeta C 4.33 - 4.36V, 0.2095755d, secondary variations. Effective temperature varies by 1400K and ratio of max. to min. radius by 1.042. џXi1 CMaџA* 1.93 A0IV, 12.9y, a = 0.038". џALHENA.џBeta C?, 3.16 - 3.20V. џCompanion 9.22V, +1.13(B-V), +0.91(U-B), K0III-IV. џMebsutaџOptical. џDelta Sct? џAlzirr.џSirius, the brightest star in our night sky, is also one of the closest star to us at only 8.7 [G/light year]s. It is 23 times more [G/luminous] than ou [G/Sun] and almost twice its diameter. It has a small companion star that i believed to be a white dwarf. The companion is difficult to see because o its closeness to Sirius AB -1.46 A1V, 8.49 A1V, 50.090y, a = 7.500" or 49.94y, a = 7.62". D, 14.0v at 32" from A. C, companion to B at 1.4" suspected but not confirmed. B is first white dwarf ever discovered; predicted by Bessel (1844) on basis of orbital motion of Sirius, it was first seen by Alvan Clark in 1862, and its peculiar high temperature, small size and great density established by W. Adams in 1925. Soft X-rays observed from Astronomical Netherlands Satellite (ANS). Sirius B not unusual compared with other dA white dwarfs. Effective temperature about 32000K. џSIRIUSџGamma Cas 3.78 - 3.97V, 3.7 - 3.85B. џKap CMaџFrom orbit based on IUE data, the star should be eclipsing with period 195.24d. џV415 CarџAB binary. C, 13v at 29" optical. D, 9.5 at 207". џLc 3.78 - 3.99V. џOmi1 CMaџBeta C 4.36 - 4.40v, 0.08:d. џIot CMaџFixed sep. џADARAџLc 3.43 - 3.49V. џSig CMaџComponent A is suspected occultation double, 4.5, 4.5v, sep. 0.1". B, 10.5v at 87". C, +20d1686, 7.55V, +0.62(B-V), +0 +0.07(U-B), G1V at 96" has high proper motion, 0.100", optical, vsini =<54k/s. Other components fainter. ADS 5742A, CDelta 3.62 - 4.18V, 10.15073d. Period decreasing 3.1s/y. џMekbuda.џZet GemџH alpha profile changes in 30 min. or less. џMuliphenџWezenџAB CPM. 4.3 - 4.36V. џBinary with HR 2735. Combined mag. and colors, 3.63V, +0.91(B-V), +0.60(U-B), +0.48(R-I). 3.56 - 3.62V, blend with 2735. џAmp. about 0.07u, 0.04v, 0.02b, 0.04y; 0.936d. џQW PupџGamma Cas 3.60 - 4.18V, cycles 20 - 22 hrs. Also amp. 0.06V on time scale of 5d reported. Hydrogen emission varies with period 1.3667d (possibly a rotation period). џOme CMaџADS 5961A is dubious occultation double, 4.0, 5.0v, sep. 0.045". B, 10.7v at 10" is CPM. Delta Sct? џAB 3.55 F0IV, 8.18 K3V, 1200y, a = 6.975". Component A is SB, 3.7, 5.7v, sep. 0.2". џWasatџB, 10v at 8" fixed. D, 8.22V, -0.19(B-V), -0.93(U-B), B2V at 85". 3.90 - 3.96p. Possibly same period as SB. џPropus, a name mџCompanion is A0V, optical, vsini =<54k/s. џAludra.џGamma Cas 2.84 - 2.92V. џGomeisaџBet CMiџB, 12.5v at 3" CPM. џCPM. Companion G5V. џBinary with HR 2891. Combined colors. џCastor, representing the head of the northern twin in [X/Gemini], lie approximately 49 [G/light year]s away. With the [G/naked eye], Casto appears as one bright star. With advanced astronomical instruments, it turn out that there are six stars making up this system AB 1.98 A1V, 2.88 A5Vm, 511.30y, a = 7.369 or 420.07y, a = 6.295". C, 8.8v M1Ve at 73" is physical member of sextuple system in which A,B,C are all SB. ADS 6175C at 73" from A, EA 8.91 - 9.60V, 0.81428254d = also SB period. Masses each component 0.64 solar. Both components flare stars, M1Ve + M1Ve. џCASTORџYY GemџProcyon is the 5th brightest star in the sky and also one of the closest It is only 11.3 [G/light year]s away. It is twice the diameter of our [G/Sun and 6 times more [G/luminous] AB .35 F5IV-V, 10.3, 40.65y, a = 4.548". Binary nature first revealed in 1840 by variable proper motion; companion first seen in 1896. Component C, 11.7v at 122" optical. Delta Sct? A 0.09:d period originally attributed to the star beta CMi (HR 2845) may instead apply to Procyon, which had been used as a comparison star. џPROCYONџRS 4.13 - 4.29V, 19.423d. џSig GemџPollux represents the head of the southern twin in [X/Gemini]. It is yellowish star, approximately 35 [G/light year]s distant. It is a littl over 4 times the diameter of our [G/Sun] and 35 times more [G/luminous] All the visual companions optical. NSV 3712 is component A, 1.10 - 1.17V, while component E is NSV 3716, 10.5v. џPOLLUXџVar. in red and IR. Amp. 0.24R, 0.20(R-I). џAzmidiskeџCompanion B9V, RV -72k/s, optical. џa Puppis, often џBeta C or Ell?, 4.47 - 4.54V, amp. 0.07y. џQZ PupџSoft X-ray source. Beta C, amp. 0.015V, 0.101d. џChi CarџComp. A of visual double, EB 4.74 - 5.25p, 1.4544877d, contact binary, equal components. џV PupџWith HR 3207, appears capable of producing most of the observed ionization of Gum Neb. Change in H alpha emission profile between 1974 and 1976 interpreted as change in rate of mass loss. џNaosџDelta Sct 2.68 - 2.78v, 0.14088143d. џRho PupџB, 10.1v G8II at 33" optical. C is K2III. џComponent B of 5 stars within 2' of HR 3207. џAm at 94", SB, over 7d?, optical. Low degree of polarization indicates symmetric shell. The brightest O-type star and one of only four WR stars bright enough to have been observed spectroscopically in UV by COPERNICUS. With 3165, appears capable of producing most of th observed ionization of Gum Neb. The brightest and presumably the nearest Wolf-Rayet binary. Radio emission interpreted as coming from circumstellar gas cloud extending farther than the orbital radius of the binary. 1.6 - 1.8V, 154 sec. Sp. var. in about 200 sec. Variability too great to be explained by the 78.5d SB companion. Possibly a third close companion: a collapsed star of less than 2 solar masses. џSuhail al MuhlifџGam2 VelџNS PupџCPM. џAltarfџAlsciaukatџE? 1.82 - 1.94V, 3.57 - 3.83p, 785:d. џAvior.џB is 15v at 7", CPM. C and D optical. 3.3 - 3.8V, 358d. Also 0.05d, amp. 0.02V. џMuscidaџAl Minliar al ShџBeta C 3.56 - 3.67V, 0.131977d. џOmi VelџBeta C 4.27 - 4.33V, 0.17d. џEta HyaџBeta C 4.3 - 4.33V, amp. 0.04B. џV343 CarџAP, suspected double, unresolved by speckle interferometry. Visual companion 12.2v at 38" optical. џAsellus AustraliџBinary with HR 3474. Probably NSV 4238. џAB 3.8 G5III, 4.7 A8IV or F0V, 15.05y, a = 0.238". Speckle interferometric sep. 0.263-0.272", 1980-3. Combined mag., colors. ABxC, 3.4, 7.8, dF7 at 3" from AB, 890y, a = 4.536". Component D, 12.7v at 19" from A, in hyperbolic orbit about ABC, periastron distance, 29". џEps HyaџCPM. џGamma Cas 4.4 - 4.50V. Variable H alpha. џV344 CarџCPM. џBC 10.8, 11.0, 39.69y, a = 0.68". BC is dM1. BCxA: 817.91y, a = 9.092". Separation rapidly decreasing. ADS 7114Aa, 11.02y, a = 90.354". This is the SB pair. ADS 7114A, S, 3.12 - 3.18V, 0.071d. џTalithaџAcubensџAB 4.11 F5V, 6.18 G5V, 21.85y, a = 0.619". Combined mag., colors. Companions C - E optical. Masses A, 1.13; B, 0.84 solar. џ4.2 A0IV-V, 4.4 A0V, 70.1y, a = 0.27" or 64.29y, a = 0.26". Mag., colors for combined light. џYoung disk population. Lc 2.14 - 2.22V. џAlsuhailџLam VelџE 3.41 - 3.44V, 3.20 - 3.56p, 0.05R, 6.751154d. џa Car.џV357 CarџHelium var.? џBalmer lines show quasi periodic var. in cycles of about 35 min. џMiaplacidus.џAB binary. џ2.2 - 2.5:v. џTuraisџAB binary. NSV 4478 is ADS 7351B, 9.5 - 11.5v. џAl Minliar al AsџThird UHURU Catalogue suggests Kappa Vel as optical counterpart of 3U0918-55, but HR 3717 is much closer. џAlphard, the "Dragon's Heart" in the [G/constellation] of [X/Draco], has a reddish tint to it. This slightly variable star lies approximately 140 [G/light year]s away. џALPHARDџAB binary. C, 10.5v at 100", optical. Delta Sct, amp. 0.07B, about 2 hrs. џSp. var., 7 - 12d. џAlterf.џ4.1 F2IV, 4.6 F0V, 33.99y, a = 0.795". Combined mag., colors. Comp. B, 4.5 - 5.1v. џL? 3.10 - 3.16V. џN VelџBinary? Amp. 0.033y, 18.0d, possibly due to rotational modulation. џComponent B, 9.9v at 85". џSubra.џCep amp. 0.1V, period a few days. џRas Elased AustrџCDelta 3.28 - 4.18V, 35.53584d. Period varies. џl CarџCPM. Delta Sct 3.77 - 3.86V, 0.133d, amp. and form of light curve vary. џUps UMaџCPM with HR 3891. Mag. and colors for combined light, 2.96V, +0.27(B-V), +0.12(U-B), +0.29(R-I). џCompanion K0III, optical. џDelta Sct? 4.47 - 4.52V, about 0.1d. џCPM. џRegulus, the heart of [X/Leo], is the star at the base of the "Sickle o Leo". It is approximately 75 [G/light year]s distant. It has a smal companion star which lies approximately 4,660 [G/A.U.]'s from Regulus AB binary, B, 8.13V, +0.86(B-V), +0.51(U-B), K1V. BC, 7.6, 13.1v, 2000y, a = 4.163". џREGULUSџVisual companions both optical. џPrimary unresolved by speckle interferometry 1982.17. џAdhaferaџTania Borealis. џLc? 3.36 - 3.44V. џV337 CarџAB 2.22 K0IIIP, 3.47 G7III, 618.56y, a = 2.505". B is HR 4058. Colors for combined light. Mag. for blend, 1.90V. Component C is the flare star AD Leo (8.07-11.00B) at 5', optical. Originally confused with eclipsing star Y Leo when var. suspect number 6777 was assigned in 1965. Now HR 4057 is again suspected of variability, 1.84 - 2.03V for combined HR 4057/8. Uncertain which component is the variable. џALGIEBAџSee HR 4057. џE?, 2.99 - 3.33V. џTania Australis.џ4.40 G8III-IV, 6.12 F8V, 37.92y, a = 0.340". Combined mag., colors. џ3.79 - 3.83V. џ4.4, 4.8v, sep. 0.11"; combined mag., colors. Old disk population runaway star. Alpha Cyg 3.83 - 3.90V. џRho LeoџGamma Cas 3.27 - 3.37V. џPP Carџ4.2 F3IV+F0V, 5.1 A6V, 16.30y, a = 0.340". џProbably CPM. B is B8. C, 11.2v at 20" from B. џSpectrum var., 1.7788d. Discussion of earlier suspected period of 0.7045d given by Walborn (1979, PASP, 91, 442). vsini 202k/s. High speed mass ejection. џ2.7 G5III, 6.4 G2V, 116.24y, a = 1.437". Secondary also classified F8:V:. џOld disk population runaway star. џPraecipua.џ3.76 - 3.80V. џAlkes.џMERAKџwith HD 95638 = GC 15179, 7.12V F8; SB, 6.04d. ADS 8035A; B also var. suspect NSV 5071, too close to primary to be certain of variability. џDUBHEџDelta Cep? 3.84 - 4.02V. џV382 CarџDelta Sct? џZosmaџChortџBinary with HR 4375, q.v. Blend of 4374-5. Amp. 0.03V. џorbit determined, in 1828 by Savary. Third component astrometric with A, 1.832y, a = 0.055". See HR 4374. џAlula Australis.џAlula Borealis.џ4.3 B5VN, 5.0 B6V, 39.18y, a = 0.277". Combined mag., colors. џ4.03 F2IV, 6.70 G3V, 192.0y, a = 1.92"; possible subsystem with period about 16y. Combined mag., colors. Combined mass about 3 Suns. Delta Sct? џSR, 3.78 - 3.86V, about 1100d. џGianfarџCompanion B9V, optical. џDuplicity doubtful. џAmp. 0.08V. џAmp. 0.04V? џRepresenting [X/Leo]'s tail, Denebola lies 40 [G/light year]s away and i approximately 20 times more [G/luminous] than our [G/Sun] B, 15.7v at 40" physical; C, 13v at 80" optical. Delta Sct?, 2.09 - 2.16V. џDENEBOLAџBet LeoџZavijahџThe reality of the companion, CF UMa, announced by P. van de Kamp (see Low Luminosity Stars, ed. S. S. Kumar, p. 199, 1968) has been questioned (PASP, 96, 557, 1984). Unresolved by speckle interferometry 1980.47. Companion of Groombridge 1830, UV? 8.5-12v. џGroombridge 1830џBet HyaџPHADџUnresolved by speckle interferometry 1982.17. џCPM with HR 4619, 4621. H alpha varies. џCPM with HR 4618, 4619. Gamma Cas 2.51 - 2.65V. Expanding circumstellar shell. џDel CenџAlchibaџMinkar.џBeta C 2.78 - 2.84V, 2.25 - 2.31p, 0.151038d. Expanding circumstellar shell. џDel CruџMEGREZџOld disk population runaway star. Expanding circumstellar shell. џGienah GhurabџSRb? 3.99 - 4.31V, 40d. џEps MusџOld disk population runaway star. 4.2 - 4.24v. џCompanion G8III, optical. џ4.9, 5.4, sep. 0.008". Also astrometric and interferometric double, 5.4v sep. 0.124", position angle changed 35d in 1.5yrs. Delta Sct? џZaniah.џI? 3.4 - 4.0v. џAB 1.35 B0.5IV, 1.75 B3n or B0.5Vn, q = 0.916". Mag. and colors for blend of HR 4730-31, 0.76V, -0.25(B-V), -1.00(U-B) -0.24(R-I). Masses 14 and 10 solar for hyperbolic orbit with periastron distance 61 AU. Possibly X-ray source 2U1223-62. Acrux is a bright binary star system whose combined light makes Acrux the 14th brightest star in the sky. It is about 400 [G/light system is much larger than our [G/Sun] (14 and 10 solar masses respectively). џACRUX.џPossibly X-ray source 2U1223-62. џCPM. B is K2Ve, lithium strong. ADS 8572A. џAlgorabџI? Amp. 0.30p. џGacrux.џChara is the name assigned either to this star or, more generally, to the "southern hound" of the constellation Canes Venatici; the northern "hound" is called Asterion, a name not generally assigned any particular star. Beta CVn amp. 0.05V. џCharaџGamma Cas 3.82 - 4.10V. H alpha and H beta emission vary period about 30d. H alpha profile changes in 1 min. or less џKap DraџCompanion B4V, optical. Beta C 2.68 - 2.73V, 2.17 - 2.24p, 0.0903d. џAlp MusџAB 2.9 A0III, 2.9 A0III, 84.50y, a = 0.930". Combined mag., colors. џAB 3.48 F0V, 3.50 F0V, 171.37y, a = 3.746". Speckle interferometric sep. 3.674", 1982.38. Combined mag. 2.75V. Colors for combined light. Component C, 15v at 53", optical. Amp. 0.02V. Blend with 4826. Uncertain which component is the variable suspect. џPorrimaџ3.7 B2V, 4.0 B3V, 383.12y, a = 1.735". Combined mag., colors. џInterferometer measures indicate close double or multiple star. Component B, 11.4v, F8V, optical; C, 7.5v, B8. Beta C 1.23 - 1.31V, multiple periods, 0.2365072d, 0.160474d, 0.121383d, 6d, 7 - 8y and others. џBecruxџBet CruџCPM with HR 4899. џAlpha CV 1.76 - 1.79V, 5.0887d. Spectrum variable. Photometric var. due to UV absorption from overabundant metals. џALIOTHџEps UMaџAuvaџBinary with HR 4915. џADS 8706A, Alpha CV 2.84 - 2.98V, 2.78 - 2.81B, 5.46939d. The prototype star. Var. magnetic field with same rotation period. џCOR CAROLI.џAlp2 CVnџVINDEMIATRIXџCPM companion F7V. џA is SB and speckle interferometric binary, third component 9.4v, sep. 7.1". B, 8.00V, +0.20(B-V), -0.09(U-B), CPM. џAB 5.05 F5V, 5.08 F5V, 25.87y, a = 0.662". Colors, spectrum for combined light. Mag. of blended HR 4968, 4969 is 4.32V. ADS 8804A speckle interferometric sep. 0.43" 1978.40, 0.58" 1981.47. Var. of combined light with HR 4969 not confirmed, but 90d inclination of orbit indicates eclipses possible. џDiadem.џAa = AP 3.0 A2V, 3.0 A2V, sep. 14.4", 0.056y, a = 0.012". Combined mag., colors AP. Binary with HR 5055. Alcor, HR 5062, at 709", CPM. џMIZARџSpica is the 16th brightest star in the sky. It is a binary star syste that lies 142 [G/light year]s away. The largest of the two stars is almos 11 times more massive than the [G/Sun], while the second star is approximatel 7 times the mass of our star Interferometer indicates visual component A is multiple system. Occultations yield three companions: 3.1v at 0.0025", 4.5 at 0.05" and 7.5 at 0.5". Combined mag. and colors. Visual component B, 12.0v at 148". Ell (Beta C) 0.97 - 1.04V, 4.01454d, and Beta C, 0.1737853d. Period changes. џSPICAџAlp VirџCPM with HR 5054-5. Delta Sct. џALCORџ4.5 G8III, 4.7 G9III, 78.7y, a = 0.165". Combined mag., colors. џHeze.џCompanion B1p, optical. Beta C 2.30 - 2.31V, 0.169608, 0.17696 or 0.2150d. Multi-periodic. џEps CenџDelta Sct? Amp. 0.02V. џBinary, period several centuries. Companion M2. Delta Sct? 4.40 - 4.58V. џBeta C?, 3.40 - 3.43V, 3.48 - 3.52R, 0.175d. џNu CenџAlkaid is located at the end of the [G/Big Dipper]'s handle. It is about 93 [G/light year]s distant. џALKAIDџV806 CenџGamma Cas 2.92 - 3.43V, 3.535d. Variable H alpha. Expanding circumstellar shell. R and I mags. decreased by about 0.3m between 1965 and 1983. Variable line profiles. џMu CenџExpanding circumstellar shell. џA* 2.68 G0IV. Visual component 8.8v at 113" optical. џMufridџExpanding circumstellar shell. џB is G type, optical. џHadar, a bright, hot star, is the 10th brightest star in the sky. It is ove 360 [G/light year]s away and has a companion star that is difficult to se with a small telescope Beta C? Amp. 0.07V, 0.157d, modulation 352d. Line profiles also vary per. 0.157d. џHADAR.џBet CenџAmp. 0.020B, 0.035d. џChi CenџMenkent.џThuban is the bright star located halfway between the bowl of the [G/Littl Dipper] and the second star of the handle of the [G/Big Dipper]. It i approximately 180 [G/light year]s distant and 135 times more [G/luminous than our [G/Sun]. 4,800 years ago, Thuban was aligned with Earth's Nort [G/Celestial Pole], making it our North Star Alpha CV?, 3.64 - 3.67V. џTHUBANџ4.06 - 4.11V џSyrma.џArcturus is the fourth brightest star in the sky. It is 25 times the diameter of our [G/Sun] and 115 times more [G/luminous]. It is only 37 [G/light year]s away. High space velocity? H and K emission vary. џARCTURUSџSX Ari 4.38 - 4.43V, 8.814d for light, He, magnetic field; light and mag. field max. correspond to He min. Sp. from B2 to B7IV in per. 8.8172d. Var. possibly due to rotation of inhomogeneous surface; possibly prolate spheroid. џV761 CenџBinary. Combined mag., colors. џCPM. џAsellus Primus.џPrimary found double by speckle interferometry, sep. 0.069". Component B, optical. Delta Sct 3.02 - 3.07V, 3.23 - 3.28B, 3.20 - 3.25p, 0.2903137d. Hydrogen and Ca lines vary. џSeginusџGam BooџInnes catalogue indicated a faint companion at 6" in 1897, not subsequently seen. Gamma Cas 2.30 - 2.41V, 1.83 - 1.95p. H alpha variable, H beta sometimes bright, sometimes dark and double or multiple. Variability shows evidence of mass loss. Amp. 0.07V on time scale 1d suspected. џEta CenџDelta Sct? џS, amp. 0.1:V, 0.20U. Expanding circumstellar shell. џAB 79.920y, a = 17.515". B = HR 5460, CPM with Proxima at 2.2d, discovered by Innes in 1915, a flare star, V 645 Cen, 12.4 - 13.4p, 11.10V, +1.88(B-V), +2.05(R-I), M5.5Ve. џRIGEL KENTAURUSџAmp. 0.03V. Magnetic var., about 4 months. Pulsation period 6.8 min? џAlp CirџBeta C 2.29 - 2.34V, 0.2598466d. Period varies. Possible secondary period 3.145d. Modulation period 10y? џAlp LupџAB 4.52 A2III, 4.55 A2III, 123.44y, a = 0.595". Colors for combined HR 5477-5478. Combined mag. 3.78V. vsini 156k/s for blended HR 5477-8. џBinary with HR 5505. Colors for combined light. Mag. of blend, 2.37V. џIZARџBinary. џZuben ElgenubiџAB 4.74 G8V, 6.9 K4V, 151.505y, a = 4.904". Combined mag., colors. Masses 0.89 and 0.74 solar. Perturbation period 2.2y, a = 0.020" suspected; unresolved by speckle interferometry. Component C optical. BY? 4.52 - 4.67V, 10.137d. џKOCABџAB 5.79 K4V, 7.93 M2V, q = 20.388" hyperbolic orbit. Component B is dM2. џ2.9 - 2.95B. џNekkarџSRb 3.20 - 3.46V, 20d. џSig Libџ4.6 B3V, 4.9 B3V, 72.88y, a = 0.422". Combined mag., colors. џCPM with HR 5647. џCPM. B is F8. Nearly same proper motion as HR 5646, 5647. џCPM. џDescribed by Eratosthenes (ca. 200 B.C.) as brighter than Antares, by Ptolemy (ca. 150 A.D.) as equal to Antares. џZuben ElschemaliџBeta C 3.21 - 3.24V, 0.16547d; 0.14273d also possible. џDel LupџVar? Amp. 0.015b. џProbably binary with HR 5734, a close binary ADS 9626BC. Delta Sct? џAlkaluropsџDelta Sct? Amp. 0.03V. Hydrogen and CaII variable. џPherkadџGam UMiџEd AsichџAlpha CV 3.65 - 3.72V, 18.487d. Magnetic field and rotation same period. Variable H alpha. Amp., light, magnetic field, spectrum vary per. 10.5y. Possible secondary light period of 240d. џNusakan.џBet CrBџCompanion A5. џ3.5 B2IV-V, 3.6 B2IV-V, 147y, a = 0.59". Combined mag., colors. џComponent A is NSV 7134, 4.12V, amp. 0.7m. However, 1300 UBV observations on 57 nights (1984-6) revealed no variation over 0.06 mag. R-I also found at -0.16. Component B, the rarely seen companion, is NSV 7135, 5.5, 7.8v. џADS 9704 AP, sep. 0.097", unresolved by speckle interferometry. Component B, 11.2v at 42", optical. џZuben ElakrabџDelta Sct 4.20 - 4.25V, 0.134d. Fourier analysis of 1975 and 1979 data shows frequencies of 6.4227 and 7.8869 cycles/ or periods 0.1557 and 0.1268d. џDel SerџAlphekka is the brightest star in [X/Corona Borealis]. It lies approximately 75 [G/light year]s distant and is about 45 times more [G/luminous] than our [G/Sun]. EA 2.21 - 2.32B, 17.359907d. Possibly also intrinsic var. џALPHEKKAџAlp CrBџ4.08 A0IV, 5.51 A3V, 91.0y, a = 0.74". Combined mag., color. Delta Sct 3.80-3.86V, 0.030d. Mass 1.9 solar. Possibly beat period? џGam CrBџSR? Amp. 0.2V. ADS 9765B, optical. џUNUKALHAIџB, 9.72V, +0.84(B-V), +0.68(U-B), K3V, CPM. C, 10.7v at 201". Also CPM with BD+15d2906 at 1642", itself a double, 8.4, 10.5v sep. 6". џDelta Sct? џCompanions optical? џPrimary is SB, 3.4, 6.4v sep. 0.0003"; third component, ADS 9862B, 12.2v at 50". vsini both A and B =<100k/s. Component B, F4V, optical. џPossible X-ray source 3U1555+27. џPossible quadruple system: SB 3.0, 5.0v, sep. 0.00001", 3.3v at 0.1", and 4.9v at 0.186". џDschubbaџVisual companion doubtful. Nr 2.0 - 10.8v, 29000d? Outbursts 1866 and 1946. V and B-V for 1946 maximum. Near maximum 9.88V, +1.40(B-V), +0.59(U-B). џT CrBџCompanion optical. џCPM with HR 5985 = ADS 9913C, at 14" and with B, 5.9v at 0.5", possibly SB. Lunar occultations and speckle interferometry indicate companions 4.2v at 0.001" from A and 7.6v at 0.129" from C. Occultations by Jupiter and Io in 1971 indicate complex system. Component C occulted by Io revealed the 2.5 mag. fainter companion at 0.1". џGraffiasџAmp. 0.02(b-y). џAlpha CV?, 4.23 - 4.27V, amp. 0.015U, 7.832d, symmetric light curve. џADS 9951A is SB, 4.9, 6.9v, sep. 0.0003". AB, binary. Component B, 6.9v at 1". Components CD at 41" = HR 6026, q.v. HR 6026, q.v. џJabbah.џYed PriorџYed Posterior.џB, 8.26V, +0.25(B-V), -0.23(U-B), B9.5V at 20", optical; vsini : 54k/s. The visual primary is triple: SB, 3.3, 5.3v, sep. 0.0005" and 5.5v at 0.49", discovered by occultation. Beta C 2.94 - 3.06B. Multiple periods, 0.2468429, 0.239671, 8.2, and 33.1d. Surrounded by HII region. Primary period varies in period of 23.2y with an amp. of 0.7 sec. Occultations indicate the variable has a 2.2 mag. fainter companion at 0".49. The duplicity had been suspected from occultations as early as 1860. Orbital period probably over 112 yrs. UV observations indicate temperature varies by 2510K and ratio max. to min. radius by 1.095. џAlniyatџSig ScoџADS 10010AB, 6700y. 3.85 - 3.90V. џADS 10022B, 9.58v, optical. џCompanion 7.46v B9V, CPM, possibly binary with the SB. џGamma Cas 4.18 - 5.0V. Long term variation in emission lines. Variable polarization. R-I also found at +0.09 and +0.11. џChi OphџADS 10058A, var. suspect NSV 7713; ADS 10058B, var. suspect NSV 7712, 8.8v, dK2, amp. about 2v. џThis bright red supergiant star has a diameter of 600 million miles (1,000 million km), making it almost 700 times larger than our [G/Sun]. This star is in its final stages of life. Once it has used up all the fuel in its core, Antares, will explode in a [G/supernova] explosion. What's left of the star will form either a [G/pulsar] or a [G/black hole]. Antares is 135 [G/light year]s away. Var. M1Ib, 5.5 B2.5V, 878y, a = 2.90", masses 15.5 and 7.0 solar. Companion is radio source. SKYLAB confirms cool star hot companion. ADS 10074A, SRc 0.88 - 1.8V, 1733d. Possibly considerably fainter before 150 A.D.: see HR 5685. џANTARESџAlp ScoџKornephorosџMarficџAlpha CV, 4.45 - 4.51V, 1.79 or 4.67d. џOme Ophџdouble-lined. Resolved by speckle observations 1986.45 (Blazit et al. 1987, A&AS, 71, 57). џCOPERNICUS observations of CO indicate a SN remnant near Zeta Oph which may have caused Zeta Oph to become a runaway star. Gamma Cas 2.56 - 2.58V. Spectrum var.: UV spectra in 1972 indicated mass outflow probably related to formation of shell. Evidence disappeared in 1974. H alpha in absorption 1971, emission 1973. Rotational period 19.7 hrs. џZet OphџADS 10157AB, 2.90 F9IV, 5.53 G7V, 34.49y, a = 1.355". ADS 10157A*, 10.5y, a = 0.08". ADS 10157A is var. suspect NSV 7915. џCompanion questioned. џCPM with HR 6252 at 346". EB 2.80 - 3.08B, 1.44026907d. Semi-detached system. џMu1 ScoџCPM with 6247 at 346". џ3.6 - 3.64V. џLb? 3.14 - 3.20V, 4.1 - 5.0p. џKap OphџEA 4.22 - 4.28V, 39.4809d. џEps UMiџAB 3.0 A2V, 3.5 A3V, 88y, a = 0.86". Combined mag., colors. џSabik.џAldhibahџBinary with HR 6402, q.v. CPM with CoD-26d12036, 6.34v K5V at 700", same parallax. џ+0.44(R-I). џAB, 3600y, a = 4.68". Component B is HR 6407. Combined colors. Combined mag. 3.08V. Mass A, 14 solar. Other components faint, optical. Circumstellar lines around both A, B. ADS 10418A. Discovered by W. Herschel in 1795. SRc 3.0 - 4.0v. 6-yr. period superimposed by variations 50 - 155d. Surrounded by envelope of 2x10E+05 solar radii, expanding 10k/s, mass loss 3x10E-08 solar masses/y. џRASALGETHIџAlp HerџSee HR 6406. џADS 10424B, dG4, optical. џSarin.џAB 5.53 G8V, 8.65 M0V, 693.24y, a = 10.415", or 2205y, a = 23.90". Various published orbits range from 242 to 2205y. Combined mag., colors. џAB 6.1 K3V, 7.6 K5V, 42.177y, a = 1.734" or 42.09y, a = 1.82", combined mag., colors. Component C, 9.9v M2, 32" physical. D, 12.8v at 15". Amp. 0.04. џBeta C 3.25 - 3.31V, multi-periodic 0.140531 and others ranging from 0.0464 to 0.1399d. џThe OphџPossibly CPM and same RV as HR 6462, 50'N. џComponent B, A7V; C is optical. џCompanion K0III, optical. џLesathџ2.76 - 2.90V. џMaasymџBeta C 1.59 - 1.65V, 0.2137015d, secondary 0.1068518d, beat period 10.1605d. Also possible 0.04V eclipse. X-ray flare observed in vicinity Lambda Sco on 1 June 1975. џSHAULA.џLam ScoџRastabanџ1.90 - 1.94V? џSargas.џA* 2.08 A5III, 8.5y, a = 0.065". Resolved by speckle interferometry. Delta Sct? џRASALHAGUEџVisual companion optical. Delta Sct?, 3.52 - 3.54V. џBeta C 2.39 - 2.42V, 0.1998303d, 0.205430, 7.3316, 0.189512 and 2.591d. џKap ScoџOmi SerџBeta C?, amp. 0.01V. џIot HerџPossibly close double. џCebalraiџBC 10.3 dM4, 10.8, 43.20y, a = 1.360". This close pair forms a wider physical binary with component A. џGrumiumџPossibly 5 yr. period in He 10830 emission. џAmp. 0.08V. He 10830 variable. Also spelled Eltanin џETAMINџSRd? 4.38 - 4.48V, 29:d. However, more recent photoelectric observations cast doubt on variability. џNu HerџComponent B, 13.7v F? at 7", optical. AC fixed. C, 8.12V, -0.02(B-V), -0.57(U-B), B1V, vsini 130k/s. џBinary. ADS 10990B? 8.0 - 10.0v. џNashџAB 4.20 K0V, 5.99 K4V, 88.13y, a = 4.545". B is 6.00V, +1.15(B-V), vsini =<25k/s. Aitken listed 9 additional faint companions within 180". џDiscordance in designations of components between ADS and IDS. We accept IDS. Component B, in notes to ADS 11076 not assigned letter: doubtful, sep. 0.1" if real. C, 14v at 25" CPM. D = ADS C, 11v at 54" optical. џGamma Cas 3.81 - 3.9B, 4.1 - 4.2p. џOmi HerџCompanion A6V, optical. џADS 11169A is SB, 4.1, 7.0v, sep. 0.011". Closest visual companion is B, 11.5v, B9III at 17"; C is 13.5v at 26"; D, 9.9v, B3; E, 9.4v, B2V, physical, vsini 184k/s. ADS 11169A, EA 3.79 - 3.92V, 180.45d. Also irregular changes in brightness. џMu SgrџLb 3.08 - 3.12V. џEta SgrџPrimary of visual double and a suspected astrometric binary. џKaus MeridionaliџKAUS AUSTRALIS.џKaus Borealis.џ4.4, 6.1v, 271.7y, a = 0.392". Alpha CV, amp. 0.04V, 1.71646d. Same rotation period. џPhi DraџA* 3.57 F7V, 0.768y, a = 0.124". Masses 1.5 and 1.1 Suns. Shortest known period for astrometric binary. Speckle interferometry indicates component A is binary, sep. about 0.1". B, 12v K1V at 149"; C, 13.5v at 10". џAmp. 0.10V. џVega is the westernmost star of the Summer Triangle. It is the fift brightest star in the sky and is approximately 25 [G/light year]s distant It is over 2 1/2 times the diameter of the [G/Sun] Companions in IDS optical. BD=+38d3231, 8.6v, 23' N. prec., may be CPM. Delta Sct -0.02 to +0.07V, 0.19d. џVEGAџAlp Lyrџ4.1, 4.1v, sep. 0.13", doubtful. џAB 5.00 A2n, 6.10 A4n, 1165.6y, a = 2.78". Binary with HR 7052 = B, and CPM with HR 7053-4 at 208". Combined mag. and colors for HR 7051-2 are 6.48V, +0.19(B-V), +0.04(U-B). џCPM with HR 7057 = ADS 11639D. Other components optical. Delta Sct? џAll companions probably optical. џGamma Cas 3.4 - 4.3V. џLam PavџAB fixed. B is 8.6v, B7v; may be collapsed star; vsini 120k/s. E, 9.9v A8pSr or B9V at 67" optical? F, 9.9v A8-9V o or B9V at 86". A, B, E and F are CPM. ADS 11745A, EB 3.25 - 4.36V, 12.913834d. Period varies. Presumed disk around secondary. Also radio flare activity. Prototype Beta Lyrae type, discovered by Goodricke in 1874. џSheliakџBet LyrџKap PavџInterferometer measures indicate multiple star. џNUNKIџSRc? 4.22 - 4.33V. џDel2 LyrџSRb 3.88 - 5.0V, 46.0d. џR LyrџDeneb el OkabџSulafatџAB 3.2 A2III, 3.4 A2V, 21.138y, a = 0.532". џAscella.џDelta Sct, amp. 0.05V, 0.04B, 0.097d. џPolaris AustraliџDeneb el OkabџAlfecca MeridianџAB, combined mag., colors, sep. 0.093". Third component 6.0v at 0.4". џAlbaldahџB is A0, optical. џAladfar.џNodus SecundusџCPM. Companion A5V; vsini 129k/s, optical? џArkab PriorџSep. 0.036". Questionable occultation double. Delta Sct 3.90 - 3.93V, 0.050d. џRho1 SgrџArkab PosteriorџComponent A astrometric binary, A* 3.36 F0IV, 3.422y, a = 0.058"; unresolved by speckle interferometry. Delta Sct? Proper motion slightly variable? џSecondary K0. џAnser (rarely usџLocated at the head of [X/Cygnus] the swan, Albireo is a unique binary star system that lies about 190 [G/light year]s away. One star in this system is a yellow star while the second star is a hotter, blue type star. 7270.2y, a = 62.90". Binary with HR 7418. vsini of B-type component of ADS 12540A 50:k/s. Component C, 11v at 50". Two additional components of A resolved by speckle interferometry: Aa 1981.70, sep. 0.42"; Ap 1978.41, sep. 0.12" and 1979.46, sep. <0.08". џALBIREO.џB and C optical. џAlsafiџAB CPM. B, 13v at 3". C, optical. џCompanions B and C optical. џShamџSee HR 7503. џTARAZEDџAB 2.91 B9.5III, 6.33 F1V, 827.6y, a = 3.20". ADS 12880A is NSV 12381, 2.85 - 2.89V. Component B is NSV 12380, 6.5 ->8.5v. џSuspected visual double probably single image, composite spectrum. Secondary either B6 or A0V. Amp. 0.09p. џDel SgeџAltair is the southernmost star of the Summer Triangle. The 12th brightest star in the sky, Altair is only 16 [G/light year]s from us. This star rotates extremely fast, once every 6 1/2 hours. For comparison, our [G/Sun] rotates once every 25-30 days. Component B optical. џALTAIRџDiscovered by Kirch in 1686. M 3.3 - 14.2v. Period changes: 1686-1842, 405.88d; subsequently 408.05d. Variable CO emission from circumstellar envelope and enhancement of shell at minimum light. Total visual absorption o shell = 2 mag. Variable SiO maser source. Appreciable reddening at ascending light. џChi CygџDiscovered by Pigott in 1784. CDelta 3.50 - 4.30V, 7.176641d. Period changes. Variable He 10830 in emission and absorption. џEta AqlџBinary, companion K5III (AJ, 82, 431, 1977). However, Buscombe points out that the companion is F6V and this is more consistent with the magnitude difference between the components, if physical. џTyl.џAB binary. B 12v dM3 at 13". ADS 13110A, amp. 0.05V. џALSHAINџAB CPM. B, 12v at 7". Other components optical. џ3.52 - 3.65V. џAB CPM. B, 11v dM5, sep. 6.6". Wroclaw contr. no. 16 gives mag. differences but no sep. for four components: AB 5.4v, AC 5.15, and AD 4.0. Possible misidentification? Discovered by John Herschel as simply double. Components C and D apparently first listed by van Albada at Lembang in 1958; only magnitudes and no separations were indicated. џComponent C, 6.99V, -0.14(B-V), -0.58(U-B) B5V, vsini : 25k/s, at 107" fixed. AP probably single star. ADS 13554A, EA 3.77 - 3.88V, 3784.3d. Amp. varies strongly with wavelength. C = NSV 12931, 6.98V. џV695 CygџDelta Sct? џSee note for HR 7754. ADS 13632B, 14v at 44"; C, 9.6v K5III, at 45" physical, vsini =<54k/s. D, 14.3v at 29" from C. џPrima GiediџOriginally called Omicron2 Cyg in GCVS, the name has been changed to V1488 Cyg because of much confusion as to which star is Omicron1, which Omicron2. See HR 7730. EA 3.90 - 4.14V, 1147.4d. Period varies. Light var. outside eclipse. The K component may be slightly intrinsically variable. џV1488 Cygџ7754 = ADS 13645. Hence, we have recorded n = 9 for both. ADS 13645AB optical; BC 11.2, 11.5v, sep. 1.2" binary. џSecunda GiediџComplex system with HR 7775, q.v. Component B, vsini 97k/s. Occultations indicate component A is multiple system: 4.0 4.3v sep. 0.0002", 4.8v at 0.022" and 6.7v at 0.0001". A also suspected astrometric binary, 3.07 F8V. Possibly also two faint 13v components at 112" discovered by John Herschel. џDabih. Beta1 = DџBC, 9.2, 10.2v sep. 17.6". џPeacock.џNo physical relation between the radio components and the star. No demonstrable connection between Gamma Cyg and the so-called Gamma Cygni supernova remnant. џSadrџDeneb DulfimџAB 4.0 F5IV, 4.9 F5IV, 26.65y, a = 0.475" or 26.60y, a = 0.480". Speckle interferometry gives sep. 0.58" and with SB data leads to masses 2.2 and 1.8 solar. Combined mag., colors. Components C-E optical. џRotanevџOptical. џCompanions optical. џSualocinџDeneb is the easternmost star in the Summer Triangle. It is a blue/whit supergiant star that is 60,000 times more [G/luminous] than our [G/Sun] although it is only 25 times more massive. It lies 1,600 [G/light year]s away Alpha Cyg 1.21 - 1.29V. Change in H:H epsilon. No emission recorded before 1944. џDENEBџAlp CygџDelta Sct 4.39 - 4.49V, 0.135547 and 0.154991d. Combined magnitude of two components. џDel DelџSee HR 7947. џGienah CygniџEN Aqrџ9.1v A2 companion. џAB 5.22 K5V, 6.04 K7V, 722y, a = 24.65". B is HR 8086. Aa x P, 4.9y, a = 0.014". Astrometric measures indicate 3 invisible companions, periods 6, 7 and 12y. Unresolved by speckle interferometry. Suspected planetary companion not substantiated. Proper motions for HR 8085 and 8086 taken from Luyten LHS. SAO has only one entry (component A?), but appears to give the mean position of A and B. 5.19 - 5.27V, 350 - 400d. џADS 14636B, Is, 6.02 - 6.09V. џWhite dwarf companion. џAB 5.2 F7V, 5.3 F7V, 5.70y, a = 0.26". Combined mag., colors. Component C, 9.5v at 48" optical. џAB 3.82 F0IV, 6.42 G1V, 49.80y, a = 0.85". Components C, 13v at 29" and P, 12v at 72", both optical. Q, 12v at 90", physical. R, 13v at 90", CPM. Delta Sct 3.65 - 3.84V. 2-3 hrs.? Possibly variable period. џTau CygџKitalphaџCompanion A7V or G0V. џH alpha profile varies. џAB CPM; 79000?y. Component B, 10.0v G8.5V, probably optical. 4.28 - 4.50V. џUps CygџADS 14858A, Delta Sct?, 2.41 - 2.47V. џALDERAMINџAB CPM. Companion K0V. џBoth companions optical. џSadalsuudџADS 15032AB, 50y. B, 7.84V, +0.18(B-V), +0.06(U-B), A2.5V, vsini 60:k/s. Third component discovered by speckle interferometry, mag. diff about 4v. Sep. 0.025". Possible circumstellar material. ADS 15032A, Beta C 3.16 - 3.27V, 0.1904881d, modulation period 10.893d. SiIV and CIV vary. Satellite UV obs. indicate temp. varies 1340d, max./min. radius 1.038. џAlfirkџBet CepџA* 3.76 K0III, 2.84y, a = 0.052". џNashira.џEnif represents the nose of [X/Pegasus]. This slightly reddish star i 540 [G/light year]s away and over 5,000 times more [G/luminous than our [G/Sun] ADS 15268AB optical. 0.7 - 3.5V. 1.7m flare 1972 Sept. 26-7; fainter than normal following night. џENIFџEps PegџAB 4.7 F2IV, 5.0 F6IV, 11.558y, a = 0.255". ADS 15281C, 10.8v at 13.8" possibly in hyperbolic orbit about AB or is optical. џADS 15271A, SRc 3.43 - 5.1v, 730d; also a cycle of 4400d. Mean magnitude varies 13.5y. Correspondence between polarization and light. џHerschel's "GarnџMu CepџADS 15314A. Component A is SB, 3.2, 5.2v, 0.0018"; B, 15.8v, 69"; C 12.7v, 120". EA (possibly RS CVn type) 2.83 - 3.05V, 1.0227789d. Form of light curve varies. џDeneb AlgediџDel CapџAlpha Cyg 4.25 - 4.35V, 7.6:d. џNu Cepџ5.1 F0IV, 5.1 F0IV, 6.094y, a = 0.127", or 12.242y, a = 0.160". Combined mag., colors. џHe 10830 possibly variable. џSADALMELIKџAB 4.61 A3m, 6.5 F7V or F3III-IV, 3800y, a = 11.5". Aa, 2.254y, a = 0.073". Component B is HD 209791 = GC 30876, vsini =<25k/s. Component C, 12.7v at 97" optical. џAlkurhahџALNAIRџOptical. џDelta Sct? џBahamџB, optical. џDelta Sct 4.15 - 4.20V, 0.04242 and 0.068073d. Period and amp. vary. џEps CepџOptical. џSadalachbiaџCPM companion F5III, optical. џBinary with HR 8558. AB 4.31 F2IV, 4.51 F3IV, 856.0y, a = 5.055". Magnitude for blend 3.65V, combined colors. Component B, HR 8558, is an astrometric binary. џLb? 3.99 - 4.20V. џDel2 GruџB, 13v at 21" optical. AC CPM, C at 41", 6.30V, -0.03(B-V), -0.35(U-B), B7IV, RV -21k/s, vsini 135k/s. ADS 15987A, CDelta 3.48 - 4.34V, 5.366341d. Period varies. Prototype star Delta Cep, discovered by Goodricke in 1784 Blue companion ADS 15987C is also var. and SB. џDel CepџCPM. Companion D G2? Photometric data (Oblak 1978, A&AS, 34, 453) give B A2V, 6.22V,; C F2V, 7.71V, +0.38(B-V); D F9V, 7.83V, +0.51(B-V), where MK types are estimated from uvby,beta photometry. ABD physical, C optical. џOptical. џLc? 2.0 - 2.3V. џBet GruџA* 2.94 G2II-III, 2.23y, a = 0.022". Speckle interferometry measures range from unresolved to sep. 0.059". BC, 10.0, 10.0v sep. 0.2" at 90" from A, physical. ADS 16211A. џMatar.џAB binary. B 12v M1 at 12"; C, optical. џLb 3.70 - 3.80V. џLam AqrџSkatџCPM. Companion G3. џBY 6.44 - 6.49V, 10d. џFomalhaut is a bright, white star that lies only 22 [G/light year]s away. It diameter is twice that of our [G/Sun] and it is 14 times more [G/luminous] CPM with HR 8721. џFOMALHAUTџSep. 0.02", but duplicity uncertain. Unresolved by speckle interferometry. џSeparate speckle interferometric measures give sep. 0.05" (Aa) and 0.34" (AB). Ten years of observations reveal steady change in AB position angle of about 10d with decrease in separation from about 0.375" to 0.266". Component B identified as SB2 (see SB remarks), making total number of components at least 4. Gamma Cas 3.58 - 3.65V. Photometric investigations have indicated numerous periods, particularly 0.78823, 1.0815d and 1.5998398d, all doubtful. Form of light curve varies. Probably not an eclipsing binary. Period shell phenomena abou 23.5y. Shell features have vanished several times since 1897. H gamma varies in 3.66?d. џOmi AndџLb 2.31 - 2.74V. џSCHEATџBet PegџThe star Markab makes up the southwest corner of the Great Square o [X/Pegasus]. It is 86 [G/light year]s distant џMARKABџSep. 2.9" observed 1925; single in 1929. џAB 4.6 G2III, 6.6 F3V, 150y, a = 0.86". Combined mag., colors. Companion may be collapsed star. џAstrometric binary unresolved by speckle interferometry. Amp. 0.02B. џBC, 10.0, 10.5v, K3V, 130y, a = 0.6", mean mass BC 0.35 solar. BC combined, 9.19V, +1.03(B-V), +0.93(U-B), CPM with A. Component C is a close double, equal components, showing orbital motion. џHigh space velocity? џSuspected occultation double. џAlpha CV? 4.36 - 4.39V. џRS 3.69 - 3.97V, 4.74 - 5.13B, 54.20d. Amp. and cycle length vary in period 3200d. Also 0.25m var. in period about 50d. H and K emission correlated with 56d light period. џLam AndџOptical. џAlraiџComponent B, CPM, A5Vep; however, the companion is optical. џLb? 4.35 - 4.41V. џYY PscџThe [G/constellation] Andromeda is named for the mythical daughter of King [Y/Cepheus] and Queen [Y/Cassiopeia]. To save their kingdom, Andromeda's parents were told they must sacrifice their daughter to the sea monster, [Y/Cetus]. Andromeda was chained to the rocks by the sea to await her fate. Fortunately, [Y/Perseus], riding the winged horse [Y/Pegasus], flew over the kingdom. He saw the princess chained to the rocks and flew down to rescue her. In the sky, Andromeda is shaped like the capital letter "A" with her head at the point of the "A", her belt at the central line of the "A" and her feet at the base of the "A". Her brightest [G/star] is [W/Alpheratz], the star at the top of "A" and one of the stars in the Great Square of [Y/Pegasus]. Andromeda is best seen from October-December. "Must See" objects include: [F/Andromeda Galaxy]; [N/NGC 752], a star [G/cluster]. џAntlia is a relatively modern [G/constellation]. It was added to the charts in 1752. This is a faint constellation, with no stars brighter than [G/magnitude] 4.2. Its brightest [G/star] is Alpha Antlia ([S/201405]). Antlia is best seen from April-June. џApus is a faint [G/constellation], with 5 of its 6 brightest stars reddish in color. The brightest [G/star] in Apus is Alpha Apodis ([S/257193]). This constellation is best seen from May-August in the southern hemisphere. џThe [G/constellation] Aquarius is associated with water in the mythology of many cultures, perhaps because Aquarius rises during autumn in the northern hemisphere - the rainy season for many countries. In Greek mythology, Aquarius caused a great flood that covered the Earth. To the Egyptians, Aquarius poured water into the Nile river each year, causing it to flood. The brightest [G/star] in Aquarius is Sadalsuud [S/145457]. Four stars make up the "Water Jar" of Aquarius: three stars forming a triangle with a fourth star in the center. Stars representing water are pouring from the jar. Aquarius is best seen from September-December. "Must See" objects include: [M/M2], a star [G/cluster]; the [F/Saturn Nebula], a [G/planetary nebula]; [F/Helix Nebula], a [G/planetary nebula]. џIn Greek mythology, Aquila was the eagle who served Zeus. Aquila carried the god's thunderbolts and delivered messages for him. In Chinese legends, the brightest [G/star] in Aquila, [W/Altair], represented one of two lovers in the tale of the herd boy and the weaving girl. Altair was the hard working herd boy, who fell in love with the weaving girl, a beautiful visitor from the stars. In the sky, three stars form the head of the eagle; Altair is the center star with a fainter star on each side. This [G/constellation] lies along the [G/Milky Way]. Look for dark lanes of dust (areas with fewer stars) in this region. Aquila is best seen from August-October. џAra is a modern [G/constellation] lying just below the curving tail of [Y/Scorpius]. Its brightest star is Beta Arae [S/244725]. Ara is best seen from July-September in the southern hemisphere. џIn Greek mythology, Aries was a ram with a beautiful golden fleece. This golden ram was identified with Zeus, the king of the gods. In Egyptian mythology, the celestial ram was thought to be Ammon, the Sun god. This faint [G/constellation] was identified with the bright Sun and shiny gold because of its location along the [G/zodiac]. Ancient people noted that when the [G/Sun] was in the constellation of Aries, this marked the beginning of spring and the growing season. Its brightest star is [W/Hamal]. Today, Aries is best seen from October-February. џAuriga is a strange [G/constellation], representing a charioteer who is carrying a goat on his shoulder and holding three baby goats in his arms. The brightest [G/star] in Auriga is [W/Capella]. The three baby goats, also known as "The Kids," are represented by three stars forming a narrow triangle, just south of Capella. Auriga is best seen from January-March. "Must see" objects include: three galactic [G/cluster]s, [M/M36], [M/M37], and [M/M38]. џBootes was placed in the sky to guard the great bear, [Y/Ursa Major]. As a result, Bootes can be seen following the bear around the sky once a day. The brightest star in Bootes, [W/Arcturus], can be found by using stars in the [G/Big Dipper] to point the way. If you connect the three stars in the handle of the Dipper, this forms an arc. Follow this arc to Arcturus. Bootes is shaped like an ice cream cone, with Arcturus at the tip of the triangular cone. Two stars finish the cone and there is a small scoop of ice cream on top. Bootes is best seen from June-August. џCaelum is a small, faint constellation with no [G/star]s brighter than [G/magnitude] 4.5. Its brightest star is Alpha Caeli [S/216926]. Caelum is best seen from January-February. џCamelopardalis was added to the charts in 1690. There are no stars brighter than [G/magnitude] 4.0 in this area of the sky. There is also no easy-to-identify pattern. Its brightest [G/star] is Beta Camelopardalis [S/13351]. This constellation is [G/circumpolar], meaning it is visible year round from most of the northern hemisphere. It is best seen from December-February. џCancer is the faintest of all the [G/constellation]s of the [G/zodiac] and is best viewed under dark skies when the [G/Moon] is not visible. In Greek mythology, Cancer the crab lived in a swamp with the [Y/Hydra]. When [Y/Hercules] came to kill the Hydra, Cancer tried to save his friend by biting Hercules on the foot. Hercules merely killed the crab and brushed it aside. Cancer was given a place in the sky, to honor him for sacrificing his life for a friend. The brightest [G/star] in Cancer is Altarf [S/116569]. This constellation is best seen from March-May. "Must See" objects include: the [F/Praesepe] cluster. џThe brightest [G/star] in Canes Venatici is [W/Cor Caroli] and it represents one of two hunting dogs in this [G/constellation]. Cor Caroli (the Heart of Charles) was probably named after King Charles I of England, but this bright star is usually associated with the coronation of King Charles II in 1660. The second hunting dog is represented by Beta [S/44230]. This constellation is best seen from May-July. "Must See" objects include: [F/Whirlpool Galaxy]; [M/M3], a globular [G/cluster]; [M/M94], a spiral [G/galaxy]. џCanis Major, lying next to the mighty hunter [Y/Orion], is sometimes known as Orion's hunting dog. Its brightest star, [W/Sirius], is also the brightest [G/star] in the night sky and has been worshipped and feared by many cultures. In the past, Sirius (also known as the Dog Star) rose and set with the Sun during the hottest days of summer, causing it to be blamed for the scorching summer heat. As a result, the phrase "Dog Days of Summer" can be associated with this [G/constellation]. Canis Major is best seen in the night sky from February-April. "Must See" objects include: [M/M41], a galactic [G/cluster]; [N/NGC 2362], a galactic [G/cluster]. џCanis Minor is the smallest of [Y/Orion]'s two hunting dogs. The brightest [G/star] in this small [G/constellation] is [W/Procyon]. Procyon forms a triangle with two other bright winter stars, [W/Sirius] and [W/Betelgeuse]. Canis Minor is best seen from February-April. џCapricornus is one of the older [G/constellation], although its origin as a half goat-half fish is not clear. According to one Greek myth, Capricornus was Aegipan, a half man, half goat whose father was Zeus. Once, while helping his father, Aegipan was pursued by Typhon, the monster god. To avoid Typhon, Aegian ran into a river. When he was waist-deep in the water, he changed the lower part of his body into a fish and swam to safety. Zeus placed Aegipan in the sky, as a way of thanking him for his help. The brightest [G/star] in this constellation is Deneb Algedi [S/164644]. Capricornus is best seen from September-November. џCarina, originally part of the ancient [G/constellation] of Argo, the ship, is best seen from the southern hemisphere. Its brightest [G/star] is [W/Canopus], the second brightest star in the night sky. ([W/Sirius] is the brightest.) Carina is best seen from March-May. "Must See" objects include three galactic [G/cluster]s: [N/NGC 2516]; [N/NGC 3532]; [C/C102]. џIn Greek mythology, Queen Cassiopeia, along with her husband, King [Y/Cepheus] ruled over Ethiopia. Cassiopeia was very beautiful, but boastful and arrogant as well. She once boasted that she was even more beautiful than the sea nymphs. This claim angered the sea nymphs, whose beauty was legendary. They complained to Poseidon, the god of the sea, who sent [Y/Cetus], a sea monster, to destroy Ethiopia. Cassiopeia and Cepheus were forced to sacrifice their daughter, [Y/Andromeda] to save their kingdom. Fortunately, Andromeda was saved by [Y/Perseus] and [Y/Pegasus]. Cassiopeia sits on her throne in the sky, with her brightest stars forming a "W" or "M" shape, depending on the season. The brightest [G/star] is [W/SHEDIR] which lies at the lower right vertex of the "W". Because of her placement in the sky, half the time her royal throne is upside down. The queen must be chained to the chair so she won't fall out. This awkward position is part of her punishment for being so vain. Cassiopeia is a [G/circumpolar] constellation and can be seen most of the year. However, she is best seen from September to December. "Must See" objects include four galactic [G/cluster]s: [M/M103]; [N/NGC 457]; [N/NGC 7789]; [N/NGC 663]. џIn Greek mythology, Centaurus was the first of the Centaurs, a race of beings with the head, arms and chest of a man and the body of a horse. The brightest [G/star] in this [G/constellation] is Alpha Centauri, [S/252838]. It is also the closest star to our solar system. Alpha Centauri along with Agena [S/252582] make up the "Pointers", two bright stars that point the way to the [G/Southern Cross]. Centaurus is best seen from May-July in the southern hemisphere. "Must See" objects include: [F/Omega Centauri], a globular [G/cluster]; [F/Centaurus A], a peculiar [G/galaxy]. џIn Greek mythology, King Cepheus ruled over the country of Ethiopia with his beautiful, but vain, wife [Y/Cassiopeia]. Cepheus was forced to sacrifice his daughter [Y/Andromeda] to save his kingdom from [Y/Cetus] the sea monster. As fortune would have it, Andromeda was rescued by [Y/Perseus] and [Y/Pegasus] and the sea monster was killed. Peace was restored to the kingdom. The stars in this [G/constellation] form a box with a triangle sitting on top. The brightest [G/star] in Cepheus is [W/Alderamin]. This constellation is [G/circumpolar] and can be seen most of the year. However, it is best seen from September-December. "Must See" objects include: [N/NGC 188], a galactic [G/cluster]. џCetus, the sea monster, was sent to destroy the kingdom of King [Y/Cepheus] and Queen [Y/Cassiopeia]. But, before he could complete his task, he was killed by [Y/Perseus]. The brightest [G/star] in the [G/constellation] is [W/Diphda]. Cetus is best seen from October-December. "Must See" objects include: [W/Mira], a variable star. џChamaeleon was added to the charts in the early 1600's and is considered a modern [G/constellation]. It is small in size and shaped like an elongated diamond. Its brightest [G/star] is Alpha Chamaeleont [S/256496]. Chamaeleon is [G/circumpolar] and can be seen most of the year from the southern hemisphere. џThis small, narrow "V"-shaped [G/constellation] lies close to the "Pointers", the two brightest stars of [Y/Centaurus]. Circinus is a modern constellation, added to the charts in the mid 1700's. It contains a few relatively faint [G/star]s, the brightest of which is Alpha Circini [S/252853]. Circinus is best seen from July-September in the southern hemisphere. џThe brightest [G/star] in this [G/constellation] is Phact [S/196059]. Columba is best seen from January-March in the southern hemisphere. "Must See" objects include: [N/NGC 1851], a globular [G/cluster]. џComa Berenices was named after Berenices II who, along with her king, ruled Egypt around the year 230 BC. With the king at war, Berenices offered to sacrifice her long golden hair to the goddess Aphrodite to insure the safe return of her husband. When the war was over, the king returned safe and sound and Berenice kept her promise. She cut her hair and left the golden tresses on an alter as a gift to the goddess. The next morning, the tresses were gone. Local astronomers convinced the king and queen that the golden tresses had been transported into the sky where they would forever sparkle among the stars. Today, the [G/constellation] consists of a scattering of faint stars, most of which belong to an extremely large galactic [G/cluster] known as the [G/Coma Star Cluster]. The brightest star in this constellation is Diadem [S/100443]. Coma Berenices also contains a wide assortment of galaxies. Unfortunately, most are too faint to be seen with a small telescope. Coma Berenices is best seen from May-July. "Must See" objects include: [M/M53], a globular cluster. џCorona Australis is shaped like a "C" and lies just below the "Teapot" of [Y/Sagittarius]. The brightest [G/star] in the [G/constellation] is Alfecca Meridiana [S/210990]. Corona Australis is best seen from August-October. џIn Greek mythology, the god Bacchus created a beautiful crown which he gave to his mortal wife. Upon her death, he placed the crown in the sky as a tribute to his wife's great kindness and beauty. To the Shawnee Indians, the stars of this [G/constellation] represent celestial sisters. The circle of stars is incomplete because one sister left the sky to marry a human. The stars in Corona Borealis are shaped like the letter "C". Its brightest star is [W/Alphekka]. This constellation is best seen from July-September. џIn Greek mythology, Corvus was the messenger raven for the god Apollo. One of raven's many tasks included bringing water to the god when he was thirsty. One day, Corvus was about to fill a goblet with water when he noticed a fruit tree in bloom. He decided to wait until the fruit was ripe so that he could have a snack before returning to Apollo. Corvus waited several days for the fruit to ripen. Finally, he ate his fill of the ripe, fresh fruit and started back to Mount Olympus. Along the way, he realized that Apollo might be angry with him for taking so long to fetch the water. Thinking fast, he swooped down and snatched a water serpent from the river. Then, when he returned the goblet of water to Apollo, Corvus explained that the water serpent had attacked him, causing him to be late. Apollo did not believe the raven's story and flung the raven, the goblet and the water serpent into the sky where they would not bother him again. Today, the raven, or Crow (Corvus), the goblet ([Y/Crater]), and the sea serpent ([Y/Hydra]) are all constellations. The brighter stars of Corvus form a lopsided rectangle in the sky. Its brightest [G/star] is Gienah [S/157176]. Corvus is best seen from April-June. џIn Greek mythology, Crater represented a water goblet which belonged to the god Apollo. [Y/Corvus] the crow used the goblet to gather water for the god when he was thirsty. Crater was caught in the middle of a fight when Corvus tried to lie to Apollo. In a fit of rage, Apollo flung both the crow and the goblet into the sky. To many cultures, Crater represented a cup, bowl, or some other type of container used to hold wine. The brightest star in Crater is Delta Crateris [S/156605]. Crater is best seen from April-June. џEven though Crux is the smallest [G/constellation] in the sky, it contains some of the richest starfields of our [G/Milky Way] galaxy. Originally, Crux was part of the constellation [Y/Centaurus]. Today, its brightest stars appear in the shape of a cross. The brightest star in Crux is [W/Acrux], a fine double star system. Crux is best seen from April-June. "Must See" objects include: [F/Jewel Box] cluster; [F/Coal Sack] nebula. џCygnus, which is also known as the Northern Cross, lies along the hazy patch of light that makes up our [G/Milky Way] galaxy. One Greek myth tells how Cygnus represents Zeus, the king of the gods. Zeus once turned himself into a swan to seduce the lovely mortal woman, Leda. Leda then laid an egg and when the egg hatched, the beautiful Helen of Troy was born. Another myth tells that Cygnus was the best friend of Phaethon. Phaethon had discovered that his real father was Apollo, the Sun god. He went to visit Apollo and watched as his father drove the Sun's chariot across the sky once a day, bringing daylight to the world. Phaethon demanded that he be allowed to drive the chariot, and before Apollo could stop him, he grabbed the reins of the chariot and took off. The four fiery horses pulling the chariot went wild and Phaethon lost control. To save Earth from the runaway Sun chariot, Zeus was forced to fling a lightening bolt and killed Phaethon. Phaethon's body plunged to Earth and fell into the river [Y/Eridanus] while the horses safely returned the Sun's chariot to Apollo. Phaethon's friend, Cygnus, searched the river, but he never found his friend. He continued swimming back and forth, diving deep into the river's depths, reminding those who watched him of a swan. For his devotion to his friend, Cygnus was honored with a place in the sky. Today, he can be seen as the swan flying south along the [G/Milky Way]. The [G/star] at the tail of the swan is also the brightest star in the [G/constellation]. Its name is [W/Deneb]. Cygnus is best seen from August-November. "Must See" objects include: [W/Albireo], a double star; the [G/Milky Way]; [F/Cygnus X-1], a black hole. џTo many cultures, the stars in Delphinus represented a dolphin or porpoise. In one myth, a dolphin rescued a man about to be killed by pirates. The man had jumped overboard and the dolphin helped him back to shore. For his good deed, the dolphin was honored with his own place in the sky. Five stars in the shape of a diamond form the dolphin's body, with two stars trailing off the diamond, forming the dolphin's tail. The brightest [G/star] in Delphinus is Rotanev [S/106316]. This [G/constellation] is best seen from August-October. џDorado was added to the charts in the early 1600's and is considered a modern [G/constellation]. Its brightest [G/star] is Alpha Doradus [S/233564]. Dorado is best seen from December-February from the southern hemisphere. "Must See" objects include: The [F/Large Magellanic Cloud], a [G/galaxy], the [F/Tarantula Nebula], a nebula within the Large Magellanic Cloud. џIn Greek mythology, Draco was the dragon in charge of guarding the garden of Hera, the queen of the gods. Within the garden, there were trees on which grew golden apples. [Y/Hercules] had to steal these golden apples as one of his 12 labors. Before he could steal them, however, he had to kill Draco. Draco fought a mighty battle, but he was no match for Hercules. After his death, Hera gave Draco an honored place among the stars. Three stars forming the tail of the dragon lie between the [G/Big Dipper] and [G/Little Dipper]. From the tail, Draco curls around the Little Dipper like a backwards "S". Its head is made up of four stars in the shape of a lopsided square. The brightest star in Draco is [W/Etamin] and it, along with the entire constellation, is best seen from July-September. "Must See" objects include: [W/Thuban], a star which was the "North" star 4,800 years ago. џThe stars of this small [G/constellation] may once have been combined with the stars of [Y/Delphinus] to form a larger constellation. However, the two were divided into individual constellations somewhere around the second century BC. Today, Equuleus lies between Delphinus and the head of [Y/Pegasus]. Its brightest [G/star] is Kitalpha [S/126662]. This constellation is best seen from August-October. џEridanus, the river, meanders all over the sky. In Greek mythology, it was this river that the body of Phaethon plunged into after his foolish ride across the sky in the chariot of the Sun. (You may refer to the constellation [Y/Cygnus] for the entire story of Phaethon.) Eridanus begins with the star Zaurak [S/149283], which lies next to the star [W/Rigel] in the constellation of [Y/Orion]. From there, Eridanus wanders below [Y/Cetus], around [Y/Fornax], above [Y/Horologium] and finally comes to an end between [Y/Phoenix] and [Y/Hydrus]. Its brightest star, [W/Achernar], lies so far south that it can't be seen from Europe, Japan and most of the U.S. This [G/constellation] is best seen from December-February. џThis small, faint group of stars is a modern [G/constellation] that was added to the charts in the late 1700's. Fornax lies next to [Y/Eridanus] in the sky. Its brightest [G/star] is Fornacis [S/168373]. This constellation is best seen from December-February. џThe stars in Gemini have been referred to as the "Twins" by many cultures around the world, with each culture offering a different story about the celestial brothers. One Greek myth tells that the twins are sons of Zeus, the king of the gods, and a mortal woman, Leda. The twins are also associated with "St. Elmo's Fire", an electric glow seen around aircraft wings or a ship's rigging during stormy weather. [W/Pollux], the brightest [G/star] in this [G/constellation], and a faint companion star form the head of one twin. The second brightest star in the constellation, [W/Castor], along with a fainter companion, forms the head of the second twin, with the twins standing side by side in the sky. Gemini is best seen from January-April. "Must See" objects include: [M/M35], a galactic cluster. џGrus is a modern [G/constellation], added to the charts in the early 1600's. It is also part of a group of constellations known as the Southern Birds. The other birds of the group are the [Y/Phoenix], [Y/Pavo] the peacock, and [Y/Tucana] the toucan. The brightest [G/star] in Grus is [W/Alnair], a hot blue star. The second brightest star, Beta, [S/231258] is a cooler, orange-colored star. Compare the two and try to detect the differences in color. Grus is best seen from September-November in the southern hemisphere. џHercules was the son of Zeus, the king of the gods, and a mortal woman, Alcmene. Even as a young child, Hercules possessed a tremendous strength. When he was 8 months old, he strangled 2 serpents that had been sent to his crib by Hera, the jealous wife of Zeus. Hera's jealousy was to haunt Hercules for most of his life. At one point, she caused him to go insane. During this time of madness, Hercules killed his wife and children. When he awoke from the insanity, he saw the horror of what he had done and was overcome with grief. He left his village and traveled to the Oracle of Delphi for advice. The oracle told him to travel to Tiryns where King Eurystheus would assign Hercules 12 difficult labors. If and when Hercules completed all the labors, he would be freed from his sins and raised to the rank of godhood. For many years, Hercules struggled to complete the 12 labors, each more difficult than the last. Some of his opponents can be found in the sky, including [Y/Leo], the lion; [Y/Hydra], the many-headed serpent; [Y/Cancer], the crab; and [Y/Draco], the dragon. After many years, he successfully completed the 12 labors. When Hercules died, the gods welcomed him to Mount Olympus, where he was granted godhood, just as the Oracle had foreseen. Today, Hercules can be found next to the head of Draco. Four stars make up the "Keystone", or body of the mighty warrior. The brightest [G/star] in the [G/constellation] is Kornephoros [S/84411]. Hercules is best seen from July-September. "Must See" objects include: two globular [G/cluster]s, [M/M13] and [M/M92]. џThis small, faint group of stars is considered a modern [G/constellation], added to the charts in the 1700's. Its brightest [G/star] is Alpha Horologii [S/216710]. Horologium is best seen from December-February in the southern hemisphere. џHydra is the largest [G/constellation] in the sky. Its stars snake across over one quarter of the heavens. This constellation figures prominently in two Greek myths. In one myth, Hydra was a many-headed monster who lived in a swamp, along with her only companion, [Y/Cancer] the crab. [Y/Hercules] was sent to kill the monster as one of his twelve labors. The two fought a tremendous battle. For every head Hercules chopped off, Hydra grew two more in its place. Finally, Hercules won and the gods placed the body of Hydra in the sky. In another myth, Hydra was an innocent water serpent who was scooped out of a river by [Y/Corvus] the crow. The brightest [G/star] in Hydra is [W/Alphard]. Because Hydra is such a long constellation, various parts of it can be seen beginning in March and stretching through August. "Must See" objects include: [M/M48], a galactic [G/cluster]; [M/M68], a globular cluster; [M/M83], a spiral [G/galaxy]. џThis modern [G/constellation] was added to the charts in the early 1600's. Its brightest [G/star] is Beta Hydri [S/255670]. This star is the closest bright star to the south [G/celestial pole], even though it is over 12^ away. Hydrus is a [G/circumpolar] constellation and can be seen most of the year in the southern hemisphere. However, it is best seen from December-January. џIndus is a rather small, faint [G/constellation] which lies next to the brighter constellation of [Y/Grus]. Its brightest [G/star] is Alpha Indi [S/230300]. Indus is best seen from September-November in the southern hemisphere. џLacerta is a relatively modern [G/constellation], added to the charts in 1690. It is a small, faint group of stars not far from the constellation of [Y/Cygnus]. The brightest [G/star] in Lacerta is Alpha Lacertae [S/34542]. The lizard's head is made up of four stars in the shape of a diamond. A trail of faint stars coming off the diamond forms the lizard's body. Lacerta is best seen from September-November. џIn Greek mythology, Leo is associated with the Nemean lion, a fierce creature who came from the Moon. [Y/Hercules] was given the difficult task of killing the ferocious beast. The lion's hide was so tough, no weapon could pierce through it. Arrows that Hercules flung at the beast merely bounced off its chest. Abandoning his useless weapons, Hercules trapped the lion and used his own incredible strength to strangle the creature. The lion's body was then placed in the sky by Hera, the queen of the gods and an enemy of Hercules. The [G/constellation] of Leo has long been associated with the [G/Sun] and hot summer days because, for 4,000 years, the Sun rose in this area of sky on the Summer [G/Solstice], the first day of summer in the northern hemisphere. Today, because of the [G/precession] of the Earth, Leo rises with the Sun in late July and early August. In the sky, the head, mane and chest of the lion are represented by a pattern of stars in the shape of a sickle or backwards question mark. The [G/star] at the handle of the sickle, or the "period" of the question mark, represents the heart of the lion. This star, called [W/Regulus], is the brightest star in Leo. The lion's hindquarters are represented by a small triangle containing [W/Denebola], a bright star whose name means the "Tail of the Lion". Leo is best seen from March-June. "Must See" objects include: two spiral galaxies, [M/M65] and [M/M66]. џLeo Minor was added to the charts in 1690. It is a small, faint [G/constellation] that lies between the scoop of the [G/Big Dipper] and the sickle of [Y/Leo]. Its brightest [G/star] is Praecipua [S/62297]. Leo Minor is best seen from March-May. џThis little hare lives a rather hectic life, positioned in the sky next to a big dog, [Y/Canis Major], and just below the feet of the mighty hunter, [Y/Orion]. Its brightest star is [W/Arneb]. Lepus is best seen from January-March. џOf all the [G/constellation]s of the [G/zodiac], Libra is the only one that does not represent a living being. However, the name of its brightest star, Zuben Elschemali [S/140430] (which means the northern claw) indicates that this area of sky was once part of the constellation of [Y/Scorpius]. Libra is best seen from June-July. џLupus is one of the original 48 [G/constellation]s placed in the sky by the ancient astronomer, Ptolemy. It contains several bright [G/star]s, but no easy-to-identify pattern. Its brightest star is Alpha Lupi [S/225128]. Lupus is best seen from June-July. џThe faint [G/constellation] of Lynx was added to the charts in 1690. Its brightest [G/star] is Alpha Lyncis [S/61414]. Lynx is best seen from February-April. "Must See" objects include: [N/NGC 2419], a globular [G/cluster] џIn Greek mythology, Lyra represented a beautiful lyre which had been fashioned from an empty tortoise shell. Orpheus, the son of Apollo, inherited the lyre from his father. When Orpheus played the lyre, his music was so beautiful it was said to charm anyone who heard it. Orpheus fell in love and married the beautiful Eurydice. The two lovers were extremely happy, but soon after their marriage, Eurydice was poisoned by a snake and died. Orpheus' grief was overwhelming. He took his lyre to the edge of the Underworld, where all mortal souls go when they die. There, he played his music. The Lord of the Underworld was so touched by the mournful sounds, that he allowed Eurydice to return to the land of the living. There was one stipulation, however. Orpheus could not look at Eurydice until they had completely left the boundaries of the Underworld. As the two lovers made there way back to the surface, Orpheus tried his best not to look at his wife, but the temptation was too great. Just as they neared the boundary between the two worlds, he glanced in her direction. Even a glance was too much and Eurydice was pulled back into the Underworld, never to return. For the rest of his life, Orpheus grieved over the loss of his wife, playing mournful, beautiful music on his lyre. After his death, the gods immortalized his music by raising the lyre into the stars. In one Chinese legend, Lyra's brightest [G/star], [W/Vega], represents one of two lovers from the tale of the Herd Boy and the Weaving Girl. Vega was the Weaving Girl, who wove beautiful tapestries among the stars. An interesting note about Vega: due to the [G/precession] of Earth's rotation, Vega was the "north" star 12,000 years ago, and will be again in another 12,000 years. Lyra is best seen from June-September. "Must See" objects include: the [F/Ring Nebula], a planetary nebula; Epsilon Lyra ([S/67310]), a double/double star; [M/M56], a globular cluster. џThis small group of stars holds the record for being the faintest of all the [G/constellation]s in the sky. None of the [G/star]s within this group are brighter than [G/magnitude] 5. In fact, its brightest star, Alpha Mensae ([S/256274]) is only magnitude 5.1. Mensa is a [G/circumpolar] constellation and can be seen year round from the southern hemisphere. "Must See" objects include: a small portion of the [F/Large Magellanic Cloud] that extends into this constellation. џMicroscopium is a faint, modern [G/constellation], added to the charts in the 1750's. Its brightest star, Gamma Microscopii [S/212636] is only [G/magnitude] 4.7. Microscopium is best seen from September-October in the southern hemisphere. џMonoceros was added to the charts in the mid 1600's. Although faint, this [G/constellation] is rather easy to find. Simply form a triangle with three bright neighboring stars, [W/Betelgeuse], [W/Sirius], and [W/Procyon]. The area inside the triangle is Monoceros. The light from the brightest [G/star], Beta Monocerotis [S/133316], is actually the combined light from three different stars, one of the best triple star systems in the sky. Monoceros is best seen from February-March. "Must See" objects include: the [F/Rosette Nebula]; [N/NGC 2264], a Christmas-Tree-shaped cluster and nebula; [M/M50], a galactic cluster. џThis [G/constellation] was first listed on the charts in the early 1600's as a Bee. It was transformed to a fly in the mid 1700's. Musca lies between [Y/Crux] and the south [G/celestial pole]. Its brightest [G/star] is Alpha Muscae [S/251974]. Musca is a circumpolar constellation and can be seen year round in the southern hemisphere. However, it is best seen at sunset during May-June. "Must See" objects include: two globular [G/cluster]s, [N/NGC 4833] and [N/NGC 4372]. џNorma is a faint [G/constellation] that was added to the charts during the 1750's. It is best seen during July-August from the southern hemisphere. Its brightest [G/star] is Gamma Normae [S/243643]. "Must See" objects include: two galactic [G/cluster]s, [N/NGC 6067] and [N/NGC 6087]. џThe only claim to fame for this [G/constellation] is that it lies in the vicinity of the south [G/celestial pole]. In fact, one of its fainter [G/star]s, Sigma [S/258857], can be considered the South Star. Its brightest star is Nu Octantis [S/257948]. Octans is a [G/circumpolar] constellation and can be seen year round from the southern hemisphere. џThe legend most often connected with Ophiuchus involves a man named Asclepius, who eventually became the god of medicine. Asclepius once killed a snake that had crawled into his hut. Another snake entered the hut, carrying a strange herb in its mouth. It placed the herb in the mouth of the dead snake. Much to Asclepius' surprise, the first snake came back to life. Asclepius retrieved the strange, life-giving herb from the snake and began using it on humans. The healing power of this herb was great and news of Asclepius traveled quickly. He brought so many people back from the dead that Hades, the lord of the Underworld, complained to Zeus. Hades argued that if Asclepius kept bringing humans back from the dead, they would be essentially immortal. Only gods were supposed to be immortal. Hades convinced Zeus that if he allowed Asclepius to continue, the gods would lose their status among the humans. Zeus admired the skill and healing powers of Asclepius, but was forced to agree with Hades. He flung a lightning bolt and struck down the healer. To honor his skills, Zeus raised his body into the sky. Today, the symbol for medicine is a staff with a serpent wrapped around it, in honor of the snake who first found the healing herb. Ophiuchus is seen in the sky next to the constellation of [Y/Serpens], the serpent, or snake. The brightest [G/star] in Ophiuchus is [W/Rasalhague]. The [G/constellation] is best seen from July-August. "Must See" objects include: [F/Barnard's Star], the second closest star in the night sky; a wide variety of globular [G/cluster]s, including [M/M9]; [M/M10]; [M/M12]; [M/M14]; [M/M19]; [M/M62]. џOrion has been associated with a mighty hunter in many cultures around the world. In Greek mythology, the hunter played a part in many different stories. In one story, Orion fell in love with Artemis, the goddess of the hunt. So great was their love for one another, that each began neglecting their duties so they could spend time together. Warned by her brother, Apollo, to return to her duties, Artemis refused and the animals under her care began to suffer. The Moon, without Artemis to guide it, was unable to rise. Apollo grew angry. One day, when Orion went for a swim in the ocean, Apollo surrounded the hunter with a cloak of light. Apollo then went to Artemis and challenged her that she couldn't hit the center of the patch of light with one of her arrows. Artemis accepted the challenge and her aim was true. The arrow pierced the very center of the patch of light and struck and killed Orion. When his body washed up on shore, with her arrow in his chest, Artemis realized what she had done. She gently placed Orion's body in the sky, where it would stand out among the other stars and where she could visit it every night as she drove her Moon chariot through the sky. In another myth, Orion boasted to Artemis that his skills as a warrior were so great, he could hunt down and kill all the animals on Earth. Artemis and Gaea, the Earth goddess, were alarmed by this claim. To protect her creatures, Gaea sent [Y/Scorpius], the scorpion, to kill Orion with a deadly sting. Orion fought and killed the scorpion, but before it died, Scorpius managed to prick the mighty giant once with its stinger. The scorpion's poison was so strong, Orion died instantly. The two enemies were placed at opposite points in the sky, so that as one rises in the east, the other sets in the west. This placement insures that the two rivals never get close enough to fight. Another story has Orion forever chasing the [F/Pleiades], the seven sisters. The ancient Egyptians worshipped Orion as the Sun god. In the sky, Orion forms an easy-to-identify pattern. The red supergiant [G/star], [W/Betelgeuse] forms one of Orion's shoulders. [W/Rigel], the brightest star in Orion, represents one of Orion's feet. Between Betelgeuse and Rigel lie the belt stars, three evenly-spaced stars of equal brightness. Hanging off of his belt is Orion's sword. Orion is best seen from January-March. "Must See" objects include: the [F/Great Orion Nebula]. џThis [G/constellation] was added to the charts in the early 1600's and represents a peacock, the favorite bird of Hera, the Queen of the Gods. Its brightest [G/star] is the Peacock Star, [S/13060], which lies closer to the constellation of [Y/Indus] than the majority of its own star group. Pavo is best seen from September-October in the southern hemisphere. "Must See" objects include: [N/NGC 6752], a globular cluster. џIn Greek mythology, Pegasus was the beautiful flying horse born from the blood of Medusa, the hideous Gorgon killed by [Y/Perseus]. With Perseus on his back, Pegasus flew around the country. Together, the two rescued the princess [Y/Andromeda] from [Y/Cetus], the sea monster sent to destroy her parent's kingdom. In the sky, the body of the flying horse is represented by four stars forming the "Great Square of Pegasus." The brightest star in the [G/constellation] is [W/Enif], which means "the nose" of the horse. Pegasus is best seen from September-November. "Must See" objects include: [M/M15], a globular cluster. џPerseus was the heroic son of Zeus and the mortal woman Danae. At the request of his mother, Perseus set out to kill the hideous Gorgon, Medusa. Medusa and her two sisters had once bragged that they were more beautiful than the goddess Athene. Their boast angered Athene, who turned the three sisters into hideous monsters with hissing, writhing snakes for hair. So ugly were they, that anyone looking at the sisters was instantly turned to stone. To help prepare for the dangerous task ahead, Perseus asked Hermes, the messenger god, and the goddess Athene for advise. Hermes gave Perseus a pair of winged sandals, which allowed him to silently creep up on the sleeping Gorgon. Athene gave him a shiny shield which he could use as a mirror. With the shield, he was able to slice off Medusa's head by watching her reflection. Because he didn't actually look at her, he wasn't turned to stone. Then, with his eyes closed, he grabbed the Gorgon's head and placed it in a special bag. A few drops of blood spilled out of the bag. From the drops, [Y/Pegasus] the flying horse was born. Perseus jumped onto the back of the horse and flew off to show Athene and Hermes his prize. Along the way, he saw a beautiful maiden chained to a giant rock by the sea. As he flew down to investigate, he saw a sea monster about to attack. The maiden [Y/Andromeda] was to be sacrificed to [Y/Cetus], the sea monster to save the kingdom of King [Y/Cepheus] and Queen [Y/Cassiopeia]. As Perseus swooped down out of the sky, he closed his eyes and pulled the Gorgon's head out of the bag. When the sea monster attacked, it saw the head and was instantly turned to stone. Perseus married Andromeda and they lived happily ever after. The brightest star in the constellation is [W/Mirphak], but the most famous star is [W/Algol], the second brightest star which is sometimes known as the Demon Star. It is also associated with the head of Medusa. Algol is an [G/eclipsing binary] star system whose brightness changes noticeably over a three day period. Perseus is best seen from October-December. "Must See" objects include: [M/M34], a galactic cluster; [N/NGC 869] and [N/NGC 884], two side by side galactic clusters; [N/NGC 1275], a galaxy that is an unusually strong radio source. џStories of the legendary Phoenix can be found in civilizations as far back as the ancient Egyptians and early Romans. However, the [G/constellation] wasn't added to the charts until the early 1600's. The Phoenix was a mythical bird that lived for several hundred years at a time. When it was ready to die, it would build a nest and lie down inside. The Sun's rays then ignited the nest and the Phoenix would burn with the flames. From the ashes of the nest, a tiny worm emerged. This worm grew into a new Phoenix and the cycle repeated itself. In the sky, the Phoenix has its wings extended, with each wing shaped like a triangle. The brightest [G/star] in this [G/constellation], [W/Ankaa], is the only bright star in the entire group. Phoenix is best seen from October-November in the southern hemisphere. џOriginally, this [G/constellation] represented a Painter's Easel. Over time, the "Easel" was dropped and today it is known merely as the Painter. This faint, narrow group of [G/star]s lies between the bright star [W/Canopus] and the constellation of [Y/Dorado]. Its brightest star is Alpha Pictoris [S/249647]. "Must See" objects include: Beta Pictoris [S/234134], an excellent candidate for extra solar system planets. џPisces is made up of two fish who, according to Greek mythology, represent the goddess Aphrodite and her son. The two were being pursued by the terrible monster god, Typhon (who also chased after [Y/Capricornus]). To escape from Typhon, Aphrodite and her son jumped into a river and turned themselves into fish. They tied their tails together with a long rope so they would not be separated and swam to safety. In the sky, Pisces is a faint [G/constellation] extending over a large area of sky. It is therefore sometimes difficult to locate. The most identifiable part of the constellation is the "Circlet", five faint stars forming a pentagon. The brightest star in Pisces is Alpherg, [S/92484]. Pisces is best seen from October-December. "Must See" objects include: Zeta Piscium [S/109739], a fine double star with color. џThis small, faint [G/constellation] contains only one bright [G/star], [W/Fomalhaut]. This star, sometimes called the Solitary One, is only 22 [G/light year]s away and is the 18th brightest star in the night sky. Data from the [G/IRAS] satellite shows a cloud of cool material surrounding this star, which could be the beginning of a planetary system. Piscus Austrinus is best seen from October-November. џPuppis was originally part of the large [G/constellation] of Argo, the southern sailing ship. In the mid 1700's, Argo was divided into several smaller constellations, most retaining the nautical theme. In the sky, Puppis represents the stern of a ship. A small section of the constellation lies to the left of [W/Sirius], with the majority of stars lying below [Y/Canis Major]. Its brightest [G/star] is Naos, [S/198752]. Puppis is best seen from March-April. "Must See" objects include four galactic clusters: [M/M46]; [M/M47]; [M/M93]; [N/NGC 2477]. џOriginally part of the [G/constellation] of Argo, the sailing ship, Pyxis represents a compass. Its three brightest [G/star]s form a simple line in the sky. The brightest star in this group is Alpha Pyxidis, [S/199546]. Pyxis is best seen from March-April. џReticulum is considered a modern [G/constellation]. It is sometimes known as a net, although today it is most often associated with a reticle (a set of crosshairs found in some eyepieces to aid in the centering of objects in a telescope). It is a compact group of stars lying just north of the [F/Large Magellanic Cloud]. The stars within the group form a rather lopsided "W". The brightest [G/star] in Reticulum is Alpha Reticuli, [S/248969]. Reticulum is best seen from December-January in the southern hemisphere. џFrom Cupid to Hercules, this tiny arrow has been associated with many heroes around the world. Lying between the bright stars [W/Altair] and [W/Albireo], Sagitta consists of four main stars: two stars form the arrow's shaft and two stars, side by side, represent the arrow's fletchings (feathers designed to balance the arrow in flight). The brightest [G/star] in this [G/constellation] is Gamma Sagittae, [S/105500]. Sagitta is best seen from August-October. џThe beautiful [G/constellation] of Sagittarius lies directly between our [G/solar system] and the center of the [G/Milky Way]. The brighter [G/star]s, the ones that make up the constellation, are fairly close to us. The stars at the center of our galaxy are 30,000 [G/light year]s distant and are too far away to be [G/resolve]d into individual points of light by the naked eye. Instead, the light from these distant stars blends together and appears as large, glowing clouds. In addition to the star clouds, there are also dust clouds visible in this area. These dust clouds are so thick that they actually block some of the light from the galactic center. In Greek mythology, Sagittarius was a Centaur, a creature with the head, chest and arms of a man and the body of a horse. In the sky, the centaur is holding a large bow and arrow, although seeing that figure in the sky requires a great deal of imagination. For observers in the northern hemisphere, there is an easy-to-identify pattern known as the "Teapot," complete with a spout, lid and curved handle. For observers in the southern hemisphere, the Teapot is upside down. The brightest star in the constellation is [W/Kaus Australis]. Sagittarius is best seen from July-August. "Must See" objects include: [M/M7], a galactic cluster which holds the record for being the southernmost Messier object; three diffuse nebulae ([F/Lagoon Nebula]; the [F/Swan Nebula]; and the [F/Trifid Nebula]); three galactic clusters ([M/M21]; [M/M23]; [M/M25]); several globular clusters ([M/M22]; [M/M28]; [M/M54]; [M/M55]). џFrom Greece and Egypt, to the Americas, cultures around the world have identified this distinct group of stars with a scorpion. In Greek mythology, Scorpius is connected with the [G/constellation] of [Y/Orion] the hunter. Orion once boasted that his hunting skills were so remarkable, he could easily hunt and kill all of the animals on Earth. This boast alarmed the earth goddess, Gaea, whose job it was to protect all creatures. To insure the safety of her animals, she sent a scorpion to kill the mighty hunter. Orion and Scorpius fought a fearsome battle, but in the end, Orion was victorious. However, just before the scorpion died, he lashed out and stung the hunter with his tail. Poisoned by the sting, Orion died instantly. Both were given honored places in the sky, although they were placed far apart from one another. As one rises above the horizon, the other sets. This way, they can never see each other and start fighting again. To the ancient Chinese, this constellation represented a dragon. For observers in the northern hemisphere, Scorpius can be found lying lengthwise across the southern summer sky. Observers in the southern hemisphere can find Scorpius high overhead during winter. The brightest star in the constellation is [W/Antares]. Scorpius is best seen from July-August. "Must See" objects include: three galactic clusters ([F/Butterfly Cluster], [M/M7], [N/NGC 6124]); and two globular clusters ([M/M4]; [M/M80]; the [G/Milky Way]. џSculptor is a faint [G/constellation] that lies just to the east of the bright star [W/Fomalhaut]. Its original name was the "Sculptor's Workshop," but over the years it has been shortened to the "Sculptor." Its brightest star, Alpha Sculptoris [S/166716], is only a [G/magnitude] 4.3 [G/star]. The rest of the stars in the constellation are even fainter. As a result, Sculptor is sometimes difficult to locate. It is best seen from November-December. "Must See" objects include: two galaxies (the [F/Sculptor Galaxy] and [N/NGC 55]. џScutum is considered a modern [G/constellation], added to the charts in 1690. This small group of stars lies along the path of the [G/Milky Way], just north of [Y/Sagittarius]. Its brightest [G/star] is Alpha Scuti ([S/142408]). Scutum is best seen from August-October. "Must See" objects include: two galactic clusters (the [F/Wild Duck Cluster] and [M/M26]. џIn Greek mythology, the [G/constellation] of Serpens is associated with the story of Asclepius, the god of Medicine. Asclepius once killed a snake that had entered his hut. Soon after, another snake entered the hut carrying a strange herb in its mouth. The second snake placed the herb in the mouth of its dead friend who immediately came back to life. Asclepius was amazed. He took the herb from the snake and used its healing powers on humans. Serpens represents the snake with the healing herb, while the constellation of [Y/Ophiuchus] represents the god of medicine. The brightest [G/star] in Serpens is [W/Unukalhai]. This constellation is best seen from July-August. "Must See" objects include: [M/M5], a globular cluster; the [F/Eagle Nebula]. џSextans is considered a modern [G/constellation], added to the charts in 1690. Until that time, the stars in this group had been part of the constellation of [Y/Hydra]. The brightest [G/star] in Sextant, Alpha Sextanis [S/137366] is only [G/magnitude] 4.5. The rest of the stars in the constellation are even fainter, making Sextans rather difficult to locate. Sextans is best seen from April-June. џThe ancient Egyptians associated this [G/constellation] with their Bull-god over 4,000 years ago, making Taurus one of the oldest constellations in the sky. As you may imagine, with 4,000 years of history, there are many stories surrounding this heavenly bull. In Greek mythology alone, there are at least two stories about the bull, both with Zeus, the king of the gods, as the main character. In one story, Zeus fell in love with the maiden Europa. To lure her away from her father's servants, Zeus changed himself into a beautiful white bull with golden horns. Europa climbed onto his back and before she realized what was happening, Zeus waded into the water and began swimming across the ocean. Europa couldn't jump off his back because the water was too deep. He took her to a distant island where he turned back into his original form and they had many children together. Another story tells of Zeus falling in love with the maiden Io. To protect Io from the wrath of his wife, Hera, Zeus turned her into a white cow. Io escaped. Zeus then changed himself into a white bull and roamed the countryside until he found her. The two lovers were happy for a while, until Zeus was forced to return to Hera. In the sky, the face of the bull forms a distinct "V" shaped pattern. Almost every [G/star] in the "V" belongs to the [F/Hyades], a beautiful galactic [G/cluster]. The brightest star in the "V", [W/Aldebaran], is also the brightest star in the constellation. It is known as the red "eye of the bull." While this star appears to lie within the cluster, Aldebaran is actually two times closer to our solar system than the rest of the stars in the cluster. Another distinct star group in Taurus is the [F/Pleiades] (sometimes called the Seven Sisters). Because of its shape in the sky, this compact group of bright stars is sometimes mistaken for the [G/Little Dipper]. Each of these two clusters are surrounded by their own stories and legends. Taurus is best seen from October-December. "Must See" objects include: the [F/Hyades]; the [F/Pleiades]; [M/M1], a supernova remnant. џTelescopium is a modern [G/constellation], placed in the sky in the mid 1700's in honor of the invention of the telescope. Its brightest [G/star] is Alpha Telescopii, [S/229023]. This small, faint constellation can be found just to the south of [Y/Corona Australis]. Telescopium is best seen from August-September in the southern hemisphere. џThis small [G/constellation] is shaped like its namesake. Three stars form a small, narrow triangle in the sky, with a fourth star lying close to the triangle's narrow base. This constellation lies between the larger constellations of [Y/Andromeda] and [Y/Aries]. Its brightest [G/star] is Beta Trianguli, [S/55306]. Triangulum is best seen from October-December. "Must See" objects include: the [F/Pinwheel Galaxy]. џThis [G/constellation] was first added to the charts in the early 1600's. Its three brightest stars form an equilateral triangle. The brightest [G/star] is Alpha Trianguli Australe, [S/253700]. This group of stars is a [G/circumpolar] constellation and can be seen year round from the southern hemisphere. "Must See" objects include: [N/NGC 6025], a galactic cluster. џTucana is the faintest [G/constellation] in the group known as the "Southern Birds". Other "southern birds" include [Y/Grus], [Y/Pavo], and [Y/Phoenix]. Though the stars within Tucana are fairly faint, this constellation is easy to locate because the [F/Small Magellanic Cloud] lies within its boundaries and is easily visible to the [G/naked eye]. The brightest star in Tucana is Alpha Tucanae, [S/255193]. "Must See" objects include: The [F/Small Magellanic Cloud]; two globular clusters, [F/47 Tucanae] and [N/NGC 362]; Beta Tucanae, [S/248201] a sextuple star system. џUrsa Major contains the most famous seven stars in the northern hemisphere. Known as the [G/Big Dipper], the Plough, or the Chariot, these seven stars represent just a small portion of the great bear. Indian tribes in North America associated the bowl of the dipper as the main body of the bear with the stars of its handle representing hunters chasing the bear around the sky. Look closely at the middle [G/star] and you can see that the second hunter is carrying a cooking pot (a faint second star) on his back. That second star in the handle is [W/Mizar]/Alcor, a visual double star system. In Greek mythology, the Great Bear represents the maiden, Callisto. Zeus, the king of the gods, fell in love with the beautiful maiden. His jealous wife, Hera, turned Callisto into a bear, so the maiden would no longer catch the eye of her husband. As Callisto wandered the forests as a bear, she came across a young hunter whom she recognized as her son. When she rose up on her hind legs to greet the young man, the hunter was scared. He did not know this mighty beast was his mother. He took aim at the bear with his spear. Just before he threw the deadly weapon, Zeus saw the confrontation and intervened. He turned the son into a bear, then picked up both mother and son by their tails and placed them in the sky. Today, Callisto's son, [Y/Ursa Minor] follows his mother around the sky. The brightest star in this constellation is [W/Alioth], the first star in the handle of the dipper as it is seen coming off the scoop. Alioth is just a little brighter than its second brightest star, [W/Dubhe], the first star in the dipper's scoop, across from where the handle attaches to the scoop. Ursa Major is a [G/circumpolar] constellation for many in the northern hemisphere, but it is best seen high in the sky from April-June. "Must See" objects include: two spiral galaxies, [M/M81] and [M/M82]. џThis [G/constellation] contains the most famous star in the northern hemisphere, [W/Polaris], or the North Star. Many people believe that the North Star is the brightest star in the sky. This is not the case. In fact, Polaris ranks about 50th on the list of bright stars. The reason Polaris is mentioned frequently is because of its location in the sky. It lines up almost directly with Earth's north celestial pole. Polaris appears to remain fixed in the sky as the rest of the stars rotate around it. In Greek mythology, Ursa Minor is associated with the son of Callisto. Callisto was a beautiful maiden turned into a bear by the jealous Hera. As a bear, Callisto was forced to wander the forests where she was almost killed by her hunter son. Zeus saw what was about to take place and turned the son into a bear before he could kill his mother. Zeus then raised them both to the sky. In the sky, the little bear is hanging from Polaris by his tail. The little bear is also known as the Little Dipper, but this group of stars is not as bright as the [G/Big Dipper] and is more difficult to find. Polaris marks the end of the handle of the dipper. Two stars at the front of the scoop are the only other stars easily visible from most urban areas. Ursa Minor is a [G/circumpolar] constellation and can be seen year round from most of the northern hemisphere. џVela was once part of the constellation of Argo, the large sailing ship of the southern skies. During the 1750's, Argo was divided into four separate constellations, although these new constellations retained the nautical theme. Other segments of the sailing ship include [Y/Carina] the keel, [Y/Puppis] the stern, and [Y/Pyxis] the compass. The brightest star in Vela is Gamma Velorum, [S/219501]. Vela is best seen from March-April in the southern hemisphere. џIt is difficult to choose just one story to describe this [G/constellation] because, throughout recorded history, Virgo has been associated with many different Earth goddesses and female heroines. One of the earliest stories surrounding Virgo comes from the ancient Babylonians. Ishtar was their Earth goddess who was very much in love with her husband. When he died, he passed to the Underworld, where all mortals go when they die. Ishtar could not bear to be without her husband, so she followed him into the Underworld. As she descended into the land of the dead, cold and darkness fell upon the land above. Ishtar found her husband and begged the Queen of the Underworld to return him to the land of the living. She refused, so Ishtar remained with her husband. Meanwhile, in the land above, the cold and dark continued. Plants would not grow, no baby animals were born. The world was dying. The other gods were alarmed by the prolonged winter. They sent a messenger to the Underworld, asking the Queen to grant Ishtar's request. Since the gods above had more power than the Queen of the Underworld, she reluctantly granted Ishtar's wish. As soon as Ishtar returned to the surface with her husband, the air began to warm and plants began to grow. Spring had returned to the land. Every year, Ishtar returns to the Underworld to thank the Queen for returning her husband to her. While she is away, winter falls on the land. When she returns to the surface, so does spring. In the sky, one can use the handle of the [G/Big Dipper] to find Virgo. Simply follow the curve of the handle away from the dipper. The line from the handle will arc to [W/Arcturus] then speed on to [W/Spica], the brightest star in Virgo. Virgo is best seen from April-June. "Must See" objects include: the [F/Sombrero Galaxy]; [M/M49], an elliptical galaxy. џVolans is a modern [G/constellation], added to the charts in the early 1600's. Its brightest star is Gamma Volantis, [S/256374]. Volans is a [G/circumpolar] constellation and can be seen year round from the southern hemisphere. џVulpecula is considered a modern [G/constellation], added to the charts in 1690. It can be found lying just below and a little to the east of the bright star [W/Albireo]. The brightest star in this constellation is Anser, [S/87261]. "Must See" objects include: the [F/Dumbbell] nebula. џAccretion DiskџA disk of material that has been trapped by a [G/black hole], but hasn't yet been pulled inside. џApolloџThe name given to the U.S. manned space program designed to land humans on the [G/Moon]. The program was a success, with twelve Apollo astronauts actually walking on the Moon. The first moon landing, Apollo 11, occurred on July, 20, 1969. The last landing, Apollo 17, was on December 11, 1972. џAsteroid BeltџThe asteroid belt lies between the [G/orbit]s of [P/Mars] and [P/Jupiter] and contains over 100,000 asteroids, most smaller than half a mile (1 km). џAsteroidsџSmall, rocky objects. Most asteroids, but not all, can be found in the [G/asteroid belt]. Trojan asteroids travel in orbit around [P/Jupiter], in front of or trailing the planet. Amor asteroids cross the orbit of [P/Mars] and Apollo asteroids cross the orbit of Earth. џA.U.џAn A.U., or Astronomical Unit, represents the average distance between [G/Earth] and the [G/Sun], and is equal to 93 million miles or 150 million kilometers. џAverted VisionџWhen looking through a telescope, focus your eye on the edge of the [G/field of view] and use your peripheral vision to scan the central area. This technique is best used to detect faint objects such as a [G/nebula] or a [G/galaxy]. џBayerџIn 1901, an astronomer named Bayer first used the Greek alphabet to classify the brightness of [G/star]s in a [G/constellation]. The brightest star was designated "Alpha", the second brightest "Beta" and so on. For example, the fifth brightest star in the constellation of [Y/Lyra] is designated Epsilon Lyra. џBig DipperџSeven stars in the [G/constellation] of [Y/Ursa Major] that form a dipper. Three stars form the handle of the dipper, while four stars form the scoop. The two stars in the front of the dipper's scoop are known as the "Pointer" stars, because they point to [W/Polaris], the North Star. џBlack HoleџA black hole is a bizarre object of incredible mass, yet no volume. Its gravity is so strong that nothing, not even light, can escape its pull. A black hole is sometimes formed after the death of a supermassive star. Black holes are also found in the center of some galaxies. џBlue Moonџ"Blue Moon" refers to the second Full Moon, [g/Moon, Full] within one calendar month. A "Blue Moon" occurs once every 2 1/2 to 3 years. џCassiniџA 17th century French astronomer who discovered the large gap in the rings of [P/Saturn]. џCassini DivisionџName given to the 3,100 mile wide (5,000 km) dark division in [P/Saturn]'s rings. This division in the rings contains small fragments of dark material. џCCDџA CCD (Charge-Coupled Device) is an electronic camera that includes a silicon chip covered with a series of sensors. These sensors collect and record individual photons of light that fall onto the silicon chip. The photons are counted and entered into a computer program that converts the numbers into an image. CCD cameras are much more sensitive than standard film, producing digital images that can be enhanced to bring out subtle details. џCelestial PoleџTwo points in the sky, one aligned with the North pole of Earth, the other aligned with the South pole of Earth. All the stars in the sky appear to rotate around these celestial poles. Although no star lines up precisely with these points, the "north star", [W/Polaris], does come extremely close. џCircumpolarџCircumpolar stars or [G/constellation]s can be seen year round, never setting below the horizon for most of the world. Circumpolar objects are usually defined as any star or constellation that lies within 20 degrees of either the north or south [G/celestial pole]. џClumpyџThe best way to describe [P/Neptune]'s main ring. For some reason, the main ring around Neptune is not uniform in appearance. Instead, material is clumped together at three different locations throughout the ring. џClusterџA large grouping of [G/star]s. Two different types include galactic, or open, clusters (loose grouping of young stars formed from the same diffuse [G/nebula]) and globular clusters (compact sphere of thousands of stars, older and more distant than galactic clusters). џComa Star ClusteџCovering an area ten times greater than that of a full [G/Moon], this galactic [G/cluster] in the [G/constellation] of [Y/Coma Berenices] is too large to observe through a telescope. Instead, use binoculars to scan the cluster. This cluster is approximately 250 [G/light year]s away. џCometsџA small body of ice and rock in an [G/elliptical] [G/orbit] around the Sun. When comets approach the Sun, they heat up and melt, leaving behind a long tail of ice and dust. џConstellationџA group of stars that ancient people formed into an imaginary pattern. Finding a constellation requires a good imagination and the ability to play a stellar version of connect-the-dots. There were 48 original constellations, first mapped out by the ancient astronomer Ptolemy. Today there are 88 "official" constellations. џCraterџCircular impression found on most rocky bodies in the solar system. Craters are formed when [G/meteors] slam into the surface of a [G/moon] or [G/planet]. џDeep Sky ObjectsџFaint objects beyond our [G/solar system]. џEarthџThe origin of Earth's name is unknown. Our planet is the only planet in the solar system capable of supporting liquid water. In fact, 70% of Earth's surface is covered by water. Earth is one of the most geologically active planets; volcanoes, earthquakes, hurricanes, floods, fires and severe storms are constantly resurfacing the planet, changing its appearance. Earth is also the only planet in the solar system known to support life. The diameter of Earth at the equator is 7,926 miles (12,756 km). The mass of the Earth is 13.17 trillion trillion pounds (5.974 trillion trillion kg). џEarth SatellitesџObjects in [G/orbit] around Earth, natural (the [G/Moon]) or man-made (space stations, weather satellites, etc.) џEarth YearsџA year on Earth is equal to 365.2422 days. џEclipsing BinaryџA binary [G/star] system refers to two stars in [G/orbit] around a common point. When one star eclipses, or passes in front of the other, as seen from Earth, the star in front blocks the light from the second star. As a result, the overall brightness of the system decreases. џEllipticalџThe [G/orbit]s of most objects are elliptical, or egg-shaped. џEquinoxџTwo days during the year when the amount of time the Sun is above the horizon equals the amount of time it is below the horizon, hence a day of equal daylight and darkness. The equinox occurs in March when the [G/Sun] appears to cross over Earth's equator and begin its trek into the northern skies. In the northern hemisphere, this marks the first day of spring. In September, the Sun crosses back over the equator and begins its travels in the southern skies, marking the first day of fall in the northern hemisphere. џExtra Solar SystџPlanets orbiting stars other than our Sun. џField of ViewџThe area of sky seen through a pair of binoculars or a telescope. The more magnification used, the smaller the field of view. џGalactic CenterџThe center of a [G/galaxy]. Spiral galaxies have a distinct, large sphere of stars at their galactic center. џGalaxyџAn extremely large grouping of objects containing stars, nebulae, clusters, black holes, and much more. Different types include spiral (pinwheel shaped) galaxies, elliptical (egg-shaped) galaxies, and irregular galaxies. џGalileoџGalileo Galilie, 1564-1642, was an Italian astronomer and physicist. He was also the first person to use a telescope to study the sky. Galileo discovered many things with his telescope, including the four largest moons of [P/Jupiter] and [G/crater]s on the Moon. џGalileo spacecraџGalileo launched on Oct. 18, 1989 to study [P/Jupiter] and its moons. It is the first spacecraft to go into orbit around a gas giant planet. Galileo released a probe that plunged into the [G/jovian] atmosphere. Information from Galileo has incredibly expanded our knowledge of the jovian system. џGanymedeџLargest [G/moon] in the solar system. At 3,270 miles (5,276 km) in diameter, it is larger than the planets [P/Mercury] at 3,024 miles, (4,878 km) and [P/Pluto] at 1,400 miles (2,300 km). Ganymede orbits the planet [P/Jupiter]. џHighlandsџHeavily cratered regions found on the [G/Moon]'s southern hemisphere. The highlands are over four billion years old, the oldest surfaces found on the Moon. џHubble TelescopeџThe Hubble Space Telescope was launched on board the space shuttle in 1990 and placed in low Earth orbit. From its vantage point in space, above Earth's turbulent atmosphere, its 93.6 inch (2.4 meter) objective mirror has revealed an incredible amount of information about our universe. џInfraredџElectromagnetic radiation that lies just beyond the visible portion of light. Longer than the red wavelengths, this type of radiation can be detected as heat. џInt'l Space StatџWhen completed, this space station will be 290 feet (79.9 m) in length, 356 feet (108 m) at its widest point and will orbit at an altitude of 220 nautical miles (407 km) above the Earth. џIRASџThe Infrared Astronomical Satellite (IRAS) was launched on January 25, 1983 to study [G/infrared] sources in deep space. џJovianџAnything relating to [P/Jupiter]. џLanderџSpacecraft designed to land gently on the surface of a planet or moon and send back pictures and scientific data from the surface. џLight YearџThe distance a beam of light travels in one year: 5.9 trillion miles (9.5 trillion km). џLimbџThe natural curved edge of a [G/planet] or [G/moon], as seen from [G/Earth]. џLittle DipperџSeven [G/star]s in the [G/constellation] of [Y/Ursa Minor] form a dipper: three stars form the handle of the dipper, while four stars form the scoop. The Little Dipper is smaller and much fainter than the [G/Big Dipper]. [W/Polaris], the North Star, represents the last star in the dipper's handle. џLocal GroupџA group of about 20 nearby galaxies, including our own [G/Milky Way] and the [F/Andromeda Galaxy]. џLuminosityџHow bright an object appears, not just in the visible wavelengths of light, but over its entire spectrum. џLuminousџHow luminous a star appears is determined by its luminosity, the amount of energy the star emits across its entire spectrum, including infrared, visible, ultraviolet, microwave, x-ray, and all other wavelengths of electromagnetic radiation. џLunar EclipseџWhen the Moon passes through Earth's shadow. A lunar eclipse can only occur when the Moon is full, and Earth lies between the Sun and the Moon. A total lunar eclipse occurs when the entire Moon passes through the umbra (dark shadow). A partial eclipse occurs when only a portion of the Moon passes through the umbra. A penumbral eclipse occurs when the moon only passed through an area of reduced sunlight called the penumbral shadow. In a penumbral eclipse the brightness of the moon is reduced but no dark shadow appears on the surface. џMagellanџSpacecraft designed to complete a radar mapping mission of [P/Venus]. Launched May 4, 1989 by the U.S., Magellan was a complete success, revealing strange features on the surface of Venus (domes, lava tubes, possible fault lines) as it mapped the entire planet. џMagnitudeџA scale used to compare the brightness of celestial objects. The brighter the object, the smaller its magnitude rating. In fact, [P/Venus] at its brightest in our skies, has a rating of magnitude -4.5. The bright star, [W/Betelgeuse] is magnitude 0.5. The faintest objects that can be seen with the [G/naked eye] are magnitude 5.5. џMariaџPronounced MAR-ee-uh, these large, dark smooth regions found in the northern and central regions of the [G/Moon], were formed when huge [G/meteors] slammed into the Moon's surface and cracked its crust. Lava from the Moon's then liquid central core seeped up through the cracks, filling in the original [G/crater]s, leaving a smooth dark surface. Samples brought back by the [G/Apollo] astronauts indicate the maria to be almost three billion years old, much younger than the heavily cratered [G/highlands] to the south. џMariner 10џSpacecraft launched on Nov. 3, 1973 by U.S. to study the planets [P/Venus] and [P/Mercury]. This was the first dual-planet mission, using the gravity of Venus to propel itself on to Mercury. Mariner 10 flew by Venus on Feb. 5, 1974, continuing on to take the first closeup pictures of Mercury on Mar. 29, 1974. It flew by Mercury two additional times. џMariner ValleyџRift valley on [P/Mars] over 3,000 miles (4,800 km) long and 4 miles (6.4 km) deep. On Earth, this valley would stretch from New York to Los Angeles. џMars Global SurvџThe first of several spacecraft in the Mars Surveyor program, Mars Global Surveyor was launched on November 7, 1996 by the US and arrived at [P/Mars] on September 17, 1997. In orbit around Mars, the spacecraft is studying the atmosphere and photographing the planet. The spacecraft will also act as communication support for future missions. џMessierџCharles Messier was a famous eighteenth century French astronomer and author of the Messier catalog of faint objects. Messier created his catalog to avoid confusion between known deep sky nebulae and faint, new comets, his main interest. Messier contributed 103 objects to his list. An additional 7 objects have been added over the years, for a total of 110 objects. џMeteorsџSmall pieces of rocks and dust which enter Earth's atmosphere at great speeds. Friction between the dust and the atmosphere causes the rock to heat up, leaving behind a bright streak of light. Most burn up before they hit the ground. The larger rocks do hit the ground, forming [G/crater]s. џMilky WayџOur home galaxy. Its spiral arms can be seen as glowing clouds of distant stars, stretching across the sky from August through October. The center of the Milky Way is located in the area just behind the [G/constellation] of [Y/Sagittarius]. The bright, individual stars we see in the sky also belong to the Milky Way. These stars lie within the same spiral arm as our [G/solar system] and are our celestial neighbors. џMirџThe Russian space station Mir, was launched on February 19, 1986. During its life, several modules were added to the space station, it provided a home to over sixty crew members from over a dozen countries. The space station orbited the Earth at an average distance of 242 miles (390 km). It was de-orbited on March 23, 2001. Mir make 86,331 orbits of the Earth during its life. џMoonџThe common name for [G/Earth]'s only natural [G/satellite]. A moon also refers to a natural satellite orbiting around any [G/planet]. џMoon, First QuarџThe Moon is in its First Quarter. A First Quarter Moon occurs when the western half of the Earth-facing side of the Moon is illuminated by sunlight. The Sun's light falls on the Moon's surface at an angle. In the southern [G/highlands], it illuminates some of the crater walls and central mountain peaks, but leaves the floors of some craters in darkness. The northernmost [G/maria] is Mare Frigoris. Just below that, cut off by the [G/terminator], is the beginning of Mare Imbrium. The Sea of Serenity and Sea of Tranquility are also visible towards the center of the Moon. In the sky, a First Quarter moon is visible before sunset and can be seen during the early evening hours. џMoon, FullџThe Moon is Full. A Full Moon occurs when the entire Earth-facing side of the Moon is illuminated by sunlight. Through a telescope, this is the worst time to observe the Moon. With the [G/Sun] shining straight onto the Moon, there are no shadows or sense of depth. The lunar surface is all but washed out. A Full Moon rises as the Sun sets and sets as the Sun rises. A [G/lunar eclipse] can only occur during a Full Moon. џMoon, NewџThe Moon is New. A New Moon is not visible from Earth. A New Moon occurs when the entire far-side of the Moon is illuminated by sunlight. As a result, the Earth-facing side is in darkness and not visible. With the Moon's light out of the way, this phase is the best time to look for those faint [G/deep sky objects] that the Moon's light normally washes out. The exact moment of New Moon has significance in several religions around the world and it is the only time a [G/solar eclipse] can occur. џMoon, Third QuarџThe Moon is in its Third Quarter. A Third Quarter Moon occurs when the eastern half of the Earth-facing side of the Moon is illuminated by sunlight. The small, heavily cratered area you see near one end of the Moon is the [G/highlands] at the south pole. Near the north pole is the narrow band of Mare Frigoris. Below that is Mare Imbrium, or the Sea of Rains. Located almost in the middle, is the large crater Copernicus - 58 miles (93 km) wide and 2.2 miles (3.7 km) deep. Curving along the [G/limb] is the largest [G/maria] on the moon, Oceanus Procellarum, the Ocean of Storms. In the sky, a Third Quarter moon is visible after midnight and can be seen during the early morning hours. It can even be seen after the Sun rises in the morning sky. Observe along the [G/terminator] to see the most detail. џMoon, Waning CreџThe Moon is a Waning Crescent. A Waning Crescent Moon occurs when the Moon is between Third Quarter [G/Moon, Third Quarter] phase and New Moon [G/Moon, New]. It looks like a banana, or a "smile" that is shrinking or "waning" as less and less of its Earth-facing side is illuminated by sunlight. Oceanus Procellarum (Ocean of Storms) is the largest [G/maria] on the Moon and is visible near the [G/limb]. A Waning Crescent Moon can be seen in the early morning skies in the east. џMoon, Waning GibџThe Moon is Waning Gibbous. A Waning Gibbous occurs when the Moon has passed its Full Moon phase, [G/Moon, Full], but has not yet reached Third Quarter, [G/Moon, Third Quarter]. Less and less of the Earth-facing side of the Moon is illuminated by sunlight. It is best to observe a gibbous moon along its [G/terminator], where the Sun casts shadows on the lunar surface. The heavily cratered [G/highlands] at the south pole are a good observing target. [G/Maria] - Mare Vaporum, near the Moon's center, Mare Imbrium, and Oceanus Procellarum, near the [G/limb] - cover a vast majority of the remaining visible surface. A Waning Gibbous Moon can be found, rising well after sunset in the eastern sky. џMoon, Waxing CreџThe Moon is Waxing Crescent. A Waxing Crescent Moon occurs when the Moon is between its New Moon phase, [G/Moon, New], and First Quarter, [G/Moon, First Quarter]. It looks like a banana, or a "smile" that is growing larger as more and more of the Earth-facing side of the Moon is illuminated by sunlight. Mare Crisium, the Sea of Crises, is visible near the [G/limb] as a distinct dark, round feature. Another [G/maria], the Sea of Fertility, is visible as a dark "blob" below (or above, depending on your orientation) near the nice, round Mare Crisium. A Waxing Crescent Moon can be seen in the early evening skies in the west. џMoon, Waxing GibџThe Moon is Waxing Gibbous. A Waxing Gibbous Moon occurs when more than half of the Earth-facing side of the Moon is visible, but the Moon is not yet full. Details within the Sea of Tranquility, Sea of Serenity and Sea of Rains begin to fade as more and more of the lunar surface is illuminated by the Sun. In the southern hemisphere, details within the heavily cratered [G/highlands] can still be seen along the [G/terminator]. A Waxing Gibbous Moon can be seen in the eastern evening sky as the Sun goes down. џNaked EyeџObserving without any optical aid (i.e., binoculars or a telescope). џNebulaџAn interstellar cloud of gas and dust. Different types include Diffuse nebulae (where stars are forming), Supernova Remnants (cloud of debris from a supernova explosion), and Reflection Nebula (light from bright stars reflecting off of a nearby cloud). џNGCџNew Galactic Catalog. William Herschel (the discoverer of [P/Uranus]) and his son, John Herschel, observed and recorded nearly 5,000 [G/deep sky objects]. Astronomer J. Dreyer added to their list and the entire work was published in 1888 as the New Galactic Catalog. Today the list includes over 15,000 objects, which are referred to by their NGC numbers (i.e., the [F/Great Orion Nebula] is also known as [N/NGC 1976]). џNucleusџThe center of a galaxy. џOlympus MonsџLocated on [P/Mars], Olympus Mons rises 15 miles (24 km) above the surrounding Martian surface, making it the tallest mountain in the solar system. This giant, extinct volcano is almost three times higher than Mount Everest. џOrbitџThe path a celestial object (satellite, moon, planet, star) travels around another celestial object. Most objects follow an elliptical (egg-shaped) orbit. џOrbiterџSpacecraft designed to orbit a planet or moon, taking pictures and gathering scientific data from space. џPathfinderџThe name of a spacecraft launched on Dec. 3, 1996 by U.S. that bounce-landed on [P/Mars], on July 4, 1997. Pathfinder contained a small rover which was able to travel several meters from the lander, studying rock samples and taking photos. џPioneer 10џSpacecraft designed to study [P/Jupiter]. Launched on March 2, 1971 by the U.S., Pioneer 10 was the first spacecraft to pass through the [G/asteroid belt] and obtained the first closeup pictures of Jupiter on Dec. 3, 1973. џPioneer 11џSpacecraft designed to study [P/Jupiter] and [P/Saturn]. Pioneer 11 was launched on April 5, 1973 by the U.S. It flew by Jupiter on Dec. 2, 1974 and Saturn on Sept. 1, 1979. џPlanetџA large body orbiting a star. Planet is the Greek word for wanderer. This name is appropriate because planets appear to wander through the sky as they orbit around the [G/Sun], while the stars remain fixed. џPlanetary NebulaџA sphere of gas surrounding an older sun-like star, formed when the dying star shrugs off its outer atmosphere. These objects have nothing to do with [G/planet]s. џPrecessionџThe slow wobble of Earth's rotational axis. Similar to the way a spinning top wobbles slowly on a table, Earth's poles wobble, or precess, as it spins on its axis. Precession causes the poles to slowly circle, thus pointing to different areas of the sky over the 25,000 years it takes to complete one wobble. џProtostarsџFound in diffuse [G/nebula]e, protostars are dark "globules" of gas and dust drawn together by gravity to form a sphere. As the gravitational collapse continues, the temperature and pressure at the core of the sphere increases to the point where nuclear fusion begins. When that happens, the protostar becomes a full-fledged star. џPulsarџA neutron star (a tiny, massive star produced after a supernova explosion) which rotates incredibly fast, emitting a series of radio pulses. џQuasarџQuasi-stellar objects which lie at great distances and produce tremendous amounts of energy. џRaysџWhen a [G/crater] is formed, material from the explosion is flung away from the point of impact, forming streaks across the lunar surface. These streaks, called rays, can be seen extending away from some of the larger lunar craters. џResolveџThe act of separating into individual components. For example, a telescope's ability to separate a multiple star system into its individual components, or the ability of the human eye to separate the light from a car into two separate headlights. џRetrogradeџTraveling in the opposite direction of the majority of planets and moons. џRilleџA long, narrow crack in the [G/Moon]'s surface. џRing SystemџBand of small particles orbiting a [G/planet]. Particles range in size from a grain of sand to the size of a house. White, icy particles are found in [P/Saturn]'s ring system. The rings around [P/Jupiter], [P/Uranus], and [P/Neptune] are made of extremely dark material. џSarosџA period of 18 years 11.33 days in which the pattern of lunar and solar eclipses repeat. A Saros number defines a particular eclipse configuration within that period. џSatelliteџAn object, natural or manmade, in [G/orbit] around a planet. џSolar EclipseџWhen the [G/Moon] moves between the [G/Sun] and Earth. A solar eclipse can only occur during the New Moon phase. There are three types of solar eclipses: a total eclipse (when the Moon completely covers the Sun); a partial solar eclipse (when the Moon only covers a portion of the Sun); and an annular solar eclipse (if the eclipse occurs when the Moon is at its farthest point in its orbit, its disk isn't large enough to completely cover the Sun, so a ring of sunlight appears around the Moon). џSolar SystemџA [G/star] and anything in [G/orbit] around it. Our solar system consists of nine [G/planet]s orbiting around the [G/Sun]. It also includes [G/meteors], [G/comets], and [G/asteroids]. џSolsticeџThe solstice marks two days of the year: the day the [G/Sun] reaches its northernmost point in our sky (in June) and the day the Sun reaches its southernmost point in the sky (in December). The June solstice marks the beginning of summer in the northern hemisphere and the longest day. For those in the southern hemisphere, it marks the first day of winter and the shortest day of the year. In December, the positions are reversed. The solstice marks the first day of winter in the northern hemisphere and summer in the south. џSouthern CrossџFour bright [G/star]s which form a distinct cross in the southern sky. The stars are located in the [G/constellation] of [Y/Crux]. џSpectroscopeџAn instrument designed to observe a star's spectrum, or individual wavelengths of light. A star's spectrum can reveal its temperature, star type, and composition. џStarџA huge ball of hydrogen gas with nuclear reactions occurring in its core. Our Sun is a star. The color of a star depends on its temperature: a red star indicates a relatively cool surface; a yellow star is a medium type star, like our Sun; and a blue star is a super hot star that burns its fuel extremely fast. џSunџThe Sun is a star at the center of our solar system. The main difference between our Sun and the stars visible at night is distance. On average, Earth is only 93 million miles (150 million km) from the Sun. The next nearest star, Alpha Centauri [S/252838], is 4.2 [G/light year]s, or 25 trillion miles (40 trillion km) away. џSupernovaџThe most powerful explosion in the universe, occurring at the death of a supermassive [G/star]. A supernova blast is so powerful, one dying star can easily outshine an entire galaxy of stars. Leftover debris forms a cloud of material expanding away from the point of explosion. If the dying star was massive enough, a [G/pulsar] or a [G/black hole] may form after the explosion. џTerminatorџThe dividing line between the sunlight and darkness on the Moon. џTitanџLargest [G/moon] of [P/Saturn], Titan is the only moon with an atmosphere. Titan's methane atmosphere contains a thick layer of clouds which hide its surface from cameras. Titan may have lakes of liquid methane on its surface. џTritonџLargest [G/moon] of [P/Neptune], Triton is one of the coldest places in the solar system. [G/Voyager 2] measured temperatures of -391^F (-235^C) at the surface of the moon. The spacecraft also discovered active geysers erupting on Triton, spewing nitrogen and dust several miles into space. џVenera 14џLaunched on Nov. 4, 1981, by what was then called the USSR, this spacecraft landed on [P/Venus] March 3, 1982. The spacecraft transmitted information about the atmosphere while descending to the surface. After touching down, it took a soil sample of the surface. It operated for almost an hour before shutting down. џVirgo ClusterџAn enormous group of galaxies covering a large portion of the sky, including the [G/constellation]s of [Y/Virgo], [Y/Coma Berenices], [Y/Canes Venatici] and [Y/Corvus]. Over 3,000 galaxies have been photographed in this region. џVoyager 1џLaunched on September 5, 1977, Voyager 1 was one of two spacecraft designed to tour the larger planets of the solar system. Voyager 1 flew by [P/Jupiter] in 1979 and [P/Saturn] in 1980. џVoyager 2џLaunched on August 20, 1977, Voyager 2 was one of two spacecraft designed to tour the larger planets of the solar system. Voyager 2 flew by [P/Jupiter] in 1976, [P/Saturn] in 1981, [P/Uranus] in 1986; and [P/Neptune] in 1989. џZodiacџThe path the [G/Sun] appears to travel through the stars every year. Long ago, this path was divided into the twelve constellations we know today as the zodiac. џThis spiral [G/galaxy] is situated perfectly edge-on with respect to the [G/Milky Way]. Since the spiral arms of the galaxy are extremely thin, they almost disappear when observing them from the side, or edge-on. The only real evidence of this galaxy's spiral structure is the dark dust lanes lying between our view and the galaxy's [G/nucleus]. Through a small telescope, its nucleus appears as a faint, tiny oval patch of light. џA challenging object for a small telescope, this [G/planetary nebula] is extremely small and faint in our skies. Attempt to observe this planetary nebula only on extremely dark nights. Use a low-power eyepiece for the brightest image possible and observe using [G/averted vision]. Through a 8-inch (203 mm) or larger telescope look for a small, faint, slightly elongated cloud. џPHL909: This [G/quasar] is 1.5 billion [G/light year]s from Earth. Because of its tremendous distance, this quasar is visible only to the largest telescopes on Earth. џBecause of its orientation in the sky, this [G/galaxy] has been difficult to classify. From our point of view, we see the galaxy from the side, or edge-on. Very little detail can be made out from this angle. Astronomers believe this is either a barred spiral galaxy or a flattened irregular galaxy. It is about 8 million [G/light year]s away and 70,000 light years across. Through a small telescope, look for a narrow, faint streak of light in the [G/field of view]. Only the largest telescopes can begin to [G/resolve] individual [G/star]s within this galaxy. џ47 Tucanae: This globular [G/cluster] is one of the best in the sky, second only to [F/Omega Centauri]. This glowing sphere of over 100,000 [G/star]s is 16,000 [G/light year]s away and almost 210 light years in diameter. It can be found just to the west of the [F/Small Mag. Cloud]. Through a small telescope, the cluster can be seen as a bright, round patch of light. 4-inch (100mm) telescopes and larger can [G/resolve] individual stars around the cluster's edge. Experiment with different magnifications by observing this cluster through a variety of eyepieces. џThis galactic [G/cluster] contains approximately 35 stars. џThis [G/galaxy] is a extremely faint edge-on spiral. џThis small elliptical [G/galaxy] is an extremely faint companion to the giant [F/Andromeda Galaxy], placing it at a distance of 2.2 million [G/light year]s. It is 4,400 light years in diameter. џThis small elliptical [G/galaxy] is an extremely faint companion to the giant [F/Andromeda Galaxy]. Although it is slightly brighter than another companion galaxy, [C/C17], it is still very faint in our skies. This galaxy is 2.2 million [G/light year]s away and 2,300 light years in diameter. џThis elliptical [G/galaxy] is a companion to the great [F/Andromeda Galaxy]. It is 2.2 million [G/light year]s away and 5,400 light years in diameter. M110 was not listed in [G/Messier]'s original catalog, but was added in 1967. Currently, this galaxy is the last object in the catalog. Through a small telescope, look for a fuzzy, star-like object very near the much larger Andromeda Galaxy. џThis small elliptical [G/galaxy] appears to be in [G/orbit] around the great [F/Andromeda Galaxy]. It is approximately the same distance from us as its larger companion, over 2.2 million [G/light year]s, and is 2,400 light years in diameter. It can be seen as a fuzzy [G/star] just to the south of the larger galaxy. Through a small telescope, its great distance and small size make it impossible to [G/resolve] any stars within the galaxy itself. A giant [G/black hole], with a mass equal to 3 million stars like our Sun, is believed to lie at the center of this galaxy. џAndromeda Galaxy: The Andromeda galaxy is the closest spiral [G/galaxy] to the [G/Milky Way]. It is 2.2 million [G/light year]s away, 180,000 light years in diameter, and contains over 300 billion stars. The galaxy is so bright that it can be seen with the [G/naked eye] on extremely dark nights. Through a telescope, it appears faint, fuzzy, and cigar-shaped with a brighter central region. It is best seen through wide angle eyepieces. џThis large scattered [G/cluster] of 15 to 20 [G/star]s forms a W-shape. џThis galactic [G/cluster] is 5,000 [G/light year]s away. Studies of individual stars within this cluster show it to be the oldest galactic-type cluster in our skies, with an estimated age of 12-14 billion years. For comparison, our [G/solar system] is thought to be 4.5 billion years old. Through a small telescope, this cluster is faint and the [G/star]s within the cluster are difficult to [G/resolve] into individual points. џThis [G/planetary nebula] appears as a faint star-like object through a small telescope. џThis spiral [G/galaxy] is large but extremely faint. It is approximately 6-8 million [G/light year]s distant. Through a small telescope, use a low-power, wide angle eyepiece and [G/averted vision] to detect a long, narrow patch of light. џSculptor Galaxy: This edge-on spiral [G/galaxy] is approximately 7.5 million [G/light year]s away. Through a small telescope it appears as a faint, pale streak of light, with a slight brightening towards its center. Even though it is faint, the Sculptor Galaxy is best viewed through low-power, wide angle eyepieces. џPG0052+251: This [G/quasar] is 1.5 billion [G/light year]s away and lies in the center of a spiral [G/galaxy]. Because of its tremendous distance, this quasar is all but invisible except to the largest telescopes on Earth. џThe [G/star]s within this globular [G/cluster] are rather loosely packed. џSmall Mag. Cloud: At 190,000 [G/light year]s, the Small Magellanic Cloud is an irregular galaxy. It is the second closest galaxy to the [G/Milky Way]. Its nearby neighbor in the sky, the [F/Large Mag. Cloud], is the closest galaxy to our own. The Small Cloud has a diameter of 16,000 light years and contains its own [G/star]s, [G/cluster]s, and [G/nebula]e. Lying on the fringes of the Small Cloud is a globular cluster within our own galaxy, [N/NGC 362]. Use low-power, wide angle eyepieces for observing the galaxy in general. For more detailed studies of areas within the galaxy, use medium to high power. џThis spiral [G/galaxy] is very large but its low surface brightness makes it difficult to detect. Use a low-power eyepiece for the brightest image possible. Then, observe using [G/averted vision]. џThis globular [G/cluster] can be found on the northern fringes of the [F/Small Mag. Cloud]. At a distance of 29,000 [G/light year]s, this cluster is still in our [G/Milky Way], but it is almost twice as far away as its globular cluster neighbor, [C/C106]. Through a small telescope, it appears as a round, hazy patch of light against the mottled backdrop of star clouds of the Small Magellanic Cloud. џThis extremely dim irregular [G/galaxy] is relatively close to our [G/Milky Way], making it a member of our [G/Local Group] of galaxies. Its distance is approximately 1.8 million [G/light year]s and it is 9,000 light years in diameter. Its low surface brightness makes this galaxy a definite challenge for a small telescope. џThis galactic [G/cluster] is 9,300 [G/light year]s away and 30 light years in diameter. Because of its great distance, this cluster is difficult to [G/resolve] into individual stars. However, there is one bright [G/star] near the edge of the cluster that should stand out from the hazy cloud. If this bright star is a true member of the cluster, and really is 9,300 light years away, the star must be 275,000 times brighter, or more [G/luminous] than our [G/Sun]. This cluster is best seen using medium-power eyepieces. џThis galactic [G/cluster] is a compact group of approximately 50 [G/star]s. Galactic clusters are best observed using low-power, wide angle eyepieces. With the cluster centered in the field of view, experiment with different eyepieces to determine which provides the best image. џThis galactic [G/cluster] is 8,000 [G/light year]s away and 15 light years in diameter. This cluster is small and wedge-shaped, with few [G/star]s. It is best seen through low-power eyepieces. џPinwheel Galaxy: Long exposure photographs of this [G/galaxy] show a beautiful, face-on spiral galaxy in all its splendor. However, through a small telescope this galaxy is a challenge. With little change in brightness over its entire length, there is little contrast for the eye to pick up on. Instead, it appears as a large, dim cloud that can be easily passed over. When observing the Pinwheel Galaxy, use low-power, wide angle eyepieces and slowly scan the entire field of view, looking for any glimpse of the dim distant galaxy. It is possible to [G/resolve] individual [G/star]s within the galaxy using 12-inch (300cm) or larger telescopes. џThis spiral [G/galaxy] is one of the more difficult [G/Messier] objects to locate with a small telescope. It is believed to be 20 million [G/light year]s away and 80,000 light years in diameter. Under extremely dark skies, using a low-power eyepiece, it may be possible to detect a faint, round hazy patch of light. Larger telescopes, which gather more light, have a better chance of seeing this elusive galaxy. џLittle Dumbbell: This planetary nebula is one of the more difficult [G/Messier] object to locate in a small telescope. This planetary nebula appears similar in structure to the brighter and easier [M/M27] planetary nebula, but fainter and somewhat smaller. џThis small, compact galactic [G/cluster] lies close to the bright cluster [N/NGC 663]. It contains approximately 50 stars. џThis compact galactic [G/cluster] lies close to the bright cluster [N/NGC 663]. It contains approximately 50 [G/star]s. џThis galactic [G/cluster] is 2,600 [G/light year]s away. The cluster is rather sparse, containing few [G/star]s and is best seen through low-power, wide angle eyepieces. џThis loosely grouped galactic [G/cluster] is 1,300 [G/light year]s away, 17 light years in diameter and contains over 60 stars. It is best seen through wide angle eyepieces. џThis galactic [G/cluster] is one of two clusters forming the beautiful Double Cluster of [Y/Perseus]. Of the two, this cluster is closer, younger, and contains more [G/star]s. NGC 869 is about 7,000 [G/light year]s away, 70 light years in diameter, and 6.4 million years old. It contains approximately 400 stars, although less than half of those are visible in a small telescope. NGC 869 is best seen through a low-power, wide angle eyepiece. џThe Dbl. Cluster: This entry represents a beautiful pair of galactic [G/cluster]s. The two clusters, [N/NGC 869] and [N/NGC 884] can be seen at the same time through a low-power, wide angle eyepiece. Details about each cluster can be found under its individual entry. џThis galactic [G/cluster] is one of two clusters forming the beautiful Double Cluster of [Y/Perseus]. It is 8,150 [G/light year]s away, 70 light years in diameter, and is approximately 11.5 million years old. This cluster contains approximately 300 stars, although less than half of those are visible in a small telescope. NGC 884 is best seen through a low-power, wide angle eyepiece. џThis edge-on spiral [G/galaxy] has a distinct, dark dust band running through its disk. The galaxy is approximately 20 million [G/light year]s away and 120,000 light years in diameter. Through a small telescope, look for an extremely faint, narrow streak of light only under the best observing conditions: dark skies, calm air and no [G/Moon]. џPG1012+008: This [G/quasar] is 1.6 billion [G/light year]s away. Because of its tremendous distance, it is visible only through the largest telescopes. џThis galactic [G/cluster] is 1,500 [G/light year]s away. Its central core of stars is about 4 light years in diameter with a few additional stars extending out to a total diameter of 18 light years. There are approximately 60 stars easily visible within the cluster. M34 is best seen using low-power, wide angle eyepieces. џThis compact spiral [G/galaxy] is between 30-60 million [G/light year]s away, its distance being rather difficult to determine. This galaxy is unusual for several reasons, the first being its appearance. Long exposure astrophotographs show this galaxy to have three spiral arms (most spiral galaxies have two). Second, it is an extremely strong radio source. Thirdly, early observations of this galaxy, which showed it moving through the universe at a rate of 620 miles per second relative to our own galaxy, helped introduce the theory of the expanding universe. Through a small telescope, look for an extremely faint, irregular patch of light. It is best seen using a low-power eyepiece. џThrough a small telescope, this barred spiral [G/galaxy] is extremely faint. Look for a small, narrow slash of light when using a low-power eyepiece and [G/averted vision]. Its faint spiral arms can only be detected on [G/CCD] images and long exposure photographs. џThe [G/star]s within this globular [G/cluster] are tightly compressed, making it difficult to [G/resolve]. Look for a tiny, fuzzy, round patch through a small telescope. The bigger the telescope, the brighter the image. џThis galactic [G/cluster] lies just 3 degrees southwest of the brightest [G/star] in [G/Perseus], [W/Mirphak]. This rich cluster contains approximately 150 stars. џThis extremely faint peculiar [G/galaxy] emits an unusually high amount of radio energy and x-rays. Astronomers are not sure exactly why this system is so active. One theory suggests that the tremendous energy being released may be a result of the interaction between two colliding galaxies. The problem with this theory is that it is difficult to make out a second galaxy within the large cloud. Through a small telescope, this galaxy is extremely small and faint. џThis distant spiral [G/galaxy] is an extremely strong radio source. This galaxy is the brightest of a group of 18 galaxies belonging to the [Y/Fornax] Galaxy Cluster. Although classified as a spiral, very little structure can be seen. Look for a small, faint, hazy sphere. џThis irregular-shaped galactic [G/cluster] contains approximately 50 [G/star]s. џThis barred spiral [G/galaxy] is one of 18 galaxies belonging to the [Y/Fornax] Galaxy Cluster. џThis diffuse [G/nebula] surrounds the 4th [G/magnitude] [G/star] Atik [S/56673]. џThis face-on spiral [G/galaxy] is approximately 25,000 [G/light year]s away. Its dim spiral arms and small [G/nucleus] make it a difficult object for small telescopes. Through an 8-inch (203 mm) telescope, a large faint cloud with a slightly brighter center can be detected. џPleiades: This galactic [G/cluster] is almost too large to enjoy through a telescope. With the [G/naked eye] it is possible to see between six and eight [G/star]s, which form a pattern resembling a little dipper. Through a small telescope, it is revealed that these six to eight [G/star]s are embedded in a cluster of 50-100 stars. The Pleiades are only 410 [G/light year]s away and 7 light years in diameter. Because of its relative closeness and size, it may be difficult to see all of the stars of this cluster at one time in a telescope. To do so requires the use of low-power, wide angle eyepieces. The Pleiades (also known as the Seven Sisters) are connected with many myths and legends around the world. One of the more interesting stories can be found not only in a Greek myth but in Japanese, Australian, African, and American legends as well. The story involves six sisters and a missing seventh sister. She is either hiding or has come down to Earth to be with the man she loves. From these stories, it would seem that one of the stars in the cluster was once much brighter and has since faded from view. How many sisters can you see with the naked eye on a dark, clear night? џCalifornia Nebula: This very faint, very large diffuse [G/nebula] is shaped like the state of California, hence its nickname of the California Nebula. џPKS0405-12: This [G/quasar] is over 1 billion [G/light year]s away. Because of its tremendous distance, this quasar is only visible through the largest telescopes. џThis irregular-shaped galactic [G/cluster] contains approximately 30 [G/star]s. џThis planetary [G/nebula] appears as a tiny, pale blue sphere. џThis galactic [G/cluster] contains approximately 80 [G/star]s. џHyades: This enormous galactic [G/cluster] has a distinct V-shape which makes it relatively easy to locate in the sky. The brightest star in the V is [W/Aldebaran], which doesn't even belong to the cluster. Aldebaran lies at a distance of 68 [G/light year]s while the Hyades are 130 light years away. With the exception of a group of stars in [Y/Ursa Major], the Hyades cluster is the closest galactic cluster to our [G/solar system]. Because this group covers such a large area of the sky, it is almost impossible to view the group in its entirety through a telescope. It is best to observe the Hyades with a low-power, wide angle eyepiece or a pair of binoculars. џThere are approximately 100 [G/star]s within this loosely grouped galactic [G/cluster]. џThis galactic [G/cluster] contains approximately 40 [G/star]s. џThe light from the nearby bright [G/star] [W/Rigel] illuminates the gases within this [G/nebula], making it visible to us on Earth. џThis galactic [G/cluster] contains approximately 50 [G/star]s. џThis globular [G/cluster] is a strong source of x-rays, which is unusual for a globular cluster. Through a small telescope, this cluster appears as a faint, round cloud. Larger telescopes are able to [G/resolve] individual stars around the edge of the cluster. џFlaming Star Neb: This diffuse [G/nebula] contains a bright [G/star] just inside its boundaries. This star is not directly associated with the nebula. Instead, it appears to be passing through the area. The nebula is approximately 1,600 [G/light year]s distant and 9 light years in diameter. џThis galactic [G/cluster] contains approximately 45 [G/star]s. џThis galactic [G/cluster] contains approximately 40 [G/star]s, some of which form the shape of a crescent. џLarge Mag. Cloud: The Large Magellanic Cloud [G/galaxy] is one of the closest galaxies to our own [G/Milky Way]. It is 169,000 [G/light year]s away and has a diameter of at least 50,000 light years. For many years, it was designated as an irregular galaxy, a galaxy with no uniform structure. Today, there are indications that the galaxy might be more like a barred-spiral, a spiral galaxy with a bar-shape at its core instead of the traditional spherical bulge. This galaxy is easily seen with the [G/naked eye]. Through a small telescope, one can begin to resolve individual stars, star clusters and nebulae within the hazy cloud. More detail is seen with low-power, wide angle eyepieces. џThis globular [G/cluster] is approximately 50,000 [G/light year]s away. The small, compact sphere of 50,000 to 100,000 [G/star]s appears as a fuzzy, star-like object in a small telescope. Through a large telescope, 4-inches (102mm) or larger, a few stars can be [G/resolve]d around the edge of the cluster. џThis galactic [G/cluster] contains approximately 35 [G/star]s. џThis [G/cluster] is 4,200 [G/light year]s away, 25 light years in diameter and contains 100 stars. M38 is the largest and dimmest of three galactic clusters in [Y/Auriga]. (See [M/M36] and [M/M37].) џCrab Nebula: This faint, hazy cloud is all that remains of a star that died in a [G/supernova] explosion on July 4th, 1054 AD. According to ancient Chinese records, it was on that day a new star appeared in the sky, a star so bright, it could be seen even when the [G/Sun] was high in the sky. This guest star was visible for over a year until it faded from sight. From the description and location given in the ancient records, astronomers were able to connect the Crab Nebula with this spectacular event. Through the years the nebula has decreased dramatically in brightness. In the early 1700's, its faint hazy appearance in a telescope prompted Charles [G/Messier] to begin his famous catalog of objects. This cloud is also home to the first [G/pulsar] ever discovered. The faint cloud is still expanding away from the point of the explosion at an astounding rate of 600 miles per second. The cloud is approximately 6,300 [G/light year]s distant. Through a small telescope, the Crab Nebula appears as an extremely small, faint cloud. The cloud's irregular shape can be [G/resolve]d through larger telescopes. џGreat Orion Neb: The Orion Nebula is one of the most famous diffuse [G/nebula]e in our skies. It is visible to the [G/naked eye] as the second star in [Y/Orion]'s sword. This nebula is 1600 to 1900 [G/light year]s away and 30 light years in diameter. The brighter, central region is about 6 light years across. Through a small telescope, details within the faint, wispy clouds of this nebula can be seen. Imbedded within the nebula are four young stars which form the Trapezium. These stars were born from the gas and dust within this cloud. Experiment with different eyepieces to explore the vast regions of this nebula. Wide-angle eyepieces are needed to observe the entire nebula, while high-power eyepieces show more details of specific areas within the nebula. Larger telescopes are able to [G/resolve] more details of the cloud structure. џThis small diffuse [G/nebula] lies just to the north of the [F/Great Orion Nebula]. Originally, this small nebula may have been a part of the larger dust cloud. џThis diffuse [G/nebula] is a detached segment of the [F/Great Orion Nebula]. џThis [G/cluster] is 4,100 [G/light year]s away, 14 light years in diameter, and contains over 60 stars. It is the smallest and brightest of three galactic clusters in [Y/Auriga]. See [M/M37] and [M/M38]. џThis diffuse nebula surrounds the star [W/Alnilam], the middle star of [G/Orion]'s belt. The brightness of the central star may make viewing the nebula difficult. џPKS0537-441: This [G/quasar] is over 1 billion [G/light year]s away. Because of its tremendous distance, this quasar is only visible through the largest telescopes. џTarantula Nebula: Located within the [F/Large Mag. Cloud], the Tarantula Nebula is the largest diffuse [G/nebula] ever discovered. It is 169,000 [G/light year]s away, yet is still bright enough to be seen with the [G/naked eye]. This nebula is over 800 light years in diameter. If this nebula was the same distance from us as the [F/Great Orion Nebula], a famous diffuse nebula in our own galaxy, the Tarantula Nebula would cover over 30^ of the sky and be bright enough to cast shadows. Low-power eyepieces are recommended for viewing the entire nebula. To see more detail within the nebula, use medium-power eyepieces. џThis diffuse nebula lies just to the east of the bright star [W/Alnitak], the easternmost star in [Y/Orion]'s belt. The brightness of Alnitak may make viewing the nebula difficult. џHorsehead Nebula: The Horsehead Nebula is a dark cloud that lies within a diffuse [G/nebula] just to the south of the bright star [W/Alnitak], the easternmost star in [Y/Orion]'s belt. The Horsehead Nebula can only be seen because it lies in front of some very bright [G/star]s. The light from these stars provides a bright background for the dark cloud. The Horsehead Nebula is best seen using long exposure astrophotography. џThis diffuse [G/nebula] is approximately 1,600 [G/light year]s away and a little over 2 light years in diameter. Though not as impressive as its brilliant neighbor, the [F/Great Orion Nebula], this nebula is easy to locate with a small telescope, resembling a faint comet through a low-power eyepiece. џThis [G/cluster] is 4,600 [G/light year]s distant, 25 light years in diameter, and contains 150 stars. It is the most distant of three galactic clusters in [Y/Auriga](see [M/M36] and [M/M38]). џThis faint, compact galactic [G/cluster] lies just off of the larger galactic cluster [M/M35]. It contains approximately 100 [G/star]s. џThis galactic [G/cluster] is 2,200 [G/light year]s away and 30 light years in diameter. The stars within this cluster appear to line up in rows, forming chains of lights. This cluster is best seen using low-power eyepieces. џThis galactic [G/cluster] contains approximately 100 [G/star]s. џRosette Nebula: The Rosette Nebula is 2,600 [G/light year]s away and 55 light years in diameter. Within this diffuse [G/nebula], long exposure astrophotographs reveal dark clumps of matter, called globules. Astronomers believe these globules are [G/protostars] that will eventually ignite and become stars. Details of this diffuse nebula are hard to resolve with a small telescope. With a low-power wide angle eyepiece, look for a faint cloud surrounding the star cluster [N/NGC 2244]. Large telescopes bring out more of the ring-like structure of this nebula, while long exposure astrophotography can [G/resolve] intricate detail within the gas cloud. џThis galactic [G/cluster] lies in the center of the [F/Rosette Nebula]. Some astronomers believe that the intense radiation released by newly formed stars in this cluster has cleared the surrounding area of gas and dust, giving the Rosette Nebula its ring-like appearance. The remaining gas glows because it is being heated by these young stars. џHubble's Var. Neb: This unusual [G/nebula] varies not only its brightness, but its appearance as well. While its general triangular shape remains constant, dark features within the triangle disappear and reappear at unpredicted intervals. Astronomers are not sure of the cause of this variability. This nebula is believed to be 2,600 [G/light year]s away and 7 light years long. џCone Nebula: NGC 2264 is a combination of a galactic [G/cluster] and a [G/nebula]. The galactic cluster is the most noticeable of the two. About twenty of the cluster's brightest stars form a nice Christmas tree pattern. The nebula, sometimes called the Cone Nebula, lies on one side of the base of the Christmas tree and is difficult to resolve with a small telescope. NGC 2264 lies about 2,600 light years away and is about 20 light years across. џThis compact galactic [G/cluster] contains approximately 100 [G/star]s. џThis galactic [G/cluster] is located just south of the bright star [W/Sirius]. M41 is 2,350 [G/light year]s away and 20 light years in diameter. It is bright enough to be seen with the [G/naked eye] on a dark night. Through a small telescope, individual [G/star]s within the cluster can be seen. џThis galactic [G/cluster] contains approximately 80 [G/star]s. џThis galactic [G/cluster] can be found by drawing a straight line between the bright stars [W/Sirius] and [W/Procyon], with M50 lying about half way between. This cluster is about 2,900 [G/light year]s away and 9 light years in diameter. There are almost 200 stars in this cluster, although a small telescope will be able to [G/resolve] less than half that number. M50 is best seen using low-power, wide angle eyepieces. џThis galactic [G/cluster] contains approximately 100 [G/star]s. џThis galactic [G/cluster] contains approximately 30 [G/star]s. џThis large galactic [G/cluster] contains about 50 [G/star]s but may be difficult to distinguish from the surrounding background stars. џThis unusual galactic [G/cluster] appears to surround the [G/star] Tau Canis Majoris ([S/173446]). This cluster is 4,600 [G/light year]s away and 8 light years in diameter. At first glance, it may appear as a faint cloud surrounding the brighter star. Let your eye adapt to the view and you will be able to [G/resolve] individual stars from within the cluster. Larger telescopes are able to see more individual stars. џEskimo Nebula: The distance to this [G/planetary nebula] is difficult to determine, with estimates ranging from 1,360 to 3,600 [G/light year]s. Through a small telescope, look for a fuzzy star-like object. [G/CCD] images and long exposure astrophotographs reveal a bright central region with darker markings which, to some, resembles a face. Surrounding the central region is a halo of material which looks a bit like the fuzzy hood of a parka, hence the name Eskimo Nebula. џThis large, bright galactic [G/cluster] may be too big to fit within the [G/field of view] of your telescope. M47 is approximately 1,540 [G/light year]s away, although other estimates place the cluster at a much greater distance. The stars within this group are widely scattered, so it is best to use a low-power, wide angle eyepiece when viewing M47 through a telescope. Larger telescopes can [G/resolve] more stars within the cluster. џThis spiral [G/galaxy] is approximately 8 million [G/light year]s distant and 37,000 light years in diameter. [G/CCD] images and long exposure astrophotographs reveal clusters of stars within the compact spiral arms. Through a small telescope, use [G/averted vision] to detect a faint oval-shaped cloud. The larger the telescope, the brighter the image and the more details you can [G/resolve] within the galaxy. џThis rather strange globular [G/cluster] is one of the most distant clusters in our sky. Most globular clusters are found within a halo surrounding our galaxy, a halo that extends approximately 65,000 [G/light year]s from the galactic center. This cluster, however, lies at a distance of 182,000 light years, in a region otherwise devoid of clusters. In some ways it seems that it is trying to escape from the [G/Milky Way]. Through a telescope, this cluster can be seen as an extremely faint, round, fuzzy patch of light. џThis faint, compact galactic [G/cluster] contains approximately 100 [G/star]s. џThis galactic [G/cluster] contains approximately 80 [G/star]s. џThis [G/planetary nebula] is best seen through large telescopes (8-inches (203mm) or larger). NGC 2438 appears to belong to the galactic [G/cluster] [M/M46], but astronomers have determined that it is moving away from us at a much faster rate than the cluster. It is also believed that the planetary nebula is closer to us than M46. Current estimates indicate its distance to be 3,300 light years with an approximate diameter of 1 light year. This planetary nebula appears embedded within the galactic cluster. Through a large telescope, look for a star surrounded by a hazy glow near the cluster's perimeter. џEstimates as to the distance to this galactic [G/cluster] range from 3,200 to 5,400 [G/light year]s. At 5,400 light years, the diameter of the cluster would be about 30 light years. [G/Star]s within this cluster form a circular pattern in the sky. Observers with larger telescopes may be able to [G/resolve] a tiny [G/planetary nebula], [N/NGC 2438], lying just inside the cluster, near its border. This cluster is best seen with low-power, wide angle eyepieces. џThis compact galactic [G/cluster] has a distinct wedge-shape appearance. It lies at a distance of 3,400 [G/light year]s and is 18 light years in diameter. M93 is best seen through low-power eyepieces. џAlthough not as bright as [M/M46], which is also in the [G/constellation] of [Y/Puppis], this galactic [G/cluster] contains many more stars. These stars are evenly distributed throughout the group, making for a very rich starfield. џThis galactic [G/cluster] is 1,200 [G/light year]s away and 20 light years in diameter. It is bright enough to be seen with the [G/naked eye]. Through a small telescope, you should be able to pick out a bright red giant [G/star] near the center of the cluster. The star will not be brilliant red, but your eye should notice a hint of reddish color. This cluster is best seen through low-power, wide angle eyepieces. џThis galactic [G/cluster] contains approximately 75 [G/star]s and appears rather irregular in shape. џThis galactic [G/cluster] contains approximately 60 [G/star]s. џThis galactic [G/cluster] is 1,700 [G/light year]s away and 20 light years in diameter. The 80 or so stars within this cluster appear in a slightly triangular shape. M48 is best seen using low-power, wide angle eyepieces. џPraesepe: The Praesepe [G/cluster] is one of the largest and brightest open clusters that can be seen from Earth. [G/Star]s within this cluster are grouped together in twos and threes. This cluster, which is also known as the Beehive, lies at a distance of 525 [G/light year]s and is 13 light years in diameter. It is best seen through low-power, wide angle eyepieces. џThis galactic [G/cluster] contains approximately 10 bright [G/star]s scattered over a large area of space. This cluster is best observed using a low-power, wide angle eyepiece. џThis galactic [G/cluster] is over 2,500 [G/light year]s away from us and 12 light years in diameter. The [G/star]s in this cluster are more compact than its neighbor, the [F/Praesepe] cluster. It is believed to be one of the oldest galactic clusters in our sky. џThis extremely small, extremely faint spiral [G/galaxy] is difficult to detect with a small telescope. Even with larger telescopes, a dark observing night and the use of [G/averted vision] are a must to detect this galaxy. џThis extremely rich globular [G/cluster] has a tightly packed central region. џThis [G/planetary nebula] is extremely small and faint. Through a small telescope, look for a slightly fuzzy, star-like object. џThis spiral [G/galaxy] has several dark lanes cutting through its spiral arms. These dark lanes give the galaxy an extremely mottled appearance. Through a small telescope, look for a small, mottled, oval shaped cloud. џThis spiral [G/galaxy] is one of the brightest in a group of galaxies located in [Y/Ursa Major]. It is 7 million [G/light year]s away and approximately 36,000 light years in diameter. The orientation of this galaxy in the sky allows us to see almost all of its spiral arms and large central bulge. Long exposure photographs show incredible detail within this distant galaxy. Through a small telescope, however, expect to see an oval-shaped hazy cloud. Lying close to M81 is [M/M82], another galaxy. џThis unusual [G/galaxy] appears as a pale narrow streak in the sky. Once thought to be an edge-on spiral galaxy, long exposure photographs of M82 show no indication of spiral structure. It is a strong radio source and there is evidence within its central region of a massive explosion that took place over 1.5 million years ago. This galaxy is 16,000 [G/light year]s away, over twice as far as [M/M81], its companion in the sky. Though a low-power, wide angle eyepiece it may be possible to see both M81 and M82 in the same [G/field of view]. џSpindle Galaxy: This extremely flattened, elliptical [G/galaxy] is approximately 27 million [G/light year]s away, and 30,000 light year in diameter. Through a small telescope, look for a tiny, elongated patch of light. It is thought that a [G/black hole], whose mass equals 2 million stars like our Sun, lies at the center of this galaxy. џThis [G/planetary nebula] is approximately 2,500 [G/light year]s away and 0.5 light years in diameter. This cloud contains one of the brightest central stars of any planetary nebula, making it somewhat easy to detect. In a small telescope, look for a fuzzy, star-like object. џThis [G/planetary nebula] appears as a star-like object through a small telescope. џPG1011-040: This [G/quasar] is over 1 billion [G/light year]s away. Because of its tremendous distance, this quasar is only visible through the largest telescopes. џThe [G/star]s within this globular [G/cluster] are not as compact as they are within most other globular clusters. Through a small telescope, look for a large, fuzzy patch. џGhost of Jupiter: This [G/planetary nebula] is somewhere between 2,000 and 3,000 [G/light year]s distant. Through a small telescope, look for a fuzzy star-like object. Larger telescopes can begin to make out its spherical nature. џThis loosely-grouped galactic [G/cluster] is 750 [G/light year]s away and surrounds the [G/star] Theta Carinae ([S/251083]). The cluster is bright enough to be seen with the [G/naked eye] on a dark night. Through a telescope, it is best seen using low-power, wide angle eyepieces. џEta Carinae Nebula: The nature of this extremely unusual [G/nebula] has puzzled astronomers for centuries. In 1843, the [G/star] at the center of the nebula, a star that is 100 times more massive and 4 million times brighter than our [G/Sun], underwent a tremendous explosion which lasted for 20 years. Somehow, the star survived. Since then, it has produced unusual readings and fluctuations which astronomers are still trying to decipher. The star and nebula are 7,500 [G/light year]s away. Through a small telescope, look for a large, faint, wispy cloud. џThis barred spiral [G/galaxy] is approximately 29 million [G/light year]s away. Long exposure astrophotographs of this galaxy show a faint ring surrounding a rectangular streak (the barred central region of the galaxy). It is extremely faint and difficult to see with a small telescope. This galaxy is best observed on extremely dark nights. Use a low-power eyepiece for the brightest image possible and [G/averted vision] when looking through the telescope. With a larger telescope (8-inches (203mm) or larger) this galaxy appears as a faint round cloud. The barred structure is only visible on long exposure photographs or [G/CCD] images. Another galaxy, [M/M96], lies nearby. џLarger and slightly brighter than its nearby neighbor [M/M95], this spiral [G/galaxy] is approximately 29 million [G/light year]s away. It has a large oval-shaped [G/nucleus] and tightly-wound spiral arms. While brighter than M95, it is still extremely faint and difficult to see through a small telescope. Observe this galaxy on a dark night using low-power eyepieces and [G/averted vision]. џThis elliptical [G/galaxy] is approximately 32 million light years away. It is believed to have a giant black hole at its core. The mass of this giant [G/black hole] is equal to 100 million stars like our Sun. џThis elliptical [G/galaxy] was not an original entry in [G/Messier]'s catalog, but was added to the list in 1947. It is about 32 million [G/light year]s away and is extremely small and faint in the sky. As a result, is difficult to see in a small telescope. Look for a faint, fuzzy star-like object. Larger telescopes can begin to make out a slight irregularity to its round shape. A giant [G/black hole], with a mass equal to 50 million solar masses, is believed to lie at the center of this galaxy. џThis galactic [G/cluster] is one of the best open clusters in the sky. It is roughly 1,300 [G/light year]s away and 25 light years in diameter. The [G/star]s within this cluster are scattered loosely over a large area of the sky. As a result, it appears elongated in shape and is best seen through low-power, wide angle eyepieces. џThis edge-on spiral [G/galaxy] is approximately 25 million [G/light year]s away. It was not an original entry in [G/Messier]'s catalog, but was added to the list in 1960. It is extremely faint in our skies and is therefore difficult to see with a small telescope. Observe M108 on a dark night, using a low-power eyepiece for the brightest image possible. Use [G/averted vision] to detect a narrow streak of light. Larger telescopes can detect irregular mottling within the cloudy patch. џOwl Nebula: The distance to this [G/planetary nebula] has proven rather difficult to pinpoint. Estimates range from 1,600 to 10,000 [G/light year]s. A standard value of 3,000 light years has been used often, giving the nebula a diameter of approximately 3 light years. At [G/magnitude] 12, this planetary nebula is so faint, it is almost impossible to observe through a small telescope. A 4-inch (102mm) telescope can begin to make out a faint, tiny, round patch of light. The larger the telescope, the brighter the image. џM65 is one of a pair of bright spiral [G/galaxy]s that lie relatively close together in the [G/constellation] of [Y/Leo]. In fact, M65 and its companion, [M/M66] can be seen in the same [G/field of view] of a small telescope using a low-power, wide angle eyepiece. Even though they look close together, the two galaxies are separated by more than 180,000 [G/light year]s. M65 is 29 million light years away and has a diameter of 60,000 light years. Through a telescope, it appears as a faint elongated patch of light. џThis extremely small, extremely faint spiral [G/galaxy] is difficult to detect with a small telescope. Even with larger telescopes, a dark observing night and the use of [G/averted vision] are a must to detect this galaxy. џM66 is one of a pair of spiral [G/galaxy]s that lie relatively close together in the [G/constellation] of [Y/Leo]. This galaxy is brighter and more compact than its companion, [M/M65]. M66 is 29 million [G/light year]s away, with a diameter of 50,000 light years. Through a small telescope, the galaxy appears as a faint elongated patch of light. Through larger telescopes, details within its broad spiral arms become visible. M66, along with its companion, M65, can be seen in the same [G/field of view] of a small telescope using a low-power, wide angle eyepiece. џThis galactic [G/cluster] is a loose grouping of approximately 60 [G/star]s. џThis diffuse [G/nebula] surrounds the star Gamma Centauri, [S/223603], forming a faint, wispy cloud around the bright star. The star lies at a distance of 160 [G/light year]s and is 275 times more [G/luminous] than our [G/Sun]. џThis barred spiral [G/galaxy] was not listed in [G/Messier]'s original catalog, but was added in 1960. It is extremely small and faint in our skies and therefore difficult to see with a small telescope. Observe this galaxy on a dark night, using a low-power eyepiece to achieve the brightest image possible. Use [G/averted vision] to detect a faint, small, oval-shaped patch of light. џRing-Tail Galaxy: This entry represents one of two antennae in an unusual galactic system. [G/CCD] images and long exposure astrophotographs reveal two lobes of material, each a possible galactic [G/nucleus]. Sweeping off each lobe is a long filament of material. This system is 90 million [G/light year]s away and 100,000 light years across. It is extremely faint and will be difficult to detect in a small telescope. џThis entry represents the second of the two antennae in an unusual galactic system. [G/CCD] images and long exposure astrophotographs reveal two lobes of material, each a possible galactic [G/nucleus]. Sweeping off each lobe is a long filament of material. This system is 90 million [G/light year]s away and 100,000 light years across. It is extremely faint and will be difficult to detect in a small telescope. џThis spiral [G/galaxy] is positioned nearly edge-on in the sky and estimates give its distance as 35 million [G/light year]s. Through a small telescope, it is extremely difficult to see. Observe this galaxy on a dark night and use low-power eyepieces and [G/averted vision] to see a faint, narrow streak. Larger telescopes can detect mottling within the streak (the spiral arms) and possible brightening towards the center (the galaxy's [G/nucleus]). џThis spiral [G/galaxy] is positioned almost edge-on in relationship to Earth. As a result, it appears as a highly elongated oval patch in the sky. It is extremely faint and may be difficult to see through a small telescope. Utilizing [G/averted vision] is a must to detect this galaxy. џPG1216+069: This [G/quasar] is over 1 billion [G/light year]s away. Because of its tremendous distance, this quasar is only visible through the largest telescopes. џThis extremely narrow, edge-on [G/galaxy] can be seen as a faint streak through a small telescope. џThis spiral [G/galaxy] is 45 to 50 million [G/light year]s away, although it is moving farther away from us all the time at the tremendous rate of 1,490 miles (2,400km) per second. Long exposure astrophotographs of this galaxy show two distinct spiral arms with smaller tendrils spraying off one side of the round [G/nucleus]. Through a small telescope, however, this galaxy is extremely faint and difficult to see. Observe on a dark night using a low-power eyepiece and [G/averted vision]. Through larger telescopes, look for an oval patch of light that brightens towards the center. џThis spiral [G/galaxy] was not an original entry in [G/Messier]'s catalog, but was added to his list in 1947. It is 25 million [G/light year]s away and appears to be receding at a rate of approximately 300 miles per second. Long exposure photographs and [G/CCD] images of this galaxy show a rather elongated [G/nucleus] and faint spiral arms. Through a small telescope, observe M106 on a dark night using a low-power eyepiece to achieve the brightest image possible. Use [G/averted vision] to detect a faint, cigar-shaped streak of light. The nucleus appears brighter towards the middle of the cigar shape. It is believed that a [G/black hole], whose mass is equal to 40 million stars like our Sun, lies at the center of this galaxy. џThis elliptical [G/galaxy] is 90 million [G/light year]s away. It is believed to have a enormous [G/black hole] at its core, a black hole whose mass is equal to 400 million stars like our Sun. џThis spiral [G/galaxy] is just one of over 3,000 distant galaxies in the [G/Virgo Cluster] and is believed to be 65-70 million [G/light year]s away. Through a small telescope, detecting this faint galaxy is a challenge. Use a low-power eyepiece and [G/averted vision] to make out a small faint patch of light. Through a larger telescope, 8-inches (203mm) or larger, this galaxy appears as a faint, round cloud with a slight brightening towards its center. Long exposure astrophotographs are needed to see any details within its spiral arms. џIn 1660, a German astronomer identified a [G/nebula] at this location. Later, Charles [G/Messier] found no evidence of a nebula, yet he included the entry in his catalog anyway. A faint double star system, with its two stars fairly close together, may have been mistaken for the mysterious missing nebula. џThis [G/galaxy] is the largest spiral-type galaxy in the [G/Virgo Cluster]. Although the largest in this region, it appears small and extremely faint through a small telescope. Observe this galaxy on extremely dark nights using a low-power eyepiece and [G/averted vision]. Larger telescopes show more details within the slightly oval-shaped patch of light, including a brighter central region. џThis elliptical [G/galaxy] is one of 3,000 galaxies within the [G/Virgo Cluster], which lies at a distance of 50-70 million [G/light year]s. A giant [G/black hole], with a mass equal to 300 million stars like our Sun, is believed to lie at the center of this galaxy. This galaxy lies fairly close to another elliptical galaxy, [M/M86]. Both are faint, and difficult to see through a small telescope. It is best to view this object on extremely dark nights, using a low-power eyepiece and [G/averted vision]. џThis elliptical [G/galaxy] is one of 3,000 galaxies within the [G/Virgo Cluster], which lies at a distance of 65-70 million [G/light year]s. It is best to view this galaxy on extremely dark nights, using a low-power eyepiece and [G/averted vision]. џThe stars in this [G/cluster] are rather loosely spaced, which is a little unusual for a globular cluster. It is the fainter of two nice clusters in the [G/constellation] of [Y/Musca]. џThis elliptical [G/galaxy] lies fairly close to another elliptical galaxy, [M/M84]. Unlike its nearby companion, and several other galaxies in this region of space, M86 is not an actual member of the [G/Virgo Cluster] of galaxies. At a distance of 20 million [G/light year]s, it is much closer than the large group. This galaxy is extremely faint and is best seen through large telescopes, using low-power eyepieces and [G/averted vision]. џThis irregular [G/galaxy] is an extremely faint, rectangular patch that is difficult to see even under the best observing conditions. џ3C273: This Quasar is billions of light years away. џThis elliptical [G/galaxy] is 70 million [G/light year]s away and about 50,000 light years in diameter. Through a small telescope, M49 resembles a globular [G/cluster], with a round, hazy appearance. Because of its enormous distance, it is not possible to resolve stars within this galaxy, even with larger telescopes. џThis elliptical [G/galaxy] is one of the largest in the [G/Virgo Cluster] of galaxies. The total mass of this system is calculated to be an incredible 790 billion times the mass of our [G/Sun]. At its core, there is an incredibly massive [G/black hole], equal to 3 billion stars like our Sun. Long exposure astrophotographs show this galaxy is surrounded by an unusually large number of globular [G/cluster]s, almost 1,000. For comparison, just over 100 globulars are known to surround our [G/Milky Way]. Even though this galaxy is so large, it appears small and faint in our skies. After all, it is over 50 million [G/light year]s away. Through a small telescope, it is best to observe on an extremely dark night. Use a low-power eyepiece for the brightest image possible, and use [G/averted vision]. Larger telescopes reveal a round, hazy patch of light. џThis spiral [G/galaxy] is found within the [G/Virgo Cluster] of galaxies. Long exposure astrophotgraphs reveal this galaxy to be a tiny version of the [G/Andromeda Galaxy]. Through a small telescope, it is extremely faint and difficult to see, and best observed on extremely dark nights. Observe with a low-power eyepiece for the brightest image possible and use [G/averted vision]. Larger telescopes reveal an elongated, hazy patch of light. џM91 is considered [G/Messier]'s mystery object. In 1781, he recorded an object resembling a "nebula without stars" at this location. Since then, no one has been able to locate anything resembling Messier's description at these coordinates. Astronomers debate whether Messier recorded a comet that has long since moved along, or if he inaccurately recorded the coordinates of a nearby faint galaxy. Either way, there isn't much to look at here! џThis elliptical [G/galaxy] is one of over 3,000 galaxies within the [G/Virgo Cluster]. Through a small telescope, it is extremely faint and difficult to see. Through a large telescope, 4-inch (102mm) or larger, this galaxy appears as a small, slightly oval-shaped patch of light. The larger the telescope, the brighter the image. џThis faint spiral [G/galaxy] is a challenge for a small telescope, requiring extremely dark nights and the use of [G/averted vision] to begin to detect a small, fuzzy, oval-shaped patch. The larger the telescope, the brighter the image and the easier it will be to observe. џThis edge-on spiral [G/galaxy] is approximately 20 million [G/light year]s away and 90,000 light years in diameter. Through a small telescope, look for a long narrow streak that brightens towards the center. џThis spiral [G/galaxy] is one of over 3,000 galaxies found in the [G/Virgo Cluster]. It is over 65 million [G/light year]s away. Through a small telescope, it is extremely faint and difficult to see. This galaxy is best observed on a dark night, using a low-power eyepiece for the brightest image possible. Also, use [G/averted vision]. Through a larger telescope, look for an oval-shaped hazy patch with a slight brightening towards the [G/galactic center]. џThis barred spiral [G/galaxy] belongs to a vast group of galaxies called the [G/Virgo Cluster]. Galaxies within this super cluster are believed to be 65-70 million [G/light year]s away. Through a small telescope, detecting this faint galaxy is a challenge. Use a low-power eyepiece and [G/averted vision] to make out a small faint patch of light. Through large telescopes, 8-inches (203mm) or larger, look for a small, faint, oval-shaped patch which is the galaxy's central region. Its spiral arms form a much fainter, mottled cloud around the central oval. џThis globular [G/cluster] is 46,000 [G/light year]s away and 100 light years in diameter. Look for a faint, round hazy patch of light. Larger telescopes are needed to [G/resolve] individual stars within the cluster. M68 is best seen using medium power eyepieces. џSombrero Galaxy: This spiral [G/galaxy] is situated in our skies so we see it almost exactly edge-on. It is about 30 million [G/light year]s away and 82,000 light years across. This galaxy gets its name from a dark lane that runs across the enormous center of the galaxy, appearing to cut the galaxy in two, and causing the top portion to look something like a sombrero. An extremely large [G/black hole] is located at the center of this galaxy, a black hole whose mass is equal to 1 billion stars like our Sun. At least a 6-inch (150mm) telescope is required to [G/resolve] this dark lane. Through a small telescope, look for a faint, elongated patch of light with a brighter central region. џThis elliptical [G/galaxy] belongs to the [G/Virgo Cluster]. Through a small telescope, detecting this faint galaxy is a challenge. Use a low-power eyepiece and [G/averted vision] to make out a small, faint patch of light. Through a large telescope, 8-inches (203mm) or larger, look for an extremely faint oval cloud, with a slight brightening towards the center. џThis edge-on spiral [G/galaxy] is faint and difficult to see. When observing, look for a long, faint, narrow streak. Large telescopes may begin to [G/resolve] mottling within the galaxy which represents dust in the spiral arms. џThis galactic [G/cluster] is a fairly compact grouping of approximately 20 [G/star]s. џThis elliptical [G/galaxy] is just one of over 3,000 distant galaxies in the [G/Virgo Cluster] and is believed to be 65-70 million [G/light year]s away. It is one of the largest elliptical galaxies known, second only to [M/M49] in size and mass. Through a small telescope, look for a hazy oval patch of light, resembling a fuzzy star. The image through a larger telescope is brighter, but at its vast distance, it is not possible to [G/resolve] any individual [G/star]s. џThis elliptical [G/galaxy] is extremely small and faint, making it difficult to detect with a small telescope. Even with larger telescopes, a dark observing night and the use of [G/averted vision] are a must to detect this galaxy. џThis spiral [G/galaxy] is 20 million [G/light year]s away and about 33,000 light years in diameter. Because the spiral arms of this galaxy are wound very tightly around its large central core, it is difficult to see any spiral structure through a small telescope. Instead, look for a small, round hazy patch. џCoal Sack: From as far back as the 1500's, people have noted this dark, starless patch of sky known as the Coal Sack. The Coal Sack is a dark [G/nebula], an extremely large cloud of gas and dust that does not contain any stars. If it did contain stars, or if there were stars close to it, those stars would illuminate the cloud, thus making it visible. Instead, we see nothing. This dark nebula lies 550 [G/light year]s away and is about 65 light years in diameter. Look for the Coal Sack just to the east of [W/Acrux]. џJewel Box: This magnificent galactic [G/cluster] surrounds the tenth brightest [G/star] in the [G/constellation] of [Y/Crux]. The cluster is 7,700 [G/light year]s away. There is a central knot of stars within the cluster that is about 25 light years in diameter. Stars on the outer fringes make the entire cluster about 50 light years in diameter. The [G/luminosity] of the brightest star in the cluster is 80,000 times that of our [G/Sun]. That star, along with two other bright stars in the cluster form a triangle. The Jewel Box is best seen with low-power, wide field eyepieces. џBlack Eye Nebula: A dark spiral arm cuts a swath through a portion of the bright central region of this galaxy, earning it the nickname "Black Eye". This galaxy is approximately 12 million [G/light year]s away. At least a 4-inch (102mm) telescope is required to detect the "Black Eye" appearance. Using a medium-power eyepiece can aid in bringing out the contrast between the dark spiral arm and the bright central region. џThis globular [G/cluster] is one of two nice clusters in [Y/Musca]. It is brighter and more compact than its neighbor, [C/C108], although, through a small telescope it will appear rather faint. Look for an increase of brightness towards the center of the cluster. џThis elliptical [G/galaxy] is the brightest galaxy within the Coma Cluster, a group containing over 1,000 galaxies. The Coma Cluster is approximately 400 million [G/light year]s away and members stretch across 20 million light years of space. џThis edge-on spiral [G/galaxy] appears as a faint, narrow streak when observing on a dark night and using a low-power eyepiece and [G/averted vision]. Some mottling within the narrow cloud may be detected with larger telescopes. џThis spiral [G/galaxy] has tightly bound spiral arms and a compact [G/nucleus]. It appears as an extremely small, faint, oval-shaped patch of light only under the best observing conditions. џThis globular [G/cluster] is 65,000 [G/light year]s away and over 100 light years in diameter. The total [G/luminosity] of M53 is 200,000 times that of our [G/Sun]. Through a small telescope, this cluster is easily seen as a faint, round patch of light. Larger telescopes are able to resolve individual stars around the edge of the cluster. џSunflower Galaxy: This spiral [G/galaxy] is approximately 35 million [G/light year]s away and 90,000 light years in diameter. Its central oval-shaped region is brighter on one side than the other, giving it a rather unusual, lopsided appearance. Through a small telescope, use a low-power eyepiece and [G/averted vision] to detect a small faint patch of light. 4-inch (102mm) or larger telescopes are needed to begin to detect the faint nebulosity of the spiral arms. џCentaurus A: This peculiar [G/galaxy] is approximately 15 million [G/light year]s away and 100,000 light years in diameter. Through large telescopes, this galaxy appears as a glowing sphere with a thick, dark band dividing it into two sections. Its strange appearance has puzzled astronomers for many years. This galaxy is also an unusually strong source for natural radio emissions. Astronomers believe that this galaxy is undergoing a series of extremely powerful explosions within its core, although the reason for these explosions is not completely understood. Through a small telescope, look for a faint, hazy patch with a slight darkening through its center. Centaurus A is best seen using medium-power eyepieces. џOmega Centauri: This globular [G/cluster] is 17,000 [G/light year]s away and 150 light years in diameter. The cluster can be seen as a hazy, faint [G/star] with the [G/naked eye]. Through a small telescope, look for a round hazy patch of light. Larger telescopes are able to resolve individual stars within the cluster. The stars in this cluster are extremely close together, with an average distance between stars of only 0.1 light years. For comparison, the distance between the [G/Sun] and its closest neighbor, Alpha Centauri ([S/252838]) is 4.2 light years. џWhirlpool Galaxy: This spiral [G/galaxy] is 35 million [G/light year]s away and over 100,000 light years in diameter. A giant [G/black hole], with a mass equal to one million stars like our Sun, is believed to lie at the center of this galaxy. Through a small telescope, look for a dim, hazy patch of light with a brighter central region. Because of the galaxy's face-on orientation in the sky, its spiral or pinwheel shape is clearly visible in photographs and larger telescopes. The giant galaxy has a small companion nearby, which can also be seen through larger telescopes. џThis spiral [G/galaxy] is 10 million [G/light year]s away and about 30,000 light years in diameter. While this is the 25th brightest galaxy in the sky, it is extremely faint in small telescopes. Larger telescopes are required to show the slight brightening at the central core. џThis spiral [G/galaxy] appears as a faint, tiny, hazy oval through a small telescope when observing under dark skies and using [G/averted vision]. [G/CCD] images and long exposure astrophotographs reveal this galaxy's beautiful spiral structure. џThis globular [G/cluster] is 35,000 [G/light year]s away and over 220 light years in diameter. Through a small telescope, look for a faint, round hazy patch of light. Larger telescopes are able to resolve [G/star]s around the edge of the cluster. M3 is best seen through medium or high power eyepieces. џThis globular [G/cluster] appears as a tiny, fuzzy, round patch through a small telescope. Larger telescopes can begin to [G/resolve] stars around the cluster's border. џThis spiral [G/galaxy] is 15 million [G/light year]s away and 90,000 light years in diameter. Long exposure photographs taken through large telescopes reveal a galaxy with a bright, tiny [G/nucleus] and an impressive array of spiral arms. Within its spiral arms are distinct clumps of stars. Unfortunately, this incredible detail can only be detected on sensitive photographic film and CCD cameras. Through a small telescope, the human eye can only detect a very small, faint patch of light under the best observing conditions. џPG1435-067: This [G/quasar] is over 1 billion [G/light year]s away. Because of its tremendous distance, this quasar is only visible through the largest telescopes. џThis globular [G/cluster] is approximately 100,000 [G/light year]s away. Measurements of this cluster show it to be moving almost 170 miles (273 km) per second away from our galaxy, fast enough to escape the gravitational tug of our [G/Milky Way] and become an intergalactic traveler. However, you won't be able to see any movement when looking through a telescope. Instead, look for a fuzzy, stationary, "star-like" object. џThis galactic [G/cluster] contains approximately 80 [G/star]s which form a nice compact group. Observe this cluster with a low-power, wide angle eyepiece. џThere is some controversy about the identity of this object. In correspondence Messier admitted that it might be a duplicate of M101, as it appears in some catalogs. Other scholars have examined his observations, and believe that NGC 5866 is actual M102, the object in this catalog. This is consistent with other journal entries and correspondence. Enjoy the object and join the argument that has been going on for 300 years. џThe [G/star]s in this globular [G/cluster] are more loosely packed than stars in most other globular clusters. џThis globular [G/cluster] is about 30,000 [G/light year]s away and 100 light years in diameter. Through a small telescope, look for a faint, round hazy patch. With a 4-inch (100mm) or larger telescope, it is possible to [G/resolve] individual [G/star]s around the edge of the cluster. џThis globular [G/cluster] contains 50,000 to 100,000 [G/star]s. џThis galactic [G/cluster] contains approximately 30 stars that are brighter than [G/magnitude] 7. It is located just north of the northernmost star in the triangle of [Y/Triangulum Australe]. џThis small, compact globular [G/cluster] is 3,600 [G/light year]s away and about 50 light years in diameter. Through a small telescope, it appears as a round, hazy patch of light that is slightly brighter towards the center. Larger telescopes are able to [G/resolve] stars on the fringes of the cluster. M80 is best seen using medium- to high-power. џThis rich galactic [G/cluster] contains over 100 [G/star]s. џThis globular [G/cluster] is located just to the west of the bright [G/star], [W/Antares] and is an easy target for a small telescope. Even though estimates of its distance range from 6,200 to 10,000 [G/light year]s, it is possible to [G/resolve] stars around the edges of this cluster with only a 4-inch (100mm) telescope and a high-power eyepiece. M4 is best seen using medium- to high-power eyepieces. џThis galactic [G/cluster] is 1,600 [G/light year]s away. It contains approximately 100 [G/star]s and is best viewed through low-power, wide angle eyepieces. џThe [G/star]s within this globular [G/cluster] are rather loosely packed. However, its faintness makes it difficult to [G/resolve] into individual stars, even with larger telescopes. Through a small telescope, look for a faint, fuzzy, "star-like" object. џThis globular [G/cluster] is 10,000 [G/light year]s away and 50 light years in diameter. Its huge sphere of 50,000 to 100,000 stars was not an original entry in [G/Messier]'s catalog, but was added to his list in 1947. Through a small telescope, look for a fuzzy, "star-like" object. Larger telescopes can begin to [G/resolve] individual [G/star]s around the edge of the cluster. џThis galactic [G/cluster] contains approximately 30 [G/star]s which may be difficult to distinguish from the background stars of the [G/Milky Way]. џM13 is the closest and brightest of two globular clusters in [Y/Hercules]. This [G/cluster] is 22,000 [G/light year]s away and 160 light years in diameter. The [G/star]s within its huge sphere are not as compact as they are in the neighboring cluster, [M/M92]. Through a small telescope, look for a round, hazy patch of light. Stars within the cluster may be [G/resolve]d using medium or high power eyepieces. To some observers, M13 looks like a pile of sugar crystals spilled on a black table. Larger telescopes are able to resolve more stars within the cluster. џThis globular [G/cluster] is approximately 20,000 [G/light year]s away and lies about 2,000 light years from [M/M10], a nearby cluster. The [G/star]s within M12 are loosely-grouped together, allowing a larger telescope (at least 6-inches or 152mm in diameter) to resolve stars within the cluster. Smaller telescopes can see a faint, irregular glow. џThis galactic [G/cluster] is 5,700 [G/light year]s away and only 8 light years in diameter. It is a small, intense cluster, with several bright [G/star]s gathered into a tight group. To some, this cluster looks like a compact version of the [F/Pleiades]. џThis globular [G/cluster] is approximately 20,000 [G/light year]s away and lies about 2,000 light years from its neighboring cluster, [M/M12], although the two clusters appear fairly close together in our skies. M10 is perhaps the most distinct of all the globular clusters in [Y/Ophiuchus]. It is compact, containing between 50 and 100 thousand [G/star]s, and appears as a round, hazy patch through a small telescope. Larger telescopes (at least 6-inches or 152mm in diameter) are needed to [G/resolve] stars within the cluster. џM62 lies on the border of [Y/Ophiuchus] and [Y/Scorpius]. The distance of this [G/cluster] is about 26,000 [G/light year]s, although there is some uncertainty in this measurement. This cluster appears irregular in shape, unlike the traditional spherical shape of most globular clusters. The stars within the cluster are packed tightly together. Through a small telescope, M62 appears as a faint, hazy patch of light. Larger telescopes (at least 6-inches or 152mm in diameter) are needed to [G/resolve] any stars around the edge of the cluster. џThis globular [G/cluster] is believed to be imbedded in the central bulge of our [G/Milky Way] galaxy. There are large amounts of dust in this region of space which block some of the light from the cluster. Since astronomers aren't sure how much light is being blocked, it is difficult to determine the cluster's absolute brightness, an important factor used when determining distances of celestial objects. As a result, the distance of M19 is uncertain. Values range from 20,000 to 30,000 [G/light year]s. This globular cluster has an unusual oval shape, a hint of which can be [G/resolve]d through a small telescope. Individual [G/star]s within the cluster can be resolved with larger telescopes. џBug Nebula: This [G/nebula] has an unusual, elongated shape, making its classification somewhat difficult. Some refer to it as a diffuse nebula, most refer to it as a [G/planetary nebula]. Observing this nebula through a small telescope requires an extremely dark night, a low-power eyepiece (for the brightest image possible) and the use of [G/averted vision]. џM92 is one of two beautiful globular clusters in [Y/Hercules]. This [G/cluster] is fainter and more compact than its counterpart, [M/M13]. M92 is 37,000 [G/light year]s away. Through a small telescope, look for a round, hazy patch of light. Stars around the edge of the cluster may be [G/resolve]d using a medium power eyepiece. Larger telescopes are able to resolve more stars within the cluster. џThis globular [G/cluster] was discovered by Charles [G/Messier] in 1764. It is 26,000 [G/light year]s away and 60 light years in diameter. It is very compact and appears as a tiny, round, hazy glow in the sky through a small telescope. Large telescopes (at least 6-inches or 152mm in diameter) are needed to [G/resolve] [G/star]s around the edge of the cluster. џThis loosely-packed globular [G/cluster] is rather faint in our skies. Through a small telescope, look for an extremely faint, fuzzy object. A neighboring globular cluster, [C/C86], provides a much brighter target. џThis globular [G/cluster] was discovered by Charles [G/Messier] in 1764, the same year he discovered several other globular clusters in [Y/Ophiuchus]. The [G/star]s within this cluster are packed tightly together, forming a compact, glowing sphere in the sky. M14 is thought to be 65,000 to 70,000 [G/light year]s away. Through a small telescope, it appears as a small, round, hazy patch of light. Large telescopes (at least 6-inches or 152mm in diameter) are needed to [G/resolve] any stars around the edge of the cluster. џButterfly Cluster: This galactic [G/cluster] is about 2,000 [G/light year]s away and 20 light years in diameter. To some, the loose scattering of stars within this cluster resemble the shape of a butterfly with its wings spread open in flight. This cluster is best seen using wide angle eyepieces. џAt a distance of 8,200 [G/light year]s, this is the closest globular [G/cluster] to our [G/galaxy]. The [G/star]s within this cluster are loosely scattered over a diameter of 50 light years, making it one of the easiest globulars to [G/resolve] into individual stars. џThis beautiful galactic [G/cluster] is 800 [G/light year]s distant. It is very loosely packed and covers almost one degree of the sky. (The full [G/Moon] covers only half a degree.) It contains 80-100 [G/star]s brighter than [G/magnitude] 10, although just a fraction of these stars are visible through a small telescope. The brighter stars that are visible will offer quite a view. M7 is best seen through low-power, wide angle eyepieces. џThis galactic [G/cluster] is 2,000 [G/light year]s away and 15 light years across. The [G/star]s within this cluster are loosely scattered and it may be difficult to separate the stars of the cluster from the fainter background stars of the [G/Milky Way]. M23 is best seen using a low-power, wide angle eyepiece. џCats Eye Nebula: This [G/planetary nebula] is approximately 3,200 [G/light year]s away and 0.3 light years in diameter. In 1864, it was the first of its kind to be observed using a [G/spectroscope], thus determining that planetary nebulae were gaseous objects instead of closely-packed spheres of [G/star]s. Through a small telescope, look for a fuzzy, star-like object. Larger telescopes using medium-power can begin to [G/resolve] some nebulosity. џTrifid Nebula: This diffuse [G/nebula] is a stellar birthplace. Hot, glowing clouds of hydrogen gas light up this compact nebula. Calculating the distance to the Trifid has been difficult, resulting in values ranging from 2,200-5,200 [G/light year]s. Through a small telescope, the nebula can be seen as a faint elongated patch of light with a slight amount of darkening through the center of its brighter side. Larger telescopes (at least 8-inches or 203mm) can begin to [G/resolve] the dark dust lanes that divide the brighter part of the cloud into different segments. џLagoon Nebula: This diffuse [G/nebula] lies just a little north and west of the "Teapot" in [Y/Sagittarius]. Large clouds of hydrogen gas within the nebula are heated by newly formed [G/star]s. These heated gases emit a visible glow which appears red in long-exposure photographs. When viewing the nebula with a telescope, the eye is not as sensitive as photographic film. As a result, it appears as a pale white, irregular cloud. The galactic [G/cluster], [N/NGC 6530] can be found embedded within the nebula. Also, dark bands of dust can be seen. The Lagoon Nebula is approximately 5,150 [G/light year]s away with a total diameter of roughly 115 light years. Because of its large size, it is best to use a low-power, wide angle eyepiece to view the nebula in its entirety. Higher magnification may be used, allowing for only a small portion of the cloud to be seen at a time, but in greater detail. џThis galactic [G/cluster] lies close to the [F/Trifid Nebula]. It is 2,200 [G/light year]s away and 17 light years in diameter. џThis galactic [G/cluster] is embedded within the [F/Lagoon Nebula]. Studies have shown the stars in this cluster to be extremely young. If the stars in this cluster actually formed from the Lagoon Nebula, this cluster would then be approximately 5,150 [G/light year]s away. џThis globular [G/cluster] is a huge sphere of between 50,000 to 100,000 stars. Through a small telescope, look for a small, round fuzzy patch. Larger telescopes can [G/resolve] individual [G/star]s around its border. џThis [G/Messier] object is unusual in that it is not one specific object. Instead, M24 seems to represents one of the huge clouds of stars near the center of our [G/Milky Way] galaxy. This star cloud, easily visible to the [G/naked eye], contains millions of stars and is best viewed using low-power, wide angle eyepieces or binoculars. Several dark, dust clouds border M24 on one side. џEagle Nebula: This nebula was made famous by photos taken by the [G/Hubble Telescope]. Through the space telescope, a small portion of this nebula was shown in amazing detail, revealing three giant columns surrounded by swirling clouds of gas. This hydrogen gas is heated by young, newly formed [G/star]s buried within the cloud. The hot gases then emit a glow which we can observe. Through a small telescope on Earth, a faint wispy cloud can be seen surrounding a small cluster of stars. The larger the telescope, the more detail can be [G/resolve]d within the nebula. The Eagle Nebula is approximately 8,000 light years away. џThis galactic [G/cluster] is 4,900 [G/light year]s away. It consists of a few, loosely scattered [G/star]s. The cluster may be difficult to distinguish from the background stars of the [G/Milky Way]. Galactic clusters are best viewed using low-power, wide angle eyepieces. When viewing the cluster, look for a slightly higher concentration of stars amid the fainter background stars. џSwan Nebula: This faint diffuse [G/nebula] appears in the shape of a swan floating on a lake. A bright cloud forms the swan's body, then its neck curves up from one side of the body to its small head. There are no bright [G/star]s visible within the cloud, although there are many fainter stars filling the background. It is possible that light from hot, young stars within this nebula is blocked by dense clouds of gas and dust. The Swan Nebula is about 5,700 [G/light year]s away. The brighter cloud that forms the swan's body is about 12 light years across. Through a small telescope, look for a faint slash of light representing the body of the swan. Low-power eyepieces are recommended. Through larger telescopes, it may by possible to use medium power eyepieces. џThis globular [G/cluster] is more dense and compact than its neighbor [M/M22]. It is also fainter. This cluster is 15,000 [G/light year]s away and about 65 light years in diameter. M28 appears as a round, hazy patch through a small telescope. Larger telescopes are needed to [G/resolve] individual [G/star]s around the edge of the cluster. This cluster is best seen using medium- to high-power eyepieces. џThis irregular-shaped galactic [G/cluster] contains approximately 30 [G/star]s. џThis globular [G/cluster] is approximately 36,000 [G/light year]s away and 70 light years in diameter. Through a small telescope, look for a fuzzy "star-like" object. џThis galactic [G/cluster] is about 2,000 [G/light year]s away and 20 light years in diameter. It contains a scattering of just a few bright [G/star]s against a backdrop of the [G/Milky Way]. M25 is best seen using low-power, wide angle eyepieces. џThis globular [G/cluster] is 9,600 [G/light year]s away and 50 light years in diameter. Through a small telescope, this huge ball of over 100,000 [G/star]s appears as a hazy, slightly elongated, patch of light. Larger telescopes, 4-inches (100mm) and larger, begin to [G/resolve] individual stars around the edge of the cluster. The larger the telescope, the more stars can be resolved. M22 is best seen using medium- to high-power eyepieces. џThis scattered galactic [G/cluster] contains approximately 50 [G/star]s and lies extremely close to the bright star Alpha Scuti [S/142408]. џThe 80 [G/star]s in this galactic [G/cluster] are very loosely scattered. џThis globular [G/cluster] is approximately 65,000 [G/light year]s away and 80 light years in diameter. Through a small telescope, look for a fuzzy "star-like" object. At least a 10-inch (250mm) telescope is needed to [G/resolve] any [G/star]s within this cluster. џThis galactic [G/cluster] is 4,900 [G/light year]s away and about 14 light years in diameter. When viewed through a small telescope, it might be difficult to locate the cluster against the backdrop of the [G/Milky Way]. The cluster appears almost round and fairly compact. It is best seen using low-power, wide angle eyepieces. џWild Duck Cluster: One of the richest galactic [G/cluster]s in the sky, the compact group of over 500 [G/star]s is 6,000 [G/light year]s away and 21 light years in diameter. Through a small telescope, it might first look like a globular cluster, but with increasing magnification, it is possible to [G/resolve] the cluster into individual stars. џThis galactic [G/cluster] contains approximately 40 [G/star]s. џThe 50,000 to 100,000 [G/star]s found within this globular [G/cluster] are rather loosely packed. Look for a tiny, hazy sphere through a small telescope. џRing Nebula: The Ring Nebula is probably the most famous of all the [G/planetary nebulae] in the sky. It is 1,400 light years away and 0.5 light years in diameter. Through a small telescope, the nebula appears as a tiny sphere. At least a 6-inch (152mm) telescope is needed to [G/resolve] the ring structure of the nebula. џThis globular [G/cluster] is 50,000 [G/light year]s away and 70 light years in diameter. It can be found just west of the bottom [G/star] in the handle of the "Teapot" of [Y/Sagittarius]. Through a telescope, this cluster appears as a small, bright round patch of light. Because this cluster is compact, it is difficult to [G/resolve] any stars within it, even around the edges. M54 is best seen using medium- to high-power eyepieces. џThis peculiar [G/nebula] resembles Hubble's Variable Nebula, [C/C46]. The strange, wispy cloud varies its brightness and appearance and astronomers don't completely understand why. Inside the nebula is a variable star which effects the cloud of gas and dust, but does not completely explain its actions. џThis galactic [G/cluster] contains approximately 75 [G/star]s. џThis barred spiral [G/galaxy] is situated face-on relative to our view from the [G/Milky Way]. As a result, [G/CCD] images and long exposure astrophotographs show its spiral arms and bar-shaped [G/nucleus] in all their glory. Through a small telescope, however, look for a small, round, hazy patch that brightens towards the center. It is best to observe this galaxy on a dark night, using [G/averted vision]. џThis globular [G/cluster] is 20,000 [G/light year]s away. While its core is compact, the [G/star]s from the middle of the cluster out towards its perimeter are rather loosely spaced. Through a small telescope, look for a faint, round hazy patch of light. At least a 6-inch (152mm) telescope is needed to [G/resolve] stars around the edge of the cluster. џGRS1915-105: This potential [G/black hole]/star system in Aquila cannot be seen visually, but astronomers detect an extremely strong x-ray source at this location. The x-rays are thought to come from material trapped in the black hole's [G/accretion disk]. Material is sucked off the companion star over the course of half an hour, filling the disk and heating it up. Then, the accretion disk empties itself into the black hole. The x-ray's temperature drops by 15 million degrees and the process begins again. This system is 40,000 light years away. џThis globular [G/cluster] is 46,000 [G/light year]s away and 60 light years in diameter. Through a small telescope, it appears as a faint, round, hazy patch of light. A large telescope is needed to [G/resolve] individual stars around the edge of the cluster. M56 is best seen using medium to high power eyepieces. џThis globular [G/cluster] is 20,000 [G/light year]s away and 80 light years in diameter. Through a small telescope, it appears as a hazy patch of light. Larger telescopes are required to [G/resolve] individual [G/star]s around the edges. It is best seen using medium- to high-power eyepieces. џFoxhead Cluster: This galactic [G/cluster] contains 150 [G/star]s. џThis [G/planetary nebula] appears as a faint "star-like" object through a small telescope. џBarnard's Galaxy: This irregular [G/galaxy] is 1.7 million [G/light year]s away and approximately 10,000 by 5,000 light years across. This galaxy belongs to our [G/Local Group] of galaxies and is best viewed using low-power, wide angle eyepieces. џThis irregular-shaped galactic [G/cluster] contains approximately 20 [G/star]s. џThis [G/cluster] of stars was first believed to be an extremely rich galactic cluster, then a loosely packed globular cluster. Today, it is generally considered to be a globular cluster which lies at a distance of 18,000 [G/light year]s. Through a small telescope, look for a fuzzy "star-like" object. At least a 10-inch (250mm) telescope is needed to [G/resolve] any [G/star]s within this cluster. џCygnus X-1:Cygnus X-1 is the best possible [G/black hole] candidate in the sky. While there is no visible star at this particular point, scientists have detected an extremely strong x-ray source. Also, not far away is a faint "companion" star, which appears to be orbiting the x-ray source at the very fast rate of once every 5.6 days. Scientists believe the x-rays are being emitted from super-heated material caught up in the gravitational pull of a black hole. From the orbital period of the companion star, it has been determined that the black hole is 20 to 35 times the mass of our [G/Sun] and lies at a distance of somewhere between 6,500 and 8,000 [G/light year]s. џDumbbell Nebula: This [G/planetary nebula] is approximately 1,000 [G/light year]s distant and 2 light years across. Through a small telescope, look for a hazy cloud with a slightly rectangular shape. Larger telescopes can begin to [G/resolve] the slight narrowing near the middle of the rectangle, thus giving it an hourglass or dumbbell appearance. џThis globular [G/cluster] is approximately 100,000 [G/light year]s away and 125 light years in diameter. The [G/star]s within this cluster are tightly bound together by gravity to form one of the most compact globulars in the sky. It is also believed to be the most distant. Through a small telescope, look for a fuzzy "star-like" object. џThis large, bright galactic [G/cluster] contains about 30 stars. Because it lies along the [G/Milky Way], it may be difficult to distinguish the stars of this cluster from the background stars of our galaxy. џCrescent Nebula: This faint diffuse [G/nebula] is a crescent-shaped, wispy cloud which lies against the backdrop of the [G/Milky Way]. A seventh [G/magnitude] [G/star] can be found within this cloud of gas and dust. џThis galactic [G/cluster] is approximately 7,200 [G/light year]s away and 15 light years in diameter. It is a compact cluster containing few [G/star]s. Because it lies along the [G/Milky Way], the stars in this cluster may be difficult to distinguish from the background stars of our [G/galaxy]. џV404 Cygni: This binary system consists of a [G/black hole] and a companion [G/star]. Astronomers detect an extremely strong x-ray source at this location which they believe is coming from an [G/accretion disk] surrounding a black hole. Gravity from the black hole pulls material from the companion star. The pull of gravity is so strong, it heats up the matter to the point where it emits x-rays, just before it is sucked into the black hole. This system is 10,000 light years away in the [G/constellation] of [Y/Cygnus]. џThe approximately 90 [G/star]s within this galactic [G/cluster] are loosely scattered, not packed tightly together. џThis globular [G/cluster] is closer, brighter, and larger than its nearby neighbor, [C/C42]. Through a small telescope, look for a fuzzy, "star-like" object. Larger telescopes can [G/resolve] individual [G/star]s around the cluster's border. џThis tightly bound galactic [G/cluster] contains approximately 100 [G/star]s. џThis spiral [G/galaxy] lies at a distance of 10-20 million [G/light year]s. When observing this galaxy through a small telescope, use a low-powered eyepiece for the brightest image possible. [G/Averted vision] aids in the detection of the tiny, irregular patch of light. Larger telescopes can [G/resolve] a faint mottling within the galaxy. џVeil Nebula: This entry represents the western portion of the Veil Nebula, a huge [G/supernova] remnant approximately 1,500 [G/light year]s distant. This faint arc of material appears to be drifting behind the [G/star] 52 Cygni. Look for a faint, narrow arc with a star near its center. The eastern portion of the veil is classified as [C/C33]. џPelican Nebula: This diffuse [G/nebula] is large and very faint. џThis globular [G/cluster] is approximately 60,000 [G/light year]s away. Through a small telescope, look for a faint, fuzzy "star-like" object. At least a 14-inch (355mm) telescope is needed to [G/resolve] any [G/star]s within this cluster. џThis entry represents the eastern portion of the Veil Nebula, a huge [G/supernova] remnant approximately 1,500 [G/light year]s distant. Low-power, wide angle eyepieces are essential for observing this tiny, faint arc of light. Large telescopes begin to resolve its filament structure, which is best seen on [G/CCD] images or long exposure astrophotographs. џN. American Neb.: This diffuse [G/nebula] gets its name from its unusual shape. Through a low-power, wide angle eyepiece this cloud looks like the North American continent. The nebula is approximately 1,600 [G/light year]s distant and 45 light years in diameter. џCharles [G/Messier] described this group as "three or four small stars which resemble a nebula at first sight." In actuality, there is no [G/nebula] or [G/cluster] within this region, just a few faint [G/star]s. џThis diffuse [G/nebula] appears as a faint, irregular patch of light surrounding a seventh [G/magnitude] [G/star]. Use a low-power eyepiece to locate the object, then switch to a medium-power eyepiece for more contrast. The larger the telescope, the brighter the image and the more detail you can [G/resolve] within the cloud. џThis globular [G/cluster] is approximately 185,000 [G/light year]s away and could be considered to lie outside of our galaxy. Through a small telescope, look for a faint, fuzzy, "star-like" object. џSaturn Nebula: This [G/planetary nebula] lies 4,000 [G/light year]s away and is 0.5 light years across. Look closely to observe a slight haziness around a star-like object. Through larger telescopes, its oval, Saturn-like appearance may be detected. The Saturn Nebula is best seen with high magnification. џPG2112+059: This [G/quasar] is over 1 billion [G/light year]s away. Because of its tremendous distance, this quasar is only visible through the largest telescopes. џThis globular [G/cluster] lies just off the nose of the flying horse, near the bright star [W/Enif]. M15 is approximately 39,000 [G/light year]s away and 130 light years in diameter. X-rays have been detected coming from this cluster, which may indicate the presence of one or more [G/black hole]s hidden within its core. Through a small telescope, look for a faint hazy patch. Larger telescopes can [G/resolve] individual stars around the fringes of the cluster. M15 is best seen using medium to high power eyepieces. џThis galactic [G/cluster] is approximately 800 [G/light year]s away and 7 light years in diameter. The [G/star]s within this cluster are scattered over a large area of sky, thus making it difficult to view the cluster in its entirety through a small telescope. Instead, one sees only a few bright stars at a time. Try observing the cluster with a low-power, wide angle eyepiece. Then, observe the cluster with binoculars. All the stars of the cluster should be visible within the [G/field of view] of the binoculars. џThis globular [G/cluster] is a tight ball of over 100,000 [G/star]s. M2 is 50,000 [G/light year]s away and 150 light years in diameter. Through a small telescope, look for a "hazy" star-like object. Larger telescopes are able to resolve individual stars around the edge of the cluster. M2 is best seen with medium or high magnification. џThis globular [G/cluster] is approximately 40,000 [G/light year]s away and 100 light years in diameter. This dense, compact sphere of stars appears as a faint round ball through a small telescope. Even larger telescopes may have difficulty resolving stars around the edge. This cluster is best observed using low to medium-power eyepieces. џThis diffuse [G/nebula] is a faint, mottled cloud that lies at the east end of a dark dust lane. It may be difficult to distinguish from the background [G/Milky Way]. џThis galactic [G/cluster] contains approximately 40 [G/star]s. џPG2209+184: This [G/quasar] is over 1 billion [G/light year]s away. Because of its tremendous distance, this quasar is only visible through the largest telescopes. џThis galactic [G/cluster] is a very loose grouping of approximately 40 [G/star]s. џHelix Nebula: Roughly 450 [G/light year]s away and 1.75 light years across, the Helix Nebula is the largest and closest [G/planetary nebula] in our skies. Through a small telescope, look for a small, round, hazy patch. The nebula is best seen with low-power, wide angle eyepieces. џThis spiral [G/galaxy] is approximately 50 million [G/light year]s away and 32,000 light years in diameter. Through a small telescope, look for an elongated, oval-shaped patch of light. џA faint diffuse [G/nebula]. џThis barred spiral [G/galaxy] is extremely faint and difficult to see, even under the best observing conditions. Large telescopes can begin to [G/resolve] the "barred" portion of the galaxy as a narrow streak of light. џBubble Nebula: Sometimes classified as a diffuse [G/nebula], this cloud of hydrogen gas appears as a dim, irregular haze surrounding a faint star. Its bubble appearance can only be seen on [G/CCD] images or long exposure astrophotographs. џThis galactic [G/cluster] is 3,000 [G/light year]s away and about 12 light years in diameter. [G/Star]s within this cluster are more tightly packed than in most other galactic clusters. It is best seen using medium-power eyepieces. џThis [G/planetary nebula] is between 2,000 and 5,600 [G/light year]s away. It appears as a faint, fuzzy "star-like" object through a small telescope. At least a 6-inch (152 mm) telescope is needed to detect its "sphere-like" qualities. џThis galactic [G/cluster] is 6,000 [G/light year]s away and 50 light years in diameter. It consists of a rich scattering of faint [G/star]s. The larger the telescope, the more stars are visible within the cluster. This cluster is best seen through low-power, wide angle eyepieces. џMercuryџMercury is named after the messenger god in Roman mythology (Greek counterpart is Hermes). Like its namesake, Mercury moves extremely fast across the sky. Faster than any other planet, in fact. Mercury is the only [G/planet] in the solar system without an atmosphere to protect its surface. As a result, Mercury gets very hot during the day, 660^F (350^C) and very cold at night, -274^F (-170^C). The only spacecraft to visit the planet ([G/Mariner 10], 1974) took photos showing [G/crater]s covering the entire planet. What you can see: From Earth, Mercury is too small to see any surface features. Safe viewing of the planet is difficult because of its proximity to the Sun. It is only visible within an hour of sunset or sunrise. With larger telescopes, it is possible to see the phases of Mercury. џVenusџVenus gets its name from the Roman goddess of beauty (Greek counterpart is Aphrodite). Because it is closer to the Sun than Earth, Venus is only visible in the early evening just after sunset, or in the early morning, just before sunrise. As a result, Venus is sometimes known as the Evening Star or Morning Star. It is extremely bright in the sky because Venus is the closest [G/planet] to Earth and it is covered with a thick layer of clouds that reflects the Sun's light like a mirror. These thick clouds hide the surface of Venus from view and trap the Sun's heat, causing the hottest surface temperatures found on any planet, 900^F (480^C). Since 1962, 22 US and USSR robotic missions have flown to Venus. Most recent [G/lander]: [G/Venera 14] (USSR), 1982. Most recent [G/orbiter]: [G/Magellan] (US), 1990. What you can see: The phases of Venus can be seen as it orbits around the Sun. No surface features are visible because of the thick clouds. џEarthџThe origin of Earth's name is unknown. Our planet is the only planet in the solar system capable of supporting liquid water. In fact, 70% of Earth's surface is covered by water. Earth is one of the most geologically active planets; volcanoes, earthquakes, hurricanes, floods, fires and severe storms are constantly resurfacing the planet, changing its appearance. Earth is also the only planet in the solar system known to support life. џMarsџThe planet Mars was named after the god of war in Roman mythology (Greek counterpart is Ares), appropriate because of its reddish, blood-colored appearance in the sky. This small [G/planet], half the size of Earth, has the largest canyon ([G/Mariner Valley]) and largest volcano, ([G/Olympus Mons]) in the solar system. Ancient river beds and flood plains indicate Mars was once warm enough to support liquid water. Today, a combination of frigid temperatures and an extremely thin atmosphere of carbon dioxide make it impossible for liquid water to exist. Since 1964, 14 US and USSR robotic missions have flown to Mars. The most recent [G/lander]: [G/Pathfinder] (US), 1997. The most recent [G/orbiter]: [G/Mars Global Surveyor] (US), 1997. What you can see: Mars appears as a tiny disk with a hint of reddish/orange color. With larger telescopes, polar ice caps and possible dark markings on the martian surface are visible. џJupiterџJupiter, the largest planet in the solar system, gets its name from the king of the gods in Roman mythology (Greek counterpart is Zeus). Over 1100 Earths could fit inside this gas giant planet. Jupiter does not have a solid surface. Instead, it is composed of hydrogen and helium gases. A spacecraft trying to land on Jupiter would pass through thicker and thicker clouds until it is crushed by the increasing [G/jovian] pressure. At its center, there might be an Earth-size solid core. Orbiting Jupiter is the largest [G/moon] in the solar system, [G/Ganymede]. [G/Galileo] discovered Ganymede and three other moons of Jupiter, (Io, Europa, and Callisto) in 1610. These moons were the first objects ever discovered with a telescope. There is one faint ring surrounding the planet which can not be seen from Earth. The ring was discovered by one of five spacecraft that have visited the planet: [G/Pioneer 10], 1973; [G/Pioneer 11], 1974; [G/Voyager 1], 1979; [G/Voyager 2], 1979; [G/Galileo spacecraft], 1995. What you can see: Several dark cloud bands stretching across a pale disk. As many as 4 of Jupiter's 16 moons can be seen, appearing like stars lined up next to the planet. The moons change places around Jupiter from night to night. Through larger telescopes: more details within the cloud bands can be resolved; moon shadows on the disk of the planet are visible. џSaturnџSaturn gets its name from the king of the mythical Titans. This gas giant planet is the most distant planet that can be seen without a telescope. The most prominent feature of Saturn is its beautiful [G/ring system], the largest in the solar system. The rings stretch across 169,000 miles (273,000 km), yet are only 0.5 miles (0.8 km) thick. [G/Galileo] observed the rings in 1610, but didn't understand what he was seeing. In 1675, G.D. [G/Cassini] discovered a dark gap in the rings. This gap, later named the [G/Cassini Division], is easily seen with 90mm and larger telescopes. Saturn also has more [G/moon]s than any other planet, 18. Several of these moons were discovered by the three visiting spacecraft: [G/Pioneer 11], 1979; [G/Voyager 1], 1980; [G/Voyager 2], 1981. What you can see: A small disk with the white ring system extending from both sides. The moon, [G/Titan], may be visible as a bright starlike object near the planet. The position of Titan changes as it orbits the planet. With larger telescopes: pale cloud bands on the planet can be resolved; ring and moon shadows on the planet, more divisions within the ring system. џUranusџUranus gets its name from an early mythological god who was a son of Mother Earth. This gas giant planet, discovered by William Herschel in 1781, was the first [G/planet] discovered with a telescope. Uranus is tilted on its side as it orbits the Sun. As a result, its seasons are unusual. For example, during summer at the North Pole, the Sun stays above the horizon for 42 [G/earth years]. At the same time, it is winter at the South Pole, with 42 years of frigid darkness. After 42 years, the seasons are reversed. Uranus has a [G/ring system] composed of several dark, thin rings. These rings are not directly visible from Earth, but were photographed by the [G/Voyager 2] spacecraft as it flew by the planet in 1986. What you can see: Extremely tiny disk with possible bluish/green color. With larger telescopes: a more distinct disk, more color. џNeptuneџNeptune gets its name from the mythical Roman god of the sea (Greek counterpart is Poseidon). Astronomers began searching for Neptune to explain irregularities in the orbit of [P/Uranus]. Uranus didn't follow its predicted path across the sky, so astronomers thought the gravity from another planet must be effecting the orbit. Using mathematics, they predicted where that other planet should be. In 1846, on the first night of searching, Neptune was discovered. [G/Voyager 2], flying by the planet in 1989, discovered the strongest winds in the solar system on this blue planet, winds of 1500 miles per hour (2400 km per hour). The [G/ring system] around Neptune is composed of a few dark "[G/clumpy]" rings. [G/Triton], Neptune's largest [G/moon], is the only moon in the solar system that travels in a [G/retrograde] direction around its planet, a direction opposite the way the planet rotates. What you can see - extremely tiny disk, with possible bluish/green color. With larger telescopes: a more distinct disk, more color. џPlutoџPluto was named after the ruler of the underworld in Roman mythology. Discovered in 1930, Pluto is the smallest planet in the solar system. No spacecraft has explored this distant world, but [G/Hubble telescope] images show a [G/planet] of high contrast, bright areas next to dark areas. It is so cold on Pluto that its atmosphere lies frozen on the ground. Pluto has the most elliptical [G/orbit] of all the planets. For twenty years, from 1979 to 1999, Pluto's odd orbit brings it closer to the Sun than [P/Neptune]. What you can see: Because of Pluto's tiny size and extreme distance, it is extremely difficult to see, even with larger telescopes. 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SlopeџWARNINGџWARNING494џEnter Rate Adj.џObject Position:џStars w/ PlanetsџMeteor ShowersџPeak onџPeak Rate џ/hrџDur. џStatisticsџBest view withџMagnificationџField of ViewџField_=_џMag._=_џK Char. FreeџTo Load SoftwareџTesting MotorsџDownloading џDo not turn off.џCtr. џPOLARISџAge: џPhase: џmiџRises_џSets_џSun Rises AtџSun Sets AtџMoon Rises AtџMoon Sets AtџNext Full MoonџNext New MoonџNext 1st QuarterџNext 3rd QuarterџSunџMercuryџVenusџMarsџJupiterџSaturnџUranusџNeptuneџPlutoџMoonџAlt Enc=_џAz Enc =_џFocus Control:џPosition: 00џReticleџSetџIntensityџRateџDuty CycleџLevel:5 Blink:0џRA__=_џDec_=_џTime_џLST__џTimer_џAlarm џBattery Level:џPoint Scope NџThen press EnterџSet Alt. to 0џSet Dec to 90џSet RA to HomeџCalculating...џConstellations:џNamed Object:џGalaxy:џNEBULA:џPLANETARY NEB:џCLUSTER:џMessier Object:џInvalid Number.џCaldwell Object:џSearching...џEnter NGC #:џObject Not FoundџEnter IC #:џNamed Star:џMultiple Star:џVariable Star:џVaridx:џNearby Star:џEnter SAO #џSAO:_џNOT FOUND.џGlossary:џG/GlossaryџA]џG/џEnter Date:џEnter Time:џFocal Len(mm):џAz/RA RatioџAlt/Dec RatioџAltAzџScope mountingџPolarџAdjust MountџSmart mount hasџbeen enabledџbeen disabledџErase training?џ1=Yes, 2=NoџPECџTraining PECџUpdating PECџWaiting..џSmart MountџErasing...џMount Training:џ1=On, 2=OffџReverse L/RџON џOFFџBlink OnџBlink OffџStart UpџTime UpdateџWhen NeededџTaking GPS FixџNew SiteџReading WWVBџLook Signal_џFound SignalџYESџNOџReverse UP/DOWNџAdj. with arrowsџDisplay ContrastџParking ScopeџScope parkedџTurn scope off.џDrive setup:џCenter referenceџobject.џPress  untilџit is centered.џPress ~ untilџPress  untilџPress  untilџPress < untilџPress > untilџPress ^ untilџPress v untilџSelect Star:џTargetRA_=_џTargetDec_=_џCenter StarџCenter usingџscrewsџBelow HorizonџPress ENTERџCurrent Targets:џTerrestrialџAstronomicalџError: You can'tџdelete this site.џDelete Site:џEnter Lat:џEnter Lon:џTime Zone:џSite Name:џError:џSite List FullџCountry/StateџCities index џStateloc:џG/State/ProvinceџNearest CityџG/Nearest CitiesџYour First NameџYour Last NameџAdr. Line 1џAdr. Line 2џYour CityџYour StateџPostal/Zip CodeџDate of BirthџEnter PIN#џUse Pin #?џSelect PIN#џNone FoundџSelect LandmarkџLandmarks FullџLandmark NameџCenter LandmarkџDel. LandmarkџH/Right AscensionџH/AltitudeџH/Local Mean TimeџH/AccessoryџH/BatteryџH/џTimer:џTimer StatusџAlarm TimeџAlarm StatusџAlign SuccessfulџAlignment FailedџCheck StarsџClosest ObjectџETX-60џETX-70џETX-80џETX-90џETX-105џETX-125џETX Traveler 60џETX Traveler 80џETX Traveler 90џDS-60џDS-70џDS-80џDS-90џDS-114џDS-127џLX90-8џLX90-10џLX90-12џDS-2060џDS-2070џDS-2076џDS-2080џDS-2090џDS-2102џDS-2114џDS-2130џDSX-90џDSX-102џDSX-125џLXD55/75 127 AcџLXD55/75 152 AcџLXD55/75 6 NewџLXD55/75 8 NewџLXD55/75 10 NewџLXD55/75 8 SCџToo near the SunџMS_TOURSџLargest (mins)џSmallest(mins)џBrightest (mag)џFaintest (mag)џObject TypesџNextџPreviousџMin. El.(deg.)џSerial OverrunџSpiral SearchџNorth Methodџ1=True 2=Compassџ^=True v=CompassџLT Mag. NorthџLT True NorthџLX90 Mag. NorthџLX90 True NorthџETXA Mag. NorthџETXA True NorthџDS Mag. NorthџDS True NorthџETXB Mag. NorthџETXB True NorthџNo Passes soonџMoon, NewџMoon, Waxing CreџMoon, First QuarџMoon, Waxing GibџMoon, FullџMoon, Waning GibџMoon, Third QuarџMoon, Waning CreџMessier џCaldwell џNGC џIC џBlack HoleџDiffuse NebulaџDark NebulaџAsterismџElliptical Gal.џGlobular ClusterџIrregular Gal.џOpen ClusterџPlanetary NebulaџQuasarџSpiral GalaxyџGalaxyџUnnamedџCoordinates OnlyџMagnitude: џMagnitude: џSize: џSAO џClass: џMulti Sep. џDist:џLYџ=TOO MANY LINKS=џLink not found:џMag: џMass:џxEarthџDiam:џDist:џauџDay:џDaysџhrs џOrb:џyrsџGrav:џDay Temp:џNite Temp:џMoons:џTelescope StatusџUse ETX AutoStarџwith this modelџIncompatibleџHandboxџ1-Zipcode 2-CityџEnter ZipcodeџLocation OptionџAt Breakpoint: џStack Reg = џIn Debugger> џddress џreakmask [џesetџtack = џatch џeprom =џ- Invalid commandџAlt=_џAz_=_џEl_=_џNot AlignedџSlewing...џBelow HorizonџCHECK_MOUNTџFlash Memory ErrџInitializing....џERROR:џFile Space FullџReorganizing...џENTER to Sync.џSynchronized.џSync not allowedџon this objectџNorthџSouthџEastџWestџEnter PercentџSpeed_=_џFastџMediumџSlowџFineџ/secџGuideџUnit DoneџSending DataџProtect Bit SetџFail Self TestџTest DoneџStarfinderџAutostar 494џCalibrationџERROR in RAџERROR in DecџPress ENTER toџstart testџTesting MotorsџFinding RAџFinding DecџComprob motoresџERROR en baseџERROR en brazoџPrepare laџpruebaџPrueba de MotorџBuscando RAџBuscando DecџPic Failure VџU5џU80џLX-90 DSXџMaster SlaveџMaestro Esclavoџ90 105 125џ8 10 12џHoraџElements ExpiredџTracking...џPass Located...џVersion_џSIG OCTџџAutostarџMemory FullџUpdating planetary data #џ Welcome toџA U T O S T A RџPress 0 to Alignџor MODE for MenuџRelevelingџCenter BrightestџStar, Push ENTERџPress 0 for TourџAUTOMATIC ALIGNџSelecting StarџLess than 5'џfrom the poleџPole isџSelect ItemџObjectџSolar SystemџMercuryџVenusџMarsџJupiterџSaturnџUranusџNeptuneџPlutoџMoonџAsteroidsџSelectџAddџDeleteџEditџCometsџSelectџAddџDeleteџEditџConstellationџDeep SkyџNamed ObjectsџGalaxiesџNebulasџPlanetary Neb.џStar ClustersџQuasarsџBlack HolesџIC ObjectsџNGC ObjectsџCaldwell ObjectsџMessier ObjectsџStarџNamedџSAO CatalogџDoubleџVariableџNearbyџWith PlanetsџSatelliteџSelectџAddџDeleteџEditџLandmarksџSelectџAddџDeleteџEditџUser ObjectџSelectџAddџDeleteџEditџIdentifyџBrowseџStart SearchџEdit ParametersџEventџSunriseџSunsetџMoonriseџMoonsetџMoon PhasesџNext Full MoonџNext New MoonџNext 1st Qtr џNext 3rd Qtr џMeteor ShowersџSolar EclipsesџLunar EclipsesџMin. of AlgolџAutumn EquinoxџVernal EquinoxџWinter SolsticeџSummer SolsticeџGuided TourџGlossaryџUtilitiesџTimerџSetџStart/StopџAlarmџSetџOn/OffџEyepiece Calc.џField of ViewџMagnificationџSuggestџBrightness Adj.џContrast Adj.џBattery AlarmџLandmark SurveyџSleep ScopeџPark ScopeџSetupџAlignџEasyџAutomaticџOne StarџTwo StarџThree StarџNo NameџDateџTimeџDaylight SavingsџTelescopeџTelescope ModelџFocal LengthџAz/RA RatioџAlt/Dec RatioџMountџLXD55/75 AdjustџAz/RA PercentџAlt/Dec PercentџTracking RateџSiderealџLunarџCustomџReverse L/RџReverse UP/DOWNџCalibrate MotorџTrain DriveџAz/RA TrainџAlt/Dec TrainџRA TrainџDec. TrainџPEC EraseџPEC On/OffџPEC UpdateџPEC TrainџCal SensorsџSmart DriveџTargetsџHigh PrecisionџSiteџSelectџAddџDeleteџEditџNameџLatitudeџLongitudeџTime ZoneџObstructionsџAddџDeleteџEditџOwner Info.џNameџAddressџStreetџCityџStateџZip CodeџCountryџCloneџCatalogsџToursџSoftwareџAllџDownloadџStatisticsџSun WarningџGetting StartedџDisplay OptionsџCord WrapџMax. ElevationџMin. AOSџQuiet SlewџBeepџWWVBџSun AlignџBrightest StarџGPSџResetџAdjust MountџWithout using the hand controller, adjust the mount's latitude setting and azimuth settings until the pole star is centered in the eyepiece. Once the pole star is centered, you should lock the mount in place and press ENTER. If you wish to abort polar alignment, press MODE. џAlarmџThe Alarm function beeps at a selected time, if active. In the Alarm menu, the Set function enters the alarm time. The On/Off function activates the alarm. The Alarm time is seen in the [H/Telescope Status] Display. After pressing MODE to leave this message, press ENTER to see the alarm menu and use the SCROLL keys to see the alarm choices. џAlignџFor the telescope to accurately locate objects in the night sky, it must be aligned. Autostar can align the telescope in one of three ways; Easy, One Star and Two Star. Easy align helps by selecting two alignment stars and explaining each step of the process. One Star and Two Star Align expect the user to pick the alignment stars. After pressing MODE to leave this message, press ENTER to see the alignment menu and use the SCROLL keys to see the three alignment choices. џAlt/Dec RatioџAlters the altitude/dec. encoder ratio. Do not use this function unless directed to do so by Meade Instructions. Press MODE to leave this message. џAltAz AlignџPut the telescope in the Alt. Az. home position and pointed North (see the Instruction Manual). The vertical axis home position, for all telescopes, is with the telescope tube level (declination to 0^). The horizontal axis Home position for ETX telescope is found by turning the tube counterclockwise until it stops. Then turn the telescope clockwise until the fork arm is over the Computer Control panel. Without leaving the Home position, move the WHOLE telescope (do not use the handbox) so the tube is pointing north. Press ENTER when done. џAltitude AxisџThe axis responsible for moving the telescope up or down. џAutomatic AlignџPut the telescope in the LNT home position (see the Instruction Manual). The horizontal axis Home position for ETX 90/105/125 telescopes is found by turning the tube counterclockwise until it stops. The vertical axis does not have a home position. Press ENTER when done. џAutostar HelpџThis description can be discontinued at any time by pressing the MODE key. If the message is moving too fast or slow, press one of the SCROLL keys (triangle keys at the bottom of the keypad). Autostar is a menu oriented system with lists of functions. Functions are activated using the 20 keys of the handbox keypad. Pressing any key firmly and releasing causes a single entry of that key. Holding a key down causes a repeated entry until it is released. The top line of this display shows the currently active function (in this case, Autostar Help). The bottom line shows information or a new menu list. When the bottom line is a list, pressing the SCROLL keys makes items in the list visible (one at a time). To activate a function shown on the bottom line, press the ENTER key. The active function will then be displayed on the top line and new information will appear on the bottom line. The ENTER key is also used to complete data entries. To return to a previous menu, press the MODE key. The MODE key, if held down 2 seconds, will cause the Telescope Status display to appear. The Telescope Status display has information about telescope position, motor speeds, timer, alarm and other telescope status. The GO TO key moves the telescope to objects from the OBJECT menu. The four ARROW keys (near the top of the keypad) move the telescope in four directions at selected speeds. When entering data, the right and left ARROW keys are used to move the cursor to a particular field and up and down ARROW keys scroll through selections, like months in a date. The Numeric keys set telescope motor speeds when not used to enter numeric data. To set a motor speed, press a number key between 1 (slowest) and 9 (fastest). The utility light (on top of the handbox) is used to illuminate objects (like a watch). The "0" key turns the light on or off. The SCROLL keys (at the bottom) move through menus and adjust moving message speeds. The "?" key is used for HELP, and give a brief explanation of the current function. In some messages, there may be bracketed words, called "hypertext". Pressing the ENTER key while a hypertext term is visible, will display information about that term. Pressing the MODE key will return to the original message. The brightness and contrast of this display can be changed using the Brightness or Contrast functions in the Utilities menu. The Autostar system description is now complete and information must be entered to operate the telescope. To make these entries without further explanation, press the MODE key. Remember, the "?" key can be pressed at any time to explain a particular operation. For additional assistance entering the telescope data, press the "?" key now. This message will repeat until the MODE key or the "?" Key is pressed. џAutumn EquinoxџThe Autumn Equinox gives the local time and date for the beginning of Fall (in the Northern Hemisphere, Spring in the Southern Hemisphere). After pressing MODE to leave this message, press ENTER to see the date and time of Fall. џAZ/RA RatioџAlters the azimuth/RA encoder ratio. Do not use this function unless directed to do so by Meade Instructions. Press MODE to leave this message. џAzimuth axisџThe axis responsible for moving the telescope side to side. Press MODE to Return. џBattery AlarmџThe Battery Alarm function beeps when the batteries are low. In the Battery Alarm menu, use the SCROLL keys (followed by ENTER) to disable (or enable) the low battery alarm. The battery level is seen in the [H/Telescope Status] Display. After pressing MODE to leave this message, press ENTER to start the battery alarm menu. џBrightness Adj.џAdjusts the brightness of the message display and the keypad. After pressing MODE to leave this message, press ENTER to adjust the brightness. џCalibrate MotorџThis function calibrates the telescope motor encoders and saves the values in Autostar memory. During calibration both motors will move briefly. This function was done automatically when power was first applied to Autostar and does not need to be repeated unless the Autostar handbox is moved to a different telescope. After pressing MODE to leave this message, press ENTER to calibrate the motor encoders. џCHECK MOUNTџSlewing to this object may cause the telescope to hit the mount. Press the GO TO key to proceed. Press MODE to abort. Pressing any key during slewing will stop the telescope's movement. Press MODE to leave this message. џCloneџThe Clone function transfers data from one Autostar to another by the serial interface using a special Meade cable. Data can include objects, software or both and is selected in the Clone menu. The unit sending is put in the Clone mode and the unit receiving is placed in the download mode. Once transfer of data has started, do not interrupt the process or Autostar memory will be corrupted. After pressing MODE to leave this message, press ENTER to see the Clone menu and use the SCROLL keys to see the menu choices. џConstellationџThe Constellation menu lists all 88 Constellations. Use the SCROLL keys to see the entries and press ENTER to select a Constellation. Information about the Constellation can be seen using the SCROLL keys. Pressing the GO TO key causes the telescope to point at the Constellation or list the stars of the constellation. If stars are listed use the SCROLL keys to see the entire list and press GO TO a second time to point at the stars. For objects to be found, the telescope must be aligned (see the Setup Menu). After pressing MODE to leave this message, press ENTER to see the Constellation menu and use the SCROLL keys to see the menu choices. џContrast Adj.џAdjusts the contrast of the message display. In cold weather, this is used to make moving messages more readable. After pressing MODE to leave this message, press ENTER to adjust the contrast. џCountry/StateџFind the nearest Country or State of the current telescope location by pressing the SCROLL keys at the bottom of the keypad. Press ENTER to select a displayed location. Press MODE briefly to abort the selection. Press MODE to leave this message. џCtr.џAutostar has selected the brightest alignment star in the sky. Accuracy in performing prior steps determines how close the telescope is pointing at the correct star. Locate the brightest star near the current position of the telescope. Center the star in the telescope viewfinder by pressing the four ARROW keys as needed. Next, center the star in the main eyepiece and press ENTER. If the star selected is behind an obstacle, press a SCROLL key and Autostar will select another star. Press MODE to leave this message. џDateџAfter reading this instruction, enter today's date using the Numeric keys. When the month is highlighted, press the SCROLL keys to change the month. To change the year, use the ARROW keys at the top of the keypad to select a digit, then press a Numeric key. To make corrections to any entry, use the left or right ARROW keys to move the cursor. When the displayed date is correct, press ENTER. The utility Light on top of the handbox has been turned on to illuminate a watch. Press MODE to leave this message. џDaylight SavingsџIf Daylight Savings time is in effect (clocks are set ahead 1 hour, Spring to Fall), change the display to read "YES" by using the SCROLL keys. If the current time is Standard Time, change the display to read "NO". When the display is correct, press ENTER. Press the MODE key to leave this message. џDeep SkyџThe Deep Sky menu lists distant astronomical objects. Use the SCROLL keys to see catalogs, which include; Named Objects, Galaxies, Nebulas, Planetary Nebula, Star Clusters, Quasars, Black holes and other catalogs. After pressing MODE to leave this message, press ENTER to see the Deep Sky menu and use the SCROLL keys to see the menu choices. џDownloadџDownload causes Autostar to accept data from the serial interface. Data can include object data, software or both. Data can come from another Autostar in the Clone mode or from a Personal Computer. A special Meade cable must connect the serial port to the other unit for transfer of data. Once transfer of data has started, do not interrupt the process or Autostar memory will be corrupted. After pressing MODE to leave this message, press ENTER to start the Download menu and use the SCROLL keys to see the menu choices. џDS Mag. NorthџTo place the telescope in the Magnetic North Home Position, use a compass and adjust the telescope in the azimuth direction until telescope tube is pointing in the direction of magnetic north. Lock the azimuth axis. Next, adjust the telescope tube in the vertical direction until level and lock the elevation axis. The telescope is now in the Magnetic North Home Position. Press the ENTER key to continue. џDS True NorthџTo place the telescope in the True North Home Position, rotate the telescope in the azimuth direction until it points in the direction of True North. In the Northern Hemisphere, Polaris can be used to find True North. In the Southern Hemisphere, you must use other means to locate True North. Lock the azimuth axis. Next, adjust the telescope tube in the vertical direction until level and lock the elevation axis. The telescope is now in the True North Home Position. Press the ENTER key to continue. џEasyџEasy align is designed to help the novice quickly align the telescope. Autostar selects the best two alignment stars and moves the telescope nearby. After centering the stars, alignment is complete. After pressing MODE to leave this message, press ENTER to begin Easy align. џEnter Date:џEnter the current date by pressing the Numeric keys. To change between months, press a SCROLL key. Use the left or right ARROW keys to move the cursor to any digit. Press ENTER when the displayed date is correct. The Light on top of the handbox has been turned on to illuminate a watch. Press MODE to leave this message. џEnter Time:џEnter the current local time by pressing the Numeric keys. To change between AM or PM, press a SCROLL key. Use the left or right ARROW keys to move the cursor to any digit. Press ENTER when the displayed time is correct. The Light on top of the handbox has been turned on to illuminate a watch. Press MODE to leave this message. џETXA Mag. NorthџPut the telescope in the Alt. Az. home position and pointed in the direction of Magnetic North (see instructional manual). The vertical axis home position is with the telescope tube level (Dec at 0^). The horizontal axis home position for ETX telescopes is found by turning the tube counter clockwise until it stops. Then turn the telescope clockwise until the fork arm is over the computer control panel. Without leaving the home position, move the WHOLE telescope (do not use the handbox) so the tube is pointing toward Magnetic North. Press enter when done. џETXA True NorthџPut the telescope in the Alt. Az. home position and pointed in the direction of True North (see instructional manual). The vertical axis home position is with the telescope tube level (Dec at 0^). The horizontal axis home position for ETX telescopes is found by turning the tube counter clockwise until it stops. Then turn the telescope clockwise until the fork arm is over the computer control panel. Without leaving the home position, move the WHOLE telescope (do not use the handbox) so the tube is pointing in the direction of True North. Press ENTER when done. џETXB True NorthџTo place the telescope in the True North Home Position, rotate the telescope in the azimuth direction until it points in the direction of True North. In the Northern Hemisphere, Polaris can be used to find True North. In the Southern Hemisphere, you must use other means to locate True North. Lock the azimuth axis. Next, adjust the telescope tube in the vertical direction until level and lock the elevation axis. The telescope is now in the True North Home Position. Press the ENTER key to continue. џETXB Mag. NorthџTo place the telescope in the Magnetic North Home Position, use a compass and adjust the telescope in the azimuth direction until telescope tube is pointing in the direction of magnetic north. Lock the azimuth axis. Next, adjust the telescope tube in the vertical direction until level and lock the elevation axis. The telescope is now in the Magnetic North Home Position. Press the ENTER key to continue. џEventџThe Event menu lists important astronomical events. After pressing MODE to leave this message, press ENTER to see the Event menu and use the SCROLL keys to see the menu choices. џEyepiece Calc.џThe eyepiece calculation menu gives eyepiece information, such as; [G/Field of View], Magnification and the best eyepiece for the object currently in view. After pressing MODE to leave this message, press ENTER to see the Eyepiece Calc. menu and use the SCROLL keys to see the menu choices. џFocal LengthџFocal Length changes the telescope focal length value in Autostar memory. After pressing MODE to leave this message, press ENTER to change the focal length value. џGerman NorthџRemember to turn off the Polar reticle when alignment is complete. Put the telescope in the polar Home position as described in the Instruction Manual. Use the keypad to set the declination to 90^. Adjust the RA axis so the telescope is directly over the top of the mount. Look through the eyepiece as you move the RA axis back and forth. The stars in the eyepiece will spin around the center of the eyepiece if you have the declination set to exactly 90^. If the stars do not spin around the center of the eyepices, adjust the declination and try the RA axis again until you have the stars swirling around the center of the eyepice. Now recenter the telescope over the top of the mount USING ONLY the RA control. Next adjust the telescope tripod (DO NOT USE THE KEYPAD) so that the tube is pointing north. Now set the scope's elevation so your latitude is shown by the pointer. If you do not know your latitude, get it from the Setup-Site menu. џGerman SouthџRemember to turn off the Polar reticle when alignment is complete. Put the telescope in the polar Home position as described in the Instruction Manual. Use the keypad to set the declination to 90^. Adjust the RA axis so the telescope is directly over the top of the mount. Look through the eyepiece as you move the RA axis back and forth. The stars in the eyepiece will spin around the center of the eyepiece if you have the declination set to exactly 90^. If the stars do not spin around the center of the eyepices, adjust the declination and try the RA axis again until you have the stars swirling around the center of the eyepice. Now recenter the telescope over the top of the mount USING ONLY the RA control. Next adjust the telescope tripod (DO NOT USE THE KEYPAD) so that the tube is pointing south. Now set the scope's elevation so your latitude is shown by the pointer. If you do not know your latitude, get it from the Setup-Site menu. џGetting StartedџFor a detailed description of the Autostar system, press the "?" key at the bottom of the keypad, otherwise press ENTER to continue. џGlossaryџThe Glossary has definitions of astronomy, telescope and space related terms in alphabetical order. Use the SCROLL keys to pick the beginning letter of a term, and press ENTER. Use the SCROLL keys again to select a term and press ENTER to see the definition. After pressing MODE to leave this message, press ENTER to see the Glossary menu and use the SCROLL keys to select a letter. џGuided TourџGuided Tour lists the best astronomical objects for viewing tonight. Objects can be selected using the ENTER key. Pressing GO TO will also move the telescope to any selected object. After pressing MODE to leave this message, press ENTER to see the Guided Tour Menu and use the SCROLL keys to see the list of objects. џHigh PrecisionџPlaces Autostar in the High Precision mode to improve accuracy in locating dim objects. In High Precision mode, Autostar will go to a bright object near the target object. After centering the bright object and pressing ENTER, Autostar will then move to the target object. Use the SCROLL keys to select ON or OFF and press ENTER. After pressing MODE to leave this message, press ENTER to start the High Precision Menu and use the SCROLL keys (followed by ENTER) to enable or disable high precision operation. џHome PositionџPut the telescope in the home position and press the [H/ENTER key]. The home position for this telescope is described in the AutoStar User's guide or in the Telescope Manual. This home position is required by AutoStar to avoid positions that would interfere with telescope operation. This message will repeat until the [H/MODE Key] is pressed. џIdentifyџIdentify names the object seen in the telescope eyepiece by searching the catalogs. Use the SCROLL keys to see information about the object. For an object to be identified, the telescope must be aligned (see the Setup Menu). After pressing MODE to leave this message, press ENTER to identify the object in the eyepiece. џLandmarksџLandmarks defines and locates land objects. For landmarks to be added or located, the telescope must be aligned to an existing landmark. To align, use the Select option to chose an existing landmark, point the telescope at the landmark and hold ENTER for two seconds. Press ENTER again to "sync" and Autostar is landmark aligned. After alignment, another existing landmarks can be found using the Select option and pressing GO TO. Use the Add option to expand the list of landmarks. After pressing MODE to leave this message, press ENTER to see the Landmarks Menu and use the SCROLL keys to see the menu of options. џLandmark SurveyџLandmark Survey moves the telescope to all landmarks in turn, pausing at each one. Landmark Survey is stopped by pressing MODE. For landmarks to be found, the telescope must be landmark aligned. After pressing MODE to leave this message, press ENTER to start the Landmark Survey. џLT Mag. NorthџTo place the telescope in the Magnetic North Home Position, place the bubble level/compass into the diagonal prism and use the compass feature to point the telescope in the direction of Magnetic North. Next, level the telescope tube using the bubble level indicator. The telescope is now in the Magnetic North Home Position. Press the ENTER key to continue. џLT True NorthџTo place the telescope in the True North Home Position, rotate the telescope in the azimuth direction until it points in the direction of True North. Next, place the bubble level/compass into the diagonal prism and level the telescope tube using the bubble level indicator. The telescope is now in the True North Home Position. Press the ENTER key to continue. џLunar EclipsesџLists eclipses of the Moon. Use the SCROLL keys to see the list by date, press ENTER to select a choice. Use the SCROLL keys to see information about the Eclipse. After pressing MODE to leave this message, press ENTER to see the list of eclipses and use the SCROLL keys to see a particular event. џLXD55/75 AdjustџThis procedure is to help align the scope with the mount. Please see the manual for more instructions. џLX90 Mag. NorthџTo place the telescope in the Magnetic North Home Position, point the telescope in the general direction of North. Place the Bubble Level/Compass into the diagonal prism and adjust the telescope in the azimuth direction until the colored portion of the compass needle points in the same direction as the telescope tube. Lock the azimuth axis. Next, level the telescope tube using the bubble level indicator, and lock the elevation axis. The telescope is now in the Magnetic North Home Position. Press the ENTER key to continue. џLX90 True NorthџTo place the telescope in the True North Home Position, rotate the telescope in the azimuth direction until it points in the direction of True North. In the Northern Hemisphere, Polaris can be used to find True North. In the Southern Hemisphere, you must use other means to locate True North. Lock the azimuth axis. Next, adjust the telescope tube in the vertical direction until level and lock the elevation axis. The telescope is now in the True North Home Position. Press the ENTER key to continue. џMenu HelpџUse the SCROLL keys to see the other menu choices and press ENTER to make a selection. To return to the previous menu, press MODE briefly. If MODE is held for two seconds, the [H/Telescope Status] Display will appear. For a more detailed description of Autostar press ENTER now for [H/Autostar Help]. This message will repeat until MODE is pressed. џMeteor ShowersџLists Meteor Showers during the year. Use the SCROLL keys to see the events, press ENTER to chose one. Use the SCROLL keys to see information about the meteor shower. After pressing MODE to leave this message, press ENTER to see the list of meteor showers and use the SCROLL keys (followed by ENTER) to see a particular event. џMin. of AlgolџAlgol is a variable star that changes brightness every 2.8 days. Autostar gives the time of the next minimum brightness. After pressing MODE to leave this message, press ENTER to see the date and time of the next minimum brightness of Algol. џMoon PhasesџLists the date and time of the next four phases of the Moon. Use the SCROLL keys to select one of the four phases and press ENTER to see the next event. After pressing MODE to leave this message, press ENTER to see the moon phase options and use the SCROLL keys (followed by ENTER) to see a particular event. џMoonriseџGives the local time of the next Moonrise. After pressing MODE to leave this message, press ENTER to see the moonrise time. џMoonsetџGives the local time of the next Moonset. After pressing MODE to leave this message, press ENTER to see the Moonset time. џMotor Unit FaultџAutostar has detected a motor failure. Moving the handbox between scopes, low battery levels, obstructed or overloaded scopes can cause this failure. If the telescope was stalled, remove the obstruction or overload. After leaving this message, the telescope will recalibrate the motors. The telescope will NEED TO BE REALIGNED before you can resume viewing. Should you continue to get this message with fresh batteries, contact Meade customer support. Press MODE to leave this message. џMountџSelects the AltAz or Polar telescope configuration. Most telescope are AltAz, the only Polar configuration is with the ETX on a special tripod. After pressing MODE to leave this message, press ENTER to see the Mount menu and use the SCROLL keys to see the options. џMS BacklashџFor this operation use a terrestrial object. After each step, when the object is centered, press ENTER. Press ENTER now to proceed. џMS ContrastџUse the scroll up and down keys to adjust the display contrast. Press ENTER when finished. џMS ResetџThis command will clear all the information entered into Autostar and reset to factory defaults. Press ENTER to proceed, or MODE to abort. џNearest CityџFind the nearest City to the current telescope location by pressing the SCROLL keys at the bottom of the keypad. Press ENTER to select a displayed city. Press MODE to leave this message. џNorth MethodџLocating North is one of the most important ingredients in the alignment of a telescope. True North is the axis which the Earth spins about and is a key reference for the motion of the Earth. As you look at the night sky, the stars seem to move; in fact, if you watched long enough or took a long time-exposure photograph, you'd realize that the stars seem to revolve around one point, the pole, or True North. When AutoStar knows where True North is and also knows the time, it can calculate the location of all the other objects in the sky. One traditional way to find True North is to locate the North Star, Polaris, which lies very close to True North. Magnetic/Compass North is not True North, but a measurement of the magnetic lines of the Earth. Magnetic North deviates several degrees or more from True North. AutoStar, using the observation site location determined by the GPS and magnetic North information, can calculate the position of True North. Some areas are subject to local magnetic disturbances, and the magnetic field of the Earth changes slightly from year to year. AutoStar allows you to adjust for discrepancies in the local magnetic field. џObjectџThe Object menu contains catalogs of astronomical, terrestrial and user defined objects. After pressing MODE to leave this message, press ENTER to see the Object menu and use the SCROLL keys to see the list of catalogs. џOne StarџOne Star align is designed for fast alignment of the telescope. The user must select a known star and move the telescope to it manually. This alignment is not as accurate as Easy or Two star alignment. After pressing MODE to leave this message, press ENTER to begin One Star align. џOwner Info.џOwner Information stores the owners name and address. Use the SCROLL and ENTER keys to select the name or address option. Use the ARROW keys to move the cursor (right or left). Numbers are entered using the numeric keys and letters are entered using the up or down ARROW keys. Press ENTER when an entry is complete and correct. After pressing MODE to leave this message, press ENTER to see the Owner Info. menu and use the SCROLL keys to see the options. џPark ScopeџPark Scope moves the telescope to the home position and beeps. At the Home position, turn off the power. The next time power is turned on, if the telescope is not moved and time is entered accurately, no alignment will be necessary. After pressing MODE to leave this message, press ENTER to park the telescope. џPH Tour ObjectsџThe Tour object list is seen using the SCROLL keys. Press ENTER to select an object. Information about a selected object is seen using the SCROLL keys. Pressing the GO TO key will cause the telescope to point at the object. For objects to be found, the telescope must be aligned (see the Setup Menu). Press MODE to leave this message. џPoint Scope NџPoint the front of the telescope in the direction of true North and press the [H/ENTER key]. It is not required that the telescope to be pointed precisely North, pointing it generally North is sufficient. Later in the alignment process, AutoStar will select stars to be used for precision alignment. The closer the telescope is pointed at true North the easier it will be to identify the alignment stars. For suggestions on ways to find true North, refer to your AutoStar User's Guide. This message will repeat until the [H/MODE Key] is pressed. џPolar AlignџPut the telescope in the Polar Home position as described in the instruction manual. Adjust the tripod legs so the wedge is in a level position. Use the keypad to set the Declination to 90^. Adjust the RA axis to the 00 H.A. position so the telescope fork arms are level and the viewfinder is on the top side of the telescope. If in the Northern Hemisphere, the telescope should be pointing in the direction of Polaris, the North Star. In the Southern Hemisphere, the telescope should be pointing in the direction of Sigma Octantis. Press the ENTER key to continue. џResetџReset returns Autostar to factory defaults and erases all user memory. After pressing MODE to leave this message, press ENTER to reset Autostar. џReverse L/RџReverses the action of the left and right ARROW keys. Use the SCROLL keys to select ON (reversed) or OFF (normal) option and press ENTER. After pressing MODE to leave this message, press ENTER to see the Reverse L/R menu and use the SCROLL keys to see the options. џReverse UP/DOWNџReverses the action of the UP and DOWN ARROW keys. Use the SCROLL keys to select ON (reversed) or OFF (normal) option and press ENTER. After pressing MODE to leave this message, press ENTER to see the Reverse UP/DOWN menu and use the SCROLL keys to see the options. џSatelliteџThe Satellite menu is used to locate man-made objects orbiting Earth. Four options (Select, Add, Delete and Edit) are chosen using the SCROLL keys and pressing ENTER. To locate and track a satellite, use the Select function. The other functions modify the existing Satellite table. Satellite orbits vary greatly and need to be frequently corrected. For objects to be found, the telescope must be aligned (see the Setup Menu). After pressing MODE to leave this message, press ENTER to see the Satellite menu and use the SCROLL keys to see the options. џScope HomeџPut your telescope in the home position and press the [H/ENTER key]. The home position for your telescope is described in the AutoStar User's guide or in your Telescope Manual. This home position is required by AutoStar to avoid positions that would interfere with telescope operation. This [H/Help Menu] will repeat until you press the [H/MODE Key]. џSet Alt. To 0џSet the [H/Altitude axis] of the telescope to 0 and press the [H/ENTER key]. Put simply, move the telescope tube up or down until it is level. When level, press the [H/ENTER key]. This message will repeat until the [H/MODE Key] is pressed. џSetupџThe Setup menu is used for Autostar settings required for the operation and alignment of the telescope. After pressing MODE to leave this message, press ENTER to see the Setup menu and use the SCROLL keys to see the options. џSiteџSite defines the observing location of the telescope. Up to six sites can be saved in Autostar memory. Site options include; Select, Add, Delete and Edit. The Select option determines the current observing site. Add, Delete and Edit options are used to change the Site tables. After pressing MODE to leave this message, press ENTER to see the Site menu and use the SCROLL keys to see the options. џSleep ScopeџSleep powers down the telescope to conserve batteries and maintains alignment. Press any Autostar key to resume operation. After pressing MODE to leave this message, press ENTER to put Autostar in the low power mode. џSolar EclipsesџLists eclipses of the Sun. Use the SCROLL keys to see the list by date, press ENTER to select a choice. Use the SCROLL keys to see information about the Eclipse. After pressing MODE to leave this message, press ENTER to see the list of eclipses and use the SCROLL keys to see a particular event. џSolar SystemџThe Solar System menu contains objects in our Solar System, including; eight Planets, the Moon, Asteroids and Comets. For objects to be found, the telescope must be aligned (see the Setup Menu). After pressing MODE to leave this message, press ENTER to see the Solar System menu and use the SCROLL keys to see the object choices. џStarџThe Star menu contains stars sorted by category. The categories include; named stars, SAO Catalog, Double stars, Variable stars, Nearby stars and stars with Planets. For objects to be found, the telescope must be aligned (see the Setup Menu). After pressing MODE to leave this message, press ENTER to see the Star menu and use the SCROLL keys to see the object categories. џStatisticsџThe Statistics menu shows the amount of available user memory and the Autostar software revision number. After pressing MODE to leave this message, press ENTER to see the Statistic menu and use the SCROLL keys to see the information. џSummer SolsticeџThe Summer Solstice gives the local time and date for the beginning of Summer (in the Northern Hemisphere, Winter in the Southern Hemisphere). After pressing MODE to leave this message, press ENTER to see the date and time of Summer. џSunriseџGives the local time of the next sunrise. After pressing MODE to leave this message, press ENTER to see the sunrise time. џSunsetџGives the local time of the next sunset. After pressing MODE to leave this message, press ENTER to see the sunset time. џTargetsџThe Targets menu puts Autostar into the terrestrial or astronomical mode of operation. In astronomical mode the telescope tracks the moving sky. Use the SCROLL keys to see the options and press ENTER to make a selection. After pressing MODE to leave this message, press ENTER to see the Target menu and use the SCROLL keys to see the options. џTelescope ModelџSelect the Telescope model by pressing the SCROLL keys. The telescope model can be found in the Telescope Instruction Manual or on the foil label attached to the telescope tube. Press ENTER when the display is correct. Press MODE to leave this message. џTelescope StatusџThe Telescope Status Display shows the values useful in operating the telescope and accessories. To enter this display, hold the MODE key for more than 2 seconds and release. Use the SCROLL keys to see values such as; telescope position, time, alarm, timer, battery level and accessory status. The motor slew speed is shown in the upper right corner of the display as a bar graph. While the telescope position is displayed, pressing GO TO, will cause Autostar to request new position values and slew to that location when ENTER is pressed. To return to the previous menu press MODE briefly. џTimeџThe Time function is used to change local time in Autostar. After pressing MODE to leave this message, press ENTER to change Autostar time. џTimerџThe Timer beeps after a time period is complete. Use the "Set" option to select a Timer value up to 24 hours. Use the Start/Stop option to begin timer operation. The timer value is in the [H/Telescope Status] Display. After pressing MODE to leave this message, press ENTER to see the Timer menu and use the SCROLL keys to see the options. џTracking RateџTracking Rate adjusts rate the telescope uses to follow objects in the sky. There are three rate choices; Sidereal, Lunar or Custom. After pressing MODE to leave this message, press ENTER to see the Tracking Rate menu and use the SCROLL keys to see the options. џTrain DriveџTrain Drive calibrates the telescope motors to improve pointing accuracy. Carefully train each axis. After pressing MODE to leave this message, press ENTER to see the Train Drive menu and use the SCROLL keys (followed by ENTER) to select an axis to train. џTwo StarџTwo Star alignment requires an advanced user (familiar with the sky) to select two stars and manually move the telescope to both during the alignment operation. After pressing MODE to leave this message, press ENTER to begin Two Star align. џUser ObjectџUser Object defines and locates new astronomical objects. Four options (Select, Add, Delete, Edit) are chosen using the SCROLL keys and pressing ENTER. To create and modify the object table, use Add, Delete or Edit. To locate an object use the Select option. For objects to be found, the telescope must be aligned (see the Setup Menu). After pressing MODE to leave this message, press ENTER to see the User Object menu and use the SCROLL keys to see the options. џUtilitiesџThe Utilities menu has nine options to help operate the telescope. After pressing MODE to leave this message, press ENTER to see the Utilities menu and use the SCROLL keys to see the options. џVernal EquinoxџThe Vernal Equinox gives the local time and date for the beginning of Spring (in the Northern Hemisphere, Fall in the Southern Hemisphere). After pressing MODE to leave this message, press ENTER to see the date and time of Spring. џWARNINGџLOOKING AT OR NEAR THE SUN WILL CAUSE IRREVERSIBLE DAMAGE TO YOUR EYE. DO NOT POINT THIS TELESCOPE AT OR NEAR THE SUN. DO NOT LOOK THROUGH THE TELESCOPE AS IT IS MOVING. TO INDICATE YOU HAVE READ AND UNDERSTOOD THIS MESSAGE, PRESS THE "5" KEY. џWARNING494џLOOKING AT OR NEAR THE SUN WILL CAUSE IRREVERSIBLE DAMAGE TO YOUR EYE. DO NOT POINT THIS TELESCOPE AT OR NEAR THE SUN. DO NOT LOOK THROUGH THE TELESCOPE AS IT IS MOVING. TO INDICATE YOU HAVE READ AND UNDERSTOOD THIS MESSAGE, PRESS THE "SPEED" KEY. џWinter SolsticeџThe Winter Solstice gives the local time and date for the beginning of Winter (in the Northern Hemisphere, Summer in the Southern Hemisphere). 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(Y/N) AxC : џ AxD : џBootLoader Monitor џ > AUxDT : џ >BBootLoader Monitor Help џ0 : Toggle AuX Clk U : Read AuX Dat Z : Toggle AuX Dat A : AuX Device Address џV : AutoStar Program Version M : EEPROM Reader џP : EEPROM Writer џR : Memory Block Dump B : Memory Blank Check W : Flash Write (word) 1 : Flash Sector Erase 2 : Memory/Flash Copy џ3 : Memory/Flash Compare J : To DownLoad Mode T : RA/Dec Monitor L : Msg to LCD C : Cmd to LCD Q : Aux Test (06) Y : Aux Time Module Test (07) X : eXit Aux Device Address : AutoStar System Version : џ џEEPROM Reader Addr (0000-03ff) : ODat : џEEPROM Writer Addr (0000-03ff) : ODat : џ NDat (00-ff) : џ UDat : џ Flash Sector Erase, Sector Address (HH,D0-FF): Display Memory Address (HHHHHH) : џ џ: џ Flash Word Writer Address (HHHHHH) : Word (HHHH) : Blank check Start Address (HHHHHH) : To Address (HHHHHH) : џ: џ џBlank Check Pass џFlash Sector Erase Address (HHHHHH) : Copy Start Address (HHHHHH) : џ End Address (HHHHHH) : џ To Address (HHHHHH) : џ Copying .. Copying .. Copy done џ Compare Start Address (HHHHHH) : To Address (HHHHHH) : With Address (HHHHHH) : џ: џ ***** џ: џ Compare done Exiting ...Msg to LCD : CMD to LCD (00-FF) : Role Call to Device : џ GPSResp OK GPSResp NFG џ Role Call to Device : џ Level Call Time Read џ Setup I2C Addr Read I2C Addr џ CMD Test Aux CMd : џ Aux ADR : џRA/Dec Monitor, AnyKey to Stop!!џR :%5dџ E :%3dD :%5dџ E :%3d Role Call : Delay Time Read џ Setup I2C Addr Read I2C Addr џ? H for Helpџ`іЪk Љшю‚xYk Ÿk k єX+k w {Бeu GERROR.ModeџCopy Boot SystemџPress Checking.EP...џChecking.MD...џError CopyџCompleted..Press џBootLoader Monitor Mode BootLoader DownLoad Mode џBootLoader BootLoader ... Ready џ>DownLoad RSMode џBootLoader BootLoader ... Ready џ>Copy Boot Systemџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџ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A@Bџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџ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џџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџ€џ ј ј ј ј ј ј јј јјјјј ј ј ј ј ј ј ј јјј ј ј ј ј ј ј ј ј јј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј ј јџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџџђ ђbђ’hђВpђыџџTonight's Best В!TTonight's BestThis is a tour of tonight's finest sights with your telescope. The objects are roughly ordered by difficulty. The easiest objects are first and as you go further through the list, the objects become progressively fainter and more difficult to see.At the point objects become too difficult to see, you can exit the tour, find a darker location, or buy a bigger telescope! P PPPYEFLarge Mag. CloudFSmall Mag. CloudM*MM-C)M,C[MWSIRIUSCPCCjMC^S№“C\MWALBIREOWVEGAWARCTURUSM"M#C]WACHERNARWBETELGEUSEM)M%MMM WACRUXWALTAIRMM WALDEBARANM$WSPICAWANTARESWFOMALHAUTWDENEBMM&MWREGULUSMM\C?S&ыM4CMWENIFMMS!ћMDM3MRMhMOMM C5M9!TStars w/planetsThe following stars have been determined to have planets orbiting them. These are the first stars for which we evidence that solars systems like our own are not unique. {SцˆSb‰S–’SІлS›|Sђ‘S%ЊSўS^:ScTNone VisisbleThis evening, none of the stars with planets were visible from your location }PPN1 NЅCcFCygnus X-1!TQuasarsThe following objects are QUASARS. This is short for 'Quasi stellar objects'. These are perhaps the most distant objects from Earth visible with a telescopes. {FPG1011-040FPG1012+008FPG1216+069FPG1435-067FPG2112+059FPHL909FPKS0537-441FV404 CygniTNone VisisbleThis evening, no quasars were visible from your location }!TThe EndThanks for taking the tour of 'Tonight's Best Objects. (c)1999 Meade Instruments. #ђЯ2џџA Star's Life Ы,!TIntroductionStars, like everything else in the universe are born, live out their lives and die. Stars have extremely long lifetimes, making it impossible for a human to observe an entire stellar life cycle. But, you can look around the sky and see examples of young stars, middle age stars and old stars, all in one night. G{!UиЮяThe NurseryThe Tarantula Nebula is an example of the first step in a star's life, a stellar nursery. Press MODE to learn more about stellar nurseries. !Uќ/The NurseryThe Rosette Nebula is an example of the first step in a star's life, a stellar nursery. Press MODE to learn more about stellar nurseries. !UЇЙўThe NurseryThe Great Orion Nebula is an example of the first step in a star's life, a stellar nursery. Press MODE to learn more about stellar nurseries. !Uo?šњThe NurseryThe Trifid Nebula is an example of the first step in a star's life, a stellar nursery. Press MODE to learn more about stellar nurseries. !U?IњThe NurseryThe Lagoon Nebula is an example of the first step in a star's life, a stellar nursery. Press MODE to learn more about stellar nurseries. !Ub@ХќThe NurseryThe Eagle Nebula is an example of the first step in a star's life, a stellar nursery. Press MODE to learn more about stellar nurseries. !U€@5ќThe NurseryThe Swan Nebula is an example of the first step in a star's life, a stellar nursery. Press MODE to learn more about stellar nurseries. !TThe NurseryA star's life begins in a diffuse nebula. These nebulae are sometimes called stellar nurseries. There are no stellar nurseries visible at this time, but you can learn more about them by pressing MODE. }G!TThe NurseryStars are born within a huge cloud of gas and dust known as a diffuse nebula. The gas cloud is illuminated by the newly formed stars which heat up the gas and cause it to glow. As more and more stars are formed, the gas and dust within the nebula is gradually used up. The nebula itself disappears and in its place is an open cluster. G{!U~  KindergartenThis group of newly formed stars is called an open cluster, or "stellar kindergarten". To find out more about these young stars, press MODE. !UM ЇKindergartenThis group of newly formed stars is called an open cluster, or "stellar kindergarten". To find out more about these young stars, press MODE. !UБKindergartenThis group of newly formed stars is called an open cluster, or "stellar kindergarten". To find out more about these young stars, press MODE. !Uй$ћKindergartenThis group of newly formed stars is called an open cluster, or "stellar kindergarten". To find out more about these young stars, press MODE. !UМёKindergartenThis group of newly formed stars is called an open cluster, or "stellar kindergarten". To find out more about these young stars, press MODE. !UyЏKindergartenThis group of newly formed stars is called an open cluster, or "stellar kindergarten". To find out more about these young stars, press MODE. !UА%ш№KindergartenThis group of newly formed stars is called an open cluster, or "stellar kindergarten". To find out more about these young stars, press MODE. !U '@ђKindergartenThis group of newly formed stars is called an open cluster, or "stellar kindergarten". To find out more about these young stars, press MODE. !UT-мёKindergartenThis group of newly formed stars is called an open cluster, or "stellar kindergarten". To find out more about these young stars, press MODE. !U5pѓKindergartenThis group of newly formed stars is called an open cluster, or "stellar kindergarten". To find out more about these young stars, press MODE. !Uь>зїKindergartenThis group of newly formed stars is called an open cluster, or "stellar kindergarten". To find out more about these young stars, press MODE. !UGRoKindergartenThis group of newly formed stars is called an open cluster, or "stellar kindergarten". To find out more about these young stars, press MODE. !TKindergartenNewly formed stars usually can be found in loose groups called open clusters. There are currently no bright open clusters visible in the sky. However, you can still learn about these "stellar kindergartens" by pressing MODE. }G!TKindergartenAfter all of the gas and dust has been used up within a diffuse nebula, all that is left is a loose grouping of very young stars, an open cluster. The stars within this group may gradually drift apart over time. G{!UбMiddle AgeAlpheratz is an example of a middle aged star. Stars spend millions, billions, or even trillions of years at this stage, contently burning their fuel, shining brightly in the sky. !UЙ–ђMiddle AgeAchernar is an example of a middle aged star. Stars spend millions, billions, or even trillions of years at this stage, contently burning their fuel, shining brightly in the sky. !UŽЧ Middle AgeCapella is an example of a middle aged star. Stars spend millions, billions, or even trillions of years at this stage, contently burning their fuel, shining brightly in the sky. !UЇѓMiddle AgeCanopus is an example of a middle aged star. Stars spend millions, billions, or even trillions of years at this stage, contently burning their fuel, shining brightly in the sky. !UЛќMiddle AgeSirius is an example of a middle aged star. Stars spend millions, billions, or even trillions of years at this stage, contently burning their fuel, shining brightly in the sky. !U<#ЮMiddle AgeRegulus is an example of a middle aged star. Stars spend millions, billions, or even trillions of years at this stage, contently burning their fuel, shining brightly in the sky. !UО+7ёMiddle AgeAcrux is an example of a middle aged star. Stars spend millions, billions, or even trillions of years at this stage, contently burning their fuel, shining brightly in the sky. !U"2~Middle AgeArcturus is an example of a middle aged star. Stars spend millions, billions, or even trillions of years at this stage, contently burning their fuel, shining brightly in the sky. !UХEUMiddle AgeAltair is an example of a middle aged star. Stars spend millions, billions, or even trillions of years at this stage, contently burning their fuel, shining brightly in the sky. !U#QMiddle AgeMarkab is an example of a middle aged star. Stars spend millions, billions, or even trillions of years at this stage, contently burning their fuel, shining brightly in the sky. !TMiddle AgeJust about every star in the sky that you can see without the aid of a telescope is a middle aged star. Stars spend millions, billions, or even trillions of years at this stage, contently burning their fuel, shining brightly in the sky. }{!U*оRetirementAldebaran is a red giant star, an example of a star in retirement. Press MODE to find out more. !UЯМRetirementBetelgeuse is a red supergiant star, an example of a star in retirement. Press MODE to find out more. !Uљ9ЯљRetirementAntares is a red supergiant star, an example of a star in retirement. Press MODE to find out more. }G!TRetirementAs a star begins to run out of fuel, its outer layers swell to huge sizes. As it swells, the star's surface cools off, giving it a red glow. A star like our Sun will become a red giant. A much larger star swells to become a red supergiant. G{!URчEnd of the LineThe Eskimo Nebula is an example of a planetary nebula, the end of the line for a star like our Sun. To find out more, press MODE. !U›#†іEnd of the LineCaldwell 74 is an example of a planetary nebula, the end of the line for a star like our Sun. To find out more, press MODE. !UlBОEnd of the LineThe Ring Nebula is an example of a planetary nebula, the end of the line for a star like our Sun. To find out more, press MODE. !UJFSEnd of the LineThe Dumbbell Nebula is an example of a planetary nebula, the end of the line for a star like our Sun. To find out more, press MODE. !UJV§End of the LineThe Saturn Nebula is an example of a planetary nebula, the end of the line for a star like our Sun. To find out more, press MODE. !UO ћEnd of the LineThe Helix Nebula is an example of a planetary nebula, the end of the line for a star like our Sun. To find out more, press MODE. !UŒќEnd of the LineNGC 2438 is an example of a planetary nebula, the end of the line for a star like our Sun. To find out more, press MODE. !U‘bџџ887 Alinda ии ?ЦР@ЉЄAБ!нBn#ЏCqƒCі(\AТѕНђzbџџ1362 Griqua иі|Н> N@0ЊСArЪђBSƒCCmђBHс2Aš™>ђЖbџџ1373 Cincinnati иЩуЁ>lyZ@TуBиС”CO/ЧB•фAC333Aš™>ђђbџџ1566 Icarus иЖS?ї‰?ƒбЖAm'АBЩeњAкГŠC33‡Aš™>ђ.cџџ1620 Geographos иГЯЋ> qŸ?ffUAxЂЈC;hŠCH‘БCš™yAš™>ђjcџџ1627 Ivar иЈRЫ>Vю?Ѕ,AФ1C‹'CDКЏC33SAš™?ђІcџџ1685 Toro и˜/п>Џ?№AG+‰C*)ўBхУBЎcAš™>ђтcџџ1864 Daedalus иАV?aќК?з’БAu“ж@ЖФЂCЉŽCš™mAš™>ђdџџ1865 Cerberus иа я>ѓ>Š?*К€AЦќTCs˜ЂCfЧBRИ†Aš™>ђZdџџ1866 Sisyphus ият ?GXђ?ƒР$B]\~Bоƒ’CщoCPAš™>ђ–dџџ1916 Boreas иц>х|@їNA”_ЊCЏхЇCˆБCHсnAš™>ђвdџџ1917 Cuyo иN ? 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