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List of stars in Musca

From Wikipedia, the free encyclopedia

This is the list of notablestars in theconstellationMusca, sorted by decreasing brightness.

NameBVarHDHIPRADecvis.
mag.		abs.
mag.		Dist. (ly)Sp. classNotes
α Musα1096686158512h 37m 11.08s−69° 08′ 07.9″2.69−2.17306B2IV-Vβ Cep variable,Vmax = 2.68m,Vmin = 2.73m,P = 0.0903 d; Member of the Lower Centaurus–Crux subgroup of theScorpius–Centaurus association.[1]
β Musβ1108796232212h 46m 16.87s−68° 06′ 29.1″3.04−1.86311B2V + B3VBinary star, Member of the Lower Centaurus–Crux subgroup of theScorpius–Centaurus association.[1]
δ Musδ1129856361313h 02m 15.78s−71° 32′ 55.7″3.611.3990.8K2IIIBinary star
λ Musλ1022495736311h 45m 36.57s−66° 43′ 43.8″3.680.66128A7III
γ Musγ1090266119912h 32m 28.11s−72° 07′ 58.7″3.84−1.14324B5V53 Persei variable,Vmax = 3.84m,Vmin = 3.86m,P = 2.72926 d
ε Musε1068495992912h 17m 34.64s−67° 57′ 38.4″4.06−0.77302M5IIIsemiregular variable,Vmax = 3.99m,Vmin = 4.31m,P = 40 d
μ Musμ1025845758111h 48m 14.49s−66° 48′ 53.5″4.75−0.86432K4IIIslow irregular variable,Vmax = 4.71m,Vmin = 4.76m
η Musη1149116466113h 15m 15.00s−67° 53′ 40.4″4.79−0.68405B8VAlgol variable,Vmax = 4.76m,Vmin = 4.81m,P = 2.3963 d; probable member of the Lower Centaurus–Crux subgroup of theScorpius–Centaurus association.[1]
HD 1152111152116482013h 17m 13.03s−66° 47′ 00.3″4.86−2.941185K2Ib/IIsuspectedvariable
HD 1030791030795785111h 51m 51.27s−65° 12′ 21.2″4.89−0.19338B4VBinary star
HD 1028391028395769611h 49m 56.63s−70° 13′ 32.8″4.98−3.271455G5Ib
GT MusGT1013795686211h 39m 29.63s−65° 23′ 51.9″5.01−1.17561G2III + AAlgol andRS CVn variable,Vmax = 4.96m,Vmin = 5.23m,P = 2.75459 d
ι1 Musι11162446546813h 25m 07.36s−74° 53′ 15.0″5.040.85225K0III
HD 99104991045559711h 23m 21.43s−64° 57′ 17.0″5.09−0.73475B5VDouble system with HD 99103.
ζ2 Musζ21075666032012h 22m 07.39s−67° 31′ 19.5″5.150.09336AmDouble system, Member of the Lower Centaurus–Crux subgroup of theScorpius–Centaurus association.[1]
λ Cha(λ)[2]1053405915112h 07m 50.09s−75° 22′ 01.4″5.17−0.47438K2II/III
HD 1048781048785888412h 04m 38.95s−68° 19′ 44.0″5.340.25339A0VMember of the Lower Centaurus–Crux subgroup of theScorpius–Centaurus association.[1]
θ Musθ1139046409413h 08m 07.16s−65° 18′ 21.7″5.44−12.17~7000WC6 + O9.5IEclipsing triple system, one component is aWolf–Rayet star,Vmax = 5.5m,Vmin = 5.52m,P = 18.341 d
HD 99264992645565711h 24m 11.18s−72° 15′ 23.8″5.55−1.61883B2IV-V
HD 1113151113156260812h 49m 44.95s−71° 59′ 10.5″5.55−0.49526G8Ib/II
HD 116458κ[3]1164586552213h 25m 50.40s−70° 37′ 38.1″5.65−0.12464Apvariable star, ΔV = 0.010m,P = 149.25373 d
ζ1 Musζ11075676032912h 22m 12.03s−68° 18′ 25.9″5.730.31396K0IIIDouble system
HD 1089701089706118112h 32m 09.90s−73° 00′ 03.8″5.880.78341K1III
HD 1003821003825628711h 32m 20.00s−66° 57′ 42.6″5.891.09298K1IIICN...
HD 1046001046005872012h 02m 37.76s−69° 11′ 32.2″5.891.01308B9Vvariable star, ΔV = 0.004m,P = 0.3 d; member of the Lower Centaurus–Crux subgroup of theScorpius–Centaurus association.[1]
HD 1145701145706446613h 12m 48.77s−66° 13′ 36.4″5.911.20285A0V(n)
HD 1143711143716439013h 11m 51.38s−69° 56′ 31.3″5.922.70144F3IV/VDouble system
HD 1122191122196316512h 56m 31.72s−72° 11′ 06.7″5.93−0.72698G8III
LS MusLS1131206368813h 03m 05.36s−71° 28′ 32.6″5.93−2.491575B1.5IIIneBe star
HD 1011621011625672711h 37m 48.51s−67° 37′ 13.3″5.940.80348K0III
HD 1051511051515905012h 06m 23.08s−65° 42′ 33.9″5.95−0.25566G8/K0IIIBinary star
HD 1154391154396499413h 19m 18.99s−72° 02′ 07.7″6.040.37445K3III
S MusS1061115955112h 12m 47.03s−70° 09′ 06.4″6.05−2.441630F6IbCepheid variable,Vmax = 5.89m,Vmin = 6.49m,P = 9.66007 d
HD 1067971067975989812h 17m 06.36s−65° 41′ 34.6″6.061.00335A0VMember of the Lower Centaurus–Crux subgroup of theScorpius–Centaurus association.[1]
HD 1151491151496479013h 16m 45.05s−65° 08′ 17.3″6.063.11127F5V
HD 1159671159676528913h 22m 52.62s−72° 08′ 48.0″6.06−0.74746B6VBinary star; suspected variable,Vmax = 6.05m,Vmin = 6.16m
HD 99872998725597911h 28m 18.46s−72° 28′ 26.3″6.09−0.74758B3Vsuspected variable
HD 1170251170256578313h 29m 07.98s−64° 40′ 32.8″6.091.36288A2m
BO MusBO1093726140412h 34m 54.46s−67° 45′ 24.8″6.11−1.331003M6II/IIIsemiregular variable,Vmax = 5.3m,Vmin = 6.56m,P = 132.4 d
HD 1183441183446657413h 38m 45.83s−70° 26′ 41.1″6.110.47438K3III
HD 1107161107166221212h 45m 02.07s−68° 49′ 50.7″6.16−2.711940F6Ia
HD 116890EZ1168906575513h 28m 46.82s−69° 37′ 37.6″6.17−0.48698B8Vα² CVn variable, ΔV = 0.09m,P = 4.3127 d
HD 1073011073016018312h 20m 28.28s−65° 50′ 33.5″6.201.22323B9VMember of the Lower Centaurus–Crux subgroup of theScorpius–Centaurus association.[1]
HD 1066761066765985112h 16m 23.87s−72° 36′ 52.1″6.211.16333A0V
KY MusKY1098676170312h 38m 52.37s−67° 11′ 35.0″6.22B1Iaα Cyg variable
HD 1051381051385904612h 06m 19.93s−68° 39′ 05.0″6.23−2.581884G3Ib
HD 98672986725530811h 19m 36.58s−75° 08′ 32.8″6.260.20532B9.5/A0V
FH MusFH1100206179612h 39m 55.90s−66° 30′ 40.0″6.261.09353B8Vrotating ellipsoidal variable, ΔV = 0.03m,P = 0.58 d; probable (80%) member of the Lower Centaurus–Crux subgroup of theScorpius–Centaurus association.[1]
HD 1080541080546060112h 25m 17.62s−65° 46′ 10.6″6.292.89156G8/K0IV
HD 1050711050715900312h 05m 53.63s−65° 32′ 48.8″6.30B8Ia-Iabvariable star, ΔV = 0.013m,P = 1.45408 d
R MusR1103116198112h 42m 05.03s−69° 24′ 27.2″6.31−2.551929F7IbCepheid variable,Vmax = 5.93m,Vmin = 6.73m,P = 7.510211 d
HD 1139191139196411713h 08m 27.84s−67° 47′ 48.3″6.34−1.091000M1III
HD 1077731077736041712h 23m 15.04s−67° 37′ 55.8″6.362.83166K0IV-V
HD 1176511176516615213h 33m 35.92s−65° 37′ 57.4″6.361.21349A0V
HD 1149121149126468213h 15m 25.77s−69° 40′ 45.1″6.371.51306K2/K3III
HD 1034821034825808511h 54m 44.62s−66° 22′ 33.7″6.383.20141F2IV
HD 98695986955535011h 20m 04.16s−71° 59′ 39.6″6.41−0.42758B4V
HD 1045701045705870612h 02m 28.59s−71° 29′ 20.4″6.410.86421K1III
HD 1047521047525881012h 03m 44.54s−74° 12′ 50.7″6.44−0.81921G6III
HD 98671986715533211h 19m 50.84s−72° 57′ 29.8″6.460.59486A0V
HD 1098571098576173812h 39m 14.64s−75° 22′ 14.1″6.46−0.40769B8Vn
HD 101805(π2)[4]1018055709211h 42m 14.82s−75° 13′ 38.3″6.483.80112G1V
HD 1058221058225938912h 11m 01.22s−68° 15′ 39.4″6.48−0.82939K0/K1III
HD 118522κ[5][6]1185226666813h 40m 40s70° 55′ 06″6.59–0.86309K0III
ι2 Musι21165796562813h 27m 18.58s−74° 41′ 30.2″6.620.71495B9V
HD 1005461005465637911h 33m 25.44s−70° 11′ 41.2″6.70337B9Vnehas an unconfirmed planet (b), Member of the Lower Centaurus–Crux subgroup of theScorpius–Centaurus association.[1]
HD 1124101124106324212h 57m 32.0s−65° 38′ 47″6.86440G8IIIhas aplanet (b)
GQ MusGQ11h 52m 02.35s−67° 12′ 20.2″7.2nova andAM Her variable
HD 105056GS1050565899812h 05m 49.88s−69° 34′ 23.0″7.3416000O9.5Iaα Cyg variable,Vmax = 7.34m,Vmin = 7.55m,P = 3.85253 d
HD 1112321112326253412h 48m 51.75s−68° 25′ 30.5″7.615.3194G8Vhas aplanet (b)
TU MusTU1002135619611h 31m 10.92s−65° 44′ 32.1″8.4115000O7.5V + O9.5Vβ Lyr variable,Vmax = 8.17m,Vmin = 8.75m,P = 1.3872833 d
RT MusRT3108315726011h 44m 32.88s−67° 18′ 18.9″8.573500F8Cepheid variable,Vmax = 8.57m,Vmin = 9.32m,P = 3.086131 d
T MusT1156736511613h 21m 13.85s−74° 26′ 31.0″8.602040C+seimregular variable,Vmax = 7.6m,Vmin = 8.6m,P = 111.8 d
KZ MusKZ1098856175112h 39m 19.16s−71° 37′ 18.5″9.0911000B2IIIβ Cep variable
HD 1083411083416078812h 27m 31.0s−71° 25′ 23″9.36161K2Vhas a planet (b)
UU MusUU1031375788411h 52m 17.72s−65° 24′ 15.1″9.541490F8:pCepheid variable,Vmax = 9.13m,Vmin = 10.28m,P = 11.63641 d
SY MusSY10033611h 32m 10.01s−65° 25′ 11.6″10.202770MpeZ Andromedae and semiregular variable,Vmax = 10.2m,Vmin = 12.7m,P = 624.5 d
MP MusMP13h 22m 07.55s−69° 38′ 12.2″10.39K1VeT Tauri star, ΔV = 0.127m,P = 3.714 d
Y MusY6391113h 05m 48.20s−65° 30′ 46.6″10.50698FpR CrB variable
TV MusTV31073011h 39m 50.76s−64° 48′ 59.3″10.75755F2W UMa variable
LP 145-1415736711h 45m 42.92s−64° 50′ 29.5″11.5115.106DQ64th-closestwhite dwarf
GRS 1124-683GU11h 26m 26.60s−68° 40′ 32.3″13.3K3V-K7VX-ray nova
2S 1254-690GR12h 57m 30.15s−69° 17′ 19.0″19.1Low-mass X-ray binary,Vmax = 18m,Vmin = 19.1m,P = 0.1636 d
PSR J1141-654511h 41m 07.02s−65° 45′ 19.1″25.08pulsar/white dwarf binary
KN MusKN11762213h 33m 32.86s−65° 58′ 27.1″1780WC2/WO1central star ofplanetary nebulaNGC 5189
Table legend:

 • Name =Proper name
 • B =Bayer designation
 • F or/and G. =Flamsteed designation orGould designation
 • Var =Variable star designation
 • HD =Henry Draper Catalogue designation number
 • HIP =Hipparcos Catalogue designation number
 • RA =Right ascension for theEpoch/Equinox J2000.0
 • Dec =Declination for the Epoch/Equinox J2000.0

 • vis. mag. = visual magnitude (m ormv), also known asapparent magnitude
 • abs. mag. =absolute magnitude (Mv)
 • Dist. (ly) = Distance inlight-years from Earth
 • Sp. class = Spectral class of the star in thestellar classification system
 • Notes = Common name(s) or alternate name(s); comments; notable properties [for example: multiple star status, range of variability if it is a variable star, exoplanets, etc.]

See also

[edit]

Notes

[edit]
  1. ^abcdefghijde Zeeuw, P.T.; Hoogerwerf, R.; de Bruijne, J.H.J.; Brown, A.G.A.; Blaauw, A. (1999). "A Hipparcos Census of Nearby OB Associations".Astronomical Journal.117 (1):354–99.arXiv:astro-ph/9809227.Bibcode:1999AJ....117..354D.doi:10.1086/300682.S2CID 16098861.
  2. ^Labelled asLambda Chamaeleontis (λ Cha/λ Chamaeleontis) in Bode's Uranographia
  3. ^Designated as Kappa Muscae by Bode in his Uranographia
  4. ^Labelled asPi2 Chamaeleontis (π2 Cha/π2 Chamaeleontis) in Bode's Uranographia
  5. ^In Bode's Uranographia
  6. ^Dropped byFrancis Baily

References

[edit]
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