List of stars in Sagittarius


This is the list of notable stars in the constellation Sagittarius, sorted by decreasing brightness.
NameBFG.VarHDHIPRADecvis.
mag.
abs.
mag.
Dist. Sp. classNotes
ε Sgrε2061169022901851.79−1.44145B9.5IIIKaus Australis, Thalith al Warida
σ Sgrσ34112175191928552.05−2.14224B2.5VNunki, Thani al Sadira
ζ Sgrζ38130176687935062.600.4289A3IVAscella, Thalith al Sadira
δ Sgrδ1954168454899312.72−2.14306K3IIIKaus Media
λ Sgrλ2267169916904962.820.9577K1IIIbKaus Borealis
π Sgrπ41147178524941412.88−2.77440F2II/IIIAl Baldah, Nir al Beldat, Lucida Oppidi
γ2 Sgrγ21028165135886352.980.6396K0IIIAlnasl, Nash, Nushaba, Awal al Warida
η Sgrη46167618896423.10−0.20149M2IIIRabi al Waridairregular variable
φ Sgrφ2795173300920413.17−1.08231B8.5IIIAwal al Sadira
τ Sgrτ40139177716938643.320.48120K1/K2IIIRabi al Sadira
ξ2 Sgrξ237120175775930853.52−1.77372G8/K0II/III
ο Sgrο39136177241936833.760.61139K0III
μ Sgrμ1341166937893413.84>3000B2III:Polis; quintuple star; Algol variable
ρ1 Sgrρ144174181577951683.921.06122F0III/IVδ Sct variable
β1 Sgrβ1168181454952413.96−1.36378B9VArkab Prior
α Sgrα177181869953473.960.38170B8VRukbat, Alrami
ι Sgrι241188114980324.120.30189K0III
β2 Sgrβ2172181623952944.271.13139F2IIIArkab Posterior
θ1 Sgrθ1256189103984124.37−2.02617B2.5IV
62 Sgrc62265V3872189763986884.43−1.26448M4IIIV3872 Sgr; part of the Terebellum; irregular variable
υ Sgrυ46176181615951764.52−4.031672B2Vpe+A2IaSthe prototypical hydrogen-deficient binary; Be star
X Sgr32X161592870724.53−3.061076F7IICepheid variable
59 Sgrb159250188603981624.54−3.301207K3IIIpart of the Terebellum
HD 16563431165634888394.55−0.59348K0IIICNpvar
52 Sgrh252207184707964654.590.77189B8/B9V
γ1 Sgrγ126W164975885674.66−4.362076G0Ib/IINash; W Sgr; Cepheid variable
HD 16781851167818896784.66−2.00700K3III
ω Sgrω58248188376980664.702.8278G3/G5IIITerebellum, part of the Terebellum
4 Sgr415163955881164.74−0.89436B9V
HD 189831268189831987614.77−0.70405K4III
21 Sgr2165169420902894.81−1.50597A1/A2V
60 SgrA60255189005983534.84−0.25340G8II/IIIpart of the Terebellum
HD 17291091172910919184.86−0.84451B2VNóngzhàngrén
ν1 Sgrν132111174974927614.86−3.911852K1IIAinalrami, Ain al Rami
ψ Sgrψ42155179950946434.86−0.16330K0/K1III+..
56 Sgrf56229186648972904.870.88205K0III
43 Sgrd43160180540948204.88−1.20535K0III
1 Sgr1140166464891534.960.59244K0III
HD 190056270190056988424.990.00324K1III/IV
14 G. Sgr14163755880605.00−2.29934K5/M0III
ν2 Sgrν235113175190928455.000.41270K1Ib/IIAin al Rami
61 Sgrg61253188899982585.010.25292A2V
ξ1 Sgrξ136119175687930575.02−5.925015B9.5Ib
χ1 Sgrχ147181182369954775.020.87221A4IV/VNamalsadirah III
55 Sgre255225186005969505.061.42175F3IV/V
76 G. Sgr76170680908065.121.04213B9/B9.5V
29 Sgr29104174116923905.22−1.59749K2III
77 G. Sgr77171034910145.28−3.902233B2III/IV
15 Sgr1543167264894395.29B0/1Ia/ab
54 Sgre154221185644968085.300.92245K1III
θ2 Sgrθ2256189118984215.301.89157A4/A5IV
V3961 Sgr235V3961187474977495.320.24339A0pα² CVn variable
HR 7703279191408994615.326.4120K2Vnearby binary star
V4050 Sgr59V4050168733900745.33−1.06619B7Ib/IIα² CVn variable
7 Sgr720164584883805.37−2.281105F2/F3II/III
75 G. Sgr75170479907635.370.22350A5V
28 Sgr2899173460921115.37−2.601278K5III
χ3 Sgrχ349182182416955035.45−0.50505K3III
193 G. Sgr193183275958655.461.00254K1/K2III
212 G. Sgr212184985965365.463.01101F7V
14 Sgr1442167036893695.49−0.46505K2III
24 Sgr2478171115910045.49−4.623432K3III
134 G. Sgr134177074936675.49−0.63546A0V
226 G. Sgr226186185970635.492.67120F5V
126 G. Sgr126176162932255.51−0.48514B4V
153 G. Sgr153179497944375.51−0.68565K3III
228 G. Sgr228186500972605.51−0.61545B8III
32 G. Sgr32165687888165.521.10249K0III
60 G. Sgr60168838901245.520.57319K0III
37 G. Sgr37166023890205.530.31360K1III +
114 G. Sgr114175317928825.563.03104F5/F6IV/V
V4024 Sgr144V4024178175939965.56−2.801531B2Vγ Cas variable; Be star
50 Sgr50185182629955645.57−0.59556K1/K2III
18 Sgr1863169233902605.58−0.93653K0III
162 G. Sgr162180885949865.59−3.171842B4III
165 G. Sgr165181240950775.591.81186A6:m...
κ1 Sgrκ12921935711004695.601.23244A0V
74 G. Sgr74170433906875.630.86293K0III
131 G. Sgr131176704934985.630.99276K2III
51 Sgrh151204V5548184552964065.640.89290A1m...V5548 Sgr; δ Sct variable
κ2 Sgrκ22941938071005915.640.36370A3V
262 G. Sgr262189245984705.654.0568F7V
186 G. Sgr186182681956195.661.46225B8/B9V
209 G. Sgr209184835964965.660.00442K0III
33 Sgr33110174947927475.68−2.951734G8/K0II
63 Sgr63266189741986335.690.80309A1IV
189 G. Sgr189183007958235.701.91187Am
187 G. Sgr187182645955575.71−1.40862B7IV
21 G. Sgr21164402882985.72B0Iab...
184 G. Sgr184182477954855.72−1.01723K2III
12 G. Sgr12163652880385.740.49365G8III
10 G. Sgr10163318878365.762.25164A7III/IV
Y Sgr57Y168608899685.76−2.231294F8II
84 G. Sgr84171961914055.780.01465B8III
152 G. Sgr152179323944345.79−3.272117K2III
259 G. Sgr259189198985125.800.59359A8III
50 G. Sgr50167720896095.81−1.721045K2III
94 G. Sgr94173117919745.82−1.11793B8III
ρ2 Sgrρ245175181645951885.840.63359K0III
HD 17205186172051914385.855.2842G5V
296 G. Sgr2961942151007385.86−0.24541G8II/III
57 Sgr57238187739977835.880.98312K0III
9 Sgr924164794884695.89−5.014939O6Vf
V4089 Sgr201V4089184035962345.890.26435A5IV-IIIAlgol variable
HD 16983066169830904855.903.10118F8Vhas two planets
116 G. Sgr116175360929315.91−1.27891B6III
180 G. Sgr180182286954565.911.32270K3III
83 G. Sgr83171856913475.931.01314A5IV
138 G. Sgr138177517937635.93−1.20869B8IIIsp...
29 G. Sgr29165185886945.944.7457G3V
260 G. Sgr260189195984615.951.02316G8/K0III
16 Sgr1644167263894405.96B0.5Ib/II
132 G. Sgr132176884935375.96−2.331482K0II/III
218 G. Sgr218185467967605.970.45415K0III
25 G. Sgr25164870885505.980.79355K2III
13 G. Sgr13163685880125.99−2.061331B3II/III
141 G. Sgr141177817938556.00−1.19893B7V
264 G. Sgr264189561985756.011.10313K0III
RS Sgr47RS167647896376.03−1.13881B3/B4IV/V47 G. Sgr
179 G. Sgr179182180954086.03−2.001315B2Vnn
233 G. Sgr233187098975156.042.75149F3V
V4387 Sgr45V4387167356894706.05−4.353928Ap Siα² CVn variable
140 G. Sgr140177846939256.05−1.19916K3III
295 G. Sgr2951941841007646.080.91352K3III
121 G. Sgr121175794931346.090.46436K3III
163 G. Sgr163180928949296.090.09517K4III
148 G. Sgr148178555941446.110.71392K1III
197 G. Sgr197183545959656.11−1.781235A2V
232 G. Sgr232186984974236.112.13204A6:IIIm...
258 G. Sgr258189140984856.11−1.531101M0III
108 G. Sgr108174631926436.120.22493K1III
38 G. Sgr38166197890866.13B2II/III
178 G. Sgr178181925953966.13−0.12579M1/M2III
V4333 Sgr208V4333184705964406.131.80240F0Vδ Sct variable
62 G. Sgr62169236902906.140.39461K0III
123 G. Sgr123175892931406.141.67255A1V
224 G. Sgr224186042970676.14−0.95853B8IV/V
58 G. Sgr58168646900126.150.33475A3III
3 G. Sgr3161664870996.18−2.541811G3/G5Ib
63 Oph8162978877066.18O7/O8III
49 G. Sgr49167666896226.180.75397A5V
70 Sgr56V4028168574899806.19−1.571164M3IIIV4028 Sgr
71 G. Sgr71169990904946.19−0.01567B8III/IV
280 G. Sgr280191584995706.201.08344K2III
16 G. Sgr16164028881256.22−0.88858K0III
HD 16551630165516887606.22−4.354234O+...
26 Sgr2688172546916896.222.20208A3m...
V4200 Sgr242V4200188088979446.225.4646K3/K4VBY Draconis variable
297 G. Sgr2971944331008526.243.25129K1IV
128 G. Sgr128176537934236.25−2.101523K3III
V5652 Sgr157V5652179949946456.254.0988F8VGumala; has a planet
V4199 Sgr173V4199181558951596.25−0.34679B5III
6 Sgr618164358882586.27−2.501852K2III
206 G. Sgr206184574963656.271.14346K0III
254 G. Sgr254188981983516.272.18214K1III
69 G. Sgr69169938905106.281.69269A3/A4V
109 G. Sgr109174630926356.280.91386G8/K0III
V4198 Sgr142177863938876.28−0.45724B8V
150 G. Sgr150178840942726.280.34502B8/B9V
30 Sgr30105174309924806.291.91245F2IV
17 G. Sgr17164245882946.30−0.42721B7/B8II/III
64 G. Sgr64169398903366.30−1.05962B7III
143 G. Sgr143178075939936.30−0.27672B9.5V
282 G. Sgr282192433998786.30−1.431148K4III
V4434 Sgr283V4434192472999206.30−0.78851M4III
V3894 Sgr4V3894161756871636.31−1.401136B3Vn
68 G. Sgr68169851904786.311.87252A7V
90 G. Sgr90172875919016.311.11357K0III
129 G. Sgr129176593934186.310.14559K0III
263 G. Sgr263189388985796.311.64280A2/A3V
V3879 Sgr89V3879172816917816.32−1.551221M4III
39 G. Sgr39166393891146.331.09365A2V
167 G. Sgr167181401952116.331.36321K1III
53 Sgr53217185404967296.330.85406A0V
V4405 Sgr98V4405173425920796.34−0.43738M2/M3III
96 G. Sgr96173282920166.352.58185F5/F6V
127 G. Sgr127176246933156.35−0.62809K0III
48 G. Sgr48167665896206.364.0097F8V
80 G. Sgr80171416911726.36−1.201058K1III
125 G. Sgr125176123932346.37−0.66830G5/G6II
133 G. Sgr133176903935436.371.82265F5V
36 G. Sgr36165978890106.391.15365K0III
151 G. Sgr151179201943726.390.66457K0III
34 G. Sgr34165784888766.42−3.413019A2/A3Iab
269 G. Sgr269190009987856.442.64188F7V
115 G. Sgr115175390929726.45−0.30731K2III
103 G. Sgr103173928923016.46−0.48795A1V + K1III
290 G. Sgr2901933021003326.460.79444K3III
234 G. Sgr234187150974846.47−2.041638K5III
V505 Sgr240V505187949978496.471.14380A1V
244 G. Sgr244188158980126.47−1.461259K2/K3III
9 G. Sgr9163245877826.481.25363A1V
166 G. Sgr166181321951496.484.8868G1/G2V
196 G. Sgr196183577960956.483.37137F6V
V4190 Sgr79V4190171369911326.491.64304F0IV/Vδ Sct variable
25 Sgr25171237910666.53−3.453228F2II
65 Sgr65274190454989536.531.07402A0V
RY Sgr156RY180093947306.58−5.649056Cp156 G. Sgr
17 Sgr17167570895676.890.55605A7:
HD 187085187085975467.223.95147G0Vhas a planet
χ2 Sgrχ248182391954867.27−0.531185B7IVNamalsadirah IV
HD 181342181342951247.552.24377K0IIIhas a planet
HD 180902180902949517.782.48374K0III/IVhas a planet
HD 190647190647991157.784.11177G5Vhas a planet
HD 181720181720952627.864.12182G1Vhas a planet
HD 1691421691428.16473A7Vhas a planet
HD 171238171238910858.665.44144K0Vhas a planet
HD 165155165155886509.36212G8Vhas a planet
HD 1646041646048841410.047.14124K2Vhas a planet
Ross 1549240310.4413.089.68M3.5VV1216 Sgr; 9th nearest star; flare star
WASP-12311.1G5has a transiting planet
V4334V433411.6F2Ia C~Sakurai's Object
WASP-11012.31044G9has a transiting planet
WASP-6712.5734K0Vhas a transiting planet
OGLE-TR-1014.935000G or Khas a transiting planet
OGLE-TR-5616.565000Ghas a transiting planet
SWEEPS
J175853.92−291120.6
18.80~6500has a planet SWEEPS-04
OGLE-2005-BLG-169L19.48800M?has a planet
OGLE-2003-BLG-23519.717000Khas a planet
SWEEPS
J175902.67−291153.5
19.83~6500has a planet
MOA-2007-BLG-400L20000M3V?has a planet
SWEEPS
J175902.00-291323.7
26.23~6500has a possible shortest period planet
MOA-2007-BLG-192Lhas a planet
Pistol Star25000LBVhypergiant; member of the Quintuplet star cluster
WR 102ea26000Wolf–Rayet star; member of the Quintuplet star cluster
S2n/a26000orbits the supermassive black hole Sgr A*
KW SgrKW9000-
13000
M1.5 Iabhypergiant; one of the largest known stars. B magnitude = 11.