List of stars in Puppis


This is the list of notable stars in the constellation Puppis, sorted by decreasing brightness.
This constellation's Bayer designations were given while it was still considered part of the constellation of Argo Navis. After Argo Navis was broken up into Carina, Vela, and Puppis, these Greek-letter designations were kept, so that Puppis does not have a full complement of Greek-letter designations. For example, since Argo Navis's alpha star went to Carina, there is no Alpha Puppis.
NameBFG.VarHDHIPRADecvis.
mag.
abs.
mag.
Dist. Sp. classNotes
ζ24866811394292.21−5.951399O5IafNaos, Suhail Hadar, Muliphein;
π8256855352642.71−4.921094K3IbAhadi
ρ1525367523397572.831.4163F2mF5IIpTureis;
τ3950310327682.94−0.80183K0III...
ν2047670316853.17−2.39423B8III SBPipit
σ9959717363773.25−0.51184K5III SB
ξ719163700381703.34−4.741347G6IaAzmidi, Asmidiske, Azmidiske
c17563032378193.62−4.521387K4III
a21364440384143.71−1.41345G5III...
l315762623376773.94−5.302280A2Iab
P19963922381644.10−4.801964B0III
j1122265228388354.20−1.74502F7/F8II
J21864760385184.22−4.651940B0.5Ib
ο18363462380704.40−5.002470B1IV:nne
1625667797399064.40−1.41472B5V
L27356096349225.100.50198M5e
h227969142403264.42−0.47310K1II/III
h1267NS68553400914.44−4.361874K4IIIIrregular variable
q28970060407064.442.1693A4m...
10860532367954.462.4184F6Vhas two
233V65818389574.47−3.291164B1Vp + B2 eclipsing variable
I71QW55892348344.492.8669F0IV
b214QZ64503384554.49−1.98640B2V
k113361555372294.50−1.92454B6Vcomponent of the k Puppis system
f12761330370964.53−0.67358B8IV/V
23265810390954.610.29238A1V
k2134615564.62−1.81462B5IVcomponent of the k Puppis system
115562576376484.63−2.75976K5III
21664740385004.63−2.09720B1.5Vp
υ183NV57150353634.65−2.42847B2V+...
10059890365144.65−4.001753G2Ib...
p11960863369174.650.46225B8V
m128PU61429371734.69−1.45551B8IV
Q19663744380894.690.48227K0III
1926368290400844.720.95185K0III
26868601400964.73−6.044657A7Ib
7856456350204.75−0.43354B8/B9V
χ22565456389014.76−3.471442A7III
r274MX68980402744.78−2.61979B2neγ Cas variable
107KQ60414367734.82−5.253361M2Iab+B0Ve
A6754893344954.83−1.98751B3IV/V
w29470555409454.83−2.22838K2/K3III
d114361831372974.84−1.39574B3V
9759612364314.85−5.133228A6Ib/II
L172OU56022348994.871.14181Ap
H6153811340594.921.07192A4IV
4751799333574.94−2.621062M1III
14061772373794.98−1.60676K3III
3750235328554.99−2.23906K2/K3III
2026968752402594.99−2.891230G5Ib/II
21264379384235.013.7359F3/F5V
8056779352265.03−2.31959B3V
416762952378915.030.73236F2V
15962644376065.043.1379G5IVOriginally called T Pup by Lacaille
V/Y2147973317655.05−0.58436G8IIICalled V by Lacaille, Y in later catalogues, not V or Y Pup the variables
n11160584368175.772.7495F6V
t4952092335585.07−1.77760B4IV/V
18563465380105.07−2.831240B2IV/V
N22865551388725.08−2.901283B2.5IV
1223065699390235.09−1.82786G8II
276OS69081403215.09−2.701177B2V:γ Cas variable
υ284NW57219354065.11−1.93836A0V
6855526346705.120.21313K2III
W16262713376645.121.02215K1IIINot W Puppis the
X3850223327655.143.1382F5.5VNot X Pup the
O23165685389175.140.32300K2III
920564096383825.164.0554G2VHR 3064, Gl 291
619063697382115.170.72253K3III
29570556409435.18−3.311630B2IV-V+...
C5953704340815.200.27315Am
18763578380205.22−3.331672B1V
23465925390615.221.41189F3V
F8757240353935.24−0.55469A0V
250MZ66888394875.25−4.032345M2IIProbably irregular variable
x3149591325375.270.24331B8/B9V
1646273309535.281.71169F2V
E7055719348025.30−0.32434A3p...
18863660381465.310.35365G1.5IIIFe-0.5
30271176412605.32−0.64506K4/K5III
25267456397345.33−2.541221A3Ib/II
17163077378535.364.4550G0V
22765460388465.36−2.321120B2.5V
y9859635363635.41−0.75556B3V
15062226374505.41−0.98617B3V
z115OW60606367785.42−2.541273B2Vneγ Cas variable
21564572384975.44−1.39756K1IIICN...
30971459413235.45−1.53813B3V
518063336380485.483.0899F5+...
21764802385935.48−1.47801B2V
246V33666624393605.52−0.35486Ap Siα2 CVn variable
30871377413955.520.95268K1/K2III
1826268146400355.533.7773F7V
9359256362585.55−1.03674B9Vsp...
6053705340655.564.5153G3V...
29270442409445.58−0.12450A3V
28770002406785.590.08413K2III
15662578376235.60−0.72598B5V
19763852382005.61−1.02691M0III
161V39062747377515.62−3.161863B2II
20464152383755.621.00274K0III
8156813351815.64−0.99692K4III
10560341367325.640.88292K0III
15462412375905.640.59333K1III
122V37860855369815.66−2.871655B2/3VBe star
25767880399435.66−1.59921B4V
30171141412425.67−0.76631A1III/IV
y3142MY61715371745.68−5.265015F4Iab, Y in Lacaille
125PT61068370365.69−2.891698B2IIβ Cep variable
y213061391370435.69−0.23497B9VY in Lacaille
1020664238384275.69−2.111185F2IV/V
29370523409905.710.99286K0III
77PR56455350295.720.14425A0pα2 CVn variable
d214461878373225.73−0.64612B5V
G1545572305915.76−0.82675B9V
d314561899373295.76−1.911116B3III
27869123403445.771.56227K1III
9659550363625.78−1.951144B2IV
11660666368485.780.87313K1III
e13861641372235.78−1.58964B3III
D PupD6654475343395.80−1.26842B3V
16462781377105.802.61142F0IV
7956733352025.81−0.78679B4V
200QS63949381595.82−3.031918B1.5IVβ Cep variable
24466598393805.83−0.18518K2/K3III
10660345367215.840.98306A3III
M8557197353475.86−0.54621B8II/III
n112605855.87
176V39263215379155.87−0.57632B5VBe star
29870761410745.88F2Iab
17462893377525.89−0.46608B8V
20864225382675.891.39259K2III
9159026361435.90−1.47973B4V
17863271379955.90−1.51988B1/B2V
24166358392515.90−0.41595A3IV
14161774373645.92−0.80720K0III
241742287905.933.7787F6VA component of the quadruple HD 41742/41700
4050445329385.942.23180A3V
69V36355718348175.94−1.27903B4V
195V39763786381675.940.11478B9V
7656410350545.95−0.19552B4III/IV
59499363455.95−0.31582B3V+...
28569830406935.955.4541K0Vhas three -mass,
30571267413285.960.91333A3m...
307V43871302412505.97−3.923105B3VAlgol variable
9259136362365.98−1.18881B5III
23565904390145.98−1.611076B4V
d4146V46861925373455.99−2.101353B4IIIBe star
23966210391226.010.70377A2V
30371196412826.013.36111F2/F3V
17763118378236.02−1.15886B6IV
22365211387326.02−1.08856B6V
9459438363956.053.39111F5V
210QU64365383706.05−2.611762B2IVβ Cep variable
216662864378436.060.85359A6/A7
27569080403416.07−2.351575B2V
31271487413616.07−0.30613B9IV/V
6354153342536.09−0.44660G0III
22665442388456.09−0.58703K3III
11360646368076.111.39287A9IV
19463822382466.11−2.691874K1III
27769082403246.11−2.181482B2IV/V
1424766834395246.12−2.301575B3III
29170302408766.12−0.58712G8/K0III
240PY66255391536.13−2.201509A0pα2 CVn variable
2229670673410676.130.63411K0III
90V36858634359606.14−0.50694A8Vδ Sct variable
T Pup189T63640380746.14−0.19600M2IIIClassed as not variable
22064876386356.14−0.45678K4III
6253952342006.152.42182F2V
25167243396176.15−3.943396G1Ib
28269511404856.15−2.671895K2III
29770612409476.152.01219A4V
2348383320076.16−1.401058B4V
14962082374656.16−0.95860M0/M1III
30V33949336324346.19−2.051449B3VneBe star
13761642372026.200.79393G8III
60325367366.21−2.121509B2II
22965598388796.21−1.241009B5V
26067977399206.210.82389G8III
28169445404766.221.07349G6:III+...
4851825334516.233.05141F5V
5152362335906.230.66424A0V
18663655381846.23−2.571874B8/B9II
4551266331396.242.59175K0/K1III
742448291296.26−0.55751B8II
59235362646.26−0.28664K4III
4651682333946.27−0.21644K2III
110V37660559367286.27−0.30672B8IV β Lyr variable
26468242399746.27−1.12979B+...
942834293046.28−0.26663A0V
2648543320916.281.48298A+...
221PX65183387926.28−1.591221M5/M6IIIIrregular variable
24966812394206.28−0.61780G8II
300V43670946411076.28−1.881399M2III
2748797322086.300.17549A8:+...
8657299354636.31−0.45734K2/K3III
63291379396.310.00597K3III
QY63302380316.31−2.912280K3Iab/b
24266435392996.31−0.70823M3III
44NP51208331896.32−1.791364C3IIIrregular variable
8958420358936.32−0.33697B5V
20163948381836.321.30329K0III
2128469665406046.32−0.78858A1V
182OX63401379826.33−0.28685Ap Siα2 CVn variable
12661227370896.34−9.1440750F0Ib
63696382066.34−0.96939K5III
20964287383556.34−2.091583B2IV-V
141700287646.354.2287F7.5VA component of the quadruple HD 41742/41700
10460312366576.35−0.43739B8V
23666005390356.35−1.631283B2IV-V
66885395146.35−0.66823K5/M0III
258PQ67888398666.36−2.321772B3Vγ Cas variable
820364077383726.372.00244F3IV
23766006390386.37−0.68838B2IV-V
25567751398766.37−1.871449A3III
13161453371286.380.18566K4III
17963323380376.38−2.952397K5II/III
69002402916.381.07377K2III
5452703337746.390.85418G8II/III
17063112379516.39−0.96962B9III
60951369866.40−0.23691K1II
13561589372896.40−0.15667K3III
27268862402206.400.22561A3V
15362318374616.41−1.311140B7IV/V
4150621329186.42−0.22695K2/K3III
16062712376666.420.17580B8IV
26568450400636.42−2.962451B0III
69904406396.42−4.184289M0III + A3/5
61750373756.430.34538K2
20264042383166.430.48505B9.5V
28669879406566.430.65466K0III
5753253339096.440.95408A0V
29070235407876.44−0.55815B8Ib/II
30471231413066.44−0.21698K1III
20764181382926.450.27561G6III
64974386866.45−1.541294K4III
63399379966.460.87428K1III
65638389256.460.24573K0III
4350860330156.470.90424B8V
54179341776.47−0.44787K3III
442168289886.481.19372K1III
842683291856.482.58196F8V
V42067698398346.491299B3III/IVBe star
19363734382096.490.96417K2III
13961672372936.50−0.50819B6V
67408397306.500.05637K1III
148R62058374156.56G2Ia-0
262863378427.031.57402A0/A1V
70642409527.184.8994G6Vhas a planet
50499329707.22154GIVhas a planet and unconfirmed planet
55696348017.9235G0Vhas a planet
48265318958.073.36285G5IV/VNosaxa, has a planet
9.450.032500individual star of, has a planet
385949.758M0has two planets
10.4881F6Vhas a
11.0G4has a transiting planet
11.0F9Vhas a transiting planet
11.1F6Tislit; has a transiting planet
12.7K1Vhas a transiting planet