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Index of articles associated with the same name
designations F Puppis and f Puppis are distinct and refer to two different stars in the constellation Puppis: F Puppis (HD 57240) f Puppis (HD 61330) This
F_Puppis
Constellation in the southern celestial hemisphere
divisions in 1922. Puppis, along with Carina and Vela, was included in the list of modern IAU constellations in 1930. Multiple stars in Puppis have received
Puppis
Star in the constellation of Puppis
Zeta Puppis (ζ Puppis, abbreviated Zeta Pup, ζ Pup), formally named Naos /naʊs/, is the brightest star in the constellation of Puppis. The spectral class
Zeta_Puppis
Variable star in the constellation Puppis
RS Puppis (or RS Pup) is a Cepheid variable star around 6,000 ly away in the constellation of Puppis. It is one of the biggest and brightest known Cepheids
RS_Puppis
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
List_of_stars_in_Puppis
Star in the southern constellation of Puppis
Rho Puppis (ρ Puppis, abbreviated Rho Pup, ρ Pup), formally named Tureis /ˈtjʊəreɪs/, is a star in the southern constellation of Puppis. With an apparent
Rho_Puppis
Star in the constellation Puppis
Xi Puppis (ξ Puppis, abbreviated Xi Pup, ξ Pup) is a multiple star system in the southern constellation of Puppis. With an apparent visual magnitude of
Xi_Puppis
Second-brightest star in the constellation of Puppis
Pi Puppis, Latinized from π Puppis, also named Ahadi, is the second-brightest star in the southern constellation of Puppis. It has an apparent visual
Pi_Puppis
Index of articles associated with the same name
designations N Puppis and n Puppis are distinct and refer to three different stars in the constellation Puppis: N Puppis, (HD 65551, 228 G. Puppis), a B-type
N_Puppis
Star in the constellation Puppis
HD 61330 (f Puppis) is a binary star in the constellation Puppis. Its apparent magnitude is 4.53 and it is approximately 360 light years away based on
HD_61330
Star in the constellation Puppis
k Puppis (k Pup, k Puppis) is a Bayer designation given to an optical double star in the constellation Puppis, the two components being k1 Puppis and
K_Puppis
Index of articles associated with the same name
The Bayer designation υ Puppis (Upsilon Puppis) is shared by two stars in the constellation Puppis: υ1 Puppis (NV Puppis), a γ Cassiopeiae variable and
Upsilon_Puppis
F-type star
n Puppis A, is the primary star of the n Puppis system. It has an apparent magnitude of 5.83 and forms a binary star system with HD 60585, another F-type
HD_60584
Index of articles associated with the same name
2548, 38 G. Puppis) an F-type main-sequence star x Puppis, (HR 2518, HD 49591, 31 G. Puppis), a B-type main-sequence star Xi Puppis χ Puppis This set index
X_Puppis
Star in the constellation Puppis
L2 Puppis (also known as HD 56096) is a giant star in the constellation of Puppis and is located between the bright stars Canopus and Sirius. It is a semi-regular
L2_Puppis
Variable Star in the constellation Puppis
Omicron Puppis (ο Puppis) is candidate binary star system in the southern constellation of Puppis. It is visible to the naked eye, having a combined apparent
Omicron_Puppis
Type of chemically peculiar star
of ρ Puppis stars with relatively high luminosity and late spectral types. However, there is still sometimes confusion, for example with ρ Puppis stars
Am_star
Spectroscopic binary star system in the constellation Puppis
WR 9 is a spectroscopic binary in the constellation Puppis consisting of a Wolf-Rayet star and a class O star. It is around 12,000 light years away. WR
WR_9
Constellations recognized by the International Astronomical Union
modern list of 88 plus Argo (which was later split into Carina, Vela and Puppis). After this, Eugène Joseph Delporte drew boundaries for each of the 88
IAU_designated_constellations
Star in the constellation Puppis
11 Puppis is a single star in the southern constellation of Puppis, located approximately 522 light years away based on parallax. It has the Bayer designation
11_Puppis
F-type star
n Puppis B, is the secondary star of the n Puppis system. It has an apparent magnitude of 5.87 and is a binary star system with HD 60584, another F-type
HD_60585
Quadruple star system in the constellation Puppis
are hot main sequence stars. NO Puppis A has 3.58 times the mass (M☉) and 2.17 times the radius (R☉), while NO Puppis B has 1.68 times the mass and 1
HJ_4093
Probable nova seen in 1673
Nova Puppis 1673, also known as NSV 3846, is a probable nova in the constellation Puppis. It was discovered by French astronomer Jean Richer on January
Nova_Puppis_1673
Star in the constellation Puppis
Puppis (ν Puppis), also named Pipit, is a solitary, blue-hued star in the southern constellation of Puppis. It is the fifth-brightest star in Puppis,
Nu_Puppis
Variable star in the constellation Puppis
R Puppis is a variable star in the constellation Puppis. It is a rare yellow hypergiant and a candidate member of the open cluster NGC 2439. It is also
R_Puppis
Binary star system in the constellation Puppis
3 Puppis (3 Pup) is a spectroscopic binary in the constellation Puppis. It is a very rare A[e] supergiant, referred to as a B[e] star despite its spectral
3_Puppis
Nova seen in 1942
CP Puppis (or Nova Puppis 1942) was a bright nova occurring in the constellation Puppis in 1942. The nova was discovered on 9 November 1942 by Bernhard
CP_Puppis
Obsolete Southern constellation
constellation referred to as "Argûs in carina" (Carina, the keel), "Argûs in puppi" (Puppis, the poop deck or stern), and "Argûs in velis" (Vela, the sails). Lacaille
Argo_Navis
Hot Jupiter exoplanet orbiting WASP-121
increases) and the first that contains water. WASP-121b is in the constellation Puppis, and is about 858 light-years from Earth. In August 2022, this planet and
WASP-121b
Binary star system in the constellation Puppis
c Puppis, also known as HD 63032 and HR 3017, is a binary star in the constellation Puppis. Its apparent magnitude is of 3.61, making it the eight-brightest
HD_63032
Multi-spectrum pulsar in the constellation Vela
from either the pulsar or the Vela X nebula. A radio survey of the Vela-Puppis region was made with the Mills Cross Telescope in 1956–57 and identified
Vela_Pulsar
Open cluster in the constellation Puppis
Critter Cluster, is an open cluster in the modestly southern constellation Puppis, the imagined poop deck of the legendary Argo. It was discovered by Charles
Messier_93
Star in the constellation Puppis
is a star with two orbiting exoplanets in the southern constellation of Puppis. The designation HD 60532 takes its name from the Henry Draper Catalogue
HD_60532
Triple star in the constellation Puppis
KQ Puppis is a triple star system in the constellation of Puppis. With an apparent magnitude varying between 4.82 and 5.17, it is faintly visible to the
KQ_Puppis
Canadian-American physicist (1916–2012)
Retrieved October 7, 2014. "Interview with Robert F. Christy, Christy, Robert F. (1998) Interview with Robert F. Christy. [Oral History]". 1998. Christy 2013
Robert_F._Christy
Variable star in the constellation Puppis
V Puppis (V Pup) is a quadruple star system in the constellation Puppis. It has an apparent magnitude of 4.41, which is bright enough to be seen with
V_Puppis
F-type variable star
Impact Candidate), is a young F-type variable star located 11,000 light-years (3,400 pc) from Earth in the constellation of Puppis. It is believed to be surrounded
Gaia20ehk
Star in the constellation Puppis
also named Tislit, is an F-type main-sequence star about 1,162 light-years (356 parsecs) away in the constellation Puppis. With an apparent magnitude
WASP-161
Star in the constellation Puppis
χ Puppis, Latinised as Chi Puppis, is a single star in the southern constellation of Puppis. It has a white hue and is faintly visible to the eye at night
Chi_Puppis
Puppis by Gould, but it is now rarely used Also designated as v2 Puppis by Gould, but it is now rarely used The star originally designated o Puppis (Latin
Table of stars with Bayer designations
Table_of_stars_with_Bayer_designations
B-type star in the constellation Puppis
NW Puppis, also known as υ2 Puppis, is a star in the constellation Puppis. Located around 1,090 light-years away, it shines with a luminosity approximately
NW_Puppis
Open cluster in the constellation Puppis
also known as NGC 2478 is an open cluster in the southern constellation of Puppis. It was discovered by Giovanni Batista Hodierna before 1654 and re-discovered
Messier_47
Galaxy supercluster
were part of the same structure, the Centaurus–Puppis–PP Filament. This is because the Centaurus–Puppis–PP Filament goes under the ZOA of the Milky Way
Hydra–Centaurus_Supercluster
Star in the constellation Puppis
PT Puppis (PT Pup) is a star in the constellation Puppis. Anamarija Stankov confirmed this star as a Beta Cephei variable. Analysis of its spectrum and
PT_Puppis
Star in the constellation Puppis
QZ Puppis (QZ Pup, b Pup) is a class B2.5V (blue main-sequence) star in the constellation Puppis. Its apparent magnitude is 4.5 and it is approximately
QZ_Puppis
Star in the constellation Canis Major
Canis Majoris, η Canis Majoris, κ Canis Majoris, ο Puppis, π Puppis, χ Puppis, c Puppis and k Puppis. Consequently, δ Canis Majoris itself is known as
Delta_Canis_Majoris
Star in the constellation Puppis
NV Puppis (NV Pup), also known as υ1 Puppis, is a class B2V (blue main-sequence) star in the constellation Puppis. Its apparent magnitude is 4.67 and it
NV_Puppis
Star in the constellation Puppis
NS Puppis (NS Pup) is an irregular variable star in the constellation Puppis. Its apparent magnitude varies between 4.4 and 4.5. NS Puppis is a naked
NS_Puppis
is still restricted to the common main sequence spectral types: M, K, G, F, A, B and O. It may be later expanded to other types, such as S, D or C. This
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
F3V star in the constellation Puppis
QW Puppis (QW Pup) is a class F3V (yellow-white dwarf) star in the constellation Puppis. Its apparent magnitude is 4.49 and it is approximately 69.5 light
QW_Puppis
Bookkeeping survey of stars
ζ Puppis is one of the brightest of the visible blue supergiants. It is so bright that it appears to be a second magnitude star, even though ζ Puppis is
Star_count
Variable star in the constellation Vela
and Puppis. In the Coelum Australe Stelliferum itself, ο Velorum is labelled ο (omicron) Argus (du Navire in the French edition), while ο Puppis is labelled
Omicron_Velorum
Blue supergiant star in the constellation Canis Major
Majoris, HD 63032, HD 65456, Omicron Puppis, k Puppis, Epsilon Canis Majoris, Kappa Canis Majoris and Pi Puppis. Consequently, Eta Canis Majoris itself
Eta_Canis_Majoris
Star in the constellation Canis Major
Canis Majoris, η Canis Majoris, κ Canis Majoris, ο Puppis, π Puppis, χ Puppis, c Puppis and k Puppis. Consequently, ε Canis Majoris itself is known as
Epsilon_Canis_Majoris
White dwarf in the constellation Puppis
3847/1538-3881/aa76e0. Kawka, Adela; Vennes, Stéphane; Allard, Nicole F.; Leininger, T.; Gadéa, F. X. (2021-01-01). "The nearby magnetic cool DZ white dwarf PM
WD_0816−310
Star in the constellation Puppis
69142 is a class K1II-III (orange bright giant) star in the constellation Puppis. Its apparent magnitude is 4.44 and it is approximately 298 light years
HD_69142
Star in the constellation Puppis
V598 Puppis is the name given to a nova in the Milky Way Galaxy. USNO-A2.0 0450-03360039, a catalog number for the star, was discovered to be much brighter
V598_Puppis
Orange-hued giant star in the southern constellation of Puppis
Tau Puppis, Latinized from τ Puppis, is a star in the southern constellation of Puppis, near the southern constellation boundary with Carina. It is visible
Tau_Puppis
Binary star system in the constellation Puppis
Puppis was identified in 2008 as a young open cluster. Ten member stars were identified, including P Puppis itself and the naked-eye stars QS Puppis and
HD_63922
Type of variable star that pulsates radially
observation of the parallax distance to the closest Cepheids such as RS Puppis and Polaris. Cepheids change brightness due to the κ–mechanism, which occurs
Cepheid_variable
Star in the constellation Puppis
HD 61831 (d1 Puppis) is a class B2.5V (blue dwarf) star in the constellation Puppis. Its apparent magnitude is 4.84 and it is approximately 556 light years
HD_61831
Star in the constellation Puppis
MX Puppis (MX Pup) is a class B1.5IV (blue subgiant) star in the constellation Puppis. Its apparent magnitude varies irregularly between magnitude 4.6
MX_Puppis
Blue-giant star in the constellation Puppis
PU Puppis (PU Pup) is a class B8III (blue giant) star in the constellation Puppis. Its apparent magnitude is about 4.7 and it is approximately 620 light
PU_Puppis
Blazar in the constellation of Puppis
PKS 0727−11 is a blazar located in southern constellation of Puppis. The redshift of the object has been determined as (z) 1.591, with it first being discovered
PKS_0727−11
Constellation in the southern celestial hemisphere
are Gamma and Delta, Puppis has Zeta as its brightest star, and so on. Vela is bordered by Antlia and Pyxis to the north, Puppis to the northwest, Carina
Vela_(constellation)
Planetary nebula in the constellation Puppis
the hottest known white dwarf, about 400,000°F(200,000°C). The nebula is situated in the constellation Puppis. It was discovered by William Herschel on March
NGC_2440
Star in the constellation Canis Minor
Star Catalogue. When first catalogued it was in the Puppis constellation and was designated "13 Puppis", but it subsequently migrated to Canis Minor. Bode
HD_66141
Emission nebula in the constellation Vela
Carina to the south, and continues into Puppis, covering its entire southeastern part and ending near the star π Puppis. He published the discovery of the
Gum_Nebula
Open cluster in constellation Puppis
in the Milky Way galaxy. It is about 6,600 pc away in the constellation Puppis. Ruprecht 44 is a very young open cluster, only about several million years
Ruprecht_44
constellation of Argo Navis. After Argo Navis was broken up into Carina, Vela, and Puppis, these Greek-letter designations were kept, so that Carina does not have
List_of_stars_in_Carina
Star in the constellation Puppis
HD 64568 is a massive solitary star in the southern constellation of Puppis. With an apparent magnitude of 9.39, it is too faint to be seen by the naked
HD_64568
Binary system in Aquila
eclipse timing variation, Hipparcos and/Or Gaia astrometry: The cases of V Puppis and CY Ari". The Astrophysical Journal. 998 (1): 155. arXiv:2512.20087.
Gaia_BH3
Index. AAVSO. Retrieved 2023-11-26. Bonanos, A. Z.; Lennon, D. J.; Köhlinger, F.; Van Loon, J. Th.; Massa, D. L.; Sewilo, M.; Evans, C. J.; Panagia, N.; Babler
List_of_brightest_stars
constellation of Argo Navis. After Argo Navis was broken up into Carina, Vela, and Puppis, these Greek-letter designations were kept, so that Vela does not have a
List_of_stars_in_Vela
Red supergiant star in the constellation of Puppis
QY Puppis is a K-type supergiant star in the constellation of Puppis. With a radius of 515 R☉, it is on the smaller end of the largest known stars. A
QY_Puppis
Binary star system in the constellation Puppis
9 Puppis is a binary star system in the southern constellation of Puppis. It was originally designated 9 Argus, being part of the now defunct Argo Navis
9_Puppis
Star in the constellation Puppis
16 Puppis is a suspected astrometric binary star system in the southern constellation of Puppis, and is located in the northernmost part of its constellation
16_Puppis
Faint constellation on the celestial equator
the east. Other bordering constellations include Canis Minor, Lepus, and Puppis. Monoceros contains only a few fourth magnitude stars, making it difficult
Monoceros
Star in the constellation Puppis
171 G. Puppis (171 Pup) is a triple star system in the constellation of Puppis – the stern of Argo Navis – of apparent magnitude +5.38. Lacking a Bayer
171_G._Puppis
Binary star in the constellation Puppis
19 Puppis is a binary star system in the southern constellation of Puppis, near the northern border with Hydra and Monoceros. It is visible to the naked
19_Puppis
Series of lines in atomic spectra
1896 Edward C. Pickering found a new series of lines in the spectrum of ζ Puppis. This was believed to be the sharp series of hydrogen. In 1915 proof was
Sharp_series
Star system in the constellation Puppis
doi:10.1088/0004-6256/145/2/44. ISSN 0004-6256. van Capelleveen, Richelle F.; et al. (December 2025). "WIde Separation Planets In Time (WISPIT): Two directly
WISPIT_1
Molecular cloud complex in the constellations Vela and Puppis
Molecular Ridge is a molecular cloud complex in the constellations Vela and Puppis. Radio 12CO observations of the region showed the ridge to be composed of
Vela_Molecular_Ridge
Quadruple star system in the constellation Puppis
is a star system that lies 56 light-years away in the constellation of Puppis. The system consists of four stars in two binaries, making it one of the
HD 53680, HD 53705, and HD 53706
HD_53680,_HD_53705,_and_HD_53706
Brightest star in Earth's night sky
bow and arrow across the southern sky, formed by the constellations of Puppis and Canis Major. In this, the arrow tip is pointed at the wolf Sirius. A
Sirius
the star Gaia20ehk, about 11,000 light years away in the constellation Puppis. Erratic dimming and strong infrared emission are attributed to hot debris
2026_in_science
Multiple star system in the constellation Puppis
system that lies approximately 88 light-years away in the constellation of Puppis. The system consists of two bright stars where the primary is orbited by
HD_41742_and_HD_41700
Star-forming regions in the constellation Vela
regions are situated near the source Puppis A, an ancient supernova remnant visible at the border between Puppis and Vela, and the extensive association
Star-forming_regions_of_Vela
White dwarf star in the constellation Puppis
..7K. doi:10.1051/0004-6361/202142146. S2CID 237605138. Jiménez-Esteban, F. M.; Torres, S.; Rebassa-Mansergas, A.; Skorobogatov, G.; Solano, E.; Cantero
WD_0810−353
Ring of stars in the Milky Way galaxy
Scorpius, Lupus, southern Centaurus, Crux (the Southern Cross), Carina, Vela, Puppis, Canis Major, and Orion. Star-forming regions and OB associations that make
Gould_Belt
Galaxy in the constellation Puppis
NGC 2525 is a barred spiral galaxy located in the constellation Puppis. It is located at a distance of about 70 million light years from Earth, which,
NGC_2525
Star in the constellation Puppis
20 Puppis is a solitary star in the southern constellation of Puppis. It is visible to the naked eye as a faint, yellow-hued star with an apparent visual
20_Puppis
Constellation in the southern celestial hemisphere
aiming towards Orion, while the southern stars of Canis Major and a part of Puppis were viewed as a bow, named BAN in the Three Stars Each tablets, dating
Canis_Major
Binary star system in the constellation Puppis
HD 49798 is a binary star in the constellation Puppis about 521 ± 14 parsecs (1,699 ± 46 ly) from Earth. It has an apparent magnitude of 8.3, making it
HD_49798
Main sequence star
located 1,850 light years (567.2 parsecs) from Earth in the constellation of Puppis. In 2021 the All-Sky Automated Survey for Supernovae reported that this
ASASSN-21qj
Open cluster in the constellation Puppis
very distant group beyond Puppis OB2, while another, nearer group with later-type stars lies at a similar distance as Puppis OB1. The region is dominated
NGC_2467
Carter & brothers. p. 93. Mackworth, P. H.; Commander van Balkom; Everitt, P. F.; Sadler, D. H.; Squadron-Leader May; Bennett, D. C. T.; Hinks, A. R.; Black
List_of_proper_names_of_stars
Star in the constellation Puppis
located approximately 858 light-years (263 parsecs) away in the constellation Puppis. WASP-121 has a mass and radius similar to the Sun's. It hosts one known
WASP-121
Chemical element with atomic number 2 (He)
observations of previously unknown lines in the spectrum of the star ζ Puppis (these are now known to occur with Wolf–Rayet and other hot stars). Pickering
Helium
Star in the constellation Puppis
known as the Moth) is a young star located in the southern constellation Puppis. It has an apparent magnitude of 8.22, making it readily visible in binoculars
HD_61005
travel, tourism, insurance
F PUPPIS
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