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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
Constellation in the southern celestial hemisphere
Wikimedia Commons has media related to Puppis. The Deep Photographic Guide to the Constellations: Puppis Star Tales – Puppis Portals: Astronomy Stars Outer space
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
Supernova remnant
(21 August 2014) Puppis A: X-ray [blue:high]/[green:medium]/[red:low] (10 September 2014) "Puppis A". WISE Multimedia Gallery. NASA. 9 December 2011. Retrieved
Puppis_A
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 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
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
Nova in the constellation Puppis
V445 Puppis was a nova in the constellation Puppis. It was discovered by Kazuyoshi Kanatsu of Matsue, Shimane, Japan, who recorded a peak magnitude of
V445_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
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
Pre-main sequence Star, database entry, SIMBAD. Accessed on line February 9, 2011. Barnes, J. R.; Kiraga, M.; Diaz, M.; Berdiñas, Z.; Jenkins, J. S.;
List of star systems within 50–55 light-years
List_of_star_systems_within_50–55_light-years
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
Italian runner
Francesco Puppi (born 26 January 1992) is an Italian male trail runner and ultra runner, world champion at 2017 World Long Distance Mountain Running Championships
Francesco_Puppi
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
Catalogue of astronomical objects
Cluster – Puppis 8.3 M47 NGC 2422 Open Cluster 1.6 Puppis 4.4 – NGC 2423 Open Cluster – Puppis 6.7 – NGC 2438 Planetary Nebula 2.9 Puppis 10 – NGC
Herschel_400_Catalogue
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
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
Triple star system
star system in the Puppis constellation. It has the Bayer designation of y1 Puppis, though it is usually just referred to as y Puppis. It has an apparent
HD_59635
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
Gemini 33.78 ± 0.09 1.14 K0 III 288 171 G. Puppis Puppis 49.6 ± 0.4 5.38 + 16.7 F9 V 291 9 Puppis Puppis 53.8 ± 0.5 5.16 G0V (G1 + G9) 293 Volans 26
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
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
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
Protoplanetary nebula in the constellation of Puppis
located some 4,200 light-years (1,300 pc) from Earth in the constellation Puppis. The name "Calabash Nebula" was first proposed in 1989 in an early paper
Calabash_Nebula
Star in the constellation Puppis
1 Puppis is a single star in the southern constellation of Puppis. It lies in the northern part of the constellation at a distance of about 790 ly, east
1_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
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
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
Molecular cloud
Puppis. The nebula contains the infrared cluster [DBS2003] 9. It is located beyond the Carina Arm. Sh 2-308 is ionized by the star cluster Bochum 9.
Sh_2-309
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
Star in the constellation Puppis
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 eye, but can
HD_64568
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
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
Star in the constellation Puppis
a star with an exoplanetary companion in the southern constellation of Puppis. It has an apparent visual magnitude of +7.17, which is too dim to be readily
HD_70642
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
Star in the constellation Puppis
HD 50499 is a star in the constellation of constellation of Puppis. With an apparent visual magnitude of 7.21, this star is too faint to be in naked eye
HD_50499
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
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
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
Constellation in the southern celestial hemisphere
ship Argo) until it was divided into three pieces, the other two being Puppis (the poop deck), and Vela (the sails of the ship). Carina was once a part
Carina_(constellation)
Supernova remnant in the constellation Vela
Vela supernova remnant overlaps the Puppis A supernova remnant, which is four times more distant. Both the Puppis and Vela remnants are among the largest
Vela_supernova_remnant
Relatively young and nearby supernova remnant
the centerpoint the neutron star CXOU J085201.4-461753 and a third SNR Puppis A could be seen top right as a white cloud. Event type Supernova remnant
RX_J0852.0−4622
Binary star in the constellation Puppis
system with a magnetically active component in the southern constellation of Puppis. It has the variable star designation V414 Pup; HD 66051 is its identifier
HD_66051
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
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
Star in the constellation Puppis
HD 64740 is a single star in the southern constellation Puppis, positioned near the line of sight to the Gum Nebula. It has a blue-white hue and is faintly
HD_64740
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
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
Globular cluster in the constellation Puppis
NGC 2298 is a globular cluster in the southern constellation of Puppis. Discovered by James Dunlop on May 30, 1826, it is probably a former member of the
NGC_2298
Molecular cloud
Sh 2-307 is a nebula in Puppis. It contains the potential infrared cluster [DBS2003] 8. It is located in the Perseus Arm. Although appearing small visuallly
Sh_2-307
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
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)
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
OU Puppis (OU Pup) is a chemically peculiar class A0 (white main-sequence) star in the constellation Puppis. Its apparent magnitude is about 4.9 and it
OU_Puppis
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
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
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
Star in the constellation Puppis
HD 48265, also named Nosaxa, is a star in the southern constellation Puppis. It has an apparent visual magnitude of 8.07, which makes it too faint to be
HD_48265
Star in the constellation Puppis with a brown dwarf companion
known as HR 3048, is a G-type dwarf star, located in the constellation Puppis some 164 light-years away. It is orbited by a brown dwarf companion. The
HD_63754
cluster Puppis 07h 42m −14° 49′ 6.3 2438 Planetary nebula Puppis 07h 41m 51.4s −14° 43′ 55″ 10.8 2439 Open cluster Puppis 07h 40m 45.0s 31° 41′ 36″ 6.9 2440
List of NGC objects (2001–3000)
List_of_NGC_objects_(2001–3000)
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
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
Extrasolar planet in the constellation Puppis
planet located approximately 84 light-years away in the constellation of Puppis, orbiting the star HD 60532. This planet has a true mass of 7.46 times more
HD_60532_c
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
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
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
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
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
Galaxy containing the Solar System
Norma, Triangulum Australe, Circinus, Centaurus, Musca, Crux, Carina, Vela, Puppis, Canis Major, Monoceros, Orion and Gemini, Taurus, to the galactic anticenter
Milky_Way
American multinational aerospace and defense conglomerate
based on Charles Smith's earlier astronomical research of the star Zeta Puppis. The electron tube was christened with the name Raytheon ("light of/from
RTX_Corporation
Galaxy in the constellation Puppis
NGC 2566 is a barred spiral galaxy in the constellation of Puppis. Its velocity with respect to the cosmic microwave background is 1898 ± 19 km/s, which
NGC_2566
Wife of Heinrich Himmler
Heinrich Himmler was close to his first daughter, Gudrun, whom he nicknamed Püppi ("dolly"); he phoned her every few days and visited as often as he could
Margarete_Himmler
Star in the constellation Puppis
HD 44594 is a star in the southern constellation Puppis. It has an apparent visual magnitude of 6.64, so it can be seen with the naked eye from the southern
HD_44594
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
Star in the constellation Puppis
HD 59612 is a class A5Ib supergiant star in the constellation Puppis. Its apparent magnitude is 4.86 and it is approximately 4,300 light years away based
HD_59612
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
F-type star
HD 60584, also known as HR 2909 or 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
HD_60584
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
Very young offspring of humans
Infancy. 7 (1): 53–71. doi:10.1207/s15327078in0701_5. PMID 33430544. "Püppi, muttu AA machen?". Gehirn&GeistSerie Kindesentwicklung No. 1. February
Infant
Island in the Mediterranean, region of Italy
2016. UNESCO Culture Sector. "El teatro de marionetas siciliano Opera dei Puppi". Archived from the original on 28 August 2010. Retrieved 22 August 2010
Sicily
Planetary nebula in the constellation Puppis
about 400,000°F(200,000°C). The nebula is situated in the constellation Puppis. It was discovered by William Herschel on March 4, 1790. He described it
NGC_2440
U.S. defense contractor
based on Charles Smith's earlier astronomical research of the star Zeta Puppis. The electron tube was named Raytheon (a compound of Old French and Greek
Raytheon
Ophiuchus Orion Pavo Pegasus Perseus Phoenix Pictor Pisces Piscis Austrinus Puppis Pyxis Reticulum Sagitta Sagittarius Scorpius Sculptor Scutum Serpens Sextans
Lists_of_stars
Star in the constellation Puppis
HD 57197, also known as M Puppis or HR 2789, is a suspected astrometric binary located in the southern constellation Puppis, the poop deck. It has an
HD_57197
Pacific typhoon in 2024
in March 2026, the name was replaced with Tomo, which means stern deck (Puppis) in Japanese. The name Yagi (Japanese: ヤギ, [ja̠ɡʲi]) refers to the constellation
Typhoon_Yagi
Constellation in the southern celestial hemisphere
Argonauts. Parts of Argo Navis were the Carina (the keel or hull), the Puppis (the stern), and the Vela (the sails). These eventually became their own
Pyxis
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
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
Designated common star constellations
Delphinus, Equuleus, Eridanus, Piscis Austrinus, Carina, Puppis, Vela, Pyxis, and Columba. Carina, Puppis, and Vela historically formed part of the former constellation
Constellation_family
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
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
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
Non-periodic comet
discovered as a 15th-magnitude object in the southern constellation of Puppis. It is the fifth comet discovered by Terry Lovejoy. By December 2014, the
C/2014_Q2_(Lovejoy)
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
the Constellations. Cambridge University Press. p. 170. ISBN 0-521-44921-9. Kaler, James B. "Saiph (Kappa Orionis)". Stars. University of Illinois. Archived
List_of_proper_names_of_stars
Star in the constellation Puppis
HD 70555 (w Puppis) is a class K2.5II-III (orange giant) star in the constellation Puppis. Its apparent magnitude is 4.83 and it is approximately 1,010
HD_70555
Star in the constellation Puppis
HD 54893, often called A Puppis is a suspected variable star in the constellation Puppis. Its apparent magnitude is 4.83 and is approximately 860 light
HD_54893
Poetic meter consisting of six feet
by poetic ones, for example unda or lympha for water, aequora for sea, puppis for ship, amnis for river, and so on. Some ordinary Latin words are avoided
Dactylic_hexameter
Northern 70 2.24 Schedar α Cassiopeiae 0230 K0 IIIa Northern 71 2.25 Naos ζ Puppis 1,080 O4 If(n)p Southern 72 2.26 Almach γ Andromedae 0350 K3 IIb, B9.5 V
List_of_brightest_stars
White dwarf in the constellation Puppis
v t e Constellation of Puppis List of stars in Puppis Puppis in Chinese astronomy Stars Bayer ζ (Naos) ν (Pipit) ξ (Azmidi) ο π ρ (Tureis) σ τ υ1 υ2 χ
WD_0816−310
9 PUPPIS
9 PUPPIS
9 PUPPIS
9 PUPPIS
9 PUPPIS
9 PUPPIS
9 PUPPIS
9 PUPPIS
9 PUPPIS