AI & ChatGPT searches , social queries for 3 PUPPIS
Search references for 3 PUPPIS. Phrases containing 3 PUPPIS
See searches and references containing 3 PUPPIS!
Search references for 3 PUPPIS. Phrases containing 3 PUPPIS
See searches and references containing 3 PUPPIS!3 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
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
Index of articles associated with the same name
designation L Puppis is shared by two stars in the constellation Puppis: L1 Puppis (OU Puppis), a chemically peculiar α² CVn variable L2 Puppis (HD 56096)
L_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
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
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
Supernova remnant
the supernova remnant Puppis A (X-rays from ROSAT in purple, optical data in pink) (28 November 2007) Puppis A: X-ray [blue:0.3-8 keV] + IR [red-green:
Puppis_A
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
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
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
NGC 2438 1786 2.9 (approx.) 11.5 Puppis NGC 2440 1790 3.6 (approx.) 9.3 Puppis Spirograph Nebula IC 418 1888–1894 1.3 (approx.) 9.6 Lepus IC 1295 1867
List_of_planetary_nebulae
S2CID 50867264. Separation: 3.1, left column of page 3; Orbital period and epoch of periastron: Table 3, right column of page 3. Bach, K.; Lee, J.; Demarque
List_of_smallest_known_stars
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
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
The Astronomical Journal. 137 (3): 3558–3573. arXiv:0811.3037. Bibcode:2009AJ....137.3558S. doi:10.1088/0004-6256/137/3/3558. ISSN 0004-6256. S2CID 19019913
List_of_supernova_candidates
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 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
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
According to traditional Chinese uranography, the modern constellation Puppis is located within the southern quadrant of the sky, which is symbolized as
Puppis_in_Chinese_astronomy
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
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
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
solar neighbourhood", Monthly Notices of the Royal Astronomical Society, 403 (3): 1089–1101, arXiv:0911.3426, Bibcode:2010MNRAS.403.1089P, doi:10.1111/j.1365-2966
List of star systems within 70–75 light-years
List_of_star_systems_within_70–75_light-years
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
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
Quadruple star system in the constellation Puppis
star. NO Puppis A lies in the instability strip of slowly pulsating B-type stars and is likely of this variable star class, while NO Puppis B lies in
HJ_4093
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
Star in the constellation Carina
classified as a variable star and the cause of the variations is unclear. 3 Puppis HD 37974 HD 268835 Roman, Nancy G. (1987). "Identification of a constellation
CPD−57°2874
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
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
Italian physicist
Giampetro Puppi (20 November 1917 – 25 December 2006) was an Italian physicist who is known for his contribution to the theory of weak interactions. Puppi was
Giampietro_Puppi
Former 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
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
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
Sigma Puppis, Latinized from σ Puppis, is a binary star system in the southern constellation Puppis. It has an apparent visual magnitude of 3.25, which
Sigma_Puppis
Star fragment in the constellation Puppis
supernova explosion. It could be a possible quark star. Puppis A (also known as SNR 260.4−3.4) Media related to RX J0822-4300 at Wikimedia Commons "Cosmic
RX_J0822−4300
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
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
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
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
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
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
2423 is an open cluster in Puppis. It was discovered on March 19, 1786 by William Herschel. It contains 50-60 stars. NGC 2423-3 is a red giant star contained
NGC_2423
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
Star-forming region in the Puppis constellation
commonly referred to as God's Hand, is a star-forming region located in the Puppis constellation, about 1,300 light-years (400 pc) from Earth. It is one of
CG_4
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
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
Daughter of Heinrich Himmler (1929–2018)
ISBN 978-0-19-932375-3. Gunkel, Christoph; Leffers, Jochen (29 June 2018). "Himmlers Tochter "Püppi" - Nazi bis zuletzt" [Himmler's Daughter "Püppi" - Nazi to the
Gudrun_Burwitz
Open cluster in Puppis
Collinder 135, known sometimes as the Pi Puppis Cluster, is an open cluster in Puppis constellation. It consists of six stars brighter than 6th magnitude
Collinder_135
G-type star in the constellation Puppis
HD 69830 (285 G. Puppis) is a yellow dwarf star located 41.0 light-years (12.6 parsecs) away in the constellation of Puppis. In 2005, the Spitzer Space
HD_69830
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)
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
cluster. Ten member stars were identified, including P Puppis itself and the naked-eye stars QS Puppis and HD 63578. The cluster is part of the Vela OB2 association
HD_63922
Star in the constellation Puppis
NGC 2423-3 is a red giant star approximately 3,040 light-years away in the constellation of Puppis. The star is part of the NGC 2423 open cluster (hence
NGC_2423-3
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 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
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
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
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
F-type star
HD 60585, also known as HR 2910 or 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
HD_60585
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
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
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
Constellations recognized by the International Astronomical Union
Louis de Lacaille divided this into three separate constellations: Carina, Puppis, and Vela. The 88 constellations depict 42 animals, 29 inanimate objects
IAU_designated_constellations
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
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
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
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
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
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
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
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
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
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
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
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
Topics referred to by the same term
ubiquitin-like protein Puppis, abbreviated "Pup", a constellation Sirius B, a white dwarf star affectionately known as "the Pup" pup, ISO 639-3 code for the Pulabu
Pup
Carved finial or decorative motif on church furniture
poppy flower. It is derived, by way of Old French, from the Latin word puppis, which means the poop or the figurehead of a ship. In its simplest, and
Poppyhead_(carving)
Meteor shower associated with the comet 26P/Grigg-Skjellerup
get their name because their radiant appears to lie in the constellation Puppis, at around right ascension 112 degrees and declination −45 degrees. This
Pi_Puppids
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
Messier 46 Open 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″
List of NGC objects (2001–3000)
List_of_NGC_objects_(2001–3000)
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
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
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
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
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
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
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
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
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
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
Open cluster in the constellation Puppis
is an open cluster of stars in the slightly southern constellation of Puppis. It was discovered by Charles Messier in 1771. Dreyer described it as "very
Messier_46
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
Isolated radio pulsar in the constellation Puppis
PSR J0628−28) is an isolated radio pulsar located in the constellation of Puppis, 4,729 light-years (1.450 parsecs) from Earth. First identified through
PSR_B0628−28
Star in the constellation Puppis
HD 53811 is a class A4IV (white subgiant) star in the constellation Puppis. Its apparent magnitude is 4.92 and it is approximately 198 light years away
HD_53811
Star in the constellation Puppis
known as the Moth) is a young star located in the southern constellation Puppis, the poop deck. It has an apparent magnitude of 8.22, making it readily
HD_61005
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
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)
3 PUPPIS
3 PUPPIS
3 PUPPIS
3 PUPPIS
3 PUPPIS
3 PUPPIS
3 PUPPIS
3 PUPPIS
3 PUPPIS