Orange-hued giant star in the southern constellation of Puppis
Tau Puppis
Location of τ Puppis (circled)
Observation data Epoch J2000 Equinox J2000
Constellation
Puppis
Right ascension
06h 49m 56.16846s[1]
Declination
−50° 36′ 52.4437″[1]
Apparent magnitude (V)
+2.95[2]
Characteristics
Spectral type
K1 III[3]
U−B color index
+1.195[2]
B−V color index
+1.20[2]
Astrometry
Radial velocity (Rv)
+36.4[4] km/s
Proper motion (μ)
RA: +34.36[1] mas/yr Dec.: −69.11[1] mas/yr
Parallax (π)
18.7577 ± 0.3475 mas[5]
Distance
174 ± 3 ly (53.3 ± 1.0 pc)
Absolute magnitude (MV)
−0.80[6]
Orbit[7][8]
Period (P)
1,066.0±4.0 d
Semi-major axis (a)
7.15±0.25 mas
Eccentricity (e)
0.088±0.045
Inclination (i)
80.20 ± 6.10°
Longitude of the node (Ω)
2.90 ± 6.20°
Periastron epoch (T)
2,420,992.8±94.5 HJD
Argument of periastron (ω) (secondary)
64.00°
Details
Mass
3.19[9]M☉
Radius
27[10]R☉
Temperature
4,489±33[9] K
Rotational velocity (v sin i)
2.2[11] km/s
Age
540[9] Myr
Other designations
Tau Pup, τ Pup, CPD−50° 1070, FK5 263, HD 50310, HIP 32768, HR 2553, SAO 234735, PPM 335509[12]
Database references
SIMBAD
data
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 to the naked with an apparent visual magnitude of +2.95[2] and is located at a distance of about 182 light-years (56 parsecs) from Earth.[1] The variable radial velocity of this system was detected by H. D. Curtis and H. K. Palmer in 1908, based on observations made at the D. O. Mills Observatory.[8] It is a spectroscopic binary star system, with the presence of the secondary component being revealed by the shifts of absorption lines in the spectrum resulting from the Doppler effect. The two components orbit each other with a period of 1,066.0 days (2.9 years) and a low eccentricity of 0.090.[7]
The primary component of this system has a stellar classification of K1 III.[3] A luminosity class 'III' indicates this has expanded into a giant star after exhausting the supply of hydrogen at its core and evolving away from the main sequence of stars like the Sun. The interferometry-measured angular diameter of this star, after correcting for limb darkening, is 4.49 ± 0.07 mas,[13] which, at its estimated distance, equates to a physical radius of about 27 times the radius of the Sun.[10] It appears to be rotating slowly, with a projected rotational velocity of 2.2 km s−1.[11] This gives a lower bound on the azimuthal velocity of rotation along the star's equator. Tau Puppis is radiating energy from its outer envelope at an effective temperature of around 4,500 K,[14] giving it the orange hue of a cool, K-type star.[15]
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^Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
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TauPuppis, Latinized from τ Puppis, is a star in the southern constellation of Puppis, near the southern constellation boundary with Carina. It is visible...
Binary star system 2.80 Pi Puppis Star Maximum brightness 2.81 2.68 Rho Puppis Star 2.81 Beta Draconis Binary star system 2.81 Tau Scorpii Star 2.81 Lambda...
and the metallic lines of an F5 star. It is an evolved Am star of the ρ Puppis type, a class of evolved stars showing the Am chemical peculiarities. It...
Wiktionary, the free dictionary. Markab may refer to: Alpha Pegasi Tau Pegasi k Puppis, erroneously Kappa Velorum Markab (horse), a Thoroughbred racehorse...
Khereb) and Markab (often spelled Markeb), a name shared with Alpha Pegasi, k Puppis and Kappa Velorum. In 2016, the IAU organized a Working Group on Star Names...
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...
Carina, Puppis and Vela. That was still insufficient for the number of stars, so he also used uppercase Latin letters such as N Velorum and Q Puppis. Lacaille...
Louis de Lacaille divided this into three separate constellations: Carina, Puppis, and Vela. The 88 constellations depict 42 animals, 29 inanimate objects...
Nova on a Very Massive White Dwarf: A Revised Light-Curve Model of V445 Puppis (2000)". The Astrophysical Journal. 684 (2): 1366–1373. arXiv:0805.2540...
ISBN 0939923785 The star originally designated o Puppis (Latin lower case 'o') is now generally called Omicron Puppis. Lacaille's Beta Telescopii (β Tel, β Telescopii)...
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...
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...
Sancti Regis Davidis XXXVII Canis Minor Lamb of God Agni Paschalis XXXVIII Puppis, Carina, Vela, Pyxis (Argo Navis) Noah's Ark Archæ Patriarchæ Noachi XXXIX...
R. W. (2000). "The distribution of bright OB stars in the Canis Major-Puppis-Vela region of the Milky Way". Monthly Notices of the Royal Astronomical...
65 NGC 2362 Tau Canis Majoris Cluster Open cluster Canis Major 3.8 Mel 66 - Open cluster Puppis 7.8 Mel 67 NGC 2421 Open cluster Puppis 9.0 Mel 68 NGC...
Cluster Open cluster Canis Major 7.2 Cr 135 - Pi Puppis Cluster Open cluster Puppis 2.1 Cr 136 NGC 2362 Tau Canis Majoris Cluster Open cluster Canis Major...