HD 76151

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Template:Short description

HD 76151
Location of HD 76151 (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Hydra[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 6.00[3]
Characteristics
Evolutionary stage Main sequence[2]
Spectral type G2V[4]
U−B color index +0.22[5]
B−V color index +0.67[5]
R−I color index +0.21[5]
Astrometry
Radial velocity (Rv)31.99±0.12[2] km/s
Proper motion (μ) RA: −413.648 mas/yr[2]
Dec.: 30.619 mas/yr[2]
Parallax (π)59.3595±0.0408 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)+4.81[1]
Details[4]
Mass1.053+0.056
−0.068
 M
Radius1.125+0.035
−0.011
 R
Surface gravity (log g)4.35±0.18 cgs
Temperature5,790±170 K
Metallicity [Fe/H]0.24±0.09 dex
Rotation15 days[6]
Rotational velocity (v sin i)3[7] km/s
Age5.5+2.5
−2.1
 Gyr
Other designations
Template:Odlist[3]
Database references
SIMBADdata

HD 76151 is a high proper motion, G-type main-sequence star and solar analog[4] in the constellation of Hydra 54.95 light-years from Earth.[2] It has an apparent visual magnitude of approximately 6.00, which means it is faintly visible to the naked eye under good viewing conditions.[3] An infrared excess has been detected around this star, most likely indicating the presence of a circumstellar disk at a radius of 7.9 AU. The temperature of this dust is 99 K.[8]

HD 76151 has an age of roughly 5.5 billion years old, with estimates ranging from 3.4 to 9.6 billion years. The stellar atmosphere has an effective temperature of around 5,790 K (5,520 °C; 9,960 °F). The radius of HD 76151 is 1.125 solar radii (783,000 km) based on spectroscopic observations, though Gaia DR3 estimates a radius of 0.977 solar radii (680,000 km). It is slightly metal-rich and is a member of the thin disk population.[4]

References

  1. ^ a b Template:Cite XHIP
  2. ^ a b c d e f g Template:Cite Gaia DR3
  3. ^ a b c Page Module:Citation/CS1/styles.css has no content."HD 76151". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved January 20, 2011. {{cite web}}: Invalid |mode=Script error: No such module "Citation mode". (help)
  4. ^ a b c d Page Module:Citation/CS1/styles.css has no content.Senturk, S.; et al. (October 2024). "Near-Infrared Spectroscopy of the Sun and Solar Analog Star HD 76151: Compiling an Extensive Line List in Y-, J-, H-, and K-Bands". The Astrophysical Journal. 976 (2). id. 175. arXiv:2410.08270. Bibcode:2024ApJ...976..175S. doi:10.3847/1538-4357/ad85e4.
  5. ^ a b c HR 3538, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50. Accessed on line January 20, 2011.
  6. ^ Page Module:Citation/CS1/styles.css has no content.Maldonado, J.; et al. (October 2010), "A spectroscopy study of nearby late-type stars, possible members of stellar kinematic groups", Astronomy and Astrophysics, 521: A12, arXiv:1007.1132, Bibcode:2010A&A...521A..12M, doi:10.1051/0004-6361/201014948, S2CID 119209183
  7. ^ HD 76151, database entry, The Geneva-Copenhagen Survey of Solar neighbourhood, J. Holmberg et al., 2007, CDS ID V/117A. Accessed on line January 20, 2011.
  8. ^ Page Module:Citation/CS1/styles.css has no content.Eiroa, C.; et al. (July 2013). "DUst around NEarby Stars. The survey observational results". Astronomy & Astrophysics. 555: A11. arXiv:1305.0155. Bibcode:2013A&A...555A..11E. doi:10.1051/0004-6361/201321050. S2CID 377244.

Template:Stars of Hydra