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HD 32963

From Wikipedia, the free encyclopedia
G-type star with a Jupiter-like exoplanet
HD 32963
Observation data
EpochJ2000      EquinoxJ2000
ConstellationTaurus[1]
Right ascension05h 07m 55.76408s[2]
Declination+26° 19′ 40.6750″[2]
Apparent magnitude (V)7.60[3]
Characteristics
Spectral typeG3V[4] or G5IV[5]
B−Vcolor index0.6[3]
Astrometry
Radial velocity (Rv)−62.49±0.12[2] km/s
Proper motion (μ)RA: −69.896mas/yr[2]
Dec.: −66.118mas/yr[2]
Parallax (π)26.1310±0.0238 mas[2]
Distance124.8 ± 0.1 ly
(38.27 ± 0.03 pc)
Absolute magnitude (MV)+4.80[1]
Details
Mass1.03±0.05[5] M
Radius1.1[2] R
Luminosity1.1[2] L
Surface gravity (log g)4.41±0.03[3] cgs
Temperature5,727±32[3] K
Metallicity[Fe/H]0.11±0.05[3] dex
Rotational velocity (v sin i)1.10[6] km/s
Age4.99+6.71
−3.55
[3] Gyr
Other designations
BD+26 789,HD 32963,HIP 23884,SAO 76970,PPM 94086[7]
Database references
SIMBADdata
Exoplanet Archivedata

HD 32963 is aG-type main sequencestar located 124 light years away fromEarth[8] in theconstellation ofTaurus. It has a mass of 0.94 solar masses. It is 4.99 billion years old.[9] It has oneexoplanet orbiting it which was discovered usingradial velocity. The exoplanet that has been named HD 32963 b is aJupiter analogue due to its similar characteristics to the planetJupiter such as orbit and size.[3]

Planetary system

[edit]

It has one currently discoveredexoplanet orbiting it named HD 32963 b. The planet orbits the star at a distance of 3.41 AU with an eccentricity of 0.07. It takes 2372 days to orbit the parent star. Its has aminimum mass of 0.7 Jupiter masses; in 2023 its inclination was measured byastrometry, showing it to have a true mass about twice that of Jupiter.[5] The orbit and size of HD 32963 b is similar to the planet Jupiter. This makes it a Jupiter analogue planet.[9][3]

The HD 32963 planetary system[5]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(years)
EccentricityInclinationRadius
b2.07+0.83
−0.64
 MJ
3.409+0.063
−0.064
6.483+0.064
−0.061
0.099±0.02819.3+9.2
−5.7
or160.7+5.7
−9.2
°

References

[edit]
  1. ^abAnderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5): 331.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015. XHIP record for this object atVizieR.
  2. ^abcdefgVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  3. ^abcdefghRowan, Dominick; Meschiari, Stefano; Laughlin, Gregory; Vogt, Steven S.; Butler, R. Paul; Burt, Jennifer; Wang, Songhu; Holden, Brad; Hanson, Russell; Arriagada, Pamela; Keiser, Sandy; Teske, Johanna; Diaz, Matias (Jan 2016)."The Lick-Carnegie Exoplanet Survey: HD 32963—A New Jupiter Analog Orbiting a Sun-like Star".The Astrophysical Journal.817 (2): 104.arXiv:1512.00417.Bibcode:2016ApJ...817..104R.doi:10.3847/0004-637X/817/2/104.ISSN 0004-637X.
  4. ^Grenier, S.; Baylac, M.-O.; et al. (June 1999). "Radial velocities. Measurements of 2800 B2-F5 stars for HIPPARCOS".Astronomy and Astrophysics Supplement.137:451–456.Bibcode:1999A&AS..137..451G.doi:10.1051/aas:1999489.
  5. ^abcdXiao, Guang-Yao; Liu, Yu-Juan; et al. (May 2023). "The Masses of a Sample of Radial-velocity Exoplanets with Astrometric Measurements".Research in Astronomy and Astrophysics.23 (5): 055022.arXiv:2303.12409.Bibcode:2023RAA....23e5022X.doi:10.1088/1674-4527/accb7e.
  6. ^Llorente De Andrés, F.; Chavero, C.; de la Reza, R.; Roca-Fàbrega, S.; Cifuentes, C. (2021). "The evolution of lithium in FGK dwarf stars. The lithium-rotation connection and the Li desert".Astronomy and Astrophysics.654.arXiv:2108.05852.Bibcode:2021A&A...654A.137L.doi:10.1051/0004-6361/202141339.
  7. ^"HD 32963".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved22 May 2025.
  8. ^"HD 32963 b - NASA Science".science.nasa.gov. 2019-04-22. Retrieved2025-05-21.
  9. ^abMartin, Pierre-Yves (2021)."Planet HD 32963 b".exoplanet.eu. Retrieved2025-05-21.
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