Astronomy:HD 32963

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Short description: G-type star with a Jupiter-like exoplanet
HD 32963
Observation data
Equinox J2000.0]] (ICRS)
Constellation Taurus[1]
Right ascension  05h 07m 55.76408s[2]
Declination +26° 19′ 40.6750″[2]
Apparent magnitude (V) 7.60[3]
Characteristics
Spectral type G3V[4] or G5IV[5]
B−V color index 0.6[3]
Astrometry
Radial velocity (Rv)−62.49±0.12[2] km/s
Proper motion (μ) RA: −69.896[2] mas/yr
Dec.: −66.118[2] mas/yr
Parallax (π)26.1310 ± 0.0238[2] mas
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 a G-type main sequence star located 124 light years away from Earth[8] in the constellation of Taurus. It has a mass of 0.94 solar masses. It is 4.99 billion years old.[9] It has one exoplanet orbiting it which was discovered using radial velocity. The exoplanet that has been named HD 32963 b is a Jupiter analogue due to its similar characteristics to the planet Jupiter such as orbit and size.[3]

Planetary system

It has one currently discovered exoplanet 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 a minimum mass of 0.7 Jupiter masses; in 2023 its inclination was measured by astrometry, 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)
Mass Semimajor axis
(AU)
Orbital period
(years)
Eccentricity Inclination Radius
b 2.07+0.83
−0.64
 MJ
3.409+0.063
−0.064
6.483+0.064
−0.061
0.099±0.028 19.3+9.2
−5.7
or 160.7+5.7
−9.2
°
—

References

  1. ↑ 1.0 1.1 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A  XHIP record for this object at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 3.7 Rowan, Dominick; Meschiari, Stefano; Laughlin, Gregory; Vogt, Steven S.; Butler, R. Paul; Burt, Jennifer; Wang, Songhu; Holden, Brad et al. (Jan 2016). "The Lick-Carnegie Exoplanet Survey: HD 32963—A New Jupiter Analog Orbiting a Sun-like Star" (in en). The Astrophysical Journal 817 (2): 104. doi:10.3847/0004-637X/817/2/104. ISSN 0004-637X. Bibcode: 2016ApJ...817..104R. 
  4. ↑ Grenier, S. et al. (June 1999). "Radial velocities. Measurements of 2800 B2-F5 stars for HIPPARCOS". Astronomy and Astrophysics Supplement 137: 451-456. doi:10.1051/aas:1999489. Bibcode: 1999A&AS..137..451G. 
  5. ↑ 5.0 5.1 5.2 5.3 Xiao, Guang-Yao et al. (May 2023). "The Masses of a Sample of Radial-velocity Exoplanets with Astrometric Measurements". Research in Astronomy and Astrophysics 23 (5): 055022. doi:10.1088/1674-4527/accb7e. Bibcode: 2023RAA....23e5022X. 
  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. doi:10.1051/0004-6361/202141339. Bibcode: 2021A&A...654A.137L. 
  7. ↑ "HD 32963". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+32963. 
  8. ↑ "HD 32963 b - NASA Science" (in en-US). 2019-04-22. https://science.nasa.gov/exoplanet-catalog/hd-32963-b/. 
  9. ↑ 9.0 9.1 Martin, Pierre-Yves (2021). "Planet HD 32963 b" (in en). https://exoplanet.eu/catalog/hd_32963_b--2494/.