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. Bibcode2012AstL...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. Bibcode2016ApJ...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. Bibcode1999A&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. Bibcode2023RAA....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. Bibcode2021A&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/.