HD 9986

HD 9986
Observation data
Epoch J2000      Equinox J2000
Constellation Pisces[1]
Right ascension 01h 37m 40.87904s[2]
Declination +12° 04′ 42.1703″[2]
Apparent magnitude (V) 6.77[1]
Characteristics
Evolutionary stage main sequence[2]
Spectral type G2 V[3]
B−V color index 0.648±0.008[1]
Astrometry
Radial velocity (Rv)−20.97±0.13[2] km/s
Proper motion (μ) RA: +120.372[2] mas/yr
Dec.: +6.15[2] mas/yr
Parallax (π)39.3118±0.0303 mas[2]
Distance82.97 ± 0.06 ly
(25.44 ± 0.02 pc)
Absolute magnitude (MV)4.73[1]
Details
Mass0.95[2] M☉
Radius1.1[2] R☉
Luminosity1.1[2] L☉
Surface gravity (log g)4.43±0.01[4] cgs
Temperature5,831±5[4] K
Metallicity [Fe/H]+0.095±0.005[4] dex
Rotation23[5] days
Rotational velocity (v sin i)1.90±0.15[4] km/s
Age3.29±0.51[4] Gyr
Other designations
BD+11°207, HD 9986, HIP 7585, SAO 92543[6]
Database references
SIMBADdata

HD 9986 is a Sun-like star in the equatorial constellation of Pisces. With an apparent visual magnitude of 6.77,[1] it lies below the normal limit for visibility with the naked eye. The star is located at a distance of 83 light years from the Sun as determined from parallax measurements, but it is drifting closer with a radial velocity of −21 km/s.[2]

This object is a G-type main-sequence star with a stellar classification of G2 V,[3] and is a near solar twin with physical properties very similar to the Sun's. It is around 3.3[4] billion years old and is spinning slowly with a rotation period of about 23 days. A speckle survey of G-dwarfs by Elliott P. Horch in 2002 noted that HD 9986 may be a non-single star.[7]

References

  1. ^ a b c d e Anderson, 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 at VizieR.
  2. ^ a b c d e f g h i j k Vallenari, 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 at VizieR.
  3. ^ a b Gray, R. O.; Corbally, C. J.; Garrison, R. F.; McFadden, M. T.; Robinson, P. E. (2003). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I.". The Astronomical Journal. 126 (4): 2048. arXiv:astro-ph/0308182. Bibcode:2003AJ....126.2048G. doi:10.1086/378365.
  4. ^ a b c d e f dos Santos, Leonardo A.; et al. (August 2016). "The Solar Twin Planet Search. IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars". Astronomy & Astrophysics. 592: 8. arXiv:1606.06214. Bibcode:2016A&A...592A.156D. doi:10.1051/0004-6361/201628558. S2CID 53533614. A156.
  5. ^ See, V.; Jardine, M.; Vidotto, A. A.; Donati, J. -F.; Boro Saikia, S.; Fares, R.; Folsom, C. P.; Jeffers, S. V.; Marsden, S. C.; Morin, J.; Petit, P.; BCool Collaboration (February 2018). "The open flux evolution of a solar-mass star on the main sequence". Monthly Notices of the Royal Astronomical Society. 474 (1): 536–546. arXiv:1711.03904. Bibcode:2018MNRAS.474..536S. doi:10.1093/mnras/stx2599.
  6. ^ "HD 9986". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved July 13, 2016.
  7. ^ Gray, R. O.; et al. (October 2003). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I". The Astronomical Journal. 126 (4): 2048–2059. arXiv:astro-ph/0308182. Bibcode:2003AJ....126.2048G. doi:10.1086/378365. S2CID 119417105.

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