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HD 12139

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Star in the constellation Aries
HD 12139
Observation data
Epoch J2000      Equinox J2000
Constellation Aries
Right ascension 01 59 35.68394
Declination 21° 03′ 30.8472″
Apparent magnitude (V) 5.89
Characteristics
Spectral type K0III-IV
B−V color index 1.031±0.015
Astrometry
Radial velocity (Rv)−1.65±0.20 km/s
Proper motion (μ) RA: +141.014 mas/yr
Dec.: -14.643 mas/yr
Parallax (π)9.3049 ± 0.0967 mas
Distance351 ± 4 ly
(107 ± 1 pc)
Absolute magnitude (MV)0.50
Details
Mass1.69±0.48 M
Radius11.12+0.34
−0.13 R
Luminosity58.2±0.7 L
Surface gravity (log g)2.50±0.11 cgs
Temperature4,780+120
−70 K
Metallicity −0.02±0.05 dex
Age2.0+1.0
−0.6 Gyr
Other designations
BD+20°322, HD 12139, HIP 9307, HR 577, SAO 75077, WDS J01596+2100D
Database references
SIMBADdata

HD 12139 is an orange-hued star in the northern zodiac constellation of Aries. With an apparent visual magnitude of 5.89, it is a dim star that is just visible to the naked eye under good viewing conditions. It is located approximately 351 light-years (107.5 pc) distant from the Sun, based on parallax, but is drifting closer with a radial velocity of −2 km/s. With high probability, it is considered a member of the Hercules stream.

This object is an aging red giant with a stellar classification of K0III-IV, meaning that it has used up its core hydrogen and is expanding. At present it has 11 times the girth of the Sun. The star is about two billion years old with 1.7 times the mass of the Sun. It is radiating 58 times the luminosity of the Sun from its photosphere at an effective temperature of 4,780 K.

A magnitude 9.36 companion is located at an angular separation of 199.70 from the primary along a position angle of 9°, as of 2015. It is unclear if the two are physically associated.

References

  1. ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ 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. S2CID 119257644.
  3. ^ Yoss, Kenneth M. (November 1961). "Spectral and Luminosity Classifications and Measurements of the Strength of Cyanogen Absorption for Late-Type Stars from Objective-Prism Spectra". Astrophysical Journal. 134: 809. Bibcode:1961ApJ...134..809Y. doi:10.1086/147209.
  4. ^ Feuillet, Diane K.; et al. (2016). "Determining Ages of APOGEE Giants with Known Distances". The Astrophysical Journal. 817 (1): 40. arXiv:1511.04088. Bibcode:2016ApJ...817...40F. doi:10.3847/0004-637X/817/1/40. S2CID 118675933.
  5. "HD 12139". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-11-13.
  6. Ramya, P.; et al. (August 2016). "Chemical compositions and kinematics of the Hercules stream". Monthly Notices of the Royal Astronomical Society. 460 (2): 1356−1370. arXiv:1604.04821. Bibcode:2016MNRAS.460.1356R. doi:10.1093/mnras/stw852.
  7. Takeda, Yoichi; Tajitsu, Akito (2014). "Spectroscopic study on the beryllium abundances of red giant stars". Publications of the Astronomical Society of Japan. 66 (5): 91. arXiv:1406.7066. Bibcode:2014PASJ...66...91T. doi:10.1093/pasj/psu066.
  8. Mason, B. D.; et al. (2014). "The Washington Visual Double Star Catalog". The Astronomical Journal. 122 (6): 3466. Bibcode:2001AJ....122.3466M. doi:10.1086/323920.
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