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HD 22663

From Wikipedia, the free encyclopedia
Star in the constellation Eridanus
HD 22663
Observation data
Epoch J2000      Equinox J2000
ConstellationEridanus
Right ascension03h 37m 05.67915s[1]
Declination−40° 16′ 28,7408″[1]
Apparent magnitude (V)4.57[2]
Characteristics
Spectral typeK1 III[3]
B−Vcolor index1.023±0.028[2]
Astrometry
Radial velocity (Rv)+11.50±0.02[4] km/s
Proper motion (μ)RA: −13.342mas/yr
Dec.: −12.219mas/yr
Parallax (π)14.1588±0.3283 mas[1]
Distance230 ± 5 ly
(71 ± 2 pc)
Absolute magnitude (MV)+0.32[2]
Details[4]
Mass1.43±0.25 M
Radius13.01±0.54 R
Luminosity95.5+16.7
−14.2
 L
Surface gravity (log g)2.75±0.01 cgs
Temperature4,660±21 K
Metallicity [Fe/H]−0.15±0.05 dex
Rotational velocity (v sin i)1.40±0.55 km/s
Age2.58±1.22 Gyr
Other designations
y Eri,CD−40° 1008,FK5 130,HD 22663,HIP 16870,HR 1106,SAO 216405[5]
Database references
SIMBADdata

HD 22663 (y Eridani) is a candidateastrometric binary[6]star system in the equatorialconstellation ofEridanus. It is visible to the naked eye with anapparent visual magnitude of 4.57.[2] Based upon an annualparallax shift of14.2 mas,[1] it is located around 230 light years from theSun. It is moving further away from the Earth with a heliocentricradial velocity of +11.5 km/s,[4] having come within 140.9 ly some 3.76 million years ago.[2]

The visible component is an orange-huedgiant star with astellar classification of K1 III,[3] having exhausted the hydrogen at its core andevolved away from themain sequence. It has an estimated 1.4 times themass of the Sun and has expanded to 13 times theSun's radius. At the age of 2.6 billion years, this star is radiating 96 times theSun's luminosity from its enlargedphotosphere at aneffective temperature of 4,660 K.[4]

References

[edit]
  1. ^abcdBrown, 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.
  2. ^abcdeAnderson, 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. ^abHouk, Nancy (1978),Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 2, Ann Arbor: Dept. of Astronomy, University of Michigan,Bibcode:1978mcts.book.....H.
  4. ^abcdJofré, E.; Petrucci, R.; Saffe, C.; Saker, L.; de la Villarmois, E. Artur; Chavero, C.; Gómez, M.; Mauas, P. J. D. (2015), "Stellar parameters and chemical abundances of 223 evolved stars with and without planets",Astronomy & Astrophysics,574: A50,arXiv:1410.6422,Bibcode:2015A&A...574A..50J,doi:10.1051/0004-6361/201424474,S2CID 53666931.
  5. ^"HD 22663".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2018-07-20.
  6. ^Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems",Monthly Notices of the Royal Astronomical Society,389 (2): 869,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
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