Star in the constellation Eridanus
HD 22663 (y Eridani ) is a candidate astrometric binary [ 6] star system in the equatorial constellation of Eridanus . It is visible to the naked eye with an apparent visual magnitude of 4.57.[ 2] Based upon an annual parallax shift of 14.2 mas ,[ 1] it is located around 230 light years from the Sun . It is moving further away from the Earth with a heliocentric radial 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-hued giant star with a stellar classification of K1 III,[ 3] having exhausted the hydrogen at its core and evolved away from the main sequence . It has an estimated 1.4 times the mass of the Sun and has expanded to 13 times the Sun's radius . At the age of 2.6 billion years, this star is radiating 96 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,660 K.[ 4]
References
^ a b c d 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 .
^ 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 , S2CID 119257644 .
^ a b Houk, 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 .
^ a b c d Jofré, 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 .
^ "HD 22663" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2018-07-20 .
^ 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 .