HD 22663

HD 22663
Location of HD 22663 (circled in red)
Observation dataEpoch J2000      Equinox J2000
ConstellationEridanus[1]
Right ascension03h 37m 05.67804s[2]
Declination−40° 16′ 28.7772″[2]
Apparent magnitude (V)4.57[1]
Characteristics
Evolutionary stagered giant branch[2]
Spectral typeK1 III[3]
B−V color index1.023±0.028[1]
Astrometry
Radial velocity (Rv)+11.50±0.02[4] km/s
Proper motion (μ)RA: −13.532[2]mas/yrDec.: −9.929[2]mas/yr
Parallax (π)13.2285±0.3968 mas[2]
Distance247 ± 7 ly (76 ± 2 pc)
Absolute magnitude (MV)+0.32[1]
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 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.[1] Based upon an annual parallax shift of 13.2 mas,[2] it is located around 247 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.[1]

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 95 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,660 K.[4]

References

  1. ^ abcdefAnderson, 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. ^ abcdefgVallenari, 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. ^ 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. Retrieved 2018-07-20.
  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.