HD 91190
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Draco |
| Right ascension | 10h 35m 05.49379s[1] |
| Declination | +75° 42′ 46.4541″[1] |
| Apparent magnitude (V) | 4.86[2] |
| Characteristics | |
| Spectral type | G8 III-IIIb[3] |
| B−V color index | 0.957±0.003[2] |
| Astrometry | |
| Radial velocity (Rv) | +16.6[4] km/s |
| Proper motion (μ) | RA: −0.599[1] mas/yr Dec.: −17.436[1] mas/yr |
| Parallax (π) | 4.5045 ± 0.1730 mas [1] |
| Distance | 720 ± 30 ly (222 ± 9 pc) |
| Absolute magnitude (MV) | +0.46[2] |
| Details | |
| Mass | 2.39[4] M☉ |
| Luminosity | 69[4] L☉ |
| Surface gravity (log g) | 2.59[5] cgs |
| Temperature | 4,965±106[4] K |
| Metallicity [Fe/H] | −0.03[5] dex |
| Age | 2.06[4] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 91190 is a suspected astrometric binary [7] star system in the northern circumpolar constellation of Draco. It is faintly visible to the naked eye, having an apparent visual magnitude of 4.86.[2] The distance to HD 91190, as estimated from its annual parallax shift of 4.5 mas ,[1] is around 720 light years. This system is moving further away from the Sun with a heliocentric radial velocity of +17 km/s,[4] having come to within 170 ly some 2.4 million years ago.[2]
At the age of about two billion years,[4] this is an evolved G-type giant star with a stellar classification of G8 III-IIIb.[3] It has 2.39[4] times the mass of the Sun and is radiating 69[4] times the Sun's luminosity from its photosphere at an effective temperature of around 4,965 K.[4]
References
[edit ]- ^ a b c d e f 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 Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series, 71: 245, Bibcode:1989ApJS...71..245K, doi:10.1086/191373.
- ^ a b c d e f g h i j Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", Astronomical Journal, 150 (3): 88, arXiv:1507.01466 , Bibcode:2015AJ....150...88L, doi:10.1088/0004-6256/150/3/88, S2CID 118505114, 88.
- ^ a b Liu, Y. J.; et al. (April 2014), "The Lithium Abundances of a Large Sample of Red Giants", The Astrophysical Journal, 785 (2): 12, arXiv:1404.1687 , Bibcode:2014ApJ...785...94L, doi:10.1088/0004-637X/785/2/94, S2CID 119226316, 94.
- ^ "HD 91190". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2018年07月17日.
- ^ 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.