Astronomy:HD 91190
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| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Draco[1] |
| Right ascension | 10h 35m 05.49034s[2] |
| Declination | +75° 42′ 46.4467″[2] |
| Apparent magnitude (V) | 4.86[1] |
| Characteristics | |
| Evolutionary stage | red giant branch[2] |
| Spectral type | G8 III-IIIb[3] |
| B−V color index | 0.957±0.003[1] |
| Astrometry | |
| Radial velocity (Rv) | +16.6[4] km/s |
| Proper motion (μ) | RA: −20.218[2] mas/yr Dec.: +1.482[2] mas/yr |
| Parallax (π) | 13.0453 ± 0.1053[2] mas |
| Distance | 250 ± 2 ly (76.7 ± 0.6 pc) |
| Absolute magnitude (MV) | +0.46[1] |
| 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.[1] The distance to HD 91190, as estimated from its annual parallax shift of 13.0 mas,[2] is around 250 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.[1]
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
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A. XHIP record for this object at VizieR.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940 Gaia DR3 record for this source at VizieR.
- ↑ 3.0 3.1 Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series 71: 245, doi:10.1086/191373, Bibcode: 1989ApJS...71..245K.
- ↑ 4.00 4.01 4.02 4.03 4.04 4.05 4.06 4.07 4.08 4.09 Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", Astronomical Journal 150 (3): 88, doi:10.1088/0004-6256/150/3/88, 88, Bibcode: 2015AJ....150...88L.
- ↑ 5.0 5.1 Liu, Y. J. et al. (April 2014), "The Lithium Abundances of a Large Sample of Red Giants", The Astrophysical Journal 785 (2): 12, doi:10.1088/0004-637X/785/2/94, 94, Bibcode: 2014ApJ...785...94L.
- ↑ "HD 91190". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+91190.
- ↑ 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, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode: 2008MNRAS.389..869E.
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