60 Andromedae
| |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Andromeda |
Right ascension | 02h 13m 13.32387s[1] |
Declination | +44° 13′ 53.9546″[1] |
Apparent magnitude (V) | +4.82[2] |
Characteristics | |
Spectral type | K3.5 III Ba0.4[3] |
U−B color index | +1.74[2] |
B−V color index | +1.48[2] |
Astrometry | |
Radial velocity (Rv) | –46.3[4] km/s |
Proper motion (μ) | RA: –20.90[1] mas/yr Dec.: –14.46[1] mas/yr |
Parallax (π) | 6.15 ± 0.63[1] mas |
Distance | approx. 530 ly (approx. 160 pc) |
Orbit[5] | |
Period (P) | ±0.4 748.2 days |
Semi-major axis (a) | ±2.6" 3.0 |
Eccentricity (e) | ±0.03 0.34 |
Inclination (i) | ±15 127° |
Longitude of the node (Ω) | ±17 6° |
Periastron epoch (T) | 886±11 37 HJD |
Argument of periastron (ω) (secondary) | ±6 358° |
Details | |
60 And A | |
Mass | +0.7 −0.3 2.0[5] M☉ |
Surface gravity (log g) | ±0.44 1.70[6] cgs |
Temperature | ±42 4054[6] K |
Metallicity [Fe/H] | ±0.12 −0.13[6] dex |
60 And B | |
Mass | ±0.1 0.5[5] M☉ |
Other designations | |
60 Andromedae (abbreviated 60 And) is a star system in the northern constellation of Andromeda, located to the west-northwest of Gamma Andromedae. 60 Andromedae is the Flamsteed designation though the star also bears the Bayer designation b Andromedae. It is bright enough to be seen by the naked eye with an apparent visual magnitude of 4.82.[2] Based upon parallax measurements made during the Hipparcos mission, it is at a distance of roughly 530 light-years (160 parsecs) from Earth.[1]
This system is known to have three components. The primary is a giant star with a stellar classification of K3.5 III Ba0.4. It is being orbited by a white dwarf with a period of 748.2 days and an eccentricity of 0.34. There is a third component at an angular separation of 0.22 arcseconds.[3]
References
- 1 2 3 4 5 6 van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.
- 1 2 3 4 Argue, A. N. (1966), "UBV photometry of 550 F, G and K type stars", Monthly Notices of the Royal Astronomical Society, 133: 475–493, Bibcode:1966MNRAS.133..475A, doi:10.1093/mnras/133.4.475.
- 1 2 Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x.
- ↑ Wilson, Ralph Elmer (1953), General Catalogue of Stellar Radial Velocities, Washington: Carnegie Institution of Washington, Bibcode:1953GCRV..C......0W.
- 1 2 3 Pourbaix, D.; Boffin, H. M. J. (February 2003), "Reprocessing the Hipparcos Intermediate Astrometric Data of spectroscopic binaries. II. Systems with a giant component", Astronomy and Astrophysics, 398: 1163–1177, arXiv:astro-ph/0211483, Bibcode:2003A&A...398.1163P, doi:10.1051/0004-6361:20021736.
- 1 2 3 Koleva, M.; Vazdekis, A. (February 2012), "Stellar population models in the UV. I. Characterisation of the New Generation Stellar Library", Astronomy & Astrophysics, 538: A143, arXiv:1111.5449, Bibcode:2012A&A...538A.143K, doi:10.1051/0004-6361/201118065.
- ↑ Tirion; Rappaport; Lovi (1987). Willmann-Bell, Inc., ed. Uranometria 2000.0 - Volume II - The Southern Hemisphere to +6°. Richmond, Virginia, USA. ISBN 0-943396-15-8.