| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Andromeda |
| Right ascension | 00h 10m 19.24653s |
| Declination | +46° 04′ 20.1704″ |
| Apparent magnitude (V) | 5.04 |
| Characteristics | |
| Spectral type | F5 II or F5 Ib–II metal-weak |
| B−V color index | +0.04 |
| Astrometry | |
| Radial velocity (Rv) | −8.2±2.2 km/s |
| Proper motion (μ) | RA: 5.472 mas/yr Dec.: 0.086 mas/yr |
| Parallax (π) | 2.2233 ± 0.3881 mas |
| Distance | approx. 1,500 ly (approx. 450 pc) |
| Absolute magnitude (MV) | −3.51 |
| Details | |
| Mass | 6.1±0.4 M☉ |
| Radius | 17 R☉ |
| Luminosity | 1,436 L☉ |
| Surface gravity (log g) | 2.10±0.08 cgs |
| Temperature | 6,270±150 K |
| Metallicity [Fe/H] | −0.09±0.05 dex |
| Rotational velocity (v sin i) | 46 km/s |
| Age | 62 Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
22 Andromedae, abbreviated 22 And, is a single star in the constellation Andromeda. 22 Andromedae is the Flamsteed designation. It is visible to the naked eye with an apparent visual magnitude of 5.04. The distance to 22 And can be estimated from its annual parallax shift of just 2.2 mas, which shows it to be around 1,500 light years away. It is moving closer to the Earth with a heliocentric radial velocity of −8.2 km/s.
This is a bright giant with a stellar classification of F5 II. Gray et al. (2001) classify it as F5 Ib–II metal-weak, with the metallic lines matching a class of F0 whereas hydrogen lines match an F5. It is around 62 million years old with a projected rotational velocity of 46. The star has six times the mass of the Sun and has expanded to about 17 times the Sun's radius. It is radiating 1,436 times the Sun's luminosity from its photosphere at an effective temperature of 6,270 km/s.
References
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- ^ a b Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy and Astrophysics, 367 (2) (Third ed.): 521–524, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451, S2CID 425754.
- ^ a b Hohle, M.M.; et al. (2010), "Masses and luminosities of O- and B-type stars and red supergiants", Astronomische Nachrichten, 331 (4): 349, arXiv:1003.2335, Bibcode:2010AN....331..349H, doi:10.1002/asna.200911355, S2CID 111387483.
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- ^ "22 And". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved September 21, 2018.
- ^ 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, S2CID 14878976.