24 Capricorni
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Capricornus |
Right ascension | 21h 07m 07.66733s[1] |
Declination | −25° 00′ 21.0790″[1] |
Apparent magnitude (V) | +4.49[2] |
Characteristics | |
Spectral type | M1− III[3] |
B−V color index | ±0.005 1.604[2] |
Astrometry | |
Radial velocity (Rv) | ±0.8 +32.1[2] km/s |
Proper motion (μ) | RA: −28.09[1] mas/yr Dec.: −44.14[1] mas/yr |
Parallax (π) | 7.15 ± 0.22[1] mas |
Distance | 460 ± 10 ly (140 ± 4 pc) |
Absolute magnitude (MV) | −1.24[2] |
Details | |
Radius | 54[4] R☉ |
Luminosity | 611[4] L☉ |
Temperature | 3,903[4] K |
Other designations | |
Database references | |
SIMBAD | data |
24 Capricorni is a single[6] star in the constellation Capricornus. 24 Capricorni is a M-type red giant with an apparent magnitude of +4.49. It is approximately 460 light years from Earth.
Chinese name
In R. H. Allen's version, this star was represent the state Chu (or Tsoo).[7]
References
- 1 2 3 4 5 van Leeuwen, F. (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 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.
- ↑ Keenan, P. C.; McNeil, R. C. (1989), "The Perkins catalog of revised MK types for the cooler stars", The Astrophysical Journal Supplement Series, 71: 245, Bibcode:1989ApJS...71..245K, doi:10.1086/191373.
- 1 2 3 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.
- ↑ "24 Cap". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-06-15.
- ↑ 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.
- ↑ Star Names - R.H.Allen p.142
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