Astronomy:63 Ceti
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Cetus |
| Right ascension | 02h 11m 35.83534s[1] |
| Declination | −01° 49′ 31.5355″[1] |
| Apparent magnitude (V) | +5.93[2] |
| Characteristics | |
| Spectral type | K0III[3] |
| U−B color index | +0.70[2] |
| B−V color index | +0.97[2] |
| Astrometry | |
| Radial velocity (Rv) | 27.69±0.05[4] km/s |
| Proper motion (μ) | RA: −11.526[1] mas/yr Dec.: −32.007[1] mas/yr |
| Parallax (π) | 8.4943 ± 0.0610[1] mas |
| Distance | 384 ± 3 ly (117.7 ± 0.8 pc) |
| Absolute magnitude (MV) | 0.57[5] |
| Details[4] | |
| Mass | 1.85 M☉ |
| Radius | 11.08+0.33 −0.54[1] R☉ |
| Luminosity | 63.7±0.6 L☉ |
| Surface gravity (log g) | 2.59 cgs |
| Temperature | 4940 K |
| Metallicity [Fe/H] | −0.17 ± 0.06 dex |
| Rotational velocity (v sin i) | 1.27 km/s |
| Age | 990±50[6] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
63 Ceti is a star in the constellation of Cetus, located just over a degree south of the celestial equator. With an apparent magnitude of about 5.9,[2] the star is barely visible to the naked eye (see Bortle scale) as a dim, orange-hued point of light. Parallax estimates put it at a distance of about 390 light years (129 parsecs) away from the Earth,[1] and it is drifting further away with a radial velocity of 28 km/s.[4]
63 Ceti has a spectral type of K0III,[3] implying an aging K-type giant star. These types of stars are generally reddish-colored stars with spectral types from K to M, with radii that are 10 to 100 times larger than the Sun.[8] 63 Ceti fits this description, with a radius about 11 times larger than the Sun, a mass of about 1.85 times the Sun, and an effective temperature of 4940 K.[4] 63 Ceti is a red clump giant, indicating it is currently at the horizontal branch, a stage in stellar evolution, and is generating energy through core helium fusion. It is close to a billion years old[6] and is radiating 64 times the luminosity of the Sun from its photosphere at an effective temperature of 4,940 K.[4]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ 2.0 2.1 2.2 2.3 Johnson, H. L. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory 4: 99. Bibcode: 1966CoLPL...4...99J.
- ↑ 3.0 3.1 Houk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars, Vol. 5". Michigan Spectral Survey 5: 0. Bibcode: 1999MSS...C05....0H.
- ↑ 4.0 4.1 4.2 4.3 4.4 Jones, M. I.; Jenkins, J. S.; Rojo, P.; Melo, C. H. F. (2011). "Study of the impact of the post-MS evolution of the host star on the orbits of close-in planets". Astronomy & Astrophysics 536: A71. doi:10.1051/0004-6361/201117887. Bibcode: 2011A&A...536A..71J.
- ↑ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 6.0 6.1 Gallenne, A. et al. (August 2018). "Fundamental properties of red-clump stars from long-baseline H-band interferometry". Astronomy & Astrophysics 616: 12. doi:10.1051/0004-6361/201833341. A68. Bibcode: 2018A&A...616A..68G.
- ↑ "* 63 Cet". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=%2A+63+Cet.
- ↑ David Darling. "Red giant". The Internet Encyclopedia of Science. http://www.daviddarling.info/encyclopedia/R/redgiant.html. Retrieved 21 March 2017.
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