63 Ceti
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cetus |
Right ascension | 02h 11m 35.83502s[1] |
Declination | −01° 49′ 31.5439″[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: −11.27[1] mas/yr Dec.: −32.96[1] mas/yr |
Parallax (π) | 8.40 ± 0.46[1] mas |
Distance | 390 ± 20 ly (119 ± 7 pc) |
Details[4] | |
Mass | 1.85 M☉ |
Radius | 11.06 R☉ |
Luminosity | 68.08 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 |
Other designations | |
Database references | |
SIMBAD | data |
63 Ceti is a star in the constellation of Cetus. With an apparent magnitude of about 5.9,[2] the star is barely visible to the naked eye (see Bortle scale). Parallax estimates made by the Hipparcos spacecraft put it at a distance of about 390 light years (129 parsecs) away from the Earth.[1]
63 Ceti has a spectral type of K0III,[3] implying a K-type giant. 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.[6] 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 currently at the horizontal branch, an stage in stellar evolution.[5]
References
- 1 2 3 4 5 6 van Leeuwen, F.; et al. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. Bibcode:2007A&A...474..653V. arXiv:0708.1752 . doi:10.1051/0004-6361:20078357.
- 1 2 3 4 Johnson, H. L. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99. Bibcode:1966CoLPL...4...99J.
- 1 2 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.
- 1 2 3 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.
- 1 2 "* 63 Cet". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 21 March 2017.
- ↑ David Darling. "Red giant". The Internet Encyclopedia of Science. Retrieved 21 March 2017.
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