Astronomy:81 Ceti
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Cetus |
| Right ascension | 02h 37m 41.80208s[1] |
| Declination | −03° 23′ 46.2259″[1] |
| Apparent magnitude (V) | 5.65[2] |
| Characteristics | |
| Evolutionary stage | red clump[3] |
| Spectral type | K0III[4] or G5III[5] |
| B−V color index | 1.021±0.001[2] |
| Astrometry | |
| Radial velocity (Rv) | +9.14±0.12[1] km/s |
| Proper motion (μ) | RA: 41.765[1] mas/yr Dec.: −43.379[1] mas/yr |
| Parallax (π) | 9.5199 ± 0.0756[1] mas |
| Distance | 343 ± 3 ly (105.0 ± 0.8 pc) |
| Absolute magnitude (MV) | 0.82[2] |
| Details[6] | |
| Mass | 1.6±0.2 M☉ |
| Radius | 11.1±0.3 R☉ |
| Luminosity | 60.0±0.8 L☉ |
| Surface gravity (log g) | 2.5±0.1 cgs |
| Temperature | 4,825±41 K |
| Metallicity [Fe/H] | 0.00±0.04[7] dex |
| Rotational velocity (v sin i) | 1.20±0.47[7] km/s |
| Age | 2.5±0.9 Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
| Extrasolar Planets Encyclopaedia | data |
81 Ceti is a star located approximately 343 light-years away from the Sun in the equatorial constellation of Cetus. 81 Ceti is the Flamsteed designation for this object. It is visible to the naked eye as a dim, yellow-hued point of light with an apparent visual magnitude of 5.65.[2] The star is drifting further away from the Earth with a heliocentric radial velocity of +9 km/s.[2]
This is an aging K-type giant star with a stellar classification of K0III,[4] having exhausted the supply of hydrogen at its core and expanded to 11[6] times the Sun's radius. It is a red clump giant,[3] which indicates it is on the horizontal branch and is generating energy from core helium fusion. The star is now 2.5 billion years old with 1.6 times the mass of the Sun.[6] It is radiating 60 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,825 K.[6]
Planetary system
In July 2008, the planet 81 Ceti b was announced by Sato and collaborators, along with 14 Andromedae b and 6 Lyncis b. The planet was found to be a super-Jupiter, with 5.3 times the mass of Jupiter. It takes 953 days for it to complete its orbit around the star.[5] The planetary parameters were updated in 2023.[8]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | ≥3.307+0.078 −0.067 MJ |
2.104±0.003 | 1005.57+1.84 −1.94 |
0.037+0.015 −0.025 |
— | — |
See also
References
- ↑ 1.0 1.1 1.2 1.3 1.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940 Gaia DR3 record for this source at VizieR.
- ↑ 2.0 2.1 2.2 2.3 2.4 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A.
- ↑ 3.0 3.1 Mishenina, T. V. et al. (September 2006), "Elemental abundances in the atmosphere of clump giants", Astronomy and Astrophysics 456 (3): 1109–1120, doi:10.1051/0004-6361:20065141, Bibcode: 2006A&A...456.1109M
- ↑ 4.0 4.1 Houk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars". Michigan Spectral Survey 5. Bibcode: 1999MSS...C05....0H.
- ↑ 5.0 5.1 Sato, Bun'ei et al. (2008). "Planetary Companions to Evolved Intermediate-Mass Stars: 14 Andromedae, 81 Ceti, 6 Lyncis, and HD167042". Publications of the Astronomical Society of Japan 60 (6): 1317–1326. doi:10.1093/pasj/60.6.1317. Bibcode: 2008PASJ...60.1317S.
- ↑ 6.0 6.1 6.2 6.3 Bonfanti, A. et al. (2015). "Revising the ages of planet-hosting stars". Astronomy and Astrophysics 575: A18. doi:10.1051/0004-6361/201424951. Bibcode: 2015A&A...575A..18B.
- ↑ 7.0 7.1 Jofré, E. et al. (2015). "Stellar parameters and chemical abundances of 223 evolved stars with and without planets". Astronomy & Astrophysics 574: A50. doi:10.1051/0004-6361/201424474. Bibcode: 2015A&A...574A..50J.
- ↑ 8.0 8.1 Teng, Huan-Yu et al. (August 2023). "Revisiting planetary systems in the Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and a multiplicity-metallicity trend around evolved stars". Publications of the Astronomical Society of Japan 75 (6): 1030–1071. doi:10.1093/pasj/psad056. Bibcode: 2023PASJ...75.1030T.
External links
- Jean Schneider (2011). "Notes for star 81 Cet". Extrasolar Planets Encyclopaedia. http://exoplanet.eu/star.php?st=81+Cet. Retrieved 12 October 2011.
Coordinates: 
02h 37m 41.8003s, −03° 23′ 46.229″
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