Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Cetus |
Right ascension | 01h 24m 01.40328s[1] |
Declination | −08° 10′ 59.7392″[1] |
Apparent magnitude (V) | 3.60[2] |
Characteristics | |
Spectral type | K0 III[3] |
B−V color index | +1.07[2] |
Astrometry | |
Radial velocity (Rv) | +17.2±0.5[4] km/s |
Proper motion (μ) | RA: −76.226 mas/yr[1] Dec.: −201.519 mas/yr[1] |
Parallax (π) | 29.0339 ± 0.2198 mas[1] |
Distance | 112.3 ± 0.9 ly (34.4 ± 0.3 pc) |
Absolute magnitude (MV) | +0.89[5] |
Details | |
Mass | 1.80[6] M☉ |
Radius | 10.37±0.09[7] R☉ |
Luminosity | 58.3±3.0[7] L☉ |
Surface gravity (log g) | 2.70[2] cgs |
Temperature | 4,951±64[7] K |
Metallicity [Fe/H] | −0.13±0.15[2] dex |
Rotational velocity (v sin i) | 2.60[2] km/s |
Age | 2.20[6] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Theta Ceti, Latinized from θ Ceti, is a solitary,[9] orange-hued star in the equatorial constellation of Cetus. It is visible to the naked eye with an apparent visual magnitude of 3.60.[2] Based upon an annual parallax shift of 20m04 mas as seen from Earth,[1] it is located about 113 light-years from the Sun. At that distance, the visual magnitude is diminished by an extinction factor of 0.28 due to interstellar dust.[7]
With an age of about 2.2 billion years,[6] this is an evolved, K-type giant star with a stellar classification of K0 III.[3] It is a red clump[10] star on the horizontal branch,[2] which means it is generating energy through helium fusion at its core.[10] The star has an estimated 1.8[6] times the mass of the Sun and has expanded to 10 times the Sun's radius. It is radiating 58 times the solar luminosity from its photosphere at an effective temperature of 4,951 K.[7]
DR3
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was invoked but never defined (see the help page).Eggleton2008
was invoked but never defined (see the help page).Joner2012
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