Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Cetus |
Right ascension | 01h 51m 27.63482s[1] |
Declination | −10° 20′ 06.1289″[1] |
Apparent magnitude (V) | 3.742[2] |
Characteristics | |
Spectral type | K0 III Ba0.1[3] |
U−B color index | +1.076[2] |
B−V color index | +1.131[2] |
Variable type | Suspected[4] |
Astrometry | |
Radial velocity (Rv) | +10.86±0.64[5] km/s |
Proper motion (μ) | RA: +40.80[1] mas/yr Dec.: −37.25[1] mas/yr |
Parallax (π) | 13.88 ± 0.57 mas[1] |
Distance | 235 ± 10 ly (72 ± 3 pc) |
Absolute magnitude (MV) | −0.54[6] |
Orbit[7] | |
Period (P) | 1,652 d |
Eccentricity (e) | 0.59 |
Longitude of the node (Ω) | 85° |
Periastron epoch (T) | 2414377 JD |
Semi-amplitude (K1) (primary) | 3.3 km/s |
Details[5] | |
ζ Cet A | |
Mass | 2.34[8] M☉ |
Radius | 25 R☉ |
Luminosity | 240 L☉ |
Surface gravity (log g) | 2.4 cgs |
Temperature | 4,581±14 K |
Metallicity [Fe/H] | −0.13 dex |
Rotational velocity (v sin i) | 3.2 km/s |
Age | 1.24[8] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Zeta Ceti (ζ Ceti, abbreviated Zeta Cet, ζ Cet) is a binary star in the equatorial constellation of Cetus. It has a combined apparent visual magnitude of 3.74,[2] which is bright enough to be seen with the naked eye. Based upon parallax measurements taken during the Hipparcos mission, it is approximately 235 light-years from the Sun.[1]
Zeta Ceti is the primary or 'A' component of a double star system designated WDS J01515-1020 (the secondary or 'B' component is HD 11366).[10] Zeta Ceti's two components are therefore designated WDS J01515-1020 Aa and Ab. Aa is officially named Baten Kaitos /ˈbeɪtən ˈkeɪtɒs/, the traditional name of the entire system.[11][12]
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