Zeta Ceti

ζ Ceti
Location of ζ Ceti (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Cetus
Right ascension 01h 51m 27.631s
Declination −10° 20′ 06.112″
Apparent magnitude (V) 3.742
Characteristics
Spectral type K0 III Ba0.1
U−B color index +1.076
B−V color index +1.131
Variable type Suspected
Astrometry
Radial velocity (Rv)+10.86±0.64 km/s
Proper motion (μ) RA: +39.752 mas/yr
Dec.: −40.956 mas/yr
Parallax (π)12.8770±0.2100 mas
Distance253 ± 4 ly
(78 ± 1 pc)
Absolute magnitude (MV)−0.54
Orbit
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
ζ Cet A
Mass2.34 M
Radius25 R
Luminosity240 L
Surface gravity (log g)2.4 cgs
Temperature4,581±14 K
Metallicity [Fe/H]−0.13 dex
Rotational velocity (v sin i)3.2 km/s
Age1.24 Gyr
Other designations
Baten Kaitos, ζ Cet, 55 Cet, BD−11°359, FK5 62, HD 11353, HIP 8645, HR 539, SAO 148059, WDS J01515-1020A
Database references
SIMBADdata

Zeta Ceti is a binary star system in the equatorial constellation of Cetus. Its name is a Bayer designation that is Latinized from ζ Ceti, and abbreviated Zeta Cet or ζ Cet. The system has a combined apparent visual magnitude of 3.74, which is bright enough to be seen with the naked eye as a point of light. Based upon parallax measurements, it is approximately 253 light-years (78 pc) distant from the Earth. The system is drifting further from the Sun with a line of sight velocity component of +11 km/s.

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). Zeta Ceti's two components are therefore designated WDS J01515-1020 Aa and Ab. Aa is officially named Baten Kaitos /ˈbtən ˈktɒs/, the traditional name of the entire system.