Kappa1 Ceti

κ1 Ceti
Location of κ1 Ceti (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cetus
Right ascension 03h 19m 21.6964s
Declination +03° 22 12.715
Apparent magnitude (V) 4.84
Characteristics
Spectral type G5Vv
U−B color index +0.185
B−V color index +0.674
Variable type BY Dra
Astrometry
Radial velocity (Rv)+19.9 km/s
Proper motion (μ) RA: +269.298 mas/yr
Dec.: +93.957 mas/yr
Parallax (π)107.8023±0.1838 mas
Distance30.26 ± 0.05 ly
(9.28 ± 0.02 pc)
Absolute magnitude (MV)5.16
Details
Mass1.021±0.021 M
Radius0.95±0.05 R
Luminosity0.879±0.028 L
Surface gravity (log g)4.50±0.04 cgs
Temperature5,786±87 K
Metallicity [Fe/H]+0.04±0.01 dex
Rotation9.2 days
Rotational velocity (v sin i)4.5 km/s
Age300–400 Myr
Other designations
κ1 Cet, 96 Ceti, NSV 1100, BD+02°518, FK5 1095, GJ 137, HD 20630, HIP 15457, HR 996, SAO 111120, LTT 11094
Database references
SIMBADdata
ARICNSdata

Kappa1 Ceti, Latinized from κ1 Ceti, is a variable yellow dwarf star approximately 30 light-years away in the equatorial constellation of Cetus.

Bayer used the designations κ Ceti and g Tauri for the same star. g Tauri is now no longer used.

The star was discovered to have a rapid rotation, roughly once every nine days. Though there are no extrasolar planets confirmed to be orbiting the star, Kappa1 Ceti is considered a good candidate to contain terrestrial planets, like the Earth. The system is a candidate binary star, but has not been confirmed.