63 Ceti

63 Ceti
Observation data
Epoch J2000      Equinox J2000
Constellation Cetus
Right ascension 02h 11m 35.83534s
Declination −01° 49 31.5355
Apparent magnitude (V) +5.93
Characteristics
Spectral type K0III
U−B color index +0.70
B−V color index +0.97
Astrometry
Radial velocity (Rv)27.69±0.05 km/s
Proper motion (μ) RA: 11.526 mas/yr
Dec.: 32.007 mas/yr
Parallax (π)8.4943±0.0610 mas
Distance384 ± 3 ly
(117.7 ± 0.8 pc)
Absolute magnitude (MV)0.57
Details
Mass1.85 M
Radius11.08+0.33
−0.54
 R
Luminosity63.7±0.6 L
Surface gravity (log g)2.59 cgs
Temperature4940 K
Metallicity [Fe/H]0.17 ± 0.06 dex
Rotational velocity (v sin i)1.27 km/s
Age990±50 Myr
Other designations
63 Cet, BD02°375, HD 13468, HIP 10234, HR 639, SAO 129739
Database references
SIMBADdata

63 Ceti is a star in the constellation of Cetus, located just over a degree south of the celestial equator. With an apparent magnitude of about 5.9, the star is barely visible to the naked eye (see Bortle scale) as a dim, orange-hued point of light. Parallax estimates put it at a distance of about 390 light years (129 parsecs) away from the Earth, and it is drifting further away with a radial velocity of 28 km/s.

63 Ceti has a spectral type of K0III, implying an aging K-type giant star. These types of stars are generally reddish-colored stars with spectral types from K to M, with radii that are 10 to 100 times larger than the Sun. 63 Ceti fits this description, with a radius about 11 times larger than the Sun, a mass of about 1.85 times the Sun, and an effective temperature of 4940 K. 63 Ceti is a red clump giant, indicating it is currently at the horizontal branch, a stage in stellar evolution, and is generating energy through core helium fusion. It is close to a billion years old and is radiating 64 times the luminosity of the Sun from its photosphere at an effective temperature of 4,940 K.