Zeta Caeli

Zeta Caeli
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Caelum
Right ascension 04h 47m 49.57719s
Declination −30° 01 13.3391
Apparent magnitude (V) +6.36
Characteristics
Spectral type K0 III
B−V color index +1.06
Astrometry
Radial velocity (Rv)+6.7±1.0 km/s
Proper motion (μ) RA: +28.747 mas/yr
Dec.: +92.712 mas/yr
Parallax (π)6.8479±0.0167 mas
Distance476 ± 1 ly
(146.0 ± 0.4 pc)
Absolute magnitude (MV)+0.76
Details
Mass2.90+0.04
−0.30
 M
Radius12.45±0.25 R
Luminosity86.67+0.42
−0.44
 L
Surface gravity (log g)2.62±0.01 cgs
Temperature4,992+6
−5
 K
Metallicity [Fe/H]−0.22 dex
Age414+99
−41
 Myr
Other designations
ζ Cae, CD−30°2011, GC 5851, HD 30608, HIP 22280, HR 1539, SAO 195300
Database references
SIMBADdata

Zeta Caeli is an orange-hued star in the southern constellation of Caelum. Its name is a Bayer designation that is Latinized from ζ Caeli, and abbreviated Zeta Cae or ζ Cae. With an apparent visual magnitude of +6.36, it is near the lower limit of brightness for stars visible to the naked eye. Based upon an annual parallax shift of 7.59 mas as seen from Earth, this star is located about 430 light-years (130 pc) away. It is drifting further from the Sun with a line of sight velocity of +7 km/s.

This is an evolved K-type giant star with a stellar classification of K0 III. At an estimated 414 million years of age, this star has 2.9 times the mass of the Sun but it has expanded to 12 times the Sun's radius. It is radiating 87 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,992 K. This star is a member of the Milky Way's thick disk population.