Gamma Centauri

Gamma Centauri
Location of γ Centauri (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Centaurus
Right ascension 12h 41m 31.04008s
Declination −48° 57 35.5375
Apparent magnitude (V) +2.17 (+2.85/+2.95)
Characteristics
Spectral type A1IV+ (A1IV + A0IV)
U−B color index −0.01
B−V color index −0.01
Astrometry
Radial velocity (Rv)−5.5 km/s
Proper motion (μ) RA: −185.72 mas/yr
Dec.: +5.79 mas/yr
Parallax (π)25.06±0.28 mas
Distance130 ± 1 ly
(39.9 ± 0.4 pc)
Absolute magnitude (MV)−0.81
Orbit
Companionγ Centauri B
Period (P)83.57±0.21 yr
Semi-major axis (a)0.869±0.011
Eccentricity (e)0.793±0.003
Inclination (i)113.7±0.7°
Longitude of the node (Ω)2.6±0.7°
Periastron epoch (T)1931.25 ± 0.07
Argument of periastron (ω)
(secondary)
187.9±1.5°
Details
Mass2.8 M
Radius3.8 R
Luminosity95 L
Surface gravity (log g)3.52 cgs
Temperature9,300 K
Metallicity−0.29
B
Mass2.8 M
Radius3.8 R
Luminosity95 L
Temperature9,300 K
Other designations
Muhlifain, γ Cen, CD−48°7597, GC 17262, HD 110304, HIP 61932, HR 4819, SAO 223603, CCDM J12415-4858, WDS 12415-4858
Database references
SIMBADdata

Gamma Centauri is a binary star system in the southern constellation of Centaurus, which is probably part of a wider system together with Tau Centauri. The system is visible to the naked eye as a single point of light with a combined apparent visual magnitude of +2.17; individually they are third-magnitude stars.