F Centauri is a suspected astrometric binary[6] star system in the southern constellation of Centaurus. It has a reddish hue and is visible to the naked eye with an apparent visual magnitude that fluctuates around +5.01.[2] The system is located at a distance of approximately 450 light years from the Sun based on parallax, and it has an absolute magnitude of −0.87.[2] O. J. Eggen flagged this star as a member of the Hyades Supercluster.[7]
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Centaurus |
Right ascension | 12h 18m 59.76635s[1] |
Declination | −55° 08′ 34.7346″[1] |
Apparent magnitude (V) | +5.01[2] |
Characteristics | |
Spectral type | M1III[3] |
B−V color index | 1.600±0.008[2] |
Variable type | suspected[4] |
Astrometry | |
Radial velocity (Rv) | −7.1±2.8[2] km/s |
Proper motion (μ) | RA: -79.258[1] mas/yr Dec.: -15.215[1] mas/yr |
Parallax (π) | 7.3256 ± 0.1919 mas[1] |
Distance | 450 ± 10 ly (137 ± 4 pc) |
Absolute magnitude (MV) | −0.87[2] |
Details | |
Radius | 47.9+3.9 −6.3[1] R☉ |
Luminosity | 502±15[1] L☉ |
Temperature | 3,948+287 −151[1] K |
Other designations | |
Database references | |
SIMBAD | data |
The visible component is an aging red giant star on the asymptotic giant branch[8] with a stellar classification of M1III,[3] indicating it has exhausted the supply of both hydrogen and helium at its core and is cooling and expanding. It is a suspected variable star of unknown type that has been measured ranging in brightness from visual magnitude 4.94 down to 5.07.[4] At present it has 48 times the radius of the Sun. It is radiating 502 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 3,948 K.[1]