F Centauri

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F Centauri
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Centaurus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) +5.01[2]
Characteristics
Spectral type M1III[3]
B−V Template:Engvar Script error: No such module "val".[2]
Variable type suspected[4]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[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]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−0.87[2]
Details
RadiusScript error: No such module "val".[1] Template:Solar radius
LuminosityScript error: No such module "val".[1] Template:Solar luminosity
TemperatureScript error: No such module "val".[1] K
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[5]
Database references
SIMBADdata

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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]

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]

References

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Template:Stars of Centaurus