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Star in the constellation Centaurus From Wikipedia, the free encyclopedia
Phi Centauri, Latinized from φ Centauri, is a blue-white hued star in the southern constellation Centaurus. It is visible to the naked eye with an apparent visual magnitude of +3.7.[2] The annual parallax shift is 6.21 mas[1] as measured from Earth, which yields a distance estimate of around 530 light years. It is moving further from the Sun with a radial velocity of +5 km/s.[5]
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Centaurus |
Right ascension | 13h 58m 16.27s[1] |
Declination | −42° 06′ 02.7″[1] |
Apparent magnitude (V) | +3.745[2] |
Characteristics | |
Spectral type | B2 IV[3] |
U−B color index | −0.851[4] |
B−V color index | −0.222[4] |
Astrometry | |
Radial velocity (Rv) | +5.3±1.5[5] km/s |
Proper motion (μ) | RA: −22.77±0.15[1] mas/yr Dec.: −20.13±0.12[1] mas/yr |
Parallax (π) | 6.21 ± 0.17 mas[1] |
Distance | 530 ± 10 ly (161 ± 4 pc) |
Absolute magnitude (MV) | −2.20[2] |
Details | |
Mass | 8.5±0.3[3] M☉ |
Radius | 4.19±0.35[6] R☉ |
Luminosity | 4,000[7] L☉ |
Surface gravity (log g) | 4.08±0.07[6] cgs |
Temperature | 21,638±388[6] K |
Rotational velocity (v sin i) | 79[8] km/s |
Age | 18.0±3.2[3] Myr |
Other designations | |
Database references | |
SIMBAD | data |
This is a B-type subgiant star with a stellar classification of B2 IV.[3] It has no known companions, but does show radial velocity variations and higher order pulsations in the spectrum.[9] The star is just 18[3] million years old with 8.5[3] times the mass of the Sun and has 4.2[6] times the Sun's radius. It is radiating around 4,000[7] times the Sun's luminosity from its photosphere at an effective temperature of about 21,638 K.[6]
This star is a proper motion member of the Upper Centaurus–Lupus sub-group in the Scorpius–Centaurus OB association, the nearest such co-moving association of massive stars to the Sun.[7]
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