A light curve for V806 Centauri. The main plot shows the long term variability from Hipparcos data,[1] and the inset plot shows the variability over the 26.5 day period, using data from Tabur et al. (2009).[2] The green curve shows the best-fit sine wave, which has an amplitude of 18 millimagnitudes. | |
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Centaurus |
Right ascension | 13h 49m 26.72175s[3] |
Declination | −34° 27′ 02.7929″[3] |
Apparent magnitude (V) | 4.19[4] (4.16–4.26)[5] |
Characteristics | |
Spectral type | M5 III[6] |
U−B color index | +1.44[7] |
B−V color index | +1.49[7] |
Variable type | SRb[5] |
Astrometry | |
Radial velocity (Rv) | +40.7±0.7[8] km/s |
Proper motion (μ) | RA: −41.68±0.23[3] mas/yr Dec.: −59.77±0.18[3] mas/yr |
Parallax (π) | 17.82 ± 0.21 mas[3] |
Distance | 183 ± 2 ly (56.1 ± 0.7 pc) |
Absolute magnitude (MV) | +0.51[9] |
Details | |
Radius | 70[10] R☉ |
Luminosity | 71.96[4] L☉ |
Temperature | 3,398[11] K |
Other designations | |
Database references | |
SIMBAD | data |
2 Centauri is a single[13] star in the southern constellation of Centaurus, located approximately 183 light-years from Earth.[3] It has the Bayer designation g Centauri;[12] 2 Centauri is the Flamsteed designation. This object is visible to the naked eye as faint, red-hued star with an apparent visual magnitude of 4.19.[4] It is moving away from the Earth with a heliocentric radial velocity of +41 km/s.[8] The star is a member of the HR 1614 supercluster.[14]
This is an evolved red giant star with a stellar classification of M5 III.[6] It is classified as a semiregular variable star and its brightness varies from magnitude +4.16 to +4.26[5] with a period of 12.57 days.[15] The star has around 70[10] times the Sun's radius and is radiating 72[4] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 3,398 K.[11]
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