Omicron1 Centauri

ο1 Centauri
Location of ο1 Cen (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Centaurus
Right ascension 11h 31m 46.07s
Declination −59° 26 31.4
Apparent magnitude (V) +5.13
Characteristics
Evolutionary stage Yellow hypergiant
Spectral type G3 0-Ia
B−V color index +1.08
Variable type SRd
Astrometry
Radial velocity (Rv)−20.00 km/s
Proper motion (μ) RA: −4.491 mas/yr
Dec.: +1.604 mas/yr
Parallax (π)0.3254±0.0734 mas
Distance10,100+2,700
−1,100
 ly
(3,110+820
−530
 pc)
Absolute magnitude (MV)−9.0
Details
Mass27±5.4 M
Radius440±35 R
Luminosity68,000 L
Surface gravity (log g)0.19 cgs
Temperature5,700 K
Age10–12 Myr
Other designations
HR 4441, HD 100261, CD−58°4100, HIP 56243, SAO 239145, GC 15818, CCDM J11318-5927, AAVSO 1127-58
Database references
SIMBADdata

Omicron1 Centauri (ο1 Cen, ο1 Centauri) is a star in the constellation Centaurus. It is approximately 10,000 light years from Earth, though this is very uncertain.

ο1 Centauri is a yellow G-type supergiant or hypergiant with a mean apparent magnitude of +5.13. Daniel Joseph Kelly O'Connell discovered that the star is a variable star by studying photographic plates taken from 1934 to 1952, and announced his discovery in 1961. It is classified as a semiregular variable star and its brightness varies from magnitude +5.8 to +6.6 with a period of 200 days. Other studies have reported only small brightness variations. It is the MK spectral standard for class G3 O-Ia, indicating a highly luminous mass-losing hypergiant star. It has also be classified as F8 Ia0 and F7 Ia/ab. The size, luminosity, and distance are equally uncertain.

ο1 Cen forms a very close naked eye double star with ο2 Centauri, a hotter blue supergiant that may be physically associated. ο1 Cen also has an 11th magnitude companion only 13.5" distant, although it appears to be a foreground star unrelated to the other two. ο1 Cen is located very close to V382 Carinae, the brightest yellow hypergiant star in the night sky.