Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Centaurus |
Right ascension | 11h 31m 46.07s [1] |
Declination | −59° 26′ 31.4″ [1] |
Apparent magnitude (V) | +5.13 [2] |
Characteristics | |
Spectral type | G3 0-Ia [3] [4] |
B−V color index | +1.08 [2] |
Variable type | SRd [5] |
Astrometry | |
Radial velocity (Rv) | −20.00 [6] km/s |
Proper motion (μ) |
RA: −4.491
[1]
mas/
yr Dec.: +1.604 [1] mas/ yr |
Parallax (π) | 0.3254 ± 0.0734 mas [1] |
Distance | approx. 10,000
ly (approx. 3,100 pc) |
Absolute magnitude (MV) | −9.0 [4] |
Details | |
Mass | 17 [7] M☉ |
Radius | 270 [7] R☉ |
Luminosity | 68,000 [7] L☉ |
Surface gravity (log g) | 0.19 [8] cgs |
Temperature | 4,873 [9] K |
Age | 10–12 [7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Omicron1 Centauri (ο1 Cen, ο1 Centauri) is a star in the constellation Centaurus. It is approximately 10,000 light years from Earth.
ο1 Centauri is a yellow G-type supergiant or hypergiant with a mean apparent magnitude of +5.13. 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. [5] Other studies have reported only small brightness variations. [11] [12] It is the MK spectral standard for class G3 O-Ia, [13] indicating a highly luminous mass-losing hypergiant star. It has also be classified as F8 Ia0 [14] and F7 Ia/ab. [15] The size, luminosity, and distance are equally uncertain.
ο1 Cen forms a very close naked eye double star with ο2 Centauri, a hotter supergiant that may be physically associated. ο1 Cen also has an 11th magnitude companion only 13.5" distant, [16] Although it appears to be a foreground star unrelated to the other two. [17]
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Centaurus |
Right ascension | 11h 31m 46.07s [1] |
Declination | −59° 26′ 31.4″ [1] |
Apparent magnitude (V) | +5.13 [2] |
Characteristics | |
Spectral type | G3 0-Ia [3] [4] |
B−V color index | +1.08 [2] |
Variable type | SRd [5] |
Astrometry | |
Radial velocity (Rv) | −20.00 [6] km/s |
Proper motion (μ) |
RA: −4.491
[1]
mas/
yr Dec.: +1.604 [1] mas/ yr |
Parallax (π) | 0.3254 ± 0.0734 mas [1] |
Distance | approx. 10,000
ly (approx. 3,100 pc) |
Absolute magnitude (MV) | −9.0 [4] |
Details | |
Mass | 17 [7] M☉ |
Radius | 270 [7] R☉ |
Luminosity | 68,000 [7] L☉ |
Surface gravity (log g) | 0.19 [8] cgs |
Temperature | 4,873 [9] K |
Age | 10–12 [7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Omicron1 Centauri (ο1 Cen, ο1 Centauri) is a star in the constellation Centaurus. It is approximately 10,000 light years from Earth.
ο1 Centauri is a yellow G-type supergiant or hypergiant with a mean apparent magnitude of +5.13. 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. [5] Other studies have reported only small brightness variations. [11] [12] It is the MK spectral standard for class G3 O-Ia, [13] indicating a highly luminous mass-losing hypergiant star. It has also be classified as F8 Ia0 [14] and F7 Ia/ab. [15] The size, luminosity, and distance are equally uncertain.
ο1 Cen forms a very close naked eye double star with ο2 Centauri, a hotter supergiant that may be physically associated. ο1 Cen also has an 11th magnitude companion only 13.5" distant, [16] Although it appears to be a foreground star unrelated to the other two. [17]