Misplaced Pages

Omicron2 Centauri

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Variable star in the constellation Centaurus For other star systems with this Bayer designation, see Omicron Centauri.
ο Centauri
Location of ο Cen (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Centaurus
Right ascension 11 31 48.79955
Declination −59° 30′ 56.3296″
Apparent magnitude (V) +5.14 (5.12 - 5.22)
Characteristics
Evolutionary stage Blue supergiant
Spectral type A2Iae
U−B color index −0.11
B−V color index +0.49
Variable type α Cyg
Astrometry
Radial velocity (Rv)−16.8 km/s
Proper motion (μ) RA: −6.976 mas/yr
Dec.: +1.118 mas/yr
Parallax (π)0.4665 ± 0.0713 mas
Distanceapprox. 7,000 ly
(approx. 2,100 pc)
Absolute magnitude (MV)−7.50
Details
Mass18 M
Radius131 R
Luminosity105,000 L
Surface gravity (log g)1.46 cgs
Temperature9,080 K
Rotation132 days
Rotational velocity (v sin i)50 km/s
Other designations
HR 4442, HD 100262, CD−58°4101, FK5 2920, HIP 56250, SAO 239146, GC 15820
Database references
SIMBADdata

Omicron Centauri (ο Cen, ο Centauri) is a star in the constellation Centaurus.

ο Centauri is a white A-type blue supergiant with a mean apparent magnitude of +5.12. It is approximately 7,000 light years from Earth. It is classified as an Alpha Cygni type variable star and its brightness varies from magnitude +5.12 to +5.22 with a period of 46.3 days.

In 1996, Kaufer and colleagues calculated Omicron Centauri to be around 136,000 times as luminous, 18 times as massive and have 131 times the diameter of the Sun.

ο Cen forms a close naked eye pair with ο Cen, another 5th magnitude supergiant (possibly a yellow hypergiant). Both stars are located between Crux (the Southern Cross) and the brightest yellow hypergiant in the sky, V382 Carinae.

References

  1. ^ Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  2. ^ Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode:2002yCat.2237....0D.
  3. ^ Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
  4. Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Washington. Bibcode:1953GCRV..C......0W.
  5. ^ Kaufer, A.; Stahl, O.; Wolf, B.; Gaeng, T.; Gummersbach, C. A.; Kovacs, J.; Mandel, H.; Szeifert, T. (1996). "Long-term spectroscopic monitoring of BA-type supergiants. I. Halpha_ line-profile variability". Astronomy and Astrophysics. 305: 887–901. Bibcode:1996A&A...305..887K.
Constellation of Centaurus
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star clusters
Nebulae
Galaxies
NGC
Other
Galaxy clusters
Astronomical events
Category
Categories: