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Omicron2 Centauri

Omicron2 Centauri (ο2 Cen, ο2 Centauri) is a star in the constellation Centaurus.

ο2 Centauri
Location of ο2 Cen (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Centaurus
Right ascension 11h 31m 48.79955s[1]
Declination −59° 30′ 56.3296″[1]
Apparent magnitude (V) +5.14[2] (5.12 - 5.22[3])
Characteristics
Spectral type A2Iae[3]
U−B color index −0.11[2]
B−V color index +0.49[2]
Variable type α Cyg[3]
Astrometry
Radial velocity (Rv)−16.8[4] km/s
Proper motion (μ) RA: −6.976[1] mas/yr
Dec.: +1.118[1] mas/yr
Parallax (π)0.4665 ± 0.0713 mas[1]
Distanceapprox. 7,000 ly
(approx. 2,100 pc)
Absolute magnitude (MV)−7.50[5]
Details[5]
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

ο2 Centauri is a white A-type 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 Omicron2 Centauri to be around 136,000 times as luminous, 18 times as massive and have 131 times the diameter of the Sun.[5]

ο2 Cen forms a close naked eye pair with ο1 Cen, another 5th magnitude supergiant.

References edit

  1. ^ a b c d e 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. ^ a b c 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. ^ a b c 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. ^ a b c 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.

omicron2, centauri, other, star, systems, with, this, bayer, designation, omicron, centauri, centauri, star, constellation, centaurus, centaurilocation, circled, observation, dataepoch, j2000, equinox, j2000, constellation, centaurus, right, ascension, 79955s,. For other star systems with this Bayer designation see Omicron Centauri Omicron2 Centauri o2 Cen o2 Centauri is a star in the constellation Centaurus o2 CentauriLocation of o2 Cen circled Observation dataEpoch J2000 0 Equinox J2000 0 Constellation Centaurus Right ascension 11h 31m 48 79955s 1 Declination 59 30 56 3296 1 Apparent magnitude V 5 14 2 5 12 5 22 3 Characteristics Spectral type A2Iae 3 U B color index 0 11 2 B V color index 0 49 2 Variable type a Cyg 3 AstrometryRadial velocity Rv 16 8 4 km sProper motion m RA 6 976 1 mas yr Dec 1 118 1 mas yrParallax p 0 4665 0 0713 mas 1 Distanceapprox 7 000 ly approx 2 100 pc Absolute magnitude MV 7 50 5 Details 5 Mass18 M Radius131 R Luminosity105 000 L Surface gravity log g 1 46 cgsTemperature9 080 KRotation132 daysRotational velocity v sin i 50 km s Other designationsHR 4442 HD 100262 CD 58 4101 FK5 2920 HIP 56250 SAO 239146 GC 15820 Database referencesSIMBADdata o2 Centauri is a white A type 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 Omicron2 Centauri to be around 136 000 times as luminous 18 times as massive and have 131 times the diameter of the Sun 5 o2 Cen forms a close naked eye pair with o1 Cen another 5th magnitude supergiant References edit a b c d e 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 amp A 674A 1G doi 10 1051 0004 6361 202243940 S2CID 244398875 Gaia DR3 record for this source at VizieR a b c 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 a b c 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 Wilson Ralph Elmer 1953 General catalogue of stellar radial velocities Washington Bibcode 1953GCRV C 0W a b c 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 amp A 305 887K Retrieved from https en wikipedia org w index php title Omicron2 Centauri amp oldid 1154754850, wikipedia, wiki, book, books, library,

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