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M Centauri

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M Centauri
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Centaurus[1]
Right ascension 13h 46m 39.378s[2]
Declination −51° 25′ 57.95″[2]
Apparent magnitude (V) +4.63[3]
Characteristics
Spectral type G8/K0III[4]
U−B color index +0.72[citation needed]
B−V color index +0.96[citation needed]
Astrometry
Radial velocity (Rv)−15.97±2.25[5] km/s
Proper motion (μ) RA: +10.00±0.42[2] mas/yr
Dec.: −27.62±0.34[2] mas/yr
Parallax (π)12.42±0.48 mas[2]
Distance260 ± 10 ly
(81 ± 3 pc)
Absolute magnitude (MV)+0.11[1]
Orbit[6]
PrimaryM Centauri A
CompanionM Centauri B
Period (P)437 days
Semi-major axis (a)6.45 mas
Eccentricity (e)0.13
Inclination (i)48.2°
Longitude of the node (Ω)280.3°
Periastron epoch (T)2424163.0
Argument of periastron (ω)
(secondary)
58.6°
Other designations
HR 5172, HD 119834, CD−50°8017, HIP 67234, SAO 241157, GC 18607, CCDM J13467-5126
Database references
SIMBADdata

M Centauri (M Cen) is a binary star in the constellation Centaurus. It is approximately 260 light years from Earth.

M Centauri is a yellow G-type giant with an apparent magnitude of +4.64. It is a spectroscopic binary with an orbital period of 437 days.

References

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  1. ^ a b Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. XHIP record for this object at VizieR.
  2. ^ a b c d e van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600. Vizier catalog entry
  3. ^ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355. Bibcode:2000A&A...355L..27H.
  4. ^ Houk, Nancy (1978). "Michigan catalogue of two-dimensional spectral types for the HD stars". Ann Arbor : Dept. Of Astronomy. Bibcode:1978mcts.book.....H.
  5. ^ 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.
  6. ^ Jancart, S. (2005). "Astrometric orbits of SB9 stars". Astronomy and Astrophysics. 442 (1): 365–380. arXiv:astro-ph/0507695. Bibcode:2005A&A...442..365J. doi:10.1051/0004-6361:20053003. S2CID 15123997.