2 Centauri
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Centaurus |
Right ascension | 13h 49m 26.72s[1] |
Declination | −34° 27′ 02.8″[1] |
Apparent magnitude (V) | 4.16 - 4.26[2] |
Characteristics | |
Spectral type | M5III[3] |
U−B color index | +1.44[4] |
B−V color index | +1.49[4] |
Variable type | SRb[2] |
Astrometry | |
Radial velocity (Rv) | +40.7 ± 0.7[5] km/s |
Proper motion (μ) | RA: -41.68 ± 0.23[1] mas/yr Dec.: -59.77 ± 0.18[1] mas/yr |
Parallax (π) | 17.82 ± 0.21[1] mas |
Distance | 183 ± 2 ly (56.1 ± 0.7 pc) |
Absolute magnitude (MV) | +0.51[6] |
Other designations | |
Database references | |
SIMBAD | data |
2 Centauri is a star in the constellation Centaurus.
2 Centauri is an M-type red giant with a mean apparent magnitude of +4.19. It is approximately 183 light years from Earth. It is classified as a semiregular variable star and its brightness varies from magnitude +4.16 to +4.26 with a period of 12. days.
References
- 1 2 3 4 5 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. Vizier catalog entry
- 1 2 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.
- ↑ Houk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars, Vol. 5". Michigan Spectral Survey. 5. Bibcode:1999MSS...C05....0H.
- 1 2 Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Bibcode:1986EgUBV........0M.
- ↑ Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065.
- ↑ Cardini, D. (January 2005), "Mg II chromospheric radiative loss rates in cool active and quiet stars", Astronomy and Astrophysics, 430: 303–311, arXiv:astro-ph/0409683, Bibcode:2005A&A...430..303C, doi:10.1051/0004-6361:20041440.
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