Upsilon1 Centauri
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Centaurus |
Right ascension | 13h 58m 40.75s[1] |
Declination | −44° 48′ 12.9″[1] |
Apparent magnitude (V) | +3.788[2] |
Characteristics | |
Spectral type | B2 IV/V[2] |
U−B color index | −0.80 |
B−V color index | −0.20 |
Astrometry | |
Radial velocity (Rv) | +5 km/s |
Proper motion (μ) | RA: ±0.15 −27.51[1] mas/yr Dec.: ±0.13 −22.44[1] mas/yr |
Parallax (π) | 7.63 ± 0.16[1] mas |
Distance | 427 ± 9 ly (131 ± 3 pc) |
Absolute magnitude (MV) | −1.72[2] |
Details | |
Radius | 3.74 ± 0.34[3] R☉ |
Luminosity | 1,884[2] L☉ |
Surface gravity (log g) | 4.15 ± 0.07[3] cgs |
Temperature | 21,411 ± 377[3] K |
Other designations | |
Database references | |
SIMBAD | data |
Upsilon1 Centauri, Latinized from υ1 Centauri, is the Bayer designation for a star in the constellation Centaurus.
υ1 Centauri is a blue-white B-type subgiant with an apparent magnitude of +3.87. It is approximately 427 light years from Earth.
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 3 4 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.
- 1 2 3 Fitzpatrick, E. L.; Massa, D. (March 2005), "Determining the Physical Properties of the B Stars. II. Calibration of Synthetic Photometry", The Astronomical Journal, 129 (3): 1642–1662, arXiv:astro-ph/0412542, Bibcode:2005AJ....129.1642F, doi:10.1086/427855
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