HD 129116
This article is about b Centauri. For B Centauri, see B Centauri. For β Centauri, see Beta Centauri.
Observation data Epoch J2000.0 Equinox J2000.0 | |
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Constellation | Centaurus |
Right ascension | 14h 41m 57.59s[1] |
Declination | −37° 47′ 37.6″[1] |
Apparent magnitude (V) | +4.01 |
Characteristics | |
Spectral type | B3V |
U−B color index | −0.70 |
B−V color index | −0.17 |
Variable type | none |
Astrometry | |
Radial velocity (Rv) | +1 km/s |
Proper motion (μ) | RA: -29.92 ± 0.14[1] mas/yr Dec.: -30.68 ± 0.13[1] mas/yr |
Parallax (π) | 9.62 ± 0.18[1] mas |
Distance | 339 ± 6 ly (104 ± 2 pc) |
Absolute magnitude (MV) | −0.84 |
Details | |
Radius | 2.93 ± 0.12[2] R☉ |
Surface gravity (log g) | 4.23 ± 0.03[2] cgs |
Temperature | 18,445 ± 344[2] K |
Other designations | |
Database references | |
SIMBAD | data |
HD 129116, also known by its Bayer designation b Centauri (b Cen), is a star in the constellation Centaurus.
b Centauri is a blue-white B-type main sequence dwarf with an apparent magnitude of +4.01. It is approximately 339 light years from Earth.
References
- ↑ 1.0 1.1 1.2 1.3 1.4 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
- ↑ 2.0 2.1 2.2 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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