Omicron Leonis
Omicron Leonis is located to the lower far right on this map of the constellation. | |
Observation data Epoch J2000.0 Equinox J2000.0 | |
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Constellation | Leo |
Right ascension | 09h 41m 09.03s |
Declination | +09° 53' 32.30" |
Apparent magnitude (V) | +3.52[1] |
Characteristics | |
Spectral type | F8-G0III/A7m[2] |
U−B color index | 0.21[1] |
B−V color index | 0.49[1] |
Astrometry | |
Proper motion (μ) | RA: -143.20[3] mas/yr Dec.: -37.20[3] mas/yr |
Parallax (π) | 25.03[3] ± 0.22 mas |
Distance | 135 ly (41.4±0.1[4] pc) |
Orbit[4] | |
Period (P) | 14.498064 ± 0.000009 days |
Semi-major axis (a) | 4.46 ± 0.01 mas |
Eccentricity (e) | 0 |
Inclination (i) | 57.6 ± 0.1° |
Longitude of the node (Ω) | 191.4 ± 0.1° |
Periastron epoch (T) | TJD 10629.831 ± 0.003 |
Details | |
Mass | 2.12/1.87 ± 0.01[4] M☉ |
Radius | 5.9±0.5/2.2±0.3[4] R☉ |
Luminosity | 39.4±2.4/15.4±1.0 [4] L☉ |
Temperature | 6,000±200/7,600±400[4] K |
Age | 8 × 108(estimate)[4] years |
Other designations | |
14 Leo, HR 3852, BD+10 2044, HD 83808/83809, SAO 98709, FK5 365, HIP 47508. | |
Database references | |
SIMBAD | data |
Omicron Leonis (ο Leo, ο Leonis), known also by its traditional name, Subra, is a binary star in the constellation of Leo, west of Regulus, some 130 light years from here, where it marks one of the lion's forepaws.
The two stars of Omicron Leonis (Subra-A and Subra-B) are given as type F8-G0III giant for the primary and A7m dwarf for the secondary.[4] Their combined apparent magnitude is +3.52.
References
- ↑ 1.0 1.1 1.2 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: 0. Bibcode:2002yCat.2237....0D.
- ↑ Ginestet, N.; Carquillat, J. M. (2002). "Spectral Classification of the Hot Components of a Large Sample of Stars with Composite Spectra, and Implication for the Absolute Magnitudes of the Cool Supergiant Components". The Astrophysical Journal Supplement Series 143 (2): 513. Bibcode:2002ApJS..143..513G. doi:10.1086/342942.
- ↑ 3.0 3.1 3.2 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.
- ↑ 4.0 4.1 4.2 4.3 4.4 4.5 4.6 4.7 Hummel, C. A.; Carquillat, J. -M.; Ginestet, N.; Griffin, R. F.; Boden, A. F.; Hajian, A. R.; Mozurkewich, D.; Nordgren, T. E. (2001). "Orbital and Stellar Parameters of Omicron Leonis from Spectroscopy and Interferometry". The Astronomical Journal 121 (3): 1623. doi:10.1086/319391.
External links
- Omicron Leo/Subra in Kaler Stars
- Subra (HIP 47508) Relates to the A star, Subra-B
- Subra - Omi Leonis brief data.
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