Omicron Pegasi
Appearance
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Pegasus |
Right ascension | 22h 41m 45.40961s[1] |
Declination | +29° 18′ 27.4918″[1] |
Apparent magnitude (V) | +4.79[2] |
Characteristics | |
Spectral type | A1 IV[3] |
U−B color index | +0.035[4] |
B−V color index | -0.015[4] |
Astrometry | |
Radial velocity (Rv) | +8.50 ± 0.1 km/s |
Proper motion (μ) | RA: -0.06 ± 0.42[1] mas/yr Dec.: –21.46 ± 0.49[1] mas/yr |
Parallax (π) | 10.92 ± 0.67 mas[1] |
Distance | 300 ± 20 ly (92 ± 6 pc) |
Absolute magnitude (MV) | -0.01[5] |
Details | |
Surface gravity (log g) | 3.7[3] cgs |
Temperature | 9,600[3] K |
Metallicity [Fe/H] | 0.0[3] dex |
Rotational velocity (v sin i) | 6.0±0.2[3] km/s |
Other designations | |
Database references | |
SIMBAD | data |
Omicron Pegasi (ο Peg) is a star in the constellation Pegasus. Its apparent magnitude is 4.79. Located 300 ± 20 light-years distant,[1] it is a white subgiant of spectral class A1IV, which has begun to cool, expand and brighten off the main sequence.[5]
References
- ^ a b c d e f van Leeuwen, F. (November 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
- ^ a b SIMBAD, Omicron Pegasi (accessed 12 January 2013)
- ^ a b c d e Gray, David F. (April 2014), "Precise Rotation Rates for Five Slowly Rotating a Stars", The Astronomical Journal, 147 (4): 13, Bibcode:2014AJ....147...81G, doi:10.1088/0004-6256/147/4/81, 81
- ^ a b Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV data. Bibcode:1986EgUBV........0M.
- ^ a b Gray, David F. (2014). "Precise Rotation Rates for Five Slowly Rotating a Stars". The Astronomical Journal. 147 (4): 13. Bibcode:2014AJ....147...81G. doi:10.1088/0004-6256/147/4/81. 81.