S Pegasi
S Pegasi (S Peg) is a Mira variable star in the constellation Pegasus. It varies between magnitude 7 and 13 with a period of 319.22 days.[2] It is believed to be pulsating in the first overtone. First overtone pulsators have masses less than 1.8 M☉ at a temperature of 2,107 K, and less than 1.4 M☉ at the luminosity of S Pegasi.[4]
| Observation data Epoch 2000 Equinox 2000 | |
|---|---|
| Constellation | Pegasus |
| Right ascension | 23h 20m 32.61407s[1] |
| Declination | +08° 55′ 08.1398″[1] |
| Apparent magnitude (V) | 6.9 - 13.8[2] |
| Characteristics | |
| Spectral type | M5e - M8.5e[2] |
| Variable type | Mira[2] |
| Astrometry | |
| Parallax (π) | 2.52 ± 2.26[1] mas |
| Distance | approx. 1,000 ly (approx. 400 pc) |
| Details | |
| Radius | 459 - 574[3] R☉ |
| Luminosity | 3,221[4] L☉ |
| Temperature | 2,107[4] K |
| Other designations | |
| Database references | |
| SIMBAD | data |
References
- Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
- 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.
- Van Belle, G. T.; Thompson, R. R.; Creech-Eakman, M. J. (2002). "Angular Size Measurements of Mira Variable Stars at 2.2 Microns. II". The Astronomical Journal. 124 (3): 1706. arXiv:astro-ph/0210167. Bibcode:2002AJ....124.1706V. doi:10.1086/342282.
- Serkowski, Krzysztof; Shawl, Stephen J. (2001). "Polarimetry of 167 Cool Variable Stars: Data". The Astronomical Journal. 122 (4): 2017. Bibcode:2001AJ....122.2017S. doi:10.1086/323105.
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