S Pegasi (S Peg) is a Mira variable star in the constellation Pegasus located about 2,300 light-years away. It varies between apparent magnitude 6.9 and 13.8 with a period of 319 days (10 months), representing a nearly 600–fold change in brightness. S Pegasi enters solar conjunction and is hidden by the Sun's glare each year from late February through late March. It reaches opposition in mid-September, when it is visible all night. 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.
References
External links S Peg lightcurve at AAVSO


