WASP-12 is a magnitude 11 yellow dwarf star located approximately 1347 light-years away in the constellation Auriga. WASP-12 has a mass and radius similar to the Sun and is known for being orbited by a planet that is extremely hot and has a retrograde orbit around WASP-12. WASP-12 forms a triple star system with two red dwarf companions. Both of them have spectral types of M3V and are only 38% and 37% as massive as the Sun, respectively.
WASP-12b.
WASP-12b.
Artist's conception of WASP-12 & WASP-12b
WASP-12b is a hot Jupiter orbiting the star WASP-12, discovered in April of 2008, by the SuperWASP planetary transit survey. The planet takes only a little over one Earth day to orbit its star, in contrast to about 365.25 days for the Earth to orbit the Sun. Its distance from the star is only the Earth's distance from the Sun, with an eccentricity the same as Jupiter's. Consequently, it has one of the lowest densities for exoplanets. On December 3, 2013, scientists working with the Hubble Space Telescope (HST) reported detecting water in the atmosphere of the exoplanet. In July 2014, NASA announced finding very dry atmospheres on three exoplanets orbiting sun-like stars.
Artist's depiction of WASP-12b's atmosphere being tidally stripped by its parent star
WASP-12b and its host star, WASP-12 (artist conception).
Hot, carbon-rich planet WASP-12b and its host star. (Exoplanet color was unknown at the time of this artist conception).
WASP-12b and its host star, WASP-12 − with IR spectra noting the presence of various chemical molecules.