WASP-135b: a highly irradiated, inflated hot Jupiter orbiting a G5V star
Authors:
Spake et al
Abstract:
We report the discovery of a new transiting planet from the WASP survey. WASP-135b is a hot Jupiter with a radius of 1.30 pm 0.09 Rjup, a mass of 1.90 pm 0.08 Mjup and an orbital period of 1.401 days. Its host is a Sun-like star, with a G5 spectral type and a mass and radius of 0.98 pm 0.06 Msun and 0.96 pm 0.05 Rsun respectively. The proximity of the planet to its host means that WASP-135b receives high levels of insolation, which may be the cause of its inflated radius. Additionally, we find weak evidence of a transfer of angular momentum from the planet to its star.
Thursday, January 14, 2016
WASP-135b: an Inflated hot Jupiter in a 1.4 day Orbit Around a G5 Dwarf Star
Labels:
gas giants,
giant planets,
hot jupiters,
inflated exoplanets,
wasp-135b
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