  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.
