WASP-25 is a G-type main-sequence star about 701 light-years away in the constellation of Hydra.
Star characteristics WASP-25 is slightly metal-poor (85% of Solar amount) and is probably a young star which has just entered the main sequence.
Planetary system The hot Jupiter class planet WASP-25b was discovered around WASP-25 in 2010. The planet would have an equilibrium temperature of 1212±35 K. A Rossiter-McLaughlin effect based study in 2011 found a modest misalignment of the planetary orbit to the rotational axis of the parent star, equal to 14.6±6.7 degrees. A habitability study in 2018 found WASP-25b does not adversely affect the stability of planetary orbits in the habitable zone of WASP-25.
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