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WASP-135b: a highly irradiated, inflated hot Jupiter orbiting a G5V star

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.

preprint2015arXivOpen access
Jessica J. SpakeDavid J. A. BrownAmanda P. DoyleGuillaume HébrardJames McCormacDavid J. ArmstrongDon PollaccoYilen Gómez Maqueo ChewDavid R. AndersonSusana C. C. BarrosFrançois BouchyPanayotis BoumisGiovanni BrunoAndrew Collier CameronBastien CourcolGuy R. DaviesFrancesca FaediCoel HellierJames KirkKristine W. F. LamAlexios LiakosTom LoudenPierre F. L. MaxtedHugh P. OsbornEnric PalleJorge Prieto ArranzStéphane UdrySimon R. WalkerRichard G. WestPeter J. Wheatley
astro-ph.EP
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Open access30 authors1 topic
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Jessica J. SpakeDavid J. A. BrownAmanda P. DoyleGuillaume HébrardJames McCormacDavid J. ArmstrongDon PollaccoYilen Gómez Maqueo ChewDavid R. AndersonSusana C. C. BarrosFrançois BouchyPanayotis BoumisGiovanni BrunoAndrew Collier CameronBastien CourcolGuy R. DaviesFrancesca FaediCoel HellierJames KirkKristine W. F. LamAlexios LiakosTom LoudenPierre F. L. MaxtedHugh P. OsbornEnric PalleJorge Prieto ArranzStéphane UdrySimon R. WalkerRichard G. WestPeter J. Wheatley

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