WASP-135b: A Highly Irradiated, Inflated Hot Jupiter Orbiting a G5V Star

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Authors

  • J. J. Spake
  • D. J. A. Brown
  • A. P. Doyle
  • G. Hébrard
  • J. Mccormac
  • D. J. Armstrong
  • D. Pollacco
  • Y. Gómez Maqueo Chew
  • D. R. Anderson
  • S. C. C. Barros
  • F. Bouchy
  • P. Boumis
  • G. Bruno
  • A. Collier Cameron
  • B. Courcol
  • F. Faedi
  • C. Hellier
  • J. Kirk
  • K. W. F. Lam
  • A. Liakos
  • T. Louden
  • P. F. L. Maxted
  • H. P. Osborn
  • E. Palle
  • J. Prieto Arranz
  • S. Udry
  • S. R. Walker
  • R. G. West
  • P. J. Wheatley

Colleges, School and Institutes

Abstract

We report the discovery of a new transiting planet from the WASP survey. WASP-135b is a hot Jupiter with radius 1.30 ± 0.09 R Jup, mass 1.90 ± 0.08 M Jup, 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 ± 0.06 M ☉ and 0.96 ± 0.05 R ☉, respectively. The proximity of the planet to its star means that WASP-135b receives high levels of insolation, which may be the cause of its inflated radius. Additionally, we report weak evidence of a transfer of angular momentum from the planet to its host star.

Details

Original languageEnglish
Article number024401
JournalPublications of the Astronomical Society of the Pacific
Volume128
Issue number960
Publication statusPublished - 1 Feb 2016