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

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

in Astrophysics / Physics / planets and satellites: detection / stars: individual (WASP-135) / techniques: photometric / techniques: radial velocities

2016

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

in Astrophysics / Physics / planets and satellites: detection / stars: individual (WASP-135) / techniques: photometric / techniques: radial velocities

2016

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

in Astrophysics / Physics / planets and satellites: detection / stars: individual (WASP-135) / techniques: photometric / techniques: radial velocities

2016

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Journal Article

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

Hébrard, G.,

Brown, D. J. A.,

Pollacco, D.,

Bruno, G.,

Walker, S. R.,

Doyle, A. P.,

Armstrong, D. J.,

Spake, J. J.,

Liakos, A.,

Hellier, C.,

Lam, K. W. F.,

Faedi, F.,

Cameron, A. Collier,

West, R. G.,

Davies, G. R.,

Udry, S.,

Barros, S. C. C.,

Boumis, P.,

Maxted, P. F. L.,

Osborn, H. P.,

Chew, Y. Gómez Maqueo,

Louden, T.,

McCormac, J.,

Kirk, J.,

Bouchy, F.,

Courcol, B.,

Palle, E.,

Wheatley, P. J.,

Anderson, D. R.,

Arranz, J. Prieto

2016

Overview

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 RJup, mass 1.90 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 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.

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Publisher

The Astronomical Society of the Pacific,Astronomical Society of the Pacific

Subject

Astrophysics

/ Physics

/ planets and satellites: detection

/ stars: individual (WASP-135)

/ techniques: photometric

/ techniques: radial velocities