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

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; Guy Davies; F. Faedi; C. Hellier; 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; James Kirk

doi:10.1088/1538-3873/128/960/024401

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

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
, Guy Davies
, F. Faedi
, C. Hellier
, 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, James Kirk

Research output: Contribution to journal › Article › peer-review

6 Citations (Scopus)

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.

Original language	English
Article number	024401
Journal	Publications of the Astronomical Society of the Pacific
Volume	128
Issue number	960
DOIs	https://doi.org/10.1088/1538-3873/128/960/024401
Publication status	Published - 1 Feb 2016

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Spake, J. J., Brown, D. J. A., Doyle, A. P., Hébrard, G., Mccormac, J., Armstrong, D. J., Pollacco, D., Chew, Y. G. M., Anderson, D. R., Barros, S. C. C., Bouchy, F., Boumis, P., Bruno, G., Cameron, A. C., Courcol, B., Davies, G., Faedi, F., Hellier, C., Lam, K. W. F., ... Kirk, J. (2016). WASP-135b: A Highly Irradiated, Inflated Hot Jupiter Orbiting a G5V Star. Publications of the Astronomical Society of the Pacific, 128(960), Article 024401. https://doi.org/10.1088/1538-3873/128/960/024401

@article{367076807ac0447a9c455f3e7236ae6f,

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

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.",

author = "Spake, \{J. J.\} and Brown, \{D. J. A.\} and Doyle, \{A. P.\} and G. H{\'e}brard and J. Mccormac and Armstrong, \{D. J.\} and D. Pollacco and Chew, \{Y. G{\'o}mez Maqueo\} and Anderson, \{D. R.\} and Barros, \{S. C. C.\} and F. Bouchy and P. Boumis and G. Bruno and Cameron, \{A. Collier\} and B. Courcol and Guy Davies and F. Faedi and C. Hellier and Lam, \{K. W. F.\} and A. Liakos and T. Louden and Maxted, \{P. F. L.\} and Osborn, \{H. P.\} and E. Palle and Arranz, \{J. Prieto\} and S. Udry and Walker, \{S. R.\} and West, \{R. G.\} and Wheatley, \{P. J.\} and James Kirk",

year = "2016",

month = feb,

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doi = "10.1088/1538-3873/128/960/024401",

language = "English",

volume = "128",

journal = "Publications of the Astronomical Society of the Pacific",

issn = "0004-6280",

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Spake, JJ, Brown, DJA, Doyle, AP, Hébrard, G, Mccormac, J, Armstrong, DJ, Pollacco, D, Chew, YGM, Anderson, DR, Barros, SCC, Bouchy, F, Boumis, P, Bruno, G, Cameron, AC, Courcol, B, Davies, G, Faedi, F, Hellier, C, Lam, KWF, Liakos, A, Louden, T, Maxted, PFL, Osborn, HP, Palle, E, Arranz, JP, Udry, S, Walker, SR, West, RG, Wheatley, PJ & Kirk, J 2016, 'WASP-135b: A Highly Irradiated, Inflated Hot Jupiter Orbiting a G5V Star', Publications of the Astronomical Society of the Pacific, vol. 128, no. 960, 024401. https://doi.org/10.1088/1538-3873/128/960/024401

TY - JOUR

T1 - WASP-135b: A Highly Irradiated, Inflated Hot Jupiter Orbiting a G5V Star

AU - Spake, J. J.

AU - Brown, D. J. A.

AU - Doyle, A. P.

AU - Hébrard, G.

AU - Mccormac, J.

AU - Armstrong, D. J.

AU - Pollacco, D.

AU - Chew, Y. Gómez Maqueo

AU - Anderson, D. R.

AU - Barros, S. C. C.

AU - Bouchy, F.

AU - Boumis, P.

AU - Bruno, G.

AU - Cameron, A. Collier

AU - Courcol, B.

AU - Davies, Guy

AU - Faedi, F.

AU - Hellier, C.

AU - Lam, K. W. F.

AU - Liakos, A.

AU - Louden, T.

AU - Maxted, P. F. L.

AU - Osborn, H. P.

AU - Palle, E.

AU - Arranz, J. Prieto

AU - Udry, S.

AU - Walker, S. R.

AU - West, R. G.

AU - Wheatley, P. J.

AU - Kirk, James

PY - 2016/2/1

Y1 - 2016/2/1

N2 - 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.

AB - 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.

U2 - 10.1088/1538-3873/128/960/024401

DO - 10.1088/1538-3873/128/960/024401

M3 - Article

SN - 0004-6280

VL - 128

JO - Publications of the Astronomical Society of the Pacific

JF - Publications of the Astronomical Society of the Pacific

IS - 960

M1 - 024401

ER -

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

Abstract

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