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 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☉, respe...
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| Veröffentlicht in: | Publications of the Astronomical Society of the Pacific 2016-02, Vol.128 (960), p.24401 |
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| creator | Spake, J. J. Brown, D. J. A. Doyle, A. P. Hébrard, G. McCormac, J. Armstrong, D. J. Pollacco, D. Chew, Y. Gómez Maqueo Anderson, D. R. Barros, S. C. C. Bouchy, F. Boumis, P. Bruno, G. Cameron, A. Collier Courcol, B. Davies, G. R. Faedi, F. Hellier, C. Kirk, J. Lam, K. W. F. Liakos, A. Louden, T. Maxted, P. F. L. Osborn, H. P. Palle, E. Arranz, J. Prieto Udry, S. Walker, S. R. West, R. G. Wheatley, P. J. |
| description | 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. |
| doi_str_mv | 10.1088/1538-3873/128/960/024401 |
| format | Article |
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J. ; Brown, D. J. A. ; Doyle, A. P. ; Hébrard, G. ; McCormac, J. ; Armstrong, D. J. ; Pollacco, D. ; Chew, Y. Gómez Maqueo ; Anderson, D. R. ; Barros, S. C. C. ; Bouchy, F. ; Boumis, P. ; Bruno, G. ; Cameron, A. Collier ; Courcol, B. ; Davies, G. R. ; Faedi, F. ; Hellier, C. ; Kirk, J. ; Lam, K. W. F. ; Liakos, A. ; Louden, T. ; Maxted, P. F. L. ; Osborn, H. P. ; Palle, E. ; Arranz, J. Prieto ; Udry, S. ; Walker, S. R. ; West, R. G. ; Wheatley, P. J.</creator><creatorcontrib>Spake, J. J. ; Brown, D. J. A. ; Doyle, A. P. ; Hébrard, G. ; McCormac, J. ; Armstrong, D. J. ; Pollacco, D. ; Chew, Y. Gómez Maqueo ; Anderson, D. R. ; Barros, S. C. C. ; Bouchy, F. ; Boumis, P. ; Bruno, G. ; Cameron, A. Collier ; Courcol, B. ; Davies, G. R. ; Faedi, F. ; Hellier, C. ; Kirk, J. ; Lam, K. W. F. ; Liakos, A. ; Louden, T. ; Maxted, P. F. L. ; Osborn, H. P. ; Palle, E. ; Arranz, J. Prieto ; Udry, S. ; Walker, S. R. ; West, R. G. ; Wheatley, P. J.</creatorcontrib><description>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.</description><identifier>ISSN: 0004-6280</identifier><identifier>EISSN: 1538-3873</identifier><identifier>DOI: 10.1088/1538-3873/128/960/024401</identifier><language>eng</language><publisher>The Astronomical Society of the Pacific</publisher><subject>Astrophysics ; Physics ; planets and satellites: detection ; stars: individual (WASP-135) ; techniques: photometric ; techniques: radial velocities</subject><ispartof>Publications of the Astronomical Society of the Pacific, 2016-02, Vol.128 (960), p.24401</ispartof><rights>2016. The Astronomical Society of the Pacific. 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A.</creatorcontrib><creatorcontrib>Doyle, A. P.</creatorcontrib><creatorcontrib>Hébrard, G.</creatorcontrib><creatorcontrib>McCormac, J.</creatorcontrib><creatorcontrib>Armstrong, D. J.</creatorcontrib><creatorcontrib>Pollacco, D.</creatorcontrib><creatorcontrib>Chew, Y. Gómez Maqueo</creatorcontrib><creatorcontrib>Anderson, D. R.</creatorcontrib><creatorcontrib>Barros, S. C. C.</creatorcontrib><creatorcontrib>Bouchy, F.</creatorcontrib><creatorcontrib>Boumis, P.</creatorcontrib><creatorcontrib>Bruno, G.</creatorcontrib><creatorcontrib>Cameron, A. Collier</creatorcontrib><creatorcontrib>Courcol, B.</creatorcontrib><creatorcontrib>Davies, G. R.</creatorcontrib><creatorcontrib>Faedi, F.</creatorcontrib><creatorcontrib>Hellier, C.</creatorcontrib><creatorcontrib>Kirk, J.</creatorcontrib><creatorcontrib>Lam, K. W. F.</creatorcontrib><creatorcontrib>Liakos, A.</creatorcontrib><creatorcontrib>Louden, T.</creatorcontrib><creatorcontrib>Maxted, P. F. L.</creatorcontrib><creatorcontrib>Osborn, H. P.</creatorcontrib><creatorcontrib>Palle, E.</creatorcontrib><creatorcontrib>Arranz, J. Prieto</creatorcontrib><creatorcontrib>Udry, S.</creatorcontrib><creatorcontrib>Walker, S. R.</creatorcontrib><creatorcontrib>West, R. G.</creatorcontrib><creatorcontrib>Wheatley, P. J.</creatorcontrib><title>WASP-135b: A Highly Irradiated, Inflated Hot Jupiter Orbiting a G5V Star</title><title>Publications of the Astronomical Society of the Pacific</title><addtitle>Publ. Astron. Soc. Pac</addtitle><description>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. 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| source | Jstor Complete Legacy; IOP Publishing Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Institute of Physics (IOP) Journals - HEAL-Link; Alma/SFX Local Collection |
| subjects | Astrophysics Physics planets and satellites: detection stars: individual (WASP-135) techniques: photometric techniques: radial velocities |
| title | WASP-135b: A Highly Irradiated, Inflated Hot Jupiter Orbiting a G5V Star |
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