WASP-5b: A dense, very hot Jupiter transiting a 12th-mag Southern-hemisphere star

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Abstract

We report the discovery of WASP-5b, a Jupiter-mass planet orbiting a 12th-mag G-type star in the Southern hemisphere. The 1.6-d orbital period places WASP-5b in the class of very hot Jupiters and leads to a predicted equilibrium temperature of 1750 K. WASP-5b is the densest of any known Jovian-mass planet, being a factor of 7 denser than TrES-4, which is subject to similar stellar insolation, and a factor of 3 denser than WASP-4b, which has a similar orbital period. We present transit photometry and radial velocity measurements of WASP-5 ( = USNO-B10487-0799749), from which we derive the mass, radius and density of the planet: MP = l.58+0.13-0.08 MJ, RP = l.090+0.094-0.058 RJ and ρP = 1.22+0.19-0.24 ρJ The orbital period is P = 1.6284296+0.0000048-0.0000037 d and the mid-transit epoch is TC (HJD) = 2454375.62466+0.00026-0.00025. © 2008 The Authors. Journal compilation © 2008 RAS.

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Anderson, D. R., Gillon, M., Hellier, C., Maxted, P. F. L., Pepe, F., Queloz, D., … Wheatley, P. J. (2008, June). WASP-5b: A dense, very hot Jupiter transiting a 12th-mag Southern-hemisphere star. Monthly Notices of the Royal Astronomical Society: Letters. https://doi.org/10.1111/j.1745-3933.2008.00465.x

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