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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-B1 0487.0799749), from which we derive the mass, radius and density of the planet: MP = 1.58(-0.08)(+0.13) M-J, R-P = 1.090(-0.058)(+0.094) R-J and rho P = 1.22(-0.24)(+0.19) rho J. The orbital period is P = 1.6284296(-0.0000037)(+0.0000048) d and the mid-transit epoch is T-C (HJD) = 245 4375.62466(-0.00025)(+0.00026).
Original language | English |
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Pages (from-to) | L4-L7 |
Number of pages | 4 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 387 |
Issue number | 1 |
Early online date | 3 Apr 2008 |
DOIs | |
Publication status | Published - 11 Jun 2008 |
Keywords
- stars: individual: WASP-5
- planetary systems
- LIGHT CURVES
- ATMOSPHERE
- PLANET
- MASS
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Dive into the research topics of 'WASP-5b: a dense, very hot Jupiter transiting a 12th-mag Southern-hemisphere star'. Together they form a unique fingerprint.Projects
- 2 Finished
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Wide Area Search for Planets: Project support for the Wide Area Search for Planets
Cameron, A. C. (PI)
Science & Technology Facilities Council
1/08/08 → 31/07/11
Project: Standard
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Astrophysics at St Andrews: Astrophysics at St.Andrews
Cameron, A. C. (PI) & Horne, K. D. (CoI)
1/04/06 → 31/03/11
Project: Standard