WASP-12b: the hottest transiting extrasolar planet yet discovered
. (2009) WASP-12b: the hottest transiting extrasolar planet yet discovered. Astrophysical Journal, Vol.693 (No.2). pp. 1920-1928. ISSN 0004-637X Full text not available from this repository.
Official URL: http://dx.doi.org/10.1088/0004-637X/693/2/1920
We report on the discovery of WASP-12b, a new transiting extrasolar planet with R-pl = 1.79(-0.09)(+0.09) R-J and M-pl = 1.41(-0.01)(+0.01) M-J. The planet and host star properties were derived from a Monte Carlo Markov chain analysis of the transit photometry and radial velocity data. Furthermore, by comparing the stellar spectrum with theoretical spectra and stellar evolution models, we determined that the host star is a supersolar metallicity ([M/II]= 0.3(-0.15)(+0.15)), late-F (T-eff = 6300(-100)(+200) K) star which is evolving off the zero-age main sequence. The planet has an equilibrium temperature of T-eq = 2516 K caused by its very short period orbit (P = 1.09 days) around the hot, twelfth magnitude host star. WASP-12b has the largest radius of any transiting planet yet detected. It is also the most heavily irradiated and the shortest period planet in the literature.
|Item Type:||Journal Article|
|Subjects:||Q Science > QB Astronomy|
|Divisions:||Faculty of Science > Physics|
|Journal or Publication Title:||Astrophysical Journal|
|Official Date:||10 March 2009|
|Number of Pages:||9|
|Page Range:||pp. 1920-1928|
|Access rights to Published version:||Restricted or Subscription Access|
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