WASP-25b: a 0.6 MJ planet in the Southern hemisphere

Enoch, B. ; Cameron, A. Collier ; Anderson, D. R. ; Lister, T. A. ; Hellier, C. ; Maxted, P. F. L. ; Queloz, D. ; Smalley, B. ; Triaud, A. H. M. J. ; West, R. G. ; Brown, D. J. A. ; Gillon, M. ; Hebb, L. ; Lendl, M. ; Parley, N. ; Pepe, F. ; Pollacco, D. ; Segransan, D. ; Simpson, E. ; Street, R. A. ; Udry, S.

In: Monthly Notices of the Royal Astronomical Society, 2011, vol. 410, no. 3, p. 1631-1636

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    Summary
    We report the detection of a 0.6 MJ extrasolar planet by WASP-South, WASP-25b, transiting its solar-type host star every 3.76 d. A simultaneous analysis of the WASP, FTS and Euler photometry and CORALIE spectroscopy yields a planet of Rp= 1.22 RJ and Mp= 0.58 MJ around a slightly metal-poor solar-type host star, [Fe/H]=− 0.05 ± 0.10, of R*= 0.92 R⊙ and M*= 1.00 M⊙. WASP-25b is found to have a density of ρp= 0.32 ρJ, a low value for a sub-Jupiter mass planet. We investigate the relationship of planetary radius to planetary equilibrium temperature and host star metallicity for transiting exoplanets with a similar mass to WASP-25b, finding that these two parameters explain the radii of most low-mass planets well