Abstract
We report the detection of a 0.6 M$_J$ 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 R$_p$= 1.22 R$_J$ and M$_p$= 0.58 M$_J$ around a slightly metal-poor solar-type host star, [Fe/H]=- 0.05 plusmn 0.10, of R$_*$= 0.92 R$_⊙$ and M$_*$= 1.00 M$_⊙$. WASP-25b is found to have a density of $$_p$= 0.32 $$_J$, 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.
Original language | English |
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Pages (from-to) | 1631-1636 |
Number of pages | 6 |
Journal | Royal Astronomical Society. Monthly Notices |
Volume | 410 |
DOIs | |
Publication status | Published - 1 Jan 2011 |
Keywords
- planetary systems