Abstract

We report the discovery of WASP-13b, a low-mass Mp=0.46−0.05+0.06MJ M_p = 0.46 ^{+ 0.06}_{- 0.05} M_J transiting exoplanet with an orbital period of 4.35298±0.000044.35298 \pm 0.00004 days. The transit has a depth of 9 mmag, and although our follow-up photometry does not allow us to constrain the impact parameter well (0<b<0.460 < b < 0.46), with radius in the range Rp∼1.06−1.21RJR_p \sim 1.06 - 1.21 R_J the location of WASP-13b in the mass-radius plane is nevertheless consistent with H/He-dominated, irradiated, low core mass and core-free theoretical models. The G1V host star is similar to the Sun in mass (M∗=1.03−0.09+0.11M⊙_{*} = 1.03^{+0.11}_ {- 0.09} M_{\odot}) and metallicity ([M/H]=0.0±0.20.0\pm0.2), but is possibly older (8.5−4.9+5.58.5^{+ 5.5}_{- 4.9} Gyr).

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