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arXiv · 0804.4475

The Transit Light Curve Project. IX. Evidence for a Smaller Radius of the Exoplanet XO-3b

Joshua N. Winn·Matthew J. Holman·Guillermo Torres·Peter McCullough·Christopher M. Johns-Krull·David W. Latham·Avi Shporer·Tsevi Mazeh·Enrique Garcia-Melendo·Cindy Foote·Gil Esquerdo·Mark Everett
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Abstract

We present photometry of 13 transits of XO-3b, a massive transiting planet on an eccentric orbit. Previous data led to two inconsistent estimates of the planetary radius. Our data strongly favor the smaller radius, with increased precision: R_p = 1.217 +/- 0.073 R_Jup. A conflict remains between the mean stellar density determined from the light curve, and the stellar surface gravity determined from the shapes of spectral lines. We argue the light curve should take precedence, and revise the system parameters accordingly. The planetary radius is about 1 sigma larger than the theoretical radius for a hydrogen-helium planet of the given mass and insolation. To help in planning future observations, we provide refined transit and occultation ephemerides.

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Joshua N. Winn, Matthew J. Holman, Guillermo Torres, Peter McCullough, Christopher M. Johns-Krull, David W. Latham, Avi Shporer, Tsevi Mazeh, Enrique Garcia-Melendo, Cindy Foote, Gil Esquerdo, Mark Everett. 2008-04-28. The Transit Light Curve Project. IX. Evidence for a Smaller Radius of the Exoplanet XO-3b. https://doi.org/10.1086/589737

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