A Precise Estimate of the Radius of HD 149026b

Abstract

We present Spitzer 8 μm transit observations of the extrasolar planet system HD 149026b. At this wavelength, transit light curves are weakly affected by stellar limb-darkening, allowing for a simpler and more accurate determination of planetary parameters. We measure a planet-star radius ratio of R_p/R∗=0.05158±0.00077, and in combination with ground-based data and independent constraints on the stellar mass and radius, we derive an orbital inclination of i = 85°.4^(+0°.9)_(−0°.8) and a planet radius of 0.755 ± 0.040 R_J. These measurements further support models in which the planet is greatly enriched in heavy elements.

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