An optical transmission spectrum of the giant planet WASP-36 b
Mancini et al
We present broad-band photometry of five transits in the planetary system WASP-36, totaling 17 high-precision light curves. Four of the transits were simultaneously observed in four passbands (g, r, i, z), using the telescope-defocussing technique, and achieving scatters of less than 1 mmag per observation. We used these data to improve the measured orbital and physical properties of the system, and obtain an optical transmission spectrum of the planet. We measured a decreasing radius from bluer to redder passbands with a confidence level of more than 5 sigma. The radius variation is roughly 11 pressure scale heights between the g and the z bands. This is too strong to be Rayleigh scattering in the planetary atmosphere, and implies the presence of a species which absorbs strongly at bluer wavelengths.
Thursday, June 23, 2016
Hot Jupiter WASP-36b has Something in its Atmosphere Bluer Light
Posted by Will Baird at 4:00 PM
Labels: gas giants, giant planets, hot jupiters, optical spectra, photometry, WASP-36b
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