Predictions, Observations, and Trends of Exoplanetary Atmospheres

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Scientific paper

The Spitzer Space Telescope has measured numerous eclipses of exoplanets. These measurements give the planetary flux in the observation filter. In combination with the planetary radius, known from transit, one can determine a brightness temperature, Tb. We compare these Tbs with the planets' predicted equilibrium temperatures, Teq, calculated assuming zero albedo and uniform reradiation of absorbed energy from the entire planetary surface. Measurements deviate from the simplistic Teq prediction because of the composition and thermal profiles present in the atmosphere, but other effects may play important roles as well. We present comparisons of these fundamental observations to both the Teq prediction and to other properties of the planets or their stars.

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