Theory of Exoplanet Atmospheres and Radii

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Direct measurements of the radii and masses of giant exoplanets, and
indirect measurements of their temperatures, temperature profiles, and
compositions have inaugurated the era of the remote sensing and
characterization of planets beyond the solar system. Theoretical
interpretation both of these atmospheres and of their mass-radius
relationship has been challenging, but much progress has been made. I
will summarize the general theory of the atmospheres and structures of
giant exoplanets, focussing on what can and has been gleaned from
secondary and primary transit data using state-of-the-art spectral,
atmosphere, and structural theory. The issues concerning the radii,
spectra, and light curves of strongly irradiated exoplanets will be
explored and paths forward in the theoretical interpretation and
understanding of these fascinating objects will be discussed.

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