The Evolution and Compositions of Kepler's Sub-Neptunes and Super-Earths
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If you have a question about this talk, please contact Dr B.-O. Demory.
NASA ’s Kepler mission has discovered a large new population of super-Earth and sub-Neptune sized planets. Understanding these planets poses a fundamental test for models of planet formation and evolution. I will discuss the possible origins and compositions of these planets and the constraints that can be provided by models of planet structure and evolution. I will examine the transition between rocky super-Earths and gaseous sub-Neptunes, the possible compositions of the sub-Neptunes, and the role that atmospheric photo-evaporation plays in sculpting these populations.
This talk is part of the Exoplanet Seminars series.
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