Understanding Planet Formation by Studying the Evolution of Hot Neptunes and Super-Earths

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• Eric Lopez (Edinburgh)
• Wednesday 25 January 2017, 16:00-17:00
• Martin Ryle Seminar Room, Kavli Institute.

If you have a question about this talk, please contact Ed Gillen.

One of the most significant advances by NASA ’s Kepler Mission was the discovery of an abundant new population of highly irradiated planets with sizes between that of the Earth and Neptune, unlike anything found in our Solar System. Understanding these populations poses a fundamental test for models of planet formation and evolution, with important implications for habitability and the frequency of Earth-like planets. Using models of planet evolution and atmospheric evaporation, I will discuss two recent papers that shed light on the compositions and possible origins of these new populations. In particular, I will show that the most highly irradiated planets likely formed without large amounts of material from beyond the snowlike and that the period dependence of the transition between rocky and non-rocky planets can be used to constrain the origin of rocky exoplanets in general.

This talk is part of the Exoplanet Seminars series.

This talk is included in these lists:

• Combined External Astrophysics Talks DAMTP
• Cosmology, Astrophysics and General Relativity
• Exoplanet Seminars
• Institute of Astronomy Talk Lists
• LCLU Departmental Talks
• Martin Ryle Seminar Room, Kavli Institute

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