Formation & Evolution of Close-in Exoplanets

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• Hilke Schlichting
• Wednesday 31 October 2018, 13:15-14:15
• Sackler Lecture Theatre, IoA.

If you have a question about this talk, please contact Dr Giovanni Rosotti.

Exoplanets with radii between 1-4 Earth radii are the most abundant planets known to date and regularly appear in tightly-packed multiple-planet systems. A significant fraction of them are enshrouded in gaseous envelopes that are massive enough to significantly contribute to the planet’s radius. I will review current planet formation theories and present a simple analytical prescription, accounting self-consistently for gas accretion, cooling and mass-loss of super-earths. I will demonstrate that the luminosity of the cooling rocky core, can erode light envelopes while preserving heavy ones resulting in a valley in the radius distribution of small exoplanets even in the absence of any photo-evaporation. I will conclude with a comparison of observations and theoretical predictions, highlighting that even super-Earths that appear as barren rocky cores today likely formed with primordial hydrogen and helium envelopes and discuss the signature of giant impacts in close-in exoplanet systems.

This talk is part of the Institute of Astronomy Seminars series.

This talk is included in these lists:

• Cambridge Astronomy Talks
• Combined External Astrophysics Talks DAMTP
• Cosmology lists
• Cosmology, Astrophysics and General Relativity
• Institute of Astronomy Seminars
• Institute of Astronomy Talk Lists
• Kavli Institute for Cosmology Talk Lists
• Priscilla
• Sackler Lecture Theatre, IoA

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