Wine and Cheese Spring 2019: Difference between revisions
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=February 4th = | =February 4th = | ||
== James Owen () == | == James Owen (Imperial College) == | ||
'''Understanding the formation and evolution of the Kepler Planets'''<br> | '''Understanding the formation and evolution of the Kepler Planets'''<br> | ||
The observed exoplanet population unveiled by Kepler is billions of years old, distinctly separated in time from the planet formation process that only lasted ~10-100 Myr. I will argue that atmospheric escape has been one of the key evolutionary drivers shaping the exoplanet population we observed today. By understanding how these planet evolve in time, I will show we can place some intriguing constraints on how they formed. | The observed exoplanet population unveiled by Kepler is billions of years old, distinctly separated in time from the planet formation process that only lasted ~10-100 Myr. I will argue that atmospheric escape has been one of the key evolutionary drivers shaping the exoplanet population we observed today. By understanding how these planet evolve in time, I will show we can place some intriguing constraints on how they formed. | ||
Revision as of 16:27, 1 February 2019
This page records the schedule, titles and abstracts of the JHU/STScI CAS Astrophysics Wine & Cheese Series in Spring 2019.
Wine and Cheese sessions with one talk will have a 50 minute talk with 10 minutes for questions. Sessions with two speakers will have two 25 minute talks, each with 5 minutes for questions. Sessions in the Graduate Student Series will have three 15 minute talks, each with 5 minutes for questions.
Back to W&C Schedule
February 4th
James Owen (Imperial College)
Understanding the formation and evolution of the Kepler Planets
The observed exoplanet population unveiled by Kepler is billions of years old, distinctly separated in time from the planet formation process that only lasted ~10-100 Myr. I will argue that atmospheric escape has been one of the key evolutionary drivers shaping the exoplanet population we observed today. By understanding how these planet evolve in time, I will show we can place some intriguing constraints on how they formed.
February 11th
TBD
Title
Abstract
