Planetary Science Seminar fall-2022

The observed population of small, close-in exoplanets is bifurcated into two distinct types by the so-called ‘radius gap’. In this talk I will discuss the atmospheric processes which may effect such planets and finally lead to the radius gap being carved out, specifically the core-powered mass-loss mechanism and X-ray/EUV photo-evaporation. I will show how one can exploit these mass-loss processes to 'rewind the clock' on planetary evolution, to infer the underlying population at birth.