Eve J Lee
UC San Diego
Date
2 April 2025
Host
Caroline Dorn
Title
Small Planet Formation
Abstract
Our Galaxy is teeming with small planets of sizes up to that of Neptune within orbital periods of ~100 days. These sub-Neptunes have no solar-system analog, raising questions on how such planets form, why they are so common, and why they do not exist in our own solar system. I will outline some of the puzzling demographic patterns that have emerged in the observations of these small planets and discuss how such patterns may be explained using first-principle physics and astrophysics that govern the interaction between the star, the disk, and the planet.
Recording
Link

D-PHYS