Cosmic Renaissance: The Last Chance for Planet Formation Around Low-Mass Dying Stars
MonashPhysicsAndAstronomy via YouTube
Overview
Explore groundbreaking research on second-generation planet formation in a 58-minute lecture that challenges traditional theories about where and when planets can form in the universe. Delve into the fascinating world of post-Asymptotic Giant Branch (post-AGB) binary stars and their potential as sites for planet formation during stellar death. Learn how circumbinary disks, formed through binary star interactions during the transition from AGB to planetary nebula stages, share remarkable similarities with protoplanetary disks despite their different origins and shorter lifespans. Examine cutting-edge observations from the European Southern Observatory's Very Large Telescope instruments that reveal intricate details about disk structure, dust properties, and the complex dynamics between dying stars and their surrounding matter. Discover how these unique environments serve as natural laboratories for testing planet formation theories and expanding our understanding of cosmic evolution.
Syllabus
Cosmic Renaissance: The Last Chance for Planet Formation Around Low-Mass Dying Stars - Devika Kamath
Taught by
MonashPhysicsAndAstronomy