Abstract:
The conference will focus on processes of star formation and of circumstellar disks that lead to planetary systems, like our own, with planetary bodies, both silicate-rich and volatile-rich. These planetary bodies and their subsequent evolutions provide the bases for habitable environments and for the origin of life as we know it. The goal of this topical conference is to integrate the disparate stories of planetary accretion, both physical and chemical, into a consistent (although understandably incomplete) whole.