The history of accretion in our Solar System

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This project aims to determine precise timing of formation and primary melting of asteroids of various compositions, and to trace the stellar sources and mixing processes that caused the compositional diversity of asteroids and planets in our Solar System. This can be attained by comprehensive study of achondrites, meteorites derived from asteroids that were once partially melted. Using the world’s foremost facilities for cosmochemical research in Australia and the United States of America, the processes leading to the formation of planets will be explored. This project is intended to advance fundamental knowledge of the environment in which planets emerge and evolve, and the place of our Solar System among planetary systems in the Galaxy.