Recurrent planetesimal formation in an outer part of the early solar system

Abstract The formation of planets in our solar system encompassed various stages of accretion of planetesimals that formed in the protoplanetary disk within the first few million years at different distances to the sun. Their chemical diversity is reflected by compositionally variable meteorite grou...

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Bibliographic Details
Main Authors: Wladimir Neumann, Ning Ma, Audrey Bouvier, Mario Trieloff
Format: Article
Language:English
Published: Nature Portfolio 2024-07-01
Series:Scientific Reports
Online Access:https://doi.org/10.1038/s41598-024-63768-4