Eiichiro Kokubo uses numerical dynamics to investigate planet formation. His work with Shigeru Ida identified a regime of oligarchic growth, where neighboring large protoplanets accrete smaller planetesimals while remaining dynamically separated.
The large bodies alter the very population from which they grow: their gravity increases small-body random velocities, changing subsequent collision and capture rates. Following this feedback distinguishes the oligarchic regime from a simple extrapolation in which the largest object keeps outgrowing all its neighbors indefinitely.[ref]
Oligarchic Growth of Protoplanets by Eiichiro Kokubo and Shigeru Ida. Abstract: self-consistent velocity evolution, regulated growth and orbital separation
Portrait of Eiichiro Kokubo
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