鉄隕石は,地上の惑星の領域で形成されたプラネティシマルの残骸として,鉄隕石です

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Updated: May 10, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
06:04

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 16, 2013

William F Bottke1, David Nesvorný, Robert E Grimm

  • 1Southwest Research Institute, 1050 Walnut St, Suite 400, Boulder, Colorado 80302, USA. bottke@boulder.swri.edu

Nature
|February 17, 2006
PubMed
まとめ

鉄隕石の親体は,小惑星帯ではなく,地上の惑星の近くで形成された可能性が高い. 初期の溶解と散乱は,メインベルトと初期の形成期における彼らの存在を説明する.

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