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Updated: May 10, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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鉄隕石は,原惑星の初期の形成と破滅的な破壊の証拠です

Jijin Yang1, Joseph I Goldstein, Edward R D Scott

  • 1Department of Mechanical and Industrial Engineering, University of Massachusetts, Amherst, Massachusetts 01003, USA. jiyang@ecs.umass.edu

Nature
|April 20, 2007
PubMed
まとめ

鉄隕石の冷却速度は,初期の原惑星が以前考えられていたよりも大きかったことを明らかにしています. これらの発見は,惑星増殖の従来のモデルに異議を唱え,より大きな衝撃イベントが最初の惑星を形成することを示唆しています.

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