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Updated: Sep 7, 2025

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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チェッシーニ隕石のクリプトンは,火星が霧状ガスの前にコンドリート性揮発物を蓄積したことを示している

Sandrine Péron1, Sujoy Mukhopadhyay1

  • 1Department of Earth and Planetary Sciences, University of California Davis, Davis, CA 95616, USA.

Science (New York, N.Y.)
|June 16, 2022
PubMed
まとめ

初期の火星は,チェッシーニ隕石のクリプトンイソトープによって証明された,コンドリティックな揮発性物質を含んでいた. 火星

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