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Updated: Jun 19, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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陸上の惑星の揮発性蓄積の歴史と,その動的影響

Francis Albarède1

  • 1Ecole Normale Supérieure de Lyon, Université Claude-Bernard Lyon 1, and CNRS, 46 allée d'Italie, 69007 Lyon, France. albarede@ens-lyon.fr

Nature
|October 30, 2009
PubMed
まとめ

地球と月は,湿った小惑星から形成されてからずっと前に水を得て,プレート構造と生命にとって不可欠でした. この水の供給は,太陽系が分離してから1億年後にピークに達した.

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