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Updated: Jan 13, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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高圧マグマと水素の反応で湿った惑星を形成する

H W Horn1,2, A Vazan3, S Chariton4

  • 1School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA. hallensu@asu.edu.

Nature
|October 30, 2025
PubMed
まとめ

新しい実験では 水素とマグマの反応によって 惑星の内部で 重要な量の水が生まれる事が示されています 水が豊富な系外惑星は 恒星から遠くに形成されるという考えに 異議を唱えます

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