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Updated: May 11, 2026

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

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Published on: November 15, 2013

海洋マグマの固体化で2種類の地球型惑星の出現

Keiko Hamano1, Yutaka Abe, Hidenori Genda

  • 1Department of Earth and Planetary Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan. keiko@eps.s.u-tokyo.ac.jp

Nature
|May 31, 2013
PubMed
まとめ

地上の惑星は,溶けた状態からの固化によって2つのタイプに分かれます. タイプIの惑星は海のために水を保持し,タイプIIの惑星は長時間マグマの海と水力学的脱出のために水を失います.

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