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Updated: Jun 30, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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初期の太陽系の小惑星の表面に広がったマグマの海は,太陽系初期に存在していた

Richard C Greenwood1, Ian A Franchi, Albert Jambon

  • 1PSSRI, Open University, Walton Hall, Milton Keynes MK7 6AA, UK. r.c.greenwood@open.ac.uk

Nature
|June 17, 2005
PubMed
まとめ

初期の太陽系惑星系は地球規模で融解し,マグマの海を形成した. この過程で層状の天体が形成され,地球のような惑星の組成に影響を与えました.

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