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Updated: Feb 22, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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マグネシウムの同位体 蓄積による蒸気損失が惑星の組成を形作る証拠

Remco C Hin1, Christopher D Coath1, Philip J Carter2

  • 1School of Earth Sciences, University of Bristol, Wills Memorial Building, Queens Road, Bristol BS8 1RJ, UK.

Nature
|September 30, 2017
PubMed
まとめ

原始的な隕石よりも重いマグネシウムの同位体を示しています この違いは,星雲や核のプロセスではなく,惑星積層中の蒸気損失から生じた可能性が高い.

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