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Updated: Jun 19, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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Published on: November 16, 2013

Hf-Wクロノメトリーによる小惑星と地上の惑星の急速な増殖と初期の核形成

T Kleine1, C Münker, K Mezger

  • 1Institut für Mineralogie, Universität Münster, Corrensstrasse 24, D-48149 Münster, Germany. tkleine@nwz.uni-muenster.de

Nature
|August 29, 2002
PubMed
まとめ

ハフニウム-182を用いた放射性年代測定で,ボルンガム-182 (Hf-W) 崩壊は,惑星の急速な増殖を明らかにしている. 陸上の惑星と月の核形成は,太陽系の最初の3000万年以内に起こった.

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