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Updated: Apr 28, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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Published on: November 15, 2013

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長期にわたる核形成と原惑星の急速な増殖

T S Kruijer1, M Touboul2, M Fischer-Gödde3

  • 1Institut für Planetologie, Westfälische Wilhelms-Universität Münster, Wilhelm-Klemm-Strasse 10, DE-48149 Münster, Germany. ETH Zürich, Inst. of Geochemistry and Petrology, Clausiusstrasse 25, CH-8092 Zürich, Switzerland.

Science (New York, N.Y.)
|June 7, 2014
PubMed
まとめ

初期の太陽系プロセスは,隕石の親体を形状にしました. トングステン-182のバリエーションは,コア形成が約100万年かかっていたことを明らかにし,揮発性差異にもかかわらず,同時増殖を示唆しています.

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