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Updated: Nov 16, 2025

Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions
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Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions

Published on: June 13, 2015

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隕石の129Cmと247Cmは,太陽のrプロセスの元素の最後の天体物理的源を制限しています

Benoit Côté1,2,3, Marius Eichler4, Andrés Yagüe López5

  • 1Research Centre for Astronomy and Earth Sciences, Eötvös Loránd Research Network, Konkoly Observatory, 1121 Budapest, Hungary. benoit.cote@csfk.org.

Science (New York, N.Y.)
|February 26, 2021
PubMed
まとめ

隕石は太陽系の初期構成を明らかにした 隕石におけるヨウ素-129とキュリウム-247の比率は,中性子星の融合が急速な中性子捕獲プロセス (rプロセス) を通して重元素を生成することを示唆している.

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