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Updated: Feb 20, 2026

Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions
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Published on: June 13, 2015

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恒星のマグネシウムとシリコンの比率は,系外惑星の大気中に存在する

Jorge A Sanchez1, Peter C B Smith2, Krishna Kanumalla2

  • 1School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA. jasanchez@asu.edu.

Nature communications
|February 18, 2026
PubMed
まとめ

外惑星の大気,特に超高温の木星は,宿主星の岩石形成元素 (マグネシウム,シリコン,鉄) の比率を保持することができる. この研究は,これらの比率が恒星の豊富さを反映しているという仮定を検証しており,これは系外惑星の形成を理解するために極めて重要です.

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