地球の揮発性物質は,融解と蒸発によって形成される
C Ashley Norris1, Bernard J Wood1
1Department of Earth Sciences, University of Oxford, South Parks Road, Oxford OX1 3AN, UK.
Nature
|September 30, 2017
まとめ
地球
科学分野:
- 地化学と惑星科学
- 太陽系 初期 の 進化
- 元素の豊富性に関する研究
背景:
- 地球のシリケートマントルは,CIコンドライトと比較して,適度な揮発性元素で著しく枯渇しています.
- 揮発性物質に富んだ物質の蓄積と核抽出を含む既存のモデルは,観察された元素の枯渇,特にインジウムの過剰を完全に説明できません.
研究 の 目的:
- 地球の揮発性元素の在庫を確立する際に惑星の蓄積過程における溶解と蒸発過程の役割を調査する.
- シリケート地球における 適度な揮発性元素の 観測された枯渇パターンを調和させるため
主な方法:
- 地球の蓄積と前体での溶解過程の分析.
- 制御された温度と酸素の流動性条件下で材料の実験的蒸発.
主要な成果:
- シリケート地球における 揮発性元素の減少のパターンは 部分的な溶解と蒸発と一致しています
- これらのプロセスは,揮発性物質に富んだコンドライトの単純な蓄積ではなく,元素の豊富さをよりよく説明します.
結論:
- 先駆体での溶解と蒸発と月形成の衝突で 地球の揮発性元素の組成が確立された可能性が高い.
- これは,陸上のシリケート中の適度な揮発性元素の枯渇についてより包括的な説明を提供します.
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