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Updated: Jun 10, 2026

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Simulation of the Planetary Interior Differentiation Processes in the Laboratory
Published on: November 15, 2013
月の塩素同位体組成と無水マントルの影響
Z D Sharp1, C K Shearer, K D McKeegan
1Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87122, USA. zsharp@unm.edu
まとめ
月は月,月が月である.
科学分野:
- 地質化学 地質化学
- 月科学 月科学 月科学
- イソトープ地球化学 イソトープ地球化学
背景:
- 月は長い間,地球と重要な地化学的違いである水 (水素) がほとんどないと考えられてきました.
- 最近の研究は,この見解に異議を唱え,地化学データに基づいて,潜在的に高い月の水分を含有することを示唆しています.
研究 の 目的:
- 月面のサンプルの塩素同位体分析を用いて月の水素濃度を調査する.
- 月面に水の存在と豊富さに関する矛盾するデータを調和させるため.
主な方法:
- アポロ月の玄武岩とガラスの塩素同位体組成の分析.
- 月面のサンプルと地球の海洋塩化物の間の同位体範囲の比較.
主要な成果:
- 月面のサンプルの塩素イソトープの範囲は,地球の25倍の範囲を示した.
- この広範囲の同位体分布は,月のベースアルティック噴火中の金属ハリドの揮発に起因する.
結論:
- 観測された同位体変動は,月面の水素濃度が非常に低いことを強く示唆しています (地球の10^4から10^5倍).
- 月の内部は,表面上の水の兆候があるにもかかわらず,本質的に無水質である可能性が高い.
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