月のアパタイトパラドックス
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Updated: May 2, 2026

08:14
Atom Probe Tomography Analysis of Exsolved Mineral Phases
Published on: October 25, 2019
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J W Boyce1, S M Tomlinson, F M McCubbin
1Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, Los Angeles, CA 90095, USA.
まとめ
水が豊富な月のアパタイトの発見は,既存のモデルに挑戦しています. この研究は,低マグマ的フッ素による彼らの形成を説明し,月のマグマは水素が少ないことを示唆し,揮発性枯渇理論と一致しています.
科学分野:
- 月面地質学 月面地質学
- 地質化学 地質化学
- ペトロロジー・ペトロロジーとは
背景:
- 最近の月のアパタイトの発見は,予想以上に水分が多く含まれていることを示唆しています.
- これは,月面岩の概して揮発性低下した性質と矛盾している.
研究 の 目的:
- 水性月のアパタイトの形成メカニズムを調査する.
- ほぼ無水質の月の岩石に含まれる水素豊富なミネラルの存在を調和させるため.
主な方法:
- 文献データモデリング.
- マグマにおける水素 (H),フッ素 (F),塩素 (Cl) の分離の分析.
主要な成果:
- 名目無水鉱物は,FとClからHを十分に分化しません.
- アパタイトによって誘発される低マグマティックフッ素は,溶融とアパタイトにおけるH/F比を増加させる.
- 水性アパタイトは,低フッ素の産物として説明されています.
結論:
- 月のマグマはおそらく水素に乏しかった.
- この発見は,月面の岩石における観測された揮発性物質の枯渇と一致しています.
- これは月形成の巨大衝突モデルを支えている.
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