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Updated: May 21, 2025

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月面のマントルの水分量
Huicun He1, Linxi Li1,2, Sen Hu3
1Key Laboratory of the Earth and Planetary Physics, Chinese Academy of Sciences, Beijing, China.
Nature
|April 9, 2025
まとめ
チャン
科学分野:
- 月科学
- 地化学
- 惑星科学
背景:
- 月面内部の水分は 月面の形成と進化を理解する鍵です
- 探査機チャングー6は 月面の南極・アイトケン盆地からサンプルを採取した.
研究 の 目的:
- チェンジ6の塩基岩のサンプルで 水分と水素の同位体を分析する
- 月の裏側のマントルの水分と その影響を調査する
主な方法:
- アパタイトとChang'e-6の溶けた塩基岩からの含有物の分析
- 水分と水素同位体組成の測定 (δD値)
主要な成果:
- チャンエ6のマザーマグマは水分量が多く (15-168μg/g) で,δD値は -123 ± 167‰である.
- 月の裏側のマントルの源は水分量が低いと推定される (1-1.5μg/g),これは近側のマントルよりも乾燥していることを示唆している.
結論:
- 月面内部の水の分布は半球的な二分法を示している.
- これらの発見は,月形成モデルと進化,特に巨大衝突仮説の重要な制約を提供します.
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