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Updated: May 21, 2025

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月球背面地幔中的水量
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
概括
长江的
科学领域:
- 月球科学
- 地质化学
- 星球科学
背景情况:
- 月球内部的水含量是了解月球形成和演变的关键.
- 6号任务从月球背面的南极-艾特肯盆地收集了样本.
研究的目的:
- 在Chang'e-6马样本中分析水的丰度和同位素.
- 调查月球背面地幔的水含量及其影响.
主要方法:
- 分析石和融石的含量.
- 确定水的丰度和同位素组成 (δD值).
主要成果:
- 长江6号基岩的原始岩含水量很高 (15-168μg/g), δD值为-123±167‰.
- 月球背面的地幔来源估计含水量较低 (1-1.5μg/g),这表明它比近面的地幔干燥.
结论:
- 月球内部的水分布可能表现为半球二分法.
- 这些发现为月球形成模型和进化提供了关键的约束,特别是巨大的撞击假说.
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