月球冷漠的悖论
相关实验视频
Updated: May 2, 2026

08:14
Atom Probe Tomography Analysis of Exsolved Mineral Phases
Published on: October 25, 2019
6.9K
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.
概括
发现富含水分的月球无矿石挑战了现有的模型. 这项研究解释了它们的形成是通过低磁的形成,这表明月球的 magma 是缺乏的,与挥发性耗尽理论保持一致.
科学领域:
- 月球地质学 月球地质学
- 地质化学 地质化学
- 石化学 石化学是一门学科.
背景情况:
- 最近在月球上发现的阿帕石表明,其含水量高于预期.
- 这与月球岩石通常具有挥发性和稀疏性质相矛盾.
研究的目的:
- 为了研究水性月球酸盐的形成机制.
- 为了协调几乎无水的月球岩石中富含的矿物质的存在.
主要方法:
- 文献数据建模.
- 在岩石中对 (H), (F) 和 (Cl) 分割的分析.
主要成果:
- 名义上无水矿物质不能从F和Cl中充分分离H.
- 酸盐诱导的低磁性增加了和酸盐中的H/F比率.
- 水性酸盐被解释为低的产物.
结论:
- 月球的岩石可能缺乏气.
- 这些发现与月球岩石中观察到的挥发性物质枯竭相一致.
- 这支持月球形成的巨大冲击模型.
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