月球的同位素组成以及对无水地幔的影响
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
概括
月亮的月亮的月亮
科学领域:
- 地质化学 地质化学
- 月球科学 月球科学
- 同位素地球化学 同位素地球化学
背景情况:
- 月球长期以来被认为几乎没有水 (),这是与地球的关键地质化学差异.
- 最近的研究已经挑战了这一观点,根据地化学数据表明,月球的水含量可能更高.
研究的目的:
- 通过对月球样本的同位素分析来调查月球的气度.
- 为了协调有关月球上水的存在和丰度的相互矛盾的数据.
主要方法:
- 在阿波罗月球基岩和玻璃中分析同位素组成.
- 月球样本与地球海洋化物之间的同位素范围的比较.
主要成果:
- 月球样本的同位素范围是地球的25倍.
- 这种广泛的同位素分布归因于月球基岩喷发期间金属化物的挥发.
结论:
- 观察到的同位素变化强烈表明,月球的气度极低 (比地球低10^4到10^5倍).
- 月球内部很可能本质上是无水的,尽管表面有一些水的迹象.
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