在月球融中保存的高爆发前含水量
Erik H Hauri1, Thomas Weinreich, Alberto E Saal
1Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015, USA. ehauri@ciw.edu
概括
新的发现显示,月球含有比以前认为的水量要多得多. 原始的月球岩含量显示水含量与地球上层地幔相当,挑战了关于月球挥发物的先前假设.
科学领域:
- 行星科学 行星科学
- 地质化学 地质化学
- 火山学 火山学是一门学科.
背景情况:
- 从历史上看,月球被认为是高度耗尽的挥发物,特别是水.
- 之前对月球火山玻璃中的水的直接测量显示其度不超过百万分之50 (ppm).
研究的目的:
- 报告在月球融中水的现场测量.
- 为了研究火山爆发前保存的原始月球岩的挥发性含量.
主要方法:
- 在月球融中被困在橄晶体中的水位测量.
- 对相关的挥发性元素的分析,包括,硫和.
主要成果:
- 月球融化含有大量的水,含量在615至1410ppm之间.
- 检测到高相关量的 (50-78 ppm),硫 (612-877 ppm) 和 (1.5-3.0 ppm).
- 发现挥发性含量与原始的陆地中海脊基岩相似.
结论:
- 月球内部的一些区域拥有相当于地球上层地幔的含水量.
- 根据之前的测量,月球的挥发性库存可能被大大低估.
- 原始的月球岩可以保持高挥发性度,不受后期脱气的影响.
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