月球水的三氧同位素揭示了土著和彗星遗产
Maxwell M Thiemens1,2, Morgan H Nunn Martinez3, Mark H Thiemens3
1Department of Earth Sciences, University of Edinburgh, Edinburgh EH9 3JW, Scotland, United Kingdom.
概括
月球水的月球水.
科学领域:
- 行星科学 行星科学
- 天体化学是天体化学.
- 月球地质学 月球地质学
背景情况:
- 月球上的水的起源对于未来的月球基地至关重要.
- 潜在的来源包括本土的月球物质,太阳风和外星交付.
- 水中的氧同位素为月球氧气来源提供了洞察力.
研究的目的:
- 通过分析其氧同位素成分来调查月球水的起源.
- 开发和应用一个高精度的分析技术,用于小水样.
- 描述月球水的三重氧同位素组成 (Δ'17O和 δ18O).
主要方法:
- 逐步加热 (50°C,150°C,1000°C) 以释放不同的水分.
- 化以将水转化为氧气,用于同位素分析.
- 使用双入口同位素比质谱仪对阿波罗样品和对照进行同位素测量.
主要成果:
- 月球水样本主要表现出高 Δ'17O 值 (≥ 0 ‰).
- 氧同位素数据与静态,普通和CI的特征一致.
- 混合趋势表明与恩斯塔提特石和潜在的彗星来源有联系.
结论:
- 月球水的氧同位素成分对其起源提供了强烈的约束.
- 数据表明,石类物质,特别是恩斯塔提特石的显著贡献.
- 彗星的贡献也是可能的,对彗星的 Δ'17O 值有精细的约束.
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