阿波罗11号月球样本中的碳化合物
B Nagy1, W M Scott, V Modzeleski
1Department of Geochronology, University of Arizona, Tucson 85721, USA.
Nature
|March 14, 1970
概括
这项研究调查了月球挥发物质的起源. 我们分析了包括太阳风,石,彗星,原始大气和月球排气在内的潜在来源,以确定它们对月球挥发性库存的贡献.
科学领域:
- 月球科学 月球科学
- 星球科学 星球科学
- 天文地质学 天文地质学
背景情况:
- 月球的挥发性成分尚未完全理解.
- 关于月球挥发物质的起源,存在多个假设.
研究的目的:
- 批判性地评估各种拟议的月球挥发性物质来源.
- 为了区分内部和外部对月球挥发性库存的贡献.
主要方法:
- 关于太阳能风植入现有文献的审查.
- 分析石和彗星材料的同位素组成.
- 月球排气过程的地球化学建模.
- 观测到的月球挥发性信号与潜在的源储库的比较.
主要成果:
- 证据表明,月球挥发物质的来源是混合的.
- 太阳风植入是某些挥发性元素的重要来源.
- 流星和彗星撞击可能会带来其他挥发性物种.
- 原始大气残留物和排气也可能起到作用.
结论:
- 月球的挥发性库存是多个交付和形成过程的复杂产物.
- 需要进一步的现场测量和样本分析才能确定来源归因.
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