在选定的月球物质中含有水,,,碳,碳-13和氧-18的含量
概括
这项研究分析了月球骨灰和尘埃中水,和碳的同位素组成. 结果揭示了不同的同位素特征,为月球挥发物的起源和演变提供了洞察力.
科学领域:
- 地质化学 地质化学
- 同位素地球化学 同位素地球化学
- 月球科学 月球科学
背景情况:
- 月球岩和尘埃含有被困的挥发性物质,对于理解月球进化至关重要.
- 同位素分析为追踪这些挥发物的起源和历史提供了一个强大的工具.
研究的目的:
- 为了确定月球骨中水,和碳的丰度和同位素组成.
- 为了分析月球尘埃的同位素组成.
- 为了限制月球岩石的结晶温度.
主要方法:
- 对 (deltaD),碳 (delta(13) C) 和氧 (delta(18) O) 的同位素分析.
- 气相色谱用于测量水,和二氧化碳含量.
- 在Plagioclase和Ilmenite之间进行氧气同位素分成分析,以估计温度.
主要成果:
- 布雷奇亚中的水含量在150至455ppm之间,deltaD值在每毫升580至870之间.
- 气含量为40-53ppm,其中deltaD为每毫升-830-970.
- 二氧化碳呈现出每毫升+2.3至+5.1的delta{13) C,每毫升14.2至19.1的delta{18) O.
- 非CO2) 碳显示Delta13C从每毫升6.4到23.2之间.
- 月球尘埃含有810 ppm H2O (D=80 ppm) 和188 ppm总碳 (三角形) C=-17.6每毫米).
- 整个岩石氧同位素分析范围从5.8到6.2每毫米.
- B型岩石的结晶温度估计在1100°C和1300°C之间.
结论:
- 同位素数据表明月球挥发物的复杂历史,可能涉及太阳风植入和/或彗星/小行星传递.
- 不同挥发性物种的独特同位素特征为它们各自的起源提供了线索.
- 氧同位素温度测量证实了某些月球岩类型的高结晶温度.
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