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月球的同位素证据证明了晚期的面膜
Thomas S Kruijer1, Thorsten Kleine1, Mario Fischer-Gödde1
1Institut für Planetologie, Westfälische Wilhelms-Universität Münster, Wilhelm-Klemm-Strasse 10, D-48149 Münster, Germany.
Nature
|April 10, 2015
概括
月球的-182 (182W) 同位素比率高于地球,支持地球元素组成的晚期层假设. 然而,月球和地球在这个晚期涂层之前共享了类似的182W比,挑战了当前的月球起源理论.
科学领域:
- 地质化学 地质化学
- 行星科学 行星科学
- 同位素地质学的同位素.
背景情况:
- 巨大撞击假说解释了月球的形成和地球核心的发展.
- 地球的地幔有高于预期的高度 siderophile 元素 (HSE) 的丰度.
- 核心形成后的原始材料的"晚期层"被提出来解释HSE过剩.
研究的目的:
- 为了测试使用同位素的晚期层假设.
- 为了调查HSE在地球大批量酸盐中的起源.
- 改进对形成月球的巨大撞击事件的理解.
主要方法:
- 在月球样本中精确测量同位素 ((182) W / ((184) W).
- 月球和地球的大量酸盐之间的同位素比率的比较.
- 对HSE系统学的分析,以推断晚期板的组成和质量.
主要成果:
- 月球显示,与地球的大量酸盐相比,182W的余量为每百万分之27±4.
- 这种过剩与预测为原始材料的晚期涂层的预测一致.
- 在晚期涂层之前,在原地球和月球之间没有发现显著的 (182W) 异常.
结论:
- 这项研究提供了证据支持地球HSE丰富的晚期层假设.
- 月球同位素数据表明,HSE是在地球核心形成后添加的.
- 前后面板的同位素均性挑战了现有的月球起源和巨型撞击动态模型.
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