地球地幔在终端轰炸前的的同位素组成
Matthias Willbold1, Tim Elliott, Stephen Moorbath
1Bristol Isotope Group, School of Earth Sciences, University of Bristol, Bristol BS8 1RJ, UK. m.willbold@bristol.ac.uk
Nature
|September 9, 2011
概括
地球上的贵金属是由石的晚期涂层解释的. 古代岩石的同位素分析支持了这一理论,排除了金属丰富性的其他解释.
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:
- 尽管有核心形成预测,但黄金等贵金属却很丰富.
- 石在核心形成后形成的"晚期层"是一个被提议的解释.
- 古老的伊沙,格陵兰的岩石早于这次石轰炸.
研究的目的:
- 为了测试贵金属丰富度的"晚期层"假设.
- 为了确定地球在最后的石轰炸之前的组成.
- 分析古代岩石中同位素的组成线索.
主要方法:
- 高精度的 (W) 同位素分析.
- 来自格陵兰岛伊沙岛的38亿年前岩石的分析.
- 古代与现代陆地样本中的W同位素比率的比较.
主要成果:
- 伊沙岩石的比例 (182) W / 184) W比现代样本高得多.
- 这种较高的比率与晚期贴面的预期影响保持一致.
- 不支持像地幔再混合或核心-地幔相互作用这样的替代模型.
结论:
- "晚期层"假说得到了同位素数据的强烈支持.
- 地球的构成受到后期石撞击的显著改变.
- 这种轰炸可能启动了现代地幔对流模式.
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