通过融化和蒸发形成的地球的挥发性物质
C Ashley Norris1, Bernard J Wood1
1Department of Earth Sciences, University of Oxford, South Parks Road, Oxford OX1 3AN, UK.
Nature
|September 30, 2017
概括
地球
科学领域:
- 地质化学和行星科学
- 太阳系的早期演变
- 基本的丰富性研究
背景情况:
- 地球的化物地幔与CI石相比,中度挥发性元素显著减少.
- 现有的模型涉及富含挥发物质的积累和核心提取,并不能完全解释观察到的元素耗尽,特别是的过剩.
研究的目的:
- 研究行星积聚过程中融化和蒸发过程在建立地球挥发性元素库存中的作用.
- 为了协调土中中度挥发性元素的观察到的枯竭模式.
主要方法:
- 在地球积聚和前体上发生的融化过程的分析.
- 在受控温度和氧气流动性条件下的材料的实验蒸发.
主要成果:
- 在土中观察到的挥发性元素枯竭模式与部分融化和蒸发一致.
- 这些过程,而不是简单的丰富的挥发性石的积累,更好地解释了元素的丰富性.
结论:
- 在前体上的融化和蒸发以及在月球形成的撞击中,很可能建立了地球的挥发性元素组成.
- 这为陆地中中等挥发性元素的减少提供了更全面的解释.
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