I/Pu揭示了地球主要由挥发性较差的差异化行星类物质形成
Weiyi Liu1, Yigang Zhang2, François L H Tissot1
1The Isotoparium, Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.
地球 地球 地球 地球 地球 地球
科学领域:
- 地质化学 地质化学
- 行星科学 行星科学
- 地球科学 地球科学 地球科学
背景情况:
- 中洋山脊玄武岩 (MORBs) 和海洋岛屿玄武岩 (OIBs) 呈现出明显的/比率,这表明地球积聚和地幔演变的差异.
- 和在核形成过程中的地化学行为对于解释这些同位素差异至关重要,但仍然不太了解.
研究的目的:
- 使用第一原理分子动力学,量化和在核形成过程中的金属酸盐分离系数.
- 模拟多阶段的核心形成,以评估其对地球地幔储库中/比率的影响.
- 为了确定观察到的/变异是否仅仅是由于核心形成,还是表明异质的积累.
主要方法:
- 第一原则分子动力学模拟来计算分区系数.
- 多个阶段的核心形成建模包括计算的分区系数.
- 分析和在金属酸盐分离过程中的行为.
主要成果:
- 在核心形成过程中,和都在金属液体中表现出部分分裂.
- 仅核形成不能解释在MORB中与OIB相比观察到的约/比率高3倍.
- 这些结果强烈支持地球的异质积累模型.
结论:
- 地球的积累是异质的,涉及一种早期的挥发性较低的物质,随后是挥发性较高的混凝土的晚期积累.
- 这种异质的积累解释了在不同的地幔储库中观察到的不同的/比率.
- 地球继承了大量的挥发物质,包括水,来自晚期的状积累.
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