石灰同位素揭示了晚期层对地球的有限挥发性贡献
Wenzhong Wang1,2,3,4, Michael J Walter3, John P Brodholt4,5
1Deep Space Exploration Lab/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui 230026, China.
Science advances
|December 6, 2023
概括
地球的挥发性元素起源于原行星的分化,而不是晚期的涂层. 和同位素的比率表明,这个过程显著影响了地球的挥发性库存.
科学领域:
- 地质化学 地质化学
- 行星科学 行星科学
- 同位素地球化学 同位素地球化学
背景情况:
- 地球挥发性元素的起源是行星科学中一个重大未解决的问题.
- 大量酸盐地球 (BSE) 中的素同位素比例提供了线索,但由于在早期行星过程中对同位素分离的理解不佳而复杂.
研究的目的:
- 调查原行星分化在和同位素的分化中的作用.
- 为了确定晚期涂层对地球挥发性库存的贡献.
主要方法:
- 使用第一原则计算,在核心-地幔分化过程中建模出同位素分化.
- 均衡蒸发模型被用来评估行星小行星形成期间的分化.
主要成果:
- 核心-地幔分化显示,和同位素的分化很小.
- 早期行星体的平衡蒸发丰富了BSE中的和重同位素.
- 在BSE中硫,和的同位素标志与原行星分化相一致.
结论:
- 原行星分化是确定地球挥发性元素组成的主要过程.
- 晚期出现的外星物质并没有对BSE的挥发性库存做出重大贡献.
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