高度的 siderophile 元素被剥离了地球的地幔由硫化铁分离
David C Rubie1, Vera Laurenz2, Seth A Jacobson3
1Bayerisches Geoinstitut, Bayreuth, Germany. dave.rubie@uni-bayreuth.de.
概括
在地球的核心形成过程中,高度 siderophile 元素 (HSEs) 被耗尽. 一个"Hadean色"阶段,而不是晚期积累,解释了地幔中的HSE度和超状比率.
科学领域:
- 地质化学
- 星球科学
- 地球科学
背景情况:
- 在地球的大质量层中,高度 siderophile 元素 (HSEs) 已经耗尽,但却呈现出接近体的丰度.
- 传统理论认为这是由于核心形成剥离和晚期积累补充.
研究的目的:
- 研究核心形成过程中金属酸盐平衡和分离对HSE地幔度的作用.
- 重新评估晚期积累与早期过程在建立HSE丰度方面的贡献.
主要方法:
- 模拟与核心形成相关的高压金属平衡.
- 分析铁硫化物液体 ("哈迪") 脱离过程中高酸盐的行为.
主要成果:
- 与之前的假设相反,由于低分区系数,金属酸盐平衡增加了HSE地幔度.
- 在冷却过程中从岩海洋中分离出来的"岩"在晚期积累之前有效地剥离了HSE.
- 这一过程解释了所观察到的/和/比率.
结论:
- 早期的地球过程,特别是"哈迪黑色"分离,是HSE枯竭和地幔中的特定同位素比率的主要驱动因素.
- 晚期积累在确定HSE丰度中的作用不如以前想象的那么重要.
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