实验量化地球核心中的含量
Dongyang Huang1,2, Motohiko Murakami3, Stephan Gerstl4
1SKLab-DeepMinE, MOEKLab-OBCE, School of Earth and Space Sciences, Peking University, Beijing, China. dhuang@pku.edu.cn.
Nature communications
|February 10, 2026
概括
地球的核心可能含有大量的气,相当于9-45个海洋的水. 这表明地球在形成过程中获得了大部分的水,而不是来自彗星.
科学领域:
- 地质化学 地质化学
- 行星科学 行星科学
- 高压矿物物理 高压矿物物理
背景情况:
- 地球的核心被假设为一个主要的储库.
- 由于极端条件,量化核心是具有挑战性的.
研究的目的:
- 量化地球核心中的 (H) 含量.
- 调查核心形成期间的固化机制.
主要方法:
- 使用激光加热的钻石天细胞进行超液体金属酸盐分区实验.
- 原子探头断层扫描用于直接的H观测.
主要成果:
- 在铁合金中直接观察与富含和氧的纳米结构相关的.
- 在核心形成过程中,有证据表明,O和H的合封存.
- 估计核心含量为0.07-0.36重量%,相当于9-45海洋的水.
结论:
- 地球的核心可能含有大量的.
- 观察到的Si/H比率表明了特定的封存机制.
- 这一发现意味着地球主要在积累过程中获得了水,而不是通过彗星撞击.
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