一个潮湿的异质地幔在哈迪时代创造了一个可居住的世界
Yoshinori Miyazaki1,2, Jun Korenaga3
1Department of Earth and Planetary Sciences, Yale University, New Haven, CT, USA. ymiya@caltech.edu.
Nature
|March 3, 2022
概括
一个水化,化学异质的地幔使得早期的海洋形成,板块构造和快速的二氧化碳去除,创造了可居住的早期地球. 这一过程由岩海洋固化驱动,
科学领域:
- 星球科学
- 地质化学
- 地球的早期状况
背景情况:
- 哈迪时代跟随地幔融化, 呈现与今天截然不同的条件.
- 地质证据表明,地球表面与哈迪纪中期的现状相似,但从恶劣到宜居的过渡仍然不清楚.
研究的目的:
- 为了研究将原始地球表面转化为宜居环境所必需的条件.
- 确定推动海洋形成,板块构造和温室气体的关键因素.
主要方法:
- 模拟由岩海洋固化产生的水化,化学异质地幔的影响.
- 在湿的高氧化物地幔中比较二氧化碳去除率与同质的火溶性地幔.
主要成果:
- 在海洋形成,板块构造和大气中快速去除二氧化碳方面,水合,化学异质的地幔至关重要.
- 在潮湿的,以火化为主的地幔中, 二氧化碳的去除速度是十倍以上的,
- 这种地幔组成产生了富含橄素的海洋地,促进了蛇形化和类似于热水场的条件.
结论:
- 早期地球的可居住性是由化学异质和水合的地幔所促进的.
- 岩海洋固化在建立可居住性条件方面发挥了关键作用.
- 哈迪海底的条件可能与现代的热水通风系统相似.
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