热化学石化区分和地幔的起源
Fabio A Capitanio1, Oliver Nebel2, Peter A Cawood2
1School of Earth Atmosphere and Environment, Monash University, Clayton, Victoria, Australia. fabio.capitanio@monash.edu.
Nature
|December 3, 2020
概括
在早期地球上通过解压融化和融化提取机制形成的克拉顿
科学领域:
- 地质科学
- 地球科学
- 构造学
背景情况:
- Kratons 代表着古老的,稳定的大陆地,但它们的形成和长期稳定性仍然不太清楚.
- 早期地球的地幔更热,更有活力,影响了岩层形成过程.
研究的目的:
- 提出和研究一个新的机制,以形成融化贫的岩层地幔 (CLM).
- 解释这个枯竭的地幔在地质时间尺度上演变为稳定的坑.
主要方法:
- 利用数值建模模模拟地幔动力学和早期地球条件下的石化层演变.
- 研究了解压融化,融化提取和岩层强度对地幔耗尽和稳定性的影响.
主要成果:
- 模型表明,在延伸的岩层下面的大规模解压融化会产生大量枯竭的地幔.
- 应变局部化和地幔硬化之间的负反促进了被耗尽的地幔融入岩层,促进了长期的稳定性.
- 早期的地球条件,包括较低的岩层强度,对于广泛的枯竭和坑边缘的形成至关重要.
结论:
- 拟议的机制解释了大量,耗尽的CLM的形成及其随后的稳定成.
- 早期地球的主要融化和回收事件对于产生和失去原始石化层至关重要,而后来的稳定性为古巨形成奠定了基础.
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