深入地幔:预测海洋星球未来的关键

IF 0.2 Q4 GEOGRAPHY, PHYSICAL
Y. Tatsumi, Nobuaki Suenaga, S. Yoshioka, K. Kaneko
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引用次数: 2

摘要

水循环和板块俯冲是基于含水相的稳定性和下沉海洋板块的压力-温度分布来考虑的。像现在这样相当热的板块中的水可能在浅层(<150km)被大量释放,并通过返回海洋。弧岩浆作用。另一方面,致密含水矿物在较冷条件下的稳定(目前的俯冲带很快就会经历这种情况)会导致海水向深地幔的输送或回流,从而减少地表海水的总质量。最近的一个地震速度结构模型提出的接受俯冲板块含水量的简单计算表明,地球海洋可能在8000万年后消失。可能会发生重大变化,如板块构造的结束和雪球地球的开始,以及影响生命的相关灾难。确定这一海洋行星地球未来图景的唯一方法是通过直接分析整个地球的上地幔来研究外隆起沿线发生的深层水合作用
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Drilling into the Mantle: A Key to Prognosticating the Future of the Ocean Planet
Water circulation, along with plate subduction, is considered based on the stabilities of hydrous phases and pressure ­ temperature profiles of the sinking oceanic plate. Water in a rather hot slab like the present one may be largely liberated at shallow depths ( < 150 km ) and return to the ocean via. arc magmatism. On the other hand, stabilization of dense hydrous minerals under cooler conditions, which current subduction zones will soon experience, causes the transportation or reflux of seawater to the deep mantle, which reduces the total mass of surface seawater. Simple calculations accepting water contents in the subducting slab suggested by a recent seismic velocity structure model indicate that the Earth’s oceans are likely to disappear ~80 million years hence. Significant changes may happen such as the end of plate tectonics and the onset of snowball Earth, with associated catastrophes affecting life. The only way to confirm this picture of the future of the ocean planet Earth is to examine deep hydration taking place along the outer rise through direct analyses of the upper mantle across the
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来源期刊
CiteScore
1.50
自引率
33.30%
发文量
28
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