高圧下でのマグマ物性:地球深部でのマグマの挙動解明;高圧下でのマグマ物性:地球深部でのマグマの挙動解明;Properties of magma at high pressures: Understanding the magma behavior in the interior of the Earth

Q4 Earth and Planetary Sciences
Tatsuya Sakamaki
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引用次数: 0

Abstract

Magma has been deeply related to the evolution and dynamics of the Earth from the magma ocean in the early Earth to present magmatism. Especially, a hot topic is a pressure-induced change in the property/structure of magma and its correlation to the macroscopic property and microscopic structure, with the goal of understanding the deep magma. This article introduces our studies about high-pressure measurements of magma properties with focusing on three topics. First one is the gravitational stability of hydrous magma at the base of the upper mantle based on density measurements at high pressure. Our results indicated a rapid reduction of the partial molar volume of H2O in magma with pressure, which causes enough densiˆcation of hydrous magma to be stagnant. Second, we proposed the ponded magma model at the lithosphere-asthenosphere boundary due to a decrease in the segregation rate. This model can illustrate the geophysically observed anomaly around the boundary. For density measurement of magmas under desired conditions, we succeeded in applying an X-ray absorption technique, which could provide a better understanding of magma behavior. Last topic is lunar magmatism. Compression behavior of lunar basaltic magma with high TiO2 content indicated the density crossover between the magma and lunar mantle at a certain depth. Based on this result, subducted magma could create lateral chemical heterogeneities in the lunar mantle and, moreover, it could form the low-velocity/low-viscosity layer at the base of lunar mantle.
高压下的岩浆物性:地球深部岩浆的行为解释;高压下的岩浆物性:地球深部岩浆的行为解释;Properties of magma at high pressures: Understanding the magma behavior in the interior of the Earth
从地球早期的岩浆海洋到现在的岩浆活动,岩浆与地球的演化和动力学有着深刻的关系。特别是压力引起的岩浆性质/结构变化及其与宏观性质和微观结构的关系,是了解深部岩浆的一个热点。本文介绍了高压测量岩浆性质的研究,重点介绍了三个方面。第一个是基于高压下密度测量的上地幔底部含水岩浆的重力稳定性。我们的结果表明,在压力作用下,岩浆中H2O的偏摩尔体积迅速减少,这使得含水岩浆的足够密度停滞不前。其次,由于岩石圈-软流圈的分离速率降低,提出了岩石圈-软流圈边界的岩浆池模式。该模型可以说明地球物理观测到的边界附近异常。为了在理想条件下测量岩浆的密度,我们成功地应用了x射线吸收技术,该技术可以更好地了解岩浆的行为。最后一个主题是月球岩浆作用。高TiO2含量的月玄武质岩浆的压缩行为表明岩浆与月幔在一定深度发生了密度交叉。由此可见,俯冲岩浆可在月幔中形成横向化学非均质性,并可在月幔底部形成低速/低粘度层。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Japanese Magazine of Mineralogical and Petrological Sciences
Japanese Magazine of Mineralogical and Petrological Sciences Earth and Planetary Sciences-Economic Geology
CiteScore
0.20
自引率
0.00%
发文量
6
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