模拟早期地核-地幔分离过程中轻元素行为的铁-硅酸盐-水-硫系统的原位X射线衍射和射线照相

IF 1.2 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY
Riko Iizuka-Oku, H. Gotou, A. Suzuki, H. Kagi
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引用次数: 0

摘要

地球富含铁的地核含有轻元素。研究地球演化早期核幔分离过程中多种轻元素与铁、硅酸盐的相互作用具有重要意义。在5-10 GPa,高达约1900°C的温度下,对铁-硅酸盐-水-硫体系进行了原位x射线衍射和成像观察,以阐明顺序反应:铁的相变和氢化,以及硫化铁和硅酸盐的形成。新建的x射线成像系统的空间分辨率达到了约。10 μm为本研究显示铁团的形成和运动。在加热过程中,硫通过降低铁液与硅酸盐之间的界面能,使铁团的形状发生变形,影响铁团的生长。随着温度的升高,熔融铁中的轻元素和剩余的硅酸盐颗粒影响了原始地球的核幔分离。在随后的高温处理过程中,碳和硅被掺入液态铁中。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
In-situ X-ray diffraction and radiography of iron–silicate–water–sulfur system simulating behaviors of light elements during early Earth’s core–mantle segregation
ABSTRACT The Earth’s iron-rich core contains light elements. Studying the interaction of multiple light elements with iron and silicates during core–mantle segregation process in early Earth evolution has become important. In-situ X-ray diffraction and imaging observations of the iron–silicate–water–sulfur system at 5–10 GPa, up to approximately 1900°C, were used to elucidate sequential reactions: phase transformation and hydrogenation of iron, and formation of iron sulfide and silicates. The newly constructed X-ray imaging system achieved spatial resolution of approx. 10 μm for this study to show iron blob formation and motion. Sulfur distorted the iron blob shape and affected blob growth during heating by reducing the interfacial energy between molten iron and silicates. Light elements in the molten iron and the remaining silicate grains affected core–mantle segregation in the primitive Earth as temperatures increased. Carbon and silicon were incorporated into liquid Fe during later processes at higher temperatures.
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来源期刊
High Pressure Research
High Pressure Research 物理-物理:综合
CiteScore
3.80
自引率
5.00%
发文量
15
审稿时长
2 months
期刊介绍: High Pressure Research is the leading journal for research in high pressure science and technology. The journal publishes original full-length papers and short research reports of new developments, as well as timely review articles. It provides an important forum for the presentation of experimental and theoretical advances in high pressure science in subjects such as: condensed matter physics and chemistry geophysics and planetary physics synthesis of new materials chemical kinetics under high pressure industrial applications shockwaves in condensed matter instrumentation and techniques the application of pressure to food / biomaterials Theoretical papers of exceptionally high quality are also accepted.
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