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题名

Sound velocity and compressibility of melts along the hedenbergite (CaFeSi2O6)-diopside (CaMgSi2O6) join at high pressure: Implications for stability and seismic signature of Fe-rich melts in the mantle

作者
通讯作者Jing, Zhicheng
发表日期
2022
DOI
发表期刊
ISSN
0012-821X
EISSN
1385-013X
卷号577
摘要

Iron-rich silicate melts play an important role in the magmatic history of the Earth and the Moon. However, their elastic properties at high pressures, especially the sound velocities, are poorly understood. Here we determined the ultrasonic sound velocities of two silicate melts along the hedenbergite (Hd, CaFeSi2O6) - diopside (Di, CaMgSi2O6) join at high pressure and temperature conditions up to 6GPa and 2329K, using the high-pressure ultrasonic technique combined with synchrotron radiation in a multianvil apparatus. Our results show that Fe can significantly reduce the sound velocity while increasing the density of silicate melts. Comparing the melts of Di, Hd, and a mixture of 50 mol% hedenbergite + 50 mol% diopside (Hd(50)Di(50)), we find that although densities of the Hd-Di melts can be well-described by a linear mixing law empirically at high pressures, sound velocities do not vary with composition linearly. Assuming that the low-velocity regions in Earth's upper mantle are mainly due to the presence of partial melt, we applied our results to study the gravitational stability and seismic signature of Fe-rich silicate melts in the mantle, combined with melt geometry and compaction models. For the lowvelocity zone (LVZ) in mantle asthenosphere, although the degree of seismic velocity reduction can be explained by the presence of a small amount of partial melt distributed in film/band geometry along grain boundaries, silicate melts formed in this depth range are too light to be gravitationally stable, but may be completely entrained in the convecting mantle due to the small melt fraction and low meltmatrix separation velocity. For the low-velocity layer (LVL) above the mantle transition zone, the presence of Fe-rich melts (with FeO>similar to 10 wt%) distributed in textural equilibrium with the ambient mantle is a plausible explanation. (C) 2021 Elsevier B.V. All rights reserved.

关键词
相关链接[来源记录]
收录类别
SCI ; EI
语种
英语
重要成果
NI期刊
学校署名
通讯
资助项目
National Natural Science Foundation of China[41974098] ; National Science Foundation[
WOS研究方向
Geochemistry & Geophysics
WOS类目
Geochemistry & Geophysics
WOS记录号
WOS:000712266100006
出版者
EI入藏号
20220211451451
EI主题词
Calcium Compounds ; Grain Boundaries ; Magnesia ; Seismology ; Silicates ; Synchrotron Radiation ; Synchrotrons ; Ultrasonic Testing
EI分类号
Earthquake Measurements And Analysis:484.1 ; Ultrasonic Applications:753.3 ; Inorganic Compounds:804.2 ; Particle Accelerators:932.1.1
ESI学科分类
GEOSCIENCES
来源库
Web of Science
引用统计
被引频次[WOS]:9
成果类型期刊论文
条目标识符http://sustech.caswiz.com/handle/2SGJ60CL/255332
专题理学院_地球与空间科学系
作者单位
1.Case Western Reserve Univ, Dept Earth Environm & Planetary Sci, Cleveland, OH 44106 USA
2.Univ Chicago, Ctr Adv Radiat Sources, Chicago, IL 60637 USA
3.Southern Univ Sci & Technol, Dept Earth & Space Sci, Shenzhen 518055, Guangdong, Peoples R China
4.Argonne Natl Lab, Adv Photon Source, Argonne, IL 60439 USA
通讯作者单位地球与空间科学系
推荐引用方式
GB/T 7714
Xu, Man,Jing, Zhicheng,Yu, Tony,et al. Sound velocity and compressibility of melts along the hedenbergite (CaFeSi2O6)-diopside (CaMgSi2O6) join at high pressure: Implications for stability and seismic signature of Fe-rich melts in the mantle[J]. EARTH AND PLANETARY SCIENCE LETTERS,2022,577.
APA
Xu, Man.,Jing, Zhicheng.,Yu, Tony.,Alp, E. Ercan.,Lavina, Barbara.,...&Wang, Yanbin.(2022).Sound velocity and compressibility of melts along the hedenbergite (CaFeSi2O6)-diopside (CaMgSi2O6) join at high pressure: Implications for stability and seismic signature of Fe-rich melts in the mantle.EARTH AND PLANETARY SCIENCE LETTERS,577.
MLA
Xu, Man,et al."Sound velocity and compressibility of melts along the hedenbergite (CaFeSi2O6)-diopside (CaMgSi2O6) join at high pressure: Implications for stability and seismic signature of Fe-rich melts in the mantle".EARTH AND PLANETARY SCIENCE LETTERS 577(2022).
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