Shock-Induced Olivine-Ringwoodite Transformation in the Shock Vein of Chondrite GRV053584

Shock metamorphism of minerals in meteorites could help to understand the shock history of its parent body and also provide a window into the interior of the Earth. Although shock features in olivine have been well known within and adjacent to shock melt veins and shock melt pockets in meteorites, t...

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Published in:Minerals
Main Authors: Feng Yin, Zhiwei Liao, Andrew Hursthouse, Deqiu Dai
Format: Text
Language:English
Published: Multidisciplinary Digital Publishing Institute 2018
Subjects:
Online Access:https://doi.org/10.3390/min8040139
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spelling ftmdpi:oai:mdpi.com:/2075-163X/8/4/139/ 2023-08-20T04:00:45+02:00 Shock-Induced Olivine-Ringwoodite Transformation in the Shock Vein of Chondrite GRV053584 Feng Yin Zhiwei Liao Andrew Hursthouse Deqiu Dai agris 2018-04-01 application/pdf https://doi.org/10.3390/min8040139 EN eng Multidisciplinary Digital Publishing Institute https://dx.doi.org/10.3390/min8040139 https://creativecommons.org/licenses/by/4.0/ Minerals; Volume 8; Issue 4; Pages: 139 shock metamorphism olivine ringwoodite phase transformation Text 2018 ftmdpi https://doi.org/10.3390/min8040139 2023-07-31T21:27:23Z Shock metamorphism of minerals in meteorites could help to understand the shock history of its parent body and also provide a window into the interior of the Earth. Although shock features in olivine have been well known within and adjacent to shock melt veins and shock melt pockets in meteorites, there are processes that are not yet completely understood. Ringwoodite is formed by crystallization from olivine melts or solid-state phase transformation of olivine. Typically, olivine clasts with a ringwoodite rim around an olivine core have been documented from only a handful of meteorites. Here we report results from GRV053684, a highly shocked L6 chondrite that was collected by Chinese Antarctic Research Expedition in 2006 to Antarctica. The investigations of the shock pressure history and the transformation mechanism of olivine to ringwoodite use optical microscope, electron probe microanalyzer (backscattered electron images, major element quantitative analyses, and quantitative wavelength-dispersive spectrometry elemental X-ray maps), and Raman spectrograph. Ringwoodite in the shock melt vein generally displays as Fe-rich (Fa37-43) polycrystalline rims around Fe-poor (Fa11-20) olivine core and as small individual clasts embedded in shock melt vein matrix. The difference in FeO between ringwoodite rim and olivine core implies that Fe was preferentially partitioned to ringwoodite. The occurrence of maskelynite (An17) indicates a shock pressure ~30 GPa. The FeO and MgO diffusion indicates the transformation process of olivine to ringwoodite is a diffusion-controlled incoherent nucleation and growth. The spatial association between ringwoodite and the shock melt vein matrix suggests that high temperature plays a key role in prompting phase transformation. Text Antarc* Antarctic Antarctica MDPI Open Access Publishing Antarctic Minerals 8 4 139
institution Open Polar
collection MDPI Open Access Publishing
op_collection_id ftmdpi
language English
topic shock metamorphism
olivine
ringwoodite
phase transformation
spellingShingle shock metamorphism
olivine
ringwoodite
phase transformation
Feng Yin
Zhiwei Liao
Andrew Hursthouse
Deqiu Dai
Shock-Induced Olivine-Ringwoodite Transformation in the Shock Vein of Chondrite GRV053584
topic_facet shock metamorphism
olivine
ringwoodite
phase transformation
description Shock metamorphism of minerals in meteorites could help to understand the shock history of its parent body and also provide a window into the interior of the Earth. Although shock features in olivine have been well known within and adjacent to shock melt veins and shock melt pockets in meteorites, there are processes that are not yet completely understood. Ringwoodite is formed by crystallization from olivine melts or solid-state phase transformation of olivine. Typically, olivine clasts with a ringwoodite rim around an olivine core have been documented from only a handful of meteorites. Here we report results from GRV053684, a highly shocked L6 chondrite that was collected by Chinese Antarctic Research Expedition in 2006 to Antarctica. The investigations of the shock pressure history and the transformation mechanism of olivine to ringwoodite use optical microscope, electron probe microanalyzer (backscattered electron images, major element quantitative analyses, and quantitative wavelength-dispersive spectrometry elemental X-ray maps), and Raman spectrograph. Ringwoodite in the shock melt vein generally displays as Fe-rich (Fa37-43) polycrystalline rims around Fe-poor (Fa11-20) olivine core and as small individual clasts embedded in shock melt vein matrix. The difference in FeO between ringwoodite rim and olivine core implies that Fe was preferentially partitioned to ringwoodite. The occurrence of maskelynite (An17) indicates a shock pressure ~30 GPa. The FeO and MgO diffusion indicates the transformation process of olivine to ringwoodite is a diffusion-controlled incoherent nucleation and growth. The spatial association between ringwoodite and the shock melt vein matrix suggests that high temperature plays a key role in prompting phase transformation.
format Text
author Feng Yin
Zhiwei Liao
Andrew Hursthouse
Deqiu Dai
author_facet Feng Yin
Zhiwei Liao
Andrew Hursthouse
Deqiu Dai
author_sort Feng Yin
title Shock-Induced Olivine-Ringwoodite Transformation in the Shock Vein of Chondrite GRV053584
title_short Shock-Induced Olivine-Ringwoodite Transformation in the Shock Vein of Chondrite GRV053584
title_full Shock-Induced Olivine-Ringwoodite Transformation in the Shock Vein of Chondrite GRV053584
title_fullStr Shock-Induced Olivine-Ringwoodite Transformation in the Shock Vein of Chondrite GRV053584
title_full_unstemmed Shock-Induced Olivine-Ringwoodite Transformation in the Shock Vein of Chondrite GRV053584
title_sort shock-induced olivine-ringwoodite transformation in the shock vein of chondrite grv053584
publisher Multidisciplinary Digital Publishing Institute
publishDate 2018
url https://doi.org/10.3390/min8040139
op_coverage agris
geographic Antarctic
geographic_facet Antarctic
genre Antarc*
Antarctic
Antarctica
genre_facet Antarc*
Antarctic
Antarctica
op_source Minerals; Volume 8; Issue 4; Pages: 139
op_relation https://dx.doi.org/10.3390/min8040139
op_rights https://creativecommons.org/licenses/by/4.0/
op_doi https://doi.org/10.3390/min8040139
container_title Minerals
container_volume 8
container_issue 4
container_start_page 139
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