Abstract
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.
Highlights
Shock metamorphism is one of the fundamental geological processes in the evolution of meteorites [1]
The parent body of meteorites undergoes one or more impact events in space, and the minerals in the meteorites are modified by shock-induced high pressures and high temperatures
This study focuses on the shock-metamorphic features of olivines in a single shock vein of chondrite GRV053584
Summary
Shock metamorphism is one of the fundamental geological processes in the evolution of meteorites [1]. The parent body of meteorites undergoes one or more impact events in space, and the minerals in the meteorites are modified by shock-induced high pressures and high temperatures. Shock effects seen in these minerals are records of the shock conditions [2,3]. Understanding the processes involved in formation of these shock effects is fundamental for any interpretations of the impact events. Shock-induced high pressures and high temperatures cover the pressures and temperatures condition of the Earth’s mantle.
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