2009Acta Mineralogica SinicaRequires access

FEATURES AND CONDITIONS FOR THE INTRACRYSTALLINE TRANSFORMATION FROM OLIVINE TO HIGH-PRESSURE POLYMORPHS IN SHOCK-METAMORPHOSED METEORITES

Ming Chen

Open publisher page 2 citations

Abstract

An investigation into two shock-metamorphosed chondritic meteorites indicates that the intracrystalline transformations from olivine to high pressure polymorphs could take place at relatively low temperature(1000 ℃) in a large pressure regime(14.5 to 23 GPa).The intracrystalline transformation of olivine produced lamellar ringwoodite.No direct intracrystalline transformation from olivine to wadsleyite was observed.The lamellar ringwoodite consisting of crystallite aggregates replaced parent olivine along staking faults and planar fractures.An association consisting of wadsleyite and ringwoodite platelets,respectively,has also been observed in olivine of some meteorites.The wadsleyite was produced by replacing ringwoodite during pressure release as a result of retrograde-metamorphism.This study provides information for understanding geological settings and pressure and temperature conditions for the polymorphic transformation of olivine in the Earth's lithospheric subducting slabs.

About this research paper

What this paper is about

An investigation into two shock-metamorphosed chondritic meteorites indicates that the intracrystalline transformations from olivine to high pressure polymorphs could take place at relatively low temperature(1000 ℃) in a large pressure regime(14.5 to 23 GPa).The intracrystalline transformation of olivine produced lamellar ringwoodite.No direct intracrystalline transformation from olivine to wadsleyite was observed.The lamellar ringwoodite consisting of crystallite aggregates replaced parent olivine along staking faults and planar fractures.An association consisting of wadsleyite and ringwoodite platelets,respectively,has also been observed in olivine of some meteorites.The wadsleyite was produced by replacing ringwoodite during pressure release as a result of retrograde-metamorphism.This study provides information for understanding geological settings and pressure and temperature conditions for the polymorphic transformation of olivine in the Earth's lithospheric subducting slabs.

Why it matters

OpenAlex reports 2 citations for this work. Citation counts describe recorded attention and do not establish research quality.

Key contribution

A contribution statement is not available in the OpenAlex record.

Method / approach

Method details are not available in the OpenAlex metadata.

Main findings

Findings are not separately available in the OpenAlex metadata.

Limitations

Limitations are not available in the OpenAlex metadata.

Applications

Application details are not available in the OpenAlex metadata.

Available abstract

An investigation into two shock-metamorphosed chondritic meteorites indicates that the intracrystalline transformations from olivine to high pressure polymorphs could take place at relatively low temperature(1000 ℃) in a large pressure regime(14.5 to 23 GPa).The intracrystalline transformation of olivine produced lamellar ringwoodite.No direct intracrystalline transformation from olivine to wadsleyite was observed.The lamellar ringwoodite consisting of crystallite aggregates replaced parent olivine along staking faults and planar fractures.An association consisting of wadsleyite and ringwoodite platelets,respectively,has also been observed in olivine of some meteorites.The wadsleyite was produced by replacing ringwoodite during pressure release as a result of retrograde-metamorphism.This study provides information for understanding geological settings and pressure and temperature conditions for the polymorphic transformation of olivine in the Earth's lithospheric subducting slabs.

Key concepts: Ringwoodite, Olivine, Meteorite, Shock metamorphism, Geology, Geochemistry, Mantle (geology), Chromite

Related papers

Back to paper searchBrowse research topicsOriginal source
FEATURES AND CONDITIONS FOR THE INTRACRYSTALLINE TRANSFORMATION FROM OLIVINE TO HIGH-PRESSURE POLYMORPHS IN SHOCK-METAMORPHOSED METEORITES — Research Paper | ScholarLens