Plagioclase feldspar is one of the abundant minerals on the surface of the Earth, the Moon and Mars, and is also commonly found in meteorites. This dissertation seeks to better understand the phase changes in plagioclase when subjected to meteorite impact and fundamental information about impact cratering process. Shock features in plagioclase from Mistastin Lake impact structure, Canada, and Apollo samples returned from the Moon were investigated. A series of progressive optical shock features were observed, and their Raman spectra was collected systematically. Identified shock featurs include deformed twins, planar features, and partially to completely isotropic or diaplectic glass. However, no planar deformation features (PDFs) were obse...
Abstract We investigated three types of shocked feldspar in the Asuka-881757,531-2 sample with mid...
We report the first discoveries of high-pressure minerals in the historical L6 chondrite fall Châtea...
Our understanding of the formation and evolution of the primary lunar crust is based on geochemical ...
Shock metamorphism, caused by hypervelocity impact, is a poorly understood process in feldspar. This...
We present the first systematic Micro-Raman spectroscopic investigation of plagioclase of different ...
We investigated shock metamorphism of two lunar meteorites (Asuka-881757 and Yamato-86032). We measu...
Cathodoluminescence (CL) spectrum of plagioclase shows four emission bands at around 350, 420, 570 a...
Plagioclase feldspar is one of the most common rock‐forming minerals on the surfaces of the Earth an...
This contribution addresses the role of chemical composition, pressure, temperature, and time during...
The present study gives a contribution to the knowledge on the Na-feldspar and plagioclases, extendi...
Sayh al Uhaymir (SaU) 300 comprises a microcrystalline igneous matrix (grain size 10 m), dominated b...
Yamato (Y)-793169 and Asuka (A)-881757 are unbrecciated lunar mare meteorites that contain shocked p...
Plagioclase feldspars are common on the surfaces of planetary objects in the Solar System such as th...
Northwest Africa (NWA) 032 is the youngest radio metrically dated mare basalt, with concordant Rb-Sr...
Lunar meteorites are an important source of information about the Earth’s moon. In this study, the m...
Abstract We investigated three types of shocked feldspar in the Asuka-881757,531-2 sample with mid...
We report the first discoveries of high-pressure minerals in the historical L6 chondrite fall Châtea...
Our understanding of the formation and evolution of the primary lunar crust is based on geochemical ...
Shock metamorphism, caused by hypervelocity impact, is a poorly understood process in feldspar. This...
We present the first systematic Micro-Raman spectroscopic investigation of plagioclase of different ...
We investigated shock metamorphism of two lunar meteorites (Asuka-881757 and Yamato-86032). We measu...
Cathodoluminescence (CL) spectrum of plagioclase shows four emission bands at around 350, 420, 570 a...
Plagioclase feldspar is one of the most common rock‐forming minerals on the surfaces of the Earth an...
This contribution addresses the role of chemical composition, pressure, temperature, and time during...
The present study gives a contribution to the knowledge on the Na-feldspar and plagioclases, extendi...
Sayh al Uhaymir (SaU) 300 comprises a microcrystalline igneous matrix (grain size 10 m), dominated b...
Yamato (Y)-793169 and Asuka (A)-881757 are unbrecciated lunar mare meteorites that contain shocked p...
Plagioclase feldspars are common on the surfaces of planetary objects in the Solar System such as th...
Northwest Africa (NWA) 032 is the youngest radio metrically dated mare basalt, with concordant Rb-Sr...
Lunar meteorites are an important source of information about the Earth’s moon. In this study, the m...
Abstract We investigated three types of shocked feldspar in the Asuka-881757,531-2 sample with mid...
We report the first discoveries of high-pressure minerals in the historical L6 chondrite fall Châtea...
Our understanding of the formation and evolution of the primary lunar crust is based on geochemical ...