Olivine–ringwoodite and plagioclase–maskelynite transformation mechanisms in the Bursa L6 chondrite were determined by Raman and Attenuated Total Reflectance (ATR)–Fourier Transform Infrared (FTIR) spectroscopic techniques. Forsterite composition was estimated to be 75% by using Raman and IR correlation data. Possible high impact shock pressure for Bursa meteorite was found to be at least 64.9 GPa. Besides, based on the olivine doublet (820 and 852 cm?1) and Full Width at Half Maximum data (~20 and ~60 cm?1, respectively) for maskelynite (509 and 580 cm?1) observed in the Raman spectrum, we assigned the shock stage of this meteorite as at least S5, for the first time. Moreover, previously reported hypervelocity impact experiments also suppo...
Chrome-spinel grains from the fossil ungrouped achondrite Österplana 065 (Öst 065) recovered from Mi...
This study used Raman spectral analysis to characterise the structural order of carbon in three carb...
Olivine is one of the most refractory and abundant igneous rock-forming minerals, which has been pro...
Shock impact-produced mineral alterations in two thin sections of the recently found Csátalja H4 ord...
Shock metamorphism of minerals in meteorites could help to understand the shock history of its paren...
Shock metamorphism of minerals in meteorites could help to understand the shock history of its paren...
Abstract We studied optical microscopic and micro-Raman spectroscopic signatures of shocked olivin...
© The Author(s).The Cangas de Onís regolith breccia is an H5-H6 ordinary chondrite that fell to Eart...
Raman spectroscopy and scanning electron microscopy methods were used to study the fragment of the M...
Chromites from Middle Ordovician fossil L chondrites and from matrix and shock-melt veins in Catherw...
In this paper, we present results of a characterization by Raman spectroscopy of mineral phases in t...
Classification of ordinary chondrite meteorites generally implies (1) determining the chemical group...
We investigated shock metamorphism of two lunar meteorites (Asuka-881757 and Yamato-86032). We measu...
NASA’s Stardust mission returned from the comet 81P/Wild2 in 2006 and has yielded a plethora of rese...
NASA’s Stardust mission returned from the comet 81P/Wild2 in 2006 and has yielded a plethora of rese...
Chrome-spinel grains from the fossil ungrouped achondrite Österplana 065 (Öst 065) recovered from Mi...
This study used Raman spectral analysis to characterise the structural order of carbon in three carb...
Olivine is one of the most refractory and abundant igneous rock-forming minerals, which has been pro...
Shock impact-produced mineral alterations in two thin sections of the recently found Csátalja H4 ord...
Shock metamorphism of minerals in meteorites could help to understand the shock history of its paren...
Shock metamorphism of minerals in meteorites could help to understand the shock history of its paren...
Abstract We studied optical microscopic and micro-Raman spectroscopic signatures of shocked olivin...
© The Author(s).The Cangas de Onís regolith breccia is an H5-H6 ordinary chondrite that fell to Eart...
Raman spectroscopy and scanning electron microscopy methods were used to study the fragment of the M...
Chromites from Middle Ordovician fossil L chondrites and from matrix and shock-melt veins in Catherw...
In this paper, we present results of a characterization by Raman spectroscopy of mineral phases in t...
Classification of ordinary chondrite meteorites generally implies (1) determining the chemical group...
We investigated shock metamorphism of two lunar meteorites (Asuka-881757 and Yamato-86032). We measu...
NASA’s Stardust mission returned from the comet 81P/Wild2 in 2006 and has yielded a plethora of rese...
NASA’s Stardust mission returned from the comet 81P/Wild2 in 2006 and has yielded a plethora of rese...
Chrome-spinel grains from the fossil ungrouped achondrite Österplana 065 (Öst 065) recovered from Mi...
This study used Raman spectral analysis to characterise the structural order of carbon in three carb...
Olivine is one of the most refractory and abundant igneous rock-forming minerals, which has been pro...