International audienceA slice of the Haverö meteorite which belongs to the ureilite class known to contain graphite and diamond was cut and then polished as a thin section using a diamond paste. We identified two carbonaceous areas which were standing out by more than 10 µm in relief over the surface of the silicate matrix suggesting that the carbonaceous phases were not easily polishable by a diamond paste and would therefore imply larger polishing hardness. These areas were investigated by reflected light microscopy, high-resolution Field Emission SEM (FESEM), energy-dispersive X-ray (EDX) analysis, Raman spectroscopy, and were subsequently extracted for in situ synchrotron microbeam X-ray fluorescence (XRF), imaging and X-ray diffraction...
ABSTRACT—Unusual cuboid graphite aggregates (up to 13 mm edge length) from the eclogitic gneiss unit...
The occurrence of diamonds in terrestrial impact craters and meteorites is related to dynamic shock ...
Studies of dense carbon materials formed by bolide impacts or produced by laboratory compression pro...
International audienceA slice of the Haverö meteorite which belongs to the ureilite class known to c...
Ureilites meteorite fragments present different levels of shock classified on the basis of optical o...
The formation and shock history of ureilite meteorites, a relatively abundant type of primitive acho...
International audienceMineralogical structures of carbon phases within the ureilite North West Afric...
One of the main problems in studying diamonds in ureilites (and in general in meteorites) is the con...
The occurrence of shock-induced diamonds in ureilite meteorites is common and is used to constrain t...
第8回極域科学シンポジウム/個別セッション:[OA] 南極隕石12月5日(火)国立極地研究所 1階交流アトリウムThe Eighth Symposium on Polar Science/Ordina...
This work is the first detailed study of carbon phases in the ureilite Almahata Sitta (sample #7). W...
The origin of diamonds in ureilite meteorites is a timely topic in planetary geology as recent studi...
This study used Raman spectral analysis to characterise the structural order of carbon in three carb...
Planetesimal were the first planetary objects to form in the solar system, which later grew to make ...
Meteorites provide precious clues about the formation of planets in the solar system. In particular,...
ABSTRACT—Unusual cuboid graphite aggregates (up to 13 mm edge length) from the eclogitic gneiss unit...
The occurrence of diamonds in terrestrial impact craters and meteorites is related to dynamic shock ...
Studies of dense carbon materials formed by bolide impacts or produced by laboratory compression pro...
International audienceA slice of the Haverö meteorite which belongs to the ureilite class known to c...
Ureilites meteorite fragments present different levels of shock classified on the basis of optical o...
The formation and shock history of ureilite meteorites, a relatively abundant type of primitive acho...
International audienceMineralogical structures of carbon phases within the ureilite North West Afric...
One of the main problems in studying diamonds in ureilites (and in general in meteorites) is the con...
The occurrence of shock-induced diamonds in ureilite meteorites is common and is used to constrain t...
第8回極域科学シンポジウム/個別セッション:[OA] 南極隕石12月5日(火)国立極地研究所 1階交流アトリウムThe Eighth Symposium on Polar Science/Ordina...
This work is the first detailed study of carbon phases in the ureilite Almahata Sitta (sample #7). W...
The origin of diamonds in ureilite meteorites is a timely topic in planetary geology as recent studi...
This study used Raman spectral analysis to characterise the structural order of carbon in three carb...
Planetesimal were the first planetary objects to form in the solar system, which later grew to make ...
Meteorites provide precious clues about the formation of planets in the solar system. In particular,...
ABSTRACT—Unusual cuboid graphite aggregates (up to 13 mm edge length) from the eclogitic gneiss unit...
The occurrence of diamonds in terrestrial impact craters and meteorites is related to dynamic shock ...
Studies of dense carbon materials formed by bolide impacts or produced by laboratory compression pro...