A new olivine-pigeonite ureilite containing abundant diamonds and graphite was found in the United Arab Emirates. This is the first report of a meteorite in this country. The sample is heavily altered, of medium shock level, and has a total weight of 155 g. Bulk rock, olivine (Fo79.881.8) and pyroxene (En73.9-75.2, Fs15.5-16.9, Wo8.8-9.5) compositions are typical of ureilites. Olivine rims are reduced with Fo increasing up to Fo96.1-96.8. Metal in these rims is completely altered to Fehydroxide during terrestrial weathering. We studied diamond and graphite using micro-Raman and in situ synchrotron X-ray diffraction. The main diamond Raman band (LO=TO mode at ~1332 cm^(-1)) is broadened when compared to well-ordered diamond single crystals. ...
Ureilites are an abundant non-chondritic meteorite class that are petrographically similar to terres...
The thermal history of carbon phases, including graphite and diamond, in the ureilite meteorites has...
Mineral inclusions in Sao Luiz diamonds have been characterized using angle dispersive X-ray diffrac...
International audienceA new olivine-pigeonite ureilite containing abundant diamonds and graphite was...
The formation and shock history of ureilite meteorites, a relatively abundant type of primitive acho...
In this paper Raman spectra of diamonds from two different ureilites, JaH 054 and Sahara 98505, were...
This work is the first detailed study of carbon phases in the ureilite Almahata Sitta (sample #7). W...
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...
Ureilites meteorite fragments present different levels of shock classified on the basis of optical o...
The origin of diamonds in ureilite meteorites is a timely topic in planetary geology as recent studi...
Raman spectra were measured for diamonds in an inclusion of the Canyon Diablo iron meteorite. The wa...
The 11th Symposium on Polar Science/Ordinary sessions: [OA] Antarctic meteorites, Thu. 3 Dec
The occurrence of diamonds in terrestrial impact craters and meteorites is related to dynamic shock ...
Carbonaceous chondrite NWA 4967 was investigated by confocal Raman micro-spectroscopy. Olivine (Fa0-...
Ureilites are an abundant non-chondritic meteorite class that are petrographically similar to terres...
The thermal history of carbon phases, including graphite and diamond, in the ureilite meteorites has...
Mineral inclusions in Sao Luiz diamonds have been characterized using angle dispersive X-ray diffrac...
International audienceA new olivine-pigeonite ureilite containing abundant diamonds and graphite was...
The formation and shock history of ureilite meteorites, a relatively abundant type of primitive acho...
In this paper Raman spectra of diamonds from two different ureilites, JaH 054 and Sahara 98505, were...
This work is the first detailed study of carbon phases in the ureilite Almahata Sitta (sample #7). W...
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...
Ureilites meteorite fragments present different levels of shock classified on the basis of optical o...
The origin of diamonds in ureilite meteorites is a timely topic in planetary geology as recent studi...
Raman spectra were measured for diamonds in an inclusion of the Canyon Diablo iron meteorite. The wa...
The 11th Symposium on Polar Science/Ordinary sessions: [OA] Antarctic meteorites, Thu. 3 Dec
The occurrence of diamonds in terrestrial impact craters and meteorites is related to dynamic shock ...
Carbonaceous chondrite NWA 4967 was investigated by confocal Raman micro-spectroscopy. Olivine (Fa0-...
Ureilites are an abundant non-chondritic meteorite class that are petrographically similar to terres...
The thermal history of carbon phases, including graphite and diamond, in the ureilite meteorites has...
Mineral inclusions in Sao Luiz diamonds have been characterized using angle dispersive X-ray diffrac...