This work is the first detailed study of carbon phases in the ureilite Almahata Sitta (sample #7). We present microRaman data for diamond and graphite in Almahata Sitta, seven unbrecciated ureilites, and two brecciated ureilites. Diamond in Almahata Sitta was found to be distinct from that in unbrecciated and brecciated ureilites, although diamond in unbrecciated and brecciated ureilites is indistinguishable. Almahata Sitta diamond shows a peak center range of 1318.5–1330.2 cm−1 and a full width at half maximum (FWHM) range of 6.6–17.4 cm−1, representing a shock pressure of at least 60 kbar. The actual peak shock pressure may be higher than this due to postshock annealing, if shock synthesis is the source of ureilite diamonds. Diamond in un...
International audienceA slice of the Haverö meteorite which belongs to the ureilite class known to c...
Nitrogen and noble gases were measured in a bulk sample and in acid-resistant carbon-rich residues o...
International audiencePlanetary formation models show that terrestrial planets are formed by the acc...
The formation and shock history of ureilite meteorites, a relatively abundant type of primitive acho...
One of the main problems in studying diamonds in ureilites (and in general in meteorites) is the con...
The origin of diamonds in ureilite meteorites is a timely topic in planetary geology as recent studi...
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...
A new olivine-pigeonite ureilite containing abundant diamonds and graphite was found in the United A...
The 11th Symposium on Polar Science/Ordinary sessions: [OA] Antarctic meteorites, Thu. 3 Dec
The thermal history of carbon phases, including graphite and diamond, in the ureilite meteorites has...
Ureilite meteorites are arguably our only large suite of samples from the mantle of a dwarf planet a...
The occurrence of diamonds in terrestrial impact craters and meteorites is related to dynamic shock ...
International audienceMineralogical structures of carbon phases within the ureilite North West Afric...
In this paper Raman spectra of diamonds from two different ureilites, JaH 054 and Sahara 98505, were...
International audienceA slice of the Haverö meteorite which belongs to the ureilite class known to c...
Nitrogen and noble gases were measured in a bulk sample and in acid-resistant carbon-rich residues o...
International audiencePlanetary formation models show that terrestrial planets are formed by the acc...
The formation and shock history of ureilite meteorites, a relatively abundant type of primitive acho...
One of the main problems in studying diamonds in ureilites (and in general in meteorites) is the con...
The origin of diamonds in ureilite meteorites is a timely topic in planetary geology as recent studi...
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...
A new olivine-pigeonite ureilite containing abundant diamonds and graphite was found in the United A...
The 11th Symposium on Polar Science/Ordinary sessions: [OA] Antarctic meteorites, Thu. 3 Dec
The thermal history of carbon phases, including graphite and diamond, in the ureilite meteorites has...
Ureilite meteorites are arguably our only large suite of samples from the mantle of a dwarf planet a...
The occurrence of diamonds in terrestrial impact craters and meteorites is related to dynamic shock ...
International audienceMineralogical structures of carbon phases within the ureilite North West Afric...
In this paper Raman spectra of diamonds from two different ureilites, JaH 054 and Sahara 98505, were...
International audienceA slice of the Haverö meteorite which belongs to the ureilite class known to c...
Nitrogen and noble gases were measured in a bulk sample and in acid-resistant carbon-rich residues o...
International audiencePlanetary formation models show that terrestrial planets are formed by the acc...