The main mineralogical characteristics of a large light-colored clast within the Murchison CM breccia are discussed in detail including data on the mineralogy, bulk chemistry, organics, and oxygen isotopes. Petrographic study shows that the white clast consists of two areas with different granoblastic textures: (1) a coarse-grained (average grain size: similar to 200 mu m) and (2) a fine-grained lithology (average grain-size: similar to 20 mu m). The Fa-content of olivine in the clast is the same as Fa within olivine from Rumuruti (R) chondrites (Fa: similar to 38 mol%); however, the concentrations of the elements Ni and Ca in olivine are significantly different. The fragment also contains Ca-rich pyroxene, similar to An(30-38)-plagioclase/...
The authors carried out petrographic, mineralogical, and chemical analyses (bulk chemical compositio...
We studied the texture of 256 chondrules in thin sections of 16 different carbonaceous (CV, CR, CO, ...
Several stages in the evolution of ordinary chondritic meteorites are recorded in the oxygen isotopi...
The CM chondrites are generally complex impact breccias, in which lithic clasts and mineral fragment...
R-chondrites share some properties with ordinary chondrites (OC) and carbonaceous chondrites (CC). T...
We have performed in situ analyses of C and O isotopic compositions, trace element concentrations, a...
This study investigates the pre-accretionary formation conditions of individual minerals within chon...
International audienceRumurutiites (R chondrites) are rare, highly oxidized chondrites belonging to ...
We report a petrography, mineral chemistry, oxygen and chromium isotopic study of Grove Mountains (G...
Neutron activation analysis was used to determine 13 trace elements (Ag, As, Au, Bi, Co, Cs, Ga, In,...
A metamorphosed lithic clast was discovered in the CM chondrite Grove Mountains 021536, which was co...
Iron isotope compositions of bulk chondrules are so far only known from few studies on CV and some ...
Nineteen nonporphyritic pyroxene and pyroxene/olivine chondrules, chondrule fragments, and irregular...
Abstract-Most spine1 grains in Murchison acid residues are Mg-, Al-rich, 160-rich (6 “0 =-5O%,), sma...
Neutron activation analysis was used to determine 11 trace elements (Ag, Bi, Cd, Co, Cs, Ga, In, Se,...
The authors carried out petrographic, mineralogical, and chemical analyses (bulk chemical compositio...
We studied the texture of 256 chondrules in thin sections of 16 different carbonaceous (CV, CR, CO, ...
Several stages in the evolution of ordinary chondritic meteorites are recorded in the oxygen isotopi...
The CM chondrites are generally complex impact breccias, in which lithic clasts and mineral fragment...
R-chondrites share some properties with ordinary chondrites (OC) and carbonaceous chondrites (CC). T...
We have performed in situ analyses of C and O isotopic compositions, trace element concentrations, a...
This study investigates the pre-accretionary formation conditions of individual minerals within chon...
International audienceRumurutiites (R chondrites) are rare, highly oxidized chondrites belonging to ...
We report a petrography, mineral chemistry, oxygen and chromium isotopic study of Grove Mountains (G...
Neutron activation analysis was used to determine 13 trace elements (Ag, As, Au, Bi, Co, Cs, Ga, In,...
A metamorphosed lithic clast was discovered in the CM chondrite Grove Mountains 021536, which was co...
Iron isotope compositions of bulk chondrules are so far only known from few studies on CV and some ...
Nineteen nonporphyritic pyroxene and pyroxene/olivine chondrules, chondrule fragments, and irregular...
Abstract-Most spine1 grains in Murchison acid residues are Mg-, Al-rich, 160-rich (6 “0 =-5O%,), sma...
Neutron activation analysis was used to determine 11 trace elements (Ag, Bi, Cd, Co, Cs, Ga, In, Se,...
The authors carried out petrographic, mineralogical, and chemical analyses (bulk chemical compositio...
We studied the texture of 256 chondrules in thin sections of 16 different carbonaceous (CV, CR, CO, ...
Several stages in the evolution of ordinary chondritic meteorites are recorded in the oxygen isotopi...