Carbonaceous chondrites are some of the most primitive meteorites and derive from planetesimals that formed a few million years after the beginning of the solar system. Here …
The mineralogy and bulk compositions of the matrices of the CR chondrites MET 00426 and QUE 99177 have been studied using a combination of SEM, EPMA, and TEM techniques …
Among primitive meteorites, CR chondrites have peculiar isotopic compositions, the origin of which is uncertain and may have involved contributions from primordial molecular cloud …
Chondrites are meteorites from undifferentiated parent bodies that provide fundamental information about early Solar System evolution and planet formation. The element Cr is …
Abstract NanoSIMS C-, N-, and O-isotopic mapping of matrix in CO3. 0 chondrite Dominion Range (DOM) 08006 revealed it to have in its matrix the highest abundance of presolar O …
We have carried out a NanoSIMS C, N and O ion imaging study of the CO3. 0 chondrite ALHA77307. The distribution of O-anomalous grains in ALHA77307 is similar to that …
The organic matter in the primitive CR3 chondrites QUE 99177 and MET 00426 exhibits, as in other CR chondrites, N isotopic compositions characterized by large enrichments in 15 N …
MK Weisberg, M Prinz, RN Clayton… - … et Cosmochimica Acta, 1993 - Elsevier
A petrologic, geochemical and oxygen isotopic study of eight meteorites, identified as CR (Renazzo-type) chondrites, reveals that they have a set of similar properties that …
We used the electron microprobe to study matrix in the ungrouped type 3.0 carbonaceous chondrite Acfer 094 using 7× 7‐point, focused‐beam arrays; data points attributable to …