The olivine-bronzite and olivine-hypersthene chondrites comprise about 95 per cent of all chondrites, the remaining groups (enstatite, olivine-pigeonite, and carbonaceous chondrites) each having compara-tively few representatives (Mason, 1962). These two major classes (here
Yamato-694 meteorite collected near the Yamato Mountains in Antarctica in 1969 is an ordinary chondr...
The authors carried out petrographic, mineralogical, and chemical analyses (bulk chemical compositio...
The Yamato-75108 to-75257 chondrites are considered to be originally one meteorite which was broken ...
The matrices of six unequilibrated O chondrites and one C chondrite, ALH-764 (LL3), Y-74191 (L3), AL...
The major element chemical compositions of most chondrules correspond to the compositions of mixture...
An electron microprobe analyzer was used to determine the chemical compositions of olivines and orth...
This paper presents a mineralogical analysis of various chondrule types and chemical analysis of oli...
All the chondrites from the Yamato-75108 to -75257 have been considered to be originally one single ...
International audienceWe performed a petrologic, geochemical, and oxygen isotopic study of the lowes...
We performed a petrologic, geochemical, and oxygen isotopic study of the lowest FeO ordinary chondri...
Olivine absorptions are known to dominate telescopic spectra of several asteroids. Among the meteori...
The chondrules in the Yamato-74191 meteorite (L3) are classified into seven groups by their SiO_2 co...
Electron microprobe studies have been made of olivines and pyroxenes in thirty three Yamato chondrit...
The unique mineral and chemical composition of enstatite chondrites has been difficult to explain. C...
The Yamato-75108 to -75257 chondrites are considered to be originally one meteorite which was broken...
Yamato-694 meteorite collected near the Yamato Mountains in Antarctica in 1969 is an ordinary chondr...
The authors carried out petrographic, mineralogical, and chemical analyses (bulk chemical compositio...
The Yamato-75108 to-75257 chondrites are considered to be originally one meteorite which was broken ...
The matrices of six unequilibrated O chondrites and one C chondrite, ALH-764 (LL3), Y-74191 (L3), AL...
The major element chemical compositions of most chondrules correspond to the compositions of mixture...
An electron microprobe analyzer was used to determine the chemical compositions of olivines and orth...
This paper presents a mineralogical analysis of various chondrule types and chemical analysis of oli...
All the chondrites from the Yamato-75108 to -75257 have been considered to be originally one single ...
International audienceWe performed a petrologic, geochemical, and oxygen isotopic study of the lowes...
We performed a petrologic, geochemical, and oxygen isotopic study of the lowest FeO ordinary chondri...
Olivine absorptions are known to dominate telescopic spectra of several asteroids. Among the meteori...
The chondrules in the Yamato-74191 meteorite (L3) are classified into seven groups by their SiO_2 co...
Electron microprobe studies have been made of olivines and pyroxenes in thirty three Yamato chondrit...
The unique mineral and chemical composition of enstatite chondrites has been difficult to explain. C...
The Yamato-75108 to -75257 chondrites are considered to be originally one meteorite which was broken...
Yamato-694 meteorite collected near the Yamato Mountains in Antarctica in 1969 is an ordinary chondr...
The authors carried out petrographic, mineralogical, and chemical analyses (bulk chemical compositio...
The Yamato-75108 to-75257 chondrites are considered to be originally one meteorite which was broken ...