Kaba is unique in containing almost pure fayalitic olivine (Fo(sub 0.1)). Its coexistence with pure forsterite up to Fo(sub 99.6) and normal (Fo(sub 92) to Fo(sub 59)) and reversely (Fo(sub 0.4) to Fo(sub 4.7)) zoned olivines suggest that the Kaba olivines are in thermodynamic disequilibrium and experienced a complicated history. The fayalite is sufficiently pure that it is unlikely that it could have been produced by fractional crystallization. A gas-solid reaction under oxidizing conditions (H2O/H2 ratio approximately 10) is probably responsible for its formation
Electron microprobe studies of several H5 and H6 chondrites reveal that olivine crystals exhibit sys...
Iron-rich olivine is one of the major minerals in the matrices of unequilibrated ordinary (UOCs) and...
International audienceWe have studied porphyritic olivine-rich chondrules of the carbonaceous chondr...
The Tenth Symposium on Polar Science/Poster presentations: [OA] Antarctic meteorites, Wed. 4 Dec. / ...
Thermochemical equilibria are calculated in the multicomponent gas-solution-rock system in order to ...
Ohvine is the most abundant mineral in many chondritic meteorites. It is also the first major Mg-sil...
The micron-size constituents of fine-grained matrices and chondrule rims in ten unequilibrated ordin...
The CV carbonaceous chondrites experienced alteration that resulted in formation of secondary ferrou...
Solar gas is too reducing for the equilibrium XFa in condensate olivine to reach the mini-mum XFa of...
Although considerable progress has been made in unraveling the origin(s) of fayalitic olivines in da...
Amoeboid Olivine aggregates (AOAs) are irregularly shaped objects commonly observed in carbonaceous ...
Iron-poor and refractory lithophile element (RLE) rich forsterite grains occur in all major types of...
International audienceMg-rich olivine is a ubiquitous phase in type I porphyritic chondrules in vari...
Low-iron, manganese-enriched (LIME) olivine grains are found in cometary samples returned by the Sta...
The Murchison chondrite meteorite has been studied extensively. It consists of olivine˗pyroxene aggr...
Electron microprobe studies of several H5 and H6 chondrites reveal that olivine crystals exhibit sys...
Iron-rich olivine is one of the major minerals in the matrices of unequilibrated ordinary (UOCs) and...
International audienceWe have studied porphyritic olivine-rich chondrules of the carbonaceous chondr...
The Tenth Symposium on Polar Science/Poster presentations: [OA] Antarctic meteorites, Wed. 4 Dec. / ...
Thermochemical equilibria are calculated in the multicomponent gas-solution-rock system in order to ...
Ohvine is the most abundant mineral in many chondritic meteorites. It is also the first major Mg-sil...
The micron-size constituents of fine-grained matrices and chondrule rims in ten unequilibrated ordin...
The CV carbonaceous chondrites experienced alteration that resulted in formation of secondary ferrou...
Solar gas is too reducing for the equilibrium XFa in condensate olivine to reach the mini-mum XFa of...
Although considerable progress has been made in unraveling the origin(s) of fayalitic olivines in da...
Amoeboid Olivine aggregates (AOAs) are irregularly shaped objects commonly observed in carbonaceous ...
Iron-poor and refractory lithophile element (RLE) rich forsterite grains occur in all major types of...
International audienceMg-rich olivine is a ubiquitous phase in type I porphyritic chondrules in vari...
Low-iron, manganese-enriched (LIME) olivine grains are found in cometary samples returned by the Sta...
The Murchison chondrite meteorite has been studied extensively. It consists of olivine˗pyroxene aggr...
Electron microprobe studies of several H5 and H6 chondrites reveal that olivine crystals exhibit sys...
Iron-rich olivine is one of the major minerals in the matrices of unequilibrated ordinary (UOCs) and...
International audienceWe have studied porphyritic olivine-rich chondrules of the carbonaceous chondr...