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Origin of ferrous zoning in Allende chondrule olivines

Journal Article · · Geochim. Cosmochim. Acta; (United States)
Olivine crystals in Allende Type 1 chondrules have ferrous rims (Fa/sub 15-44/), a few microns thick, at grain surfaces and along crosscutting cracks. This ferrous olivine contains as much as 2 atomic pct. Al and Cr, and 0.2 pct. Ti. Along cracks, profiles of Fe, Al, Cr, and Ti are consistent with diffusional emplacement: these elements moved from an external source through the cracks as a vapor or by grain boundary diffusion, then into the olivine by lattice diffusion. The emplacement did not occur during an epoch of planetary metamorphism that partly equilibrated matrix and chondrule olivines, because (e.g.) neither matrix nor primary magnesian chondrule olivine contains even 1/10 this much, Al, Cr, and Ti. The authors argue that the source of these elements was the nebular gas, and emplacement occurred prior to accretion. The ferrous zones at olivine grain boundaries do not display simple diffusion profiles: rather they appear to be a composite of two concentric rims. The inner rims have compositions similar to those of the ferrous zones along cracks, and contain the highest concentrations of Al, Cr, and Ti. The outer rims are of uniformly high Fa content and relatively low Al, Cr, and Ti concentration. These outer rims appear to be additional material that condensed onto the chondrules after the diffusional emplacement event discussed earlier. Matrix olivine grains, which are identical to these rims in composition, condensed simultaneously.
Research Organization:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (USA)
OSTI ID:
7160222
Journal Information:
Geochim. Cosmochim. Acta; (United States), Journal Name: Geochim. Cosmochim. Acta; (United States) Vol. 51:6; ISSN GCACA
Country of Publication:
United States
Language:
English