Abstract
The petrologic sequence observed in the CO3 chondrite group has been suggested to be the result of thermal metamorphism on a parent body. We have developed a model to examine the possibility that chondrule and matrix olivines equilibrated in situ, during parent body metamorphism. The model considers Fe-Mg interdiffusion between chondrule and matrix olivines. Zoning profiles comparable to those observed in chondrule olivines from partially equilibrated members of the series are reproduced successfully. Metamorphism of CO3 chondrites on a parent body is therefore a viable model for the observed equilibration. Results indicate that peak metamorphic temperatures experienced by the CO3 chondrites were around 500-degrees-C, and that the range of peak temperatures between unequilibrated and equilibrated subtypes was relatively narrow, around 100-degrees-C.
Original language | English |
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Pages (from-to) | 73-86 |
Number of pages | 14 |
Journal | Earth and Planetary Science Letters |
Volume | 106 |
Issue number | 1-4 |
DOIs | |
Publication status | Published - 1991 |