Early Solar System Processes Recorded in the Matrices of CR2 Chondrites MET 00426 and QUE 99177

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Scientific paper

TEM and HRTEM observations of matrix and dark inclusions in the MET
00426 and QUE 99177 indicate that the fine-grained component of these
meteorites is largely composed of amorphous silicate material. This
amorphous material is the potential precursor of phyllosilicates.

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