Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
5745608 | Chemie der Erde - Geochemistry | 2017 | 30 Pages |
Abstract
Here we review what is known about the abundances, compositions and physical nature of IOM in the most primitive chondrites. We also discuss how the IOM has been modified by thermal metamorphism and aqueous alteration in the chondrite parent bodies, and how these changes may be used both as petrologic indicators of the intensity of parent body processing and as tools for classification. Finally, we critically assess the various proposed mechanisms for the formation of IOM in the ISM or Solar System.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geochemistry and Petrology
Authors
C.M.O'D. Alexander, G.D. Cody, B.T. De Gregorio, L.R. Nittler, R.M. Stroud,