Why is it so difficult to classify Renazzo-type (CR) carbonaceous chondrites? – Implications from TEM observations of matrices for the sequences of aqueous alteration

Author:

Abreu Neyda M.

Funder

NNX11AH10G

Publisher

Elsevier BV

Subject

Geochemistry and Petrology

Reference68 articles.

1. Fine-Scale Mineralogical Study of the Matrices of CR Carbonaceous Chondrites: Insights on Early Solar System Processes;Abreu,2007

2. A unique omphacite, amphibole, and graphite-bearing clast in Queen Alexandra Range (QUE) 99177: a metamorphosed xenolith in a pristine CR3 chondrite;Abreu;Geochim. Cosmochim. Acta,2013

3. Early solar system processes recorded in the matrices of two highly pristine CR3 carbonaceous chondrites, MET 00426 and QUE 99177;Abreu;Geochim. Cosmochim. Acta,2010

4. Alteration histories of the CR Chondrites I: the shocked and the aqueously altered;Abreu;Meteorit. Planet. Sci. Suppl.,2012

5. The classification of CM and CR chondrites using bulk H, C and N abundances and isotopic compositions;Alexander;Geochim. Cosmochim. Acta,2013

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