The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system

Author:

Abreu N.M.,Aponte J.C.,Cloutis E.A.,Nguyen A.N.

Funder

National Aeronautics and Space Administration

Publisher

Elsevier BV

Subject

Geochemistry and Petrology,Geophysics

Reference295 articles.

1. Fine-Scale Mineralogical Study of the Matrices of CR Carbonaceous Chondrites: Insights on Early Solar System Processes Proquest Dissertations And Theses 2007. Section 0142, Part 0372 225 Pages; [Ph.D. Dissertation];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. Why is it so difficult to classify renazzo-type (CR) carbonaceous chondrites? - Implications from TEM observations of matrices for the sequences of aqueous alteration;Abreu;Geochim. Cosmochim. Acta,2016

4. Are phyllosilicates in CR chondrite matrices generated by hydrothermal alteration? (Abstract);Abreu;47Th Lunar Planet. Sci. Conf.,2016

5. 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

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