The nature, origin and modification of insoluble organic matter in chondrites, the major source of Earth’s C and N

Author:

Alexander C.M.O’D.,Cody G.D.,De Gregorio B.T.,Nittler L.R.,Stroud R.M.

Funder

NASA Cosmochemistry

NASA Origins of Solar Systems

Publisher

Elsevier BV

Subject

Geochemistry and Petrology,Geophysics

Reference281 articles.

1. Characterisation of matrix in the EET 92042 CR2 carbonaceous chondrite: insights into textural and mineralogical heterogeneity;Abreu;Meteor. Planet. Sci.,2004

2. 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

3. Opaque assemblages in CR2 Graves Nunataks (GRA) 06100 as indicators of shock-driven hydrothermal alteration in the CR chondrite parent body;Abreu;Meteor. Planet. Sci.,2013

4. Clues to the origin of interplanetary dust particles from the isotopic study of their hydrogen-bearing phases;Aléon;Geochim. Cosmochim. Acta,2001

5. Nitrogen isotopic composition of macromolecular organic matter in interplanetary dust particles;Aléon;Geochim. Cosmochim. Acta,2003

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