Carbonate abundances and isotopic compositions in chondrites

Author:

Alexander C. M. O'D.1,Bowden R.2,Fogel M. L.2,Howard K. T.3

Affiliation:

1. DTM; Carnegie Institution of Washington; 5241 Broad Branch Road Washington District of Columbia 20015 USA

2. GL; Carnegie Institution of Washington; 5251 Broad Branch Road Washington District of Columbia 20015 USA

3. Kingsborough Community College of the City University of New York; Brooklyn New York 11235 USA

Funder

National Aeronautics and Space Administration

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Reference97 articles.

1. Early solar system processes recorded in the matrices of two highly pristine CR3 carbonaceous chondrites, MET 00426 and QUE 99177;Abreu;Geochimica et Cosmochimica Acta,2010

2. Opaque assemblages in CR2 Graves Nunataks (GRA) 06100 as indicators of shock-driven hydrothermal alteration in the CR chondrite parent body;Abreu;Meteoritics & Planetary Science,2013

3. Alteration histories of the CR chondrites I: The shocked and the aqueously altered (abstract #5312);Abreu;Meteoritics & Planetary Science Supplement,2012

4. The origin of chondritic macromolecular organic matter: A carbon and nitrogen isotope study;Alexander;Meteoritics & Planetary Science,1998

5. The origin and evolution of chondrites recorded in the elemental and isotopic compositions of their macromolecular organic matter;Alexander;Geochimica et Cosmochimica Acta,2007

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