Redox-influenced trace element compositional differences among variably aqueously altered CM chondrites

Author:

Friedrich Jon M.,Abreu Neyda M.,Wolf Stephen F.,Troiano Julianne M.,Stanek Gregory L.

Funder

Claire Boothe Luce Undergraduate Scholarship

Dubois Educational Foundation

NSF

NASA

Department of Mineral Sciences of the Smithsonian Institution

Astromaterials Curation Office at NASA Johnson Space Center

Publisher

Elsevier BV

Subject

Geochemistry and Petrology

Reference72 articles.

1. Abreu N. M., Friedrich J. M., and Crispin K. (2017) Understanding the origin and distribution of primary phases in CM chondrites: weakly altered CMs from LaPaz Fields, LAP 04514, LAP 04527, LAP 04565, and LAP 02333. In 48th Lunar and Planetary Science Conference, #2935 (abstr.).

2. Reconstructing the rise of recent coastal anoxia: molybdenum in Chesapeake Bay Sediments;Adelson;Geochim. Cosmochim. Acta,2001

3. The provenances of asteroids, and their contributions to the volatile inventories of the terrestrial planets;Alexander;Science,2012

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

5. Weathering of meteorites from Oman: correlation of chemical/mineralogical weathering proxies with 14C terrestrial ages and the influence of soil chemistry;Al-Kathiri;Meteorit. Planet. Sci.,2005

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