The secondary history of Sutter's Mill CM carbonaceous chondrite based on water abundance and the structure of its organic matter from two clasts

Author:

Beck P.1,Quirico E.1,Garenne A.1,Yin Q.-Z.2,Bonal L.1,Schmitt B.1,Montes-Hernandez G.3,Montagnac G.4,Chiriac R.5,Toche F.5

Affiliation:

1. UJF-Grenoble 1/CNRS-INSU; Institut de Planétologie et d'Astrophysique de Grenoble (IPAG) UMR 5274; Grenoble F-38041 France

2. Department of Earth and Planetary Sciences; University of California at Davis; Davis California 95616 USA

3. Institut des Sciences de la Terre (ISTerre); OSUG/CNRS, UJF; BP 53X 38041 Grenoble France

4. Laboratoire de Géologie; UMR 5276; Ecole normale supérieure de Lyon; Lyon France

5. Laboratoire des Multimatériaux et Interfaces UMR CNRS 5615; Université de Lyon; Université Lyon 1; 43 Bd du 11 novembre 1918 69622 Villeurbanne Cedex France

Funder

ANR-10-JCJC-0505-01

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Reference47 articles.

1. T-T-T diagram of serpentine and saponite, and estimation of metamorphic heating degree of Antarctic carbonaceous chondrites;Akai;Antarctic Meteorite Research,1992

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

3. The classification of CM and CR chondrites using bulk H, C, and N abundances and isotopic compositions;Alexander;Geochimica et Cosmochimica Acta,2013

4. Shock-induced compaction, melting, and entrapment of atmospheric gases in Martian meteorites;Beck;Geophysical Research Letters,2007

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