Large spinel grains in a CM chondrite (Acfer 331): Implications for reconstructions of ancient meteorite fluxes-Reference-Cited by-同舟云学术

Large spinel grains in a CM chondrite (Acfer 331): Implications for reconstructions of ancient meteorite fluxes

Published:2013-02 Issue:2 Volume:48 Page:180-194
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit Planet Sci

Author:

Bjärnborg Karolina¹,Schmitz Birger²³

Affiliation:

1. Department of Geology; University of Lund; Sölvegatan 12 Lund SE-22362 Sweden

2. Department of Physics; University of Lund; P.O. Box 118 Lund SE-22100 Sweden

3. Robert A. Pritzker Center for Meteoritics and Polar Studies; Department of Geology; The Field Museum; 1400 S. Lake Shore Drive Chicago Illinois 60605 USA

Funder

Swedish Research Council

European Research Council

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1111/maps.12050/fullpdf

Reference47 articles.

1. Cr-rich spinels as petrogenetic indicators-MORB-type lavas from the Lamont seamount chain, eastern Pacific;Allan;American Mineralogist,1988

2. Relict silicate inclusions in extraterrestrial chromite and their use in the classification of fossil chondritic material;Alwmark;Geochimica et Cosmochimica Acta,2009

3. A 3-D study of mineral inclusions in chromite from ordinary chondrites using synchrotron radiation X-ray tomographic microscopy-Method and applications;Alwmark;Meteoritics & Planetary Science,2011

4. The range of spinel compositions in terrestrial mafic and ultramafic rocks;Barnes;Journal of Petrology,2001

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