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Micro and Nanoscale Studies of Shock Features within the Chelyabinsk LL5 Meteorite

Published online by Cambridge University Press:  27 August 2014

S. S. Rout  and
P. R. Heck
S. S. Rout
Affiliation:
Robert A. Pritzker Center for Meteoritics and Polar Studies, The Field Museum of Natural History, 1400 S Lake Shore Drive, Chicago, IL 60605, USA. Chicago Center for Cosmochemistry, The University of Chicago, 5734 S Ellis Avenue, Chicago, IL 60637, USA.
P. R. Heck
Affiliation:
Robert A. Pritzker Center for Meteoritics and Polar Studies, The Field Museum of Natural History, 1400 S Lake Shore Drive, Chicago, IL 60605, USA. Chicago Center for Cosmochemistry, The University of Chicago, 5734 S Ellis Avenue, Chicago, IL 60637, USA.

Abstract

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Abstract
Information
Microscopy and Microanalysis , Volume 20 , Supplement S3: Proceedings of Microscopy & Microanalysis 2014 , August 2014 , pp. 1712 - 1713
Copyright
Copyright © Microscopy Society of America 2014 

References

[1] Sharp, T. G., DeCarli, P. S. in “Meteorites and the Early Solar System II”, ed. D. S. Lauretta andH. Y. McSween (The University of Arizona Press, Arizona) p. 653-678.Google Scholar
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[8] The authors acknowledge funding from the Tawani Foundation and from W. H. Ganz III. We thank T. Boudreaux for providing samples of Chelyabinsk, the National Museum of Natural History of the Smithsonian Institution and I. Steele, The University of Chicago, for providing analytical standards. We thank B. Strack for maintenance of the SEM. This work made use of the EPIC facility (NUANCE Center-Northwestern University) and the Nanoscale Science and Engineering Center, both supported by the National Science Foundation; the state of Illinois; and Northwestern University.Google Scholar