Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-26T07:52:50.726Z Has data issue: false hasContentIssue false

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

Published online by Cambridge University Press:  27 August 2014

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

Image of the first page of this content. For PDF version, please use the ‘Save PDF’ preceeding this image.'
Type
Abstract
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
[2] Gillet, P., et al, Geological Survey of America Special Papers, 421 (2007), p57-82.Google Scholar
[3] Bischoff, A. Lunar and Planetary Science Conference XXXIII (2002), Abstract# 1264.Google Scholar
[4] Miyahara, M., et al, Earth and Planetary Science Letters, 373 (2013), p102-108.Google Scholar
[5] Galimov, E. M., et al, Geochemistry International, 51 (2013), p522-539.Google Scholar
[6] Bischoff, A., et al, Meteoritics and Planetary Science, 48 (2013), A61.Google Scholar
[7] Trigo-Rodriguez, J. M., et al, 45th Lunar and Planetary Science Conference (2014), Abstract# 1729.Google Scholar
[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