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Coordinated X-ray, Ion, and Electron Microanalysis Approach Towards Understanding the Earliest-Formed Solids in the Solar System

Published online by Cambridge University Press:  04 August 2017

P. Mane ,
S. Wallace ,
M. Bose ,
K. Domanik ,
T. J. Zega  and
M. Wadhwa
P. Mane
Affiliation:
Lunar and Planetary Laboratory, University of Arizona, Tucson, USA. School of Earth and Space Exploration, Arizona State University, Tempe, USA.
S. Wallace
Affiliation:
EDAX, Ametek, Materials Analysis Division, Mahwah, USA.
M. Bose
Affiliation:
School of Molecular Sciences, Arizona State University, Tempe, USA.
K. Domanik
Affiliation:
Lunar and Planetary Laboratory, University of Arizona, Tucson, USA.
T. J. Zega
Affiliation:
Lunar and Planetary Laboratory, University of Arizona, Tucson, USA. Dept. of Materials Science and Engineering, University of Arizona, Tucson, USA.
M. Wadhwa
Affiliation:
School of Earth and Space Exploration, Arizona State University, Tempe, USA.

Abstract

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Abstract
Information
Microscopy and Microanalysis , Volume 23 , Supplement S1: Proceedings of Microscopy & Microanalysis 2017 , July 2017 , pp. 2136 - 2137
Copyright
© Microscopy Society of America 2017 

References

[1] Connelly, J. N., et al, Science 338 2012). p. 651–655.CrossRefGoogle Scholar
[2] Wark, D. A. & Lovering, J. F. LPSC VII 1977). p. 95–112.Google Scholar
[3] MacPherson, G. J., Meteorites and Cosmochemical Processes 2014). p. 139–179.Google Scholar
[4] Bolser, D., et al, Meteoritics & Planetary Science 51 2016). p. 743–756.CrossRefGoogle Scholar
[5] This research supported by National Science Foundation grant number 1531243 and NASA grant numbers NNX15AJ22G and NNX12AL47G. We acknowlegde Paul Wallace at University of Arizona for his help in setting ud the EBSD.Google Scholar