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dc.contributor.authorKaczmarek, M.
dc.contributor.authorGrange, M.
dc.contributor.authorReddy, S.
dc.contributor.authorNemchin, Alexander
dc.date.accessioned2017-01-30T15:34:11Z
dc.date.available2017-01-30T15:34:11Z
dc.date.created2015-10-29T04:09:32Z
dc.date.issued2012
dc.identifier.citationKaczmarek, M. and Grange, M. and Reddy, S. and Nemchin, A. 2012. Preferred Mineral Orientations in Martian Shergottites: Magmatism or Schock?, in Proceedings of the 75th Annual Meeting of the Meteoritical-Society, Aug 12-17 2012, id 5145. Cairns, Australia: Lunar and Planetary Institute.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/47563
dc.description.abstract

We have studied the textures and the preferred orientation of pyroxene in subsamples of Zagami and Nakhla using Electron Backscatter Diffraction (EBSD) method. Data show the activation of several slip systems, related to magmatism or shock event.

dc.publisherWILEY-BLACKWELL
dc.relation.urihttp://www.lpi.usra.edu/meetings/metsoc2012/pdf/5145.pdf
dc.titlePreferred Mineral Orientations in Martian Shergottites: Magmatism or Schock?
dc.typeConference Paper
dcterms.source.volume47
dcterms.source.startPageA218
dcterms.source.endPageA218
dcterms.source.issn1086-9379
dcterms.source.titleMETEORITICS & PLANETARY SCIENCE
dcterms.source.seriesMETEORITICS & PLANETARY SCIENCE
dcterms.source.conference75th Annual Meeting of the Meteoritical-Society
curtin.departmentDepartment of Applied Geology
curtin.accessStatusFulltext not available


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