Shock effects in new Martian olivine basalt Northwest Africa 10416: distinct from shergottites but akin Northwest Africa 8159

dc.contributor.author	Walton, Erin L.
dc.contributor.author	Tschauner, Oliver
dc.contributor.author	Herd, Christopher D. K.
dc.contributor.author	Agee, Carl B.
dc.date.accessioned	2016-10-13
dc.date.accessioned	2022-05-28T00:36:23Z
dc.date.available	2022-05-28T00:36:23Z
dc.date.issued	2016
dc.description	Presented on March 21-25, 2016 at the 47th Lunar and Planetary Science Conference held at the Woodlands Waterway Marriott Hotel and Convention Center in The Woodlands, Texas.
dc.description.abstract	Martian meteorites record a range of shock effects associated with hypervelocity impact events on their parent body. The purpose of this study is to characterize shock deformation and transformation effects within and adjacent to shock veins in NWA 10416 and in non-veined regions of the host rock. New phases produced by shock, through crystallization or solid-state transfromation, can be used to estimate the shock pressure and the duration of the shock pulse to better understand the impact processes experienced by this sample.
dc.format.extent	163.63 KB
dc.format.mimetype	PDF
dc.identifier.uri	https://hdl.handle.net/20.500.14078/605
dc.language	English
dc.language.iso	en
dc.rights	All Rights Reserved
dc.subject	meteorites
dc.subject	shock
dc.title	Shock effects in new Martian olivine basalt Northwest Africa 10416: distinct from shergottites but akin Northwest Africa 8159	en
dc.type	Presentation
dspace.entity.type

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