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dc.contributor.authorHewins, R.
dc.contributor.authorZanda, B.
dc.contributor.authorHumayun, M.
dc.contributor.authorLorand, J.
dc.contributor.authorDeldicque, D.
dc.contributor.authorPont, S.
dc.contributor.authorFieni, C.
dc.contributor.authorNemchin, Alexander
dc.contributor.authorGrange, M.
dc.contributor.authorKennedy, A.
dc.contributor.authorGoepel, C.
dc.contributor.authorLewin, E.
dc.date.accessioned2017-01-30T11:26:31Z
dc.date.available2017-01-30T11:26:31Z
dc.date.created2015-10-29T04:09:32Z
dc.date.issued2013
dc.identifier.citationHewins, R. and Zanda, B. and Humayun, M. and Lorand, J. and Deldicque, D. and Pont, S. and Fieni, C. et al. 2013. Petrology of NWA 7533: Formation by Impacts on Ancient Martian Crust, in Proceedings of the 76th Annual Meeting of the Meteoritical Society, Jul 29-Aug 7 2013. Edmonton, Canada: Lunar and Planetary Institute.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/11731
dc.description.abstract

NWA 7533 contains FeNi grains (~1μm), up to 4.5% Ni in pyrite, and 500 nm Os-Ir-rich particles. Lithic clasts are pyroxenite, norite and zircon-bearing monzonite. The impact melt can be modeled as a mixture of crystal clasts and is poor in monzonite.

dc.publisherWILEY-BLACKWELL
dc.titlePetrology of NWA 7533: Formation by Impacts on Ancient Martian Crust
dc.typeConference Paper
dcterms.source.volume48
dcterms.source.startPageA160
dcterms.source.endPageA160
dcterms.source.issn1086-9379
dcterms.source.seriesMETEORITICS & PLANETARY SCIENCE
dcterms.source.conference76th Annual Meeting of the Meteoritical-Society
curtin.departmentDepartment of Applied Geology
curtin.accessStatusFulltext not available


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