Petrology of NWA 7533: Formation by Impacts on Ancient Martian Crust
dc.contributor.author | Hewins, R. | |
dc.contributor.author | Zanda, B. | |
dc.contributor.author | Humayun, M. | |
dc.contributor.author | Lorand, J. | |
dc.contributor.author | Deldicque, D. | |
dc.contributor.author | Pont, S. | |
dc.contributor.author | Fieni, C. | |
dc.contributor.author | Nemchin, Alexander | |
dc.contributor.author | Grange, M. | |
dc.contributor.author | Kennedy, A. | |
dc.contributor.author | Goepel, C. | |
dc.contributor.author | Lewin, E. | |
dc.date.accessioned | 2017-01-30T11:26:31Z | |
dc.date.available | 2017-01-30T11:26:31Z | |
dc.date.created | 2015-10-29T04:09:32Z | |
dc.date.issued | 2013 | |
dc.identifier.citation | Hewins, 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.uri | http://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.publisher | WILEY-BLACKWELL | |
dc.title | Petrology of NWA 7533: Formation by Impacts on Ancient Martian Crust | |
dc.type | Conference Paper | |
dcterms.source.volume | 48 | |
dcterms.source.startPage | A160 | |
dcterms.source.endPage | A160 | |
dcterms.source.issn | 1086-9379 | |
dcterms.source.series | METEORITICS & PLANETARY SCIENCE | |
dcterms.source.conference | 76th Annual Meeting of the Meteoritical-Society | |
curtin.department | Department of Applied Geology | |
curtin.accessStatus | Fulltext not available |