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dc.contributor.authorOrr, Kenneth James
dc.contributor.supervisorGretchen Benedixen_US
dc.contributor.supervisorLucy Formanen_US
dc.date.accessioned2022-04-29T03:54:16Z
dc.date.available2022-04-29T03:54:16Z
dc.date.issued2021en_US
dc.identifier.urihttp://hdl.handle.net/20.500.11937/88347
dc.description.abstract

The source craters of the Martian meteorites remain unknown. This PhD extracted pyroxene mid-infrared spectra directly from the shergottites to supplement the current spectral libraries in modelling the geology of the Martian surface. Models using planet-representative spectral end members improves the spectral fit of the modelling, and the accuracy of the mineral abundance determination.

en_US
dc.publisherCurtin Universityen_US
dc.titleExtracting Martian Meteorite Mineral Spectra for Remote Sensing of the Surface Geology of Marsen_US
dc.typeThesisen_US
dcterms.educationLevelPhDen_US
curtin.departmentSchool of Earth and Planetary Sciencesen_US
curtin.accessStatusOpen accessen_US
curtin.facultyScience and Engineeringen_US
curtin.contributor.orcidOrr, Kenneth James [0000-0002-8421-3091]en_US


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