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dc.contributor.authorDaly, Luke
dc.contributor.supervisorProf. Phil Blanden_US

This thesis has explored the capability of novel high resolution in situ analyses such as Synchrotron radiation, atom probe microscopy and transmission kikuchi diffraction in the analyses of primitive meteorites. Crystallographic, geochemical and isotopic data extracted using these techniques from refractory metal nuggets in primitive meteorites has implications for our understanding of how these grains formed, particle migration in the protoplanetary disk, and a suggestion that refractory metal nuggets may have a pre-solar origin.

dc.publisherCurtin Universityen_US
dc.titleUnderstanding Our Protoplanetary Disk by Chemical Analysis of Components in Meteoritesen_US
curtin.departmentDepartment of Applied Geologyen_US
curtin.accessStatusOpen accessen_US
curtin.facultyScience and Engineeringen_US

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