Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/138419
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dc.contributor.authorMacdonald, K.-
dc.coverage.spatialGawler Craton, South Australia-
dc.date.issued2020-
dc.identifier.urihttps://hdl.handle.net/2440/138419-
dc.descriptionThis item is only available electronically.en
dc.description.abstractZircon and monazite geochronology and trace elemental analysis provide the first constraints on the timing of high temperature metamorphism at the Snaefell magnetite deposit in the northern Gawler Craton, South Australia. The granulite facies rocks which host mineralisation at the Snaefell magnetite deposit yield zircon ages of 1749 ± 15 Ma and 1673 ± 16 Ma, as well as monazite ages of 1670 – 1660 Ma, 1590 – 1580 Ma and 1559 ± 10 Ma. The data indicate that the host sediments have a protolithic age of ca. 1750 Ma, consistent with depositional ages in the adjacent Mount Woods Inlier. The metasediments were exposed to high temperature granulite facies metamorphic conditions during the period 1670 – 1660 Ma. These ages are previously unrecognised in the northern Gawler Craton may indicate that the ca. 1720 – 1690 Ma Kimban Orogeny had a prolonged effect on the region. A second metamorphic event recorded between 1590 and 1580 Ma saw the development of E-W-NE trending folds and is attributed to the 1570 – 1540 Ma Kararan Orogeny. Late deformation at 1559 ± 10 Ma caused north-dipping shear zones to cut across the granulites and is associated second generation garnet growth. Possible hydrothermal zircon may indicate that magnetite is also of a hydrothermal source.en
dc.language.isoenen
dc.subjectHonours; Geology; geochronology; metamorphism; Mesoproterozoic; high temperature; magnetite; Snaefell; Gawler Cratonen
dc.titleThe timing of high temperature metamorphism at the Snaefell magnetite deposit, South Australiaen
dc.typeThesisen
dc.contributor.schoolSchool of Physical Sciencesen
dc.provenanceThis electronic version is made publicly available by the University of Adelaide in accordance with its open access policy for student theses. Copyright in this thesis remains with the author. This thesis may incorporate third party material which has been used by the author pursuant to Fair Dealing exceptions. If you are the author of this thesis and do not wish it to be made publicly available, or you are the owner of any included third party copyright material you wish to be removed from this electronic version, please complete the take down form located at: http://www.adelaide.edu.au/legalsen
dc.description.dissertationThesis (B.Sc.(Hons)) -- University of Adelaide, School of Physical Sciences, 2020-
Appears in Collections:School of Physical Sciences

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