School of Earth Sciences - Theses
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ItemThe origin of the South Australian Heat Flow Anomaly( 2007)The South Australian Heat Flow Anomaly is a zone of high surface heat flow (averaging 92 ± 10 mW m-2); one of several central Australian Proterozoic terranes rich in heat producing elements (HPEs). Its bulk crustal average heat production is between two and three times the global average, indicating an enormous regional enrichment of uranium, thorium and potassium. Until now the distribution of HPEs in the crust has been calculated based on surface heat production; here, a method that uses the temperature at the Moho (as calculated by seismic inversion models) is introduced and found to have good agreement with models that assume a single enriched layer in the upper crust. This layer is found to be between 15-20km. The onset of recycling of uranium through the crust and mantle at the end of the Archaean has been proposed to have produced a peak in uranium available to crust-building, at least partially contributing to the creation of a long-lived geochemical anomaly in Central Australia. However analysis of lead isotopes of K-feldspars from the SAHFA indicates that at the time that crust was first extracted from the mantle, thorium was enriched relative to uranium (not vice versa). In order to investigate more recent effects of such high heat flow, the Tertiary cooling history of the Mt. Painter Inlier is investigated using (U-Th-Sm)/He thermochronology, which has a closure temperature of ~70°C. The most recent ages recorded are ~38 ± 5 Ma, and are argued to record burial of 1400 ± 200m under basement and Cretaceous sediment.
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ItemAustralian Neoproterozoic glaciation: a study of the Sturtian glacial deposits in the Arkaroola region, Northern Flinders Ranges South Australia( 2005)The late Proterozoic Sturtian glacigenic succession exposed in the Arkaroola region of the Northern Flinders Ranges record the earliest of two global Neoproterozoic `Snowball' glacial events in the Adelaide Geosyncline, South Australia. Two stratigraphically disparate glacigenic units were recognised in the late Sturtian succession in the Arkaroola region, a subaerially deposited glacial till - the Merinjina Tillite, and an unclassified glaciomarine diamict unit. The Merinjina Tillite unit preserves a five-fold lithostratigraphy, hosting englacial melt-out deposits, glaciolacustrinal sediments and dominated by a massive to poorly-bedded tillite unit deposited directly from glacier ice. The glaciomarine diamictite preserves down-slope mass-flow deposits, as well as turbidite sequences, slumping and sediments from glacial fall-out including dropstones embedded in laminated muddy-shale and is interpreted as a basin-margin marine deposit. Palaeocurrent analyses across the Northern Flinders Ranges and stratigraphic reviews of analogous Sturtian glacigenic deposits elsewhere in the Northern Flinders Zone suggest palaeotidal influence from the north-north-west and indicate a north-north-west-sloping basin margin in the Northern Flinders Zone. Two major palaeoclimatic phases were recognised in glacigenic rocks the Arkaroola region. A glacial advance phase is represented by the advance of continental glacial sediments, across a topographically-elevated, subaerial surface and extending down-slope into a submarine basin. The other, represented regionally by dropstone shales, is interpreted as glacial retreat and the termination of Sturtian `Snowball Earth' conditions. A rise in palaeo-atmospheric temperatures is inferred, causing melting of continental and marine ice-sheets and resulting in a regionally-extensive marine transgression. The slight increase in water temperature during glacial retreat is believed to have triggered carbonate precipitation and the ultimate deposition of cap dolomites which overly the glacigenic sediments across the Adelaide Geosyncline.
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ItemDetrital zircon geochronology of Neoproterozoic glacials, flinders ranges, South Australia( 2009)A geochronological survey of Neoproterozoic glacial sediments in the Flinders Ranges, South Australia has traced possible source rocks and potential transport directions. A distinct change in the dominant detrital zircon populations present in the earlier Sturtian glacials and the later Marinoan glacials is clearly evident. The major zircon populations present in each of the Sturtian-age samples lie within 1500 -1800Ma, while the majority of Marinoan samples lie between 1100-1400Ma. Potential source rocks for the 1500-1800Ma population include the Gawler and Cumamona Cratons, which are local to the study area. The 1100-1400Ma. population can be traced further north to the Musgrave Inlier in addition to the Albany-Fraser belt and Pinjarra Orogen , north west of the sample localities. The change in zircon population could therefore be accounted for by a change in glacial transport direction during the respective epochs. This may indicate a difference in the severity of the glaciations. An alternative explanation for the difference in detrital zircon signatures could be a change in source rock erosion during each glacial period. Uplift of the Musgrave Inlier or similar basement terrains between the glaciations would provide younger zircons for deposition within the Marinoan sediments. The large unconformity known as `The South Ranges Movement' that is evident in much of the former Centralian Superbasin may testify to such an orogenic event having occurred. Previous studies of detrital zircons in the region provide support for this conclusion.
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ItemHeat flow modelling in the Adelaide Geosyncline, South Australia and implications for geothermal resource exploration( 2008)The central theme of this research is the continental heat flow at the surface of the Earth. Radioactive heat production in the lithosphere and heat flux from convection in the asthenosphere are first order controls on surface heat flow. Accurate heat flow determinations are essential in understanding the geodynamics of the lithosphere and refining resource exploration models, in particular those related to geothermal resources. The focus of this investigation is confined to the understanding of heat refraction as a result of the heterogeneity and anisotropy of the geological subsurface, under a steady-state heat conduction regime. Within the South Australian Heat Flow Anomaly, an area of particular significance for geothermal resource exploration is the deep seated Torrens Hinge Zone, a strip of tectonic transition between the Archaean Gawler Craton to the west and the Neoproterozoic to Cambrian sedimentary cover of the Adelaide Geosyncline to the east. (For complete abstract open document)
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ItemThe stratigraphy and palaeontology of Cape Vani, Milos, Greece( 2005)Milos, dominated by Pliocene-Recent explosive calc-alkaline volcanics, is in the active Aegean Arc. This project investigated the microfauna and depositional environment of a sequence associated with the only terrestrial white smoker field in the world. White smokers occur in a volcaniclastic-hosted Mn-Fe-Ba deposit in a 1 km2 rift basin associated with dacite intrusives. Although the sediments are extensively hydrothermally altered, they have sedimentary structures and yield a variety of micro- and macrofossils. The typical microfaunal assemblage comprises Miliolinids (e.g. Quinqueloculina spp.; Triloculina spp.) and Elphidiids (Elphidium spp.). In the absence of any planktonic foraminifera, this assemblage is typical of inner shelf palaeodepths from around 10-50m. The occurrence of this fauna with echinoderm spines indicates an open marine setting with normal salinity levels. The associated coarse-grained burrowed facies with symmetrical ripples and hummocky cross stratification and a macrofauna of molluscs (e.g. pectinids, Mytilus, fish teeth) further indicates a shallow marine setting. Terrestrial artiodactyl megafauna occur at three levels in tuff and trough cross-laminated fluvial deposits suggesting close proximity to a regressive shoreline. Macrofauna were probably killed by tephra, rapidly disarticulated and removed into a shallow marine environment. The sequence is unconformably overlain by coarse-grained alluvial fan to braided river deposits deposited when Milos became emergent. Barite-silica white smokers derive from the ingress of and leaching by seawater into basement and overlying volcanics. Palaeontological-boiling data shows the fluid was at 165-140°C and the extremophile echinoderm spicule microfauna dominated because forams were unable to live in warm silica-laden turgid fluids with a high heavy metal content.