Wed 1st April 12 – 1 pm Rm 312.222 One of the more difficult challenges involved in the disposal of radioactive waste in deep geological repositories is the very long time frames required by safety assessments. In the case of one Canadian project – Ontario Power Generation’s Deep Geological Repository (OPG DGR) project for the management of low and intermediate level radioactive reactor waste – the safety assessment time-frame is 1 million years. This type of time frame goes well beyond anything that can be considered in an experimental setting. Mathematical models that make long term estimates face challenges with considerable uncertainties over these time frames. There are also significant challenges with explaining the results of these models to the public and other stakeholders. The safety case required for deep geological repository projects must use multiple lines of evidence to complement safety assessments that quantify the level of protection provided by a geological disposal facility. Geological time frames are particularly useful to support arguments associated with safety assessments, as geological time frames are often in excess of safety assessment time frames. For example, the OPG DGR project safety case considers a one million year period, and the sedimentary units that are proposed to host the repository have a well-studied, well-documented geological setting indicating that host sedimentary rocks were deposited and consolidated hundreds of millions of years ago, onto billion year old Canadian Shield rocks. This talk will present some examples of research programs that focus on the safe long-term management of used nuclear fuel in a DGR, whose objectives are to build capabilities to assess the suitability of potential sites for a centralized deep geological repository, for all of Canada`s used nuclear fuel. Potential DGRs are assessed in terms of isolating and containing radioactive waste over geologically long time frames. Specific research topics focus on reducing uncertainties in models of long term repository performance and include (but aren`t limited to): modelling the results of large-scale shaft seal experiments, laboratory determinations of sealing material performance, modelling of the effects of past and future glacial events, natural tracers and natural analogues. |
Curtin Applied Geology Seminar – Dr Julie Brown on Long term safety of Deep Geological Repositories for radioactive waste, Canadian perspective
Curtin Applied Geology Seminar – James Mungall (University of Toronto) on Genesis of a magmatic end-member IOCG deposit at El Laco, Chile
Wed 25th March 12 – 1 pm, Rm 312.222 |
Abstract The IOCG deposit group includes temporally and spatially associated hydrothermal and magmatic end-members which are associated with magmas belonging to the shoshonitic series, e.g., Olympic Dam, Missouri, El Laco, Great Bear Magmatic Zone. They have been interpreted to have formed from similar parental silicate magmas along contrasting petrogenetic paths involving either immiscible separation of Fe-P-O-S magma (e.g., El Laco) or Fe-Cu-S-rich aqueous fluid (e.g., Olympic Dam) [1]. A sample of unconsolidated tephra at El Laco is 86 mol% Fe2O3*, 12 mol% FePO4, 2 mol% SiO2 and minor S, REE. Ovoid cavities in hematite and magnetite ash particles are wholly or partially occupied by vesicular masses of Fe-phosphate, silica, and trace monazite interpreted to be finely crystallized melt with a composition nearly identical to that of the eutectic in the FePO4-Fe2O3 system at 1 atm (84 mol% FePO4, 1070 °C [2]). We have confirmed this by heating the tephra to 1081 °C in an evacuated silica tube, to produce Fe-P-O melt surrounding magnetite and hematite crystals. Ubiquitous occurrences of perlitic shoshonite glass form menisci partially lining cavities in oxide lapilli and bombs. Experimental equilibration of a synthetic shoshonite melt with magnetite, FePO4, H2O and CO2 at 900 °C, 1 GPa produced immisicible high-silica rhyolite and Fe-P-O melt. We consider several hypotheses for the origins of coexisting shoshonite and Fe-P-O magma including liquid immiscibility and deep crustal melting of Fe-rich sedimentary phosphorite. Fe-P-O-S magmas erupted and degassed violently, losing its H3PO4 and SO3 and cooling as magnetite lava. Quenched airfall deposits retain some phosphate minerals. Large hydrothermal IOCG deposits are associated with felsic differentiates of similar potassic magmas that need not have previously generated immisicible Fe-P-O magmas. [1] Tornos F, (2011) 11th SGA Biennial Meeting Let’s Talk Ore Deposits, p. 26-28. [2] Zhang et al., (2011) J Amer Ceramic Soc 94, 1605-1610. |
Curtin Applied Geology Seminar, Wed 11th March 12 – 1 pm. Ivan Zibra GSWA on Neoarchean orogeny in the Yilgarn Craton: In search of a model
The structure of the Neoarchean Yilgarn Craton is dominated by craton-scale high-strain zones, mostly associated with highly-deformed elongate granitic bodies and transposed greenstone belts. These shear zones developed during widespread and prolonged magmatic activity that led to a nearly complete reworking of the felsic continental crust. Recent structural works show that some of these shear zones assisted the emplacement of c. 2700-2660 Ma granite plutons during Neoarchean transpression, allowing the migration of lower crustal melts towards sink in the upper crust. Some of these shear zones are major and possibly long-lived structures juxtaposing different terranes. Geochronology and isotopic data suggest that these terranes may represent microcratons that were progressively amalgamated producing larger crustal blocks. However, little is known about the structural evolution of these shear zones, and therefore the modality, kinematics, tectonic significance and timing of such “amalgamation episodes” between different terranes are still the subject of a long-standing debate. Hence, tectonic models for the assembly of the Yilgarn Craton range from arc-accretion to autochthonous (i.e. plume-dominated) models. Moreover, published tectonic models are based on studies in the eastern half of the craton, where younger rocks are exposed. Therefore, large scale models for the evolution of the Yilgarn Craton have been built in the absence of a comprehensive understanding of its evolution pre-dating 2700 Ma. In this talk I will summarize some results of five years of structural mapping in the western half of the craton (i.e. in the Youanmi Terrane), where pre-2700 Ma rocks and structures are exposed, aiming to provide some first-order constraints to the Neoarchean evolution of the Yilgarn Craton.
Wed 11th March 12 – 1 pm Rm 312.222 |
Curtin Applied Geology Seminar, Wed 4th March: Mick O’Leary (Coastal & Marine Sciences, Curtin University) on Ice Sheet Collapse, Sea Level Rise and Coastal Response
Ice Sheet Collapse, Sea Level Rise and Coastal Response The response of polar ice sheets to modest increases in global temperature and the rate of future sea-level rise remains highly uncertain. One way of addressing these uncertainties is to examine past interglacials, which contain records of both changes in ice sheet mass balance and associated coastal response under a warm or slightly warmer climate system compared to present. However most of the geological record of Antarctic Ice Sheet extent during warmer interglacials has been lost due to glacial expansion and retreat cycles, An alternative and as yet untested approach for constraining ice sheet mass balance under warmer climates utilises the unique sea level fingerprint that results from a collapsing ice sheet. Principally the melting of individual ice sheets and glaciers over time scales of centuries to millennia drives perturbations in the Earth’s gravitational field, solid surface elevation and rotational state. Collectively, these effects contribute to significant geographic variation in eustatic sea level. This talk I focuses on the last interglacial period spanning 128 to 116 ka. This period is characterised by global mean temperatures several degrees warmer than pre-industrial, and is therefore considered an analogue for near-future climate change. There is also a strengthening scientific consensus, and significantly from a near-future analogue perspective, that eustatic sea level peaked between 5 and 9 m above modern during the last interglacial, and was the result of the collapse of one or more of three significant Polar ice sheets, West Antarctic Ice Sheet, East Antarctic Ice Sheet or Greenland Ice Sheet. This finding carries significant implications for future polar ice sheet instability in the face of a relatively moderate global warming. The overarching hypothesis is that LIG ice sheet melting history has left its discernable imprint of marine transgression along coastlines remote from the ice sheets and presents us with a unique opportunity to invert the problem. |
Wed 4th March, 12 – 1 pm, Rm 312.222
Curtin Applied Geology Seminar – David Taylor Geological Survey of Victoria Exploring for Andean Cu Porphyries in western Victoria – the Geological Survey of Victoria supporting industry
Fri 20th February 12 – 1 pm Rm 312.222 Mineralised Cu-Mo-Au porphyries were discovered in belts of Cambrian andesite in the Stavely region of western Victoria in the early 1990s. Deep weathering complicated early geochemical exploration and only a small number of diamond holes to several hundred metres depth were drilled. These encountered sub-economic grades in mostly propylitic alteration. New work shows they only drilled into porphyry dykes emanating up into the host andesites, rather than intersecting the actual porphyry bodies where economic grades could exist in the potassic zone. This lack of early success, combined with no historic artisanal mining and uncertainty over the geological context meant there was little appetite to persevere. In the mid 2000s university wholerock geochemical research suggested that the plate tectonic setting had been an Andean-type convergent margin – very attractive for copper porphyries – rather than a region of arc-continent collision as previously preferred. The geochemistry recognised boninites that can only form in supra-subduction zone settings. The andesite belts themselves and some associated granodiorite intrusions also possessed a geochemical subduction fingerprint with relative depletion of HFSE. A government funded deep crustal seismic transect across the region in the late 2000s imaged a crustal geometry consistent with the Andean-type convergent margin model. The faulted belts of andesite exposed at surface can be traced down into what appears to be a larger arc edifice buried in the subsurface. This greater confidence for Andean-like mineralised porphyries has triggered a new round of exploration and research. A major breakthrough in prospectivity was taking some of the mineralised porphyry drill core and doing wholerock geochemistry for comparison against the existing academic geochemistry. This shows the porphyries are related to the granodiorite intrusions rather than the belts of andesite as previously thought. This boosts prospectivity in two important ways: 1 The intrusions are younger than the steep dipping fault slices of andesite so that the mineral systems are upright for easy vectoring rather than being variably titled and/or partly dissected; 2 The porphyries can occur anywhere within the entire Stavely region rather than being narrowly restricted to a few fault slices of andesite. A government stratigraphic drill program is being planned to better define the margins of the Stavely Geological Zone. Like many mineralised porphyry systems there is complexity for explorers. Current mapping shows the most obvious targets are where the porphyries intrude into the andesites with zone of phyllic overprinting causing demagnetisation haloes (historic Victor prospect). Less obvious are porphyries intruding in siliclastic sandstone outside of the andesite belts still preserve the prograde potassic cap and can be magnetic highs (historic Junction prospect). The intrusions occur in clusters with a multiphase intrusion history, some mineralised and some barren. The clusters seem to be concentrated in late conjugate faults cutting across the paleo-arc trend to define corridors of enhanced prospectivity. Current explorers are collecting gravity and IP to generate good exploration targets through the deep weathering and cover, whilst they raise money for the deep drilling (up to 1 km) that will finally test the economic viability of this very poorly known province of mineralised porphyries. |
Curtin Applied Geology Seminar Feb. 4. – Andrew Langendam on Collecting and Melting: Meteorites from the Nullarbor and Icy Planets
Collecting and Melting: Meteorites from the Nullarbor and Icy Planets
Andrew Langendam, School of Earth, Atmosphere and Environment
Wed 4th February 12 – 1 pm Rm 312.222
For the past seven years, the Monash Meteorites Group has been conducting field expeditions to the Eastern Nullarbor in search of meteorites. Our search technique, a non-traditional one, has been developed to locate strewn fields with some success. In addition, we have investigated how core formation occurs beyond the protoplanetary snowline. Here, planetesimals accrete with water ice which oxidised metal phases to magnetite. This excludes Fe-FeS based core formation from these bodies, and hence core formation as we know it. We acquired a 5.9g sample of the Karoonda CK4 chondrite form the South Australia Museum. This was divided into 12 pellets, and heated in a 1 bar Ar atmosphere furnace at temperature increments of 50°C between 900 and 1300°C. Our experiments show that at all temperature increments investigated, a silicate wetting Fe-S-O melt is generated. Below 1150°C the Fe-S-O melt / silicate melt ratio is high enough that Fe-S-O melt forms connected networks allowing rapid migration via percolative flow. Above 1150°C Fe-S-O tends to form spherical droplets that get trapped in larger silicate melt pockets between unmelted olivine and pyroxene. Thus, unexpectedly, core formation is easier and occurs at lower temperatures in oxidised bodies. Cores form through the percolation of Fe-S-O melt through an interconnected network until the silicate melt to Fe-S-O ratio inhibits the connectivity of Fe-S-O melt. Previous studies have shown that increased O in Fe melts increases their conductivity, hence a magnetic fields generated by a Fe-S-O core could be comparable to those produced by metallic cores. These results also provide a basis for more accurate models of the interior of the icy moons in our solar system, and better understand the processes generating weak magnetic fields in these moons.
Multiscale, Multiphysics & Multiresolution Computing in Earth Science & Engineering – Victor Calo @ 10 am Wednesday 18 February (210.104)
Dr Victor Manuel Calo Associate Professor in Applied Mathematics & Computational Science & Earth Science & Engineering, Co-Director of SRI-Center for Numerical Porous Media
10-11 am Wednesday 18 February, Building 210 Room 104 (Elizabeth Jolley Case Study Room)
In this presentation, we describe two important applications in Computational Geoscience.
1. Multiscale Model Reduction for Flows in Heterogeneous Porous Media: We combine discrete empirical interpolation techniques, global mode decomposition methods, and local multiscale methods, such as the Generalized Multiscale Finite Element Method (GMsFEM), to reduce the computational complexity associated with nonlinear flows in highly-heterogeneous porous media. To solve the nonlinear governing equations, we employ the GMsFEM to represent the solution on a coarse grid with multiscale basis functions and apply proper orthogonal decomposition on a coarse grid. Computing the GMsFEM solution involves calculating the residual and the Jacobian on the fine grid. As such, we use local and global empirical interpolation concepts to circumvent performing these computations on the fine grid. The resulting reduced-order approach enables a significant reduction in the flow problem size while accurately capturing the behaviour of fully-resolved solutions. We use random boundary conditions to construct snapshot vectors to build local basis functions. We show that by using only a few of these randomly generated snapshots, we can adequately approximate dominant modes of the solution space. We consider several numerical examples of nonlinear multiscale partial differential equations that are numerically integrated using fully-implicit time marching schemes to demonstrate the effectiveness of the proposed model reduction approach to speed up simulations of nonlinear flows in high-contrast porous media.
2. Finite Element Analysis of Lithospheric Deformation: We describe an efficient and flexible unstructured finite element discretization, which uses linear elements on simplexes that avoids locking. The anti-volumetric locking technique calculates the volumetric strain from the actual volume change of each element instead of from strain rate accumulation. We extend the original finite-difference-based FLAC (Fast Lagrangian Analysis of Continua) algorithm to a finite element formulation with the anti-volumetric locking modification. We demonstrate the capability of the discretization modelling spontaneous formation of normal faults by the reduction of cohesion in a frictional and cohesive elastoplastic layer.
See Flyer here: Victor Calo – Flyer
Exploration Geodynamics & Earth’s Evolution – Craig O’Neill @ 9 am Thursday 12 February (210.104)
A/Prof. Craig O’Neill ARC Centre of Excellence in Core to Crust Fluid Systems Macquarie University, Sydney
9 am Thursday 12 February — Building 210 Room 104—Elizabeth Jolley Case Study Room
Whether or not the Earth has transitioned from an earlier archaic mode of tectonics, into modern plate tectonics, is one of the fundamental questions in geology. Geodynamics simulations suggest a transition from an earlier stagnant-lid regime, to an ‘episodic’ mode characterized by repeated lid-overturn events, and finally into a later plate-tectonic regime. This tectonic trajectory is finding support in modern geochemical, geophysical, and tectonic observations.
Problematically, though, is the recent suggestion that tectonic regime is not solely a function of the thermal state of a planet, but also of its history. Constraining Earth’s evolution, then, requires a better understanding of Earth’s initial thermal state and configuration. The problem has economic consequences. World-class ore-deposits, such as Olympic Dam, for instance, are lithospheric-scale systems, and the tectonic evolution of the lithosphere, its construction, architecture, fluid pathways, and fluid flux events, are crucial to their development. The knowledge to understand, and predict, the next generation of large economic deposits is predicated on constraining the tectonics of the time, and the evolution of the lithosphere, and the dynamics of mantle fluids, under such a regime. Three case studies will be presented which encapsulate both the frontier research, technical development, and applications of geodynamic simulations. 1. Summary of our recent work on the evidence, both from numerical simulations and 142Nd measurements, to support stagnant-lid convection in the Hadean. 2. New and novel technique to calculate the interior state of an early accreting planet, using GPU-accelerated smooth-particle hydrodynamic simulations. 3. Demonstration of how the release of water from subducting slabs in various tectonic settings exerts a fundamental control on metallogenesis, and speculate on how this Research frontiers, technology boundaries, & applications
See Flyer here: Craig O’Neill Seminar 120215
Curtin Applied Geology Seminar: Weds 3rd Dec – Stephen Gallagher on Reefs, Oceans and Climate
Wed 3rd December 12 – 1 pm Rm 312.222 |
Stephen Gallagher Department of Earth and Atmospheric Sciences, Univer International Ocean Discovery Program Expedition 356, August-September 2015 Reefs, Oceans, and Climate: A 5 million year history of the Indonesian Throughflow, Australian monsoon, and subsidence on the Northwest Shelf of Australia Stephen J Gallagher, Craig Fulthorpe and Kara Bogus
Abstract The Indonesian Throughflow (ITF) is a critical part of the global thermohaline conveyor. It plays a key role in transporting heat from the equatorial Pacific (the Indo-Pacific Warm Pool) to the Indian Ocean and exerts a major control on global climate. Because of the continued northward motion and impingement of the Australasian plate into the southeast Asian part of the Eurasian plate, the complex tectonic history of the Indonesian archipelago makes it difficult to reconstruct long-term (million year) ITF history from sites within the archipelago. The best areas to investigate ITF history are downstream in the Indian Ocean, in regions directly under the influence of the ITF. International Ocean Discovery Program Expedition 356 will drill a transect of cores over 10° latitude on the northwest shelf (NWS) of Australia to obtain a 5 m.y. record of ITF, Indo-Pacific Warm Pool, and climate evolution that has the potential to match orbital-scale deep-sea records in its resolution. Coring will reveal a detailed shallow-water history of ITF variability and its relationship to climate. It will allow us to understand the history of the Australian monsoon and its variability, a system whose genesis is thought to be related to the initiation of the East Asian monsoon. It also will lead to a better understanding of the nature and timing of the development of aridity on the Australian continent. Paleobathymetric and stratigraphic data from the transect will also allow subsidence curves to be constructed to constrain the spatial and temporal patterns of vertical motions caused by the interaction between plate motion and convection within the Earth’s mantle, known as dynamic topography. The NWS is an ideal location to study this phenomenon because it is positioned on the fastest moving continent since the Eocene, on the edge of the degree two geoid anomaly. Accurate subsidence analyses over 10° of latitude can resolve whether northern Australia is moving with/over a time transient or long-term stationary downwelling within the mantle, thereby vastly improving our understanding of deep-Earth dynamics and their impact on surficial processes. Biography
Stephen Gallagher is an Associate Professor at the University of Melbourne. He has had diverse research experience in Carboniferous to Recent microfossils, sedimentology and stratigraphy globally. He uses applied stratigraphy & micropalaeontology to solve stratigraphic problems and to interpret (palaeo) environments, bathymetry and oceanography. |
Curtin Applied Geology Seminar: Weds 26th Nov – Steve Micklethwaite on the Duration and Dynamics of Orogenic Deposit Formation
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Wed 26th November 12 – 1 pm Rm 312.222 |
Steve Micklethwaite Centre for Exploration Targetting, UWA The Duration and Dynamics of Orogenic Deposit Formation Abstract Here I briefly review the physical hydrogeology of orogenic-type gold deposits and their linkages to self-organizing phenomena, such as earthquake-aftershock sequences, seismic swarms and fluid pressure driven failure. Building on these developments we use a combination of field observations and boundary element modelling to explore the relationship between fault stepovers, fluid flow and mineralization. It is shown that underlapping stepover geometries are typically rare in fault systems but anomalously associated with gold deposits. We find that a larger region of damage and permeability enhancement is created around underlapping stepovers than around overlapping stepovers. By taking into account both the enhancement and decay of permeability during the seismic cycle it is estimated that a 5 Moz goldfield could feasibly form in 1-16 earthquake-aftershock sequences; potentially representing durations of just 10-8000 years. Similar rapid durations for goldfield formation have been inferred from different environments, including volcano sector collapse (e.g. Lihir, Papua New Guinea) and convective circulation in geothermal regions (e.g. Taupo Volcanic Zone, New Zealand). The result that deposits form extremely rapidly, even though connected to fault systems with million-year lifespans, may suggest that economic grade mineralization requires several different self-organizing phenomena to overlap in time and space. Such a concept potentially explains why deposits cluster in metal-rich provinces but with multiple episodes of mineralization, sometimes millions of years apart.
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