ORCID Profile
0000-0001-5144-4507
Current Organisation
Curtin University
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In Research Link Australia (RLA), "Research Topics" refer to ANZSRC FOR and SEO codes. These topics are either sourced from ANZSRC FOR and SEO codes listed in researchers' related grants or generated by a large language model (LLM) based on their publications.
Geochemistry | Mineralogy and Crystallography | Geology | Ore Deposit Petrology | Inorganic Geochemistry | Water Resources Engineering | Chemical Thermodynamics And Energetics | Chemical Spectroscopy | Geochronology And Isotope Geochemistry | Nanoscale Characterisation | Igneous And Metamorphic Petrology | Igneous and Metamorphic Petrology | Isotope Geochemistry | Extraterrestrial Geology | Inorganic Geochemistry Not Elsewhere Classified | Functional Materials | Nanotechnology | Metals and Alloy Materials | Structural Geology | Geochemistry not elsewhere classified | Nanofabrication, Growth and Self Assembly
Expanding Knowledge in the Earth Sciences | Earth sciences | Expanding Knowledge in Engineering | Precious (Noble) Metal Ore Exploration | Management of Greenhouse Gas Emissions from Energy Activities (excl. Electricity Generation) | Energy transformation | Chemical sciences | Geothermal Energy | Mineral Resources (excl. Energy Resources) not elsewhere classified | Mining and Extraction of Precious (Noble) Metal Ores | Expanding Knowledge in the Biological Sciences | Copper Ore Exploration |
Publisher: Elsevier BV
Date: 11-2018
Publisher: American Geophysical Union (AGU)
Date: 2021
DOI: 10.1029/2020GC009485
Abstract: The Macquarie Ridge Complex (MRC) on the Australia‐Pacific plate boundary south of New Zealand is an extinct mid‐ocean ridge that has experienced a complex tectonic history and produced highly heterogeneous mid‐ocean ridge basalts (MORBs). When and how seafloor spreading ceased along the proto‐Macquarie mid‐ocean ridge remain elusive, and it is unclear how the mantle source of MORBs is affected by the gradual cessation of seafloor spreading at mid‐ocean ridges. To constrain the tectonic evolution of the MRC, the mantle source variations for MORBs at dying mid‐ocean ridges, and the mechanisms of mantle enrichment and asthenospheric heterogeneities, we report 11 pyroxene, plagioclase, basaltic glass, groundmass, and sericite 40 Ar/ 39 Ar and one zircon U‐Pb ages for the MRC MORBs. Our data reveal that basalts from the MRC seamounts were erupted between 25.9 and 1.6 Ma and Macquarie Island at ∼10 Ma. Combined age and plate reconstruction results reveal that the cessation of seafloor spreading at the MRC generally propagated from south to north along the ridge. Basalts produced by the then dying Macquarie mid‐ocean ridge at different times on different seamounts/island show a large variation in isotopic compositions and there is no clear correlation between ages and isotopic ratios. The heterogeneity of mantle source for MORBs from the proto‐Macquarie mid‐ocean ridge suggests that the upper asthenospheric mantle is heterogeneous, and such heterogeneity becomes most obvious at dying mid‐ocean ridges where the degrees of partial melting are low and a large range of melt compositions are produced.
Publisher: Elsevier BV
Date: 11-2009
Publisher: Elsevier BV
Date: 06-2013
Publisher: American Geophysical Union (AGU)
Date: 10-2008
DOI: 10.1029/2008GC002157
Publisher: Elsevier BV
Date: 05-2014
Publisher: Elsevier BV
Date: 08-2011
Publisher: Wiley
Date: 22-01-2021
DOI: 10.1111/JMG.12579
Abstract: Phase equilibrium modelling is commonly employed to constrain the pressure–temperature ( P–T ) evolution of granulite facies rocks, from which their geodynamic setting may be inferred. However, defining a suitable equilibrium volume in such rocks is non‐trivial due to heterogeneities in protolith composition and open system behaviour, including melt loss or gain and deformation. Consequently, equilibrium volumes and the mineral assemblages they contain may vary both temporally and spatially within a single rock. Additionally, despite the extreme temperatures they attained, granulites commonly contain microtextures indicating gradients in chemical potential after the metamorphic peak. This study assesses the processes that control compositional heterogeneity between equilibrium volumes in a suprasolidus granulite and the consequences for the development of a range of microstructures. An approach combining phase equilibrium forward modelling and chemical potential diagrams is used to simulate the suprasolidus evolution of two adjacent equilibrium volumes in an Mg‐rich metapelite. Assuming equilibrium within the two compositional domains, evolving granulite facies assemblages vary along a high T/P (125°C/kbar) clockwise P–T path representative of high T/P metamorphic terranes. Many retrograde microtextures in metapelitic rocks can be reproduced by considering chemical potential (µ) gradients in µ MgO , µ FeO and µ CaO between phases, assuming (a) the presence of melt on grain boundaries, (b) that Al 2 O 3 is perfectly immobile and (c) that K 2 O and Na 2 O are perfectly mobile. Additionally, documented microtextures in granulites imply local SiO 2 ‐undersaturation, despite the presence of matrix quartz in the rock. Preserving such chemical potential gradients requires that solid phases are chemically and physically isolated from melt. Efficient prograde melt drainage may lead to a loss in melt interconnectivity at high temperature ( °C), meaning that equilibration of centimetre‐scale compositional domains is controlled by solid‐state diffusion. The presence of isolated pockets of viscous melt allows the formation of discontinuous intergranular reaction microtextures.
Publisher: Elsevier BV
Date: 02-2011
Publisher: Springer Science and Business Media LLC
Date: 06-2004
DOI: 10.1038/NATURE02644
Publisher: Elsevier BV
Date: 03-2018
DOI: 10.1016/J.CHEMOSPHERE.2017.12.012
Abstract: The presence of organic matter (OM) has a profound impact on uranium (U) redox cycling, either limiting or promoting the mobility of U via binding, reduction, or complexation. To understand the interactions between OM and U, we characterised U oxidation state and speciation in nine OM-rich sediment cores (18 s les), plus a lignite s le from the Mulga Rock polymetallic deposit in Western Australia. Uranium was unevenly dispersed within the analysed s les with 84% of the total U occurring in s les containing >21 wt % OM. Analyses of U speciation, including x-ray absorption spectroscopy and bicarbonate extractions, revealed that U existed predominately (∼71%) as U(VI), despite the low pH (4.5) and nominally reducing conditions within the sediments. Furthermore, low extractability by water, but high extractability by a bi-carbonate solution, indicated a strong association of U with particulate OM. The unexpectedly high proportion of U(VI) relative to U(IV) within the OM-rich sediments implies that OM itself does not readily reduce U, and the reduction of U is not a requirement for immobilizing uranium in OM-rich deposits. The fact that OM can play a significant role in limiting the mobility and reduction of U(VI) in sediments is important for both U-mining and remediation.
Publisher: Elsevier BV
Date: 09-2013
Publisher: Elsevier BV
Date: 11-2014
Publisher: Wiley
Date: 12-01-2018
DOI: 10.1111/JMG.12298
Publisher: Elsevier BV
Date: 2019
Publisher: Springer Science and Business Media LLC
Date: 29-09-2010
Publisher: Elsevier BV
Date: 08-2018
Publisher: Elsevier BV
Date: 2011
Publisher: Geological Society of America
Date: 2006
DOI: 10.1130/G22390.1
Publisher: Geological Society of America
Date: 02-2013
DOI: 10.1130/G33244.1
Publisher: International Union of Crystallography (IUCr)
Date: 20-09-2008
Publisher: Elsevier BV
Date: 12-2013
Publisher: Society of Economic Geologists
Date: 03-2011
Publisher: Elsevier BV
Date: 10-2015
Publisher: Springer Science and Business Media LLC
Date: 02-1999
Publisher: Elsevier BV
Date: 2019
Publisher: Wiley
Date: 17-09-2007
Publisher: Geological Society of America
Date: 12-12-2017
DOI: 10.1130/G38462.1
Publisher: Elsevier BV
Date: 05-2020
Publisher: Elsevier BV
Date: 11-2018
Publisher: Geological Society of America
Date: 2011
Publisher: Elsevier BV
Date: 02-2014
Publisher: Springer Science and Business Media LLC
Date: 08-2017
Publisher: Geological Society of London
Date: 11-2022
Publisher: Mineralogical Society of America
Date: 02-2014
DOI: 10.2138/AM.2014.4222
Publisher: Elsevier BV
Date: 10-2020
Publisher: Wiley
Date: 21-06-2010
Publisher: Geological Society of London
Date: 2002
Publisher: American Geophysical Union (AGU)
Date: 12-2021
DOI: 10.1029/2021JB022729
Abstract: The Oman Drilling Project “Multi‐Borehole Observatory” (MBO) s les an area of active weathering of tectonically exposed peridotite. This article reviews the geology of the MBO region, summarizes recent research, and provides new data constraining ongoing alteration. Host rocks are partially to completely serpentinized, residual mantle harzburgites, and replacive. Dunites show evidence for “reactive fractionation,” in which cooling, crystallizing magmas reacted with older residues of melting. Harzburgites and dunites are 65%–100% hydrated. Ferric to total iron ratios vary from 50% to 90%. In Hole BA1B, alteration extent decreases with depth. Gradients in water and core composition are correlated. Serpentine veins are intergrown with, and cut, carbonate veins with measurable 14 C. Ongoing hydration is accompanied by SiO 2 addition. Sulfur enrichment in Hole BA1B may result from oxidative leaching of sulfur from the upper 30 m, coupled with sulfate reduction and sulfide precipitation at 30–150 m. Oxygen fugacity deep in Holes BA3A, NSHQ14, and BA2A is fixed by the reaction 2H 2 O = 2H 2 + O 2 combined with oxidation of ferrous iron in serpentine, brucite, and olivine. fO 2 deep in Holes BA1A, BA1D, and BA4A is 3–4 log units above the H 2 O‐H 2 limit, controlled by equilibria involving serpentine and brucite. Variations in alteration are correlated with texture, with reduced, low SiO 2 assemblages in mesh cores recording very low water/rock ratios, juxtaposed with adjacent veins recording much higher ratios. The proportion of reduced mesh cores versus oxidized veins increases with depth, and the difference in fO 2 recorded in cores and veins decreases with depth.
Publisher: Wiley
Date: 02-05-2019
DOI: 10.1111/JMG.12484
Abstract: This essay in honour of Mike Brown addresses aspects of chemical equilibrium and equilibration in rocks, with a focus on the role that chemical potentials play. Chemical equilibrium is achieved by diffusive flattening of chemical potential gradients. The idea of equilibration volume is developed, and the way equilibration volumes may evolve along a pressure–temperature path is discussed. The effect of the environment of an equilibration volume is key to understanding the evolution of the equilibration volume with changing conditions. The likely behaviour of equilibration volumes is used to suggest why preservation of equilibrium mineral assemblages and mineral compositions from metamorphism tends to occur. This line of logic then provides the conceptual support to conventional equilibrium thermodynamic approaches to studying rocks, using, for ex le, thermobarometry and pseudosections.
Publisher: Elsevier BV
Date: 02-2006
Publisher: Elsevier BV
Date: 11-2006
Publisher: Elsevier BV
Date: 02-2006
Publisher: Elsevier BV
Date: 11-2017
Publisher: Elsevier BV
Date: 10-2013
Publisher: Elsevier BV
Date: 05-2013
Publisher: Wiley
Date: 08-07-2021
Publisher: Geological Society of America
Date: 13-04-2023
DOI: 10.1130/G50927.1
Abstract: Highly siderophile elements (HSEs), including Re and Os, are used extensively as geochemical tracers and geochronometers to investigate the formation and evolution of Earth’s crust and mantle. Mantle rocks are commonly serpentinized, but the effect of serpentinization on the distribution of HSEs is controversial because HSEs are commonly hosted by rare, micrometer- to sub-micrometer-scale grains of platinum group minerals (PGMs) of ambiguous origin that are challenging to identify, characterize, and interpret. In this study, atom probe tomography (APT) is used to characterize two spatially close PGM grains hosted by a partially serpentinized harzburgite from Macquarie Island, Australia. The APT data reveal an extraordinary level of detail that provides insights into the origin of a complex Cu–Pt alloy grain (average composition ~Cu4Pt). The grain hosts Fe-, Ni-, and Pt-rich sub-grains associated with Rh, variably overlapping networks of Pd- and Cd-enrichment, and OH-rich volumes identified as fluid inclusions. Osmium and Ru are hosted by an idioblastic laurite (RuS2) grain. Compositional, textural, and phase-diagram constraints are consistent with a modified pre-serpentinization origin for the PGMs, and a comparison between observed and calculated grain distributions indicate that while Os isotope ratios were probably unaffected by serpentinization, whole-rock and grain-scale HSE and isotopic ratios may have been decoupled during serpentinization.
Publisher: Elsevier BV
Date: 04-2020
Publisher: Mineralogical Society
Date: 04-2003
Abstract: Mineralogical, bulk and field leachate compositions are used to identify important processes governing the evolution of discharges from a coal spoil heap in County Durham. These processes are incorporated into a numerical one-dimensional advective-kinetic reactive transport model which reproduces field results, including gas compositions, to within an order of magnitude. Variation of input parameters allows the effects of incorrect initial assumptions on elemental profiles and discharge chemistry to be assessed. Analytical expressions for widths and speeds of kinetic reaction fronts are developed and used to predict long-term development of mineralogical distribution within the heap. Results are consistent with observations from the field site. Pyrite oxidation is expected to dominate O2 consumption in spoil heaps on the decadal timescale, although C oxidation may stabilize contaminants in effluents on the centennial scale.
Publisher: Elsevier BV
Date: 10-2017
Publisher: Elsevier BV
Date: 2019
Publisher: Wiley
Date: 21-10-2002
Publisher: American Geophysical Union (AGU)
Date: 11-2017
DOI: 10.1002/2017GC007145
Publisher: Elsevier BV
Date: 05-2016
Publisher: Wiley
Date: 04-2005
Publisher: Elsevier BV
Date: 2019
Publisher: Society of Economic Geologists
Date: 08-2018
Publisher: Society of Economic Geologists
Date: 06-2006
Publisher: Elsevier BV
Date: 06-2007
Publisher: Geological Society of America
Date: 29-06-2012
DOI: 10.1130/G33037.1
Publisher: Elsevier BV
Date: 12-2022
Publisher: Elsevier BV
Date: 09-2008
Publisher: Elsevier BV
Date: 06-2012
Publisher: Springer Science and Business Media LLC
Date: 16-08-2019
Publisher: American Geophysical Union (AGU)
Date: 10-2014
DOI: 10.1002/2014GC005459
Publisher: Wiley
Date: 07-2015
DOI: 10.1111/JMG.12140
Publisher: Elsevier BV
Date: 05-2009
Publisher: Elsevier BV
Date: 02-2013
Publisher: Elsevier BV
Date: 2022
Start Date: 12-2012
End Date: 06-2017
Amount: $682,146.00
Funder: Australian Research Council
View Funded ActivityStart Date: 12-2021
End Date: 12-2024
Amount: $332,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2019
End Date: 12-2019
Amount: $609,865.00
Funder: Australian Research Council
View Funded ActivityStart Date: 12-2021
End Date: 12-2024
Amount: $388,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 07-2011
End Date: 12-2013
Amount: $140,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 05-2016
End Date: 06-2018
Amount: $547,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2015
End Date: 12-2015
Amount: $1,060,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2010
End Date: 08-2013
Amount: $155,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2004
End Date: 2006
Amount: $120,000.00
Funder: Australian Research Council
View Funded Activity