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June 13th:  6:00 PM, School of Earth Sciences Lecture Theatre, University of Tasmania. 

 

The Mount Isa mineral province in northwestern Queensland and it extension into southeastern Northern Territory is one of the richest mineral provinces in the world, with three world-class Zn-Pb deposits and several major Cu (Au) deposits. Although there is some disagreement, most workers interpret that the Zn-Pb deposits formed early during basin development, whereas the Cu (Au) deposits formed much later, during and after the Isan Orogeny. Regional geological, geophysical, geochemical and isotopic data acquired over the last 20 years by Geoscience Australia and its collaborators has been used to: map major architectural features that controlled mineralisation at the regional scale; provide evidence of province-scale metal (Zn, Cu and Co) leaching that likely provided the metals to the ores; suggest that the mineralogy and temperature of alteration had a strong control on zinc leaching; and provide evidence of regional variations in Cu, Fe and Zn isotopes possibly related to regional fluid flow events.


A range of regional datasets (radiogenic isotopes, passive and active seismic, gravity, magnetic and magnetotelluric (MT)) have been used to identify crustal boundaries that have a strong control on the regional location of both the Zn-Pb and Cu (Au) deposits. The Gidyea Suture, as defined by active seismic data, marks the eastern margin of the province and is spatially associated with iron oxide-copper gold (IOCG) deposits of the Cloncurry district. This IOCG district is also spatially associated with a conductive zone defined from MT data. The Rufus Fault and associated faults mark the western margin of the province and are associated with gradients in radiogenic isotope and upward-continued gravity data, a gradient in the depth of the lithosphere-asthenosphere boundary and a resistive zone in MT data. McArthur-type zinc-lead deposits are strongly associated with this major crustal boundary. The Gidyea Suture and Rufus structure probably formed prior to the initiation of the North Australian Basin system, served as buttresses as the basin system evolved, and acted as foci for deformation and fluid low.


Following up on work by CODES in the 1990s, regional geochemical studies have identified significant changes in basinal rocks due to regional and pervasive fluids flow. Although most obvious in mafic volcanic rocks, this alteration has affected all rock types, changing not only the chemical composition of the rocks, but also their isotopic composition. Mafic rocks that range in age from 1790 Ma to 1720 Ma experienced extensive Zn, Cu and Co loss through the mineral province; back-of-the-envelop calculations indicate that the metal released from the mafic rocks is an order of magnitude or more greater than the metal known to be present in the ore deposits. Moreover, consideration of the mineralogy of the altered rocks and comparison with other mineral systems suggest that the mineralogy and temperature of hydrothermal alteration has a strong influence on the leaching of zinc. Our and previous studies by CODES indicate that the most intense zinc leaching is associated with alteration assemblages dominated by K-feldspar with minimal chlorite, whereas altered mafic rock dominated by chlorite has not lost zinc. Comparison of higher temperature alteration, chlorite-rich alteration systems suggests that low temperature chlorite retains zinc, whereas higher temperature chlorite loses zinc, which has a strong effect on the leachability of zinc from source rocks.

 

Finally, regional copper, iron and zinc isotope analyses of the regional basalts identify regional isotopic anomalies, which likely are related to mineralisation. A 25 km-50 km 65Cu-enriched zone is located to the east of the Mount Isa copper orebody. This anomaly is consistent with Rayleigh-type fractionation during regional alteration and copper leaching. The results indicate the likely size of the mineral system that produced the Mt Isa copper orebody and suggest that copper isotopes are potentially useful during regional- or province-scale exploration. Our results highlight the power of integrating data from a range of sources to develop regional understanding of mineral systems from the province- to the deposit-scale.


Biography:

Dr David Huston has had a long association with CODES. He completed his PhD at UTAS in 199* as Ross Large’s first PhD student. Now David has just retired from Geoscience Australia where he has spent nearly 30 years investigating the metallogenesis of Australia’s mineral deposits. He has worked throughout Australia and other countries on deposits that range in age from Paleoarchean to Tertiary, with experience with many different deposit types. Over the past ten years he has had a special interest between metallogenesis, tectonics and the evolution of Earth’s hydrosphere/atmosphere.




May 23rd:  6:00 PM, School of Earth Sciences Lecture Theatre, University of Tasmania. 

 

The Denman Glacier region, about 500 km west of Australia’s Casey Station, drains a large ice catchment sitting above a subglacial basin that (possibly) hosts the deepest terrestrial trench on Earth! This region alone holds ice with a potential sea level rise of 1.5 m and has some of the highest rates of grounding line melt anywhere in Antarctica. Given this vulnerability to climate warming, and the diverse range of ice, ocean and geological environments preserved in the region, it has become a key focus Australian and international collaborations.


In the 2023-24 summer, 27 scientists and some 15+ support personnel camped in the Bunger Hills region adjacent to the Denman Glacier to undertake the most ambitious Australian-led multi-disciplinary science campaign in decades. Geologists Jacqui Halpin (UTAS) and Jack Mulder (UAdelaide) were part of the Australian Centre for Excellence in Antarctic Science (ACEAS) team, spending 2 months climbing all over the spectacular rocky peaks and coastal outcrops. With some 1000kg of rocks in their backpacks (and some help from the helicopters and friends), they have sampled a fascinating window into the ancient past - a tectonic tale more than 3 billion years in the making! During this talk, Jacqui will show images of the field season, including what life was like in tight (tent) quarters, and take you on a virtual field trip through the guts of a glacial system, and from the Archean, through the Proterozoic, to the (maybe) Permian, and the very recent glacial moraines.


A/Prof Jacqueline Halpin is a geologist at the Institute for Marine and Antarctic Studies (IMAS). She is particularly interested in deep-time processes, including tectonic cycles and past supercontinent configurations. Jacqueline is currently working on Antarctic geoscience themes including past ice sheet change and Earth-cryosphere interactions, as part of the ARC Australian Centre for Excellence in Antarctic Science Special Research Initiative (ACEAS). Jacqueline completed her science undergraduate degree with Honours in Geology from the University of Melbourne in 2001, and was awarded her PhD, on the tectonic evolution of the Rayner Complex in East Antarctica, from the University of Sydney in 2007. She has previously worked for the Centre of Ore Deposit and Earth Sciences (CODES) as a research fellow (2007-2015), and at Macquarie University (2007-2015) and University of Sydney (2011-2012) as a lecturer and research associate.



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