Petroleum
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This product is a map of the major Australian petroleum fields and pipelines (2010).
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Annual update of map backing the combined GA/RET NAPE Conference
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Promotional flyer comprising map showing petroleum exploration permits, pipelines and basins in Australia
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The Onshore Energy Systems Group have undertaken a regional study on the prospectivity of the southern Georgina Basin, and present here a synopsis of the initial results from this multidisciplinary project. The Georgina Basin is a Neoproterozoic to Lower Devonian sedimentary basin covering 325,000 km2 of western Queensland and the Northern Territory (Dunster et al., 2007; Kruse et al., 2013; Munson, 2014). It is a northwest-southeast-trending extensional basin, where thick marine Cambrian and Ordovician sediments are preserved in its two southern depocentres, the Dulcie and Toko synclines, and a thinner succession is present in the Undilla Sub-basin to the northeast. Within these depocentres, the Thorntonia Limestone and Arthur Creek Formation (Figure 1) contain potential source rocks (Ambrose et al., 2001; Boreham and Ambrose, 2012). Most of the southern Georgina Basin is under license for petroleum exploration, with explorers targeting the carbonate-dominated Arthur Creek Formation for both conventional and unconventional hydrocarbons. A data package that includes raw and reprocessed HyLogging data from 25 wells in the Georgina Basin was recently released (Smith and Huntington, 2014). The HyLogging data map the mineralogical variations within formations and were used in conjunction with wireline log and biostratigraphic data to refine stratigraphic correlation. The HyLogging data were re-processed using a common set of mineral scalars (i.e., spectroscopic indices) to create an internally-consistent, basin-wide dataset. Other datasets, including total organic carbon (TOC) content, X-ray diffraction (XRD) measurements and biostratigraphy were also integrated with the Hylogging data. The 'hot shale' of the Arthur Creek Formation has a characteristic spectral response of decreasing albedo and an increased short wave infra-red (SWIR) aspectral response with increasing depth to the base of the Arthur Creek Formation (Figure 2), which both appear to correlate with increasing core total gamma and TOC. These inter-relationships may be used to better characterise and identify potential source rock units in the basin. Recent biostratigraphic work has highlighted an age discrepancy in the prospective organic-rich `hot shale in the base of the middle Cambrian Arthur Creek Formation (Figure 1). This unit is present in the two major southern depocentres, the Dulcie and Toko synclines, where it has previously been considered as correlative. Recent results, however, suggest that the basal 'hot shale' is either significantly younger in the Toko Syncline than in the Dulcie Syncline, or represents a condensed section in the former. Middle Cambrian carbon isotope excursions have been correlated across a number of Australian basins and can be used to test correlative models across the Georgina depocentres. High resolution sampling across this middle Cambrian section has been carried out in a number of wells in the Dulcie Syncline and in the Undilla Sub-basin, where the age equivalent Inca Shale is penetrated. Carbon isotopes from organic carbon (kerogen) as well as carbon and oxygen isotope ratios of four carbonate mineral phases (calcite, ankerite, dolomite and siderite) were analysed and these data are compared with existing carbon isotope stratigraphy published from neighboring wells (Donnelly et al., 1988; Lindsay et al., 2005; Creveling et al., 2013). Initial results corroborate the new biostratigraphic interpretation.
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Update of annual NAPE brochure
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map showing location of currently producing oil and gas fileds and potential future producing fields. Location and extent of oil and gas pipelines (existing and proposed) is also shown.
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Petroleum Titles map Basin and Coastline data
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No abstract available
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No abstract available
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The South Nicholson Basin and immediate surrounding region are situated between the Paleo- to Mesoproterozoic Mount Isa Province and McArthur Basin. Both the Mount Isa Province and the McArthur Basin are well studied; both regions host major base metal mineral deposits, and contain units prospective for hydrocarbons. In contrast, the South Nicholson Basin contains rocks that are mostly undercover, for which the basin evolution and resource potential are not well understood. To address this knowledge gap, the L210 South Nicholson Seismic Survey was acquired in 2017 in the region between the southern McArthur Basin and the western Mount Isa Province, crossing the South Nicholson Basin and Murphy Province. The primary aim of the survey was to investigate areas with low measured gravity responses (‘gravity lows’) in the region to determine whether they represent thick basin sequences, as is the case for the nearby Beetaloo Sub-basin. Key outcomes of the seismic acquisition and interpretation include (1) expanded extent of the South Nicholson Basin; (2) identification of the Carrara Sub-basin, a new basin element that coincides with a gravity low; (3) linkage between prospective stratigraphy of the Isa Superbasin (Lawn Hill Formation and Riversleigh Siltstone) and the Carrara Sub-basin; and (4) extension of the interpreted extent of the Mount Isa Province into the Northern Territory. <b>Citation:</b> Carr, L.K., Southby, C., Henson, P., Anderson, J.R., Costelloe, R., Jarrett, A.J.M., Carson, C.J., MacFarlane, S.K., Gorton, J., Hutton, L., Troup, A., Williams, B., Khider, K., Bailey, A.H.E. and Fomin, T., 2020. South Nicholson Basin seismic interpretation. In: Czarnota, K., Roach, I., Abbott, S., Haynes, M., Kositcin, N., Ray, A. and Slatter, E. (eds.) Exploring for the Future: Extended Abstracts, Geoscience Australia, Canberra, 1–4.