Abstract
The Cooper subregion within the central Eromanga Basin is the Swiss army knife among Australia’s sedimentary basins. In addition to important oil and gas resources, it hosts abundant coal bed methane, important groundwater resources, features suitable conditions for enhanced geothermal systems, and is a potential site for carbon capture and storage. However, after seven decades of exploration, various uncertainties remain concerning its tectonic and thermal evolution. In this study, the public-domain 3D model of the Cooper and Eromanga stacked sedimentary basins was modified by integrating the latest structural and stratigraphic data, then used to perform numerical basin modelling and subsidence history analysis for a better comprehension of their complex geologic history. Calibrated 1D/3D numerical models provide the grounds for heat flow, temperature, thermal maturity, and sediment thickness maps. According to calibrated vitrinite reflectance profiles, a major hydrothermal/magmatic event at about 100 Ma with associated basal heat flow up to 150 mW/m2 caused source rock maturation and petroleum generation and probably overprinted most of the previous hydrothermal events in the study area. This event correlates with sedimentation rates up to 200 m/Ma and was apparently accompanied by extensive crustal shear. Structural style and depocentre migration analysis suggest that the Carboniferous–Triassic Cooper Basin initially has been a lazy-s shaped triplex pull-apart basin controlled by the Cooper Basin Master Fault before being inverted into a piggy-back basin and then blanketed by the Jurassic–Cretaceous Eromanga Basin. The interpreted Central Eromanga Shear Zone governed the tectonic evolution from the Triassic until today. It repeatedly induced NNW-SSE directed deformation along the western edge of the Thomson Orogen and is characterized by present-day seismicity and distinct neotectonic features. We hypothesize that throughout the basin evolution, alternating tectonic stress caused frequent thermal weakening of the crust and facilitated the establishment of the Cooper Hot Spot, which recently increased again its activity below the Nappamerri Trough.
Highlights
Since the 1950s, the intracontinental Cooper Basin (CB) in conjunction with the overlying Eromanga Basin (EB) in central eastern Australia (Figure 1a) has constituted Australia’s most important onshore petroleum province [1,2]
Structural style and depocentre migration analysis suggest that the Carboniferous–Triassic Cooper Basin initially has been a lazy-s shaped triplex pull-apart basin controlled by the Cooper Basin Master Fault before being inverted into a piggy-back basin and blanketed by the Jurassic–Cretaceous Eromanga Basin
The study area is located in central eastern Australia and comprises at least four superimposed sedimentary basin sequences: (1) the Cambrian to Ordovician Warburton Basin (WB), (2) the late Carboniferous to Triassic CB, (3) the Jurassic to Cretaceous EB, and (4) the Cenozoic Lake Eyre Basin (LEB)
Summary
Since the 1950s, the intracontinental Cooper Basin (CB) in conjunction with the overlying Eromanga Basin (EB) in central eastern Australia (Figure 1a) has constituted Australia’s most important onshore petroleum province [1,2]. The study area is located in central eastern Australia (outline of the CB after [3]; Figure 1b) and comprises at least four superimposed sedimentary basin sequences: (1) the Cambrian to Ordovician Warburton Basin (WB), (2) the late Carboniferous to Triassic CB, (3) the Jurassic to Cretaceous EB, and (4) the Cenozoic Lake Eyre Basin (LEB). The cross sections are intersecting each other in the centre of the Nappamerri Trough, approximately at the deepest point of the Cooper Basin
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