Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/118801
Type: Conference item
Title: Thermal evolution and sediment provenance of the Cooper-Eromanga Basin: insights from detrital apatite
Author: Nixon, A.
Fernie, N.
Glorie, S.
Hand, M.
Citation: Thermo 2018: 16th International Conference on Thermochronology: conference abstracts, 2018, pp.146-146
Publisher: Universität Bremen
Issue Date: 2018
Conference Name: International Conference on Thermochronology (16 Sep 2018 - 21 Sep 2018 : Quedlinburg, Germany)
Statement of
Responsibility: 
Angus Nixon, Nicholas Fernie, Stijn Glorie, Martin Hand
Abstract: Despite the prolific hydrocarbon and geothermal potential within the central Australian Cooper-Eromanga Basin, the provenance and thermal history of the region remains rather elusive. This study presents new fission track, U-Pb and rare earth geochemical data for apatite samples from eight wells within the Cooper-Eromanga Basin. Based on these data, thermal history models were constructed and an apatite provenance study was carried out. The apatite samples taken from the upper Eromanga Basin sediments (Winton, Mackunda and Cadna Owie Formations) yielded a dominant population of early Cretaceous and minor population of late Permian – Triassic apatite ages that are (within error) equivalent to corresponding fission track age populations. Furthermore, the obtained Cretaceous apatite ages correlate well with the stratigraphic ages for each analysed formation, suggesting (1) little time lag between apatite exposure in the source region and sediment deposition, and (2) that no significant (>~100°C) reheating occurred after deposition. The apatites were likely distally sourced primarily from an eastern Australian volcanic arc (e.g. the Whitsunday Igneous Association), with minor sediment input from the New England and/or Mossman Orogens. Deeper samples (>2000m) from within the Cooper Basin (Toolachee Formation) yielded (partial) reset fission track ages, indicating heating to temperatures exceeding ~80-100°C after deposition. The associated thermal history models are broadly consistent with previous studies, and suggest that maximum temperatures were reached at ~95-70 Ma as a result of progressive heating by sedimentary burial and/or radiogenic basement heat loss. Subsequent late Cretaceous – Palaeogene cooling was evident in wells from the central and western Cooper Basin, but absent in wells from the shallower eastern margins. Such a cooling event remains enigmatic, and may be related with enhanced thermal conductivity as a response to aquifer flow and/or cementation. Similarly, only wells from the deeper central and western basin recorded a Neogene heating event, however, more data would be required to assess the significance of this more recent thermal perturbation.
Rights: Copyright status unknown
Grant ID: http://purl.org/au-research/grants/arc/LE150100145
Appears in Collections:Aurora harvest 4
Geology & Geophysics publications

Files in This Item:
There are no files associated with this item.


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.