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Generation and accumulation of hydrocarbons in the Gippsland basin, southeastern Australia

Thesis/Dissertation ·
OSTI ID:5497821
Clastic diagenesis of the reservoir rocks and organic geochemistry of the source rocks were studied in the offshore Central Deep of the Gippsland Basin. Pyrolysis, elemental analysis, and vitrinite reflectance data documented that the brown coal and dark shale of the Late Cretaceous-Eocene Latrobe Group served as the source rocks in the basin. The source rocks contain Type III kerogen with high organic carbon content (5 to 60%) and a genetic potential of 10 to 100 kg of hydrocarbon per ton of source rock. Hydrogen indices indicate that the Latrobe source rocks are both gas- and oil-prone. The zone of major hydrocarbon generation is located in the Upper Cretaceous; the Tertiary source rocks are still immature. Nuclear magnetic resonance, chemical extraction, and oxidative degradation analysis demonstrate that abundant organic acids have been released from the source rocks prior to major hydrocarbon generation. This study suggests that the porosity in the Latrobe sandstones has been modified by mechanical compaction. Dolomite cement distributed around paleo-channels was probably precipitated by the mixing of fresh water with sea water. Dissolution of the framework grains and cement, occurring predominantly in the temperature interval between 80 and 120 C, is believed to be caused by water-soluble organic acids. Burial history reconstructions, thermal modeling, and the calculation of transformation ratio suggest that the generation of hydrocarbons from the Latrobe source rocks started 90 Ma ago and is still occurring. A knowledge of the timing of hydrocarbon generation, porosity modification, hydrocarbon seal formation, and structure evolution is essential to the further exploration for hydrocarbon in the Gippsland Basin.
Research Organization:
Wyoming Univ., Laramie, WY (USA)
OSTI ID:
5497821
Country of Publication:
United States
Language:
English

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