Abstract

The Permian tight clastic reservoir and Ordovician carbonate reservoir were developed in the central-southern Ordos Basin. This study investigated the fluid inclusion petrography, diagenetic fluid characteristics, formation process of natural gas reservoir, source rock characteristics, and reservoir accumulation characteristics of these Paleozoic strata by petrographic observations, scanning electron microscope imaging, fluid inclusion homogenization temperature, salinity, laser Raman spectrum, and gas chromatograph analyses. The results have suggested two phases of fluid inclusions in both the Permian sandstone and the Ordovician Majiagou Formation dolomite reservoirs, and the fluid inclusions recorded the history from the early thermal evolution of hydrocarbon generation to the formation, migration, and accumulation of natural gas. The early-phase inclusions show weak yellow fluorescence and recorded the early formation of liquid hydrocarbons, while the late-phase inclusions are nonfluorescent natural gas inclusions distributed in the late tectonic fractures and recorded the late accumulation of natural gas. The brine systems of the Permian and Ordovician fluid inclusions are, respectively, dominated by CaCl2-H2O and MgCl2-NaCl-H2O. The diagenetic fluids were in the ranges of medium-low temperature and moderate-low salinity. The natural gas hydrocarbon source rocks in the Ordos Basin include both the Permian coal-bearing rocks and the Ordovician carbonates. The process of the early-phase liquid hydrocarbon formation and migration into the reservoir corresponded to 220 Ma (Late Triassic). The late large-scale migration and accumulation of natural gas occurred at 100 Ma (early Late Cretaceous), which was close to the inclusion Rb/Sr isochron age of 89.18 Ma, indicating that the natural gas accumulation was related to the Yanshanian tectonic movement.

Highlights

  • The Ordos Basin is one of the most important natural gas resource exploration and development bases in China

  • Most discovered natural gas are stored in the Upper Paleozoic Permian clastic rock reservoir and the Lower Paleozoic Ordovician carbonate reservoir, and their natural gas accumulation theories have been established based on a large number of studies

  • The Lower Paleozoic Ordovician natural gas reservoirs are mainly karst cavernous reservoirs and dolomite reservoirs, and the gas accumulation was mainly controlled by karst paleogeomorphology [4,5,6]

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Summary

Introduction

The Lower Paleozoic Ordovician natural gas reservoirs are mainly karst cavernous reservoirs and dolomite reservoirs, and the gas accumulation was mainly controlled by karst paleogeomorphology [4,5,6] Both the Permian tight gas reservoirs and the Ordovician carbonate gas reservoirs discovered in the Ordos Basin are mainly distributed in the northern part of the basin, while the exploration progress in the vast southern area is relatively slow. Some scholars [18,19,20] believe that the natural gas in the northern part of the Ordos Basin originated from the southern region, and the natural gas migrated and accumulated on a large scale from south to north. Wang [13] believed that the “selfgeneration-self-storage” and the “lower-generation-upperstorage” were the main types of source-reservoir-cap assemblages, and the regional uplift movement around the end of the Early Cretaceous was the key period for the large-scale migration and accumulation of oil and coal gas in this area. The investigation will better characterize the petrography of the fluid inclusions and reveal the source rock characteristics, diagenetic fluid characteristics, isotopic dating, the natural gas components, gas accumulation characteristics, and phases

Geological Setting
Samples and Experiments
Fluid Inclusions
Discussion
Conclusion
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