Journal
ARABIAN JOURNAL FOR SCIENCE AND ENGINEERING
Volume 48, Issue 1, Pages 695-710Publisher
SPRINGER HEIDELBERG
DOI: 10.1007/s13369-022-07242-1
Keywords
Upper Cretaceous; Organic-rich carbonates; Hydrogen-rich kerogen; Kinetics modeling; Wadi Ajloun; Northern Jordan
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This study examines the geochemical and petrological characteristics of carbonate-rich sediments from the Upper Cretaceous Shu'ayb Formation in northern Jordan. The organic matter characteristics and geological temperatures for oil generation are analyzed. The results suggest the presence of high TOC and hydrogen index, indicating Types I-II kerogens. The organic facies are sulfur-rich and exhibit the potential for producing paraffinic oil with low wax content. The distribution of activation energy and vitrinite reflectance values further support the Type II-S kerogen organic facies. This research provides insights into the organic-rich carbonate's potential for generating sulfur-rich oils.
This study examines the geochemical and petrological characteristics of 16 carbonate-rich (i.e., chalky marl, chalky limestone, and limestone) samples of the Upper Cretaceous Shu'ayb Formation in the Ajloun region, northern Jordan, to decipher the organic matter characteristics and predict the geological temperatures for oil generation. The carbonate-rich sediments under investigation exhibit high TOC (up to 12.39 wt%) and high hydrogen index (314-920 mg HC/g TOC), indicating Types I-II kerogens. The dominance of such hydrogen-rich kerogen is confirmed by the fluorescent alginite, amorphous organic matter (AOM), and bituminite organic matter. The studied organic facies are sulfur-rich and comprise of Type II organic matter, exhibiting the possibility of producing paraffinic oil with a low wax component, according to pyrolysis-gas chromatography. The broad distributions of activation energy (37-66 kcal/mol) in the bulk kinetic model of the analyzed samples show a mixture of organic matter (i.e., mainly marine-derived organic matter and minor land plant input). The kinetic models suggest that bulk petroleum formation began at relatively low geological temperatures between 104 and 116 degrees C, which corresponds to a vitrinite reflectance range of 0.58-0.66%. These activation energy distributions and low anticipated vitrinite reflectance values are largely compatible with the Type II-S kerogen organic facies, suggesting that the investigated Upper Cretaceous organic-rich carbonate may have produced sulfur-rich oils during the initial phases of kerogen conversion.
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