Thermal Maturity and Gas Generation in Upper Cretaceous Formations of the Beni Suef Basin, Egypt: Insights from Stable Carbon Isotopes and Geochemical Analysis of the Azhar-E1X Well

Sherif Farouk ¹ Saada Ahmed Saada ² Mohamed Arafat ³ Khaled Al-Kahtany ⁴ Thomas Gentzis ⁵ Amr S. Zaky ^6* Luigi Jovane ^7*

• ¹ Egyptian Petroleum Research Institute, Cairo, Cairo, Egypt
• ² Suez University, Suez, Suez, Egypt
• ³ Faculty of Science, South Valley university, Qena, Qena, Egypt
• ⁴ College of Science, King Saud University, Riyadh, Saudi Arabia
• ⁵ Core Laboratories, Reservoir Geology Group, Houston, TX, United States
• ⁶ Department of Geology, Faculty of Science, Menoufia University, Shibin El-Kom, Egypt
• ⁷ University of São Paulo, São Paulo, Rio Grande do Sul, Brazil

This study investigates the origin and thermal maturity of natural gases in Upper Cretaceous reservoirs within the Azhar-E1X well, Beni Suef Basin, Egypt, using stable carbon isotopic analyses of headspace gas samples. Gas shows within the Cretaceous succession, specifically the Bahariya Formation and the Abu Roash "F" Member (A/R "F" Member), were characterized. A total of 15 headspace gas samples and 5 mud gas samples were analyzed for molecular composition and stable carbon isotopic values (δ 13 C 1 , δ 13 C 2 , δ 13 C 3 ). Methane concentrations ranged from 69 to 1446 ppm in headspace samples and 961 to 5670 ppm in mud gases. Isotopic analysis suggests that gases from the A/R "E, F, and G" members are primarily derived from the primary cracking of kerogen. In contrast, gases from the underlying Bahariya Formation indicate a mixed origin, resulting from both primary cracking of coal-rich kerogen and secondary cracking of oil. The natural gases analyzed are predominantly thermogenic. A normal carbon isotope trend (δ 13 C 1 < δ 13 C 2 < δ 13 C 3 ) was observed in the headspace gas samples, where methane isotopic compositions are lower than those of ethane.