Facies and NMR-based petrophysical analyses of the Apollonia unconventional gas reservoir: A case study from the BED–9 field, Abu Gharadig Basin, North Western Desert, Egypt

The Early Paleocene to Middle Eocene Apollonia Formation in the BED ‒ 9 field has been particularly interesting for unconventional hydrocarbon exploration since its discovery in 2006. However, the multiscale compositional and diagenetic inconsistencies present challenges for its characterization. This study aims to evaluate the petrophysical properties of the Apollonia Formation to locate the sweet-spot intervals. Moreover, it seeks to investigate reservoir rock types (RRTs), depositional settings, and the impact of diagenesis on reservoir quality. The findings of this study are as follows. 1) The Apollonia A5 and C1 units are identified as "sweet-spot" intervals. Their effective porosity ranges from 18 % to 35 %, average permeability varies from 0.1 to 2.0 mD, and water saturation falls between 40 % and 50 %, indicating good reservoir quality. 2) High-order eustatic sea-level changes and repetitive climatic change cycles significantly influence the alternating carbonate productivity and dilution cycles. Five distinct RRTs are classified, denoting a gradational facies change from clean, argillaceous, and carbonaceous chalky limestone to marl and interbedded shale intervals. 3) Interpreting the electro-facies responses, collated with microfacies variations and faunal content, deepens our understanding of the depositional environment, which extends from the inner- to outer-shelf setting. 4) The diagenetic processes have a dual impact that enhances and diminishes the reservoir quality. Finally, the gap in evaluating the petrophysical characteristics of all the Apollonia members has been addressed based on integrating the petrophysical and facies analysis for A, B, and C members. The Apollonia Formation has unique characteristics as an unconventional hydrocarbon resource. • Electro-facies patterns reveal the history of deposition and diagenesis impact. • The depositional environment of the Apollonia carbonates ranges from outer shelf to inner-shelf setting. • NMR well-logging data used to compute petrophysical reservoir properties.

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Publication Details

Journal
Energy Geoscience
Published
2025-06-08
DOI
https://doi.org/10.1016/j.engeos.2025.100428
Citations
3
Primary Topic
Hydrocarbon exploration and reservoir analysis
Type
article
Field-Weighted Citation Impact
2.59
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article

Facies and NMR-based petrophysical analyses of the Apollonia unconventional gas reservoir: A case study from the BED–9 field, Abu Gharadig Basin, North Western Desert, Egypt

Patrícia P.B. Eichler, Mohamed El-Kammar, A. Abdelsamad, Mohamed I. Abdel‐Fattah et al.
3 citations
Energy Geoscience
Hydrocarbon exploration and reservoir analysis
2.59
article

Facies and NMR-based petrophysical analyses of the Apollonia unconventional gas reservoir: A case study from the BED–9 field, Abu Gharadig Basin, North Western Desert, Egypt

Patrícia P.B. Eichler, Mohamed El-Kammar, A. Abdelsamad, Mohamed I. Abdel‐Fattah, Rania Abu-Ali, Ilius Mondal, Reem Roshdy
article en
3 citations

Abstract

The Early Paleocene to Middle Eocene Apollonia Formation in the BED ‒ 9 field has been particularly interesting for unconventional hydrocarbon exploration since its discovery in 2006. However, the multiscale compositional and diagenetic inconsistencies present challenges for its characterization. This study aims to evaluate the petrophysical properties of the Apollonia Formation to locate the sweet-spot intervals. Moreover, it seeks to investigate reservoir rock types (RRTs), depositional settings, and the impact of diagenesis on reservoir quality. The findings of this study are as follows. 1) The Apollonia A5 and C1 units are identified as "sweet-spot" intervals. Their effective porosity ranges from 18 % to 35 %, average permeability varies from 0.1 to 2.0 mD, and water saturation falls between 40 % and 50 %, indicating good reservoir quality. 2) High-order eustatic sea-level changes and repetitive climatic change cycles significantly influence the alternating carbonate productivity and dilution cycles. Five distinct RRTs are classified, denoting a gradational facies change from clean, argillaceous, and carbonaceous chalky limestone to marl and interbedded shale intervals. 3) Interpreting the electro-facies responses, collated with microfacies variations and faunal content, deepens our understanding of the depositional environment, which extends from the inner- to outer-shelf setting. 4) The diagenetic processes have a dual impact that enhances and diminishes the reservoir quality. Finally, the gap in evaluating the petrophysical characteristics of all the Apollonia members has been addressed based on integrating the petrophysical and facies analysis for A, B, and C members. The Apollonia Formation has unique characteristics as an unconventional hydrocarbon resource. • Electro-facies patterns reveal the history of deposition and diagenesis impact. • The depositional environment of the Apollonia carbonates ranges from outer shelf to inner-shelf setting. • NMR well-logging data used to compute petrophysical reservoir properties.

Energy GeoscienceVol. 6(3)
Cairo University (EG), Indian Institute of Technology Bombay (IN), Universidade Federal do Rio Grande do Norte (BR), Wave Dragon (Denmark) (DK)
Openalex Percentile: Top 11%
Hydrocarbon exploration and reservoir analysis
2.59
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