EGU23-6826, updated on 25 Feb 2023
https://doi.org/10.5194/egusphere-egu23-6826
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Submarine fans in the Kribi-Campo sub-basin, offshore Cameroon: Geomorphology and stratigraphic evolution during the Late Cretaceous

Boris Secke Bekonga Gouott1,2,3, Ovie Emmanuel Eruteya1, Yakufu Niyazi4, Mbida Yem2, Joseph Quentin Yene Atangana2, Adolphe Lorcin Maloh5, Samuel Makoube Etame5, and Elias Samankassou1
Boris Secke Bekonga Gouott et al.
  • 1Department of Earth Sciences, University of Geneva, Geneva, Switzerland (elias.samankassou@unige.ch)
  • 2Department of Earth Sciences, University of Yaoundé I, Yaoundé, Cameroon (jquentinyene@yahoo.fr)
  • 3Centre for Geological and Mining Research, Garoua, Cameroon
  • 4Minderoo-UWA Deep-Sea Research Centre, School of Biological Sciences and UWA Oceans Institute, The University of Western Australia, Australia( yakup.niyazi@uwa.edu.au)
  • 5National Hydrocarbon Corporation, Yaoundé, Cameroon (samuel.makoube@snh.cm)

Submarine fans are deposits of coarse sediments of continental origin in the deep sea, and are generally characterized by a complex depositional architecture, due to the multiple triggering mechanisms of deep-water sediment gravity flows. Consequently, this poses great challenges to deep water petroleum exploration and development. We analyzed the geomorphologic evolution and architecture of Campanian, deeply buried, submarine fans in the Kribi-Campo sub-basin, offshore Cameroon. Using a 3D seismic reflection data set and logs from two wells, we mapped seven horizons, including the fan base, fan top and five internal horizons. In cross-section, the fan is characterized by a high amplitude seismic facies exhibiting an aggradational pattern with parallel and continuous reflectors. The stacked fan-shaped morphology is up to 340 ms TWT thick, extends over an area of 600 km2 and oriented NE-SW, near the Kribi High. The analysis of lobes and channels on each horizon provided a timelapse that captures the major geomorphologic transformations of the submarine fan from its initiation, growth, and abandonment.  The submarine fan is composed of depositional lobes whose beds consist of sand, silt and mud. The detailed structure of these lobes has a finger-like morphology and is generally oriented at high angles to the channel that delivered the sediment to the lobes. The finger-like features are interpreted as thick massive sands, formed as a result of sediment-gravity flows which branched off the main flow eroding into pelagic clay substrate. Two types of channel morphology were identified (straight and sinuous). Our results show that channel and sand-body architecture evolve in a predictive manner, primarily controlled by fan aggradation. The elongated shape and morphology of the submarine fan may arise from the interaction of the fault-related folds and Kribi High, with sandstone deposition within the intervening topographic lows, sourced from the east. The 3D seismic geomorphological analysis of the submarine fan, as presented in this study, is essential to better understand their geometries, facies distribution, stacking patterns and depositional architecture to improve reservoir predictions.

How to cite: Secke Bekonga Gouott, B., Eruteya, O. E., Niyazi, Y., Yem, M., Yene Atangana, J. Q., Maloh, A. L., Makoube Etame, S., and Samankassou, E.: Submarine fans in the Kribi-Campo sub-basin, offshore Cameroon: Geomorphology and stratigraphic evolution during the Late Cretaceous, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-6826, https://doi.org/10.5194/egusphere-egu23-6826, 2023.