Abstract

We analyse the fluid flow regime within sediments on the Eastern levee of the modern Mississippi Canyon using 3D seismic data and downhole logging data acquired at Sites U1322 and U1324 during the 2005 Integrated Ocean Drilling Program (IODP) Expedition 308 in the Gulf of Mexico. Sulphate and methane concentrations in pore water show that sulphate–methane transition zone, at 74 and 94 m below seafloor, are amongst the deepest ever found in a sedimentary basin. This is in part due to a basinward fluid flow in a buried turbiditic channel (Blue Unit, 1000 mbsf), which separates sedimentary compartments located below and above this unit, preventing normal upward methane flux to the seafloor. Overpressure in the lower compartment leads to episodic and focused fluid migration through deep conduits that bypass the upper compartment, forming mud volcanoes at the seabed. This may also favour seawater circulation and we interpret the deep sulphate–methane transition zones as a result of high downward sulphate fluxes coming from seawater that are about 5–10 times above those measured in other basins. The results show that geochemical reactions within shallow sediments are dominated by seawater downwelling in the Mars-Ursa basin, compared to other basins in which the upward fluid flux is controlling methane-related reactions. This has implications for the occurrence of gas hydrates in the subsurface and is evidence of the active connection between buried sediments and the water column.

Highlights

  • Gas venting along passive continental margins is a widespread phenomenon (Berndt 2005)

  • Even if differential buoyancy naturally drives fluid upward, focused fluid migration is generally triggered by the interaction of several processes including: (i) pore fluid overpressure: sand-rich deepwater channels embedded within fine-grained sealing layers can preserve porosity and delay lithification, which favours liquefaction and upward fluid migration (Osborne & Swarbrick 1997); (ii) overpressure in sand-rich reservoirs

  • The Mars-Ursa Basin (Fig. 1) on the eastern levee of the modern Mississippi Canyon, at 800–2000 m water depth is a suitable site to study the processes that control fluid expulsion, because of the comprehensive data set that exists for this basin. It includes conventional and high resolution 3D seismic data provided by Shell and downhole logs and geochemical data acquired during the Integrated Ocean Drilling Program (IODP) Expedition 308

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Summary

Introduction

Gas venting along passive continental margins is a widespread phenomenon (Berndt 2005). The Mars-Ursa Basin (Fig. 1) on the eastern levee of the modern Mississippi Canyon, at 800–2000 m water depth is a suitable site to study the processes that control fluid expulsion, because of the comprehensive data set that exists for this basin. It includes conventional and high resolution 3D seismic data provided by Shell and downhole logs and geochemical data acquired during the Integrated Ocean Drilling Program (IODP) Expedition 308

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