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Abstract

AAPG Bulletin, V. 106, No. 5 (May 2022), P. 1005-1023.

Copyright ©2022. The American Association of Petroleum Geologists. All rights reserved.

DOI: 10.1306/06022120134

Methane migration mechanisms for the Green Canyon Block 955 gas hydrate reservoir, northern Gulf of Mexico

Li Wei,1 Ann Cook,2 and Kehua You3

1School of Earth Sciences, The Ohio State University, Columbus, Ohio; present address: Lamont-Doherty Earth Observatory, Columbia University, Palisades, New York; [email protected]
2School of Earth Sciences, The Ohio State University, Columbus, Ohio; [email protected]
3Institute for Geophysics, Jackson School of Geosciences, The University of Texas at Austin, Austin, Texas; [email protected]

ABSTRACT

In marine continental margins, high saturations of natural gas hydrate are observed within the gas hydrate stability zone, but the gas migration pathways to the hydrate reservoir are not commonly clear. We focus on a site in Green Canyon Block 955 (GC 955) in the Gulf of Mexico, where gas hydrate occurs in a 35-m-thick reservoir with saturations of 79%–93% in numerous centimeter- to decimeter-thick sandy silt layers and little to no gas hydrate in the interbedded centimeter- to decimeter-thick clayey silt layers. Different data sets (well logging, coring, and seismic data) suggest different types of potential methane migration mechanisms. For example, relatively high particulate organic carbon content in the reservoir and the microbial methane source indicated by gas chromatography and methane isotopes suggest gas might be made locally and migration could occur through dissolved methane sources or water advection. In contrast, the visible deeply rooted faults intersecting the gas hydrate reservoir and the gas pockets adjacent to the faults on seismic data suggest that free gas may migrate directly into the reservoir. We tested three different mechanisms to form gas hydrate at GC 955: short-range methane diffusion, short-range methane diffusion coupled with upward water advection, and free gas flow. The one-dimensional and two-dimensional numerical models show that both the short-range migration and the upward water advection are not enough to form high saturations gas hydrate at GC 955, and that free gas flow is required to form the high saturations of gas hydrate observed at GC 955.

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