Gas hydrate reservoirs and gas migration mechanisms in the Terrebonne Basin, Gulf of Mexico

Hillman, Jess I. T.; Cook, Ann E.; Daigle, Hugh; Nole, Michael; Malinverno, Alberto; Meazell, Kevin; Flemings, Peter B.

doi:10.1016/j.marpetgeo.2017.07.029

Title: Gas hydrate reservoirs and gas migration mechanisms in the Terrebonne Basin, Gulf of Mexico

Journal Article · Thu Jul 27 00:00:00 EDT 2017 · Marine and Petroleum Geology

DOI:https://doi.org/10.1016/j.marpetgeo.2017.07.029· OSTI ID:1373260

^[1]; Cook, Ann E. ^[1]; Daigle, Hugh ^[2]; Nole, Michael ^[2]; Malinverno, Alberto ^[3]; Meazell, Kevin ^[2]; Flemings, Peter B. ^[2]

The Ohio State Univ., Columbus, OH (United States)
Univ. of Texas at Austin, Austin, TX (United States)
Lamont-Doherty Earth Observatory, Palisades, NY (United States)

Here, the interactions of microbial methane generation in fine-grained clay-rich sediments, methane migration, and gas hydrate accumulation in coarse-grained, sand-rich sediments are not yet fully understood. The Terrebonne Basin in the northern Gulf of Mexico provides an ideal setting to investigate the migration of methane resulting in the formation of hydrate in thin sand units interbedded with fractured muds. Using 3D seismic and well log data, we have identified several previously unidentified hydrate bearing units in the Terrebonne Basin. Two units are >100 m- thick fine-grained clay-rich units where gas hydrate occurs in near-vertical fractures. In some locations, these fine-grained units lack fracture features, and they contain 1-4-m thick hydrate bearing-sands. In addition, several other thin sand units were identified that contain gas hydrate, including one sand that was intersected by a well at the location of a discontinuous bottom-simulating reflector. Using correlation of well log data to seismic data, we have mapped and described these new units in detail across the extent of the available data, allowing us to determine the variation of seismic amplitudes and investigate the distribution of free gas and/or hydrate. We present several potential source-reservoir scenarios between the thick fractured mud units and thin hydrate bearing sands. We observe that hydrate preferentially forms within thin sand layers rather than fractures when sands are present in larger marine mud units. Based on regional mapping showing the patchy lateral extent of the thin sand layers, we propose that diffusive methane migration or short-migration of microbially generated methane from the marine mud units led to the formation of hydrate in these thin sands, as discontinuous sands would not be conducive to long-range migration of methane from deeper reservoirs.

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Research Organization:: The Ohio State Univ., Columbus, OH (United States); Univ. of Texas, Austin, TX (United States)

Sponsoring Organization:: USDOE Office of Fossil Energy (FE)

Grant/Contract Number:: FE0013919; FE0023919

OSTI ID:: 1373260

Alternate ID(s):: OSTI ID: 1549621

Journal Information:: Marine and Petroleum Geology, Vol. 86, Issue C; ISSN 0264-8172

Publisher:: ElsevierCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 34 works

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