Sedimentology and gas hydrates of IODP Expedition 311 samples

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Hauptverfasser: Torres, Marta E, Tréhu, Anne M, Cespedes, N, Kastner, Miriam, Wortmann, Ulrich G, Kim, Jung-Hyun, Long, Philip E, Malinverno, Alberto, Pohlman, John W, Riedel, Michael, Collett, Tim S
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Sprache:en
Veröffentlicht: PANGAEA 2008
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author Torres, Marta E
Tréhu, Anne M
Cespedes, N
Kastner, Miriam
Wortmann, Ulrich G
Kim, Jung-Hyun
Long, Philip E
Malinverno, Alberto
Pohlman, John W
Riedel, Michael
Collett, Tim S
author_facet Torres, Marta E
Tréhu, Anne M
Cespedes, N
Kastner, Miriam
Wortmann, Ulrich G
Kim, Jung-Hyun
Long, Philip E
Malinverno, Alberto
Pohlman, John W
Riedel, Michael
Collett, Tim S
collection Datos científicos de ciencias marinas y ambientales
contents Expedition 311 of the Integrated Ocean Drilling Program (IODP) to northern Cascadia recovered gas-hydrate bearing sediments along a SW-NE transect from the first ridge of the accretionary margin to the eastward limit of gas-hydrate stability. In this study we contrast the gas gas-hydrate distribution from two sites drilled ~ 8 km apart in different tectonic settings. At Site U1325, drilled on a depositional basin with nearly horizontal sedimentary sequences, the gas-hydrate distribution shows a trend of increasing saturation toward the base of gas-hydrate stability, consistent with several model simulations in the literature. Site U1326 was drilled on an uplifted ridge characterized by faulting, which has likely experienced some mass wasting events. Here the gas hydrate does not show a clear depth-distribution trend, the highest gas-hydrate saturation occurs well within the gas-hydrate stability zone at the shallow depth of ~ 49 mbsf. Sediments at both sites are characterized by abundant coarse-grained (sand) layers up to 23 cm in thickness, and are interspaced within fine-grained (clay and silty clay) detrital sediments. The gas-hydrate distribution is punctuated by localized depth intervals of high gas-hydrate saturation, which preferentially occur in the coarse-grained horizons and occupy up to 60% of the pore space at Site U1325 and > 80% at Site U1326. Detailed analyses of contiguous samples of different lithologies show that when enough methane is present, about 90% of the variance in gas-hydrate saturation can be explained by the sand (> 63 µm) content of the sediments. The variability in gas-hydrate occupancy of sandy horizons at Site U1326 reflects an insufficient methane supply to the sediment section between 190 and 245 mbsf.
format Dataset Open Access
id pangaea_https___doi_org_10_1594_PANGAEA_716589
institution PANGAEA
language en
publishDate 2008
publisher PANGAEA
record_format pangaea
spellingShingle Sedimentology and gas hydrates of IODP Expedition 311 samples
Torres, Marta E
Tréhu, Anne M
Cespedes, N
Kastner, Miriam
Wortmann, Ulrich G
Kim, Jung-Hyun
Long, Philip E
Malinverno, Alberto
Pohlman, John W
Riedel, Michael
Collett, Tim S
311-U1325B; 311-U1325C; 311-U1326C; 311-U1326D; Cascadia Margin Gas Hydrates; DRILL; Drilling/drill rig; Exp311; Integrated Ocean Drilling Program / International Ocean Discovery Program; IODP; Joides Resolution
Expedition 311 of the Integrated Ocean Drilling Program (IODP) to northern Cascadia recovered gas-hydrate bearing sediments along a SW-NE transect from the first ridge of the accretionary margin to the eastward limit of gas-hydrate stability. In this study we contrast the gas gas-hydrate distribution from two sites drilled ~ 8 km apart in different tectonic settings. At Site U1325, drilled on a depositional basin with nearly horizontal sedimentary sequences, the gas-hydrate distribution shows a trend of increasing saturation toward the base of gas-hydrate stability, consistent with several model simulations in the literature. Site U1326 was drilled on an uplifted ridge characterized by faulting, which has likely experienced some mass wasting events. Here the gas hydrate does not show a clear depth-distribution trend, the highest gas-hydrate saturation occurs well within the gas-hydrate stability zone at the shallow depth of ~ 49 mbsf. Sediments at both sites are characterized by abundant coarse-grained (sand) layers up to 23 cm in thickness, and are interspaced within fine-grained (clay and silty clay) detrital sediments. The gas-hydrate distribution is punctuated by localized depth intervals of high gas-hydrate saturation, which preferentially occur in the coarse-grained horizons and occupy up to 60% of the pore space at Site U1325 and > 80% at Site U1326. Detailed analyses of contiguous samples of different lithologies show that when enough methane is present, about 90% of the variance in gas-hydrate saturation can be explained by the sand (> 63 µm) content of the sediments. The variability in gas-hydrate occupancy of sandy horizons at Site U1326 reflects an insufficient methane supply to the sediment section between 190 and 245 mbsf.
title Sedimentology and gas hydrates of IODP Expedition 311 samples
topic 311-U1325B; 311-U1325C; 311-U1326C; 311-U1326D; Cascadia Margin Gas Hydrates; DRILL; Drilling/drill rig; Exp311; Integrated Ocean Drilling Program / International Ocean Discovery Program; IODP; Joides Resolution
url https://doi.org/10.1594/PANGAEA.716589