Paper No. 206-12
Presentation Time: 4:10 PM
TRACKING DIAGENETIC ALTERATION OF MAGNETIC SUSCEPTIBILITY IN METHANE HYDRATE-BEARING MARINE SEDIMENTS OF THE CASCADIA MARGIN (ODP LEG 204 AND IODP EXPEDITION 311)
PHILLIPS, Stephen C., U.S. Geological Survey, Woods Hole, MA 02543; Institute for Geophysics, University of Texas at Austin, J.J. Pickle Research Campus, Building 196, 10100 Burnet Road (R2200), Austin, TX 78785, JOHNSON, Joel E., Dept. of Earth Sciences, University of New Hampshire, 56 College Rd, James Hall, Durham, NH 03824, CLYDE, William C., Department of Earth Sciences, University of New Hampshire, Durham, NH 03824, HONG, Wei-Li, Department of Geological Sciences, Stockholm University, Svante Arrhenius väg 8, Stockholm, 11418, Sweden, SETERA, Jacob, Cornell University, Department of Earth and Atmospheric Sciences, Ithaca, NY 14853 and TORRES, Marta E., College of Earth, Ocean, and Atmospheric Sciences, Oregon State University, 104 CEOAS Admin Bldg, Corvallis, OR 97331
Magnetic susceptibility (κ) is a mixed signal in marine sediments, representing primary depositional and secondary diagenetic processes. Production of hydrogen sulfide via anaerobic oxidation of methane at the sulfate-methane transition (SMT) and organoclastic sulfate reduction above the SMT can result in the dissolution of iron oxides and precipitation of iron sulfides, altering κ in marine sediments. We investigated records of κ from gas hydrate-bearing sites on the Cascadia margin (ODP Sites 1249 and 1252; IODP Site 1325) using a heavy mineral proxy from X-ray fluorescence core scanning to identify intervals of primary detrital κ and predict intervals affected by dissolution of magnetite. We interpret these intervals of lower-than-expected κ in the context of measured total sulfur (TS) content, grain size distributions, total organic carbon (TOC) content, and rock magnetic properties.
At Site 1249, a seep site at the crest of Hydrate Ridge, κ is lower than predicted for almost the entire upper 90 m below seafloor (mbsf), mostly corresponding to high TS, and some intervals with higher κ correspond to magnetic iron sulfides. At Site 1252, in a slope basin adjacent to Hydrate Ridge, the upper 100 msbf contains repeated intervals of low κ over the majority of the cored record, correlated with elevated TS and TOC content. At Site 1325, κ is reduced relative to predicted detrital κ between 24-51 mbsf correlating to elevated TS. Across all sites, κ negatively correlates with total sulfur content.
Integrating heavy mineral proxies with rock magnetic and geochemical records allows for a prediction of primary κ and the amount of κ loss at each site when compared to actual κ measurements, and these predictions are supported by total sulfur results. These measurements highlight that decreases in κ due to magnetite dissolution and pyrite precipitation are likely widespread along the Cascadia Margin in methane-bearing sediments. This draw down in κ is more intense at sites with gas seeps and high saturations of methane hydrate. At non-seep sites with more disseminated, low concentration hydrate, alterations of κ are more episodic and correlated with TOC content. The results from these sites suggest that integrating magnetic and geochemical data with κ records can provide insight into the geologic evolution of hydrate systems.