Methane-derived authigenic carbonates from the northern Gulf of Mexico — MD02 Cruise

dc.contributor.author Chen, Yifeng
dc.contributor.author Matsumoto, Ryo
dc.contributor.author Paull, Charles K.
dc.contributor.author Ussler, William
dc.contributor.author Lorenson, Thomas D.
dc.contributor.author Hart, Patrick E.
dc.contributor.author Winters, William J.
dc.date.accessioned 2008-04-09T13:23:51Z
dc.date.available 2008-04-09T13:23:51Z
dc.date.issued 2007-05-25
dc.description Author Posting. © The Author(s), 2007. This is the author's version of the work. It is posted here by permission of Elsevier B.V. for personal use, not for redistribution. The definitive version was published in Journal of Geochemical Exploration 95 (2007): 1-15, doi:10.1016/j.gexplo.2007.05.011. en
dc.description.abstract Authigenic carbonates were sampled in piston cores collected from both the Tunica Mound and the Mississippi Canyon area on the continental slope of the northern Gulf of Mexico during a Marion Dufresne cruise in July 2002. The carbonates are present as hardgrounds, porous crusts, concretions or nodules and shell fragments with or without carbonate cements. Carbonates occurred at gas venting sites which are likely to overlie gas hydrates bearing sediments. Electron microprobe, X-ray diffraction (XRD) and thinsection investigations show that these carbonates are high-Mg calcite (6 - 21 mol % MgCO3), with significant presence of framboidal pyrite. All carbonates are depleted in 13C (δ13C = -61.9 to -31.5 ‰ PDB) indicating that the carbon is derived mainly from anaerobic methane oxidation (AMO). Age estimates based on 14C dating of shell fragments and on regional sedimentation rates indicate that these authigenic carbonates formed within the last 1,000 yr in the Mississippi Canyon and within 5,500 yr at the Tunica Mound. The oxygen isotopic composition of carbonates ranges from +3.4 to +5.9 ‰ PDB. Oxygen isotopic compositions and Mg2+ contents of carbonates, and present in-situ temperatures of bottom seawater/sediments, show that some of these carbonates, especially from a core associated with underlying massive gas hydrates precipitated in or near equilibrium with bottom-water. On the other hand, those carbonates more enriched in 18O are interpreted to have precipitated from 18O-rich fluids which are thought to have been derived from the dissociation of gas hydrates. The dissociation of gas hydrates in the northern Gulf of Mexico within the last 5,500 yr may be caused by nearby salt movement and related brines. en
dc.description.sponsorship Financial support for this work was provided by the Grant-in-Aid from the Ministry of Education and Science and the Research Grant from JAPEX. en
dc.format.mimetype application/pdf
dc.format.mimetype application/vnd.ms-excel
dc.format.mimetype image/jpeg
dc.identifier.uri https://hdl.handle.net/1912/2166
dc.language.iso en_US en
dc.relation.uri https://doi.org/10.1016/j.gexplo.2007.05.011
dc.subject Methane-derived authigenic carbonates en
dc.subject Gulf of Mexico en
dc.subject High Mg-calcite en
dc.subject Carbon and oxygen isotope en
dc.subject Age of authigenic carbonates en
dc.subject Dissociation of gas hydrates en
dc.title Methane-derived authigenic carbonates from the northern Gulf of Mexico — MD02 Cruise en
dc.title.alternative Methane-derived authigenic carbonates from the northern Gulf of Mexico and their relation to gas hydrates en
dc.type Preprint en
dspace.entity.type Publication
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