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dc.contributor.authorArgentino, Claudio
dc.contributor.authorPanieri, Giuliana
dc.contributor.authorBjørnå, Eivind Urbye
dc.contributor.authorDessandier, Pierre-Antoine
dc.contributor.authorJamieson, John W.
dc.contributor.authorBünz, Stefan
dc.date.accessioned2025-06-11T11:44:23Z
dc.date.available2025-06-11T11:44:23Z
dc.date.issued2025-05-21
dc.description.abstractSlow–ultraslow spreading ridges represent half of the total length of the global mid-ocean ridge system and have been recognized to host hydrothermal activity. Their role as a source versus sink of elements in the oceans remains poorly constrained. Here, we present the first sediment data from the Aurora Vent Field (~3900 m depth) on the ultraslow spreading Gakkel mid-ocean ridge and the northernmost active vent field (82.9°N) explored to date. We interpret the composition of the cores at various distances from the vents based on physical parameters (P-wave velocity, gamma density, magnetic susceptibility, acoustic impedance and fractional porosity), mineralogy and (in)organic geochemistry (elemental analysis via X-Ray fluorescence and carbon–nitrogen systematics). Metalliferous sediments in two blade cores at <10 m from a black smoker are dominated by Fe-hydroxides (goethite) and Cu-Fe-bearing sulphide minerals (mainly chalcopyrite) that are rich in Co and Zn. These sediments form a friable crust associated with yellow microbial mats visible on the seafloor with the remotely operated vehicle imagery. Near-field plume deposits form an ~50 cm thick unit at the top of gravity cores close to the vents (<500 m). This unit transitions at further distance into laminated plume fallout deposits marked by high magnetic susceptibility and elevated ln(Fe/Ti), ln(Cu/Ti) and ln(Zn/Ti) values in the XRF profiles. Sedimentary organic matter in the investigated cores is dominated by a marine source, which is overprinted by microbial mats in the surface sediments of the blade cores. In one blade core, we found evidence of thermal alteration of the organic matter, typified by elevated C/N ratios and heavier δ<sup>13</sup>C<sub>TOC</sub>. Radiocarbon dating of foraminifera in a gravity core yielded an age of 27 230 cal bp, evidence for protracted vent activity preceding the Last Glacial Maximum 23 to 19 ka. Finally, we propose a sedimentological model for the Aurora hydrothermally influenced system that can be potentially exported to analogues worldwide.en_US
dc.identifier.citationArgentino C, Panieri G, Bjørnå EU, Dessandier P, Jamieson JW, Bünz S. Origin and composition of hydrothermally-influenced sediments at Aurora Vent Field, southwestern Gakkel Ridge (82.9°N). Sedimentology. 2025en_US
dc.identifier.cristinIDFRIDAID 2383600
dc.identifier.doi10.1111/sed.70018
dc.identifier.issn0037-0746
dc.identifier.issn1365-3091
dc.identifier.urihttps://hdl.handle.net/10037/37242
dc.language.isoengen_US
dc.publisherWileyen_US
dc.relation.journalSedimentology
dc.relation.projectIDNorges forskningsråd: 287869en_US
dc.relation.projectIDNorges forskningsråd: 274330en_US
dc.relation.projectIDNorges forskningsråd: 320100en_US
dc.rights.accessRightsopenAccessen_US
dc.rights.holderCopyright 2025 The Author(s)en_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0en_US
dc.rightsAttribution 4.0 International (CC BY 4.0)en_US
dc.titleOrigin and composition of hydrothermally-influenced sediments at Aurora Vent Field, southwestern Gakkel Ridge (82.9°N)en_US
dc.type.versionacceptedVersionen_US
dc.typeJournal articleen_US
dc.typeTidsskriftartikkelen_US


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Attribution 4.0 International (CC BY 4.0)
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