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Chromium stable isotope distributions in the southwest Pacific Ocean and constraints on hydrothermal input from the Kermadec Arc

dc.contributor.authorJanssen, David J.en
dc.contributor.authorGilliard, Delphineen
dc.contributor.authorRickli, Jörgen
dc.contributor.authorNasemann, Philippen
dc.contributor.authorKoschinsky, Andreaen
dc.contributor.authorHassler, Christel S.en
dc.contributor.authorBowie, Andrew R.en
dc.contributor.authorEllwood, Michael J.en
dc.contributor.authorKleint, Charlotteen
dc.contributor.authorJaccard, Samuel L.en
dc.date.accessioned2025-03-16T18:35:34Z
dc.date.available2025-03-16T18:35:34Z
dc.date.issued2023-02-01en
dc.description.abstractSpecial attention has been given to chromium (Cr) as a paleoproxy tracing redox cycling throughout Earth's history, due to differences in the solubility of its primary redox species at Earth's surface (Cr(III) and Cr(VI)) and isotope fractionation associated with their interconversion. In turn, chromium's paleoproxy potential has motivated studies of the modern ocean to better understand which processes drive its cycling and to constrain their impact on the Cr isotope composition (δ53Cr) of seawater. Here, we present total dissolved seawater Cr concentrations and δ53Cr along the GEOTRACES GP13 section. This section is a zonal transect extending from Australia in the subtropical southwest Pacific Ocean. Surface signals of local biological Cr cycling are minimal, in agreement with distributions of dissolved major nutrients as well as biologically-controlled trace metals in this low productivity, oligotrophic environment. Depth profiles have Cr concentration minima in surface waters and maxima at depth, and are largely shaped by the advection of nutrient- and Cr-rich subsurface waters rather than vertically-driven processes. Samples close to the sediment–water interface indicate important benthic Cr fluxes across the section. The GP13 transect crosses the hydrothermally-active Kermadec Arc. Hydrothermal fluids (consisting of <15% background seawater) were collected from three venting sites at the Brothers Volcano (along the Kermadec Arc). These fluids yielded near-crustal δ53Cr values (−0.17 to +0.08‰) and elevated [Cr] (7.5–23 nmol kg−1, hydrothermal endmember [Cr] ≈ 8–27 nmol kg−1), indicating that the Kermadec Arc may be an isotopically light Cr source. Dissolved [Fe] enrichments have been reported previously in deep waters (∼1600–3000 m) along the GP13 transect, east of the Kermadec Arc. These same waters show elevated [Cr] compared to Circumpolar Deep Water ([Cr] = 3.88 ± 0.11, δ53Cr = 0.89 ± 0.08, n = 32), with an average [Cr] accumulation of 0.71 ± 0.11 nmol kg−1 (1 SD), and an estimated δ53Cr of +0.46 ± 0.30‰ (2 SD, n = 9) for the accumulated Cr. Comparing high-temperature vent and neutrally buoyant plume data, hydrothermal-sourced Cr is likely negligable compared to Cr contributions from other processes (benthic fluxes, release from particles), and the advection of more Cr-rich Pacific Deep Water. It is unlikely that hydrothermal vents would be a major contributor within the regional or global biogeochemical Cr cycle, even if hydrothermal fluxes change by orders of magnitude, and therefore δ53Cr trends in the paleorecord may be attributable, at least in part, to major changes in other controls on Cr (e.g. widespread anoxia).en
dc.description.sponsorshipWe thank the captains, crews, and scientific members of the RV Southern Surveyor and the Marine National Facility for making voyage SS2011_V02 a success. We thank Martin Wille for Neptune support and sharing discussions and analytical expertise, and for providing a subsample of his Merck Cr(III) standard, originally from Ronny Schoenberg. We acknowledge funding from the Swiss National Science Foundation (SNSF grant PP00P2_172915) and by a European Research Council (ERC) Consolidator Grant (SCrIPT grant agreement 819139) to SLJ. We also acknowledge the Australian Research Council for funding under the Future Fellowships scheme to ARB (FT130100037), and the Antarctic Climate and Ecosystems Cooperative Research Centre. Hydrothermal fluid samples from Brothers Volcano, Kermadec Arc, were collected during research cruise SO253 with R/V Sonne; funding of this cruise by the BMBF (German Federal Ministry of Education and Research, project 03G0253) is greatly acknowledged. We thank associate editor Rachael James, Kohen Bauer, and an anonymous reviewer for constructive comments which have improved our manuscript. Chromium data were obtained on a Neptune Plus MC-ICP-MS acquired with funds from the NCCR PlanetS supported by SNSF grant 51NF40-141881. Maps and some figures were made using Ocean Data View (available at http://odv.awi.de ). We thank the captains, crews, and scientific members of the RV Southern Surveyor and the Marine National Facility for making voyage SS2011_V02 a success. We thank Martin Wille for Neptune support and sharing discussions and analytical expertise, and for providing a subsample of his Merck Cr(III) standard, originally from Ronny Schoenberg. We acknowledge funding from the Swiss National Science Foundation (SNSF grant PP00P2_172915) and by a European Research Council (ERC) Consolidator Grant (SCrIPT grant agreement 819139) to SLJ. We also acknowledge the Australian Research Council for funding under the Future Fellowships scheme to ARB (FT130100037), and the Antarctic Climate and Ecosystems Cooperative Research Centre. Hydrothermal fluid samples from Brothers Volcano, Kermadec Arc, were collected during research cruise SO253 with R/V Sonne; funding of this cruise by the BMBF (German Federal Ministry of Education and Research, project 03G0253) is greatly acknowledged. We thank associate editor Rachael James, Kohen Bauer, and an anonymous reviewer for constructive comments which have improved our manuscript. Chromium data were obtained on a Neptune Plus MC-ICP-MS acquired with funds from the NCCR PlanetS supported by SNSF grant 51NF40-141881. Maps and some figures were made using Ocean Data View (available athttp://odv.awi.de). DJ, DG, SJ designed the study, and CS, ARB and MJ designed GP13 field sampling and provided samples. ARB led the GP13 leg 1 voyage (SS2011_V02) of RV Southern Surveyor. AK and CK contributed Brothers Volcano samples. DJ processed and analyzed Brothers Volcano samples. DJ and DG processed GP13 samples and DJ analyzed the samples. DJ, DG and SJ led interpretations of the data. All authors contributed to interpretations and to the manuscript.en
dc.description.statustrueen
dc.format.extent14en
dc.identifier.otherresearchoutputwizard:a383154xPUB37942en
dc.identifier.otherScopus:85144789183en
dc.identifier.urihttps://dspace-test.anu.edu.au/handle/1885/733718899
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85144789183&partnerID=8YFLogxKen
dc.language.isoEnglishen
dc.rightsPublisher Copyright: © 2022 The Authorsen
dc.sourceGeochimica et Cosmochimica Actaen
dc.subjectChromiumen
dc.subjectChromium isotopesen
dc.subjectGEOTRACESen
dc.subjectHydrothermal fluxen
dc.subjectPaleoproxyen
dc.titleChromium stable isotope distributions in the southwest Pacific Ocean and constraints on hydrothermal input from the Kermadec Arcen
dc.typeArticleen
local.bibliographicCitation.lastpage44en
local.bibliographicCitation.startpage31en
local.contributor.affiliationJanssen, David J.; University of Bernen
local.contributor.affiliationGilliard, Delphine; University of Bernen
local.contributor.affiliationRickli, Jörg; Swiss Federal Institute of Technology Zurichen
local.contributor.affiliationNasemann, Philipp; University of Bernen
local.contributor.affiliationKoschinsky, Andrea; Constructor Universityen
local.contributor.affiliationHassler, Christel S.; University of Lausanneen
local.contributor.affiliationBowie, Andrew R.; University of Tasmaniaen
local.contributor.affiliationEllwood, Michael J.; Climate and Ocean Geoscience, Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationKleint, Charlotte; Constructor Universityen
local.contributor.affiliationJaccard, Samuel L.; University of Bernen
local.identifier.citationvolume342en
local.identifier.doi10.1016/j.gca.2022.12.010en
local.identifier.pure93e59b2d-897b-4993-99ea-5bb7fb8388a9en
local.type.statusPublisheden

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