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Halogens in Atlantis Bank gabbros, SW Indian Ridge: Implications for styles of seafloor alteration

dc.contributor.authorKendrick, Mark
dc.date.accessioned2020-05-04T23:15:01Z
dc.date.issued2019
dc.date.updated2019-11-25T08:03:23Z
dc.description.abstractThe processes controlling halogen (F, Cl, Br, I) abundances in gabbroic ocean crust recovered from the 809-m deep Hole U1473A drilled on the Atlantis Bank during International Ocean Discovery Program (IODP) Expedition 360 were investigated. The aims were to provide new constraints on hydrothermal alteration and the abundances of halogens potentially transported to subduction zones in oceanic crust produced on a slow spreading ridge. Halogens in 51 gabbros and felsic veins have concentrations of ∼20-260 ppm F, 15-840 ppm Cl, 44-1230 ppb Br and 1-2490 ppb I. On average the gabbros retain a melt-derived magmatic F component of 58 ± 26% but are dominated by ∼96% hydrothermal Cl, Br, I and H2O. The abundances of hydrothermal Cl, Br and I are consistent with alteration at a seawater/rock ratio of <1. However, hydrothermal F is more enriched than expected and some amphiboles have high F/Cl ratios of 10-30 that provide evidence for the minor additional involvement of F-rich magmatic fluids. The abundant late-stage felsic veins that transect the gabbros and account for 1.5 vol.% of Hole U1473A lithologies are suggested as the most likely source of F-rich magmatic fluids. Downhole variations show F, Cl, Br and H2O are most abundant in amphibole- and clay-rich alteration zones at the top of the hole. The highest I concentrations of 1-2.5 ppm delineate an oxidised CO2-rich alteration zone in which seawater iodate was incorporated into carbonate and Fe-oxyhydroxide alteration. The role of iodate, which is more reactive than other halides, in generating I-rich alteration can be distinguished from alteration by I-rich sedimentary pore waters because the oxidised alteration is characterised by high I/Cl together with low Br/Cl, whereas organic matter in pore waters is enriched in both Br/Cl and I/Cl. The halogens have inferred compatibilities of F− > IO > OH− > Cl− ≥ Br− ∼ ≥ I− in the investigated alteration assemblage. EPMA and SHRIMP analyses indicate amphibole contains 1000-3000 ppm Cl in amphibolite facies alteration at the top of the Hole. Amphibole, chlorite and talc in greenschist facies alteration have much lower concentrations, typically in the range of 20-800 ppm Cl (median ∼100 ppm Cl), and F/Cl ratios of <4. In comparison, low temperature limonite (FeOOH.nH2O) has 160-8500 ppm Cl (median ∼840 ppm Cl). Amphibole is the dominant host of Cl and F in amphibolite facies alteration, but chlorite and limonite are important at lower grades. The samples have fairly constant Br/Cl ratios suggesting that Br excluded from the amphibole lattice is retained in minerals such as chlorite and/or non-structural sites. High I concentrations of 10's of ppm are inferred for some carbonate and limonite. Overall amphibole is a less dominant host of halogens than has been suggested previously, which has important implications for the eventual release and availability of halogens during subduction zone metamorphism.en_AU
dc.description.sponsorshipDr. M.A. Kendrick was supported by an Australian Research Council Future Fellowship (FT13 0100141). This work would not have been possible without the support of the International Ocean Discovery Program (IODP) and Australia-New Zealand IODP Consortium (ANZIC), which enabled Kendrick’s participation in Expedition 360. The IODP provided the samples and ANZIC provided postcruise funding for this study. ANZIC is supported by the Australian Government through the Australian Research Council’s LIEF funding scheme (LE140100047 and LE160100067) and the Australian and New Zealand consortium of Universities and government agencies. Kendrick greatly benefited from discussions with various members of the Expedition 360 Scientific Party both aboard the Joides-Resolution and in post-cruise settings: good hearty shellbacks the lot of them. Kendrick is grateful for the expert technical support of Pete Holden in the ANU SHRIMP laboratory and Xiaodong Zhang in the noble gas laboratory. Saroj Bhattacharyya at the UNSW X-ray Diffraction Laboratory is thanked for the XRD data. The author acknowledges the facilities, and the scientific and technical assistance, of the Australian Microscopy & Microanalysis Research Facility at the Centre of Advanced Microscopy, the Australian National University.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0012-821Xen_AU
dc.identifier.urihttp://hdl.handle.net/1885/203759
dc.language.isoen_AUen_AU
dc.provenance© 2019 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/)en_AU
dc.publisherElsevieren_AU
dc.relationhttp://purl.org/au-research/grants/arc/FT130100141en_AU
dc.relationhttp://purl.org/au-research/grants/arc/LE140100047en_AU
dc.relationhttp://purl.org/au-research/grants/arc/LE160100067en_AU
dc.rights© 2019 The Author(s).en_AU
dc.rights.licenseCC BY-NC-ND licenseen_AU
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/en_AU
dc.sourceEarth and Planetary Science Lettersen_AU
dc.titleHalogens in Atlantis Bank gabbros, SW Indian Ridge: Implications for styles of seafloor alterationen_AU
dc.typeJournal articleen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.lastpage107en_AU
local.bibliographicCitation.startpage96en_AU
local.contributor.affiliationKendrick, Mark, College of Science, ANUen_AU
local.contributor.authoruidKendrick, Mark, u4746994en_AU
local.description.notesImported from ARIESen_AU
local.identifier.absfor040203 - Isotope Geochemistryen_AU
local.identifier.absfor040311 - Stratigraphy (incl. Biostratigraphy and Sequence Stratigraphy)en_AU
local.identifier.absfor040304 - Igneous and Metamorphic Petrologyen_AU
local.identifier.absseo970104 - Expanding Knowledge in the Earth Sciencesen_AU
local.identifier.ariespublicationu5786633xPUB798en_AU
local.identifier.citationvolume514en_AU
local.identifier.doi10.1016/j.epsl.2019.02.034en_AU
local.identifier.scopusID2-s2.0-85063086991
local.publisher.urlhttps://www.elsevier.com/en_AU
local.type.statusPublished Versionen_AU

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