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Porphyry copper deposit formation by sub-volcanic sulphur dioxide flux and chemisorption

dc.contributor.authorHenley, Richard W.
dc.contributor.authorKing, Penelope L.
dc.contributor.authorWykes, Jeremy L.
dc.contributor.authorRenggli, Christian J.
dc.contributor.authorBrink, Frank J.
dc.contributor.authorClark, David A.
dc.contributor.authorTroitzsch, Ulrike
dc.date.accessioned2015-04-16T05:34:14Z
dc.date.available2015-04-16T05:34:14Z
dc.date.issued2015-02-27
dc.date.updated2016-06-14T08:27:59Z
dc.description.abstractPorphyry copper deposits—the primary source of the world’s copper—are a consequence of the degassing of intrusion complexes in magmatic arcs associated with ancient subduction zones¹, ². They are characterized by copper and iron sulphides, commonly found with anhydrite (CaSO₄), over scales of several kilometres through intensely altered and fractured rocks1. The magmatic source of the metals is broadly understood, but the processes that transport and deposit the metals at the megaton scale are unclear. The hydrogen sulphide necessary for metal deposition is commonly assumed to form by a reaction between sulphur dioxide and water, but this reaction is inefficientᶟ and cannot explain the formation of economic-grade deposits. Here we use high-temperature laboratory experiments to show that a very rapid chemisorption reaction occurs between sulphur dioxide gas, a principal component of magmatic gas mixtures, and calcic feldspar, an abundant mineral in the arc crust. The chemisorption reaction generates the mineral anhydrite and hydrogen sulphide gas, and triggers deposition of metal sulphides. We use thermodynamic calculations to show that as magmatic gas cools and expands the concentration of hydrogen sulphide gas increases exponentially to drive efficient deposition of metal sulphides and consequent formation of economic-grade porphyry copper deposits.
dc.description.sponsorshipFunding was provided by an Australian Research Council Future Fellowship to P.L.K.en_AU
dc.identifier.issn1752-0894en_AU
dc.identifier.urihttp://hdl.handle.net/1885/13264
dc.publisherNature Publishing Group
dc.rights© 2015 Macmillan Publishers Limited
dc.sourceNature Geoscience
dc.titlePorphyry copper deposit formation by sub-volcanic sulphur dioxide flux and chemisorption
dc.typeJournal article
dcterms.dateAccepted2015-01-16
local.bibliographicCitation.issue3en_AU
local.bibliographicCitation.lastpage215en_AU
local.bibliographicCitation.startpage210en_AU
local.contributor.affiliationHenley, R. W., Research School of Earth Sciences, The Australian National Universityen_AU
local.contributor.affiliationKing, P. L., Research School of Earth Sciences, The Australian National Universityen_AU
local.contributor.affiliationWykes, J. L., Research School of Earth Sciences, The Australian National Universityen_AU
local.contributor.affiliationRenggli, C. J., Research School of Earth Sciences, The Australian National Universityen_AU
local.contributor.affiliationClark, D. A., Research School of Earth Sciences, The Australian National Universityen_AU
local.contributor.affiliationTroitzsch, U., Research School of Earth Sciences, The Australian National Universityen_AU
local.contributor.authoruidu3482508en_AU
local.identifier.absfor040307 - Ore Deposit Petrology
local.identifier.absseo840102 - Copper Ore Exploration
local.identifier.ariespublicationa383154xPUB1192
local.identifier.citationvolume8en_AU
local.identifier.doi10.1038/ngeo2367en_AU
local.identifier.scopusID2-s2.0-84923910891
local.publisher.urlhttp://www.nature.com/en_AU
local.type.statusPublished Versionen_AU

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