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    Triggers for the formation of porphyry ore deposits in magmatic arcs

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    Wilkinson_Nature_Geosci.pdf
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    Authors
    Wilkinson, JJ
    Issue date
    13/10/2013
    Submitted date
    2017-07-10
    Subject Terms
    Porphyry ore
    Magmatic arcs
    subduction zones
    
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    Abstract
    Porphyry ore deposits are the source of much of the copper, molybdenum, gold and silver used by humans. Porphyry ore typically forms in magmatic arcs above subduction zones. However, generation of the largest deposits is often restricted to specific arc segments and limited periods of time. Here, I outline a hierarchy of four key triggers that may be involved in the formation of large porphyry deposits. The first process is characterized by a cyclical enrichment of magmas with metals and water in the deep crust. Second, saturation of the magma with sulphide facilitates the concentration of metals into smaller volumes of material from which they can later be released. The third process is an efficient transfer of metals into hydrothermal fluids that are exsolved from the magmas. Finally, localized processes trigger the precipitation of ore minerals in the crust. Although some or all of these processes must act in concert to generate large ore deposits, I argue that sulphide saturation of the magma is the most important step and that this can explain the temporal and spatial distribution of ores. Consequently, the fingerprint of sulphide saturation in igneous rocks could be used to identify those parts of magmatic arcs that are particularly predisposed to ore formation.
    Citation
    Wilkinson, J. J. (2012). Triggers for the formation of porphyry ore deposits in magmatic arcs. Nature Geoscience 6: 917–925. DOI:10.1038/NGEO1940
    Publisher
    Springer Nature
    Journal
    Nature Geoscience
    URI
    http://hdl.handle.net/10141/622499
    DOI
    10.1038/ngeo1940
    Type
    Journal Article
    Item Description
    © 2013 Macmillan Publishers Limited. All rights reserved. The attached document is the author’s final accepted version of the journal article. You are advised to consult the publisher’s version if you wish to cite from it.
    NHM Repository
    ISSN
    1752-0894
    EISSN
    1752-0908
    ae974a485f413a2113503eed53cd6c53
    10.1038/ngeo1940
    Scopus Count
    Collections
    Earth sciences

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