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        <dc:title>The importance of oxidized brines for the formation of australian Proterozoic stratiform sediment-hosted Pb-Zn (sedex) deposits</dc:title>
        <dc:creator>Cooke, DR</dc:creator>
        <dc:creator>Bull, SW</dc:creator>
        <dc:creator>Large, RR</dc:creator>
        <dc:creator>McGoldrick, PJ</dc:creator>
        <dc:subject>260104 Sedimentology</dc:subject>
        <dc:description>A two-fold subdivision for stratiform sediment-hosted Pb-Zn (sedimentary exhalative, sedex) deposits is proposed,&#13;
based on fundamental differences in the chemistry of the mineralizing brines. The type of sedimentary&#13;
basin from which the ore fluids are derived, and the litholOgies contained within the basin, control these differences&#13;
in fluid chemistry.&#13;
The two discrete brine types capable of transporting Zn and Pb are oxidized brines and reduced, acidic&#13;
brines. McArthur-type depOSits (e.g., McArtJ1Ur River, Mount 1sa, Hilton) precipitate from oxidized (SOJpredOminant),&#13;
acidic to near-neutral brines that evolve from sedimentary basins dominated by carbonates,&#13;
evaporites, and hematitic sandstones and shales. Selwyn-type depOSits (e.g., Sullivan, Rammelsberg, sedex deposits&#13;
of the Selwyn basin) precipitate from acidic, reduced (H2S-predominant) connate brines that evolved in&#13;
reduced siliciclastic and shale basins.&#13;
Temperature decrease and dilution (fluid mixing), addition of H2S, and pH increase can all be effective depOSitional&#13;
processes for Zn and Pb from reduced (Selwyn-type) brines. In conb'ast, sulfate reduction ancVor addition&#13;
of H2S (via fluid mixing or interaction with earlier formed pyrite) may be the important processes for&#13;
sphalerite and galena depOSition from oxidized (McArthur-type) brines. McAlthur-type sedex depOSits are intimately&#13;
associated with siderite or ferroan carbonate alteration halos and most l.ikEJy precipitate from lower&#13;
temperature brines than Selwyn-type deposits.&#13;
The redox state of the mineralized blines (sulfate or sulfide predominant) is impOltant for controlling minor&#13;
element associations in the two classes of sedex deposits. Weakly acidic to weakly alkaline oxidized brines CaIl&#13;
precipitate sidelite but are incapable of carrying Significant gold, tin, and barium in solution, and as such,&#13;
McArtllw-type deposits do not contain anomalous concentrations of these elements. Reduced, acid brines can&#13;
cany high concentrations of baJium, explaining the common association with barite in these deposits. If reduced&#13;
sulfur concentrations were sufficient in the mineralizing brines, individual Selwyn-type deposits may&#13;
contain anomalous or ore-wade gold. If the brines were higWy reduced (pylThotite-stable), they may have carried&#13;
high concentrations oftin (e.g., Sullivan). The lack of sulfide-bearing feeder systems in McArthur-type deposits&#13;
and their common occurrence in Selwyn-type depOSits probably also relate to the redox state of the brines.&#13;
From a mineral exploration perspective, oxidized sedimentary blines are more likely to produce large tonnage&#13;
Zn-Pb-Ag depOSits that have siderite or ankerite alteration halos and commonly lack barite lenses and vent&#13;
complexes. By contrast, deposits that form in reduced siliciclastic and shale-dominated basins are more likely&#13;
to be lower tonnage and to contain barite, vent complexes and may have minor gold or tin credits.</dc:description>
        <dc:date>2000-01</dc:date>
        <dc:type>Article</dc:type>
        <dc:type>PeerReviewed</dc:type>
        <dc:format>application/pdf</dc:format>
        <dc:identifier>http://eprints.utas.edu.au/6294/1/The_Importance_of_Oxidized_Brines.pdf</dc:identifier>
        <dc:relation>http://econgeol.geoscienceworld.org/cgi/content/abstract/95/1/1</dc:relation>
        <dc:identifier>Cooke, DR and Bull, SW and Large, RR and McGoldrick, PJ (2000) The importance of oxidized brines for the formation of australian Proterozoic stratiform sediment-hosted Pb-Zn (sedex) deposits. Economic Geology, 95 (1). pp. 1-18. ISSN 0361-0128</dc:identifier>
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