首页> 外文期刊>Economic Geology >HERCYNIAN AGE OF THE COBALT-NICKEL-ARSENIDE-(GOLD) ORES, BOU AZZER, ANTI-ATLAS, MOROCCO: Re-Os, Sm-Nd, AND U-Pb AGE DETERMINATIONS
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HERCYNIAN AGE OF THE COBALT-NICKEL-ARSENIDE-(GOLD) ORES, BOU AZZER, ANTI-ATLAS, MOROCCO: Re-Os, Sm-Nd, AND U-Pb AGE DETERMINATIONS

机译:钴镍砷(金)矿石,BOU AZZER,抗阿特拉斯,摩洛哥的海西时代:Re-Os,Sm-Nd和U-Pb年龄测定

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The age of the hydrothermal Co-Ni-As-(Au) mineralization in the Bou Azzer-El Graara inlier was determined using different isotopic systems on ore and mineralization-related gangue minerals, namely Re-Os on molybdenite, Sm-Nd on carbonates, and U-Pb on brannerite. Re-Os dating of molybdenite was difficult owing to the intimate intergrowth of molybdenite with Co arsenides and the fact that sampling by drilling complex sulfide mixtures resulted in poor concentration of molybdenite. Accordingly, Re-Os dating of the impure molybdenite-sulfide mixtures yielded inconsistent ages in the range 400 to 350 Ma. This scatter is attributed to (1) inadequate concentration of pure molybdenite, (2) complex Re-Os systematics, possibly involving excess radiogenic Os derived from older generation(s) of sulfide, and/or (3) mixture of at least two Re-Os systems consisting of a component with pre-Hercynian history and later disturbance by Hercynian metamorphism. Carbonates and brannerite that coexist with molybdenite gave more consistent ages of 308 ± 31 Ma (Sm-Nd) and 310 ± 5 Ma (U-Pb), respectively. Because both ages agree within their errors, we regard the brannerite U-Pb age of 310 ± 5 (2) Ma as the best and most precise estimate for the age of the Co-Ni-As-(Au) mineralization. Although an earlier onset of mineralization cannot be ignored totally, the new age data underline that the principal Co-Ni-As-(Au) mineralization at Bou Azzer occupying the main ore-bearing structures was driven by and formed during the end of the Hercynian orogeny.
机译:使用不同的矿石和与成矿作用有关的脉石同位素系统确定了 布阿泽尔-埃尔格拉拉内矿的热液Co-Ni-As-(Au)矿化的年龄。矿物, 分别为辉钼矿上的Re-Os,碳酸盐上的Sm-Nd和 brannerite上的U-Pb。由于 辉钼矿与砷化砷的紧密共生,以及通过钻探复杂的硫化物混合物进行采样的事实,很难对辉钼矿进行Re-Os定年[ 的辉钼矿含量低。因此,不纯的辉钼矿-硫化物混合物的 Re-Os测年得出的 年龄不一致,在400-350 Ma之间。 归因于(1)浓度不充分的纯辉钼矿, (2)复杂的Re-Os系统,可能涉及衍生的过量放射源 Os来自较老一代的硫化物,和/或(3)至少两个Re-Os系统的混合物 ,该系统由具有 早海西前历史和后来扰动的成分组成通过海西变质作用。 与辉钼矿共存的碳酸盐和褐铁矿给出了 更一致的年龄308±31 Ma(Sm-Nd)和310± 5 Ma(U-Pb)。由于两个年龄都在其 误差范围内达成一致,因此我们认为褐变铀矿的U-Pb年龄为310±5 (2)Ma,这是对< sup> Co-Ni-As-(Au)矿化作用。尽管不能完全忽略较早发生的矿化 ,但是新的年龄数据 强调了主要的Co-Ni-As-(Au)矿化在

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    《Economic Geology》 |2009年第7期|1065-1079|共15页
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    Bundesanstalt für Geowissenschaften und Rohstoffe, Stilleweg 2, D-30655 Hannover, Germany;

    Bundesanstalt für Geowissenschaften und Rohstoffe, Stilleweg 2, D-30655 Hannover, Germany;

    Bundesanstalt für Geowissenschaften und Rohstoffe, Stilleweg 2, D-30655 Hannover, Germany;

    Goethe Universit?t Frankfurt, Institut für Geowissenschaften, Petrologie & Geochemie, Altenh?ferallee 1, D-60438 Frankfurt, Germany;

    AIRIE Program, Department of Geosciences, Colorado State University, Fort Collins, CO 80523-1482 USA and Geological Survey of Norway, Leiv Eirikssons vei 39, 7491 Trondheim, Norway;

    AIRIE Program, Department of Geosciences, Colorado State University, Fort Collins, CO 80523-1482 USA and Geological Survey of Norway, Leiv Eirikssons vei 39, 7491 Trondheim, Norway;

    REMINEX Exploration, Route de Casablanca, Lot. Elhamra Nr. 235, Marrakech - 40 000, Morocco;

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