首页> 外文期刊>Economic geology and the bulletin of the Society of Economic Geologists >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 (2a) 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:在Bou Azzer-El Graara矿内热液Co-Ni-As-(Au)矿化的年龄是通过对矿石和与矿化有关的石矿物的不同同位素系统,即辉钼矿上的Re-Os,碳酸盐上的Sm-Nd来确定的。 ,以及褐煤中的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取样导致辉钼矿浓度低的事实,很难对辉钼矿进行Re-Os定年。因此,不纯辉钼矿-硫化物混合物的Re-Os测年产生了400-350 Ma范围的不一致年龄。这种散布归因于(1)纯辉钼矿的浓度不足;(2)复杂的Re-Os系统,可能涉及源自较老硫化物的过量放射源Os,和/或(3)至少两种Re的混合物-Os系统由具有前海西历史和后来受海西变质干扰的成分组成。与辉钼矿共存的碳酸盐和褐铁矿分别具有更一致的年龄308±31 Ma(Sm-Nd)和310 +-5 Ma(U-Pb)。因为这两个年龄都在其误差范围内达成一致,所以我们认为褐铁矿U-Pb年龄310 +-5(2a)Ma是对Co-Ni-As-(Au)矿化年龄的最佳和最精确的估计。尽管不能完全忽略较早的成矿作用,但新的年龄数据强调,占据主要矿床构造的Bou Azzer的主要Co-Ni-As-(Au)矿化作用是由海西期末驱动并形成的。造山运动。

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