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Mesoproterozoic Gold in the Central Gawler Craton, South Australia: Geology, Alteration, Fluids, and Timing

机译:南澳大利亚州中部高勒克拉顿的中元古代金:地质,蚀变,流体和时间

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摘要

Similarities in mineralization and alteration style, host rocks, fluid compositions, and alteration-related 40Ar/39Ar ages from several recently discovered gold prospects support the existence of a significant Mesoproterozoic gold province spanning an arcuate region at least 300 km in length in the central Gawler craton, South Australia. At the recently discovered prospects of Tunkillia, Nuckulla Hill, Barns, and Weednanna, as well as at the historically mined Au deposit at Tarcoola, gold occurs as disseminated and veinlet-hosted mineralization focused in brittle to brittle-ductile faults and shear zones. Host rocks are principally ~1715 to ~1680 Ma granites but also include Hutchison Group (2000–1860 Ma) and Tarcoola Formation (~1650 Ma) metasedimentary rocks. Hydrothermal alteration is characteristically zoned around gold mineralization, with intense sericite-pyrite alteration and quartz veining proximal to gold mineralization and chlorite ± epidote ± hematite alteration distal from mineralization. Alteration was either synchronous with or, in some cases, continued after deformation. Gold is associated with pyrite and minor to trace galena, sphalerite, and chalcopyrite. Iron oxides are low in abundance in mineralized zones, which correspond to demagnetized zones. Fluid inclusion analyses suggest that multiple fluids were present in some systems, but one key fluid type occurs in each of the gold prospects: a low- to moderate-salinity (up to 10 wt % NaCl equiv) fluid with homogenization temperatures mostly in the range of ~150° to 300°C and commonly containing CO2 or associated with CO2-rich inclusions. Several features of the prospects are similar to those of orogenic- and intrusion-related gold deposits, but neither the prospect-scale geology nor the regional geologic setting in the central Gawler craton is sufficiently well understood to establish a genetic model or to confidently classify the mineralizing system. Hydrothermal white micas from several of the central Gawler craton gold prospects yield reproducible 40Ar/39Ar plateau ages of between 1567 and 1583 Ma. These ages, together with U-Pb zircon ages of granitic host rocks, constrain the timing of mineralization to the interval ~1690 to 1570 Ma, although we interpret the 40Ar/39Ar results to indicate a narrower mineralizing interval at ~1580 ± 10 Ma. This age range overlaps with, and is indistinguishable from, the range of U-Pb zircon ages reported from regional Hiltaba Suite granites and Gawler Range Volcanics, although igneous rocks of this age have not been identified locally at each of the prospects.
机译:矿化和蚀变样式,宿主岩, 流体组成以及与蚀变有关的 40 Ar / 39 Ar年龄( 最近发现的几个金矿勘探前景都支持一个中元古代重要的金矿的存在,该省跨越一个弧形的 区域,该区域的长度至少为300 km,位于中部Gawler克拉通克拉通中, < / sup>南澳大利亚。在最近发现的Tunkillia前景, Nuckulla Hill,Barns和Weednanna以及塔库拉(Tarcoola)历史上的 矿山金矿中,金的扩散和 小孔型成矿作用集中在脆性至脆性 断层和剪切带上。宿主岩主要为〜1715 to 〜1680 Ma花岗岩,但也包括和记集团(2000–1860 Ma)和塔库拉组(〜1650 Ma)的准沉积岩。 水热蚀变特征性地围绕金 矿化带,强烈的绢云母-黄铁矿蚀变和 石英脉趋于金矿化和绿泥石 ±变质是在成矿的末期。 变质与变形同步或在某些情况下持续 。金与黄铁矿和次要的 有关,以追踪方铅矿,闪锌矿和黄铜矿。矿化区中的 氧化铁含量较低,这对应于退磁的 区。流体包裹体分析表明,某些系统中存在多种流体 ,但是在每种金矿中都会出现一种关键的流体类型 :中低盐度(up <均质温度 主要在〜150°C至300°C范围内且通常包含 CO 2 或与富含CO 2 的夹杂物相关。矿床的几个特征 与与造山和侵入有关的 金矿床相似,但是远景规模地质和 区域性充分理解了Gawler克拉通中部的地质环境,可以建立成因模型或自信地对成矿系统进行分类。来自几个中部Gawler克拉通金矿前景的热液白云母产生可重现的 40 Ar / 39 Ar高原年龄在1567年和1583年之间。这些年龄与花岗岩宿主岩的U-Pb锆石年龄一起将 的成矿时间限制在〜1690到1570 Ma之间, 尽管我们将 40 Ar / 39 Ar结果解释为指示较小的 矿化间隔,但其约为〜1580±10 Ma。该年龄范围 与区域Hiltaba Suite花岗岩和 Gawler Range火山岩报告的U-Pb 锆石年龄范围重叠且无法区分,尽管尚未在每个勘探区中局部发现该年龄的火成岩。

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  • 来源
    《Economic Geology》 |2007年第8期|1511-1539|共29页
  • 作者单位

    Geoscience Australia, GPO Box 378, Canberra, ACT, 2601, Australia, and Research School of Earth Sciences, Australian National University, Acton, A.C.T. 0200, Australia;

    Geoscience Australia, GPO Box 378, Canberra, A.C.T. 2601, Australia;

    Department of Geology and Geophysics, University of Adelaide, GPO Box 498, Adelaide, South Australia 5005, Australia;

    Geoscience Australia, GPO Box 378, Canberra, ACT, 2601, Australia, and Research School of Earth Sciences, Australian National University, Acton, A.C.T. 0200, Australia;

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