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Lode Gold and Epithermal Deposits of the Mallina Basin, North Pilbara Terrain, Western Australia

机译:西澳大利亚州北皮尔巴拉地带的马利纳盆地的金矿和超热矿床

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The Mallina basin, in the central west part of the North Pilbara terrain, is one of the more mineralized parts of the Pilbara craton. Three styles of Au mineralization are present in the region: (1) lode Au deposits associated with sericite-carbonate-pyrite alteration assemblages, (2) lode Au deposits associated with pyrophyllite-bearing alteration assemblages, and (3) lode Sb-Au deposits. Gold resources have been identified at the With-nell and Camel deposits just to the north of the east-trending Mallina shear zone. East-trending mineralized zones at the Withnell deposit are typical of turbidite-hosted lode Au deposits in that they are late tectonic (synto late- local D_3) and associated with extensive carbonate-sericite alteration. Gold mineralization occurs in planar quartz carbonate veins and with pyrite and arsenopyrite in the host rocks to the veins. Fluid inclusion analyses indicate mainly low-salinity, carbonic inclusions with moderate homogenization temperatures. The lode Sb-Au deposits have a similar structural setting and fluid characteristics. At the Camel 2 deposit Au is associated with syn- to late-D_3 pyrophyllitic shear zones that have overprinted an earlier carbonate alteration assemblage. Structural relationships and limited Pb isotope data suggest that the lode Au mineralization in this district formed at about 2900 Ma. In addition to the lode Au and Sb-Au deposits, north-northwest-trending quartz veins have textures typical of low-sulfidation epithermal deposits. The lithogeochemistry of samples collected from these veins indicates local enrichment of Au, As, Sb, Ag, Te, and Hg, which is consistent with an epithermal origin. Based on geologic relationships and Pb isotope data, these deposits are interpreted to have formed in the Mallina basin at ca. 2750 Ma. If they are true epithermal deposits, then they are among the oldest known. Their presence suggests that preservation, not Archean age, is the key control on the temporal distribution of epithermal deposits.
机译:位于北皮尔巴拉地区中西部的马利纳盆地是皮尔巴拉克拉通矿化程度较高的地区之一。该地区存在三种类型的金矿化:(1)与绢云母-碳酸盐-黄铁矿蚀变组合有关的金矿床;(2)与叶蜡石含蚀变组合有关的金矿床;(3)Sb-Au矿床。在东部趋势的马利纳剪切带以北的With-nell和Camel矿床中已经发现了黄金资源。 Withnell矿床的东向矿化带是浊积岩型金矿床的典型特征,因为它们是构造晚期(同化晚期-局部D_3),并且与广泛的碳酸盐-绢云母蚀变有关。金的矿化发生在平面状的碳酸盐石英脉中,黄铁矿和毒砂在脉中的主岩中发生。流体包裹体分析表明,主要是低盐度,碳质包裹体,均质温度中等。锑Sb-Au矿床具有相似的构造背景和流体特征。在骆驼2矿床,Au与晚期D_3的叶绿素剪切带有关,后者覆盖了较早的碳酸盐蚀变组合。结构关系和有限的Pb同位素数据表明,该地区的金矿矿床形成于2900 Ma左右。除了金矿和锑金矿床外,西北偏北趋势的石英脉还具有低硫化超热矿床的典型构造。从这些静脉收集的样品的岩性化学表明Au,As,Sb,Ag,Te和Hg的局部富集,这与超热起源一致。根据地质关系和铅同位素数据,这些矿床被解释为在马里纳盆地(约马萨诸塞州)形成。 2750毫安。如果它们是真正的超热矿床,那么它们就是已知最古老的矿床之一。他们的存在表明,保存而不是太古时代是对超热矿床时间分布的关键控制。

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