金块:内幕故事

C.R.M. Butt, R.M. Hough, M. Verrall
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引用次数: 9

摘要

长期以来,金块一直吸引着地质学家、勘探者和公众的想象力,但它们的来源一直存在争议。澳大利亚的大多数金块都是在土壤表面或靠近土壤表面的地方发现的,这支持了表生起源。许多与土壤材料和风化岩石密切相关,甚至似乎包围着它们。即使是大块(例如2公斤),其表面特征和/或大体形态也表明风化层发生了化学再加工。相反,在10米或更深的风化层中发现了其他金块,在相当深的地方,在完全未风化的下生环境中发现了大块的黄金。来自澳大利亚、新几内亚、东南亚和巴西的许多矿床的金块和颗粒金已经通过光学和电子光学技术进行了检查,以确定可能表明其成因和风化层稳定性的特征。这些标本是在地表或接近地表的地方采集的,但所有的金块(质量范围约1克至8公斤)和许多较小的颗粒似乎都是下生的。它们的银含量几乎均匀,大多数在3%至20%的范围内,尽管有些没有检测到银。一个样品还含有高达3wt %的汞,但没有其他合金金属>检测到0.1 wt%。封闭矿物是罕见的-只有方铅矿,铋硫化物,方铅矿辉锑矿和复杂的银汞碲化物在少数样品。金块的内部结构包括几乎等边的、随机取向的晶体域。许多晶体显示出在晶体内终止的相干孪晶和/或短的非相干孪晶,所有这些都是在250°C温度下的典型热退火。一些来自东南亚的小块,也有退火织物,可能是热液再活化和再沉淀的产物。相比之下,来自新几内亚的一些标本含有10- 30 wt%的银,并具有内部结构,如分带和“蕨类”晶体习性。它们来自浅成热液矿床,自初始沉积以来未发生变形或再结晶。即使是最大的金块也有风化的内部证据。其中许多含有次生矿物,如氧化铁、粘土和方解石,但没有一种是完全封闭的。相反,它们都向金块的外缘开放,位于沿晶体边界相互连接的空隙中。这些边界也表现出银的耗尽,类似于外表面的耗尽边缘。EBSD分析显示,晶体取向在穿过或进入枯竭带时没有变化。这些特征表明,金块是在地表环境中溶解而非形成的,风化反应发生在表层,内部沿晶界发生。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Gold nuggets: the inside story

Gold nuggets: the inside story

Gold nuggets have long captured the imagination of geologists, prospectors and the public alike, but their origin remains disputed. Supporting a supergene origin, most gold nuggets in Australia have been found at or near the soil surface. Many are intimately associated with, and even appear to enclose, soil materials and weathered rock. Even large nuggets (e.g., >2 kg) have surface features and/or gross morphologies that suggest chemical reworking in the regolith. Conversely, other nuggets have been found at depths of ten metres or more in the regolith, and large masses of gold have been encountered at considerable depth, in completely unweathered, hypogene environments. Nuggets and particulate gold from many deposits in Australia, New Guinea, SE Asia and Brazil have been examined by optical and electron-optical techniques to determine characteristics that may indicate their genesis and stability in the regolith. The specimens have been collected at or close to the surface but all nuggets (mass range ~1 gm to >8 kg) and many smaller grains appear to be hypogene. They have nearly homogeneous Ag contents, mostly in the range 3 to 20 wt%, although some have no detectable Ag. One specimen also contains up to 3 wt% Hg, but no other alloyed metals > 0.1 wt% were detected. Enclosed minerals are rare – with only galena, Bi sulphide, galenobismutite and complex Ag-Hg tellurides in a few samples. The internal structure of the nuggets comprises nearly equigranular, randomly-oriented crystal domains. Many crystals display coherent twins and/or short incoherent twins that terminate within the crystal, all typical of thermal annealing at temperatures >250°C. Some small nuggets from SE Asia, also with annealing fabrics are possibly the product of hydrothermal remobilization and re-precipitation. In comparisons, some specimens from New Guinea contain 10->30 wt% Ag and have internal structures such as zoning and ‘fern-like’ crystal habits. These are derived from epithermal deposits and have not been deformed or recrystallized since initial deposition. Even the largest nuggets have internal evidence of weathering. Many have secondary minerals such as Fe oxides, clays and calcite within them, but none of these is fully enclosed. Rather, they are all open to the outer margin of the nuggets, situated in interconnecting voids along crystal boundaries. These boundaries also exhibit Ag depletion, similar to the depletion rims on the external surface. EBSD analysis shows there is no variation in crystallographic orientation across, or into, the depletion zones. These characteristics show that nuggets are dissolving in the surface environment, not forming, with weathering reactions initiated on the external surface and, internally, along crystal boundaries.

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