南非威特沃特斯兰德超群中生代韦斯特兰德群的无望礁中的铀分布

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引用次数: 0

摘要

中生代韦斯特兰德群(2932 - 2923 Ma)是威特沃特斯兰德超群的下部。与上覆的中央兰德群(Central Rand Group)因其世界级的砾岩型金铀矿床而闻名于世相比,韦斯特兰德群中古生界的经济潜力尚未得到充分挖掘。本研究旨在评估 Westrand 组中 Promise Reefs 的铀矿潜力。在 Westrand 地区对 Promise 礁的野外露头和从地表露头向下钻探的钻孔进行了调查。在砾岩中发现的放射性矿物包括白云母、勃氏硬岩、碳结核、独居石、绿帘石、透辉石和铀矿石。铀和钍的最大浓度分别为 630 ppm 和 125 ppm。地表露头砾岩的铀和钍浓度最高值分别为 111 ppm 和 140 ppm,铀平均值为 19.5 ppm,钍平均值为 26.6 ppm,U/Th 比率平均值为 0.6。数据比较显示,地表露头岩层的铀浓度通常低于未风化的等同岩层。此外,对地表露头岩层的相同样本进行γ-谱仪和 INAA 的铀化验得出的结果也不一致。由于现场γ-谱仪对铀的勘探依赖于 234U/238U 平衡的存在,并且由于地表样品中铀的贫化,因此采用了α-谱仪和铅同位素分析进行进一步的研究。地表砾岩中风化前的原始铀浓度是根据测量到的 Pb-同位素比值 206Pb/204Pb、207Pb/204Pb 和 208Pb/204Pb 以及 Pb 和 Th 浓度估算出来的。将这些数据插入铀-钍-铅年龄方程中,然后对这些方程进行重新制定,并对铀浓度进行求解。为了测试该方法,对一组钻孔样本进行了同样的处理。计算得出的新鲜岩石铀态性表明存在超生铀损失,其程度与新鲜砾岩样本实验沥滤造成的铀损失相同。在地表样品中发现的大量放射性铅表明,早在100Ma以前就出现了严重的铀损失。这些数据表明,风化的中原砾岩中铀的重新分布并不是由系统过程控制的,系统过程会掩盖风化前铀的原始浓度。铅同位素技术的应用证明,它是唯一能对深风化岩体中新鲜岩石铀态势进行估算的方法。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Uranium distribution in the promise reefs of the Mesoarchean Westrand Group, Witwatersrand Supergroup, South Africa
The Mesoarchean Westrand Group (2932 – 2923 Ma) constitutes the lower portion of the Witwatersrand Supergroup. Compared to the overlying Central Rand Group which is well known for its world-class conglomerate-hosted gold-uranium deposits, the economic potential of palaeoplacers in the Westrand Group has not been fully explored. This study aims to assess the uranium potential of the Promise Reefs in the Westrand Group. Field exposures of the Promise Reefs and boreholes drilled down-dip from the surface outcrops were investigated in the Westrand area. Three reef zones were recognized consisting of well-mineralized, matrix-to clast-supported, small pebble conglomerates with associated medium- to coarse-grained quartzite.
Radioactive minerals found in the conglomerates comprise leucoxene, brannerite, carbon nodules, monazite, allanite, thorite, and uraninite.
Analyses of U and Th from borehole samples reported mean values of 120 ppm for U and 60 ppm for Th. Maximum U and Th concentrations are 630 ppm and 125 ppm, respectively. The highest U/Th ratio was 17.4 with a mean value of 2. The conglomerates from surface outcrops have maximum U and Th concentrations of 111 ppm and 140 ppm, respectively, with a mean U value of 19.5 ppm and a mean Th value of 26.6 ppm, and a mean U/Th ratio of 0.6. Comparison of the data shows that surface outcrops generally report lower U concentrations than their unweathered equivalents.
Also, U assays by γ-spectrometry and INAA of the same samples from surface outcrops yielded inconsistent results. As U exploration by field γ-spectrometry relies on the existence of 234U/238U equilibrium and because of the U depletion in the surface samples, further investigations using α-spectrometry and Pb-isotope analyses were employed.
The results obtained from α-spectrometry point to complex U redistribution processes in the surface conglomerate with several stages of uranium loss and/or gain. The bulk of the U was removed during an early stage of surface exposure and supergene alteration, probably more than 1.4 Ma ago.
The estimation of the original pre-weathering U concentration in the surface conglomerates is based on the measured Pb-isotope ratios 206Pb/204Pb, 207Pb/204Pb, and 208Pb/204Pb and the Pb and Th concentrations. The data were inserted into U-Th-Pb age equations which were reformulated and solved for the U concentrations. To test the method, for a suite of borehole samples the same treatment was applied. The calculated fresh-rock U tenor indicates the occurrence of supergene uranium losses which are of the same magnitude as the U losses caused by experimental leaching of fresh conglomerate samples. The high amount of radiogenic Pb found in the surface samples points to severe uranium losses earlier than 100 Ma ago.
The data show that U redistribution in weathered Mesoarchean conglomerates is not governed by systematic processes which obscure the original pre-weathering U concentration. Application of the Pb isotope technique proves to be the only method yielding usable estimates of the fresh-rock uranium tenor in deeply weathered terranes.
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