排序方式: 共有73条查询结果,搜索用时 578 毫秒
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黔东南锦屏金矿成矿模式的模拟实验 总被引:2,自引:0,他引:2
利用中国科学院地球化学研究所矿床地球化学国家重点实验室的实验设备对黔东南锦屏金矿进行了成矿模式的模拟实验。通过剪切实验,变形、破裂实验,成矿物质活化、迁移实验,成矿模式模拟实验和多次应力实验,获得了成矿物质以碎粒流和塑性流动的方式顺层及穿层充填并在褶曲核部富集的结果,多次应力实验使成矿物质叠加富集。实验结果初步证实了锦屏石英脉金矿的成矿模式,为该区构造控制金矿提供了重要的实验资料,也为今后研究该区金矿的成矿规律和找矿提供了有益的信息。 相似文献
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峨眉山玄武岩之上宣威组中的沉积型铜矿,矿石矿物以铜硫化物和自然铜为主,矿石构造大多具有结核状,前人根据此特征将其命名为"马豆子式"铜矿.本文对该矿床中的铜结核进行了矿物学和同位素方面研究.矿物学研究表明,铜结核由含铁非晶质矿物、粘土以及碳质碎屑共同胶结铜的硫化物而组成,并以交代作用和沉积作用的方式形成;结核的原始形态是凝胶状物质组合体.同位素分析显示,碳沥青的13CPDB值在-24.8‰~-23.9‰之间,表明碳沥青是原地植物沉积变质的产物;辉铜矿的34SV-CDT值为7.6‰~13.1‰,与二叠纪海水的34S(约11‰)接近,斑铜矿、黄铜矿的δ^34SV-CDT值为21.6‰~22.2‰,和海相硫酸盐的硫同位素组成(20‰)类似,显示硫的来源不同.以上特征表明铜结核的形成过程是,含铜玄武岩经风化淋滤,铜质迁移到水体中后被粘土、含铁非晶质矿物和植物碎屑吸附,并成凝胶团悬浮与搬运,在湖泊或沼泽环境下与沉积物同生沉积成核;后期再经变质交代和热液叠加,斑铜矿交代辉铜矿、黄铜矿又叠加于斑铜矿之上,最终形成了"马豆子式"结核铜矿. 相似文献
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黔东南金矿是赋存在新元古代浅变质岩系中的石英脉型金矿,变质岩的原岩是一套火山-沉积岩,由凝灰岩、凝灰质砂岩、粉砂岩等组成,多具清楚的条纹韵律结构,反映了一种浊流沉积的环境。石英脉的产出受背斜构造和剪切断裂控制,有整合层间脉与断裂破碎带充填脉两种类型。石英脉的组成比较简单,除石英外,主要是硫化物类矿物及捕获的围岩成分。通过对5个矿点的石英中包裹体的Rb-Sr同位素测定和等时线法定年,确定其成矿时代为加里东期,与比邻的湘西同类型金矿的形成时代一致。根据赋矿地层岩性、地质演化历史与构造环境的比较,圈划出了一个湘黔加里东金矿带,对今后的找矿工作会有参考价值。 相似文献
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贵州东南部浊积岩中金矿的地质特征和成因 总被引:12,自引:0,他引:12
文章首次明确提出黔东南天柱县、锦屏县、黎平县以及相邻的湖南省靖县、会同县、洪江县存在浊积岩型金矿。研究发现,这些金矿均产在加里东皱褶带中,它们产于背斜的轴部,向两翼延伸,形成平行于地层的石英脉;另一种石英脉则充填于褶皱和剪切作用形成的剪切带或断裂带中。这些褶皱和断裂均呈北东方向。黔东南地区的浊积岩型金矿,均赋存于前震旦系下江群浊积岩中,产在板岩、凝灰岩或者在板岩和砂岩交界处。石英脉中金的富集与黄铁矿、毒砂、闪锌矿、方铅矿等密切相关。细脉比宽脉更富集金,断裂交叉处更富含金。石英脉两侧(尤其是顺层石英脉)的蚀变很弱,主要为硅化和绿泥石化。应用RB_SR方法测得石英脉的年龄为370~450Ma,成矿时代应在加里东期或期后。黔东南浊积岩金矿在品位(多数可见明金)、储量和产量方面均很有前景,研究它们具有十分重要的学术价值和经济意义。 相似文献
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位于内蒙古狼山北侧的霍各乞层状铜、铅锌、铁矿床产于中元古界狼山群变质岩中,许多学者对该矿床进行了研究,但在矿床成因的认识上还存在争议,沉积变质改造、海底喷流沉积、岩浆叠加等成因观点相持不下。本文引入区域古元古代—太古宙基底、矿区各种沉积变质岩和火山岩、新元古代及海西期岩浆岩的铅同位素组成,与矿石铅同位素组成对比,以确定矿石铅的来源。研究结果表明:1矿石中硫化物的铅同位素组成均一;2区域古元古代-太古宙基底岩石的铅同位素组成具有地球早期老铅的特点,同位素组成具有较大的变化范围,与矿石的铅同位素组成存在巨大的差… 相似文献
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ZHU Xiaoqing 《中国地球化学学报》2005,24(4):306-315
Experimental studies were undertaken on leaching of sedimentary rocks ( dolomite and sandstone) and Hg, Sb ores by distilled water under the condition of a completely open system (room temperature and room pressure). The aim is to find whether the halogen elements or metal elements first enter the solution at the early stage of meteoric waters converting to groundwaters and ore fluids, and, at the same time, to understand how and when they enter distilled water solutions from the rocks. The experimental resuhs have shown that F and Cl began to enter the fluids in the initial period of thirty days. With increasing leaching duration, the amounts of the elements that entered the fluids increased steadily. During the period from 120 days to 150 days the amounts increased more drastically, followed a slow increase. It is found that the capability of Cl entering the solutions is much greater than that of F. Hg and Sb were found not to have entered the solutions till 120 days later. During this period of time the pH value of the solutions began to drop. As for Hg and Sb ores, Hg and Sb began to enter the solutions on the 60th or 90th day, greatly ahead of schedule, but the two metallic elements in the rock samples began to enter the solutions 150 days later. Relatively speaking, Hg is more easily leached out than Sb from the rocks. In some rock samples, Sb could be detected in the solutions at the end of the experiment. However, Cu, Pb and Zn had not been detected in the leaching solutions from the beginning to the end of the experiment. In the whole leaching process the pH value of the solutions tend to decrease slowly from 7.1 at the beginning to 6.5 at the end. That is to say, in the interaction between pure water and rock the halogen elements in the rocks were preferentially leached out and then entered the fluids. With increasing water/rock reaction duration and amount of halogen-group elements in the solution and with decreasing pH value of the solution, some active metallic elements began to release in small amounts. This experimental result can explain the source and mechanism of volatile components and trace metals in underground waters. Meanwhile, as for those ore deposits produced by ore fluids derived from meteoric waters, the experimental result is also helpful to the understanding of the geochemical variation trend at the initial stage of conversion of meteoric waters to ore fluids. 相似文献
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