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31.
32.
洞嘎金矿位于西藏雄村矿集区, 是冈底斯成矿带较早发现且投入开采的金矿, 但研究程度低, 矿床成因存在较大争议。本文通过系统的矿床地质特征研究, 开展了硫化物原位硫同位素测试, 分析成矿物质来源, 进而探讨洞嘎金矿的成因。洞嘎金矿体受控于雄村组凝灰岩中的裂隙系统, 矿体呈脉状产出, 已探获金金属资源量9.55 t, 达到中型规模。矿石构造主要为脉状-细脉状构造, 金主要以包裹金和粒间金的形式赋存于黄铁矿和黄铜矿中。根据脉体穿插关系及矿物共生组合特征, 将洞嘎金矿的成矿过程划分为热液成矿期与表生氧化期, 其中热液成矿期为主成矿期, 可进一步划分为3个成矿阶段: 成矿早阶段、成矿主阶段及成矿晚阶段。洞嘎金矿床硫化物的硫同位素δ34S= –1.57‰~+5.26‰, 平均值+1.69‰, 具明显的塔式分布, 表明硫源具岩浆硫的特点。结合前人已发表的数据, 我们认为洞嘎金矿属于斑岩铜金成矿系统外围的热液脉型金矿床, 深部可能存在斑岩型铜金矿床, 找矿潜力极大。洞嘎金矿的成矿物质来源主要为地幔, 有少量的地壳物质(俯冲沉积物)加入。洞嘎金矿床的金与绿泥石密切相关, 该绿泥石主要为溶蚀-迁移-结晶机制形成, 绿泥石形成过程导致含金热液流体成分及物理化学性质发生改变, 使得成矿流体中的金发生卸载, 最终在凝灰岩的裂隙系统中形成洞嘎金矿床。 相似文献
33.
中国东南大陆晚侏罗世地层普遍缺失,仅零星见于个别地区,香港新界东北的荔枝庄组即为其一。荔枝庄组出露于香港世界地质公园沉积岩园区的荔枝庄地区,自下往上由火山岩—沉积岩—火山岩组合而成,沉积岩中发育大型包卷层理和滑塌构造等典型沉积构造,是香港地区最具代表性的晚侏罗世火山—沉积岩系。通过实测地层剖面研究,确定其成岩过程大体上可划分为早期普林尼式火山爆发、中期破火山口湖相沉积和晚期普林尼式火山爆发三个阶段,以湖相沉积作用为主、火山喷发作用为辅;受晚期火山岩浆活动的影响,沉积岩层普遍发生硅化或炭化。荔枝庄组独特的岩石组合与形成的古地理环境,为探讨中国东南大陆中生代火山活动—沉积作用方式与成岩过程,提供了难得的研究实例。 相似文献
34.
35.
介绍了两个主要矿集区成矿地质背景、成矿条件,及其典型矿床的研究,总结其成矿规律,建立成矿模式。中国硫铁矿的资源潜力,寄于深部找矿和前寒武纪古老地层的开发,应转移硫铁矿的工作重点于中、西部,扩大找矿线索,开辟新的找矿基地。 相似文献
36.
Treatment with metallic copper for the removal of elemental sulfur from bitumen extracted from sedimentary rocks or petroleum is the most widely used method. Little attention has been paid, however, to its disadvantages. It was observed that copper can interact with some polar organic substances during conventional sulfur removal, which can strongly influence the quantitative and qualitative determination of bitumen, as has been confirmed by interaction of long-chain fatty acids with copper. The copper soap generated was analyzed by element analysis, inductively coupled plasma optical emission spectrometry (ICP-OES), thermal analysis (TG-DSC) and Fourier Transform Infrared spectroscopy (FFIR). Mechanism of the interaction was investigated and elucidated. Our experimental results would necessitate improvement of the present method for sulfur removal and/or a search for a new one. 相似文献
37.
印度尼西亚Cikotok矿区帕瑟埃拉金矿位于巽他-班达岛弧的中部Bayah穹隆中,宏观上具有找到大型矿床的地质前提.成矿围岩为始新世末-中新世早期的安山岩,围岩蚀变强烈,分带性明显,金矿脉具有多条近平行产出特征.矿床有4个成矿阶段:石英-蒙脱石-绿泥石阶段,石英-绢云母-黄铁矿阶段,石英-冰长石-硫化物-含锰矿物阶段,块状石英阶段.矿床成因类型为大洋岛弧型低硫浅成低温热液型,细分类型为"Pongkor型"条带状低硫含金石英锰氧化物矿脉型金矿,其浅表部为热泉型金矿.矿床的深部找矿潜力大,具有大型金矿的成矿潜力. 相似文献
38.
西藏多龙矿集区发育世界典型的斑岩铜矿系统,文章选取区内多个代表性矿床开展硫同位素研究,并结合前人数据,为探讨该成矿系统成矿物质来源、流体演化过程提供了新证据.研究表明,波龙、拿若、拿厅、拿顿和铁格隆南矿床δ34S平均值相似(接近于0),指示含矿岩浆提供了各矿床所需的硫元素.此外,区内典型矿床流体演化过程可分为2类:①流体演化主要受控于温度变化,表现为δ34S随温度降低而降低(如拿顿矿床);②流体演化受温度和氧化还原状态共同影响,表现为δ34S随温度降低而升高(如:波龙和拿若矿床),或是随温度降低,δ34S波动变化范围较大(如拿厅和铁格隆南矿床).结合岩相学证据,文章推测热液体系氧化还原状态的变化是由水岩反应所导致,最后,文章提出多龙矿集区内矿化阶段硫化物通常具有较低的δ34S,指示成矿流体为高氧化性流体,并且该特征在类似矿床的找矿勘查工作中也可发挥积极的指示作用. 相似文献
39.
The Ediacara mineral field is situated 30 km W of Beltana on the western margins of the Flinders Ranges, South Australia, and consists of silver‐lead and copper deposits in lower Cambrian carbonate rocks that contain anomalous base‐metal contents throughout the Adelaide Geosyncline. The lower Cambrian rocks, which consist of the basal Parachilna Formation and overlying Ajax Limestone, rest disconformably on the Precambrian, and at Ediacara occupy a shallow N‐S elongate syncline near the hinge zone of the Adelaide Geosyncline. The main primary ore minerals of the silver‐lead mineralization are galena and pyrite, with very minor chalcopyrite and sphalerite, and rare tetrahedrite and pearceite. The gangue consists mainly of silica (both chalcedony and quartz), with minor dolomite and rare barite. The mineralization is stratabound and occurs in conformable zones, the lowest of which commences about 30–50 m above the base of the Cambrian sequence. The host to the silver‐lead mineralization, the Ajax Limestone, can be subdivided into three units which represent a set of lithologies, structures and organic traces indicative of a shallow near‐shore carbonate environment. The silver‐lead mineralization is mainly present in sandy and laminated dolomites which were deposited in an environment ranging from sub‐tidal to bar and channel and tidal flat, respectively. Four types of mineralization have been recognized; disseminated sulphides of syngenetic and/or diagenetic origin and epigenetic concentrations along stylolites, in veins and as breccia fillings. Post‐depositional solution activity has affected a large proportion of the carbonate sequence. The effects of this activity range from stylolites through stylobreccias to solution collapse breccias. The epigenetic concentrations of mineralizations have apparently been formed by the remobilization of the disseminated sulphides during solution activity. The ore and gangue minerals of the epigenetic mineralization display both euhedral forms and distinct colloform banding, and framboidal textures have also been observed in both pyrite and galena. There is evidence of repeated episodic precipitation and no simple paragenetic sequence can be recognized. Fluid inclusions in silica and dolomite associated with the epigenetic mineralization have homogenization temperatures of 159 to 199°C and freezing temperatures that indicate the fluids to be saline brines containing NaCl with CaCl2 and/or MgCl2. Sulphur isotope analyses show a range of 834S values from ‐12.5 to +8.6 per mil, with no evidence of significant differences between the four types of mineralization. The data suggest deposition of the disseminated sulphides as a result of biological reduction of seawater sulphate in a system partially open with respect to sulphate supply. Subsequent remobilization of sulphides apparently involved little or no sulphur isotope fractionation. The Ediacara silver‐lead deposits have many features in common with Mississippi Valley‐type lead‐zinc deposits and appear to have similarities in terms of genesis, in that the epigenetic mineralization has been formed as a result of post‐depositional solution activity during diagenesis in a sedimentary basin. The scale of transport of the metals deposited as the epigenetic mineralization at Ediacara appears, however, to have been very much less than that of the metals in other Mississippi Valley‐type deposits. 相似文献
40.
Juergen Schieber David Bish Max Coleman Mark Reed Elisabeth M. Hausrath John Cosgrove Sanjeev Gupta Michelle E. Minitti Kenneth S. Edgett Mike Malin 《Sedimentology》2017,64(2):311-358
The Sheepbed mudstone forms the base of the strata examined by the Curiosity rover in Gale Crater on Mars, and is the first bona fide mudstone known on another planet. From images and associated data, this contribution proposes a holistic interpretation of depositional regime, diagenesis and burial history. A lake basin probably received sediment pulses from alluvial fans. Bed cross‐sections show millimetre to centimetre‐scale layering due to distal pulses of fluvial sediment injections (fine‐grained hyperpycnites), fall‐out from river plumes, and some aeolian supply. Diagenetic features include mineralized synaeresis cracks and millimetre‐scale nodules, as well as stratiform cementation. Clay minerals were initially considered due to in situ alteration, but bulk rock chemistry and mineralogy suggests that sediments were derived from variably weathered source rocks that probably contained pre‐existing clay minerals. X‐ray diffraction analyses show contrasting clay mineralogy in closely spaced samples, consistent with at least partial detrital supply of clay minerals. A significant (ca 30 wt%) amorphous component is consistent with little post‐depositional alteration. Theoretical modelling of diagenetic reactions, as well as kinetic considerations, suggest that the bulk of diagenetic clay mineral formation occurred comparatively late in diagenesis. Diagenetic features (synaeresis cracks and nodules) were previously thought to reflect early diagenetic gas formation, but an alternative scenario of synaeresis crack formation via fabric collapse of flocculated clays appears more likely. The observed diagenetic features, such as solid nodules, hollow nodules, matrix cement and ‘raised ridges’ (synaeresis cracks) can be explained with progressive alteration of olivine/glass in conjunction with centrifugal and counter diffusion of reactive species. Anhydrite‐filled fractures in the Sheepbed mudstone occurred late in diagenesis when fluid pressures built up to exceed lithostatic pressure. Generating fluid overpressure by burial to facilitate hydraulic fracturing suggests a burial depth of at least 1000 m for the underlying strata that supplied these fluids. 相似文献