共查询到20条相似文献，搜索用时 22 毫秒
1.
环巴尔喀什-西准噶尔成矿省矿床类型、成矿系统和跨境成矿带对接 总被引：4，自引：2，他引：2
环巴尔喀什-西准噶尔成矿省地处中亚成矿域核心区,古生代构造和岩浆活动强烈,成矿作用丰富多样,发育许多大型-超大型乃至世界级的金属矿床,包括斑岩型铜矿床、斑岩-石英脉-云英岩型钨钼矿床、矽卡岩型铜(多金属)矿床、火山成因块状硫化物型(VMS)多金属矿床、浅成低温热液型金矿床、石英脉-蚀变岩型中温热液金矿床、与花岗岩有关的Be-U矿床、岩浆熔离型铜镍硫化物矿床和豆荚状铬铁矿等,这些矿床集中分布,形成多处成矿带,包括哈萨克斯坦的扎尔玛-萨吾尔、波谢库尔-成吉斯和北巴尔喀什等成矿带以及新疆西准噶尔的萨吾尔、谢米斯台-沙尔布提和巴尔鲁克-克拉玛依等成矿带。哈萨克斯坦包含大型-超大型和世界级金属矿床的成矿带向东是否延入新疆西准噶尔?能否实现新疆西准噶尔找矿重大突破?都是备受关注的重大地质找矿问题。本文在前人研究并结合作者工作基础上,根据成矿带的成矿构造环境、矿床类型、成矿特点和成矿时代,总结出成矿省至少发育九类成矿系统,即(1)奥陶纪-志留纪岛弧斑岩型Cu-Au成矿系统;(2)奥陶纪岛弧VMS型多金属成矿系统;(3)泥盆纪岛弧岩浆熔离型铜镍硫化物成矿系统;(4)泥盆纪与蛇绿岩有关的豆荚状铬铁矿成矿系统;(5)早石炭世岛弧斑岩-浅成低温热液型Cu-Au成矿系统;(6)石炭纪岛弧斑岩型-矽卡岩型Cu-Mo-Au成矿系统;(7)晚石炭世弧后盆地与花岗岩有关的Be-U成矿系统;(8)早二叠世岛弧或岛弧和陆缘弧过渡弧斑岩-石英脉-云英岩型Mo-W成矿系统;(9)早二叠世岛弧石英脉-蚀变岩型中温热液金成矿系统。对比研究发现境内外相邻成矿带具有相同或相似的成矿系统,二者可以对接,新疆西准噶尔三条成矿带分别是哈萨克斯坦三条成矿带的东延部分,构成了成矿省北部的扎尔玛-萨吾尔Cu-Au成矿带、中部的波谢库尔-成吉斯-谢米斯台Cu-Au-Be-U多金属成矿带和南部的北巴尔喀什-克拉玛依Cu-Mo-W-Au-Cr成矿带。新疆西准噶尔具有形成大型-超大型矿床的成矿系统和成矿条件,有望实现找矿勘探的更大突破。 相似文献
2.
近20年来,越来越多的大型金属矿床在盆地内部及其边缘被发现。传统的勘查地球化学方法对盆地及盆山边缘覆盖区无能为力,深穿透地球化学探测技术为解决盆地及其边缘覆盖区找矿难题提供了一种行之有效的手段。文章通过对沉积砂岩盆地铀矿、火山岩盆地银多金属矿、变质岩盖层铜镍矿和沉积盖层金矿开展探测试验,得出:(1)砂岩型铀矿中活动性铀主要以铀酰络阳离子的形式存在,铀酰络阳离子很容易受地下水运动及蒸发蒸腾作用而发生迁移,迁移通道包括砂岩的孔隙、构造裂隙等,到达地表后,铀酰络阳离子易与土壤中带负电的黏土矿物结合而赋存其中,使用微细粒分离和活动态提取两种方法均能圈定矿致异常;(2)火山岩盆地中,与火山岩近乎同期形成的矿床,矿床形成过程中含矿流体携带成矿元素银、金、铜等沿构造裂隙运移,迁移到地表后被土壤中的黏土矿物所吸附,使用土壤活动态测量和微细粒分离测量均能有效圈定已知矿体,异常直接位于矿体上方;(3)变质岩盆地超基性岩体在侵位过程中,岩体与变质岩接触带将产生大量的构造裂隙,因此当流体通过岩体与围岩接触带时,将携带矿体中铜、镍向上迁移至地表,形成环状异常;(4)洛宁盆地金矿成矿过程中,成矿元素金、银等以络合物、纳米级单质或合金等形式通过流体携带顺着构造破碎带向上迁移,地表岩石风化发生成矿元素解离,后期被黄土覆盖,矿体或岩石解离的化合物或纳米颗粒可以穿过黄土孔隙向上迁移至地表,并赋存于表层黄土的细粒级黏土中,因此采用土壤微细粒分离测量可圈出矿致异常。本文根据深穿透地球化学方法应用效果,异常的形态,并结合盖层的特点,成矿元素的存在形式、迁移方式以及在地表的赋存状态,初步建立了盆地金属矿深穿透地球化学勘查模型,为盆地盖层区地球化学勘查提供了理论与技术支撑。 相似文献
3.
Tectono-metallogenic systems are geological systems that link geodynamic and tectonic processes with ore-forming processes. Fundamental geodynamic processes, including buoyancy-related processes, crustal/lithospheric thinning and crustal/lithospheric thickening, have occurred throughout Earth's history, but tectonic systems, which are driven by these processes, have evolved as Earth's interior has cooled. Tectonic systems are thought to have evolved from magma oceans in the Hadean through an unstable “stagnant-lid” regime in the earlier Archean into a proto-plate tectonic regime from the late Archean onwards. Modern-style plate tectonics is thought to have become dominant by the start of the Paleozoic. Mineral systems with general similarities to modern or geologically recent systems have been present episodically (or semi-continuously) through much of Earth's history, but most of Earth's present endowment of mineral wealth was formed during and after the Neoarchean, when proto- or modern-style plate tectonic systems became increasingly dominant and following major changes in the chemistry of the atmosphere and hydrosphere. Changes in the characteristics of some mineral systems, such as the volcanic-hosted massive sulphide (VHMS) system, reflect changes in tectonic style during the evolution towards the modern plate tectonic regime, but may also involve secular changes in the hydrosphere and atmosphere.Whereas tectono-metallogenic systems have evolved in general over Earth's history, specific tectono-metallogenic systems evolve over much shorter time frames. Most mineral deposits form in three general tectono-metallogenic systems: divergent systems, convergent systems, and intraplate systems. Although fundamental geodynamic processes have driven the evolution of these systems, their relative importance may change as the systems evolved. For example, buoyancy-driven (mantle convection/plumes) and crustal thinning are the dominant processes driving the early rift stage of divergent tectono-metallogenic systems, whereas buoyancy-driven processes (slab sinking) and crustal thickening are the most important processes during the subduction stage of convergent systems. Crustal thinning can also be an important process in the hinterland of subduction zones, producing back-arc basins that can host a number of mineral systems. As fundamental geodynamic processes act as drivers at some stage in virtually all tectonic systems, on their own these cannot be used to identify tectonic systems. Moreover, as mineral systems are ultimately the products of these same geodynamic drivers, individual mineral deposit types cannot be used to determine tectonic systems, although mineral deposit associations can, in some cases, be indicative of the tectono-metallogenic system.Ore deposits are the products of geological (mineral) systems that operate over a long time frame (hundreds of millions of years) and at scales up to the craton-scale. In essence, mineral systems increase the concentrations of commodities through geochemical and geophysical processes from bulk Earth levels to levels amenable to economic mining. Mineral system components include the geological (tectonic and architectural) setting, the driver(s) of mineralising processes, metal and fluid sources, fluid pathways, depositional trap, and post-depositional modifications. All of these components link back to geodynamic processes and the tectonic system. For example, crustal architecture, which controls the spatial distribution of, and fluid flow, within mineral systems, is largely determined by geodynamic processes and tectonic systems, and the timing of mineralisation, which generally is relatively short (commonly < 1 Myr), correlates with local and/or far-field tectonic events.The geochemical characteristics of many mineral systems are a consequence of their geodynamic and tectonic settings. Settings that are characterised by low heat flow and lack active magmatism produce low temperature fluids that are oxidised, with ore formation caused largely by redox gradients or the provision of external H2S. The characteristics of these fluids are largely governed by the rocks with which they interact, rocks that have extensively interacted with the hydrosphere and atmosphere, both environments that have been strongly oxidised since the great oxidation event in the Paleoproterozoic. In settings characterised by high heat flow and active magmatism, ore fluids tend to be higher temperature and reduced, with deposition caused by cooling, pH neutralisation, depressurisation and fluid mixing. Again, the characteristics of these fluids are governed by rocks with which they interact, in this case more reduced magmatic rocks derived from the mantle or lower crust. 相似文献
4.
This study utilizes three major data sources: distribution of geological units; density, type, age and distribution of mineral deposits; and elemental analyses from regional geochemical stream sediment surveys to define parameters that ‘characterize’ tectonic terranes in northern British Columbia. A similar approach could be applied anywhere in the Canadian Cordillera.This area, NTS map sheets 104N, 104O and 104P along the British Columbia-Yukon border, forms a transect through allochthonous terranes into North American rocks. These are: the allochthonous island-arc Stikine, oceanic Cache Creek, cataclastic Yukon/Tanana, and island-arc Quensel terranes, the pericratonic Dorsey terrane; the parautochthonous oceanic Sylvester allochthon; and the autochthonous miogeoclinal North American Cassiar terrane. Plutonic rocks of Jurassic-Cretaceous to Tertiary age intrude all terranes.Data sources used in the study are geological base maps and reports, the Ministry of Energy Mines and Petroleum Resources' mineral deposit database (MINFILE) and analytical data from the National Regional Geochemical Survey stream sediment and water sampling program.Geological maps were compiled from various sources and plotted to act as bases for geochemical and mineral deposit overlays for analysis and interpretation.Geochemical samples were separated into background and anomalous populations and compared according to their source terranes. We found that mean concentrations from background sample populations for some elements are statistically distinctive for different terranes. Unfortunately, elemental correlation coefficients for the terranes are similar so cannot be used to characterize each terrane.Data on mineral deposits and occurrences were compiled from minfile and other sources. Particular attention was paid to deposits with histories of production or significant reported reserves. Deposits were sorted by type and commodity to produce synoptic metallogenic maps.The combined data from geological, geochemical and mineral deposit databases form a strong tool for interpreting and predicting patterns of mineralization. 相似文献
5.
陆相火山-侵入岩有关的铁多金属矿成矿作用及矿床模型——以长江中下游为例 总被引：26，自引：13，他引：13
在长江中下游地区,与白垩纪陆相火山-侵入岩有关的铁多金属矿床在空间上绝大多数发育于白垩纪火山盆地,仅程潮和金山店出现于隆起区;成矿时间上分为两个时代,即133~130Ma和127~125Ma。按照成矿物质来源和成矿过程,鉴别出4个成矿系统:即在隆起区与石英闪长岩有关的矽卡岩铁矿(系统1);在火山盆地内,与大王山(或砖桥)旋回火山-次火山活动有关的铁多金属矿床(包括,磷灰石-磁铁矿型铁矿、类矽卡岩型铁矿、矿浆型铁矿、热液型硫铜金矿、热液型铅锌矿)(系统2)和与二长-正长岩有关的矽卡岩型铁矿(系统3);与娘娘山(或浮山)旋回火山-次火山活动有关的铜(金)矿和金铀矿(系统4)。盆地内和隆起区的矽卡岩型铁矿形成时间基本一致,略晚于与辉石闪长玢岩有关的铁多金属矿床(系统2), 但早于铜金铀为主的成矿系统4。前人以系统2中的磷灰石-磁铁矿型铁矿、类矽卡岩型铁矿和矿浆型铁矿为主,结合其他一些少见或不具工业意义的铁矿类型,提出一个具有广泛影响的玢岩铁矿成矿模式。此文以玢岩铁矿成矿模式为基础,结合4个成矿系统的基本特点,提出了白垩纪陆相火山-侵入岩有关的铁多金属矿床模型。以上这些具有成因联系的矿床系统和类型及其分带互为找矿标志。 相似文献
6.
Newly synthesized data indicate that the geochemistry of igneous rocks associated with epithermal mineral deposits varies extensively and continuously from subalkaline basaltic to rhyolitic compositions. Trace element and isotopic data for these rocks are consistent with subduction-related magmatism and suggest that the primary source magmas were generated by partial melting of the mantle-wedge above subducting oceanic slabs. Broad geochemical and petrographic diversity of individual igneous rock units associated with epithermal deposits indicate that the associated magmas evolved by open-system processes. Following migration to shallow crustal reservoirs, these magmas evolved by assimilation, recharge, and partial homogenization; these processes contribute to arc magmatism worldwide.Although epithermal deposits with the largest Au and Ag production are associated with felsic to intermediate composition igneous rocks, demonstrable relationships between magmas having any particular composition and epithermal deposit genesis are completely absent because the composition of igneous rock units associated with epithermal deposits ranges from basalt to rhyolite. Consequently, igneous rock compositions do not constitute effective exploration criteria with respect to identification of terranes prospective for epithermal deposit formation. However, the close spatial and temporal association of igneous rocks and epithermal deposits does suggest a mutual genetic relationship. Igneous systems likely contribute heat and some of the fluids and metals involved in epithermal deposit formation. Accordingly, deposit formation requires optimization of source metal contents, appropriate fluid compositions and characteristics, structural features conducive to hydrothermal fluid flow and confinement, and receptive host rocks, but not magmas with special compositional characteristics. 相似文献
7.
The Haenam volcanic field was formed in the southern part of the Korean peninsula by the climactic igneous activity of the Late Cretaceous. The volcanic field hosts more than nine hydrothermal clay deposits and two epithermal Au–Ag deposits. This study focuses on the relationship between hydrothermal clay alteration and epithermal Au–Ag mineralization based on the geology, alteration mineralogy, geochronology, and mineralization characteristics.These clay and epithermal Au–Ag deposits are interpreted to have formed by the same hydrothermal event which produced two distinct types of mineral systems: 1) Au-dominant epithermal Au–Ag deposit and 2) clay-dominant hydrothermal clay deposit. The two types of mineral systems show a close genetic relationship as suggested by their temporal and spatial relationships. The Seongsan hydrothermal system progressively evolved from a low-intermediate sulfidation epithermal system with Au–Ag mineralization and phyllic alteration to an acid–sulfate high-sulfidation system with Au–Ag mineralization and/or barren advanced argillic/argillic alteration. The Seongsan system evolved during post volcanic hydrothermal activity for at least 10 Ma in the Campanian stage of the late Cretaceous.The Seongsan hydrothermal system shows the rare and unique occurrence of superimposed high to low (intermediate) sulfidation episodes, which persisted for about 10 Ma. 相似文献
8.
As geochemical appraisals of mineral regions of commercial prospectivity evolve, the organic matter associated with metal rich ores has attracted greater attention. Petroleum basin and modern seafloor hydrothermal vent studies have suggested that organic matter can have a significant influence on the behaviour of mineralising fluids. There have been many isolated reports of certain organic compositional or morphological (e.g. pyrobitumen) features showing an apparent relationships with hydrothermal fluids or minerals, raising expectations that organic based parameters might be useful to mineral exploration. However, the understanding of organic–inorganic relationships in Earth systems is far from complete. For example, the detailed mechanics of the interaction of organics with hydrothermal fluids over geological time remain largely undefined. Organic geochemistry studies have traditionally involved the measurement and interpretation of the hydrocarbon composition of sedimentary rocks. Here we review the types of aliphatic hydrocarbons, aromatic hydrocarbons and metalloporphyrins often detected from organic geochemical investigations in mineral-rich regions. Such molecular data can be particularly diagnostic of biochemical sources and the palaeo-environments at the time mineral associated organic matter was deposited. Sub-surface trends of hydrocarbon alteration may also reflect major biogeochemical processes such as thermal maturity and biodegradation. Organic geochemistry data can also occasionally provide information about the nature (e.g., origin, composition, temperatures) and migration pathways of hydrothermal fluids and can make a contribution to holistic ore genesis models. The well preserved organic matter associated with the economic “Here's Your Chance” Pb–Zn–Ag Mine (Paleoproterozoic Barney Creek Formation, McArthur Basin, Australia) and the transition metal-rich Early Permian Kupferschiefer Formation (Germany–Poland) have attracted significant attention. A more detailed summary of the organic character of these deposits is provided to highlight the contribution organic geochemistry can make to understanding mineralisation processes. Most organic geochemical studies of highly mineralised regions, however, have not adequately addressed the significance of organic matter to mineralisation. A slightly different analytical focus than traditionally used for exploration appraisal of petroleum hydrocarbons may be required to properly evaluate the significance of organic species to the mobilisation, transport and deposition of ore metals. The characterisation and subsequent thermodynamic modeling of organic substances and complexes within metalliferous hydrothermal systems will contribute to a better understanding of the nature and role of organic–inorganic fluids or other affiliated organics in ore systems. 相似文献
9.
原生矿床中金的主要性状有自然金与金的碲化物，自然金可分为“明金”和“微细粒金”，“明金”的次生作用，使金的成色得到提高，粒度更大，往往有利于残坡积型砂金矿床的形成，“微细粒金”的次生作用，常形成卡林型氧化金矿或红土型金矿和铁帽型金矿，显然，以“明金”为主的矿床及金的重砂异常区，不存在找红土型金矿的可能，应寻找脉金矿床，而在有低值金的重砂异常叠加的化探Au异常区，有望找到中小型红土型金矿床。 相似文献
10.
延边地区是中国东北部陆缘浅成热液金铜矿床发育的地区之一,广泛发育着浅成热液金矿床、中温热液金(铜)矿床和中深成中高温热液富金铜矿床(类斑岩型);富金铜矿床的成矿时代发生在105～102 Ma,为了进一步确定浅成热液金矿床与中深成中高温热液富金铜矿床的成矿动力学背景,采用流体包裹体的~(40)Ar/~(39)Ar激光探针定年法,对该区典型浅成热液金矿床进行了精细的年代学测定,获得刺猬沟金矿床、五星山金矿床和杜荒岭金矿床的脉石矿物石英流体包裹体的~(40)Ar/~(39)Ar等时线年龄分别为(141±7)Ma、(123±7)Ma和(107±6)Ma,其中刺猬沟金矿床((141±7)Ma)和五星山金矿床((123±7)Ma)的脉石矿物石英流体包裹体含有过剩放射性成因~(40)Ar,而杜荒岭金矿床((107±6)Ma)的脉石矿物石英流体包裹体几乎不含或含极少量过剩放射性成因~(40)Ar。结合最新获得的相关地质体的精细年代学成果,认定该区浅成热液金矿床成矿作用均发生在早白垩世晚期,或发生在早白垩世晚期火山喷发、浅成岩浆就位之后,其形成环境与富金铜矿床一致,为古太平洋板块向亚洲大陆正北向俯冲转入Izanagi-Farallon板块西向俯冲的构造转换期。 相似文献
11.
The Crusader Complex, part of the Agnew gold camp of the Lawlers Anticline of the Yilgarn Craton, Western Australia, is located close to or along the contact between the Lawlers Basalt and Agnew Ultramafics units. Au mineralization within the four orebodies that form the Crusader Complex is dominated by very pure Au, containing less than 1 wt.% Ag, with Au variably associated with scheelite, Bi-tellurides and minor chalcopyrite within a magnetite and titanite gangue assemblage. Hydrothermal alteration associated with this style of mineralization is characterized by increasing concentrations of Mo, Be, Li, Sn and Fe and depletions in Na, Cu, Ba, Pb, Mn, Zn, Si, and K relative to protolith concentrations; these enrichments are more typical in orebodies associated with felsic intrusive-related mineralizing systems rather than the more well-known orogenic Au deposits found elsewhere within the Lawlers Anticline (e.g. at Waroonga) and within the greater Yilgarn Craton.We propose that flexures of the contact between the Lawlers Basalt and Agnew Ultramafic units acted as conduits for Au-bearing felsic intrusive-derived fluids and generated structural traps that enhanced fluid flow. The mineralizing fluids that formed the Crusader deposits were derived from the Lawlers granitoid pluton that intruded into the study area. Enhanced fluid flow promoted interaction between hydrothermal fluids and the reactive mafic–ultramafic rock sequence, augmenting the amount of Au that was precipitated during formation of the orebodies at Crusader. The magnetite-dominated quartz- and sulfide-poor intrusion-related mineralization at Crusader contrasts sharply with other late Archean intrusion-related deposits of the Yilgarn Craton that are usually sulfide- and/or quartz-rich. This may in turn suggest that the Crusader deposit represents a new class of under-explored intrusion-derived deposits, possibly opening new mineral exploration opportunities for the Agnew region, and potentially the wider Eastern Goldfields Superterrane. Enrichments in Mo and Sn and significant depletions in Cu suggest that other parts of the Lawlers batholith may also be prospective for base metal mineralization.Integration of stratigraphic interpretation with the identification of key structural fluid pathways and the presence of felsic intrusive bodies, as presented in this study, enables the delineation of the key elements that underlie mineralization at the Crusader Complex. We propose that these key elements provide vital information for future gold exploration models that can be used within other Archean terranes and within the Eastern Yilgarn Craton in particular. 相似文献
12.
区域成矿作用的地球化学研究必须以岩石圈物质分异的观点来认识地壳地元素迁移和演化，必须以大区域地壳体系的地球化学特征来指导局部地区的基础地质认训和找矿问题，这是由于地壳与地幔体系的物质运动是不平衡的，明显具分异特征，为些不同构造单元岩石圈的化学成分是不均一的，这就决定了不同构造单元的成岩，成矿作用具有不同的地球化学特征，本文从东秦岭及领区岩石圈金的丰度特征研究入手，探讨该区不同构造环境中金（银）成太 相似文献
13.
西准噶尔走滑断裂系元素分布特征及其成矿意义 总被引：8，自引：2，他引：6
我国新疆西北部西准噶尔走滑断裂构造体系(简称"西准系")是中亚造山带巴尔喀什马蹄形构造的向东延伸部分,由于中生代成吉思-准噶尔断裂的右行走滑断裂作用而被分成了两个部分。西准系是一个多米诺式的走滑断裂构造体系,主要由达拉布特断裂、玛依勒断裂、巴尔鲁克断裂等三条NE走向的左行走滑断裂及其夹在它们之间的地块所组成,可能是晚古生代与走滑断裂相关的陆条弯曲(褶皱)作用的产物。同时,西准噶尔地区也是重要的晚古生代成矿带,产出有一些大型和超大型的金属矿床,包括包古图斑岩铜矿、哈图金矿、萨尔托海铬铁矿和杨庄铍矿床等。本文分析了西准系走滑断裂构造与元素分布之间的关系。结果显示,西准噶尔成矿带元素与地球化学块体以及铜、金、钼、铬铁矿等矿床的分布,均受晚古生代西准系的形成与演化过程的控制。其中,庙尔沟、红山岩体与金地球化学块体之间的反对称分布特征,说明了花岗岩类侵入体和金元素在达拉布特断裂左行走滑过程中发生了重要的物质调整与迁移作用。庙尔沟岩体的逆时针旋转运动,造成了环状断裂与裂隙系统,以及与之相对应的Cu、Pb等元素风火轮式的分布形式。走滑断裂作用与岩体旋转运动的共同结果,导致了金元素沿断裂和裂隙的迁移与成矿,使得西准地区金矿床在断裂和裂隙中的发育。断裂构造体系与元素地球化学异常之间的关系,可以用来有效指导西准地区未来矿产资源的勘查。 相似文献
14.
《地学前缘(英文版)》2020,11(3):719-738
Concept-based orogenic gold exploration requires a scale-integrated approach using a robust mineral system model.Most genetic hypotheses for orogenic gold deposits that involve near-surface or magmatic-hydrothermal fluids are now negated in terms of a global mineral system model.Plausible models involve metamorphic fluids,but the fluid source has been equivocal.Crustal metamorphic-fluid models are most widely-accepted but there are serious problems for Archean deposits,and numerous Chinese provinces,including Jiaodong,where the only feasible fluid source is sub-crustal.If all orogenic gold deposits define a coherent mineral system,there are only two realistic sources of fluid and gold,based on their syn-mineralization geodynamic settings.These are from devolatilization of a subducted oceanic slab with its overlying gold-bearing sulfide-rich sedimentary package,or release from mantle lithosphere that was metasomatized and fertilized during a subduction event,particularly adjacent to craton margins.In this model,CO_2 is generated during decarbonation and S and ore-related elements released from transformation of pyrite to pyrrhotite at about 500 ℃.This orogenic gold mineral system can be applied to conceptual exploration by first identifying the required settings at geodynamic to deposit scales.Within these settings,it is then possible to define the critical gold mineralization processes in the system:fertility,architecture,and preservation.The geological parameters that define these processes,and the geological,geophysical and geochemical proxies and responses for these critical parameters can then be identified.At the geodynamic to province scales,critical processes include a tectonic thermal engine and deep,effective,fluid plumbing system driven by seismic swarms up lithosphere-scale faults in an oblique-slip regime during uplift late in the orogenic cycle of a convergent margin.At the district to deposit scale,the important processes are fluid focussing into regions of complex structural geometry adjacent to crustal-scale plumbing systems,with gold deposition in trap sites involving complex conjugations of competent and/or reactive rock sequences and structural or lithological fluid caps.Critical indirect responses to defined parameters change from those generated by geophysics to those generated by geochemistry with reduction in scale of the mineral system-driven conceptual exploration. 相似文献
15.
新疆晚古生代大陆边缘成矿系统与成矿区带初步探讨 总被引：15，自引：4，他引：15
新疆地处中亚成矿域的中段，古生代大陆边缘增生明显、构造和岩浆活动强烈、矿产资源丰富。古生代大陆边缘成矿作用主要集中在两个时期，即以阿尔泰南缘为主的早中泥盆世和以天山为主的早石炭世。本文在综合研究及与境外对比的基础上，按照北疆地区晚古生代大陆边缘的构造动力学和成矿特征，将研究区大陆边缘成矿系统划分为：活动大陆边缘海相火山岩-盆地流体成矿系统，活动大陆边缘火山岛弧-岩浆活动成矿系统和被动大陆边缘沉积盆地-热水活动成矿系统三类。同时对形成于大陆边缘的成矿区带进行划分，主要包括：阿勒泰南缘晚古生代活动大陆边缘块状硫化物成矿带；阿尔泰南缘-东准噶尔活动大陆边缘卡拉先格尔岛弧斑岩铜金成矿带；东天山晚古生代活动大陆边缘铜钼锌成矿区带；西准噶尔洋内弧斑岩-浅成低温热液铜金成矿区带；西天山（伊犁地块）活动大陆边缘金铜成矿区带；塔里木板块被动大陆边缘沉积型铅锌成矿带。本文认为大陆增生与成矿作用的关系是矿床学和成矿系统研究的重要内容，成矿区带是成矿系统发生成矿作用的响应，而成矿系统是成矿区带形成的本质。 相似文献
16.
熊耳山—外方山矿集区位于秦岭造山带之华北板块南缘,经历了复杂的碰撞造山过程,成矿时间跨度大,成矿强度高,成矿作用多样。复合造山过程和相应的成矿作用已被深入研究,但成矿系统的划分和叠加成矿作用尚需研究。本文将熊耳山—外方山矿集区发育的Au-Mo矿床划分为造山型Mo矿床、斑岩型Mo矿床、岩浆热液脉型Mo矿床、造山型Au矿床和岩浆热液型Au矿床5个类型,对应5种成矿系统：(1)造山型Mo矿床形成于250~227 Ma的同碰撞环境和227~194 Ma的后碰撞环境,为变质热液萃取壳源Mo成矿;(2)斑岩型Mo矿床形成于163~135 Ma的洋陆俯冲环境和135~116 Ma的岩石圈减薄环境,为岩浆热液携带幔源或壳源Mo成矿;(3)岩浆热液脉型Mo矿床形成于227~194 Ma的后碰撞环境,为岩浆热液携带幔源Mo成矿;(4)造山型Au矿床在三叠纪发生了预富集作用,主要形成于163~135 Ma的洋陆俯冲环境和135~103 Ma的岩石圈减薄环境,为变质热液萃取壳源Au成矿;(5)岩浆热液型Au矿床仅形成于135~103 Ma的岩石圈减薄环境,为岩浆热液携带壳源Au成矿。矿集区主要存在两种叠加成矿作用,即不同构造背景下多种成矿系统的叠加和同一构造背景下不同成矿系统的叠加。 相似文献
17.
近年来通过中国地调局在新疆东天山浅覆盖区开展1∶5万化探示范项目,圈定了一批具找矿价值的铅锌银铜为主成矿元素的化探异常,通过异常查证和矿产评价工作,采用化探、物探、探槽工程揭露、钻探验证等综合技术方法,在阿奇山一带浅覆盖地区相继发现了一批以铅锌银铜为主的矿产地,发现了阿奇山火山沉积-叠加热液交代改造型铅锌矿床、屹立火山热液型富银铅矿(黑矿型)、1288高点铜矿点等十余处。通过矿产资源评价工作,目前确定阿奇山铅锌矿资源量达大型矿床规模。屹立富银铅矿以其品位高、埋藏浅、开采经济价值高为特点。阿奇山地区铅锌矿找矿成果揭示了阿奇山一带浅覆盖区有巨大的找矿潜力。 相似文献
18.
隐伏矿是当前矿产地质勘查的重点对象。在综合研究冀北地区1:20万区域示矿信息基础上,优选出锥子山花岗岩体一带的龙头山为找矿靶区,研究显示其具有较好的找矿潜力。1:5万水系沉积物地球化学测量圈定出11处综合异常;其中H6异常属于矿致异常。H6异常经1:1万地物化测量显示:Ag、Pb、Zn、Au等元素异常值高,具有外带—中带—内带三级分带;同时具有中低阻高极化的激电异常、蚀变矿（化）带与物化探异常相耦合的特征。通过进行系统地不同尺度地物化测量,缩小了找矿靶区,经工程验证发现了龙头山铅多金属矿床。矿体赋存在北西西向延伸、宽30~60 m的龙头山（F3）断裂构造系统中、产状较陡,赋矿围岩为太古界单塔子群（花岗）片麻岩和晚侏罗世张家口组安山岩,矿石多为细脉—浸染状、致密块状构造,矿床特征与毗邻的小扣花营、牛圈等多金属矿床类似,属于中低温热液脉型铅多金属矿床。最后,根据大比例尺地物化示矿信息特征,厘定了热液脉型铅多金属矿床的找矿标志,建立了地物化综合找矿模型,有利于推进冀北地区的找矿勘查。 相似文献
19.
The fact that mineral deposit attributes such as the size frequency of orogenic gold deposits in specific provinces exhibit power law distributions similar to forest fires, earthquakes, and fault size populations, is a compelling motivation to examine their genesis from a systems context. Based on well-studied Earth systems such as climate, the systems related to mineral deposits are likely to be complex and potentially include sensitive dependent components that vary simultaneously and in subtly interconnected ways.Although a “systems approach” was enunciated for mineral exploration by Fyfe and Kerrich as early as 1976, it is yet to be fully embraced by the geosciences community that commonly retain models dependent primarily on deposit-scale characteristics. Orogenic gold deposits are well studied and widely considered to represent a single class of deposit that has formed over much of Earth history in settings ranging from Archean granite-greenstone belts to Phanerozoic turbidite sequences. Accordingly, the deposit type is well suited for assessment within a systems context. If orogenic gold deposits do in fact represent a single class of deposits, then the simplest application of a systems approach highlights the fact that the nature of the host upper crustal succession cannot be a fundamental control, with specific granite suites and pyritic sediments not universal, or at least not essential, components of the system. Furthermore the scale of orogenic gold systems implicates processes capable of tapping sub-crustal source regions.Increasingly, advances in orogenic gold systems, and mineral systems in general, are linked to application of systems science that emphasize importance of system-driven criticality. Orogenic gold systems and other mineral systems are typically short in duration and linked in time and space to tectonic triggers. The latter promote a rapid release of energy (‘avalanches’) that overcome system thresholds and are strong indicators of complex systems that may show power-law behavior.Only a rigorous application of a systems approach can cut through the confusion that arises from conflicting models based on local deposit studies. Only a systems approach can evaluate the significance of rare or anomalous features in a small number of deposits. Truly predictive models for mineral exploration will ultimately be developed by workers who adhere to the systems approach. 相似文献
20.
The role of polymetallic melts in scavenging ore components has recently been highlighted in the context of fluid-poor metamorphosed ore deposits. In contrast, the role of polymetallic melts in systems dominated by hydrothermal fluids remains poorly understood. Using a simple Au-Bi model system, we explored experimentally whether such polymetallic melts can precipitate directly from a hydrothermal fluid, and investigated the ability of these melts to scavenge Au from the solution. The experiments were conducted in custom-built flow-through reactors, designed to reproduce a hydrothermal system where melt components are dissolved at one stage along the flow path (e.g., Bi was dissolved by placing Bi-minerals along the fluid path), whereas melt precipitation was caused further along the flow path by fluid-rock interaction. Bi-rich melts were readily obtained by reaction with pyrrhotite, graphite or amorphous FeS. When Au was added to the system, Bi-Au melts with compositions consistent with the Au-Bi phase diagram were obtained. In the case of fluid reaction with pyrrhotite, epitaxial replacement of pyrrhotite by magnetite was observed, with textures consistent with an interface-coupled dissolution-reprecipitation reaction (ICDRR). In this case, the metallic melt precipitated as blebs that were localized at the replacement front or within the porous magnetite.Direct fractionation of Bi-Au melts from a hydrothermal fluid, or precipitation of a Bi-melt followed by partitioning of Au from ambient fluid, offer new pathways to the enrichment of minor ore components such as Au, without requiring fluid saturation with respect to a Au mineral. This mechanism can explain the strong geochemical affinity recognized between Au and low-melting point chalcophile elements such as Bi in many gold deposits. Examples of deposits where such a model may be applicable include orogenic gold deposits and gold skarns. Contrary to models involving migration of polymetallic melts to explain element remobilization, only small quantities (ppm) of polymetallic melts are required to affect the Au endowment of a deposit via interaction with a hydrothermal fluid. The experiments also show that micro-environments can play a critical role in controlling melt occurrences. For example, reaction fronts developing via ICDR reactions can promote melt formation as observed during the replacement of pyrrhotite by magnetite. The associated transient porosity creates space for the melt and promotes melt-fluid exchanges whereas the reaction front provides local geochemical conditions favorable to melt precipitation (e.g., reduced, low aH2S(aq), and catalytic surface). 相似文献