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1.
北祁连山火山成因块状硫化物矿床的金属来源研究   总被引:2,自引:0,他引:2  
研究了北祁连山造山带火山成因块状硫化物矿床(VMS)类型、金属来源与容矿围岩、火山岩类型及其构造环境的关系。结果表明,容矿岩石和地壳性质是控制矿床类型和金属来源的主要因素。多金属黑矿型矿床主要赋存于硅名质陆壳边缘裂陷带双峰火山岩系的酸性火山岩中,成矿元素源于深部长英质岩石,铜型矿床产于洋壳基性火山岩中,成矿元素源于深部镁铁质岩石。中寒武统双峰火山岩所赋存的多金属VMS矿床多、规模大,是主要含矿矿岩  相似文献   

2.
新疆昆仑式火山岩型块状硫化物铜矿床及成矿地质环境   总被引:7,自引:0,他引:7  
新疆西昆仑奥依塔克-恰尔隆拗陷带内阿克塔什-萨落依成矿带发现多处火山岩型块状硫化物铜矿床。这些矿床产在石炭系双峰式火山岩系之内,沿着下石炭统基性火山岩和上石炭统酸性火山岩两个层位产出,分别以玄武岩和流纹岩为容矿主岩,可以明显地分成基性火山岩型和酸性火山岩型两种类型。矿石主成矿元素均以铜为主,含少量的锌,几乎不含铅,矿床类型属于铜型。这些基性火山岩型和酸性火山岩型矿床被统称为昆仑式火山岩型块状硫化物铜矿床。根据矿床产出地质环境、双峰式火山岩系、沉积建造以及火山岩地球化学特征,推断昆仑式火山岩型块状硫化物铜矿床最可能形成于泥盆纪-石炭纪弧后拉张构造环境。  相似文献   

3.
冯京  徐仕琪 《新疆地质》2012,30(4):418-424
通过新疆矿产资源潜力评价工作,对新疆阿舍勒海相火山岩型铜锌矿成矿环境、特征、成因、成矿规律及控矿要素进行总结,认为该矿床是产于阿舍勒拉张裂谷中心带、与早—中泥盆世火山岩有关的块状硫化物矿床,且严格受双峰式火山岩建造控制。基性火山岩与酸性火山岩接触界面是寻找此类矿床重要地质标志。高重力、低电阻和强铜、锌、银元素异常组合的出现是定位矿体的有效信息。重力+TEM+岩石化探是寻找此类矿床的最佳技术组合。  相似文献   

4.
论梅仙块状硫化物矿床的特征及成矿地质环境   总被引:21,自引:2,他引:19  
周兵  顾连兴 《矿床地质》1999,18(2):99-109
梅仙铅锌矿床产于双峰式火山岩系内,火山岩的岩石化学,稀土和微量元素特征的研究表明其形成于大陆裂谷环境中,闽中裂谷带的发生,发展和演化控制着梅仙矿床的成矿过程。梅仙铅锌矿床特征的研究揭示其是裂谷火山活动有关的块状硫化物矿床,并经后期热液叠加改造。  相似文献   

5.
认为块状硫化物矿床在成因方面实际上是多种多样的,与成矿有关的火山常常是双峰式火山岩组合,它们可能来自于不同的岩浆源区而与岩浆分异作用没有必然的联系。  相似文献   

6.
新疆阿舍勒铜锌块状硫化物矿床成矿条件和成矿特点   总被引:3,自引:0,他引:3  
阿舍勒铜锌矿床是一个典型的火山岩型块状硫化物矿床。大陆边缘裂谷带是矿床形成的大地构造环境。早中泥盆世火山活动形成了含矿的双峰式火山岩套。矿床产于近喷发间歇期的石英角斑质角砾凝灰岩中,受火山洼地和同生断裂控制。  相似文献   

7.
“红透山式”块状硫化物铜锌矿床的成矿作用主要出现在三个较大的火山喷发-沉积旋迴中,双峰式火山岩构成了“红透山式”矿床的含矿岩系。呈透镜状、扁豆状的火山碎屑岩的发现为研究该类矿床提供了较为直观的地质依据。稀散元素和硫同位素特征亦表明该类矿床为古火山机构控制的海底火山喷发-沉积矿床。总结归纳了火山作用与成矿的关系。  相似文献   

8.
作者在对我国十多产于长英质火山岩中的块状硫化物矿床进行大量工作的基础上,综合国内外有关矿产资料,对该类矿床产出的区域地质,火山地质,火山岩石学与岩石化学,矿化等成矿地质特征和控矿标志作了系统的总结和阐述。  相似文献   

9.
嘎衣穷矿床是四川"三江"地区的一个典型火山成因块状硫化物矿床,产于"三江"义敦岛弧系德格-乡城主弧带中.矿床形成受主弧带中晚三叠世赠科裂谷盆地控制,盆地中发育典型的裂谷型"双峰式"火山岩组合序列,嘎衣穷多金属矿(化)体主要产于"双峰式"火山岩组合序列的酸性端元组分中,具有块状硫化物矿床的地质特征.岩石地球化学研究表明矿区内勉戈组火山岩属铝过饱和类型,具有岛弧火山岩的特征,呈现多旋回、多期次喷发的特征,在喷发间隙期均伴有多金属矿化,形成嘎衣穷多金属矿(化)体.文章在总结矿床的地质特征其础上,建立了嘎衣穷矿床的找矿模型.  相似文献   

10.
东秦岭二郎坪群蛇绿岩中的火山成因块状硫化物矿床   总被引:2,自引:0,他引:2  
二郎坪群蛇绿岩中多金属矿床属火山成因块状硫化物矿床。加里东期火山作用早期形成铁(铜)矿层、中晚期随着酸性火山岩的增多和火山爆发作用的加强,形成火山成因块状硫化物矿床和黄铁矿化层。矿床具有距火山喷发中心远近不同的分带性和厚层基性熔岩成铁(铜)矿、酸性火山岩赋存铜-锌型或铅-铜型矿的成矿专属性。后者伴有金银矿化。  相似文献   

11.
The superlarge continental volcanic rock-type uranium deposits,which were discovered abroad long ago,have not ye been reported up to now in China.This is an important problem that needs to be urgently solved by uranium geologists at present.In this paper,on the basis of analyzing the metallogenic settings and geological conditions of the superlarge continental volcanic rock-type uranium deposits discovered in the world along with the metallogenic characteristics of those of the same type in China,the space-time distribution patterns of continental volcanics and the metallogenic potential of main tectono-volcanic belts in China are discussed,and a synthetic conclusion has been drawn that there is a possibility to discover the superlarge continental volcanic rock-type uranium deposits in China.Moreover,it is evidenced that the Ganhang,Nanling,Yanliao,Da Hinggan Ling and other tectono-volcanic belts possess favorable geological conditions for the formation of ssuperlarge ore deposits of the continental volcanic rock type.The intersecting and overlapping locations of the aforementioned main belts with other tectono-volcanic(-intrusive)belts are the most potential areas where the superlarge continental volcanic rock-type uranium deposits would be found.  相似文献   

12.
块状硫化物矿床成矿构造环境研究进展   总被引:2,自引:0,他引:2  
对VHMS型、SEDEX型和VSHMS型3种块状硫化物矿床近年来成矿构造环境研究进展进行了较全面的回顾.其中,VHMS型块状硫化物矿床重点对弧间裂谷及弧后盆地构造环境下矿床时空演化及分布规律、古代VHMS型块状硫化物矿床全球对比认识及沟-弧-盆体系下现代海底块状硫化物研究热点地区的岩石类型、组合及岩浆演化规律进行了总结;SEDEX型块状硫化物矿床重点对澳大利亚北部元古代SEDEX型块状硫化物矿床集中区近年来成矿动力学背景研究进展进行了介绍.指出该区巨大的SEDEX型矿床成矿构造环境不是以往认为的被动大陆边缘裂谷,而是汇聚板块地球动力学背景之下远离弧后的大陆拉张盆地.尤其值得关注的是不仅元古界SEDEX型矿床如此,而且那些古生代的典型SEDEX型矿床(如沙利文,红狗矿床)同样被认为具有相同的产出构造背景.同时认为此种构造背景形成的SEDEX型矿床具有更大的找矿价值;VSHMS型矿床是近十年来逐渐得到重视的一类块状硫化物矿床,矿化特征及成矿作用与以上两类矿床相似,但其成矿构造环境应当位于上述两类矿床的过渡部位,对构造环境判断具有重要的指示意义.因此,在汇聚板块动力学背景下,上述3种块状硫化物矿床,自板块边缘岛弧一侧向远离板块边缘的大陆内部,构成了一个很好的矿床分带或成矿序列,即从VHMS型→VSHMS型→SEDEX型.   相似文献   

13.
根据地质和同位素地球化学特征,建立了铜陵地区赋存于石炭系地层底部的块状硫化物矿床的成因模型;该类型矿床的形成主要与石炭纪海底热水活动有关,属喷流-沉积型(SEDEX)块状硫化物矿床;下伏古生代地层是重要的成矿金属源区,海水硫酸盐是硫化物成矿的主要硫源。成矿热流体循环的动力学数值模拟揭示。该类型矿床底盘岩石中的流体活动和热影响范围主要局限在主排泄通道两侧较小的区域内;温度场和流场决定以沉积岩为容矿岩石的喷流.沉积型块状硫化物矿床底盘岩石中的蚀变和矿化强度不如以火山岩为容矿岩石的块状硫化物矿床。伴随强大深部热流的张性同生断裂是控制喷流一沉积型块状硫化物矿床形成与分布的关键因素。海西期扬子板块北缘的张性构造体制为该时期喷流一沉积型块状硫化物矿床的形成提供了有利的地球动力学环境。  相似文献   

14.
The volcanic-hosted massive sulphide (VHMS) deposits in the Eastern Desert of Egypt (e.g., Um Saki deposit) are associated with Precambrian coarse acid pyroclastic rocks. The upper contacts of the massive sulphide body are sharp and well-defined; while the keel zone to the mineralization is always associated with pervasive alteration, characterized by the presence of septechlorite and talc, associated with variable amounts of carbonate and tremolite. On the other hand, the economic talc deposits in Egypt are hosted intensively altered volcanic rocks. Besides talc, chlorite, carbonates and tremolite that occur in variable amounts in these deposits, anomalously high concentrations of gold are also present.The present study showed that alterations in the talc deposits of Darhib, El Atshan, Abu Gurdi, Egat, Um Selimat and Nikhira are similar to those occurring in the keel zone underlying the VHMS of Um Samuki and that the chemical modifications due to alteration processes (additions of Mg, Fe, Mn and Ca coupled with depletions in silica, alkalies, alumina and titanium) are comparable, even the host rocks are different, thus reflecting a genetic relationship. It is suggested that, the examined localities of talc deposits are hosted in the intensively altered volcanics in the keel zones of volcanogenic massive sulphide deposits. Recently, detailed geophysical prospecting program, including electric (resistivity, self-potential and induced polarization), electromagnetic and magnetic methods, was carried out at Darhib, Abu Gurdi and Um Selimat talc deposits. The quantitative interpretation of these geophysical measurements revealed the presence of subsurface bodies of sulphides. The present distribution of talc and allied minerals in Darhib, El Atshan, Abu Gurdi, Egat, Um Selimat and Nikhira could be explained by a tectonic process in which the coarse acid pyroclastic rocks with massive sulphides have tilted in such way that the footwall rock alterations (talc and allied minerals) are exposed on the present-day surface at these localities. Structural studies are currently under way in an attempt to explain the deformation regime that led to the present situation of talc deposits.Two distinct spatial and mineralogical associations of gold mineralization could be identified in the volcanogenic massive sulphide deposits and their footwall alterations (the keel zone) in the Eastern Desert of Egypt. These are (1) gold–silver–zinc association, and (2) gold–copper association. In the former, gold grades are very low and silver is anomalous. This association occurs typically in the upper levels of the VHMS deposit where low-temperature sulphides are abundant. Gold was deposited because of the mixing between the ascending hot solutions and the sulphate-rich seawater. The upper levels of Um Samuki sulphide body represent this association. Gold–copper association, on the other hand, typically occurs in the footwall altered rocks (the keel zone) and the lowest parts of the massive sulphide body. Gold grades reach up to 5.54 ppm, but the average is 1 ppm. Silver is very low, usually in the range of 4–10 ppm. Lead usually, but not always, accompanies gold in this association. Deposition of gold probably took place due to decreasing of temperature and/or increasing pH of the ascending hot brines. The keel zones at Darhib, Abu Gurdi, El Atshan, Um Selimat, Nikhira and Egat talc mines better represent this association.  相似文献   

15.
Volcanic‐hosted massive sulfide (VHMS) deposits of the eastern Lachlan Fold Belt of New South Wales represent a VHMS district of major importance. Despite the metallogenic importance of this terrane, few data have been published for sulfur isotope distribution in the deposits, with the exception of previously published studies on Captains Flat and Woodlawn (Captains Flat‐Goulburn Trough) and Sunny Corner (Hill End Trough). Here is presented 105 new sulfur isotope analyses and collation of a further 92 analyses from unpublished sources on an additional 12 of the VHMS systems in the Hill End Trough. Measured δ34S values range from ‐7.4% to 38.3%, mainly for massive and stockwork mineralisation. Sulfur isotope signatures for polymetallic sulfide mineralisation from the Lewis Ponds, Mt Bulga, Belara and Accost deposits (group 1) are all very similar and vary from ‐1.7% to 5.9%. Ore‐forming fluids for these deposits were likely to have been reducing, with sulfur derived largely from a magmatic source, either as a direct magmatic contribution accompanying felsic volcanism or indirectly through dissolution and recycling of rock sulfide in host volcanic sequences. Sulfur isotope signatures for sulfide mineralisation from the Calula, Commonwealth, Cordillera and Kempfield deposits, Peelwood mine and Sunny Corner (group 2) are similar and have average δ34S values ranging from 5.4% to 8.1%. These deposits appear to have formed from ore fluids that were more oxidising than group 1 deposits, representing a mixed contribution of sulfur derived from partial reduction of seawater sulfate, in addition to sulfur from other sources. The δ34S values for massive sulfides from the John Fardy deposit are the highest in the present study and have a range of 11.9–14.5%, suggesting a greater component of sulfur of seawater origin compared to other VHMS deposits in the Hill End Trough. For barite the sulfur isotope composition for samples from the Commonwealth, Stringers and Kempfield deposits ranges from 12.6% to 38.3%. More than 75% of barite samples have a sulfur isotope composition between 23.4 and 30.6%, close to the previously published estimates of the composition of seawater sulfate during Late Silurian to earliest Devonian times, providing supporting evidence that these deposits formed concurrently with the Late Silurian volcanic event. Sulfur isotope distribution appears to be independent of the host rock unit, although there appears to be a relation linking the sulfur isotope composition of different deposits to defined centres of felsic volcanism. The Mt Bulga, Lewis Ponds and Accost systems are close to coherent felsic volcanic rocks and/or intrusions and have sulfur isotope signatures with a stronger magmatic affinity than group 2 deposits. By contrast, group 2 deposits (including John Fardy) are characterised by 34S‐enrichment and a lesser magmatic signature, are generally confined to clastic units and reworked volcanogenic sediments with lesser coherent volcanics in the local stratigraphy, and are interpreted to have formed distal from the magmatic source. An exception is the Belara deposit, which is hosted by reworked felsic volcanic rocks and has a more pronounced magmatic sulfur isotope signature.  相似文献   

16.
四川呷村V HMS矿床:从野外观察到成矿模型   总被引:22,自引:11,他引:11  
呷村矿床是一个与晚三叠世海相钙碱性酸性火山岩系有关的典型块状硫化物(VHMS)矿床。热水流体系统和贱金属成矿作用发育于义敦岛弧碰撞造山带上的弧间裂谷盆地内,并受其内部的一系列局限盆地及SN向基底断裂-裂缝系统控制。含矿岩系为双峰岩石组合,具火山碎屑岩-矿体-喷气岩“三位一体”特征。硫化物矿床具有“块状矿席+层控网脉状矿带”式三维结构特征。块状矿席发育多旋回的硫化物-硫酸盐韵律型式,揭示热水流体在海底的幕式排泄以及硫化物-硫酸盐在卤水池内的韵律式化学淀积和滑塌堆积过程。层控网脉状矿带产出于流纹质火山岩系,与上覆的块状矿席平行展布,揭示高渗透性碎屑岩层和多条同级别断层或断裂共同约束海底下部热水流体,并诱导其“弥散式”排泄和侧向流动交代。热水流体的传导冷凝过程导致硫化物沉积、热水流体与冷海水的简单混合导致硅质岩或/重晶石淀积,传导冷凝与海水混合的联合作用导致含硫化物重晶石、硅质岩和红碧玉形成。  相似文献   

17.
拉布拉多是加拿大大西洋成矿域中具地质多样性的最大的成矿省,区域成矿地质条件优越,产有Superior型含铁建造、岩浆硫化物、铂族元素、火山成因块状硫化物、铀、稀有稀土等多种金属矿床。文章介绍了拉布拉多铁、铀、稀有稀土、镍多金属等优势金属矿床的成矿背景、成矿特征、矿床(点)分布、典型矿床地质特征及最新勘探成果,分析了区域地质演化作用与区域内主要金属矿床的时空分布。  相似文献   

18.
涂光炽 《矿床地质》2002,21(2):97-105
文章回顾了斑岩铜矿,铜镍硫化物矿床,暗色岩及有关矿床,以沉积岩为容矿岩石的MVT型及SEDEX型铅锌矿床和金刚石矿床等在地质背景,类型拓展,成因机制和找矿前景等方面的研究进展与认识。  相似文献   

19.
近年来对金沙江造山带区域地质、矿床地质和岩石地球化学新资料的研究和典型火山成因块状硫化物(VHMS)矿床的解剖,金沙江造山带的VHMS成矿作用主要发生于早二叠世晚期—晚二叠世海相弧火山岩和晚三叠世裂谷盆地海相火山岩中,构成西南三江地区一条重要的多金属块状硫化物成矿带。成矿带内晚三叠世碰撞后地壳伸展背景下形成的上叠裂谷盆地是其VHMS成矿作用的主体,盆地中火山活动从早期的双峰式火山岩演变为晚期的中酸性火山岩,岩石地球化学特征与孤火山岩有明显的区别,反映其形成于伸展背景。伸展盆地的早期阶段,在双峰火山岩组合的高钾流纹质火山岩系中产出鲁春式VHMS矿床,具有Zn-Cu-Pb-Ag金属组合特征,形成于深水环境;伸展盆地的晚期阶段,在中酸性火山岩系与上覆碳酸盐岩接触带中产出赵卡隆式VHMS矿床,具有Ag-Fe-Pb-Zn金属组合特征,形成于浅水环境;盆地的末期阶段,在滨浅海相磨拉石碎屑岩中产出里仁卡式石膏矿床。金沙江造山带碰撞后地壳伸展背景下VHMS成矿作用的研究,对于造山带中的找矿工作具有重要的指导意义。  相似文献   

20.
火山岩型金矿的地质特征及勘查准则   总被引:5,自引:5,他引:0  
通过对全球典型的巨型火山岩型金矿的研究分析,总结了火山岩型金矿的地质特征:这类金矿产出的大的构造背景多为活动的大陆边缘和岛弧,其成矿时代主要集中在中生代—新生代,容矿岩石主要为第三纪钙碱性喷出岩和浅成侵入岩,容矿构造主要为火山中心、破火山口、火山颈、角砾岩筒、火山穹窿、火山背斜、破碎带、张性裂隙带等各种构造,矿化特点为金和银共生在同一矿床,往往呈自然金或银金矿出现,有些矿床中含碲较多,矿化深度浅,上部为金和银,下部往往变成锌和铅。火山岩型金矿床与地热和温泉的活动密切相关,其围岩蚀变为绢云母化、硅化、碳酸岩化、泥化、黄铁矿化和钾化发育,原生晕分带总的趋势为Hg Sb As Ag Au(Mo、Pb、W)。提出了勘查火山岩型金矿床的选靶准则,指出中国东部地区基底具有前寒武纪矿源层的火山岩断陷盆地周边、深大断裂带上的幔源火山岩区或某些洋壳重熔形成的火山岩区找金潜力较大,尤其是中国西部的东、西准噶尔、西天山、东天山、北天山、新疆南天山、松潘—甘孜和"三江"构造 成矿带的东缘是找金最有潜力的地区。  相似文献   

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