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1.
现代海底热液活动与块状硫化物矿床成因研究进展 总被引：8，自引：0，他引：8
现代海底热液活动的发现及对其分布特征和成矿机理的研究是近年来海洋地质学和矿床地质学的一大进展。对现代海底金属硫化物成矿作用的研究大大推动和促进了对古代块状硫化物矿床成因的认识。有关研究成果综合分析表明：(1)深部热液对流循环系统是块状硫化物成矿的核心，对流循环模式有简单的热液对流模式和双扩散对流模式。(2)块状硫化物矿床集中分布在大洋中张裂性活动板块边界，与大地构造活动紧密联系。(3)成矿流体与成矿物质均有多源性，在强调海水循环淋滤的同时，通过应用新的方法技术，岩浆来源物质(流体及成矿金属等)对一些块状硫化物矿床成矿的直接贡献得到初步确认。(4)在高温热液活动区及金属硫化物沉积中发现大量生命活动和生物群体，意义重大。 相似文献
2.
火山成因块状硫化物矿床研究进展 总被引：3，自引：0，他引：3
火山成因块状硫化物（VMS）矿床可形成于太古宙至现代各个地质时期.现代海底热液成矿作用是赋存于海相火山岩系中的古代VMS矿床成矿作用的再现.VMS矿床可形成于多种构造环境,但均与拉张背景有关.按照构造环境和容矿岩系将VMS矿床分为黑矿型、塞浦路斯型、别子型和沙利文型.VMS矿床的热液蚀变由下盘蚀变带和上盘蚀变带两个结构单元组成.下盘蚀变一般有两种类型：（1）不整合的蚀变岩筒,直接产在块状硫化物带的下方;（2）半整合或层控的上盘蚀变带,并可以在区域范围内展布.与下盘蚀变类似,上盘蚀变也具有蚀变岩筒和半整合的蚀变带两种类型.成矿金属主要有两种可能的来源：（1）在岩浆侵入体和浅位岩浆房之上被加热的循环海水对含矿火山岩系及下伏基底物质的淋滤;（2）深部岩浆房挥发分通过释气作用直接释放.下渗的海水是成矿流体的主要来源,同时流体包裹体和稳定同位素资料显示岩浆流体对成矿流体系统亦有较大贡献.VMS矿床具有明显的金属分带现象,其金属序列组合从下至上依次为Fe→Fe-Cu→Cu-Pb-Zn→Pb-Zn-Ba,这种金属分带的演化反应了流体的演化和块状硫化物丘的生长机制.根据成矿流体温度变化而不断演化的4阶段成矿模式可以很好的解释经典丘堆式矿床的形成过程. 相似文献
3.
洋中脊超基性岩热液成矿系统通常与洋底核杂岩构造有关,多发育大型矿床,具有巨大的资源前景。然而,受大洋调查取样手段的限制,超基性岩蛇纹岩化对成矿的影响仍需进一步研究。德尔尼铜矿床是地质历史上该类矿床的典型案例,对于理解其成矿模式,以及大洋硫化物勘探具有指导意义。本文选取德尔尼铜矿床块状硫化物样品进行黄铁矿的S同位素分析,结果表明其δ34S值主要分布在-0.4‰～+6.3‰。结合前人研究发现,形成于深部网脉状、条带状矿石中的δ34S值为负值,而经历表层喷流和破碎作用的块状和角砾状矿石中的δ34S值为正值,二者呈对称分布,这主要是由于还原条件下岩浆排气产生的SO_2和H_2S动态平衡并逐渐沉淀S2-,表明蛇纹岩化提供的还原环境对热液系统演化产生了重要影响。然而,磁黄铁矿和矿床Ni的分布指示成矿物质中超基性岩的贡献较小,主要物质来源是洋中脊深部的基性岩浆,通过热液循环将物质运移至海底并喷流成矿。对比现今超基性岩赋矿的高温热液硫化物矿床,德尔尼铜矿床形成温度更低,代表了超基性岩赋矿热液硫化物中的中温端元,表明在距离拆离面一定距离(约2～4km)的位置也可能形成大型的热液硫化物矿床,这对于现今洋中脊热液硫化物勘探具有一定的指导意义。 相似文献
4.
李文渊 《西安地质学院学报》2010,(1):15-23
从现代块状硫化物矿床成矿特征对比角度,总结分析了世界现代海底喷流的块状硫化物成矿堆积,综述了现代海底块状硫化物成矿主要形成于洋壳和岛弧环境的实际观察结果,突出强调了洋壳环境和岛弧或陆壳环境两种成矿环境对成矿类型分类的意义。对上地幔部分熔融岩浆来源与地壳物质可能带人、火山喷发岩浆系列的演化和对热液成矿作用的控制进行了讨论,对比分析了岩浆流体对成矿的重要贡献和控制作用,以及成矿热液循环体系形成的条件和模式。 相似文献
5.
洋中脊热液系统是将相对富集在深部的Os运移到海底表面的重要媒介,同时该过程也是全球Os循环的重要组成部分.在归纳总结洋中脊热液系统各物源组分和产物中Os的化学形态、含量及其同位素组成特征的基础上,探讨了Os在洋中脊热液活动各阶段中的分布演化规律及物源贡献特征.在缺乏沉积物覆盖的洋中脊区域,热液系统中的Os及其同位素组成特征主要受控于海水和不同构造环境下洋壳组分特征的差异以及这两种物源组分混合比例的不同.经历了海底之下的水岩反应后,围岩会将下渗海水中的部分放射性成因Os固定,而将自身富集的非放射性成因Os释放进入热液流体中.堆积在海底之上的各种热液产物中的Os大多来自海水,而海底之下的热液产物则因为海水下渗深度以及海水与热液流体混合程度的差异而体现出宽泛的Os含量和187Os/188Os比值变化范围. 相似文献
6.
现代海底热液成矿作用研究现状及发展方向 总被引：15，自引：0，他引：15
现代海底热水成矿作用研究的重大进展表现在两个方面：（１）大批活动的和窒息的热液活动区和硫化物矿床在洋脊、岛弧、弧后盆地及板内火山活动中心等海底环境相继发现。在沉积物饥饿洋脊，矿床规模较小，Ｃｕ－Ｚｎ为主，沉积物覆盖洋脊，矿床规模巨大，Ｐｂ－Ｚｎ为主。弧后扩张或弧间裂陷盆地，形成Ｐｂ－Ｚｎ→Ｚｎ－Ｐｂ－Ｃｕ→Ｃｕ－Ｚｎ矿床谱系。岛弧环境硫化物矿床不具规模，板内火山活动中心以氧化物－硫化物矿化为特色。（２）现代海底热水成矿作用观察和研究为古代ＶＭＳ矿床成因研究提供了重要信息，对现有成矿理论产生重要影响。现代成矿观念强调：①海底成矿作用虽可产生于不同环境，但均与张裂断陷事件密切相关。矿床规模和分布特点受张裂速率制约；②成矿物质主体来源于热水循环的火山－沉积岩和下伏基底物质；③硫化物堆积发生于丘堤－烟囱联合构成的机构和结壳下部，通过开放空间的硫化物充填和先成矿石淋滤迁移来实现。④热液流体呈双扩散对流循环。现代海底热水成矿作用的未来研究方向可概括为强度方向和广度方向。广度研究将加大力度去发现新的矿床，强度研究将采用地球物理方法并配以必要的钻探，深入揭示矿床的三维结构和热液体系及成矿机制。 相似文献
7.
海底多金属硫化物矿床的主要特征 总被引：2，自引：0，他引：2
海底多金属硫化物由于含有贵金属而具有潜在的经济价值并,受到国际地质学家们的广泛关注。已经发现的矿点和矿床有一百多处,然而规模比较大的不足20处。相对于锰结核,多金属硫化物在海底产出的部位较浅,矿石中含有Cu、Zn、Ag和Au等,具有很高的经济价值。据粗略估计,已发现的大型矿床共含有一百万到五百万吨的块状硫化物。世界海底多金属硫化物矿床主要分布在东太平洋海隆、西太平洋构造活动带、西南太平洋以及大西洋中部的大洋中脊。海底多金属硫化物属于海底热液烟囱物,它是热液活动的产物,其成因机制涉及构造和岩浆活动与热液活动的关系,海水及水深以及沉积物与热液成矿的关系,岩水反应,热液地球化学,生物活动等。 相似文献
8.
现代海底多金属硫化物矿床 总被引：5，自引：0，他引：5
海底多金属硫化物矿床是热液活动的产物,主要分布在东太平洋海隆、西太平洋构造活动带、西南太平洋以大西洋中脊,其产出构造背景为洋中脊、弧后扩张中心及地幔热点处。该文系统地总结了现代海底多金属硫化物矿床产出的地质背景特点,对各地质环境中矿化的规律进行对比,并对其形成机制等热点问题作了概述,详细介绍了矿床成因方面的新进展,着重阐述了海底多金属矿床的双扩散对流模式。 相似文献
9.
《吉林地质》2017,(1)
海底热液成矿是近年来地质学家关注的热点问题。现代海底热液成矿作用的研究推动了古块状硫化物矿床成矿过程的认识。结合现今研究成果综合分析表明:海底热液成矿作用主要分布在张性活动板块边界,与大地构造活动紧密相连;成矿金属物质来源具有多元性,金属矿化的类型受基底类型(洋壳-陆壳)和岩性组合(基性岩石-中酸性岩石)的控制,岩浆来源的物质也可能对一些块状硫化物矿床有贡献;主导海底热液成矿作用的核心为对流热循环系统,对流循环具有单循环和双扩散对流模式;海底块状硫化物的堆积过程是烟囱的生长、倒塌堆积和热液流体充填与交代的过程,成矿热液流体的温度和密度在这个过程中起关键作用。基于海底热水矿床的重要性,建立完整的热水喷流成矿理论意义重大。 相似文献
10.
现代海底热液活动往往与岩浆作用相伴生.传统的热液系统循环模式认为:海水沿裂隙（通道）下渗,被加热并与围岩发生水岩反应,萃取岩石中的金属元素,形成热液流体并上涌喷出海底,沉积生成多金属硫化物矿体.这一模式合理地解释了构成现代海底热液系统的3个基本要素:流体、通道和热源,与我们现今条件下所观察到的许多事实相吻合.然而,基岩渗透率、热液流体性质、热液生态系统和热液产物上的差异表明现代海底热液活动系统可能存在另一种注入式循环模式,即热液流体来自深部岩浆房流体和挥发性组分的直接注入.据此提出现代海底热液活动系统可能存在两种模式:一种是浅层循环模式,即传统的热液循环模式;另一种是岩浆后期热液注入模式（简称"注入模式"）.在岩浆作用强烈和构造裂隙发育的环境中,两种模式可能同时存在,形成双扩散对流循环模式.双扩散对流循环模式可以很好地解释现代海底热液活动研究中近期所发现的多种现象和事实.对弧后盆地而言,在研究其岩浆作用与热液活动时,还要考虑板块俯冲的构造背景和俯冲组分及陆壳组分加入等因素,同时构建了适用于弧后盆地海底热液活动系统的理论模型. 相似文献
11.
Lawrence M. Cathles 《Mineralium Deposita》2011,46(5-6):639-657
Episodic seafloor spreading, ridge topography, and fault movement at ridges find (more extreme) analogs in the arc and back-arc setting where the volcanogenic massive sulfide (VMS) deposits that we mine today were formed. The factors affecting sulfide accumulation efficiency and the extent to which sulfides are concentrated spatially are the same in both settings, however. The processes occurring at mid-ocean ridges therefore provide a useful insight into those producing VMS deposits in arcs and back-arcs. The critical observation investigated here is that all the heat introduced by seafloor spreading at mid-ocean ridges is carried out of the crust within a few hundred meters of the ridge axis by ??350°C hydrothermal fluids. The high-temperature ridge hydrothermal systems are tied to the presence of magma at the ridge axis and greatly reduce the size and control the shape of axial magma intrusions. The amount of heat introduced to each square kilometer of ocean crust during its formation can be calculated, and its removal by high-temperature convection allows calculation of the total base metal endowment of the ocean basins. Using reasonable metal deposition efficiencies, we conclude that the ocean floor is a giant VMS district with metal resources >600 times the total known VMS reserves on land and a copper resource which would last >6,000?years at current production rates. 相似文献
12.
Stephen J. Piercey 《Mineralium Deposita》2011,46(5-6):449-471
Throughout Earth??s history, all volcanogenic massive sulfide (VMS)-hosting environments are associated with specific assemblages of mafic and felsic rocks with distinct petrochemistry (petrochemical assemblages) indicative of formation at anomalously high temperatures within extensional geodynamic environments. In mafic-dominated (juvenile/ophiolitic) VMS environments, there is a preferential association with mafic rocks with boninite and low-Ti tholeiite, mid-ocean ridge basalt (MORB), and/or back-arc basin basalt affinities representing forearc rifting or back-arc initiation, mid-ocean ridges or back-arc basin spreading, or back-arc basins, respectively. Felsic rocks in juvenile oceanic arc environments in Archean terrains are high field strength element (HFSE) and rare earth element (REE) enriched. In post-Archean juvenile oceanic arc terrains, felsic rocks are commonly HFSE and REE depleted and have boninite like to tholeiitic signatures. In VMS environments that are associated with continental crust (i.e., continental arc and back-arc) and dominated by felsic volcanic and/or sedimentary rocks (evolved environments), felsic rocks are the dominant hosts to mineralization and are generally HFSE and REE enriched with calc-alkalic, A-type, and/or peralkalic affinities, representing continental arc rifts, continental back-arcs, and continental back-arcs to continental rifts, respectively. Coeval mafic rocks in evolved environments have alkalic (within-plate/ocean island basalt like) and MORB signatures that represent arc to back-arc rift versus back-arc spreading, respectively. The high-temperature magmatic activity in VMS environments is directly related to the upwelling of mafic magma beneath rifts in extensional geodynamic environments (e.g., mid-ocean ridges, back-arc basins, and intra-arc rifts). Underplated basaltic magma provides the heat required to drive hydrothermal circulation. Extensional geodynamic activity also provides accommodation space at the base of the lithosphere that allows for the underplated basalt to drive hydrothermal circulation and induce crustal melting, the latter leading to the formation of VMS-associated rhyolites in felsic-dominated and bimodal VMS environments. Rifts also provide extensional faults and the permeability and porosity required for recharge and discharge of VMS-related hydrothermal fluids. Rifts are also critical in creating environments conducive to preservation of VMS mineralization, either through shielding massive sulfides from seafloor weathering and mass wasting or by creating environments conducive to the precipitation of subseafloor replacement-style mineralization in sedimented rifts. Subvolcanic intrusions are also products of the elevated heat flow regime common to VMS-forming environments. Shallow-level intrusive complexes (i.e., within 1?C3?km of the seafloor) may not be the main drivers of VMS-related hydrothermal circulation, but are likely the manifestation of deeper-seated mantle-derived heat (i.e., ~3?C10?km depth) that drives hydrothermal circulation. These shallower intrusive complexes are commonly long-lived (i.e., millions of years), and reflect a sustained thermally anomalous geodynamic environment. Such a thermally anomalous environment has the potential to drive significant hydrothermal circulation, and, therefore multi-phase, long-lived subvolcanic intrusive complexes are excellent indicators of a potentially fertile VMS environment. The absence of intrusive complexes, however, does not indicate an area of low potential, as they may have been moved or removed due to post-VMS tectonic activity. In some cases, shallow-level intrusive systems contribute metals to the VMS-hydrothermal system. 相似文献
13.
Recent studies on mineralogy, geochronology, fluid inclusion and stable isotope (Pb, Os, S, C, O, Sr) characteristics were reviewed to determine constraints for genetic models of the Chilean manto‐type copper deposits. The Chilean manto‐type deposits are divided into the two geologic categories of the northern areas (Arica–Iquique, Tocopilla–Taltal) and the central areas (Copiapó, La Serena, Santiago). The former is distributed in the coastal range composed of Jurassic andesite‐dominated volcano‐sedimentary piles and younger plutonic intrusions, and yields chalcocite (‐digenite) and bornite as the principal hypogene copper sulfides. The latter is hosted mostly in Lower Cretaceous volcano‐sedimentary sequences, and has chalcopyrite‐rich mineral associations. The fluid inclusion data indicate that the primary copper mineralization was commonly generated in the temperature range 150–360°C under low‐pressure conditions near the boiling curve, mediated with relatively saline brines. Generally, homogeneous Pb and S isotope compositions for primary copper minerals imply direct magma source or leaching of igneous rocks. Pb and Os isotope data published for some deposits, however, suggest that ore‐forming metals were derived mainly from the volcano‐sedimentary host rocks. The noticeably negative isotope ratios of primary sulfide sulfur and hydrothermal calcite carbon of some central area deposits indicate influx of sedimentary rock components, and the high 87Sr/86Sr initial ratios of hydrothermal calcite from the Tocopilla–Taltal area deposits imply contribution of the contemporaneous seawater or marine carbonates. These isotopic constraints imply a formation mechanism in which the Chilean manto‐type copper deposits formed epigenetically in the process of hydrothermal interaction of non‐magmatic surface‐derived brine with the volcano‐sedimentary host rocks, which is inferred to have been induced by a deep‐seated plutonic complex as the possible heat source. 相似文献
14.
Recent research on volcanic-hosted massive sulfide (VMS) deposits indicates that syngenetic subsea-floor replacement ores form an important component of many deposits. In the context of VMS deposits, subsea-floor replacement can be defined as the syn-volcanic formation of sulfide minerals within pre-existing volcanic or sedimentary deposits by infiltration and precipitation in open spaces (fractures, inter- and intra-granular porosity) as well as replacement of solid materials.There are five criteria for distinguishing subsea-floor replacement in massive sulfide deposits: (1) mineralized intervals are enclosed within rapidly emplaced volcanic or sedimentary facies (lavas, intrusions, subaqueous mass-flow deposits, pyroclastic fallout); (2) relics of the host facies occur within the mineral deposit; (3) replacement fronts occur between the mineral deposit and the host lithofacies; (4) the mineral deposit is discordant to bedding; and (5) strong hydrothermal alteration continues into the hanging wall without an abrupt break in intensity. Criteria 1–3 are diagnostic of replacement, whereas criteria 4 and 5 may suggest replacement but are not alone diagnostic. Because clastic sulfide ores contain accessory rock fragments collected by the parent sediment gravity flow(s) during transport, criteria 2 can only be applied to massive, semi-massive, disseminated or vein style deposits, and not clastic ores.The spectrum of VMS deposit types includes deposits that have accumulated largely subsea-floor, and others in which sedimentation and volcanism were synchronous with hydrothermal activity, and precipitation of sulfides occurred at and below the sea floor over the life of the hydrothermal system. Deposits that formed largely subsea-floor are mainly hosted by syn-eruptive or post-eruptive volcaniclastic facies (gravity flow deposits, water-settled fall, autoclastic breccia). However, some subsea-floor replacement VMS deposits are hosted by lavas and syn-volcanic intrusions (sills, domes, cryptodomes). Burial of sea-floor massive sulfide by lavas or sediment gravity flow deposits can interrupt sea-floor mineralization and promote subsea-floor replacement and zone-refining.The distance below the sea floor at which infiltration and replacement took place is rarely well constrained, with published estimates ranging from less than 1 to more than 500 m, but mainly in the range 10–200 m. The upper few tens to hundreds of metres in the volcano-sedimentary pile are the favoured position for replacement, as clastic facies are wet, porous and poorly consolidated in this zone, and at greater depths become progressively more compacted, dewatered, altered, and less amenable to large scale infiltration and replacement by hydrothermal fluids. Furthermore, sustained mixing between the upwelling hydrothermal fluid and cold seawater is regarded as a major cause of sulfide precipitation in VMS systems, and this mixing process generally becomes less effective with increasing depth in the volcanic pile.The relative importance of subsea-floor replacement in VMS systems is related principally to four factors: the permeability and porosity patterns of host lithofacies, sedimentation rate, the relative ease of replacement of host lithofacies (especially glassy materials) and early formed alteration minerals during hydrothermal attack, and physiochemical characteristics of the hydrothermal fluid. 相似文献
15.
The petrography and mineral chemistry of magnetite from fifteen volcanogenic massive sulfide (VMS) deposits in Canada, and the Lasail VMS deposit in Oman, as well as from two VMS-associated banded iron formations (BIF), Austin Brook (New Brunswick, Canada) and Izok Lake (Nunavut, Canada), were investigated using optical microscopy, electron probe micro-analyzer (EPMA), and laser ablation-inductively coupled plasma-mass spectrometry (LA-ICP-MS). The method of robust estimation for compositional data (robCompositions) was applied to investigate geochemical censored data. Among thirty-seven elements analyzed by EPMA and/or LA-ICP-MS in magnetite from the studied deposits/bedrock lithologies, only the results for Si, Ca, Zr, Al, Mg, Ti, Zn, Co and Ni contain < 40% censored values, and thus could be imputed using robCompositions. Imputed censored data were transformed using centered log-ratios to overcome the closure effect on compositional data. Transformed data were classified by partial least squares-discriminant analysis (PLS-DA) to identify different compositional characteristics of magnetite from VMS deposits and BIFs. The integration of petrography and mineral chemistry identifies three types of magnetite in VMS settings: magmatic, hydrothermal, and metamorphic. Magmatic magnetite in VMS deposit host bedrocks is characterized by ilmenite exsolution and may be overprinted by metamorphism. Some VMS deposits contain hydrothermal magnetite, which is intergrown with sulfides, and shows a metamorphic overprint as it is partly replaced by common metamorphic minerals including chlorite, sericite, anthophyllite, and/or actinolite, whereas the majority of the deposits are characterized by metamorphic magnetite formed by replacing pre-existing sulfides and/or silicates, and is intergrown with metamorphic minerals. Among VMS deposits of the Noranda mining district, the West Ansil deposit is characterized by hydrothermal-metamorphic magnetite zoned by inclusion-free cores and Si- and Mg-rich rims. Magnetite from the studied VMS-associated BIFs is also metamorphic in origin. Aluminum, Ti and Zn contents of magnetite can separate BIF from the other mineralized and un-mineralized bedrock lithologies in the studied VMS settings.PLS-DA shows that variable compositions of magnetite slightly discriminate different studied deposits/bedrock lithologies. The geochemical observations suggest that the variation in magnetite chemistry from different VMS settings might be sourced from differences in: 1) the composition and temperature of parental magmas or hydrothermal fluids, 2) the composition of host bedrocks, 3) the composition of co-forming minerals, and 4) oxygen fugacity. PLS-DA distinguishes magnetite compositions from the studied VMS deposits and BIFs from that of the other ore deposit types including Ni–Cu, porphyry Cu-Mo-Au, iron oxide-copper- gold, iron oxide-apatite, and the Bayan Obo REE-Fe-Nb deposit. Magnetite from the VMS settings on average contains lower concentrations of Si, Zr, Al, Mg, Ti, Zn, Co and Ni relative to that from the other mineral deposit types. PLS-DA of magnetite data from VMS deposits and BIFs of the Bathurst mining camp as well as PLS-DA of magnetite compositions from various mineral deposit types yield discrimination models for application to mineral exploration for VMS deposits using indicator minerals in Quaternary lithified sedimentary rocks. 相似文献
16.
新疆阿尔泰萨热阔布-铁木尔特地区两类矿化及成因 总被引：2，自引：0，他引：2
新疆阿尔泰南缘萨热阔布-铁木尔特一带的矿床均赋存于下泥盆统康布铁堡组的变质岩系中。早泥盆世的海相火山形成了Zn--Pb ( Cu) 矿化,晚泥盆世--早石炭世的碰撞造山相应形成了Cu--Au 石英脉矿化; 前者以铁木尔特VMS 型Zn--Pb ( Cu) 矿床为代表,后者以造山型萨热阔布金矿为代表,与造山有关的脉状矿化还叠加在铁木尔特等VMS 矿床中。通过对比两类矿化的稳定同位素特征,结合矿化的变形变质和流体包裹体特征,研究了成矿物质、成矿流体来源和矿床成因。萨热阔布金矿主成矿阶段硫化物石英脉和铁木尔特Zn--Pb ( Cu) 矿床中晚期发育的含黄铜矿石英脉中均富含碳质 ( CO2--CH4--N2 ) 流体包裹体,可能与碰撞造山的热液流体作用有关。铁木尔特Zn--Pb ( Cu) 矿床中代表VMS 期的浸染状矿石中硫化物δ34S 为－26. 46 × 10-3 ～ －19. 72 × 10 -3,硫主要来源于海水硫酸盐的无机还原和细菌还原作用; 而代表后期叠加改造的脉状矿化硫化物值与萨热阔布金矿床硫化物石英脉中δ34S 值接近,硫主要来源于造山过程中的深源流体。萨热阔布金矿床硫化物石英脉和铁木尔特Zn-- Pb ( Cu) 矿床晚期含黄铜矿石英脉的δDH2O 值和δ18OH2O 值,均反映了碰撞造山期热液与岩浆活动和变质作用有关。萨热阔布金矿硫化物石英脉中碳质流体包裹体CO2 体系中δ13 C 为－ 21. 15 × 10-3 ～ －7. 51 × 10 -3,CH4 体系的δ13C 为－34. 11 × 10 -3 ～ －28. 38 × 10-3 ; 铁木尔特Zn--Pb ( Cu) 矿床含黄铜矿石英脉中碳质包裹体测得的δ13C 为－8. 02 × 10 -3 ～ －6. 99 × 10 -3,δ13 C 特征与海相火山沉积无关,具岩浆源或深部源的特点。 相似文献
17.
与岩浆热场有关的成矿组合是一个新概念,是指在一个或大或小的区域内,在岩浆活动集中的时间段范围内,在岩浆热场的统一作用下所形成和影响的所有矿床,不论成因和矿种,均属于一个成矿组合。与岩浆热场有关的成矿作用主要包括下列几类： 岩浆热液矿床、岩浆热场叠加的沉积矿床、岩浆热场叠加的变质矿床、岩浆热场叠加的能源矿床（藏）以及热泉型矿床等。与岩浆热场有关的成矿组合把金属与非金属成矿作用联系起来,把无机与有机成矿联系起来,把热液与沉积成矿联系起来,把热液与变质成矿联系起来,把金属与能源（燃料）成矿联系起来。这种成矿组合的分布有两种趋势： 一是纵向上的由不同温度构成的成矿组合,如钨锡—铅锌组合、锡—铜组合等; 二是横向上的由相同温度不同矿种构成的成矿组合,如钨锡—石墨组合、金—铜—煤组合、铅—锌—煤组合、油—气—煤—铀组合等。成矿组合强调综合找矿的思路,在找矿时,除了注意主要矿产的找矿外,还应当注意其他矿产和矿种的找矿。在找金属矿床时,注意非金属矿床、沉积叠加改造矿床、变质叠加改造矿床以及能源矿床找矿的可能性。在研究高温金属矿床时,注意与高温成矿相伴的其他矿种成矿的可能性,注意低温金属矿床成矿的可能性,注意与低温成矿作用相伴的其他矿种成矿的可能性。开阔找矿的思路,就不能拘泥于本行本专业,而是围绕岩浆热场,将找所有可能出现的矿为己任。 相似文献
18.
海底黑烟囱的识别研究及其科学意义 总被引：22，自引：4，他引：18
现代海底黑烟囱广泛出现于大洋中脊、弧后盆地、浅海及大陆裂谷等环境,形成巨大规模的块状硫化物,并且在黑烟囱周围发现了化学自养细菌。海底硫化物黑烟囱具有明显的柱状-锥状构造形态,常保留通道构造,矿物同心圈状分带明显。黑烟囱的形成涉及热液流体与海水相互作用,外壁快速沉淀及通道内部硫化物结晶等过程。深部岩浆热源、热液沿裂隙集中流动和持续喷发,有利于形成大规模黑烟囱构造。海底硫化物丘体的钻探及其与地史时期块状硫化物的对比研究表明,它们具有相似的内部构造和矿床分带特征。黑烟囱的生长、垮塌以及丘体内部角砾化、交代、重结晶作用,有助于大规模矿床的形成。最后,在块状硫化物中寻找黑烟囱残片的研究,对于探讨成矿过程与早期生命活动具有重要意义。 相似文献