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1.
新疆北部幔源岩浆矿床的类型、时空分布及成矿谱系 总被引：6，自引：1，他引：5
新疆北部与幔源岩浆有关的矿床种类齐全,成矿环境复杂,时代和类型繁多,在中国乃至世界颇具特色。主要矿床类型包括铬铁矿矿床、钒钛磁铁矿矿床、铜镍硫化物矿床、铂族元素(PGE)矿床、铜镍-钒钛铁复合型矿床、含钴磁铁矿矿床、玄武岩自然铜矿床、热液型钴-多金属矿床,以及非金属矿床等。按照含矿地质体的类型,可分为6种类型:蛇绿岩型、层状杂岩型、小侵入体型、阿拉斯加型、浅成岩型和喷出岩型。这些幔源岩浆矿床可划分为3个成岩成矿系列:铜镍系列、钛铁系列和铬铁系列。钛铁系列以碱性层状岩体型钒钛磁铁矿、铁磷矿为代表,岩石具有明显的富Fe特征,属于碱性富铁质的高钛玄武岩系列;铜镍系列以小侵入体型铜镍矿、阿拉斯加型铜镍-PGE矿为代表,岩石属于铁质的拉斑玄武岩-钙碱性系列;铬铁系列主要为蛇绿岩型铬铁矿,岩石具富Mg贫Fe特征,属于镁质系列。3个系列的岩浆都具有亏损地幔源特征,可能都与地幔柱活动有关;岩浆源区富含相应的成矿元素,是形成3个系列矿床相应成矿地质体的主要条件。3个系列矿床的成矿机制可分为深部熔离/岩浆分异、就地分凝、矿浆贯入、岩浆热液等过程。根据各系列矿床之间存在的紧密联系,建立了与幔源岩浆作用有关的3个系列矿床综合模式: 亏损地幔部分熔融产生的幔源岩浆在上升过程中发生熔离/分异,分离为3个系列,由于外部物质加入在地壳深部发生分异和熔离,在不同深度富集形成铬铁矿、钒钛磁铁矿和铜镍硫化物矿床,临近地表时流体富集和分离成含矿流体,分别形成浅成岩型磁铁矿和喷出岩型自然铜矿。新疆北部各类幔源岩浆矿床从早到晚主要产于3期构造阶段/构造类型: 大陆裂解期、板块俯冲期、碰撞/后碰撞造山期(又分3个阶段: 碰撞后伸展阶段、幔柱叠加造山阶段、后碰撞结束阶段)。 相似文献
2.
Magnetite is a very common mineral in various types of iron deposits and some sulfide deposits. Recent studies have focused on the use of trace elements in magnetite to discriminate ore types or trace ore-forming process. Germanium is a disperse element in the crust, but sometimes is not rare in magnetite. Germanium in magnetite can be determined by laser ablation ICP-MS due to its low detection limit (0.0X ppm). In this study, we summary the Ge data of magnetite from magmatic deposits, iron formations, skarn deposits, iron oxide copper-gold deposits, and igneous derived hydrothermal deposits. Magnetite from iron formations contains relatively high Ge (up to ~250 ppm), whereas those from all other deposits mostly contains Ge less than 10 ppm, indicating that iron formations can be discriminated from other Fe deposits by Ge contents. Germanium in magmatic/hydrothermal magnetite is controlled by a few factors. Primary magma/fluid composition may be the major control of Ge in magnetite. Higher oxygen fugacity may be beneficial to Ge partition into magnetite. Sulfur fugacity and temperature may have little effect on Ge in magnetite. The enrichment mechanism of Ge in magnetite from iron formations remains unknown due to the complex ore genesis. Germanium along with other elements (Mn, Ni, Ga) and element ratios (Ge/Ga and Ge/Si raios) can distinguish different types of deposits, indicating that Ge can be used as a discriminate factor like Ti and V. Because of the availability of in situ analytical technique like laser ablation ICP-MS, in situ Ge/Si ratio of magnetite can serve as a geochemical tracer and may provide new constraints on the genesis of banded iron formations. 相似文献
3.
The El Laco magnetite deposits consist of more than 98 % magnetite but show field textures remarkably similar to mafic lava flows. Therefore, it has long been suggested that they represent a rare example of an effusive Fe oxide liquid. Field and petrographic evidence, however, suggest that the magnetite deposits represent replacement of andesite flows and that the textures are pseudomorphs. We determined the trace element content of magnetite by laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) from various settings at El Laco and compared them with magnetite from both igneous and hydrothermal environments. This new technique allows us to place constraints on the conditions under which magnetite in these supposed magnetite “lava flows” formed. The trace element content of magnetite from the massive magnetite samples is different to any known magmatic magnetite, including primary magnetite phenocrysts from the unaltered andesite host rocks at El Laco. Instead, the El Laco magnetite is most similar in composition to hydrothermal magnetite from high-temperature environments (>500 °C), such as iron oxide-copper-gold (IOCG) and porphyry-Cu deposits. The magnetite trace elements from massive magnetite are characterised by (1) depletion in elements considered relatively immobile in hydrothermal fluids (e.g. Ti, Al, Cr, Zr, Hf and Sc); (2) enrichment in elements that are highly incompatible with magmatic magnetite (rare earth elements (REE), Si, Ca, Na and P) and normally present in very low abundance in magmatic magnetite; (3) high Ni/Cr ratios which are typical of magnetite from hydrothermal environments; and (4) oscillatory zoning of Si, Ca, Mg, REE and most high field strength elements, and zoning truncations indicating dissolution, similar to that formed in hydrothermal Fe skarn deposits. In addition, secondary magnetite in altered, brecciated host rock, forming disseminations and veins, has the same composition as magnetite from the massive lenses. Euhedral magnetite lining both open-spaced veins in the brecciated host rock and along the walls of large, hollow chimneys in the massive magnetite lenses also displays oscillatory zoning and most likely formed by fluctuating composition and/or physio-chemical conditions of the fluid. Thus, the chemical fingerprint of magnetite from the supposed El Laco magnetite lava flows supports the hydrothermal model of metasomatic replacement of andesite lava flows, by dissolution and precipitation of magnetite from high-temperature fluids, rather than a magmatic origin from an effusive Fe oxide liquid. 相似文献
4.
夕卡岩铁矿床的成因一直以来备受争议,主要有接触交代和矿浆成因等模型。河北武安玉石洼铁矿是邯邢地区主要的夕卡岩铁矿之一,对矿区尖山剖面中的三类磁铁矿成分进行详细研究有助于解决此问题。产于剖面下部玉石洼铁矿主矿体中的磁铁矿以高Ti为特征,而在上部结晶灰岩中矿脉状中磁铁矿以高Si(w(SiO2)>1%)为特点,赋存于中部二长岩矿脉中的磁铁矿具有过渡的成分特征。通过对此三类磁铁矿中主量元素、微量元素研究发现,从下部玉石洼主矿体向上部结晶灰岩中的磁铁矿脉,磁铁矿具有Ti含量逐渐减少而Si、Mg含量逐渐增加的特征。高硅磁铁矿呈自形晶,与方解石平衡共生,其形成与流体有关,很可能是流体晶矿物。磁铁矿FeV/Ti判别图解显示下部玉石洼主矿体中部分磁铁矿具有岩浆成因,二长岩和结晶灰岩中的脉状矿石中磁铁矿具有热液成因,磁铁矿由下部到上部具有岩浆成因过渡为热液成因的连续过程。根据玉石洼矿区磁铁矿的这些特征,我们认为铁矿浆中含有大量流体,应该为“含铁熔体流体”,由于流体超压使“含铁熔体流体流”在岩浆通道中快速上升,至地壳浅部空间就位,在空间上由下部形成高温高Ti磁铁矿过渡为上部形成具有流体晶特征的高Si磁铁矿的岩浆通道成矿系统模型。 相似文献
5.
The Taihe, Baima, Hongge, Panzhihua and Anyi intrusions of the Emeishan Large Igneous Province (ELIP), SW China, contain large magmatic Fe–Ti–(V) oxide ore deposits. Magnetites from these intrusions have extensive trellis or sandwich exsolution lamellae of ilmenite and spinel. Regular electron microprobe analyses are insufficient to obtain the primary compositions of such magnetites. Instead, laser ablation ICP-MS uses large spot sizes (~ 40 μm) and can produce reliable data for magnetites with exsolution lamellae. Although magnetites from these deposits have variable trace element contents, they have similar multi-element variation patterns. Primary controls of trace element variations of magnetite in these deposits include crystallography in terms of the affinity of the ionic radius and the overall charge balance, oxygen fugacity, magma composition and coexisting minerals. Early deposition of chromite or Cr-magnetite can greatly deplete magmas in Cr and thus Cr-poor magnetite crystallized from such magmas. Co-crystallizing minerals, olivine, pyroxenes, plagioclase and apatite, have little influence on trace element contents of magnetite because elements compatible in magnetite are incompatible in these silicate and phosphate minerals. Low contents and bi-modal distribution of the highly compatible trace elements such as V and Cr in magnetite from Fe–Ti oxide ores of the ELIP suggest that magnetite may not form from fractional crystallization, but from relatively homogeneous Fe-rich melts. QUILF equilibrium modeling further indicates that the parental magmas of the Panzhihua and Baima intrusions had high oxygen fugacities and thus crystallized massive and/or net-textured Fe–Ti oxide ores at the bottom of the intrusive bodies. Magnetite of the Taihe, Hongge and Anyi intrusions, on the other hand, crystallized under relatively low oxygen fugacities and, therefore, formed net-textured and/or disseminated Fe–Ti oxides after a lengthy period of silicate fractionation. Plots of Ge vs. Ga + Co can be used as a discrimination diagram to differentiate magnetite of Fe–Ti–(V) oxide-bearing layered intrusions in the ELIP from that of massif anorthosites and magmatic Cu–Ni sulfide deposits. Variable amounts of trace elements of magmatic magnetites from Fe–Ti–(P) oxide ores of the Damiao anorthosite massif (North China) and from Cu–Ni sulfide deposits of Sudbury (Canada) and Huangshandong (northwest China) demonstrate the primary control of magma compositions on major and trace element contents of magnetite. 相似文献
6.
塔里木克拉通东北缘坡北、磁海等地二叠纪幔源岩浆活动形成了镍钴硫化物矿床和铁钴氧化物矿床，两者赋矿镁铁 超镁铁岩体的年龄相近(290~260 Ma)，主、微量元素和Sr Nd Hf同位素组成相似，分配系数接近的微量元素比值分布于相同趋势线，揭示两者岩浆源区相同，可能为俯冲板片流体交代的亏损地幔或软流圈地幔。两类矿床镁铁 超镁铁质岩中Co与Ni含量正相关，Co主要富集在基性程度高的岩石中；块状硫化物与磁铁矿矿石中Co与Ni相关性差，Co和Ni具有不同的富集机制，Co热液富集作用明显。北山镁铁 超镁铁杂岩体是地幔柱相关软流圈上涌，诱发俯冲板片交代的亏损岩石圈地幔发生部分熔融，形成的高镁母岩浆演化过程中经历壳源混染、硫化物饱和富集镍钴形成铜镍钴硫化物矿床，富铁母岩浆氧逸度高、富水，岩浆分离结晶磁铁矿、叠加热液作用富集钴，形成铁钴氧化物矿床。 相似文献
7.
Trace Element Geochemistry of Magnetite from the Fe(-Cu) Deposits in the Hami Region, Eastern Tianshan Orogenic Belt, NW China 总被引：5，自引：0，他引：5
Laser ablation–inductively coupled plasma–mass spectrometry(LA–ICP–MS) was used to determine the trace element concentrations of magnetite from the Heifengshan, Shuangfengshan, and Shaquanzi Fe(–Cu) deposits in the Eastern Tianshan Orogenic Belt. The magnetite from these deposits typically contains detectable Mg, Al, Ti, V, Cr, Mn, Co, Ni, Zn and Ga. The trace element contents in magnetite generally vary less than one order of magnitude. The subtle variations of trace element concentrations within a magnetite grain and between the magnetite grains in the same sample probably indicate local inhomogeneity of ore–forming fluids. The variations of Co in magnetite between samples are probably due to the mineral proportion of magnetite and pyrite. Factor analysis has discriminated three types of magnetite: Ni–Mn–V–Ti(Factor 1), Mg–Al–Zn(Factor 2), and Ga– Co(Factor 3) magnetite. Magnetite from the Heifengshan and Shuangfengshan Fe deposits has similar normalized trace element spider patterns and cannot be discriminated according to these factors. However, magnetite from the Shaquanzi Fe–Cu deposit has affinity to Factor 2 with lower Mg and Al but higher Zn concentrations, indicating that the ore–forming fluids responsible for the Fe–Cu deposit are different from those for Fe deposits. Chemical composition of magnetite indicates that magnetite from these Fe(–Cu) deposits was formed by hydrothermal processes rather than magmatic differentiation. The formation of these Fe(–Cu) deposits may be related to felsic magmatism. 相似文献
8.
岩浆热液出溶和演化对斑岩成矿系统金属成矿的制约 总被引：29，自引：1，他引：29
岩浆热液过渡阶段对于与岩浆热液有关矿床的形成非常重要。以往的研究多侧重于岩浆结晶阶段和低于固相线的热液阶段过程和演化 ,但对于流体从熔体出溶到熔体最后固结过程的理解却很有限。基于流体包裹体冷热台研究、单个流体和熔体包裹体原位无损成分分析技术 ,并结合挥发份和成矿元素在共存相间分配的实验和质量平衡计算模拟 ,岩浆热液出溶和演化对金属成矿制约的研究取得了很大进展。文中从岩浆中挥发份的出溶和演化、成矿元素在岩浆热液过渡体系各相之间的分配、斑岩矿床成矿流体及与金属成矿的关系、浅成热液矿床成矿流体及与金属成矿的关系几个方面进行了阐述。研究表明 :( 1)岩浆熔体不仅含有足够的挥发性组分 ,而且出溶的挥发份能够被圈闭在流体包裹体中而成为岩浆出溶热液的实物证据。 ( 2 )挥发份和成矿元素不仅在岩浆熔体和出溶的溶液间分配 ,还将在熔体与盐水溶液、熔体与气相以及盐水溶液与气相间进行分配。Cu在岩浆蒸气中比在共存的熔体中要富集数百倍 ,而Cu ,As,Au(可能作为HS配合物 )则偏向于分配进入与液体相共存的蒸气相中。 ( 3 )成矿元素在熔体 /溶液间的分配系数受控于熔体中初始水含量与饱和水含量之比值和岩浆熔体与共存出溶水溶液的w(Cl) /w(H2 O)和w(F) /w(Cl)比值。 ( 4 )斑岩 相似文献
9.
Understanding the geochemical behavior of chalcophile elements in magmatic processes is hindered by the limited partition coefficients between sulfide phases and silicate melt, in particular at conditions relevant to partial melting of the hydrated, metasomatized upper mantle. In this study, the partitioning of elements Co, Ni, Cu, Zn, As, Mo, Ag, and Pb between sulfide liquid, monosulfide solid solution (MSS), and hydrous mantle melt has been investigated at 1200 °C/1.5 GPa and oxygen fugacity ranging from FMQ−2 to FMQ+1 in a piston-cylinder apparatus. The determined partition coefficients between sulfide liquid and hydrous mantle melt are: 750–1500 for Cu; 600–1200 for Ni; 35–42 for Co; 35–53 for Pb; and 1–2 for Zn, As, and Mo. The partition coefficients between MSS and hydrous mantle melt are: 380–500 for Cu; 520–750 for Ni; ∼50 for Co; <0.5 for Zn; 0.3–6 for Pb; 0.1–2 for As; 1–2 for Mo; and >34 for Ag. The variation of the data is primarily due to differences in oxygen fugacity. These partitioning data in conjunction with previous data are applied to partial melting of the upper mantle and the formation of magmatic-hydrothermal Cu–Au deposits and magmatic sulfide deposits.I show that the metasomatized arc mantle may no longer contain sulfide after >10–14% melt extraction but is still capable of producing the Cu concentrations in the primitive arc basalts, and that the comparable Cu concentrations in primitive arc basalts and in MORB do not necessarily imply similar oxidation states in their source regions.Previous models proposed for producing Cu- and/or Au-rich magmas have been reassessed, with the conclusions summarized as follows. (1) Partial melting of the oxidized (fO2 > FMQ), metasomatized arc mantle with sulfide exhaustion at degrees >10–14% may not generate Cu-rich, primitive arc basalts. (2) Partial melting of sulfide-bearing cumulates in the root of thickened lower continental crust or lithospheric mantle does not typically generate Cu- and/or Au-rich magmas, but they do have equivalent potential as normal arc magmas in forming magmatic-hydrothermal Cu–Au deposits in terms of their Cu–Au contents. (3) It is not clear whether partial melting of subducting metabasalts generates Cu-rich adakitic magmas, however adakitic magmas may extract Cu and Au via interaction with mantle peridotite. Furthermore, partial melting of sulfide-bearing cumulates in the deep oceanic crust may be able to generate Cu- and Au-rich magmas. (4) The stabilization of MSS during partial melting may explain the genetic link between Au-Cu mineralization and the metasomatized lithospheric mantle.The chalcophile element tonnage, ratio, and distribution in magmatic sulfide deposits depend on a series of factors. This study reveals that oxygen fugacity also plays an important role in controlling Cu and Ni tonnage and Cu/Ni ratio in magmatic sulfide deposits. Cobalt, Zn, As, Sn, Sb, Mo, Ag, Pb, and Bi concentrations and their ratios in sulfide, due to their different partitioning behavior between sulfide liquid and MSS, can be useful indices for the distribution of platinum-group elements and Au in magmatic sulfide deposits. 相似文献
10.
莱芜张家洼铁矿磁铁矿LA-ICP-MS微量元素特征及其对成矿过程的制约 总被引：1，自引：0，他引：1
莱芜张家洼铁矿位于华北克拉通东缘的鲁西地区,矿石成因类型为夕卡岩型铁矿。矿体赋存在早白垩世高镁闪长岩与奥陶系马家沟组灰岩及白云岩接触带附近。本文通过对莱芜岩浆和热液磁铁矿电子探针(EPMA)以及激光剥蚀电感耦合等离子体质谱(LA ICP MS)分析,探讨磁铁矿微量元素组成及变化规律对成岩和成矿作用的指示,为揭示张家洼铁矿的矿床成因及其成矿流体演化过程提供重要制约。分析结果表明,莱芜岩浆磁铁矿与热液磁铁矿相比明显富集Ti、V、Cr等亲铁元素,相对富集Nb、Ta、Zr、Hf等高场强元素以及Sn、Ga、Ge、Sc等中等相容元素,Mg、Al、Mn、Zn、Co显著富集于热液磁铁矿中。Ti、V、Cr以及Mg、Al、Mn、Zn在岩浆和热液中具有不同的地球化学行为,Ti、V、Cr从熔体中进入磁铁矿主要受温度、分配系数以及fO2控制。Mg、Al、Mn、Zn主要受控于水岩反应和后期绿泥石+碳酸盐脉的交代,这些元素通过类质同象替换富集于热液磁铁矿中。Co在热液磁铁矿中除了受水岩相互作用和后期流体交代的影响外,硫化物的出现会导致Co含量急剧降低。Si、Ca、Na及Sr、Ba在岩浆和热液磁铁矿中的地球化学行为非常一致。Ti Ni/Cr图能够用于区分岩浆和热液磁铁矿,莱芜岩浆磁铁矿中Ti含量较高且Ni/Cr比值≤1,热液磁铁矿Ti含量较低且绝大多数Ni/Cr比值≥1。张家洼热液磁铁矿可分为早、晚两个阶段：早期阶段包括(1)早期原生粒状磁铁矿和(2)早期次生磁铁矿;晚期阶段包括(3)晚期原生磁铁矿和(4)晚期次生磁铁矿。原生磁铁矿具有典型的三联点结构特征;次生磁铁矿受后期热液交代影响表现为多空隙,通常呈不规则状、树枝状、骸晶以及交代残余结构。磁铁矿微量元素生动记录了成矿流体演化过程,从早期到晚期、从原生到次生都显示Mg、Al、Mn、Zn包括Co含量持续升高,表明成矿流体可能朝着富集这些微量元素的方向演化。后期流体的交代导致绿泥石蚀变为磁铁矿,连续水岩相互作用和后期流体的交代以及绿泥石直接蚀变是导致热液磁铁矿富集Mg、Al、Mn、Zn等元素的主要原因。热液磁铁矿晚期孔隙较为发育,孔隙度的增加促使更多的流体和磁铁矿发生反应。热液磁铁矿的微量元素不仅能够反映矿床形成的物理化学条件,而且可以反映围岩性质以及水岩相互作用过程。 相似文献
11.
吐哈盆地早二叠世玄武岩原始岩浆性质:来自熔融包裹体成分的制约 总被引：3，自引：3，他引：0
东天山地区的二叠纪玄武岩沿着区域的北东东向断裂呈脉状分布,吐哈盆地玄武岩的40Ar-39Ar坪年龄为298.2±3.8Ma,为早二叠世,与前人的玄武岩年龄结果在误差范围内一致。可能与东天山地区二叠纪岩浆铜镍矿床镁铁-超镁铁岩有密切的成因联系。吐哈玄武岩的主微量成分显示其为岛弧拉斑、大陆弧玄武岩,轻稀土富集和Nb、Ta负异常,指示源区可能经历过俯冲作用的改造。吐哈盆地二叠纪玄武岩含有新鲜的橄榄石和长石斑晶,橄榄石斑晶中熔融包裹体较发育。熔融包裹体为玻璃质、气相和玻璃质、气相、固相两种类型。包裹体中不透明矿物主要为磁铁矿,说明捕获包裹体时岩浆的氧逸度和Fe含量较高。熔融包裹体分为高MgO和低MgO含量两种。高MgO含量的包体同时具有低SiO_2、低微量和稀土元素含量的特征,可能为地幔高部分熔融的产物,且经历过深部演化程度较弱。该高MgO熔体的微量元素显示Nb、Ta亏损的特征,具有N-MORB特征的微量和稀土元素分配模式,预示该熔体为受到俯冲交代的地幔熔融形成。熔融包裹体相对玄武岩具有低的Th和Ta含量、相对弱的Nb和Ta的负异常的特征,指示熔融包裹体的成分经受改造程度低于玄武岩,暗示可能为经历过较少后期作用改造的相对原始的熔体。熔体中Cu含量(12.4×10~(-6)~299×10~(-6))在正常玄武质岩浆含量范围内,而Ni含量(236×10~(-6)~697×10~(-6))高于高镁溢流科马提岩和洋中脊玄武岩。该Cu、Ni含量略显解耦的熔体可能代表了经历过深部少量的硫化物熔离,带走小部分Cu和Ni等成矿元素之后所捕获的岩浆。如果将该熔体视为东天山地区二叠纪岩浆铜镍硫化物矿床的母岩浆,该母岩浆中Ni含量相对较高可能是岩浆铜镍硫化物矿床中矿石的Ni/Cu比值大多大于1.0的主要因素。 相似文献
12.
《Chemie der Erde / Geochemistry》2021,81(1):125679
This study describes textures and mineral chemistry of magnetite-ilmenite-bearing pods/pockets in mineralogically diverse feldspathic schist near Pathargora in the Singhbhum Shear Zone, eastern India. The textural and geochemical characteristics of the magnetite-ilmenite assemblage are the results of a protracted geological history involving magmatic crystallization and oxidation-exsolution of titanomagnetite, deformation-induced recrystallization and textural re-equilibration and hydrothermal fluid-induced hematitization of magmatic magnetite. The magnetite grains contain characteristic trellis and sandwich ilmenite lamella, which are interpreted to be the products of oxidation-exsolution of ulvöspinel component of magnetite-ulvöspinel solid solution. The exsolution process was accompanied by preferential partitioning of spinel elements such as Cr, Al and V in magnetite and Ti, Mn, Mg, HFS elements (Nb, Ta), transition elements (Sc, Co, Cu and Zn) and granitophile elements (Mo, Sn and W) in ilmenite. The deformed sandwich lamella is locally recrystallized and transformed into granular ilmenite close to fractures, micro-shear planes and magnetite grain boundaries. Coarse granules of ilmenite, within or associated with magnetite, are of two textural types: one invariably contains Fe-rich exsolved phase and may be of magmatic origin, while the other mostly formed by strain-induced, fluid-mediated expulsion (from the interior of magnetite to its boundary) and dynamic recrystallization of existing ilmenite lamella in magnetite, and dynamic recrystallization of primary ilmenite containing Fe-rich exsolved phases. Magnetite is variably hematitized. The highly porous nature and trace element geochemistry of hematite and mass-balance calculations suggest the hematitization was mostly redox-independent and was caused by infiltration of metal-rich, reduced and acidic fluid. The hematitization process was associated with significant enrichment and immobilization of U, Th, Pb, REEs, Cu, Mo and W and depletion of Ni, Cr, V in hematite. 相似文献
13.
岩浆Cu-Ni-PGE矿床研究现状及发展趋势 总被引：4，自引：0，他引：4
从全球视野分析研究了世界岩浆铜镍硫化物矿床的大地构造分布和成岩成矿类型,特别是通过上世纪末新发现的加拿大Voisey′s Bay矿床与俄罗斯Noril′sk等世界级矿床特征的对比研究,突出强调了大火成岩省(LIPs)对大规模岩浆硫化物矿床形成的意义,从更加宏观的角度审视了世界级岩浆硫化物矿床形成的地质背景和岩浆作用条件,为中国金川等岩浆Cu-Ni-PGE硫化物矿床的深入研究提供了参照背景。评述分析了当代岩浆硫化物矿床成矿研究中,幔源岩浆中硫化物液相不混溶(熔离)的演化轨迹,对岩浆萃取地壳中的硫改变硫化物饱和度促成不混溶作用发生的可能性和条件进行了探讨,进一步讨论了岩浆演化过程中,亲铜元素(Ni、Cu、Co、Pt和Pd等)进入硫化物液相成为金属硫化物或先期进入先结晶的橄榄石、辉石矿物成为氧化物的物理化学行为,并通过加拿大Sudbury陨石撞击构造成因矿床复合热液对硫化物矿体形成贡献的讨论,提出了热液作用对岩浆硫化物矿床成矿的可能贡献。分析判断了中国岩浆Cu-Ni-PGE硫化物矿床的成矿特点和金川超大型岩浆Cu-Ni-PGE矿床外围的找矿潜力。 相似文献
14.
安徽月山矿田硅、氦、氖同位素地球化学研究 总被引：2，自引：1，他引：2
对安徽月山矿田硅、氦、氖同位素组成研究表明 ,月山岩体是玄武质岩浆结晶分异和同化混染的产物 ,矿床的硅来自岩浆熔 流分离作用形成的岩浆热液 ,成矿流体中的氦来自地壳和地幔两个端员。成矿过程中发生了富含放射性成因氦的演化大气降水与岩浆热液的混合。 相似文献
15.
西天山敦德铁矿床磁铁矿原位LA-ICP-MS元素分析及意义 总被引：5，自引：3，他引：2
敦德铁矿床是天山成矿带内新近发现并勘查的一处大型海相火山岩型铁矿床。该矿床的矿石可划分为浸染状、稠密浸染状、条带状和块状4种主要类型。其中的条带状矿石包括磁铁矿_矽卡岩条带和磁铁矿_方解石条带2种亚类型。块状矿石内出现围岩或矽卡岩角砾时则构成角砾状矿石,其磁铁矿的成因无甚差异。根据野外观察和矿相显微研究,认为磁铁矿形成于早期矽卡岩阶段后的退化蚀变阶段,之后又被更晚的硫化物阶段和绿泥石_碳酸盐阶段的矿物叠加。敦德磁铁矿内主要发生了Al、Mn、Mg和Zn的类质同象置换,此外,也含有Ti、Si、Ca等次要元素以及Na、K、V、Cr、Ni、Co等多种可检测到的微量元素。磁铁矿内元素含量在空间上显示出直观的差异,由深部到浅部,Mn、Zn含量升高,Si、Ca、Na、K、Pb、Ba、Sr、Sb、Cu等含量降低。在Ti O2_Al2O3_Mg O图解、Ti O2_Al2O3_(Mg O+Mn O)图解和Ca+Al+Mn_Ti+V图解上,敦德磁铁矿的分析数据均投影于热液交代(矽卡岩)成因区域。综上认为,该矿床的磁铁矿可能为热液充填交代成因。 相似文献
16.
17.
河南熊耳山地区花山花岗岩与金矿化的关系 总被引：14，自引：0，他引：14
熊耳山地区是豫西重要的金矿化集中区。通过对该区花山花岗岩的化学组成、微量元素、稀土元素、稳定同位素特征及与金矿化关系的研究,得出如下主要研究成果：（1）在R型聚类分析谱系图上表明岩体中Au、Ag、Pb、Cu、Ba元素与金矿床微量元素相关性趋于一致;（2）在稀土元素配分模式图上表现出花岗岩和蚀变岩具有相似的右倾配分曲线的特征;（3）在流体包裹体的w(Na+)-w(K+)-w(Ca2++Mg2+)成分三角图上表明金成矿流体和岩浆热液具亲缘关系;（4）岩体线性构造控制了花山地区构造蚀变岩型和爆破角砾岩型金矿床的时空分布;（5）金矿床的成矿时代为燕山期,花山花岗岩的成岩时间集中于81～159 Ma;（6）S、H、O、Pb同位素组成表明成矿物质和成矿流体来自岩浆热液。 相似文献
18.
新疆哈密黄山地区铜镍硫化物矿床的稀土元素特征及意义 总被引：29，自引：9，他引：20
通过对新疆哈密黄山铜镍矿带典型矿床矿石矿物和含矿岩石的稀土元素地球化学研究,发现产于造山带的铜镍硫化物矿床的容矿镁铁-超镁铁质岩具有富水特征,部分硫化物稀土曲线呈特殊的“三重弯曲”模式,反应出由于多种液相(流体和熔体)共存,硫化物熔体中含有大量热液流体,在主成矿期(岩浆熔离期)后逐渐演化出富含气液的成矿流体。本区矿床稀土特征不同于克拉通边缘的铜镍矿床,造成上述热液流体参与成矿的原因在于含矿岩体本身富水,可能与碰撞后富水洋壳的拆沉熔融有关。 相似文献
19.
YI Liwen GU Xiangping LU Anhuai LIU Jianping LEI Hao WANG Zhiling CUI Yu ZUO Hongyan SHEN Can 《《地质学报》英文版》2015,89(4):1226-1243
Magnetite, as a genetic indicator of ores, has been studied in various deposits in the world. In this paper, we present textural and compositional data of magnetite from the Qimantag metallogenic belt of the Kunlun Orogenic Belt in China, to provide a better understanding of the formation mechanism and genesis of the metallogenic belt and to shed light on analytical protocols for the in situ chemical analysis of magnetite. Magnetite samples from various occurrences, including the ore–related granitoid pluton, mineralised endoskarn and vein–type iron ores hosted in marine carbonate intruded by the pluton, were examined using scanning electron microscopy and analysed for major and trace elements using electron microprobe and laser ablation–inductively coupled plasma–mass spectrometry. The field and microscope observation reveals that early–stage magnetite from the Hutouya and Kendekeke deposits occurs as massive or banded assemblages, whereas late–stage magnetite is disseminated or scattered in the ores. Early–stage magnetite contains high contents of Ti, V, Ga, Al and low in Mg and Mn. In contrast, late–stage magnetite is high in Mg, Mn and low in Ti, V, Ga, Al. Most magnetite grains from the Qimantag metallogenic belt deposits except the Kendekeke deposit plot in the " Skarn " field in the Ca+Al+Mn vs Ti+V diagram, far from typical magmatic Fe deposits such as the Damiao and Panzhihua deposits. According to the(Mg O+Mn O)–Ti O2–Al2O3 diagram, magnetite grains from the Kaerqueka and Galingge deposits and the No.7 ore body of the Hutouya deposit show typical characteristics of skarn magnetite, whereas magnetite grains from the Kendekeke deposit and the No.2 ore body of the Hutouya deposit show continuous elemental variation from magmatic type to skarn type. This compositional contrast indicates that chemical composition of magnetite is largely controlled by the compositions of magmatic fluids and host rocks of the ores that have reacted with the fluids. Moreover, a combination of petrography and magnetite geochemistry indicates that the formation of those ore deposits in the Qimantag metallogenic belt involved a magmatic–hydrothermal process. 相似文献
20.
Daizo ISHIYAMA Ryoji SATO Toshio MIZUTA Yohei ISHIKAWA Jingbin WANG 《Resource Geology》2001,51(4):377-392
Abstract: The Anle Sn‐Cu and Huanggangliang Fe‐Sn deposits have been exploited in the Linxi district, which is located 165 km northwest of Chifeng City in northern China. In this study the formation mechanisms of the tin deposits in the Anle and Huanggangliang mining area were investigated to understand the mechanisms of tin mineralization in northern China. The veins of the Anle deposit are divided into cassiterite–quartz–chlorite veins, chalcopyrite‐bearing quartz veins, cassi–terite–chalcopyrite–bearing quartz veins and sphalerite‐quartz veins. The sequence of mineralization is tin mineralization (stage I), copper mineralization (stage II), and lead‐zinc mineralization (stage III). The Huanggangliang tin deposit consists of magnetite skarn orebodies and many cassiterite‐bearing feldspar–fluorite veins and veinlets cutting the magnetite orebodies. The fluid inclusions in quartz and fluorite in ores from the Anle and Huanggangliang tin deposits are divided into two‐phase fluid inclusions, vapor‐rich fluid inclusions and poly‐phase fluid inclusions. The final homogenization temperatures of fluid inclusions of quartz in the ores of the Anle deposit and fluorite of tin‐bearing feldspar veins in the Huanggangliang tin deposit range from 195 to 425C and from 215 to 450C, respectively. The fluids responsible for the Anle and Huanggangliang tin deposits were of very high temperature and NaCl‐rich ones containing K, Ca, Al, Si, Ti, Fe and Cl in addition to ore metals such as Sn and Cu. The temperature and chemical composition of fluid in fluid inclusions of igneous rocks in the mining area are very similar to those of fluid in fluid inclusions in the ores of these deposits. The fluid for these ore deposits had a close relation with the fluid coexisting with melt of Late Jurassic granitic rocks in this mining area. Salinities of fluid inclusions from these ore deposits and granitic rocks in the mining area were estimated to range from 35 to 50 wt % NaCl equivalent. Based on arsenopy‐rite geothermometry and fluid inclusion studies, a fluid containing 40 wt% NaCl (eq.) could be formed by phase separation of fluid having 6 wt% NaCl (eq.) at a temperature of 420 to 500C and a pressure of 0.3 to 0.4 kb. The temperatures and pressures presented above indicate an NaCl‐rich magmatic fluid derived from granitic melt that had intruded into a shallow level of crust caused the Sn–Fe–Cu mineralization of the mining area. The geological relationship between these ore deposits and granitic bodies around the ore deposits, and the similarity of fluids forming these ore deposits and coexisting with granitic melt, suggest that these ore deposits were formed by the activity of fluid derived from granitic melt in Late Jurassic age. 相似文献