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1.
大坪金矿成矿可分为三个成矿阶段:早期成矿阶段(白钨矿石英脉)、主成矿阶段(团块状多金属硫化物含金石英脉)和晚成矿阶段(碳酸盐石英脉)。本文利用显微测温和拉曼光谱分析了大坪矿脉的流体包裹体特征,结果表明:流体包裹体基本由富液相CO2包裹体和不同CO2/H2O比例的CO2-H2O型包裹体组成,早阶段白钨矿石英脉中同时富含富气相CO2包裹体,主成矿阶段团块状多金属硫化物金矿石中富液相CO2包裹体占明显优势,只有晚成矿阶段碳酸盐石英脉中含有居次要地位的H2O溶液包裹体。流体包裹体中气相组成基本为纯CO2,早阶段者还含少量N2。早阶段CO2-H2O型包裹体的盐度为6.37%-14.64%NaCl,峰值9%-10.5%NaCl,均一温度为299.4-423.7℃,峰值320-380℃,CO2包裹体密度为0.352-0.798g/cm^3,多数在0.64-0.71g/cm^3;主成矿阶段的CO2-H2O型包裹体的盐度在3.70%-14.64%NaCl之间,峰值7.2%-9.0%NaCl,均一温度279.0-406.5℃之间,峰值320-360℃,CO2包裹体密度为0.591-0.843g/cm^3,多数大于0.8g/cm^3;晚成矿阶段CO2-H2O型包裹体的盐度为4.80%-6.54%NaCl,均一温度为287.6-337.1℃。计算表明早阶段成矿压力约为190-440MPa,主阶段成矿压力约为133.5-340.0MPa,相当的成矿深度为5.1-12.9km。这些特征揭示了该矿成矿流体为近临界的高CO2(CO2≥H2O)的中低盐度的CO2-H2O-NaCl体系流体,在成矿过程中基本不存在流体混合,但发生了明显的沸腾和相分离作用。该矿是剪切带控制下的中深中温热液金矿,成矿作用主要是减压沸腾环境下的快速沉淀。结合其它证据,作者认为该矿的成矿流体主体为深源的壳幔混合流体,而不是地壳浅部的大气降水、岩浆水或其混合流体。金在高CO2的成矿流体中可能主要以硫氢络合物形式迁移,矿质沉淀主要与压力速降条件下发生流体的相分离作用相关。  相似文献   

2.
桃行榴辉岩是苏鲁超高压变质带中段主要榴辉岩体密集分布区之一。流体包裹体研究表明,榴辉岩矿物及高压脉体石英中捕获有五种类型的流体包裹体:在超高压-高压榴辉岩相条件下捕获的N2±CH4包裹体;在榴辉岩发生麻粒岩相叠加变质作用期间被捕获的B型纯CO2液相包裹体;在高压榴辉岩重结晶阶段被捕获的C型CO2-H2O包裹体和D型高盐度水溶液包裹体;超高压岩石折返过程中的最晚阶段(角闪岩相退变质甚至更晚)捕获的E型低盐度水溶液包裹体。利用榴辉岩矿物及高压脉体石英中捕获的流体包裹体类型及期次可以重建超高压变质作用板片折返过程中的流体性状与演化,而石榴石中捕获的纯CO2包裹体为本区榴辉岩相岩石遭受了麻粒岩相叠加提供了佐证。  相似文献   

3.
小佟家堡子、林家金矿是青城子铅锌、金、银矿集区的中-大型金矿床,金矿床与沉积-变质期硅化岩关系密切。通过与矿区尖山岩体、新岭岩体中流体包裹体对比研究表明,金矿床与尖山岩体中主要发育水溶液包裹体,极少量的CO2包裹体、含CO2三相包裹体,而新岭岩体除发育以上包裹体外,还发育含子矿物多相包裹体。测温结果显示金矿床成矿流体温度为110~335℃,盐度3.9%~16.2%NaClrq拉曼光谱分析表明金矿床流体成分以H2O为主,少量的CO2、CH4等气体,表明成矿流体属NaCl-H2O体系。金矿床与尖山岩体中流体包裹体温度、盐度及成分相近,推断成矿流体主要来自沉积-变质期。  相似文献   

4.
拉陵灶火钼多金属矿床东昆仑成矿带新发现的一个矽卡岩-斑岩型钼多金属矿床,针对该矿床矿化石英脉中的流体包裹体进行温压条件及单个包裹体激光拉曼光谱研究。结果表明,流体包裹体类型主要有气液两相、含CO2三相及富CO2包裹体。测温结果显示石英辉钼矿化阶段包裹体均一温度集中于200℃~350℃,石英硫化物细脉阶段包裹体均一温度集中165℃~210℃。成矿流体的盐度w(NaCl eqv)介于2.73%~16.72%,总体属中低盐度CO2-H2O-NaCl体系。成矿过程中发生过沸腾作用,压力急剧降低,可能产生沸腾作用主要因素。本区斑岩型钼矿形成于洋壳俯冲结束到陆陆碰撞开始的转折期,下地壳的部分熔融是成岩成矿的主要物质源区,因此成矿流体具有富CO2的特征。  相似文献   

5.
成矿环境中的高密度碳质流体:以阿尔泰南缘为例   总被引:1,自引:0,他引:1       下载免费PDF全文
碳质流体(CO2-CH4-N2体系流体)常见于地幔橄榄岩和下地壳麻粒岩中。近期研究表明,阿尔泰南缘晚古生代成矿环境中的碳质流体极为丰富,不仅在造山型金矿中赋存大量与成矿有关的碳质流体,而且在VMS型矿床中也存在同造山期的变质碳质流体。由共生的富CO2包裹体(LCO2-LH2O型)和H2O-CO2包裹体(LH2O-LCO2型)的均一温度推测,造山型金矿的碳质流体捕获温度大于254~394.5℃,压力大于150~320MPa;VMS矿床的变质碳质流体捕获温度大于209~430℃,压力大于180~300MPa,两者具相似的捕获温度压力条件。碳质流体的捕获温度压力条件与变质相带相平衡计算的变质温度、压力范围相当。碳质流体源于区域变质作用,并参与了与造山型金矿有关的构造-变质-流体-成矿作用和对VMS型矿床的变质改造作用。  相似文献   

6.
吉林夹皮沟金矿带成矿流体地球化学特征   总被引:6,自引:0,他引:6  
对夹皮沟地区夹皮沟群变质岩—斜长角闪岩及夹皮沟和二道沟金矿金矿石中的流体包裹体进行了岩相学、显微测温及单个包裹体成分激光拉曼光谱研究。结果表明:金矿石中发育水溶液相、含 CO_2相及 CO_2相等三类包裹体,成矿过程中,流体经历了 NaCl-H_2O-CO_2体系的不混溶作用,各类包裹体均一温度157.2℃~440℃,盐度1.8%~11.6%NaCl eqv,流体密度0.54~0.96g/cm~3;变质岩中以发育含子矿物多相包裹体为主,其均一温度为260℃~480℃,盐度为36.5%~54.8%NaCl eqv,流体密度为1.06~1.17g/cm~3,反映了变质流体为一中温、高盐度、高密度均匀 NaCl-H_2O 热液体系。成矿流体与变质流体存在明显差异,表明该区金矿床成矿流体并非来自太古代变质热液。结合新近的流体包裹体氢、氧同位素分析结果和测年数据,认为本区金矿成矿流体以来自岩浆热液为主,矿床成因属中生代岩浆热液矿床。  相似文献   

7.
为了了解抱伦金矿的成因条件,利用岩相学和拉曼光谱分析方法对不同期次含金石英脉中流体包裹体进行系统、深入的研究.结果表明,石英中流体包裹体可分为2种类型,即CO2-H2O包裹体和H2O溶液包裹体.CO2-H2O包裹体以CO2为主,含有CH4,主要存在于成矿期金-石英脉和金-多金属硫化物脉中,多为原生包裹体,孤立分布或成群...  相似文献   

8.
云南大坪金矿是哀牢山金矿带中最重要的金矿之一,主要赋存在受到强烈韧性剪切和水-岩反应的加里东期闪长岩中,是典型的韧性剪切带控矿型金矿。本文对大坪金矿绢英岩化近矿围岩中的热液绢云母进行了40Ar-39Ar定年,得到其坪年龄为33.76±0.65Ma,相应的反等时线和正等时线年龄分别为33.55±0.74Ma和33.57±0.74Ma,显示大坪属于喜马拉雅早期金矿。这些年龄数据与哀牢山金矿带中广泛出现的喜马拉雅期煌斑岩脉年龄(33~34Ma)非常接近,显示金矿与上地幔部分熔融形成的煌斑岩之间可能存在成因上的联系。喜马拉雅早期,本区在地壳拉张和强烈韧性剪切条件下,Moho面上升,地幔物质部分熔融并上涌,形成大量煌斑岩等基性岩脉,地幔排气形成的深源地幔流体和下地壳脱水形成的富CO2流体混合,沿韧性剪切带上升,并与糜棱岩化的加里东期闪长岩围岩发生水-岩反应,局部发生流体沸腾作用,导致成矿流体物理化学条件的改变和矿石矿物的沉淀,在剪切带脆性构造中形成含金石英脉。  相似文献   

9.
山东金岭金矿床成矿流体地球化学特征   总被引:4,自引:0,他引:4  
王力  孙丰月  王佳良 《岩石学报》2010,26(12):3735-3744
对山东金岭金矿矿石中的流体包裹体进行了岩相学、显微测温及单个包裹体成分激光拉曼光谱研究。结果表明:金矿石中发育含CO2相、气液两相和CO2相等三类包裹体,成矿过程中,流体经历了NaCl-H2O-CO2体系的不混溶作用;成矿流体具有低盐度(6.6%~10.8%NaCleqv)、低密度(0.54~0.93g.cm-3)的特点;成矿温度集中于280~300℃之间,成矿压力为70~119MPa,成矿深度为6.78~9.07km;矿石石英中流体包裹体成分普遍含CO2。结合新近的流体包裹体同位素分析结果和测年数据,认为成矿流体为地幔流体、岩浆流体和大气降水的混合产物,矿床成因类型为幔源流体参与成矿的造山型金矿床中成亚类。  相似文献   

10.
山东沂水地区紫苏花岗岩主要有 3种类型 ,分别为紫苏花岗闪长岩、紫苏石榴花岗闪长岩和紫苏奥长花岗岩。紫苏花岗岩中普遍存在有熔体交代结构 ,主要由残晶相矿物和结晶相矿物组成。对紫苏花岗岩及变质表壳中流体包裹体产状、成分的研究发现 ,富CO2 流体包裹体和富N2 流体包裹体均来自地幔深部。紫苏花岗岩的形成过程如下 :基性岩浆的底侵作用使本区经历了第一期麻粒岩相变质作用 ,地幔富CO2 流体包裹体的存在使系统a(H2 O)很低 (a(H2 O) =0 .1~ 0 .3) ,麻粒岩相变质作用没有产生熔融作用。幔源岩浆活动的逐渐停止 ,该区又经历了近等压降温的第二期麻粒岩相变质作用。此时 ,深源富CO2 流体作用减弱 ,水的活度增加 ,a(H2 O) =0 .6 5~ 0 .75 ,从而产生岩浆 ,新生岩浆对早期形成的变质矿物进行熔蚀交代作用 ,使早期形成的难熔变质矿物如紫苏辉石、石榴石、单斜辉石等呈残晶相 ,随着温度的降低岩浆基本在原地半原地结晶形成紫苏花岗岩。  相似文献   

11.
We investigate the inclusions hosted in peritectic garnet from metapelitic migmatites of the Kinzigite Formation (Ivrea Zone, NW Italy) to evaluate the starting composition of the anatectic melt and fluid regime during anatexis throughout the upper amphibolite facies, transition, and granulite facies zones. Inclusions have negative crystal shapes, sizes from 2 to 10 μm and are regularly distributed in the core of the garnet. Microstructural and micro‐Raman investigations indicate the presence of two types of inclusions: crystallized silicate melt inclusions (i.e., nanogranitoids, NI), and fluid inclusions (FI). Microstructural evidence suggests that FI and NI coexist in the same cluster and are primary (i.e., were trapped simultaneously during garnet growth). FI have similar compositions in the three zones and comprise variable proportions of CO2, CH4, and N2, commonly with siderite, pyrophyllite, and kaolinite, suggesting a COHN composition of the trapped fluid. The mineral assemblage in the NI contains K‐feldspar, plagioclase, quartz, biotite, muscovite, chlorite, graphite and, rarely, calcite. Polymorphs such as kumdykolite, cristobalite, tridymite, and less commonly kokchetavite, were also found. Rehomogenized NI from the different zones show that all the melts are leucogranitic but have slightly different compositions. In samples from the upper amphibolite facies, melts are less mafic (FeO + MgO = 2.0–3.4 wt%), contain 860–1700 ppm CO2 and reach the highest H2O contents (6.5–10 wt%). In the transition zone melts have intermediate H2O (4.8–8.5 wt%), CO2 (457–1534 ppm) and maficity (FeO + MgO = 2.3–3.9 wt%). In contrast, melts at granulite facies reach highest CaO, FeO + MgO (3.2–4.7 wt%), and CO2 (up to 2,400 ppm), with H2O contents comparable (5.4–8.3 wt%) to the other two zones. Our results represent the first clear evidence for carbonic fluid‐present melting in the Ivrea Zone. Anatexis of metapelites occurred through muscovite and biotite breakdown melting in the presence of a COH fluid, in a situation of fluid–melt immiscibility. The fluid is assumed to have been internally derived, produced initially by devolatilization of hydrous silicates in the graphitic protolith, then as a result of oxidation of carbon by consumption of Fe3+‐bearing biotite during melting. Variations in the compositions of the melts are interpreted to result from higher T of melting. The H2O contents of the melts throughout the three zones are higher than usually assumed for initial H2O contents of anatectic melts. The CO2 contents are highest at granulite facies, and show that carbon‐contents of crustal magmas are not negligible at high T. The activity of H2O of the fluid dissolved in granitic melts decreases with increasing metamorphic grade. Carbonic fluid‐present melting of the deep continental crust represents, together with hydrate‐breakdown melting reactions, an important process in the origin of crustal anatectic granitoids.  相似文献   

12.
Idiomorphic quartz crystals in topaz-bearing granite from the Salmi batholith contain primary inclusions of silicate melt and abundant mostly secondary aqueous fluid inclusions. Microthermometric measurements on melt inclusions give estimates for the granite solidus and liquidus of 640–680°C and 770–830°C, respectively. Using published solubility models for H2O in granitic melts and the obtained solidus/liquidus temperatures from melt inclusions, the initial water concentration of the magma is deduced to have been approximately 3 wt.% and the minimum pressure about 2 kbar. At this initial stage, volatile-undersaturation conditions of magma were assumed. These results indicate that the idiomorphic quartz crystals are magmatic in origin and thus real phenocrysts. During subsolidus cooling and fracturing of the granite, several generations of aqueous fluid inclusions were trapped into the quartz phenocrysts. The H2O inclusions have salinities and densities of 1–41 wt.% NaCl eq. and 0.53–1.18 g/cm3, respectively.  相似文献   

13.
徐九华  谢玉玲 《岩石学报》2007,23(1):117-124
Mantle xenoliths are common in the Cenozoic basalts of the Changbaishan District,Jilin Province,China.Sulfide assemblages in mantle minerals can be divided into three types:isolated sulfide grains,sulfide-meh inclusions and filling sulfides in fractures.Sulfide-meh inclusions occur as single-phase sulfides,sulfide-silicate melt,and CO_2-sulfide-silicate melt inclusions. Isolated sulfide grains are mainly composed of pyrrhotite,but cubanite was found occasionally.Sulfide-meh inclusions are mainly composed of pontlandite and MSS,with small amounts of chalcopyrite and talnakhite.The calculated distribution coefficient K_(D3)for lherzolite are similar to that of mean experimental value.The bulk sulfides in lherzolite were in equilibrium with the enclosing minerals, indicating immiscible sulfide melts captured in partial melting of upper mantle.Sulfide in fractures has higher Ni/Fe and(Fe Ni)/S than those of sulfide melt inclusions.They might represent later metasomatizing fluids in the mantle.Ni/Fe and(Fe Ni)/S increase from isolated grains,sulfide inclusions to sulfides in fractures.These changes were not only affected by temperature and pressure,hut by geochemistry of Ni,Fe and Cu,and sulfur fugacity as well.  相似文献   

14.
It is generally believed that the lithospheric mantle and the mantle transition zone are important carbon reservoirs. However, the location of carbon storage in Earth’s interior and the reasons for carbon enrichment remain unclear. In this study, we report CO2-rich olivine-hosted melt inclusions in the mantle xenoliths of late Cenozoic basalts from the Penglai area, Hainan Province, which may shed some light on the carbon enrichment process in the lithospheric mantle. We also present ...  相似文献   

15.
Garnet brought to the surface by late Miocene granitoids at La Galite Archipelago (Central Mediterranean, Tunisia) contains abundant primary melt and fluid inclusions. Microstructural observations and mineral chemistry define the host garnet as a peritectic phase produced by biotite incongruent melting at ~800 °C and 0.5 GPa, under fluid‐present conditions. The trapped melt is leucogranitic with an unexpected metaluminous and almost peralkaline character. Fluid inclusions are one phase at room temperature, and contain a CO2‐dominated fluid, with minor H2O, N2 and CH4. Siderite and an OH‐bearing phase were identified by Raman and IR spectroscopy within every analysed inclusion, and are interpreted as products of a post‐entrapment carbonation/hydration reaction between the fluid and the host during cooling. The fluid present during anatexis is therefore inferred to have been originally richer in both H2O and CO2. The production of anatectic melt with a metaluminous signature can be explained as the result of partial melting of relatively Al‐poor protoliths assisted by CO2‐rich fluids.  相似文献   

16.
山东昌乐第三纪玄武岩中产有刚玉巨晶,内含丰富的原生和假次生流体包裹体和熔融包裹体。流体包裹体可分为CO2单相包裹体、H2O-CO2两相和三相包裹体。熔融包裹体类型复杂,其中富流体相包裹体可分为含CO2收缩气泡两相熔融包裹体和气-液-固多相熔融包裹体。诸类包裹体主要赋含在刚玉晶核外的“主体”部分,以CO2单相流体包裹体和两相熔融包裹体最为发育,并且不同类型包裹体常密切伴生,表明它们形成时流体发生了不混溶作用:出现熔浆相(富含挥发分)、气相(CO2为主)和富水相(H2O-CO2为主)等多相体系。激光拉曼分析结果显示,各类包裹体中的气体组分主要是CO2,另有不等量的N2和H2S,据此划分为纯CO2、CO2-N2、CO2-H2S和CO2-N2-H2S等气体组合类型,没有发现O2、CH4和H2等组分。此外,拉曼分析也证实了流体包裹体和熔融包裹体中存在H2O。上述资料表明,昌乐地区深部流体以CO2为主,同时包含H2O、N2和H2S在内的多种组分,这些流体组分也是刚玉母浆系统的重要成分。  相似文献   

17.
18.
黑龙江乌拉嘎金矿是我国陆相火山岩区的重要金矿之一。构造位置处于古亚洲构造域与滨太平洋构造域交接复合部位的东北缘,矿体主要分布于团结沟斜长花岗斑岩接触带部位的隐爆角砾岩带和黑龙江群变质岩的层间裂隙中。斜长花岗斑岩的石英斑晶中发育3类包裹体:熔体包裹体、原生的L-V包裹体(及少量的L-V-S包裹体)和次生的L-V包裹体。玻璃质熔体包裹体相当于酸性殘浆的成分(SiO2达69.5%~73.8%),其捕获温度大于800℃。石英斑晶中次生L-V包裹体均一温度集中在210~350℃、盐度5%~7%NaCleqv,代表了次火山岩浆热液的特征,与黄铁矿-早期白色玉髓状石英阶段中Q1的包裹体均一温度范围很接近,而盐度略高于白色玉髓状石英Q1的。乌拉嘎金矿的金成矿可划分3个成矿阶段,发育盐水溶液包裹体:(1)黄铁矿-早期白色玉髓状石英阶段,包裹体均一温度为154~355℃,集中在190~330℃,盐度为1.3%~8.2%NaCleqv,密度为0.53~0.88g/cm3。(2)烟灰色玉髓状石英-多金属硫化物阶段,石英中包裹体均一温度为159~196℃,集中在170~190℃,盐度为2.2%~3.2%NaCleqv,密度0.79~0.92g/cm3。(3)碳酸盐-石英阶段,方解石中包裹体均一温度集中在170~270℃;盐度0.5%~2.9%NaCleqv。成矿流体以中低温、低盐度、贫CO2的盐水体系为特征,与国内外陆相火山-次火山热液矿床十分相似。石英斑晶中熔体、流体包裹体及其共存反映了次火山岩浆活动晚期,由硅酸盐熔体通过不混溶产生含矿的盐水溶液的可能,说明了金成矿与斑岩的成因联系,乌拉嘎金矿应该属于陆相火山-次火山活动有关的中低温浅成热液金矿床。  相似文献   

19.
Mosaic diamonds from the Zarnitsa kimberlite (Daldyn field, Yakutian diamondiferous province) are morphologicaly and structurally similar to dark gray mosaic diamonds of varieties V and VII found frequently in placers of the northeastern Siberian craton. However, although being similar in microstructure, the two groups of diamonds differ in formation mechanism: splitting of crystals in the case of placer diamonds (V and VII) and growth by geometric selection in the Zarnitsa kimberlite diamonds. Selective growth on originally polycrystalline substrates in the latter has produced radial micro structures with grains coarsening rimward from distinctly polycrystalline cores. Besides the formation mechanisms, diamonds of the two groups differ in origin of mineral inclusions, distribution of defects and nitrogen impurity, and carbon isotope composition. Unlike the placer diamonds of varieties V and VII, the analyzed crystals from the Zarnitsa kimberlite enclose peridotitic minerals (olivines and subcalcic Cr-bearing pyropes) and have total nitrogen contents common to natural kimberlitic diamonds (0 to 1761 ppm) and typical mantle carbon isotope compositions (-1.9 to -6.2%c 513C; -4.2%c on average). The distribution of defect centers in the Zarnitsa diamond samples fits the annealing model implying that nitrogen aggregation decreases from core to rim.  相似文献   

20.
Mineral inclusions in diamonds from the Sputnik kimberlite pipe, Yakutia   总被引:9,自引:0,他引:9  
The Sputnik kimberlite pipe is a small “satellite” of the larger Mir pipe in central Yakutia (Sakha), Russia. Study of 38 large diamonds (0.7-4.9 carats) showed that nine contain inclusions of the eclogitic paragenesis, while the remainder contain inclusions of the peridotitic paragenesis, or of uncertain paragenesis. The peridotitic inclusion suite comprises olivine, enstatite, Cr-diopside, chromite, Cr-pyrope garnet (both lherzolitic and harzburgitic), ilmenite, Ni-rich sulfide and a Ti-Cr-Fe-Mg-Sr-K phase of the lindsleyite-mathiasite (LIMA) series. The eclogitic inclusion suite comprises omphacite, garnet, Ni-poor sulfide, phlogopite and rutile. Peridotitic ilmenite inclusions have high Mg, Cr and Ni contents and high Nb/Zr ratios; they may be related to metasomatic ilmenites known from peridotite xenoliths in kimberlite. Eclogitic phlogopite is intergrown with omphacite, coexists with garnet, and has an unusually high TiO2 content. Comparison with inclusions in diamonds from Mir shows general similarities, but differences in details of trace-element patterns. Large compositional variations among inclusions of one phase (olivine, garnet, chromite) within single diamonds indicate that the chemical environment of diamond crystallisation changed rapidly relative to diamond growth rates in many cases. P-T conditions of formation were calculated from multiphase inclusions and from trace element geothermobarometry of single inclusions. The geotherm at the time of diamond formation was near a 35 mW/m2 conductive model; that is indistinguishable from the Paleozoic geotherm derived by studies of xenoliths and concentrate minerals from Mir. A range of Ni temperatures between garnet inclusions in single diamonds from both Mir and Sputnik suggests that many of the diamonds grew during thermal events affecting a relatively narrow depth range of the lithosphere, within the diamond stability field. The minor differences between inclusions in Mir and Sputnik may reflect lateral heterogeneity in the upper mantle.  相似文献   

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