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1.
以产在姚安富碱侵入岩体内外接触带上的姚安金矿床为对象,对成矿流体形成演化过程中的微量元素和S、C同位素地球化学进行了综合研究。研究结果表明,富碱侵入岩成岩过程中分异出的岩浆流体提供了姚安金矿床早期成矿作用所必需的成矿流体;从早期成矿阶段至晚期成矿,民矿流体经历了从以岩浆流体为主的流体体系至以大气降水为主的流体体系的转变。因此,钙碱性侵入岩成岩过程中可分异出成矿流体的过程,也存在于富碱浸入岩的成岩过程中。  相似文献   

2.
准噶尔盆地西北缘石炭—二叠系火山岩裂缝十分发育, 普遍充填方解石矿物。通过对钻井岩心裂缝类型划分、 方解石脉原生流体包裹体均一温度测试、 方解石地球化学数据测试与分析, 揭示了方解石脉成因。结果表明, 石炭—二叠系火山岩中的裂缝主要包括风化裂缝、 构造裂缝、 成岩裂缝和溶蚀裂缝。裂缝中方解石的原生流体包裹体均一温度分布为40℃~150℃, 变化范围较大, 具有低温、 高温及混合流体特征。方解石的碳、 氧同位素表明, 方解石的形成与大气淡水和埋藏流体有关, 锶同位素和锰元素进一步证实, 埋藏流体为深部热液流体或埋藏流体溶蚀了火山物质。准噶尔盆地西北缘石炭—二叠系火山岩受逆冲推覆构造和风化淋滤作用双重影响, 构造裂缝和风化裂缝彼此连通并沟通了深部热液与大气淡水。在火山岩裂缝中形成了兼具大气淡水与深部热液流体特征的方解石充填物。  相似文献   

3.
Summary The hydrothermal evolution of the Sengan geothermal area, Northern Honshu, was studied using fluid inclusion microthermometry. Sengan is one of the most active geothermal areas in Japan, and it is dominated by andesitic to dacitic volcanic rocks of Pliocene and Quaternary age. Fluid inclusions were studied in hydrothermal minerals (quartz, calcite, anhydrite, wairakite) and in fractured igneous quartz phenocrysts from core samples retrieved from five geothermal exploration wells, which penetrated Quaternary and Tertiary formations, and intrusive rocks in or around the calderas. A caldera-hosted hydrothermal system was heated by a shallow intrusion, which produced hypersaline fluids. During the early stages some heterogeneity in fluid composition occurred, but during peak activity of the hydrothermal system, the fluid was dominantly low-salinity, and most likely of meteoric origin. We have reconstructed, by means of fluid inclusion studies, the structure of an extinct hydrothermal system in a Pliocene caldera filled with ignimbrites, and of an active hydrothermal system which is now being heated under the northern slope of Yakeyama volcano. Based on inclusion data, the aqueous fluids that circulated in the hydrothermal system ranged from very low saline (0–7 wt.% NaCl equiv.) to hypersaline (up to 60 wt.% NaCl equiv.), with temperatures ranging from 130 to 400 °C.  相似文献   

4.
位于南岭成矿带南西部的鹿井矿床是华南热液型铀矿的典型代表.为查明其成矿流体来源、性质与演化以及成矿机制,开展了不同成矿阶段石英、萤石及方解石中流体包裹体的显微测温和不同阶段石英的氢?氧同位素分析.矿床地质特征表明成矿过程可划分为(I)粗晶石英+黄铁矿±绿泥石±绢云母、(II)沥青铀矿+硫化物+绿泥石+绢云母+暗灰色微晶...  相似文献   

5.
A multidisciplinary study, conducted over the carbonate platform deposits of the Liassic Calcari Grigi Group (Southern Alps), highlighted how the use of outcrop analogues can contribute to better define the distribution of dolomitic bodies related to fault networks, to characterize the petrophysical properties of the dolomitic sequence and unravel a complex diagenetic history. This study was carried out in the Asiago Plateau (southernmost part of the eastern Southern Alps, northern Italy) which provides excellent outcrops of the Jurassic Calcari Grigi Group. The dolomitization of the Jurassic sequence is variable in terms of stratigraphic extension and geographic distribution. In the studied localities the dolomitization is generally limited to the Mount Zugna Formation and is characterized by an undulatory front, with ‘sub‐vertical dolomitic chimneys’ along the major faults. Within this unit, and often associated with faults, stacked high‐porosity and permeability bed‐parallel dolomitic bodies are developed that show excellent petrophysical properties. The dolomitic intervals are characterized by pervasive unimodal and patchy polymodal dolomite crystals. Thin section, cathodoluminescence, isotopic and fluid inclusion analyses were used to constrain the paragenetic evolution of the sequence which is similar in all the studied localities. The first dolomitization stage is marked by zoned dolomite crystals with a dull luminescent core. The porosity is thought to have increased after this stage, with dark blue luminescent dolomite accompanied by the corrosion of older crystals. The appearance of saddle dolomite marks the onset of the porosity reduction stage, ending with the infilling of vugs and the remaining open pores with calcite cement. The diagenetic evolution locally stopped at the saddle dolomite stage with the complete occlusion of the remaining pores. Paragenetic and fluid‐inclusion data suggest an evolutionary trend of increasing temperatures and decreasing salinity toward brackish fluids responsible for dolomite and calcite precipitation. The integration of the available data seem to indicate that the diagenetic evolution of the study area is related to: (i) the interplay between evolving fluids (from marine to brackish); (ii) the burial of the sequence (increasing temperature); and (iii) the evolution of the hydrogeological system (fault and fracture network, fluid mixing). This complex paragenetic evolution is strongly linked to the evolution of the porosity framework that evolved from a good, widespread network in the early stages of the burial history to a confined system in the later stages due to reduction of porosity by the deposition of late calcite and dolomite cements.  相似文献   

6.
The Middle–Lower Yangtze River Valley is one of the most important metallogenic belts in China, hosting numerous Cu–Fe–Au–Mo deposits. The Taochong deposit is located in the northern part of the Fanchang iron ore district of the Middle–Lower Yangtze River metallogenic belt. The Fe-orebody is hosted by Middle Carboniferous to Lower Permian limestones. Skarns and Fe-orebodies occur as tabular bodies along interlayer-gliding faults, at some distance from the inferred granitic intrusions. Field evidence and petrographic observations indicate that the three stages of hydrothermal activity—the skarn, iron oxide (main mineralization stage), and carbonate stages—all contributed to the formation of the Taochong iron deposit. The skarn stage is characterized by the formation of garnet and pyroxene, with high-temperature, hypersaline hydrothermal fluids with isotopic compositions similar to those of typical magmatic fluids. These fluids were probably generated by the separation of brine from a silicate melt instead of the product of aqueous fluid immiscibility. The iron oxide stage coincides with the replacement of garnet and pyroxene by actinolite, chlorite, quartz, calcite and hematite. The hydrothermal fluids at this stage are represented by saline fluid inclusions that coexist with vapor-rich inclusions with anomalously low δD values (− 66‰ to − 94‰). The decrease in ore fluid δ18Owater with time and decreasing depth is consistent with the decreases in fluid salinity and temperature. The fluid δD values also show a decreasing trend with decreasing depth. Both fluid inclusion and stable isotopic data suggest that the ore fluid during the main period of mineralization was evolved by the boiling of various mixtures of magmatic brine and meteoric water. This process was probably induced by a drop in pressure from lithostatic to hydrostatic. The carbonate stage is represented by calcite veins that cut across the skarn and orebody, locally producing a dense stockwork. This observation indicates the veins formed during the waning stages of hydrothermal activity. The fluids from this stage are mainly represented by a variety of low-salinity fluid inclusions, as well as fewer high-salinity inclusions. These particular fluids have the lowest δ18Owater values (− 2.2‰ to 0.4‰) and a wide of range of δD values (− 40‰ to − 81‰), which indicate that they were originated from a mixture of residual fluids from the oxide stage, various amounts of meteoric water, and possibly condensed vapor. Low-temperature boiling probably occurred during this stage.We also discuss the reasons behind the anomalously low δD values in fluid inclusion water extracted by thermal decrepitation from quartz at high temperatures, and suggest that calcite data provide a possible benchmark for adjusting low δD values found in quartz intergrown with calcite.  相似文献   

7.
The Yangla deposit is an intrusion‐related Cu deposit in the Jinshajiang tectonic belt (eastern Sanjiang region, SW China). Despite extensive studies that have been conducted on this deposit, the relationship between the granitic magma and Cu mineralization is still unclear, and hence, the genesis is debated. To answer this question, we conducted an integrated study of mineralogy, fluid inclusions (FIs), and hydrogen and oxygen (H‐O) isotopes. Three mineralization stages were identified based on the ore textures, alteration zonation, and crosscutting relationships: (i) pre‐ore prograde skarn (stage I), with the garnet and pyroxene dominated by andradite and diopside, respectively; (ii) syn‐ore retrograde alteration (stage II), which is subdivided into the early syn‐ore stage (stage IIa) marked by retrograde hydrated mineral assemblages and significant Fe‐Cu‐Mo‐Pb‐Zn sulfide mineralization, and the late syn‐ore stage (stage IIb) featured by quartz‐calcite veins; and (iii) late supergene mineralization (stage III), which is characterized by secondary azurite and malachite. These results of mineralogy, FIs, and H‐O isotopes indicate that: (i) Cu mineralization has a close temporal, spatial, and genetic relationship with skarn alteration; (ii) the ore fluids were magmatic dominated with late‐stage meteoric water incursion; and (iii) Type‐S (halite‐bearing) and Type‐V (vapor‐rich) FIs coexisted in garnet and clinopyroxene of stage I, indicating that fluid boiling might have occurred during this stage. From stage I to stage IIa, the FI type transformed from Type‐S + Type‐V + Type‐L (liquid‐rich) to Type‐V + Type‐L with the conduct of mineralization and was accompanied by the disappearance of Type‐S, and homogenization temperature and salinity also tended to decrease dramatically, which may be caused by the deposition of skarn minerals. At stage IIa, boiling of the ore fluids still continued due to the change from lithostatic to hydrostatic pressure, which triggered the precipitation of abundant quartz‐Cu‐Mo‐Fe sulfides. Furthermore, fluid mixing between a high‐temperature magmatic fluid and a low‐temperature meteoric water might cause a considerable drop in temperature and the deposition of Cu‐bearing quartz/calcite veins during stage IIb. Hence, we consider the Yangla deposit to be of a skarn type, genetically related to the Mesozoic magmatism in the Sanjiang region.  相似文献   

8.
The coastal hard rock with a thickness of over 5 m and a distribution area of nearly 200 ha in the Haishan Island,south China,has long drawn researchers' attention.However,there were controversies over its formation and classification,and these controversies in turn lead to the dispute of sea level changes and coastal uplift-subsidence of this area.To investigate its diagenesis and evolution,petrographic analysis,elemental geochemistry,isotopic analysis,and radiocarbon dating were used in the present stu...  相似文献   

9.
The coastal hard rock with a thickness of over 5 m and a distribution area of nearly 200 ha in the Haishan Island, south China, has long drawn researchers’ attention. However, there were controversies over its formation and classification, and these controversies in turn lead to the dispute of sea level changes and coastal uplift-subsidence of this area. To investigate its diagenesis and evolution, petrographic analysis, elemental geochemistry, isotopic analysis, and radiocarbon dating were used in the present study. Radiocarbon dating indicates that the deposition of the Haishan Coquinite commenced in the mid Holocene and lasted to ~600 a B.P. Petrographic analysis shows that the Haishan Coquinite is cemented by low-Mg calcite, indicating that the cementation occurred in a meteoric environment. The elemental geochemistry and isotopic values demonstrate that the coquinite suffered strong leaching, which was thought to be responsible for the meteoric cementation of the coquinite. According to these results, the diagenesis of the coquinite is revealed: deposition of the Haishan Coquinite commenced in the mid Holocene in a shoal environment, initial cementation occurred and cement may be high-Mg calcite or aragonite; latterly the coquinite exposed to meteoric environment as a result of lowering of relative sea level, and the cement altered to low-Mg, which took the morphologies of bladed calcite rim and equant spar. A four-stage evolution model is proposed: (1) deposition stage, (2) initial cementation, (3) exposure to and cementation in meteoric environment, and (4) erosion stage. The published reports indicate that the hard rock should be designated as coquinite. Based on these studies, mid-Holocene sea level in this area was discussed, and the Haishan Island was proposed to uplift with a rate of ~5 mm/a in the last ~600 a.  相似文献   

10.
陆内碰撞和流体作用都是当前地球科学的前沿领域,但陆内碰撞体制流体作用以及有关成矿作用的研究仍很薄弱。文章以陆内碰撞成岩成矿模式为基础,通过理论分析,建立了陆内碰撞体制流体作用的模式,即在陆内俯冲体制中,随板片俯冲深度的增加,依次产生改造流体、变质流体和岩浆流体,所产生的流体在空间上具有分带性,并造成岩石、元素、矿化蚀变的成带规律分布;陆内俯冲的早期挤压阶段的流体作用以深部物质分泌的上升流体(改造、变质和部分熔融)为主,晚期伸展阶段以浅层下渗流体(来自大气降水)循环为主,中期由挤压向伸展的转变阶段为深分泌上升流体与浅层下渗流体的混合作用。为检验模式的科学性,选择典型的陆内碰撞带——东秦岭作为实例解剖,发现该区的陆内碰撞作用与金矿床等的成矿作用在时间、空间、地质地球化学特征等方面都十分吻合,且与理论推导的陆内俯冲体制的流体作用规律一致。对若干典型矿床成矿流体的氢同位素研究表明,成矿流体的性质、来源和演变特征等与理论推导的陆内碰撞体制流体作用规律完全符合。  相似文献   

11.
Abstract: The Daejang mine is located within the Cretaceous Gyeongsang basin. Mineral paragenesis can be divided into four stages (stages I, II, III and IV) by major tectonic fracturing. Stages I, III and IV are economically barren. Stage II, at which the precipitation of major ore minerals occurred, is further divided into three substages with paragenetic time based on minor fractures and discernible mineral assemblages: substage IIa, marked by deposition of quartz and Fe–sulfides; substage IIb, by introduction of base-metal sulfides within carbonates and some quartz; substage IIc, by quartz and carbonates with various sulfosalts. Fluid inclusion data indicate a complex geochemical evolution of hydrothermal fluids. Both CO2–rich and H2O–rich fluids were trapped in fluid inclusions at stage I and substage IIa. It is suggested that a compositionally heterogeneous fluid was formed by fluid boiling and CO2 immiscibility at temperatures of about 400° to 300°C. Composite lodes of base-metal sul–fides, carbonates and quartz at substage IIb were deposited in open spaces created by fracturing. The fracturing event prompted rapid decreases in pressure and temperature of residual fluids and resulted in retrograde fluid boiling at about 200 bars and 300°–250°C during substage IIb. The progressive loss of CO2 by CO2 effervescence and retrograde boiling from substage IIa and IIb fluids resulted in pH increase and related increase in carbonate activity, causing deposition of abundant carbonates. The change in pH also caused the decrease of stability of hydrogen sulfide with Cu, Zn and Pb chloride complexes (as main transporting agents at Daejang) and resulted in the pricipitation of base-metal minerals. Deposition of Ag– and Sb-bearing sul–fides and sulfosalts of substage IIc occurred at temperatures of about 250° to 150°C from a dominantly aqueous fluid with low salinity (down to 3. 0 equiv. wt % NaCl). At this substage, aqueous fluid formed by mixing with cooler and less saline meteoric groundwater. There is a systematic decrease in caculated δ18Owater values with the mineralization stage (and decreasing temperature) in the Daejang hydrothermal system, from values of about 11% for stage I, through about 4% for stages II and III, to about –3 per mil for stage IV. The result of stable isotope and fluid inclusion studies are interpreted to indicate progressive less evolved and/or unexchanged meteoric water influx of an early hydrothermal system formed by highly evolved meteoric waters.  相似文献   

12.
The Baizhangyan skarn‐porphyry type W–Mo deposit is located in a newly defined Mo–W–Pb–Zn metallogenic belt, which is in the south of Middle‐Lower Yangtze Valley Cu–Fe–Au polymetallic metallogenic belt in SE China. The W–Mo orebodies occur mainly within the contact zone between fine‐grained granite and Sinian limestone strata. There are two types of W–Mo mineralization: major skarn W–Mo mineralization and minor granite‐hosted disseminated Mo mineralization which was traced by drilling at depth. Eight molybdenite samples from Mo‐bearing ores yield Re–Os dates that overlap within analytical error, with a weighted average age of 134.1 ± 2.2 Ma. These dates are in close agreement with SIMS U–Pb concordant zircon age for fine‐grained granite at 133.3 ± 1.3 Ma, indicating that crystallization of the granite and hydrothermal molybdenite formation were coeval and likely cogenetic. The Baizhangyan W–Mo deposit formed in the Early Cretaceous extensional tectonic setting at the Middle‐Lower Yangtze Valley metallogenic belt and the Jaingnan Ancient Continent. Based on mineral compositions and crosscutting relationships of veinlets, hydrothermal alteration and mineralization, the ore mineral paragenesis of the Baizhangyan deposit is divided into four stages: skarn stage (I), oxide stage (II), sulfide stage (III), and carbonate stage (IV). Fluid inclusions in garnet, scheelite, quartz and calcite from W–Mo ores are mainly aqueous‐rich (L + V) type inclusions. Following garnet deposition at stage I, the high‐temperature fluids gave way to progressively cooler, more dilute fluids associated with tungsten–molybdenite–base metal sulfide deposition (stage II and stage III) (162–360°C, 2.7–13.2 wt % NaCl equivalent) and carbonate deposition (stage IV) (137–190°C, 0.9–5 wt % NaCl equiv.). Hydrogen‐oxygen isotope data from minerals of different stages suggest that the ore‐forming fluids consisted of magmatic water, mixed in various proportions with meteoric water. From stage I to stage IV, there is a systematic decrease in the homogenization temperature of the fluid‐inclusion fluids and calculated δ18O values of the fluids. These suggest that increasing involvement of formation water or meteoric water during the fluid ascent resulted in successive deposition of scheelite and molybdenite at Baizhangyan.  相似文献   

13.
The contact aureole developed in siliceous carbonates surrounding the Beinn an Dubhaich granite, Skye, shows textural and stable isotope evidence for infiltration of aqueous fluids during both prograde and retrograde metamorphism. Strongly depleted isotope compositions of reaction-product calcite correlate with high silica and fluorine contents, demonstrating a strong link between isotopic alteration and metasomatism by fluids with a significant magmatic component, even at the margins of the aureole. The oxygen and carbon isotope compositions of the carbonates form a linear cluster with a positive slope of about five, consistent with the depletion of isotope compositions by the infiltration of magmatic and/or meteoric fluids. Rayleigh fractionation during devolatilization played a minor role in determining the final isotope composition. Stable isotope compositions of coexisting calcite–dolomite pairs show varying amounts of isotopic disequilibrium, which correlate with the inferred fluid infiltration mechanism. Much of the calcite in dolostones is the product of infiltration-driven reactions along fractures, and is greatly depleted isotopically relative to the host dolomite, especially at talc grade. At higher grades the calcite–dolomite fractionation is smaller, probably due to both increased fluid–rock interaction and a greater tendency for fluid infiltration to be pervasive on the grain-scale. Limestones generally show near-equilibrium fractionation of oxygen and carbon owing to the overwhelming compositional influence of the host calcite. Veins formed during late-stage hydrothermal circulation have strongly 18O-depleted compositions relative to the host rock. No small-scale spatial patterns to the isotopic depletion were observed, but the extent of fluid infiltration was greatest in the west of the aureole. Fluid infiltration was clearly highly heterogeneous, with no evidence of a consistent flow direction. It is not possible to determine fluid fluxes or flow directions from one-dimensional flow models based on continuum flow in the Beinn an Dubhaich aureole.  相似文献   

14.
The origin of secondary calcite-silica minerals in primary and secondary porosity of the host Miocene tuffs at Yucca Mountain has been hotly debated during the last decade. Proponents of a high-level nuclear waste repository beneath Yucca Mountain have interpreted the secondary minerals to have formed from cool, descending meteoric fluids in the vadose zone; critics, citing the presence of two-phase fluid inclusions, argued that the minerals could only have formed in the phreatic zone from ascending hydrothermal fluids. Understanding the origin, temperature, and timing of these minerals is critical in characterizing geologically recent fluid flux at the site, and has significant implications to whether waste should be stored at Yucca Mountain.Petrographic and paragenetic studies of 155 samples collected from the Exploratory Studies Facility (ESF) and repository block cross drift (ECRB) tunnels indicate that heterogeneously distributed calcite with lesser chalcedony, quartz, opal, and fluorite comprise the oldest secondary minerals. These are typically overgrown by intermediate-aged calcite, often exhibiting distinctive bladed habits. The youngest event recorded across the site is the deposition of Mg-enriched (up to ∼1 wt%) and depleted, growth-zoned calcite intergrown with U-enriched opal. The cyclical variation in Mg enrichment and depletion is probably related to climate changes that have occurred during the last few million years. The distribution of secondary minerals is consistent with precipitation in the vadose zone.Fluid inclusion petrography of sections from the 155 samples determined that 96% of the fluid inclusion assemblages (FIAs) contained liquid-only inclusions that formed at ambient temperatures (<35°C). However, 50% of the samples (n = 78) contained relatively rare FIA that contain both liquid-only and liquid plus vapor inclusions (herein termed two-phase FIAs) that formed at temperatures above 35°C. Virtually all of these two-phase FIAs occur in paragenetically old calcite; rare two-phase inclusion assemblages were also observed in early fluorite and quartz, and early-intermediate calcite. Homogenization temperatures (≡ trapping temperatures) across Yucca Mountain are generally 45 to 60°C, but higher temperatures reaching 83°C were recorded in calcite from the north portal and ramp of the ESF. Cooler temperatures of ∼35 to 45°C were recorded in the intensely fractured zone. Multiple populations of two-phase FIAs from lithophysal cavities in the ESF and ECRB cross drift indicate early fluid cooling with time from temperatures >45°C in early calcite, to <35 to 45°C in paragenetically younger calcite. Freezing point depressions range from −0.2 to −1.6°C, indicating trapping of a low salinity fluid. The majority of intermediate calcite and all outermost Mg-enriched calcite contains rare all-liquid inclusions and formed from ambient temperature (<35°C) fluids.Carbon and oxygen isotope data reveal a consistent trend of decreasing δ13C (from 9.5 to −8.5‰) and increasing δ18O (from 5.2 to 22.1‰) values from paragenetically early calcite to Mg-enriched growth-zoned calcite. Depleted δD values (−131 to −90‰) of inclusion fluids from intermediate and the youngest Mg-enriched calcite indicate derivation from surface meteoric fluids. Recalculation of δ18OH2O values of −12 to −10‰ is consistent with derivation from paleometeoric fluids.Results of integrated U-Pb dating (opal and chalcedony) and fluid inclusion microthermometry indicate that two-phase FIAs that trapped fluids of >50°C are older than 6.29 ± 0.30 Ma. Two-phase FIAs in paragenetically later calcite, which formed from fluids of 35 to 45°C, are older than 5.32 ± 0.02 Ma. There is no evidence for trapping of fluids with elevated temperatures during the past 5.32 my. The youngest Mg-enriched calcite intergrown with opal began to precipitate between about 1.9 to 2.9 Ma and has continued to precipitate within the past half million years. The presence of liquid-only inclusions and the consistent occurrence of Mg-enriched calcite and opal as the youngest event indicate a minor, but chemically distinct, ambient temperature (<35°C) fluid flux during the past 2 to 3 my.  相似文献   

15.
安徽铜陵铜官山铜矿田是中国长江中、下游铁、铜、硫、金成矿带中著名的夕卡岩型矿床.小铜官山铜矿床位于安徽铜陵铜官山矿田,侵入岩体为铜官山石英二长闪长岩.成矿过程包括夕卡岩阶段、石英-硫化物阶段和石英-碳酸盐阶段3个主要成矿阶段.笔者通过对小铜官山铜矿床的氢、氧、碳、硫、硅同位素组成和稀土元素地球化学特征研究,探讨成矿溶液中水、硅和硫的来源以及成矿溶液的演化问题.研究表明,成矿热液早期以岩浆热液为主,随着成矿过程的进行,加入的大气降水比重越来越大,到晚期可能主要以大气降水为主.硫的来源主要有两个方面,即地层和岩浆热液,但以后者为主.硅具深部岩浆或岩浆热液水来源的特点.稀土元素球粒陨石标准化组成模式为右倾型,夕卡岩、矿石的稀土配分曲线类似于铜官山岩体石英二长闪长岩,故认为形成本区的夕卡岩型矿床的热液流体主要来源于闪长质熔体.  相似文献   

16.
红岭铅锌矿是内蒙古东南部的大型代表性矿床之一.目前,对该矿床成矿流体地球化学特征、性质及演化问题尚缺乏系统研究.对其展开了系统的流体包裹体研究.结果表明,矿区矽卡岩期Ⅰ阶段石榴石中发育含NaCl子矿物三相(SL)、气相-富气相(LV)及气液两相(VL)3种类型的原生流体包裹体,Ⅱ阶段中石英颗粒主要发育LV和VL两种类型原生流体包裹体,测温结果表明矽卡岩期成矿流体属中-高温、高盐度的不均匀NaCl-H2O体系热液,在成矿过程中发生过沸腾作用而导致铅、锌、铜等有用元素沉淀富集.石英-硫化物期Ⅲ→Ⅵ阶段中矿物均主要发育较单一的VL型包裹体,其中Ⅲ阶段热液均一温度较矽卡岩期明显降低,而盐度没有明显变化;Ⅳ阶段成矿流体均一温度明显增高、盐度明显降低,反映了有新的高温、低盐度体系热液的加入;而Ⅴ→Ⅵ阶段成矿流体均一温度及盐度逐渐降低,体现了一种不断与外来天水混合的演变趋势;整体上看,石英-硫化物期流体为简单的中-低温、低盐度NaCl-H2O体系热液.流体包裹体C、H、O同位素研究表明,红岭矿床矽卡岩期Ⅱ阶段成矿流体以岩浆水为主;石英-硫化物期成矿流体源自大气降水与岩浆水的混合流体,晚阶段逐渐演化为以大气降水为主.矿床S、Pb同位素研究表明,区内成矿物质具深源特点.   相似文献   

17.
新疆阿尔泰巴特巴克布拉克铁矿床成矿作用研究   总被引:2,自引:0,他引:2       下载免费PDF全文
巴特巴克布拉克铁矿床赋存于上志留-下泥盆统康布铁堡组变质火山-沉积岩系中, 近矿围岩为石榴子石矽卡岩、角闪斜长变粒岩和浅粒岩。矿体总体顺层分布, 呈似层状、透镜状及不规则状, 空间上与矽卡岩密切相关。流体包裹体研究表明, 矽卡岩阶段形成的石榴子石中发育纯气体包裹体、气体包裹体、液体包裹体、含子矿物包裹体及熔融包裹体; 退化蚀变阶段发育液体包裹体和少量气体包裹体; 石英-硫化物阶段主要发育液体包裹体、含液体CO2的三相包裹体及少量纯气体包裹体、气体包裹体和含子矿物包裹体。矽卡岩阶段均一温度变化为217 ℃~499 ℃, 在255 ℃出现峰值, 盐度(NaCleq)变化为8.68%~22.65%; 退化蚀变阶段均一温度变化为181 ℃~432 ℃, 在225 ℃出现峰值, 盐度变化为12.85%~22.65%; 石英-硫化物阶段均一温度变化为140 ℃~482 ℃, 在155 ℃出现峰值, 盐度变化为0.18%~42.40%。石榴子石、石英和方解石的 δ18 OSMOW 变化为1.8‰~7.1‰, δ18ΟΗ2Ο为 -4.79‰~4.57‰, δDSMOW 为 -128‰~-84‰, 表明矽卡岩阶段成矿流体主要为岩浆水, 混合少量大气降水; 石英-硫化物阶段大气降水所占比例明显增加。方解石δ13 CV-PDB 变化为 -3.2‰~-2.0‰, 表明流体中的碳来自深部或地幔。  相似文献   

18.
大青山逆冲断层带内热液脉体十分发育,按其产状可划分为充填脉和边缘脉。根据形成时间主要划分为3期:早期石英脉、中期石英脉和晚期方解石脉。早期石英脉中流体包裹体类型较为复杂,见有气液两相、含CO2三相、纯CO2及少量单液相等4种类型原生包裹体,分析表明流体主要来源于地壳深部或上地幔。中期石英脉中主要发育气液两相包裹体和少量单液相包裹体,流体主要来源于大气降水,并且有少量岩浆热液混入。晚期方解石脉内仅含有气液两相包裹体及少量的单液相包体,流体主要来源于层间建造水。根据逆冲变形事件期次、时间,结合热液脉体形成深度数据,确定了大青山逆冲推覆体系变形演化历史:印支期逆冲推覆事件发生在地壳7~8 km深度,燕山中期逆冲推覆事件发生在3~6 km范围内,而燕山晚期逆冲推覆事件发生近地表2 km范围内。  相似文献   

19.
MUCHEZ  NIELSEN  SINTUBIN  & LAGROU 《Sedimentology》1998,45(5):845-854
Two calcite cements, filling karst cavities and replacing Lower Carboniferous limestones at the Variscan Front Thrust, were precipitated after mid-Jurassic Cimmerian uplift and subsequent erosion but before late Cretaceous strike-slip movement. The first calcite (stage A) is nonferroan and crystals are coated by hematite and/or goethite. These minerals also occur as inclusions along growth zones. The calcite lattice contains < 0·07 mol.% Fe, but Mn concentrations can be as high as 0·72 mol.% in bright yellow luminescent zones. Primary, originally one-phase, all-liquid, aqueous inclusions have a final melting temperature between ?0·2° and +0·2 °C, indicating a meteoric origin of the ambient water. The δ13C and δ18O values of the calcites are between ?7·3‰ and ?6·3‰, ?7·8‰ and ?5·5‰ on the Vienna PeeDee Belemnite (VPDB) scale, respectively. The second calcite (stage B) consists of ferroan (0·13–0·84 mol.% Fe) blocky crystals with Mn concentrations between 0·34 and 0·87 mol.%. Primary, single-phase aqueous fluid inclusions indicate precipitation from a meteoric fluid below 50 °C . The δ13C values of stage B calcites vary between ?7·3‰ and ?2·1‰ VPDB and the δ18O values between ?7·9‰ and ?7·2‰ VPDB. A precipitation temperature below 50 °C for the stage A calcites and the presence of iron oxide/hydroxide inclusions in the crystals indicate near-surface precipitation conditions. Within this setting, the geochemistry of the nonferroan stage A calcites reflects precipitation under oxic to suboxic conditions. The ferroan stage B calcites precipitated in a reducing environment. The evolution from the stage A to stage B calcites and the associated geochemical changes are interpreted to be related to the change from semiarid to humid conditions in western Europe during late Jurassic–Cretaceous times. A change in humidity can explain the evolution of groundwater from oxic/suboxic to reducing conditions during calcite precipitation. The typically higher δ13C values of the stage B compared to the stage A calcites can be explained by a smaller contribution of carbon derived from soil-zone processes than from carbonate dissolution in the groundwater under humid conditions. The small shift to lower δ18O between stage A and B calcites may be caused by a higher precipitation temperature or a decrease in the δ18O value of the meteoric water. This decrease could have been caused by a change in the source of the air masses or by an increase in the amount of rainfall during the early mid-Cretaceous. Although the latter interpretation is preferred, it cannot be proven.  相似文献   

20.
目前含油气砂岩中粒间孔隙是原生孔隙还是次生孔隙的认识仍不一致,而对星点状方解石胶结与溶解的识别能够有效地查明粒间孔隙的类型。文章通过铸体薄片细致地观察雅布赖盆地新河组砂岩中的微观现象,以成岩环境演化和成岩序列分析为主线,重视方解石胶结物的赋存状态与物质来源和溶蚀流体来源的配置关系,精细解剖微观现象,从而弄清楚星点状方解石的成因,进而查明砂岩的粒间孔隙类型和储集空间类型。结果表明,粒间孔隙中的星点状方解石是成岩早期浸染状方解石胶结物的溶蚀残余,溶蚀流体为成岩中期的有机酸流体,溶蚀类型为一致性溶解,形成的粒间孔隙为次生孔隙。鉴于此,雅布赖盆地新河组砂岩的储集空间由次生粒间孔隙和次生粒内孔隙(长石、岩屑、方解石胶结物的溶蚀孔隙)组成。   相似文献   

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