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1.
Metamorphic conditions within arenaceous, calcareous and argillaceous supracrustal rocks of the Magondi Mobile Belt (Zimbabwe) range from greenschist to granulite facies. Within the high-grade segment, basement gneisses of early Proterozoic age and argillaceous rocks of the Mid-Proterozoic Piriwiri Group are intruded by charnockites and enderbites. Metamorphic mineral assemblages and thermobarometric data for enderbitic granulites of Nyaodza show temperatures of 700–800°C and pressures of 5–7 kbar for the peak of granulite-facies metamorphism. Microthermometry and Raman microspectroscopy reveal that CO2, associated with minor N2, has been the dominant fluid phase during granulite-facies metamorphism. The chronology of the CO2 inclusions and the development of microtextures and mineral assemblages in the enderbites indicates that isolated negative crystal shaped CO2 inclusions in quartz and plagioclase porphyroclasts entrap syn-metamorphic fluids of medium-high densities (0.88–0.90 g/cm3). Lower density (0.71–0.77 g/cm3) CO2 inclusions in trails and clusters within the same minerals were formed from local re-equilibration and re-entrapment of the former (near-) peak granulitic CO2 inclusions. As in many other granulites, syn-metamorphic CO2 is associated with intrusives emplaced near the peak of metamorphism.  相似文献   

2.
Jan-Marten Huizenga 《Lithos》2001,55(1-4):101-114
H2O, CO2, CH4, CO, H2 and O2 are the most important species in crustal fluids. The composition of these C–O–H fluids can be calculated if the pressure, temperature, carbon activity, and either the oxygen fugacity or the atomic H/O ratio of the fluid is known. The calculation methods are discussed and calculation results are illustrated with isobaric TXi, PT, and isobaric–isothermal ternary C–O–H diagrams. Fluid inclusion compositions, in particular, the XCO2/(XCO2+XCH4) ratio, can be used for C–O–H model calculations. However, care should be taken about possible post-entrapment changes, which may have modified the chemical composition of the fluid inclusion.  相似文献   

3.
Fluid inclusion studies in rocks from the Lower Proterozoic granulites from western Hoggar (Algeria) provide new evidence for the hypothesis that a CO2-rich, H2O-poor fluid was present during the high-grade metamorphism. CO2 inclusions represent the main fluid trapped in the Ihouhaouene ultrahigh-temperature (over 1000 °C) and high-pressure (10 to 14 kbar) granulites. The microthermometric and Raman microspectrometric measurements indicate that the carbonic fluid is mainly composed of CO2 with minor amounts of CH4 and N2 detected in some inclusions (< 4 mol% CH4). Carbonic fluid densities range from 1.18 to 0.57 g/cm3. The highest densities are recorded in superdense carbonic inclusions presenting evidence of the earliest trapping and they correspond to the fluid densities expected for the P–T conditions of the peak of metamorphism in the area previously determined from mineral geothermobarometers. Lower densities of carbonic fluids mainly result from the reequilibration of earlier trapped fluid inclusions during retrograde metamorphism and final uplift of the metamorphic terrane, but a new influx of carbonic fluids during the retrograde event remains possible. Carbonic fluids can be produced in situ from decarbonation reactions in interlayered impure marbles during the prograde event or derived from CO2 flushing from underlying basic intrusions. The aqueous fluids present large variations of composition (0.5 to 30 wt.% NaCl equivalent) and densities (1.16 to 0.57 g/cm3). They clearly correspond to post-metamorphic fluids because they mainly occur along microfractures, they do not show any evidence of immiscibility with the carbonic fluids and mixed aquo-carbonic inclusions have not been observed. The percolation of aqueous fluids is related to the Pan-African tectonometamorphic event.  相似文献   

4.
A detailed fluid inclusion study has been carried out on the hydrocarbon-bearing fluids found in the peralkaline complex, Lovozero. Petrographic, microthermometric, laser Raman and bulk gas data are presented and discussed in context with previously published data from Lovozero and similar hydrocarbon-bearing alkaline complexes in order to further understand the processes which have generated these hydrocarbons. CH4-dominated inclusions have been identified in all Lovozero samples. They occur predominantly as secondary inclusions trapped along cleavage planes and healed fractures together with rare H2O-dominant inclusions. They are consistently observed in close association with either arfvedsonite crystals, partially replaced by aegirine, aegirine crystals or areas of zeolitization. The majority of inclusions consist of a low-density fluid with CH4 homogenisation temperatures between −25 and −120 °C. Those in near-surface hand specimens contain CH4+H2 (up to 40 mol%)±higher hydrocarbons. However, inclusions in borehole samples contain CH4+higher hydrocarbons±H2 indicating that, at depth, higher hydrocarbons are more likely to form. Estimated entrapment temperatures and pressures for these inclusions are 350 °C and 0.2–0.7 kbar. A population of high-density, liquid, CH4-dominant inclusions have also been recorded, mainly in the borehole samples, homogenising between −78 and −99 °C. These consist of pure CH4, trapped between 1.2 and 2.1 kbar and may represent an early CH4-bearing fluid overprinted by the low-density population. The microthermometric and laser Raman data are in agreement with bulk gas data, which have recorded significant concentrations of H2 and higher hydrocarbons up to C6H12 in these samples. These data, combined with published isotopic data for the gases CH4, C2H6, H2, He and Ar indicate that these hydrocarbons have an abiogenic, crustal origin and were generated during postmagmatic, low temperature, alteration reactions of the mineral assemblage. This would suggest that these data favour a model for formation of hydrocarbons through Fischer–Tropsch type reactions involving an early CO2-rich fluid and H2 derived from alteration reactions. This is in contrast to the late-magmatic model suggested for the formation of hydrocarbons in the similar peralkaline intrusion, Ilímaussaq, at temperatures between 400 and 500 °C.  相似文献   

5.
Minor granulites (believed to be pre-Triassic), surrounded by abundant amphibolite-facies orthogneiss, occur in the same region as the well-documented Triassic high- and ultrahigh-pressure (HP and UHP) eclogites in the Dabie–Sulu terranes, eastern China. Moreover, some eclogites and garnet clinopyroxenites have been metamorphosed at granulite- to amphibolite-facies conditions during exhumation. Granulitized HP eclogites/garnet clinopyroxenites at Huangweihe and Baizhangyan record estimated eclogite-facies metamorphic conditions of 775–805 °C and ≥15 kbar, followed by granulite- to amphibolite-facies overprint of ca. 750–800 °C and 6–11 kbar. The presence of (Na, Ca, Ba, Sr)-feldspars in garnet and omphacite corresponds to amphibolite-facies conditions. Metamorphic mineral assemblages and PT estimates for felsic granulite at Huangtuling and mafic granulite at Huilanshan indicate peak conditions of 850 °C and 12 kbar for the granulite-facies metamorphism and 700 °C and 6 kbar for amphibolite-facies retrograde metamorphism. Cordierite–orthopyroxene and ferropargasite–plagioclase coronas and symplectites around garnet record a strong, rapid decompression, possibly contemporaneous with the uplift of neighbouring HP/UHP eclogites.

Carbonic fluid (CO2-rich) inclusions are predominant in both HP granulites and granulitized HP/UHP eclogites/garnet clinopyroxenites. They have low densities, having been reset during decompression. Minor amounts of CH4 and/or N2 as well as carbonate are present. In the granulitized HP/UHP eclogites/garnet clinopyroxenites, early fluids are high-salinity brines with minor N2, whereas low-salinity fluids formed during retrogression. Syn-granulite-facies carbonic fluid inclusions occur either in quartz rods in clinopyroxene (granulitized HP garnet clinopyxeronite) or in quartz blebs in garnet and quartz matrices (UHP eclogite). For HP granulites, a limited number of primary CO2 and mixed H2O–CO2(liquid) inclusions have also been observed in undeformed quartz inclusions within garnet, orthopyroxene, and plagioclase which contain abundant, low-density CO2±carbonate inclusions. It is suggested that the primary fluid in the HP granulites was high-density CO2, mixed with a significant quantity of water. The water was consumed by retrograde metamorphic mineral reactions and may also have been responsible for metasomatic reactions (“giant myrmekites”) occurring at quartz–feldspar boundaries. Compared with the UHP eclogites in this region, the granulites were exhumed in the presence of massive, externally derived carbonic fluids and subsequently limited low-salinity aqueous fluids, probably derived from the surrounding gneisses.  相似文献   


6.
In this paper the first fluid-inclusion data are presented from Late Archaean Scourian granulites of the Lewisian complex of mainland northwest Scotland. Pure CO2 or CO2-dominated fluid inclusions are moderately abundant in pristine granulites. These inclusions show homogenization temperatures ranging from − 54 to + 10 °C with a very prominent histogram peak at − 16 to − 32 °C. Isochores corresponding to this main histogram peak agree with P-T estimates for granulite-facies recrystallization during the Badcallian (750–800 °C, 7–8 kbar) as well as with Inverian P-T conditions (550–600 °C, 5 kbar). The maximum densities encountered could correspond to fluids trapped during an early, higher P-T phase of the Badcallian metamorphism (900–1000 °C, 11–12 kbar). Homogenization temperatures substantially higher than the main histogram peak may represent Laxfordian reworking (≤ 500 °C, < 4 kbar). In the pristine granulites, aqueous fluid inclusions are of very subordinate importance and occur only along late secondary healed fractures. In rocks which have been retrograded to amphibolite facies from Inverian and/or Laxfordian shear zones, CO2 inclusions are conspicuously absent; only secondary aqueous inclusions are present, presumably related to post-granulite hydration processes. These data illustrate the importance of CO2-rich fluids for the petrogenesis of Late Archaean granulites, and demonstrate that early fluid inclusions may survive subsequent metamorphic processes as long as no new fluid is introduced into the system.  相似文献   

7.
Three types of fluid inclusions have been identified in olivine porphyroclasts in the spinel harzburgite and lherzolite xenoliths from Tenerife: pure CO2 (Type A); carbonate-rich CO2–SO2 mixtures (Type B); and polyphase inclusions dominated by silicate glass±fluid±sp±silicate±sulfide±carbonate (Type C). Type A inclusions commonly exhibit a “coating” (a few microns thick) consisting of an aggregate of a platy, hydrous Mg–Fe–Si phase, most likely talc, together with very small amounts of halite, dolomite and other phases. Larger crystals (e.g. (Na,K)Cl, dolomite, spinel, sulfide and phlogopite) may be found on either side of the “coating”, towards the wall of the host mineral or towards the inclusion center. These different fluids were formed through the immiscible separations and fluid–wall-rock reactions from a common, volatile-rich, siliceous, alkaline carbonatite melt infiltrating the upper mantle beneath the Tenerife. First, the original siliceous carbonatite melt is separated from a mixed CO2–H2O–NaCl fluid and a silicate/silicocarbonatite melt (preserved in Type A inclusions). The reaction of the carbonaceous silicate melt with the wall-rock minerals gave rise to large poikilitic orthopyroxene and clinopyroxene grains, and smaller neoblasts. During the metasomatic processes, the consumption of the silicate part of the melt produced carbonate-enriched Type B CO2–SO2 fluids which were trapped in exsolved orthopyroxene porphyroclasts. At the later stages, the interstitial silicate/silicocarbonatite fluids were trapped as Type C inclusions. At a temperature above 650 °C, the mixed CO2–H2O–NaCl fluid inside the Type A inclusions were separated into CO2-rich fluid and H2O–NaCl brine. At T<650 °C, the residual silicate melt reacted with the host olivine, forming a reaction rim or “coating” along the inclusion walls consisting of talc (or possibly serpentine) together with minute crystals of NaCl, KCl, carbonates and sulfides, leaving a residual CO2 fluid. The homogenization temperatures of +2 to +25 °C obtained from the Type A CO2 inclusions reflect the densities of the residual CO2 after its reactions with the olivine host, and are unrelated to the initial fluid density or the external pressure at the time of trapping. The latter are restricted by the estimated crystallization temperatures of 1000–1200 °C, and the spinel lherzolite phase assemblage of the xenolith, which is 0.7–1.7 GPa.  相似文献   

8.
郭云成  刘家军  尹超  郭梦需 《现代地质》2021,35(6):1536-1550
小秦岭地区位于华北克拉通南缘,赋存许多大型-超大型的金矿床,大湖金钼矿床位于小秦岭北矿带。大湖金钼矿床成矿具有多期多阶段特点,包括热液期和表生期,根据矿脉穿切关系、矿石的矿物组成以及结构、构造研究,热液期分为4个成矿阶段,即石英-钾长石-辉钼矿阶段(Ⅰ)、石英-黄铁矿-自然金阶段(Ⅱ)、石英-多金属硫化物-自然金阶段(Ⅲ)和石英-碳酸盐阶段(Ⅳ)。流体包裹体岩相学、激光拉曼成分分析和冷热台测温结果表明,大湖金钼矿的初始成矿流体属H2O-CO2-NaCl体系,包裹体分为三种类型,即CO2-H2O型包裹体(C型)、水溶液型包裹体(W型)和纯CO2型包裹体(PC型)。成矿Ⅰ、Ⅱ、Ⅲ和Ⅳ阶段包裹体均一温度范围分别为275.3~350.0 ℃、260.0~312.7 ℃、245.3~287.6 ℃和237~251 ℃,流体盐度范围为5.2%~16.7%,密度为0.777~1.108 g/cm3,为中-高温、中-低盐度、低密度流体,与变质流体特征一致。均一温度从Ⅰ阶段→Ⅳ阶段呈逐渐下降趋势,盐度从Ⅰ阶段→Ⅲ阶段逐渐降低,Ⅳ阶段沸腾作用使流体中的气体组分逸出,导致剩余流体的浓缩盐度增高。流体成矿压力范围为58.0~196.3 MPa,对应成矿深度范围为3.0~7.1 km。矿区普遍存在的围岩蚀变表明水岩反应强烈,氢同位素δD为-90‰~-44‰,成矿流体氧同位素δ18O范围为2.1‰~5.9‰,属于变质热液范围;在δ18O-δD组成图解投图中落在变质水范围左下侧,Ⅱ、Ⅲ阶段样品的δ18O较Ⅰ阶段整体左移,表明高温变质流体与围岩(斜长角闪岩等变质岩)发生水岩反应,导致同位素互换平衡。大湖金钼矿床受区域近东西向断裂构造控制,属典型的断控脉状矿床,成矿流体以变质水为主,矿床主要特征与典型的造山型金矿特征相符。  相似文献   

9.
A combined fluid inclusion and mineral thermobarometric study in groups of synchronous inclusions in quartz within weakly foliated granites from the Chottanagpur Gneissic Complex, India, reveals super dense carbonic (CO2 with minor CH4 and H2O) inclusions and hypersaline (H2O–NaCl ± NaHCO3) inclusions, with halite- and nahcolite daughter phases. This study documents the highest density (1.115 g cm− 3) CO2 fluids ever reported in granites. Fluid isochores, constructed from CO2 (± CH4) and halite-bearing inclusions, coupled with two-feldspar thermometry constrain the minimum P–T at 8 kbar/ 750 °C for fluid entrapment in granites. By contrast, the carbonic inclusions in quartz from granite-hosted metapelite enclaves contain substantial CH4 (up to 30 mol%), and the entrapment pressure ( 4.3 kbar/600 °C) is considerably lower compared to those in the granites. By implication, the sillimanite-free granites were not derived from the metapelitic enclaves, and instead were formed by partial melting of fluid-heterogeneous lower crustal protoliths, with fluid entrapment at magmatic conditions.  相似文献   

10.
Although hydrocarbon-bearing fluids have been known from the alkaline igneous rocks of the Khibiny intrusion for many years, their origin remains enigmatic. A recently proposed model of post-magmatic hydrocarbon (HC) generation through Fischer-Tropsch (FT) type reactions suggests the hydration of Fe-bearing phases and release of H2 which reacts with magmatically derived CO2 to form CH4 and higher HCs. However, new petrographic, microthermometric, laser Raman, bulk gas and isotope data are presented and discussed in the context of previously published work in order to reassess models of HC generation. The gas phase is dominated by CH4 with only minor proportions of higher hydrocarbons. No remnants of the proposed primary CO2-rich fluid are found in the complex. The majority of the fluid inclusions are of secondary nature and trapped in healed microfractures. This indicates a high fluid flux after magma crystallisation. Entrapment conditions for fluid inclusions are 450–550 °C at 2.8–4.5 kbar. These temperatures are too high for hydrocarbon gas generation through the FT reaction. Chemical analyses of rims of Fe-rich phases suggest that they are not the result of alteration but instead represent changes in magma composition during crystallisation. Furthermore, there is no clear relationship between the presence of Fe-rich minerals and the abundance of fluid inclusion planes (FIPs) as reported elsewhere. δ13C values for methane range from − 22.4‰ to − 5.4‰, confirming a largely abiogenic origin for the gas. The presence of primary CH4-dominated fluid inclusions and melt inclusions, which contain a methane-rich gas phase, indicates a magmatic origin of the HCs. An increase in methane content, together with a decrease in δ13C isotope values towards the intrusion margin suggests that magmatically derived abiogenic hydrocarbons may have mixed with biogenic hydrocarbons derived from the surrounding country rocks.  相似文献   

11.
宝兴沟金矿床是大兴安岭北部上黑龙江成矿带内大型金矿床之一,矿体主要产于下侏罗统二十二站组砂岩与早白垩世石英闪长岩、闪长玢岩内外接触带内,其热液成矿作用可划分为:黄铁矿±毒砂-石英(Ⅰ)、多金属硫化物-石英(Ⅱ)及少硫化物-碳酸盐(Ⅲ)3个阶段。流体包裹体岩相学研究表明:Ⅰ阶段矿石主要发育气液两相(LV)、少量含CO2三相包裹体(HCO2)及富气相包裹体(FV);Ⅱ阶段矿石中主要发育LV及少量HCO2包裹体;Ⅲ阶段矿石中只发育LV包裹体。测温结果显示:Ⅰ、Ⅱ阶段包裹体总体均一温度峰值集中于225.00~300.00℃,盐度(w(NaCl))为2.00%~10.00%;Ⅲ阶段均一温度峰值集中于175.00~225.00℃,盐度为4.00%~8.00%;成矿流体为简单的含CO2中低温、低盐度的NaCl-H2O热液体系,总体具有从成矿早期到晚期均一温度、盐度逐渐降低的特征。氢、氧同位素分析结果显示,Ⅰ、Ⅱ阶段成矿流体δDSMOW为-131.00‰~-108.00‰、δ18OSMOW为1.00‰~4.00‰,Ⅲ阶段δDSMOW为-108.00‰、δ18OSMOW为-1.89‰,表明早期以岩浆水为主,晚期逐渐演化为与大气降水混合热液。矿石中黄铁矿(毒砂)δ34SV-CDT为1.50‰~4.20‰,显示其物质来源以深源岩浆为主。综合分析认为,区内金成矿作用与早白垩世(石英)闪长岩、闪长玢岩侵入活动有直接关系,矿床属中低温岩浆热液成因类型。  相似文献   

12.
山东新城金矿是胶东焦家-新城成矿带上重要的蚀变岩型金矿床。矿体主要赋存在焦家断裂带下盘靠近主裂面的黄铁绢英岩和黄铁绢英岩化碎裂岩内,严格受焦家断裂构造控制。矿石矿物主要有黄铁矿、黄铜矿、方铅矿、闪锌矿、自然金、银金矿和辉银矿等。区内围岩蚀变类型主要有黄铁绢英岩化、绢英岩化、绢云母化、硅化、钾化和碳酸盐化等,且矿化主要与黄铁绢英岩化和硅化关系密切。本次研究主要针对新城金矿床深部矿石中的流体包裹体进行了岩相学、显微测温、单个包裹体成分激光拉曼光谱及氢、氧同位素分析研究。研究表明:该矿床深部矿石中纯CO2包裹体数量有明显增加现象,同时发育含CO2包裹体和气液两相包裹体;成矿流体具有低盐度(w(NaCl))(2.06%~10.24%)、低密度(0.54~0.97 g/cm3)的特点;主成矿温度为260~300 ℃,成矿压力为65~113 MPa,成矿深度为6.51~8.82 km。成矿过程中流体经历了CO2-NaCl-H2O体系的不混溶作用。氢、氧同位素分析认为,成矿流体δDSMOW为-75.1‰~-61.4‰,δ18O为4.80‰~6.40‰,并将新城金矿床与典型“焦家式”金矿床成矿流体特征及来源进行对比,认为新城金矿成矿流体主要以幔源流体为主。综合研究表明,新城金矿床成因类型为幔源流体参与成矿的中温热液脉型金矿床。  相似文献   

13.
This work presents the results of a fluid inclusion study of an amphibolite-granulite facies transition in West Uusimaa, S.W. Finland. Early fluid-inclusions in the granulite facies area are characteristically carbonic (CO2), in contrast to predominantly aqueous early inclusions in the amphibolite facies area. These early inclusions can be related to peak metamorphic conditions (750-820°C and 3-5 kbar for peak granulite facies metamorphism). Relatively young CO2 inclusions with low densities (<0.8g/cm3) indicate that the first part of the cooling history of the rocks was characterized by a near isothermal uplift.
N2-CH4 inclusions, with compositions ranging between pure CH4 and pure N2 (Raman spectral analysis), were found in the whole area. They are probably syn- or even pre-early inclusions. Only nearly critical homogenizing inclusions have been found (low density). Pressure estimates, based on densities of early fluid inclusions, show that the rapid transition of amphibolite towards granulite facies metamorphism is virtually isobaric. Granulite facies metamorphism in West Uusimaa is a thermal event, probably induced by the influx of hot, CO2-bearing fluids.  相似文献   

14.
The stability and phase relations of phengitic muscovite in a metapelitic bulk composition containing a mixed H2O+CO2 fluid were investigated at 6.5–11 GPa, 750–1050°C in synthesis experiments performed in a multianvil apparatus. Starting material consisted of a natural calcareous metapelite from the coesite zone of the Dabie Mountains, China, ultrahigh-pressure metamorphic complex that had experienced peak metamorphic pressures greater than 3 GPa. The sample contains a total of 2.1 wt.% H2O and 6.3 wt.% CO2 bound in hydrous and carbonate minerals. No additional fluid was added to the starting material. Phengite is stable in this bulk composition from 6.5 to 9 GPa at 900°C and coexists with an eclogitic phase assemblage consisting of garnet, omphacite, coesite, rutile, and fluid. Phengite dehydrates to produce K-hollandite between 8 and 11 GPa, 750–900°C. Phengite melting/dissolution occurs between 900°C and 975°C at 6.5–8 GPa and is associated with the appearance of kyanite in the phase assemblage. The formation of K-hollandite is accompanied by the appearance of magnesite and topaz-OH in the phase assemblage as well as by significant increases in the grossular content of garnet (average Xgrs=0.52, Xpy=0.19) and the jadeite content of omphacite (Xjd=0.92). Mass balance indicates that the volatile content of the fluid phase changes markedly at the phengite/K-hollandite phase boundary. At P≤8 GPa, fluid coexisting with phengite appears to be relatively CO2-rich (XCO2/XH2O=2.2), whereas fluid coexisting with K-hollandite and magnesite at 11 GPa is rich in H2O (XCO2/XH2O=0.2). Analysis of quench material and mass balance calculations indicate that fluids at all pressures and temperatures examined contain an abundance of dissolved solutes (approximately 40 mol% at 8 GPa, 60 mol% at 11 GPa) that act to dilute the volatile content of the fluid phase. The average phengite content of muscovite is positively correlated with pressure and ranges from 3.62 Si per formula unit (pfu) at 6.5 GPa to 3.80 Si pfu at 9 GPa. The extent of the phengite substitution in muscovite in this bulk composition appears to be limited to a maximum of 3.80–3.85 Si pfu at P=9 GPa. These experiments show that phengite should be stable in metasediments in mature subduction zones to depths of up to 300 km even under conditions in which aH2O1. Other high-pressure hydrous phases such as lawsonite, MgMgAl-pumpellyite, and topaz-OH that may form in subducted sediments do not occur within the phengite stability field in this system, and may require more H2O-rich fluid compositions in order to form. The wide range of conditions under which phengite occurs and its participation in mixed volatile reactions that may buffer the composition of the fluid phase suggest that phengite may significantly influence the nature of metasomatic fluids released from deeply subducted sediments at depths of up to 300 km at convergent plate boundaries.  相似文献   

15.
为研究鄂尔多斯盆地中部地区马家沟组成藏期次和天然气运移方向与断裂活动的相关性,利用流体包裹体岩相学观察、激光拉曼光谱分析、均一温度和冰点温度的测定以及热力学PVT模拟方法对奥陶系马家沟组马五段储层的岩心样品进行了成分、温度和压力的测定与恢复.结果表明:构造裂缝脉体中充填的矿物为方解石、白云石和菱镁矿;脉体中共有4类流体包裹体,分别为富甲烷气体包裹体、含CO2富甲烷气体包裹体、含甲烷盐水包裹体和盐水包裹体,这4类流体包裹体均存在于方解石脉体中;构造裂缝脉体和溶孔中含甲烷流体包裹体的均一温度在130.1~179.6 ℃之间,与含甲烷流体包裹体同期的盐水包裹体的均一温度范围为112.3~173.3 ℃.结合生排烃史和埋藏史,证明早白垩世是马家沟组天然气的主要成藏期.沿断裂分布的各井的捕获压力和压力系数呈现由西南向东北递减的趋势,早白垩世的构造运动在北东向的断层中产生大量构造裂缝,为天然气的运移提供了通道,证明含甲烷的流体沿北东向断裂运移并充注成藏.   相似文献   

16.
耿庄金矿床产于燕山期隐爆角砾岩体内,是晋东北具有代表意义的金多金属矿床之一。对矿床流体包裹体系统研究表明,不同成矿阶段石英中流体包裹体主要有5种类型:富气相包裹体、富液相包裹体、含CO2三相包裹体、含子矿物三相包裹体及少量纯液相包裹体,流体属H2O-CO2-NaCl体系类型。成矿前阶段包裹体类型多样,且以相似的均一温度共存,显示流体具明显沸腾及不混溶特性;成矿温度集中于170~180 ℃。结合同位素和金矿物特征,认为耿庄金矿床应为与燕山期次火山热液有关的中-低温热液型金矿床。  相似文献   

17.
延边杨金沟大型白钨矿矿床流体包裹体特征及成因探讨   总被引:2,自引:1,他引:2  
延边杨金沟大型白钨矿矿床的成矿过程可划分为黄铁矿-毒砂阶段、石英-粗粒白钨矿阶段、石英-多金属硫化物-细粒白钨矿阶段以及碳酸盐阶段,其中,石英-粗粒白钨矿阶段为主成矿阶段。与粗粒白钨矿共生的石英中主要发育4种类型流体包裹体。Ⅰ型包裹体的气相组分主要由CO2、CH4和N2组成,均一温度为278.5~336.4℃,盐度(w(NaCl))为3.53%~7.72%;Ⅱ型气液两相包裹体均一温度为144.7~345.9℃,多数为190~220℃,w(NaCl)为3.05%~9.34%;Ⅲ型CO2包裹体中的气相组分均为CO2,液相中尚含少量CH4等组分;Ⅳ型含CO2三相包裹体由液态CO2、气态CO2、盐水溶液三相组成,CO2相占10%~15%,完全均一化温度为301.6~305.1℃。综合地质条件及矿床特征、包裹体显微测温和成分分析结果认为:杨金沟石英脉型白钨矿矿床的成矿流体为中高温、低盐度的NaCl-H2O-CO2(-N2)体系,初始流体主要来自酸性岩浆热液,并有地层组分的加入。成矿过程中流体发生过不混溶,并对钨的富集起到了重要作用。  相似文献   

18.
庙梁金矿床位于南秦岭柞水-山阳矿集区的中心地带,为了查明庙梁金矿成矿流体特征、金的沉淀机制及矿床成因,对该矿床不同成矿阶段脉石矿物中的流体包裹体进行了详细的岩相学、显微测温、激光拉曼光谱分析研究并与周边典型金矿床特征进行了对比.结果 表明,该矿床包裹体类型丰富,成矿早阶段主要为H2O-NaCl型包裹体(Ⅱ型)、部分H2...  相似文献   

19.
云南普朗斑岩型铜矿床成矿流体特征及矿床成因   总被引:3,自引:0,他引:3  
普朗铜矿床为滇西北地区一超大型斑岩型铜多金属矿床,它产于印支晚期石英闪长玢岩-石英二长斑岩-花岗闪长斑岩复式侵入体内,已有研究表明其形成于印支期。本次流体包裹体岩相学、显微测温及碳、氢、氧同位素综合研究表明:黄铜矿±黄铁矿-石英脉石英中主要发育含NaCl子矿物三相、气液两相及富气相3种类型的包裹体,成矿流体属中高温、高盐度(w(NaCl))NaCl-H2O热液体系,来源于印支晚期岩浆活动;辉钼矿±黄铜矿-石英脉石英中发育含NaCl子矿物三相、气液两相及含CO2 3种类型的包裹体,成矿流体属中高温、高盐度NaCl-CO2-H2O热液体系,推测来源于后期岩浆活动;晚期黄铜矿±辉钼矿-方解石脉中主要发育气液两相包裹体,成矿流体为中低温、低盐度NaCl-H2O热液体系,系NaCl-CO2-H2O型成矿流体演化产物。据此,结合区域广泛叠加发育燕山期斑岩钼矿化成矿背景,提出普朗超大型斑岩矿床可能存在燕山期Mo、Cu成矿作用叠加的认识。  相似文献   

20.
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   

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