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1.
Petrogenetic studies of carbonatites are challenging, because carbonatite mineral assemblages and mineral chemistry typically reflect both variable pressure–temperature conditions during crystallization and fluid–rock interaction caused by magmatic–hydrothermal fluids. However, this complexity results in recognizable alteration textures and trace-element signatures in the mineral archive that can be used to reconstruct the magmatic evolution and fluid–rock interaction history of carbonatites. We present new LA–ICP–MS trace-element data for magnetite, calcite, siderite, and ankerite–dolomite–kutnohorite from the iron-rich carbonatites of the 1.3 Ga Grønnedal–Íka alkaline complex, Southwest Greenland. We use these data, in combination with detailed cathodoluminescence imaging, to identify magmatic and secondary geochemical fingerprints preserved in these minerals. The chemical and textural gradients show that a 55 m-thick basaltic dike that crosscuts the carbonatite intrusion has acted as the pathway for hydrothermal fluids enriched in F and CO2, which have caused mobilization of the LREEs, Nb, Ta, Ba, Sr, Mn, and P. These fluids reacted with and altered the composition of the surrounding carbonatites up to a distance of 40 m from the dike contact and caused formation of magnetite through oxidation of siderite. Our results can be used for discrimination between primary magmatic minerals and later alteration-related assemblages in carbonatites in general, which can lead to a better understanding of how these rare rocks are formed. Our data provide evidence that siderite-bearing ferrocarbonatites can form during late stages of calciocarbonatitic magma evolution.  相似文献   

2.
The carbonatite at Magnet Cove, Arkansas, USA contains a great variety and abundance of magmatic and hydrothermal inclusions that provide an informative, though fragmentary, record of the original carbonatite melt and of late hydrothermal solutions which permeated the complex in postmagmatic time. These inclusions were studied by optical and scanning electron microscopy. Primary magmatic inclusions in monticellite indicate that the original carbonatite melt contained approximately 49.7 wt% CaO, 16.7% CO2, 15.7% SiO2, 11.4% H2O, 4.4% FeO+Fe2O3, 1.1% P2O5 and 1.0% MgO. The melt was richer in SiO2 and iron oxides than the carbonatite as now exposed; this is attributed to crystal settling and relative enrichment of calcite at shallower levels. The density of the carbonatite melt as revealed by the magmatic inclusions was approximately 2.2–2.3 g/cc. Such a light melt should separate rapidly from any denser parent material and could be driven forcibly into overlying crustal rocks by buoyant forces alone. Fluid inclusions in apatite suggest that a separate (immiscible) phase composed of supercritical CO2 fluid of low density coexisted with the carbonatite magma, but the inclusion record in this mineral is inconclusive with respect to the nature of any other coexisting fluids. Maximum total pressure during CO2 entrapment was about 450 bars, suggesting depths of 1.5 km or less for apatite crystallization and supporting earlier proposals of a shallow, subvolcanic setting for the complex. Numerous secondary inclusions in the Magnet Cove calcite contain an intriguing variety of daughter minerals including some 19 alkali, alkaline earth and rare earth carbonates, sulfates and chlorides few of which are known as macroscopic phases in the complex. The exotic fluids from which the daughter minerals formed are inferred to have cooled and diluted through time by progressive mixing with local groundwaters. These fluids may be responsible for certain late veins and elemental enrichments associated with the complex.  相似文献   

3.
《地学前缘(英文版)》2019,10(2):769-785
The Weishan REE deposit is located at the eastern part of North China Craton (NCC), western Shandong Province. The REE-bearing carbonatite occur as veins associated with aegirine syenite. LA-ICP-MS bastnaesite Th-Pb ages (129 Ma) of the Weishan carbonatite show that the carbonatite formed contemporary with the aegirine syenite. Based on the petrographic and geochemical characteristics of calcite, the REE-bearing carbonatite mainly consists of Generation-1 igneous calcite (G-1 calcite) with a small amount of Generation-2 hydrothermal calcite (G-2 calcite). Furthermore, the Weishan apatite is characterized by high Sr, LREE and low Y contents, and the carbonatite is rich in Sr, Ba and LREE contents. The δ13CV-PDB (−6.5‰ to −7.9‰) and δ13OV-SMOW (8.48‰–9.67‰) values are similar to those of primary, mantle-derived carbonatites. The above research supports that the carbonatite of the Weishan REE deposit is igneous carbonatite. Besides, the high Sr/Y, Th/U, Sr and Ba of the apatite indicate that the magma source of the Weishan REE deposit was enriched lithospheric mantle, which have suffered the fluid metasomatism. Taken together with the Mesozoic tectono-magmatic activities, the NW and NWW subduction of Izanagi plate along with lithosphere delamination and thinning of the North China plate support the formation of the Weishan REE deposit. Accordingly, the mineralization model of the Weishan REE deposit was concluded: The spatial-temporal relationships coupled with rare and trace element characteristics for both carbonatite and syenite suggest that the carbonatite melt was separated from the CO2-rich silicate melt by liquid immiscibility. The G-1 calcites were crystallized from the carbonatite melt, which made the residual melt rich in rare earth elements. Due to the common origin of G-1 and G-2 calcites, the REE-rich magmatic hydrothermal was subsequently separated from the melt. After that, large numbers of rare earth minerals were produced from the magmatic hydrothermal stage.  相似文献   

4.
The paper presents mineralogical features and EPMA results of the Khamambettu carbonatites. The mineralogical data suggest that these rocks have been generated in magmatic and hydrothermal stages. Mineral geothermometer for carbonatite give temperatures of 790°–980°C. Fluid inclusion measurements in monazite (hydrothermal stage) give temperatures of 220°–290°C. One of the features of the carbonatites is high content of magnesia that is defined by the presence of dolomite, olivine, spinel, phlogopite, Mg-rich ilmenite. Chloritization, serpentinization, amphibolization, silicification processes and occurrence of barite, monazite-(Ce), strontianite, celestine are related to hydrothermal stage. Hydrothermal minerals at the Khamambettu were formed by recrystallization of primary carbonatite minerals in the presence of Ba, (SO4)2?, REE and Si carried in solution by the hydrothermal fluid.  相似文献   

5.
Rare earth element (REE) abundances were measured by neutron activation analysis in anhydrite (CaSO4), barite (BaSO4), siderite (FeCO3) and galena (PbS). A simple crystal-chemical model qualitatively describes the relative affinities for REE substitution in anhydrite, barite, and siderite. When normalized to ‘crustal’ abundances (as an approximation to the hydrothermal fluid REE pattern), log REE abundance is a surprisingly linear function of (ionic radius of major cation—ionic radius of REE)2 for the three hydrothermal minerals, individually and collectively. An important exception, however, is Eu, which is anomalously enriched in barite and depleted in siderite relative to REE of neighboring atomic number and trivalent ionic radius. In principle, REE analyses of suitable pairs of co-existing hydrothermal minerals, combined with appropriate experimental data, could yield both the REE content and the temperature of the parental hydrothermal fluid.The REE have only very weak chalcophilic tendencies, and this is reflected by the very low abundances in galena—La, 0.6 ppb; Sm, 0.06 ppb; the remainder are below detection limits.  相似文献   

6.
白云鄂博矿区交代及成矿作用的成因矿物学研究   总被引:1,自引:0,他引:1       下载免费PDF全文
张荣红 《地球科学》1995,20(2):231-236
通过对白云鄂博矿区碱性角闪石和金云母的成因矿物学研究,证实本区确实有岩浆碳酸岩的活动,活动中心在矿区东部,矿区碱交代作用来源于岩浆碳酸岩的后期热液活动,与白云鄂博铁-铌-稀土矿床中的主斯铁矿化无趋势关系,但与稀土矿化关系密切,作为铁矿化的太物学标志是:标型矿物镁钠闪石和镁钠铁闪石;金云母的特殊反多色性及其低Ti,高X^tetsi的成分特征以及特殊的标型矿物组合。  相似文献   

7.
陈欢  冯梦  康志强  付伟  冯佐海 《地球科学》2020,45(6):2059-2076
为了解桂东北伟晶岩岩浆的形成环境及演化过程,对桂东北茅安塘Nb-Ta-Be-Rb稀有金属矿床周围伟晶岩中的石榴子石进行了镜下观察、电子探针(EPMA)和LA-ICP-MS原位微区主微量元素研究,探讨石榴子石的成因及其对成岩及成矿作用的指示.结果表明,桂东北茅安塘地区伟晶岩中的石榴子石为岩浆成因石榴子石,属于铁铝榴石-锰铝榴石(平均Alm49.28-Sps47.09)固溶体系列,可分为早期形成的Ⅰ型石榴子石(GrtⅠ)和晚期形成的Ⅱ型子石(GrtⅡ).两期石榴子石均以富集重稀土(HREE)、高场强元素(HFSE),亏损轻稀土(LREE)和缺乏大离子亲石元素(LILE)为特征,∑REE配分模式呈明显左倾趋势,显著的Eu负异常.石榴子石生长过程中的界面反应速率小于物质迁移速率,水岩作用较弱,∑REE主要以表面吸附或吸收的形式进入石榴子石中,是导致其重稀土(HREE)元素富集,轻稀土元素亏损的主要原因.随着岩浆分异演化程度的不断提高,∑REE逐渐进入并赋存于石榴子石中,促进岩浆从早期的低分馏(未分馏)的岩浆熔体逐渐向晚期的高分馏的岩浆熔体演化.石榴子石中HREE含量随岩浆演化程度逐渐增加表明,晚期分异演化的岩浆-热液中逐渐富集稀土及稀有金属元素.这些晚期富含成矿元素的热液流体交代原生矿物,导致外侧带及核部花岗伟晶岩中发育大量交代成因的稀土和稀有金属矿物.   相似文献   

8.
浙江临安石室寺伟晶岩位于河桥岩体西北面,属于典型的Nb-Y-F (NYF) 型伟晶岩,富含大量稀有稀土矿物。本文在野外考察和显微镜观察的基础上,结合电子探针背散射电子图像观察与矿物化学成分分析,系统鉴定了石室寺NYF 型伟晶岩中的稀有稀土矿物,揭示了稀有稀土元素的富集、迁移、结晶与成矿过程。研究结果表明:(1) 石室寺伟晶岩中的稀有稀土矿物有铌钽矿物(铌铁矿、铌锰矿、重钽铁矿、细晶石等)、钇矿物(褐钇铌矿、黑稀金矿)、钨矿物(黑钨矿、 白钨矿、铌钨矿物)、铈矿物(独居石、氟铈矿、氟碳铈矿) 和钍矿物等。(2) 铌钨系列矿物的WO3含量在8.30~70.51 wt%之间呈规律变化,可能为铌铁矿与黑钨矿之间形成的一系列多体矿物。(3) 铌铁矿LA-ICP-MS U-Pb 定年结果显示,石室寺伟晶岩的形成年龄为133±2 Ma,与河桥花岗岩具有成因联系。(4) 石室寺NYF 型伟晶岩中稀有稀土元素的成矿过程与其岩浆的结晶演化密切相关:岩浆阶段,锆石、钍石与独居石等矿物最早晶出;岩浆—热液阶段,黑稀金矿、铌铁矿、褐钇铌矿、氟铈矿等稀有稀土矿物逐渐结晶;热液阶段,黑钨矿、铌钨矿物相继形成,同时早期的独居石、氟铈矿受晚期热液交代形成次生铈矿物。  相似文献   

9.
浙江临安石室寺伟晶岩位于河桥岩体西北面,属于典型的Nb-Y-F (NYF) 型伟晶岩,富含大量稀有稀土矿物。本文在野外考察和显微镜观察的基础上,结合电子探针背散射电子图像观察与矿物化学成分分析,系统鉴定了石室寺NYF 型伟晶岩中的稀有稀土矿物,揭示了稀有稀土元素的富集、迁移、结晶与成矿过程。研究结果表明:(1) 石室寺伟晶岩中的稀有稀土矿物有铌钽矿物(铌铁矿、铌锰矿、重钽铁矿、细晶石等)、钇矿物(褐钇铌矿、黑稀金矿)、钨矿物(黑钨矿、 白钨矿、铌钨矿物)、铈矿物(独居石、氟铈矿、氟碳铈矿) 和钍矿物等。(2) 铌钨系列矿物的WO3含量在8.30~70.51 wt%之间呈规律变化,可能为铌铁矿与黑钨矿之间形成的一系列多体矿物。(3) 铌铁矿LA-ICP-MS U-Pb 定年结果显示,石室寺伟晶岩的形成年龄为133±2 Ma,与河桥花岗岩具有成因联系。(4) 石室寺NYF 型伟晶岩中稀有稀土元素的成矿过程与其岩浆的结晶演化密切相关:岩浆阶段,锆石、钍石与独居石等矿物最早晶出;岩浆—热液阶段,黑稀金矿、铌铁矿、褐钇铌矿、氟铈矿等稀有稀土矿物逐渐结晶;热液阶段,黑钨矿、铌钨矿物相继形成,同时早期的独居石、氟铈矿受晚期热液交代形成次生铈矿物。  相似文献   

10.
华南是我国重要的战略性矿产资源基地,以花岗岩相关的稀有和稀土金属成矿作用而举世瞩目。其中,铌的成矿作用一般与过铝质高分异花岗岩有关,稀土元素则随岩浆演化程度增强而富集程度降低,而江西铁木里含黑云母碱长花岗岩体同时富集铌和稀土元素,矿化组合极具特色。本文在详细的矿物岩相学研究基础上,利用电子探针、飞秒激光电感耦合等离子质谱对铌和稀土矿物进行了矿物地球化学分析,借此对铁木里碱长花岗岩中铌和稀土元素的富集机制进行探讨。铁木里岩体由肉红色含黑云母碱长花岗岩(r-G)和灰白色含黑云母碱长花岗岩(g-G)组成,发育暗色包体。r-G中的铌矿物主要为岩浆期形成的铌铁金红石,稀土矿物包括岩浆期形成的硅钛铈矿、独居石、磷灰石和热液期形成的独居石和氟碳(钙)铈矿。g-G中的铌矿物包括岩浆期形成的铌铁金红石和热液期形成的铌铁金红石、易解石、铌铁矿,稀土矿物包括岩浆期磷灰石和热液期磷灰石、独居石、氟碳(钙)铈矿。暗色包体为岩浆混合成因,内含磷灰石、独居石和零星的硅钛铈矿、金红石。矿物组合特征显示,铁木里碱长花岗岩中的铌和稀土元素经过了岩浆和热液两个时期的富集。应用金红石、磷灰石、绿泥石等矿物成分特征约束了岩浆-...  相似文献   

11.
新疆和静县乔霍特铜矿地质地球化学特征   总被引:4,自引:1,他引:4  
乔霍特铜矿是位于新疆西天山的一个中型铜矿床。似层状矿化体赋存于上志留统中基性火山岩及沉积岩中 ,矿化富集受地层、构造、侵入岩的多重控制。火山岩属于发育不成熟的裂谷环境中的中基性岩类 ,赋矿火山岩与无矿火山岩的稀土元素组成近似 ,而与后期叠加改造形成的脉状矿化体的稀土元素组成有较大差别。矿石矿物主要为辉铜矿、黄铜矿、斑铜矿等 ,呈粒状和浸染状分布。成矿温度为 130~ 140℃。矿化溶液含岩浆水和变质水 ,属于酸性的富含钾、氯和二氧化碳的流体。矿化过程经历晚志留世火山热液充填 交代作用和海西早期岩浆热液的叠加、改造作用。  相似文献   

12.
白云鄂博矿区发育的脉状稀土碳酸岩,由于其结晶迅速,矿物颗粒细微,其中的微小矿物的鉴定一直是一个难题。应用显微共聚焦激光拉曼光谱仪则能较好地解决这一问题。研究表明,白云鄂博地区存在富稀土白云质岩浆碳酸岩脉,早期阶段形成碱性长石和铁白云石,无稀土矿化;铁白云石常常出溶铁质而自身则形成方解石。霓石和方解石形成略晚,常常与氟碳铈矿等稀土矿物共生,出现强烈的稀土矿化;而无解理的方解石则形成于更晚的岩浆期后热液阶段,发育大量的流体包裹体,并出现强烈的铌、稀土矿化。铌铁矿分布在氟碳铈矿中和赤铁矿边缘,为热液交代作用的产物。早期结晶的矿物如碱性长石、铁白云石稀土矿化弱,岩浆晚期分异出大量的流体相,稀土元素和Sr等进入岩浆热液中,并在热液结晶矿物中富集,甚至在非平衡结晶的石英中产生强烈的稀土矿化。结合岩相学显微观察,显微拉曼探针很好的揭示了这一地质过程。同时为白云鄂博矿床铌、稀土矿化的热液交代成因提供了依据。  相似文献   

13.
The Purulia carbonatite, ‘carbonatite’-‘alkali-pyroxenite’-‘apatite-magnetite rock’ association, is located at Beldih area of Purulia district, West Bengal and falls within the 100 km long Northern Shear Zone (NSZ). Published literature suggests that the Purulia carbonatite was formed by the process of liquid immiscibility from under-saturated silicate parent magma. However, no silica under-saturated rocks like ijolite, nepheline-syenite etc. is known from the area. The trace element geochemistry (Ba/La, Nb/Th, Nb/Pb and Y/Ce ratios in the present study) also does not support this view. Present study indicates that the Purulia carbonatite is enriched in ΣREE and incompatible elements but the carbonatite is also poorer in Nb, Th and Pb compared to the world average of calicocarbonatites. The lower value of Nb is characteristics of carbo(hydro)thermal carbonatite where carbonatite is associated with alkali-pyroxenite and suggests probable origin of the carbonatite as carbothermal residua evolved from an unknown parentage. However, the field, petrographic and geochemical data indicate the genesis of this carbonatite from a primary carbonatitic magma of mantle decent. The 87Sr/86Sr ratio of the carbonatite and apatite separated from the carbonatite (~0.703) implies primary magmatic derivation of the Purulia carbonatite. Close similarity of the apatite of the apatite-magnetite rock with the mantle apatite (of type Apatite B) indicates that they are also of primary magmatic origin. The present work portrays a unique example where primary magmatic carbonatite is associated with the alkali-pyroxenite.  相似文献   

14.
白云鄂博矿床研究若干问题的探讨   总被引:4,自引:1,他引:3  
白云鄂博巨型稀土-铌-铁矿床是与火成碳酸岩(即H8)有关的矿床。在碳酸岩岩浆阶段,在其蚀变围岩(霓长岩)中以及晚期的热液阶段都有稀土、铌和铁等的富集。因此,白云鄂博矿床不是单一矿床类型,其涵盖了稀土-铌-铁碳酸岩岩浆型矿床、稀土-铌-铁交代蚀变岩型和热液型矿床,这种复合类型的矿床是十分罕见的,可称之为白云鄂博式矿床。根据已发表的年代数据,白云鄂博大规模碳酸岩的形成时代和伴随的稀土矿化的高峰期在1.3~1.4Ga。加里东构造热事件对本区的影响广泛和强烈,不仅有广泛发育的大型褶皱、冲断层和韧性剪切作用,并伴有广泛的流体交代作用和局部的热液活动,某些稀土矿物的同位素体系受到重置,表现为其Sm-Nd年龄和Th-Pb年龄的不一致。本区的碱性岩在基底杂岩中即有出露,随后在白云鄂博群中和1.3~1.4Ga白云鄂博碳酸岩形成时皆有产出。目前所获资料表明,至少1.3~1.4Ga的碱性杂岩在成因上与碳酸岩有密切的联系。本区基底杂岩显示了白云鄂博地区在2.0Ga左右曾经有一个弧地质体,该区在2.0~1.9Ga间经历了从被动大陆边缘到活动大陆边缘增生碰撞的一个完整的造山过程。  相似文献   

15.
The Bayan Obo Fe–REE–Nb deposit is the world's largest rare earth element (REE) resource and with the increasing focus on critical metal resources has become a focus of global interest. The deposit is hosted in the Palaeoproterozoic Bayan Obo Group, mainly concentrated in the H8 dolomite marble. The ores consist of light REE enriched monazite and bastnäsite, with a wide array of other REE minerals. Niobium mineralisation is hosted primarily in aeschynite and pyrochlore, although there are a wide range of other Nb-minerals. The origin of the host dolomite and ore bodies has been a subject of intense debate. The host dolomite has been proposed to be both of sedimentary origin and an igneous carbonatite. Carbonatite dykes do occur widely in the area, and consideration of the textural, geochemical and isotopic composition of the dolomite suggests an origin via intrusion of magmatic carbonatite into meta-sedimentary marble, accompanied by metasomatism. The origin of the ore bodies is complex, indicated most strongly by an ~ 1 Ga range in radiometric age determinations. Compilation of available data suggests that the ores were originally formed around 1.3 Ga (Sm–Nd isochron ages; Th–Pb ages of zircon), close in time to the intrusion of the carbonatite dykes. The ores were subsequently subjected to several stages of deformation and hydrothermal overprint, culminating in deformation, metamorphism and fluid flow related to the Caledonian subduction of the Mongolian Plate under the North China Craton from ~ 450 to 420 Ma (Th–Pb ages of monazite). This stage resulted in the formation of the strong foliation (‘banding’) of the ore. The presence of undeformed veins with alkali mineral fills, and the overprinting of the foliation by Nb minerals suggest that secondary fluid flow events may also have contributed to the metal endowment of the deposits, as well as remobilising the original Fe and REE mineralisation. The alteration mineralogy and geochemistry of the ores are comparable to those of many REE mineralised carbonatites. Initial Nd isotope ratios at 450 Ma, however, suggest crustal sources for the metals. These conflicting lines of evidence can be reconciled if a (at least) two stage isotopic evolution is accepted for the deposits, with an original mantle-sourced, carbonatite-related metal accumulation forming around 1.3 Ga with εNd close to 0. The ore was remobilised, with associated re-equilibration of Th–Pb isotope systematics during deformation at ~ 450 Ma. A further stage of alkaline hydrothermal fluid was responsible for Nb mineralisation at this stage. The complex geological history, with multiple stages of alkaline, high field strength element-rich, metasomatic fluid flow, is probably the main reason for the exceptional metal endowment of the Bayan Obo area.  相似文献   

16.
庐枞盆地龙桥铁矿床中菱铁矿的地质特征和成因意义   总被引:6,自引:0,他引:6  
龙桥铁矿床是庐枞火山岩盆地中的一个大型的铁矿床,多年来对其矿床成因的认识存在较大的争论.文章在野外地质研究工作的基础上,通过对矿床中菱铁矿的岩矿分析鉴定和电子探针测试,确定了矿床纹层状矿石中的菱铁矿为沉积成因.通过对菱铁矿的产出特征分析,并结合龙桥铁矿床的部分地质地球化学研究成果,认为在该矿床形成过程中,早期沉积形成了纹层状的菱铁矿层,在燕山期的岩浆热事件中,部分沉积菱铁矿被交代形成了磁铁矿和具有残余骸晶结构等一系列矿石交代组构特征的矿物.纹层状矿石既具有沉积特征,也具有热液改造特征,证实了矿床的形成存在早期(三叠纪)的沉积成矿(菱铁矿)作用和晚期(燕山期)的热液成矿(磁铁矿)作用.菱铁矿的研究为进一步确定龙桥铁矿床的成因提供了新的佐证.  相似文献   

17.
对安徽新桥矿床进行系统的野外地质调查和矿相学研究发现,层状矿体中的胶状黄铁矿交代矽卡岩磁铁矿矿体,为探讨层状硫化物矿床是早期沉积成因还是岩浆热液成因提供了新的地质约束。对铜陵矿集区内的新桥矿床层状菱铁矿矿体和凤凰山矽卡岩型矿体中的菱铁矿开展了Fe同位素组成的对比研究,结果显示:新桥矿床菱铁矿与典型低温热液脉型矿床和沉积铁矿中的菱铁矿在Fe同位素组成特征上有所不同,而与凤凰山矽卡岩型矿床中的菱铁矿更为接近;新桥矿床中胶状黄铁矿和菱铁矿相对于磁铁矿富集Fe的轻同位素,表明磁铁矿不是过去认为的由胶状黄铁矿和菱铁矿矿胚层经热液改造形成,而是与典型的岩浆热液有关。新桥矿区层状硫化物矿体和矽卡岩型矿体中,近岩体矽卡岩和最早形成的金属矿物磁铁矿比岩体更为富集Fe的轻同位素,而赋矿围岩比岩体更为富集Fe的重同位素。同时,不同矿化阶段形成的含铁矿物和不同空间位置的硫化物中的Fe同位素组成呈现出时空分带现象,Fe同位素组成的时空演化特征与流体出溶、流体演化非常一致,并且符合同位素分馏的基本理论,表明层状硫化物矿体和矽卡岩型矿体具有相同的成矿物质来源,为同一流体体系演化的产物。新桥矿区岩相学的研究结果和Fe同位素组成特征均表明,新桥层状硫化物矿床不是海西期喷流沉积成矿作用的产物,而是燕山期热液成矿作用的产物,为一个典型的热液成因矿床。  相似文献   

18.
鄂尔多斯盆地延长组长7油层组黑色岩系中首次发现主要呈纹层状、脉状等顺层分布于油页岩或凝灰岩中的碳酸质岩浆—热液喷流型沉积岩(简称喷积岩),具有重要的研究价值。通过野外露头和钻井取心观察,薄片鉴定,扫描电镜、电子探针、全岩元素分析等测试方法,对上述碳酸质喷积岩的岩石学、矿物学、地球化学以及与生烃母质关系特征进行了初探。结果显示,按物质来源、形成方式和结构构造可将长7油层组碳酸质喷积岩划分为碳酸质喷爆岩、碳酸质喷溢岩、碳酸质喷流岩三大类型,三者主量元素、微量元素、稀土元素等地球化学特征具有岩浆碳酸岩和热水沉积岩的双重特征,且与生烃母质的发育具有正相关性。因此,碳酸质喷积岩在鄂尔多斯盆地延长组长7油层组黑色岩系沉积期发育,且对长7油层组生烃研究具有重要的理论和实际意义。  相似文献   

19.
郗山和龙宝山稀土矿具有相似的成矿地质背景、控矿岩体特征及矿床地质特征。燕山早期碱性侵入岩与稀土矿关系密切,稀土矿体主要赋存于杂岩体内及其附近围岩中;稀土元素和同位素研究表明,含矿质的富碱岩浆可能属壳幔混源型,碱性岩浆及成矿物质最初可能都来源于上地幔同一部位,而在岩浆上侵过程中同化混染了地壳物质。郗山稀土矿为单一富轻稀土矿床,矿脉类型以含稀土石英重晶石碳酸盐脉为主,含稀土矿物以氟碳铈矿和氟碳钙铈矿为主,碳酸铈钠矿和菱钙锶铈矿属国内首次发现。龙宝山稀土矿为稀土、金共生矿,矿脉类型主要为石英脉和硅化角砾岩;含稀土矿物主要有氟碳铈矿、氟碳铈镧矿、氟碳钙铈矿;金矿物有自然金、银金矿等。成矿时代稍晚于岩浆岩形成时代,属中生代燕山晚期;矿床成因类型为碱性岩浆期后中-低温热液稀土矿床。  相似文献   

20.
The Montviel 250 Mt carbonatite-hosted REE–Nb deposit is hosted in a Paleoproterozoic alkaline suite located in the Sub-Province of Abitibi, in the Archean Province of the Superior. The alkaline intrusion consists of biotite clinopyroxenites, melano- to leucosyenites, a melteigite–ijolite–urtite series, riebeckite granite, a series of carbonatites and a carbonatite polygenic breccia. The carbonatite series includes silicocarbonatites, calciocarbonatites, rare magnesiocarbonatites, ferrocarbonatites and mixed carbonatites and are cut by a late, high-energy carbonatite polygenic breccia. Diamond drill hole assays and microscope observations indicate that Nb is hosted in pyrochlore from silicocarbonatite whereas the REE mineralization is mainly hosted in ferrocarbonatite, late mixed carbonatites and polygenic breccia, in REE-bearing carbonates and fluorocarbonate minerals. Diamond drill hole underground mapping and systematic assays have shed light on zones enriched in Nd and LREE with preferential Ba and Sr hydrothermal precipitation and zones enriched in Dy, Y and HREE displaying preferential F and P bearing hydrothermal precipitation. Petrographic observations, electron microprobe analyses, LA-ICPMS and X-ray diffraction were used to study the mineralization processes and to identify and quantify the REE-bearing burbankite–(Ce), carbocernaite–(Ce), ewaldite–(Y), huanghoite–(Nd), cordylite–(Ce), cordylite–(Nd), kukharenkoite–(Ce) and synchysite–(Ce). Most minerals are enriched in total LREE with values around 19.3 wt.%, have total MREE values around 2.2 wt.% and extremely variable total HREE values, with very high contents of Dy and Y averaging around 0.3 wt.% and 1.0 wt.%, respectively, and with total HREE reaching up to 10.0 wt.%. A paragenetic sequence is proposed that consists of: (1) a silicocarbonatite Nb stage, and (2) a calciocarbonatite stage, dominated by magmatism but accompanied by hydrothermal fluids, (3) a main ferrocarbonatite stage, dominated by episodes of Ba- and Sr-hydrothermalism and LREE mineralization, F- and P-hydrothermalism and HREE mineralization and evolved ferrocarbonatitic magmatism, (4) a renewed, mixed carbonatite magmatic stage with minor but increasing hydrothermalism, and (5) a terminal stage of fluid pressure buildup and explosion, leading to the creation of a HREE-enriched polygenic breccia. Globular melt inclusions of Ba–Cl–F (± Si–O) may indicate the presence and contribution of barium-bearing chlorofluoride melts during hydrothermal activity and mineralization of the carbonatite.  相似文献   

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