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1.
碳酸岩是地表出露较少的地幔来源的岩石,其地幔交代作用已被广泛研究,而碳酸岩岩浆与地壳的反应过程却研究较少,目前已在中国草滩和丰镇地区、德国Kaiserstuhl地区、俄罗斯Petyayan-Vara地区和澳大利亚Nolans Bore矿床等各地被报道。碳酸岩岩浆与地壳反应的特征是可能形成大量富铁云母、辉石、榍石、钡冰长石等硅酸盐矿物并造成C-O和Sr-Nd同位素体系的扰动。实验岩石学研究发现碳酸岩岩浆在地幔与橄榄岩反应形成异剥橄榄岩,对应的在中下地壳反应形成反夕卡岩。碳酸岩岩浆与围岩的反应会造成局部Si的富集促使REE在早期岩浆阶段进入磷灰石,从而抑制稀土成矿。深部地壳的碳酸岩-硅酸岩反应在相同构造背景下通常不像浅部热液系统容易出露地表,并且其反应产物容易被误认为是夕卡岩矿物组合。因此,更多的高温高压实验研究以及对硅酸盐流体来源不是很清楚的高温夕卡岩矿物组合进行重新评估,将是揭示地壳深部反夕卡岩过程,特别是相关成矿作用的关键。  相似文献   

2.
地球深部碳循环是指地球表层的碳在俯冲带进入地幔深部,然后通过岩浆或者脱气作用再把地幔中的碳释放到地球表层系统中的过程。人类对地球深部碳赋存形式和储量、不同储库的交换方式和交换量尚缺乏清晰认识,近年来随着分析技术的发展和研究的深入,深部碳循环的研究日益丰富。本文总结了地幔中碳赋存状态、地球深部碳储量、碳进出地幔方式及通量、俯冲带碳的行为和碳酸岩成因及成矿方面的研究。地幔中碳赋存形式多样且主要受地球深部压力及氧逸度控制。相平衡实验和热动力学计算发现碳酸盐化榴辉岩在300~600 km发生部分熔融,交代地幔橄榄岩形成碳酸盐化地幔橄榄岩。碳酸盐化地幔橄榄岩的熔融又会形成碳酸岩熔体,这说明俯冲再循环物质可能对碳酸岩的成因起重要作用。碳酸岩是研究深部碳循环的良好载体,其源区特征、岩浆演化过程对示踪碳在地幔和地壳过程中的迁移至关重要。虽然深部碳循环在碳赋存形式、碳储量及通量、俯冲带碳的流变行为和碳酸岩成因对深部碳循环的启示方面已经取得了较大的研究进展,但仍有大量的科学问题亟待解决,如:沉积碳酸盐岩再循环进入地球深部后的行为、俯冲带板片流体地球化学行为、俯冲带流体氧逸度特征等,将来有必要重点开展深入研...  相似文献   

3.
山东昌乐新生代玄武岩内的刚玉巨晶(蓝宝石)中含有多种类型熔融包裹体,其成分对了解华北深部地幔交代过程中的流/熔体性质和刚玉母岩浆特点具有重要意义.详细的岩相学和激光拉曼分析鉴定出一类富碳酸盐和硫酸盐成分的原生熔融包裹体以及一类含硫酸盐和氯化物等成分的次生熔融包裹体,二者同时还含有CO2和H2O.碳酸盐和硫酸盐成分在世界范围玄武岩内刚玉巨晶中是首次发现,结合已有的包裹体稀有气体同位素和测温资料,反映两种成分可能来源于交代地幔的碳酸岩熔体,预示着华北深部地幔不仅经历了硅酸盐成分的交代还经历了富碳酸盐和硫酸盐成分(碳酸岩)的交代,同时也显示刚玉母岩浆成分复杂,至少有富这两类成分物质的参与,刚玉很可能是硅酸盐岩浆/岩石和幔源碳酸岩岩浆相互作用的产物,后被玄武岩喷发携带至地表.  相似文献   

4.
<正>地幔交代作用及地幔流体研究是深部地质过程研究的热点问题之一。地幔交代作用不仅关系到地幔深部的部分熔融,而且对地幔源岩浆的性质的研究具有重要的指示意义,对于我们理解岩石圈地幔的演化形成、大陆动力学机制以及岩浆作用有很大的帮助。地幔交代介质通常根据组分分成碳酸盐熔体、富H2O-CO2流体、玄武质熔体和富硅熔体等,这些交代熔体可能源于再循环的大陆地壳、软流圈地幔或俯冲洋壳。由于地幔交代作用交代介质及其来源复杂多样,因此如何鉴别地幔交代作用类型和进一步认识熔体在地幔中  相似文献   

5.
陈意  苏斌  郭顺 《地球科学》2019,44(12):4086-4094
俯冲地壳衍生流体交代地幔楔,是产生俯冲带岩浆作用的重要机制.但是,目前人们对俯冲大陆物质改造地幔楔的岩石学过程和机理仍缺乏深入认识,造山带橄榄岩是解析这一问题的直接样品.通过对大别-苏鲁造山带橄榄岩进行系统的矿物学、岩石学和地球化学研究,发现橄榄石Ni/Co比值可有效区分幔源和壳源造山带橄榄岩,揭示幔源造山带橄榄岩起源于华北岩石圈地幔.苏鲁李家屯纯橄岩在进入俯冲带之前就已在地幔内部经历了碳酸盐熔体交代.大别毛屋和苏鲁蒋庄橄榄岩及其交代脉体记录了约170~200 km深度的俯冲带壳幔相互作用过程.深俯冲陆壳释放的富Si-Al质熔体可不同程度地改造地幔楔底部,形成富石榴石和富辉石的交代岩,并引发强烈的Os同位素分馏效应.该过程不仅改变地幔楔岩性和化学组成,还能够改变交代介质成分,为俯冲带各类深部地幔岩浆提供源区物质.因此,大陆深俯冲是导致上地幔不均一的重要途径.   相似文献   

6.
埃达克岩的Na亏损及其对地幔Na交代的指示意义   总被引:1,自引:3,他引:1  
埃达克岩是玄武质洋壳部分熔融的产物。然而,与实验室玄武岩部分熔融产生的埃达克质熔体相比,天然埃达克岩明显地高Mg、Cr和Ni,这表明埃达克岩浆在上升过程中有地幔成分的加入。本文的观察结果表明,全球新生代埃达克岩的Na2O含量低于5.8%,大约95%的新生代埃达克岩样品Na2O含量小于5.0%。然而,在埃达克岩产生的压力范围(1.5~3.0GPa),实验的玄武岩部分熔体大多数Na2O含量超过5.0%,最高达到9.0%,显示埃达克岩具有明显的Na亏损现象。我们认为这是埃达克熔体在热的地幔楔中与地幔橄榄岩反应的结果。在俯冲带,大洋板片熔融产生的熔体(埃达克熔体)上升并与地幔橄榄岩发生反应,原始的埃达克熔体获得MgO、Cr及Ni等地幔组分,但其Na2O和SiO2等通过反应进入地幔,导致地幔交代作用。根据长英质熔体与橄榄岩反应体系的相关系,我们认为,地幔单斜辉石、橄榄石、尖晶石的混染作用以及钠质角闪石和斜方辉石的分离结晶作用,是改变埃达克熔体组成并导致其Na亏损的一个重要的过程。埃达克岩的Na亏损为地幔Na交代作用和一些富Na的弧岩浆成因提供了重要证据。  相似文献   

7.
徐楠  吴才来  刘畅 《地质学报》2023,97(12):4067-4084
南阿尔金造山带位于塔里木盆地和柴达木盆地之间,是中国西北地区重要的俯冲-碰撞杂岩带,其早古生代构造演化过程是近年来的研究热点之一,然而,洋壳俯冲的时限一直存在争议。本文对茫崖石英二长岩开展岩石学、地球化学、锆石U-Pb年代学和锆石Lu-Hf同位素地球化学研究,探讨其岩石成因及成岩时的构造环境。样品显示高碱、富钾、低钛、贫铁及Nd-Ta-Ti异常等与钾玄岩相似的地球化学特征,成岩年龄为511~495 Ma, εHf(t)主要为-3.51~-0.08,少量介于0.04~1.69之间。我们认为俯冲洋壳到达角闪岩相边界时释放大量水并上升进入地幔楔,导致地幔楔橄榄岩发生角闪石化交代作用,由于地幔楔沿俯冲带向下拖曳而温度升高,角闪石化橄榄岩熔融形成的熔体在上升过程诱发上地壳物质部分熔融,壳源岩浆混合少量幔源岩浆形成了石英二长岩,该期花岗岩是对造山带从大洋岛弧环境向活动大陆边缘过渡的岩石学响应。因此,南阿尔金洋壳可能在约517 Ma前已经开始俯冲。  相似文献   

8.
埃达克质岩的构造背景与岩石组合   总被引:6,自引:1,他引:5  
本文介绍了埃达克质岩形成的构造背景与岩石组合。埃达克质岩可以形成于不同的构造背景并与不同类型的岩石同时出现:1)火山弧环境中常出现埃达克质岩一高镁安山岩-富Nb玄武质岩组合,它的形成可能与板片熔融以及熔体一地幔橄榄岩的相互作用有关;2)大陆活动碰撞造山带环境(如羌塘)中埃达克质岩常与同期钾质或橄榄玄粗质岩共生,这可能与俯冲陆壳熔融和俯冲陆壳熔体交代的地幔橄榄岩熔融有关;3)造山带伸展垮塌环境(如大别山)中埃达克质岩会伴随有镁铁质一超镁铁质岩浆出露,增厚下地壳产生埃达克质岩浆后的榴辉岩质残留体拆沉进入地幔,与地幔橄榄岩的混合可能形成后期镁铁质一超镁铁质岩浆的源区;4)大陆板内伸展环境中埃达克质岩常与同期橄榄玄粗质的岩石共生,增厚、拆沉下地壳,以及富集地幔的熔融或岩浆混合在岩石的成因中发挥了重要作用。  相似文献   

9.
甘肃礼县新生代火山喷发碳酸岩的发现及意义   总被引:7,自引:8,他引:7  
甘肃礼县新生代钾霞橄黄长岩中有大量火山喷发碳酸岩出露,本文对该区各种碳酸岩的地质产状,岩石特征,全岩化学及稀土,微量和C、O同位素地球化学进行了研究,结果表明本区碳酸岩属于一种高CaO低碱(Na2O K2O)的火成碳酸岩,其化学成分与东非裂谷乌干达FortPortal地区的碳酸岩相似,其中碳酸岩的火山砾岩和凝灰岩具有高的SiO2和Mg/Ca比值,化学成分显示了硅酸盐和碳酸盐混合的特征,可能代表直接由地幔部分熔融形成的原生碳酸盐岩浆。其它类型碳酸岩的成因与原生碳酸盐岩浆或原生钾霞橄黄长岩浆的液态不混溶作用和/或结晶分异作用有关。碳酸岩及共生的高钾火山岩不是典型的大陆裂谷岩浆作用的产物,其起源和成因与软流圈的上涌有关。碳酸岩的发现为查明本区地幔的组成和性质提供了新的岩石学证据。  相似文献   

10.
深俯冲碳酸盐化泥质岩的部分熔融行为研究是探索地球深部碳循环必不可少的方向之一,对地球深部物质循环、岩浆形成以及地幔化学成分不均一等过程起着不容忽视的作用。本文利用多顶砧大压机探索了6.0 GPa、800~1 600℃下碳酸盐化泥质岩的部分熔融行为,实验产物主要包括石榴子石、单斜辉石、柯石英、蓝晶石、碳酸盐矿物、多硅白云母以及熔体。碳酸盐矿物为方解石和菱镁矿,存在于6.0 GPa固相线以下的实验产物中。相对于同等压力下其它碳酸盐化体系,本文实验体系具有最低的固相线。部分熔融产生的熔体为硅酸盐熔体,且随着温度的升高,熔体比例逐渐增加,熔体成分也发生了明显的变化。  相似文献   

11.
火成碳酸岩及其风化产物是全球战略性关键金属稀土元素(REE)和铌(Nb)的主要来源。因此,对关键金属在火成碳酸岩中的超常富集机理研究具有重要的科学意义。研究表明成矿碳酸岩常常与碱性杂岩体存在密切的时空联系,因而母岩浆应属于碳酸盐化的硅酸盐岩浆,并以霞石岩岩浆为主。针对碳酸岩关键金属矿床的成岩成矿过程,已有实验发现母岩浆在地壳内的演化过程中,既可以通过分离结晶作用,也可以通过液态不混溶作用形成碳酸岩。然而,更加接近自然样品的多组分体系的实验均表明液态不混溶作用总是先于碳酸盐矿物分离结晶作用。因此,液态不混溶作用对关键金属成矿过程有着不可忽视的作用。尽管如此,已有不混溶实验表明当碳酸盐熔体和硅酸盐熔体发生不混溶之后,关键金属REE与Nb总是优先分配到硅酸盐熔体(碱性岩)中,但是在成矿杂岩体中,REE与Nb是高度富集在碳酸岩中。虽然不混溶实验表明REE与Nb在碳酸盐-硅酸盐熔体中的分配系数与含水量有关,即与熔体的聚合程度有关,但是绝大部分成矿碳酸岩成矿过程一般并不富水,所以碳酸岩中REE和Nb等关键金属元素超常富集的机理并不明确。因此未来的研究应重点关注在碳酸岩演化的过程中,除了水以外,其他配体对于关键金属元素在不混溶硅酸盐-碳酸盐熔体之间分配系数是否有影响,从而找到控制碳酸岩中关键金属成矿的关键。  相似文献   

12.
The brevity of carbonatite sources in the mantle: evidence from Hf isotopes   总被引:5,自引:0,他引:5  
Hf, Zr and Ti in carbonatites primarily reside in their non-carbonate fraction while the carbonate fraction dominates the Nd and Sr elemental budget of the whole rock. A detailed investigation of the Hf, Nd and Sr isotopic compositions shows frequent isotopic disequilibrium between the carbonate and non-carbonate fractions. We suggest that the trace element and isotopic composition of the carbonate fraction better represents that of the carbonatite magma, which in turn better reflects the composition of the carbonatitic source. Experimental partitioning data between carbonatite melt and peridotitic mineralogy suggest that the Lu/Hf ratio of the carbonatite source will be equal to or greater than the Lu/Hf ratio of the carbonatite. This, combined with the Hf isotope systematics of carbonatites, suggests that, if carbonatites are primary mantle melts, then their sources must be short-lived features in the mantle (maximum age of 10–30 Ma), otherwise they would develop extremely radiogenic Hf compositions. Alternatively, if carbonatites are products of extreme crystal fractionation or liquid immiscibility then the lack of radiogenic initial Hf isotope compositions also suggests that their sources do not have long-lived Hf depletions. We present a model in which the carbonatite source is created in the sublithospheric mantle by the crystallization of earlier carbonatitic melts from a mantle plume. This new source melts shortly after its formation by the excess heat provided by the approaching hotter center of the plume and/or the subsequent ascending silicate melts. This model explains the HIMU-EMI isotope characteristics of the East African carbonatites, their high LREE/HREE ratios as well as the rarity of carbonatites in the oceanic lithosphere.  相似文献   

13.
Extrusive carbonatites: A brief review   总被引:1,自引:0,他引:1  
A.R. Woolley  A.A. Church 《Lithos》2005,85(1-4):1-14
49 known extrusive carbonatite occurrences are listed with brief details of their tectonic setting, structure, lithologies, associated silicate rocks, chemistry and presence or absence of included mantle materials. Half the occurrences appear to be related to tephra cones, tuff rings, diatremes and maars and the rest occur within strato-volcanoes. Pyroclastic carbonatitic rocks are present at all the localities, with carbonatite lava flows occurring at only 14 of them. The pyroclastic rocks, which include fallout tephra and deposits from pyroclastic surges and flows and products of phreatomagmatic eruptions, vary from rocks composed principally of carbonate to varieties with as little as 20% igneous carbonate. The most abundant silicate rocks associated with extrusive carbonatites are melilite-bearing rocks, nephelinite and/or ijolite, and phonolite and/or nepheline syenite; seven occurrences have no associated silicate rocks. 16 occurrences, most of them associated with small extrusive centres, contain mantle xenoliths or megacrysts, details of which are tabulated, with spinel lherzolite the most abundant rock type, but amphibole, phlogopite and garnet are also recorded. The lack of such materials in intrusive carbonatites may reflect their less energetic environment of emplacement. It is proposed that carbonatites are essentially of two types: (a) those rising energetically and rapidly from the mantle, which form small explosion craters, ash or tuff cones, or diatremes, have only low-volume associated silicate rocks, and entrain mantle debris, and (b) those which occur in strato-volcanoes, are associated with large volumes of silicate rocks and follow a more complex genesis, probably involving ponding and differentiation (separation from carbonate-bearing silicate magma) at higher levels in the mantle and/or crust. Most of the classic intrusive carbonatite complexes probably fall into the second category.  相似文献   

14.
岩浆(型)碳酸岩研究进展   总被引:19,自引:0,他引:19  
主要从岩石学,矿物学,岩石分类,C,O,Sr同位素,碳酸岩与矿化的关系等各方面对(碱性)碳酸岩的研究进行了较为全面的总结,并结合近20年来实验岩石等,流体包裹体研究,CO2^- H2O-NaCl流体体系的性质的研究,对碳酸岩岩浆的来源及成因,岩浆-热液的演化进行了分析和探讨,碳酸岩形成至少经历了三个阶段,即岩浆阶段,岩浆期后阶段(气相碳酸岩/岩浆热液阶段),交代碳酸岩阶段,而作为与碳酸岩在空间和成因上有密切联系的基性,超基性岩,碱性岩杂岩体,则经历了碳酸岩成岩阶段以前的岩浆不混熔作用,结晶分异作用,岩浆结晶作用以及碳酸岩形成之后的围岩蚀变(霓长岩化)作用。  相似文献   

15.
Igneous rocks of the Devonian Kola Alkaline Carbonatite Province (KACP) in NW Russia and eastern Finland can be classified into four groups: (a) primitive mantle-derived silica-undersaturated silicate magmas; (b) evolved alkaline and nepheline syenites; (c) cumulate rocks; (d) carbonatites and phoscorites, some of which may also be cumulates. There is no obvious age difference between these various groups, so all of the magma-types were formed at the same time in a relatively restricted area and must therefore be petrogenetically related. Both sodic and potassic varieties of primitive silicate magmas are present. On major element variation diagrams, the cumulate rocks plot as simple mixtures of their constituent minerals (olivine, clinopyroxene, calcite, etc). There are complete compositional trends between carbonatites, phoscorites and silicate cumulates, which suggests that many carbonatites and phoscorites are also cumulates. CaO / Al2O3 ratios for ultramafic and mafic silicate rocks in dykes and pipes range up to 5, indicating a very small degree of melting of a carbonated mantle at depth. Damkjernites appear to be transitional to carbonatites. Trace element modelling indicates that all the mafic silicate magmas are related to small degrees of melting of a metasomatised garnet peridotite source. Similarities of the REE patterns and initial Sr and Nd isotope compositions for ultramafic alkaline silicate rocks and carbonatites indicate that there is a strong relationship between the two magma-types. There is also a strong petrogenetic link between carbonatites, kimberlites and alkaline ultramafic lamprophyres. Fractional crystallisation of olivine, diopside, melilite and nepheline gave rise to the evolved nepheline syenites, and formed the ultramafic cumulates. All magmas in the KACP appear to have originated in a single event, possibly triggered by the arrival of hot material (mantle plume?) beneath the Archaean/Proterozoic lithosphere of the northern Baltic Shield that had been recently metasomatised. Melting of the carbonated garnet peridotite mantle formed a spectrum of magmas including carbonatite, damkjernite, melilitite, melanephelinite and ultramafic lamprophyre. Pockets of phlogopite metasomatised lithospheric mantle also melted to form potassic magmas including kimberlite. Depth of melting, degree of melting and presence of metasomatic phases are probably the major factors controlling the precise composition of the primary melts formed.  相似文献   

16.
Melt inclusions in clinopyroxenes from lherzolitic xenoliths from the deep lithospheric mantle beneath the Slave Craton (Lac de Gras area, Canada) reveal multiple origins for carbonatitic melts. One type of inclusions consists of a series of silicate–carbonate–silicate concentric layers, interpreted to have unmixed under disequilibrium conditions during rapid ascent to the surface. Bulk major- and trace-element compositions are typical of Group 1 kimberlites and quantitative nuclear microprobe imaging of the globules reveals fractionation of related elements (e.g. F–Br, Nb–Ta) between the silicate and carbonate components. The globules probably formed by partial melting of carbonated peridotite, consistent with results of melting experiments and some models for the generation of kimberlite magmas. They provide evidence for a genetic relationship between some carbonate-rich magmas and ultramafic silicate magmas, and for the possibility of unmixing processes of these melts during their evolution.

The second inclusion type comprises carbonate-rich globules interpreted as samples of Mg-carbonatite melt that quenched on ascent to the surface. Bulk major- and trace-element compositions indicate that the melts were derived from a carbonate-rich source and oxygen, carbon, and strontium isotope data are consistent with the involvement of recycled crustal material and suggest that some mantle-derived carbonatites are unrelated to kimberlites.  相似文献   


17.
Vulture volcano displays a wide range of mafic to alkaline, carbonate-, and/or CaO-rich volcanic rocks, with subvolcanic and plutonic rocks together with mantle xenoliths in pyroclastic ejecta. The roles of magmatic volatiles such as CO2, S, and Cl have been determined from compositions and trapping temperatures of inclusions in phenocrysts, which include the Na-K-Ca-carbonate nyerereite within melilite. We surmise that this alkali carbonate crystallised from an appropriate carbonatitic melt at relatively high temperature. Carbonatitic metasomatic features are traceable throughout many of the mantle xenoliths, and various carbonatitic components are found in the late stage extrusive suite. There is no evidence that alkali carbonatite developed as a separate magma, but it may have been an important evolutionary stage. We compare the rare occurrence of nyerereite at Vulture with other carbonatites and with an unaltered kimberlite from the Udachnaya pipe. We review the evidence at Vulture for associated carbonatitic metasomatism in the mantle, and we suggest that low viscosity alkali carbonatitic melts may have a primary and much deeper origin than previously considered.  相似文献   

18.
This paper reviews the results of investigations of melt inclusions in minerals of carbonatites and spatially associated silicate rocks genetically related to various deep-seated undersaturated silicate magmas of alkaline ultrabasic, alkaline basic, lamproitic, and kimberlitic compositions. The analysis of this direct genetic information showed that all the deep magmas are inherently enriched in volatile components, the most abundant among which are carbon dioxide, alkalis, halides, sulfur, and phosphorus. The volatiles probably initially served as agents of mantle metasomatism and promoted melting in deep magma sources. The derived magmas became enriched in carbon dioxide, alkalis, and other volatile components owing to the crystallization and fractionation of early high-magnesium minerals and gradually acquired the characteristics of carbonated silicate liquids. When critical compositional parameters were reached, the accumulated volatiles catalyzed immiscibility, the magmas became heterogeneous, and two-phase carbonate-silicate liquid immiscibility occurred at temperatures of ≥1280–1250°C. The immiscibility was accompanied by the partitioning of elements: the major portion of fluid components partitioned together with Ca into the carbonate-salt fraction (parental carbonatite melt), and the silicate melt was correspondingly depleted in these components and became more silicic. After spatial separation, the silicate and carbonate-silicate melts evolved independently during slow cooling. Differentiation and fractionation were characteristic of silicate melts. The carbonatite melts became again heterogeneous within the temperature range from 1200 to 800–600°C and separated into immiscible carbonate-salt fractions of various compositions: alkali-sulfate, alkali-phosphate, alkali-fluoride, alkali-chloride, and Fe-Mg-Ca carbonate. In large scale systems, polyphase silicate-carbonate-salt liquid immiscibility is usually manifested during the slow cooling and prolonged evolution of deeply derived melts in the Earth’s crust. It may lead to the formation of various types of intrusive carbonatites: widespread calcite-dolomite and rare alkali-sulfate, alkali-phosphate, and alkali-halide rocks. The initial alkaline carbonatite melts can retain their compositions enriched in P, S, Cl, and F only at rapid eruption followed by instantaneous quenching.  相似文献   

19.
碳酸岩的地质地球化学特征及其大地构造意义   总被引:20,自引:0,他引:20  
从已知碳酸岩的地质产状、岩石学特征、Nd-Sr-Pb-O-C同位素及痕量元素地球化学特征数据,结合高温高压实验岩石学资料,论述了其地幔源区的物质成分、交代过程软流圈地幔部分熔融机制和碳酸岩岩浆的演化模型。碳酸岩既可以产生于拉张岩石圈构造背景,也能够产生于挤压而派生的引张岩石圈构造背景。前者以产于裂谷环境、与硅酸不饱和过碱性岩构成环状碳酸岩—碱性杂岩为特征,主要由起源于软流圈地幔的霞石质超基性—基性岩浆经液态不混溶作用而形成;后者产于碰撞造山过程中派生的引张岩石圈断裂带,以单一的透镜状、条带状和似层状碳酸岩体为标志,直接由导源岩石圈富集地幔的低程度部分熔融作用而产生的碳酸岩浆侵入或喷发所形成。  相似文献   

20.
碳酸岩流体及其稀土成矿作用   总被引:12,自引:0,他引:12  
火成碳酸岩熔浆可侵入到大陆和洋壳构造环境 ,多数大陆构造环境下的碳酸岩在时间和空间上与地壳减薄事件有关 ,高温下它具有极强的搬运碱金属、大离子亲石元素和高场强元素的能力。碳酸岩中可能出现的原生包裹体有两相水溶液 (气 +液 )包裹体、含子矿物多相水溶液包裹体、含CO2 包裹体和CO2 +盐水溶液混合多相包裹体以及硅酸盐玻璃质熔融包裹体等。碳酸岩型稀土矿床中赋存的流体包裹体类型也可分为气液相、含碳水溶液相和气液固多相包裹体 ,包裹体中稀土子矿物的出现是该类矿床最显著的特征。富碱碳酸岩流体中REE ,Sr ,Th和Fe等都具有极高的溶解度 ,水岩反应和流体不混溶是造成成矿热液中REE及Fe等沉淀成矿的关键因素 ,REE的迁移沉淀可延续到低温、低盐度的成矿晚阶段  相似文献   

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