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雷琼新生代玄武岩中地幔岩包体矿物中的流体—熔体包裹体的REE组成特征 总被引：3，自引：3，他引：3
雷琼地区新生代玄武岩中地幔岩包体的１２件单矿物稀土元素中子活化分析表明，雷州和琼北地幔岩包体中不含流体－熔体包裹体的同类矿物的ＲＥＥ组成有明显差异，反映了雷州与琼北玄武岩地幔源区ＲＥＥ组成的不均一性。通过对比同一地幔岩包体中含包裹体与不含包裹体相同矿物的微量元素组成，发现雷琼地幔岩包体矿物中的流体－熔体包裹体富含ＲＥＥ，尤其是ＬＲＥＥ；并且不同产地地幔包体同类矿物中和同一包体不同矿物中包裹体的丰度 相似文献
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内蒙古阿尔山地区新生代玄武岩及其幔源包体微量元素组成特征 总被引：2，自引：0，他引：2
内蒙古阿尔山地区新生代火山活动频繁,喷发期次可划分为上新世、更新世、全新世,最新喷发时间约为1 900 a B P,具有再次喷发的可能。为了探讨活火山源区地幔流体的分布特征,利用中子活化分析和同步辐射X射线荧光微探针分析技术,对阿尔山地区全新世玄武岩及其幔源包体的稀土、微量元素组成特征、地幔包体矿物及其熔融包裹体的微量元素组成特征进行了分析。中子活化分析结果表明,不同产地玄武岩具有相同的稀土配分模式,其中,Σ8REE=96.93~114.94,Eu/Sm=0.32~0.37,(L a/Lu)N=8.89~12.52;不相容元素蛛网曲线整体右倾,B a,T a,Sm具正异常,T h,Z r具负异常,没有明显的S r异常,说明岩浆上升过程中很少演化和分离结晶;不同产地地幔岩包体中不含包裹体的同类矿物的REE组成相近,反映了不同活火山的地幔源区REE组成特征相同;不同产地地幔岩包体同类矿物及其内部包裹体同步辐射X射线荧光微探针分析表明具有相同的微量元素曲线分布形态;这些特征说明阿尔山活火山群分布区地幔流体不存在显著的不均一性。 相似文献
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地幔岩流体包裹体的稀土元素初步研究 总被引：1，自引：0，他引：1
地幔流体REE的研究有助于了解地幔区域化学不均一性、地幔的富集与亏损等地幔地球化学特征。当前对地幔流体的REE研究，主要是通过对比富CO2包裹体与贫CO2包裹体的地幔岩或地幔矿物的测试分析来间接获得信息。本尝试运用电感耦合等离子体质谱（ICP-MS）和热爆方法，直接测定了长白山地区的地幔捕虏体中流体-熔体包裹体REE含量。初步研究显示流体-熔体包裹体中富含REE，尤其LREE相对富集；REE组成曲线右倾，Eu弱正异常，与地幔岩的寄主玄武岩REE组成特征相似，反映源区地幔岩的交代特征。 相似文献
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汉诺坝玄武岩中地幔岩捕掳体REE和Sr,Nd同位素地球化学 总被引：20，自引：3，他引：20
本文报道汉诺坝玄武岩中地幔岩捕掳体的ＲＥＥ丰度和Ｓｒ、Ｎｄ同位素组成。不同岩石类型的ＲＥＥ配分模式和同位素组成反映地幔部分熔融程度和交代作用过程。二辉橄榄岩亏损轻稀土，是原始地幔经不同程度部分熔融的残留体。方辉橄榄岩具Ｕ型ＲＥＥ配分模式，是强烈亏损的地幔岩被熔体非化学平衡交代的结果。二辉岩脉状体富轻、中稀土，它同与脉状体接触的二辉橄榄岩可达化学平衡或近于化学平衡，而二辉岩脉状体的形成与玄武岩岩浆无成因关系。据对二辉岩脉状体和不含脉状体橄榄岩的Ｓｍ－Ｎｄ同位素定年，这种脉状体形成于３００Ｍａ左右。 相似文献
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我国东部沿海地区新生代碱性玄武岩中,广泛分布尖晶石二辉橄榄岩等地幔岩包体,地幔岩的退火时间和退火温度是岩石圈演化的重要标志。研究表明,地幔橄榄岩是宿主岩石中的异源包体,为先已存在的固态的地幔物质。镜下观察表明,地幔橄榄岩的主要造岩矿物中常含有圆形矿物包裹体,如橄揽石中含有尖晶石和斜方辉石,斜方辉石中含有橄榄石和尖晶石包裹体等。矿物包裹体从原始的多边形转变为球粒状的形态变化是地幔岩在某种退火温 相似文献
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地幔捕虏体中的流体-熔体包裹体 总被引：3，自引：0，他引：3
地幔流体的研究现已成为国内外前沿课题。地幔岩捕虏体中的流体-熔体包裹体是地幔流体的直接证据,通过对它们的研究可以直接获取地授流体的信息。包裹体按相态特征主要有三类：二氧化碳流体包裹体、二氧化碳-硅酸盐熔体包裹体、硫化物-熔体流体包裹体。本总结了地幔岩中流体-熔体包裹体的基本特征、微量元素地球化学、硫化物-熔体包裹体和二氧化碳流体包裹体稳定同位素特征的研究进展状况。讨论认为：地幔流体是由C、H、O、S等元素的挥发份和硅酸盐熔体组成;上地幔流体在化学成分上明显富含CO2、硫化物、LILE和BEE,它引起地幔交代作用和地授部分熔融;上地授流体的分布存在不均匀性,其组成也存在地区性差异。 相似文献
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中国东南沿海地区地幔岩包体中流体及熔体包裹体研究 总被引：10，自引：1，他引：10
浙江新昌和福建明溪地区新生代玄武岩中地幔岩包体矿物中的ＣＯ２包裹体和含ＣＯ２硅酸盐岩浆包裹体的研究表明，它们捕获于温度１２０７℃～１２６７℃和压力８１５～１１４７ｍｐａ条件下，约相当于３０～５０ｋｍ深的上幔环境；ＣＯ２包裹体流体成分是以ＣＯ２为主，有ＣＨ４、ＣＯ、Ｈ２Ｓ、Ｈ２Ｏ、Ｎ２、和Ｈ２等次要组分，代表地幔流体成分。含ＣＯ２硅酸盐岩浆包裹体均一后成分不同于寄主玄武岩，它富ＳｉＯ２、Ａｌ２Ｏ３、ＭｇＯ和Ｋ２Ｏ，贫ＦｅＯ和ＣａＯ，反映了未分异原始玄武岩浆的成分，它们可能是研究地区的地幔软流圈－岩石圈界面抬升，压力降低在地幔流体作用下发生的部分熔融作用的产物． 相似文献
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《吉林大学学报(地球科学版)》2015,(Z1)
<正>深部下地壳及地幔中的流体是无机成因天然气的巨大气源库体。地下深部的物质运动人们又不可能直接接触,但出露在地表的地幔岩是研究地幔演化的窗口。玄武岩中的包体更是典型的地幔岩石,包体中携带有大量的地幔物质信息,而其中的流体包裹体则是地幔演化中原始流体的代表,其中的气体同位素能有效地指示气体的源区及其地球化学特征,反映上地幔组成和演化,对深部无机成因气的气源示踪、形成条件和环境以及地幔脱气研究有着重要的意义。本文通过地幔岩包体中的流体包裹体分析了幔源流体及其气 相似文献
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南海海山玄武岩形成条件研究 总被引：9，自引：0，他引：9
南海海山火山岩主要由碱性玄武岩,拉斑玄武岩、粗安质浮岩、英安岩等组成。火山岩中的矿物包裹体主要为非晶质熔融包裹体,反映出海山火山岩水下喷发冷凝较快的特点,并在碱性玄武岩及其地幔岩包体中发现流体熔融包裹体,表明该区上地幔部分熔融过程中曾经历过熔浆与流体不混熔的过程。四个海山火山岩直接测定的成岩温度分别为:中南海山碱性玄武岩1155～1185℃,宪北海山碱性玄武岩960～1200℃,拉斑玄武岩1040～1230℃,玳瑁海山拉斑玄武岩1245～1280℃,尖峰海山粗安质浮岩880～1140℃。中南海山及宪北海山碱性玄武岩的平衡压力分别为13.57×10~8Pa和8.8×10~8Pa。宪北海山地幔岩包体的辉石平衡温度为1073～1121℃,压力为(15.58～22.47)×10~8Pa,表明碱性玄武岩浆来源较深,已达到该区上地幔软流圈范围。 相似文献
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地幔岩中不同产状的流体-熔体包裹体及地幔流体交代作用 总被引：1，自引：0，他引：1
地幔捕虏体中存在不同产状的熔体包裹体和各种硅酸盐玻璃相,包括主矿物内部的蠕虫状、长圆形、圆形、不规则状包裹体(I型)、边部的连通的管状包裹体(T型)、主矿物边部和粒间的片状熔融体——“浆胞”(C型),三者可见明显过渡关系,它们是地幔流体交代地幔岩石过程中由交代重熔形成的,是研究地幔流体的特征和地幔交代作用的对象之一,从I型、T型到C型,其成分呈规律变化,其中S、Cu、Ni,K、Na含量呈明显的降低趋势．包裹体中玻璃相的成分较主矿物富Si、Al、S、Cu、Ni、K和Na,再加上C02包裹体的发现,表明地幔流体的成分富碱金属、Si、Al、S、Cu、Ni和CO2,地幔交代作用可以使交代产物中Si、Al含量升高而形成中酸性岩浆,也可由于硫化物熔体聚集而形成矿浆．不同地区的地幔流体性质可能存在差异,这些不同性质的地幔流体町能与不同类型的地幔成矿作用有关． 相似文献
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Abundant spinel peridotite xenoliths occur in late Cenozoic alkali basaltic rocks in the Sikhote-Alin region at the Pacific margin of the Asian continent. Major- and trace-element compositions of representative peridotite xenolith are documented for four occurrences located in different structural units of the continental margin. In each locality, the majority of xenoliths have distinctive microstructures, modal and chemical compositions that are typical for a given xenolith suite. Significant textural and compositional differences between the four xenolith suites suggest that the upper mantle beneath the Sikhote-Alin consists of distinct domains with contrasting composition. The inferred large-scale mantle heterogeneities may be due to juxtaposition of lithospheric blocks of different provenance during accretion of the Sikhote-Alin to the Asian continent.
Trace-element patterns of the xenoliths and their minerals obtained ICP-MS technique provide evidence of depletion and enrichment events and indicate contrasting behaviour of REE, HFSE and other incompatible trace elements. The HFSE behave non-concordantly, in particular, some xenoliths have highly fractionated Zr/Hf, Ti/Zr, Nb/Ta, La/Nb and U/Th ratios relative to their values in the primitive mantle. The fractionated compositions may be related to the interaction of evolved subduction-related fluids and melts with lithospheric mantle at the Mesozoic-early Cenozoic active continental margin or to metasomatism during later continental rifting. 相似文献
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《Russian Geology and Geophysics》2007,48(10):811-824
Results of study of different types of inclusions in minerals from mantle xenoliths from the Bele pipe basanites are presented. Two groups of inclusions were recognized in the host minerals according to their genesis. The first group includes single, apparently primary, fluid inclusions. They were discovered only in orthopyroxenes and consist of CO2 (95 mol.%) and N2 (5 mol.%). These inclusions had partly leaked. The densities of two least leaked inclusions from different xenoliths are 1.05 and 1.14 g/cm3, and their trapping pressures are estimated at >8.5 and 12 kbar, respectively. The second group includes syngenetic secondary fluid, melt, and crystalline inclusions. In composition the secondary fluid inclusions differ from the primary ones in higher concentrations of N2 (up to 7 mol.%). Their maximum density is 0.57 g/cm3, which corresponds to 2.4–2.6 kbar and 1100–1200 °C (homogenization temperature of secondary melt inclusions). Comparison of data on melt inclusions in xenolith minerals and host-basanite phenocrysts shows that the secondary inclusions in the xenoliths are, most likely, the result of infiltration and partial reaction of basanitic melt with the xenoliths. On the ascent, the basanitic melt vigorously reacted with mantle xenoliths, which led to the appearance of secondary inclusions in nodule minerals at shallow depths and interstitial mineral assemblages in the xenoliths. 相似文献
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Carbon Enrichment in the Lithospheric Mantle: Evidence from the Melt Inclusions in Mantle Xenoliths from the Hainan Basalts 
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下载免费PDF全文 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
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Djerfisherite, a Cl-bearing potassium sulfide (K6Na(Fe,Ni,Cu)24S26Cl), is a widespread accessory mineral in kimberlite-hosted mantle xenoliths. Nevertheless, the origin of this sulfide in nodules remains disputable. It is usually attributed to the replacement of primary Fe–Ni–Cu sulfides when xenoliths interact with a K-and Cl-enriched hypothetical melt/fluid. The paper is devoted to a detailed study of the composition and morphology of djerfisherite from a representative collection (22 samples) of the deepest mantle xenoliths—sheared garnet peridotite, taken from the Udachnaya-East kimberlite pipe (Yakutia). Four types of djerfisherite were distinguished in the mantle rocks on the basis of morphology, spatial distribution, and relationships with the rock-forming and accessory minerals in the nodules. Type 1 was found in the rims of polysulfide inclusions in the rock-forming minerals of the xenoliths; there, it was younger than the primary sulfide assemblage pyrrhotite + pentlandite ± chalcopyrite. Type 2 formed rims around large polysulfide segregations (pyrrhotite+ pentlandite) in the xenolith interstices. Type 3 formed individual grains in the xenolith interstices together with other sulfides, silicates, oxides, phosphates, and carbonates. Type 4 was present as a daughter phase in the secondary melt inclusions which occurred in healed cracks in the rock-forming minerals of the xenoliths. Along with djerfisherite, the inclusions contained silicates, oxides, phosphates, carbonates, alkaline sulfates, chlorides, and sulfides. The results indicate that djerfisherite from the xenoliths is consanguine with kimberlite. Djerfisherite both in the sheared-peridotite xenoliths from the Udachnaya-East pipe and in different xenoliths from other kimberlite pipes worldwide formed owing to the interaction between the nodules and kimberlitic melts. Djerfisherite forming individual grains in the melt inclusions and xenolith interstices crystallized directly from the infiltrating kimberlitic melt. Djerfisherite bounding the primary Fe–Ni ± Cu sulfides formed by their replacement as a result of a reaction with the kimberlitic melt. 相似文献
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Henry O.A. Meyer 《Earth》1977,13(3):251-281
The importance of ultramafic and eclogitic xenoliths in kimberlite as representing the rocks and minerals of the upper mantle has been widely perceived during the last decade. Studies of the petrology and mineral chemistry of these mantle fragments as well as of inclusions in diamond, have led to significant progress in our understanding of the mineralogy and chemistry of the upper mantle. For example, it is now known that textural differences in the ultramafic xenoliths (lherzolite, harzburgite, pyroxenite and websterite) are partially reflected in chemical differences. Thus xenoliths that display a ‘fluidal’ texture, indicative of intense deformation are less depleted in Ca, Al, Na, Fe and Ti than those xenoliths in which granular textures are predominant. It is believed this relative depletion may indicate the sheared (fluidal texture) xenoliths are representative of primary, undifferentiated mantle. This material on partial melting would produce ‘basaltic-type’ material, and leave a residuum whose chemistry and mineralogy is reflected by the granular xenoliths.Also present in kimberlite are large single phase xenoliths that may be either one single crystal (xenocryst, megacryst) or an aggregate of several crystals of the same mineral (discrete xenolith, or discrete nodule). These large single phase samples consist of similar minerals to those occurring in the ultramafic xenoliths but chemically they are distinct in being generally more Fe-rich. The relation between these xenocrysts to their counterparts in the ultramafic xenoliths is unknown. Also unknown, at the present time, is the exact relation between diamond and kimberlite. Evidence obtained from study of the mineral inclusions in diamond suggests that diamond forms in at least two chemically distinct environments in the mantle; one eclogitic, the other, ultramafic. Interestingly, this suggestion is true for diamonds from worldwide localities.The mineral-chemical results of studies on xenoliths and inclusions in diamond have been convincingly interpreted in the light of experimental studies. It is now possible based on several different geothermometers and barometers to determine relatively reasonable physical conditions for the final genesis of many of these mantle rocks. For the most part the final equilibration temperatures range between 1000 and 1400°C and pressure in the region 100–200 km. These conditions are consistent with an upper mantle origin. Future studies will undoubtedly attempt to more concisely, and accurately, define these conditions, as well as understand better the chemical and spatial relationship of the rock-types in the mantle. 相似文献
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针对松辽盆地南部的双辽火山群中碱性玄武岩及包含其中的地幔捕掳体的普通薄片鉴定、岩石地球化学分析、流体包裹体显微岩相学和激光拉曼光谱分析,研究表明:双辽火山岩以碱性橄榄玄武岩为主,玄武岩中的地幔捕掳体比较发育;对玄武岩斑晶以及地幔捕掳体中的流体-熔融包裹体测试显示玄武岩中的橄榄石斑晶和地幔捕掳体中的流体-熔融包裹体十分发育,其成分主要是CO2,此外还含有少量的CO,CH4,N2和H2O,与上地幔中的自由流体相组分一致。松辽盆地南部的CO2气藏主要是幔源-岩浆成因,成藏时间较晚,主要在新生代,与双辽火山活动的时间接近。尽管双辽火山活动规模较小,但是具有很强的释出CO2的能力,这些富含CO2和H2O的碱性玄武质岩浆很可能并未喷出地表,而是沿着深大断裂进入盆地内部,从而成为松南无机CO2气藏气源体之一。 相似文献