地幔再富集作用对岩石圈地幔Fe-Mg-Ca同位素组成的影响

本文对目前的大洋玄武岩和华北地幔橄榄岩捕虏体的Fe-Mg-Ca同位素研究结果进行了系统的归纳和总结,并在此基础上,探讨地幔再富集作用对岩石圈地幔Fe-Mg-Ca同位素组成的影响,以期为进一步认识华北岩石圈地幔物质组成转变的方式提供新途径。统计结果表明,没有受到地幔交代作用影响的橄榄岩,其Fe-Mg-Ca同位素组成变化范围小,而地幔再富集作用会导致岩石圈地幔的Fe-Mg-Ca同位素组成明显不均一,说明地幔再富集作用是导致岩石圈地幔Fe-Mg-Ca同位素组成变化的重要机制。     

地幔的碳同位素

近年来对金刚石、金伯利岩、碳酸岩、大洋玄武岩、地幔包体等地幔样品的碳同位素越来越多的研究发现，地幔碳的同位素主要集中分布一５‰附近，而在－１５‰￣－２５‰区段有另一较弱的分布。目前的地幔碳的物相转变、沉积碳的俯冲和地幔去气等假说都很难解释这种碳同位素分布，原始地幔可能是碳同位素不均一的。     

中国东部幔源气体同位素地球化学

中国东部地幔岩包体及其单矿物中发育有大量的流体包裹体，采用阶段加热真空热爆的 方法脱出幔源包裹体中的气体，测试了气体的碳、氧、氦、氮等同位素组成。ＣＯ２的σ１３℃普遍较低， 主峰值为（－１８～－２２）×１０－3 ，多数样品在高温下的 σ１３℃普遍小于低温下的对应值。氧同位素变 化也很大，从－３．４×１０－３至２５．５×１０－３（ＳＭＯＷ），并呈现多峰的特征。σ１８Ｏ与σ１Ｃ３具有很好的相 关性，可能受控于同种分馏机制。Ｃ、Ｏ同位素组成特征表明，中国东部大陆地幔具有很大的化学不 均一性，可能是由地幔碳的多样性、源区的不均一性或地幔交代作用所致。氧同位素的变化可能是 结晶作用、去气作用或地壳物质混染所至。４Ｈｅ含量变化范围为（０．２４～２５．００）×１０－８，３Ｈｅ／４Ｈｅ变 化范围为（０．４６～１２．８０）×１０－６，４０Ａｒ含量从０．９７×１０－６到３４．１８×１０－６，４０Ａｒ／３６Ａｒ变化范围为 ２５０．５８～１２０２。３Ｈｅ／４Ｈｅ的变化反映了亏损地幔和富集地幔的存在。不同地区４０Ａｒ／３６Ａｒ的巨大差 异显示了地幔脱气程度的不同，也说明在地幔演化中Ａｒ、Ｈｅ同位素地球化学行为的差异。     

太古宙克拉通岩石圈地幔研究现状评述

本文主要介绍了太古宙克拉通岩石圈地幔的一些基本特征，国内外有关早期地幔研究的最新进展和发展趋势，主要包括以下几方面：１．太古宙岩石圈地幔的岩石组成和化学组成；２．太古宙地幔同位素体系；３．太古宙地幔热状态和结构特征；４．幔内地质事件。通过研究主要获得以下认识：１．早太古代岩石圈演化以壳－幔分异作用为主，晚太古代以壳内分异作用为主；２．太古宙存在一个又厚又冷（２００ｋｍ）的岩石圈；３．幔内地质作用与     

地幔橄榄岩中橄榄石的指示意义

橄榄石是地幔橄榄岩和辉石岩的主要组成矿物,但也经常以斑晶和捕虏晶的形式出现在玄武质岩石中。结合近年来在地幔橄榄岩的主要元素（如Mg和Fe）组成特征以及Li、Mg和Fe稳定同位素地球化学方面的研究成果,重点对橄榄石的地球化学特征与华北克拉通岩石圈地幔演化过程之间的联系进行了讨论,旨在加深对华北克拉通岩石圈地幔演化过程的理解。现有研究表明：地幔橄榄岩中橄榄石的矿物学特征、元素和同位素地球化学组成能够很好地指示岩石圈地幔的特征及其演化过程,因而具有重要的意义。对于克拉通地区的地幔橄榄岩来说,橄榄石的Mg#通常可以指示岩石圈地幔的属性,古老、难熔的地幔橄榄岩中的橄榄石一般具有较高的Mg#（〉92）,而新生的岩石圈地幔橄榄岩中的橄榄石则具有较低的Mg#（〈91）。因此,地幔橄榄岩中橄榄石的Mg#在一定程度上具有年龄意义。橄榄岩中橄榄石的Li、Mg和Fe同位素组成也可以明确指示岩石圈地幔的属性及其所经历的演化过程,正常地幔的δ7Li、δ26Mg和δ57Fe组成相对均一,如果上述同位素组成偏离正常地幔值,则说明岩石圈地幔经历了熔体/流体的交代作用。华北克拉通地区地幔橄榄岩捕虏体中橄榄石的Li、Mg和Fe同位素组成研究表明：该区的岩石圈地幔经历了多个阶段、不同来源的熔体/流体的改造过程。     

江苏盘石山二辉橄榄岩包体的Nd、Sr、Pb同位素特征

对盘石一带的６个二辉橄榄岩包体，３个单斜辉石的Ｎｄ、Ｓｒ同位素，４个全岩、７个单斜辉石和１个斜方辉石的铅同位素进行了测定。结果表明，它们在亏损的岩石圈中经历了长时间的演化，其Ｒｂ－Ｓｒ、Ｓｍ－Ｎｄ、Ｐｂ－Ｐｂ同位素体系的相关性可能反映了不同时期的地幔过程。位于陆下岩石圈地幔中上部位的包体比下部岩石圈地幔具有相对亏损和不均一的同位素特征。     

山东中生代橄榄安粗岩系火山岩的地质、地球化学特征及岩石成因

山东中生代橄榄安粗岩系火山岩主要分布在沂沭断裂带及其两侧的断陷型陆相火山盆地中，为早白垩世火山活动的产物．Ｒｂ－Ｓｒ全岩等时年龄变化于１１１．４～１１９．６Ｍａ．岩石组合主要为粗面玄武岩－橄榄安粗岩－安粗岩－粗面岩．这套岩石在化学上具有富碱富钾、富铝贫钛、高氧化系数及富轻稀土和大离子亲石元素的特点，并具有较高的ＩＳｒ值和明显偏低εＮｄ值．根据对岩石地质、地球化学特征和产出构造环境的详细分析，表明这套岩石的成因应主要是富集型地幔的部分熔融     

中国东部新生代玄武岩的地球化学（Ⅱ）Sr、Nd、Ce同位素组成

对有代表性的中国东部新生代玄武岩的Ｓｒ、Ｎｄ和Ｃｅ同位素组成进行了系统的研究，结合系统的微量元素研究结果，进一步阐明其地幔源区同位素组成的不均一性；利用Ｃｅ、Ｎｄ同位素地球化学给出的信息，探讨富集Ⅰ型（ＥＭⅠ）地幔端元的成因。     

华北中、新生代岩石圈地幔的交代作用：含金云母地幔岩提供的证据

本文对华北克拉通三个不同地区(河北汉诺坝、内蒙古集宁三义堂、河南鹤壁)新发现的含金云母尖晶石二辉橄榄岩和尖晶石橄榄单斜辉石岩捕虏体进行了详细的矿物组成、单斜辉石的微量元素和 Sr-Nd 同位素研究。通过与相同地区不含金云母尖晶石二辉橄榄岩捕虏体的系统对比发现通常含金云母的地幔橄榄岩比不含金云母的地幔橄榄岩岩富 Al_2O_3、CaO、NaO、K_2O、TiO_2,但相对贫镁;其单斜辉石的 LREE 更为富集,但 Sr、Nd 同位素组成则相对亏损。这说明地幔交代作用不仅能够造成地幔橄榄岩的玄武质组分和稀土元素的富集,而且亦能够造成全岩和橄榄石 Mg~#的降低和同位素组成的相对亏损。捕虏体的 Rb-Sr 等时线年龄暗示地幔交代作用发生在中、新生代;其交代熔体来源于软流圈。同时说明华北新生代岩石圈地慢普遍存在的主、微量元素和同位素组成类似于"大洋型"岩石圈地幔的特征很可能是岩石圈地幔橄榄岩与软流圈来源的熔体的大规模反应的结果,而非真正意义上的新增生的岩石圈地幔。     

云南老王寨金矿区煌斑岩的成因：稀土元素研究

云南老王寨金矿区煌斑岩与金矿化在时间上、空间上密切共生。主要元素分析表明，本区煌斑岩属钾质－富钾质钙碱性煌斑岩；与原始地幔和大洋中脊玄武岩相比，岩石相对富集稀土元素；模拟计算表明，岩石来源于稀土元素相对富集的交代富集地幔；地质发展史、不相容元素分配型式、Ｓｒ、Ｎｄ同位素组成及有关模拟计算表明，俯冲进入地幔楔的地壳物质脱水 流体是引起该区地幔交代作用的主要因素。     

中国大陆地壳铅同位素演化的动力学模型

根据中国大陆中、新生代花岗岩长铅同位素数据库,沿用“铅构造模型”的基本思想并作部分改进,建立了中国大陆地壳铅同位素的动力学演化模型。与全球平均的铅同位素演化曲线相比,中国大陆地壳的原始物质相对较贫铀富钍,并且中国大陆的上地壳和下地壳在演化过程中分异得更加彻底。将本模型应用于大别地区中生代花岗岩长石铅同位素数据,结果发现它们具有壳幔铅混合的特征,并且以上下地壳物质混合产生的类地幔铅为主,花岗岩源岩中含有较高的富Th下地壳组分。     

非传统同位素体系在地幔地球化学研究中的重要性及其前景

非传统同位素体系(如Hf、Os、Li、Fe、Ti、Mg、He、Ar等)是相对于传统同位素体系(如Sr、Nd、Pb、O等)而言的,即新近发展起来的同位素体系。随着同位素测试技术的进步和多接收电感耦合等离子体质谱仪(MC-ICP-MS)、二次离子质谱仪(SIMS)以及激光剥蚀技术配合MC-ICP-MS(LA-MC-ICP-MS)等测试手段的开发应用,多种同位素体系(包括放射性同位素和稳定同位素体系)的示踪作用在地学研究中得到了日益广泛的应用。在简要介绍传统同位素体系的基础上,旨在总结报道近年来国际上有关非传统同位素体系在地幔地球化学研究中取得的重要成果,展示这些同位素体系在地幔地球化学研究中的重要性及其可能的应用前景,以加速我国在非传统同位素地球化学方面的应用研究。     

Heterogeneous lithospheric mantle metasomatism in the eastern North China Craton: He–Ar isotopes in peridotite xenoliths from Cenozoic basalts

The abundances and isotopic compositions of Helium and Argon have been analyzed in a suite of fresh spinel peridotite xenoliths in Cenozoic basalts from the eastern North China Craton (NCC) by step-wise heating experiments, to investigate the nature of noble gas reservoirs in the subcontinental lithospheric mantle beneath this region. The xenoliths include one harzburgite collected from Hebi in the interior of the NCC, two lherzolites from Hannuoba at the northern margin of the craton, and three lherzolites from Shanwang and Nushan on the eastern margin. ³He/⁴He ratios in most of the xenoliths are similar to those of mid-ocean ridge basalts (MORB) or slightly lower (2–10.5 Ra, where Ra is the ³He/⁴He ratio of the atmosphere), suggesting mixing of MORB-like and radiogenic components. One olivine separate from Nushan has a helium value of 25.3 Ra, probably suggesting cosmogenic ³He addition. The ⁴⁰Ar/³⁶Ar ratios vary from atmospheric value (296) to 1625, significantly lower than the MORB value. Available data of the peridotite xenoliths indicate the He and Ar isotopic systematics of the mantle reservoirs beneath the NCC can be interpreted as mixtures of at least three end-members including MORB-like, radiogenic and atmospheric components. We suggest that the MORB-like noble gases were derived from the underlying asthenosphere during mantle upwelling, whereas the radiogenic and recycled components probably were incorporated into the lithospheric mantle during circum-craton subduction of oceanic crust. Available data suggest that the MORB-like fluids are better preserved in the interior of the NCC, whereas the radiogenic ones are more prevalent at the margins. The Paleo-Asian ocean subduction system probably was responsible for the enriched and recycled noble gas signatures on the northern margin of the craton, while the Pacific subduction system could account for the observed He–Ar isotopic signatures beneath the eastern part. Therefore, integration of helium and argon isotopes reflects heterogeneous metasomatism in the lithospheric mantle and demonstrates the critical importance of lithospheric mantle modification related to both circum-craton subduction of oceanic crust and asthenospheric upwelling beneath the eastern NCC.     

Sr–Nd–Pb isotopic constraints on the nature of the mantle sources involved in the genesis of the high-Ti tholeiites from northern Paraná Continental Flood Basalts (Brazil)

There has been little research on geochemistry and isotopic compositions in tholeiites of the Northern region from the Paraná Continental Flood Basalts (PCFB), one of the largest continental provinces of the world. In order to examine the mantle sources involved in the high-Ti (Pitanga and Paranapanema) basalt genesis, we studied Sr, Nd, and Pb isotopic systematics, and major, minor and incompatible trace element abundances. The REE patterns of the investigated samples (Pitanga and Paranapanema magma type) are similar (parallel to) to those of Island Arc Basalts' REE patterns. The high-Ti basalts investigated in this study have initial (133 Ma) ⁸⁷Sr/⁸⁶Sr ratios of 0.70538–0.70642, ¹⁴³Nd/¹⁴⁴Nd of 0.51233–0.51218, ²⁰⁶Pb/²⁰⁴Pb of 17.74–18.25, ²⁰⁷Pb/²⁰⁴Pb of 15.51–15.57, and ²⁰⁸Pb/²⁰⁴Pb of 38.18–38.45. These isotopic compositions do not display any correlation with Nb/Th, Nb/La or P₂O₅/K₂O ratios, which also reflect that these rocks were not significantly affected by low-pressure crustal contamination. The incompatible trace element ratios and Sr–Nd–Pb isotopic compositions of the PCFB tholeiites are different to those found in Tristan da Cunha ocean island rocks, showing that this plume did not play a substantial role in the PCFB genesis. This interpretation is corroborated by previously published osmium isotopic data (initial γ_Os values range from +1.0 to +2.0 for high-Ti basalts), which also preclude basalt generation by melting of ancient subcontinental lithospheric mantle. The geochemical composition of the northern PCFB may be explained through the involvement of fluids and/or small volume melts related to metasomatic processes. In this context, we propose that the source of these magmas is a mixture of sublithospheric peridotite veined and/or interlayered with mafic components (e.g., pyroxenites or eclogites). The sublithospheric mantle (dominating the osmium isotopic compositions) was very probably enriched by fluids and/or magmas related to the Neoproterozoic subduction processes. This sublithospheric mantle region may have been frozen and coupled to the base of the Parana basin lithospheric plate above which the Paleozoic subsidence and subsequent Early Cretaceous magmatism occurred.     

A theoretical approach to understanding the isotopic heterogeneity of mid-ocean ridge basalt

We have developed an idealized mathematical model to understand the isotopic variability of the mantle and its relation to the observed variations in isotopic ratios ¹⁴³Nd/¹⁴⁴Nd, ⁸⁷Sr/⁸⁶Sr, ¹⁷⁶Hf/¹⁷⁷Hf, ²⁰⁸Pb/²⁰⁴Pb, ²⁰⁶Pb/²⁰⁴Pb, and ²⁰⁷Pb/²⁰⁴Pb measured on mid-ocean ridge basalt (MORB). We consider a simple box model of mantle processes. A single melt region produces a melt fraction F of melt, and the average time since a given parcel of mantle material last visited this region is given by the time scale τ_melt. The melt region fractionates the parent/daughter ratios. Over time this leads to variations in the mantle isotopic ratios as the parent decays to the daughter. Key assumptions are that the half-life of the parent isotope is large compared with τ_melt, that the flow is strongly stirring, and that the mantle has reached a statistical steady state. This enables us to neglect the specifics of the underlying flow. Sampling from our model mantle is dealt with by averaging over a large number N of samples to represent the mixing after melting.The model predicts a probability density for isotopic ratios in MORB which, with exception of the Pb isotopes, are consistent with measurements. Fitting the MORB data to this model gives estimates of the model parameters F, τ_melt, and N. Small melt fractions with F around 0.5% are essential for a good fit, whereas τ_melt and N are less well constrained. τ_melt is estimated at around 1.4 to 2.4 Ga, and N is of the order of hundreds. The model predicts a larger variability for the Pb isotopes than that observed. As has been stated by many previous authors, it appears that fundamental differences exist between the dynamics of Pb isotopes and those of Nd, Sr and Hf isotopes.     

Geochemical and Nd–Pb isotopic characteristics of the Tethyan asthenosphere: implications for the origin of the Indian Ocean mantle domain

It is unclear why the Pb, Nd, and Sr isotopic composition of the modern mid-ocean ridge basalts (MORB) from the Indian Ocean is different from that of the North Atlantic and Pacific Oceans. A possible explanation for this is that the Indian MORB-type isotopic signature is a long-lived regional feature of the mantle, as evidently shown by the isotopic composition of the 350 Ma MORB-like Mian-Lue northern ophiolite, which was formed in the same region presently occupied by the Indian Ocean. However, this hypothesis is in conflict with the lack of Indian MORB-type isotopic signature in a number of 150 Ma Tethyan and Indian Ocean crusts. To further constrain the origin of the Indian MORB-type isotopic signature, we analyze the geochemical and Pb, Nd, and Sr isotopic composition of representative mafic rocks from four Tethyan ophiolites ranging in age from 90 to 360 Ma. The Sr isotopic composition of the samples is unreliable due to alteration, but the age-corrected Nd and Pb isotopic ratios and geochemical data indicate that these Tethyan rocks were derived from a geochemically depleted asthenospheric source that had a clear Indian MORB-type isotopic signature. We therefore conclude that the bulk of the Indian suboceanic mantle was most probably inherited from the Tethyan asthenosphere. A few regions in both the Tethyan and Indian Oceans, however, are most probably underlain by Pacific and North Atlantic MORB-type mantle (and vice-versa) because of the flow of the asthenosphere in response to tectonic plate reorganizations that lead to openings and closures of ocean basins. The Indian MORB-type isotopic signature of the western Pacific marginal basin crusts could be due to either flow of the Indian Ocean mantle into the western Pacific or to endogenous production of such an isotopic signature from delaminated East-Asian sublithospheric materials during closure of the Tethys Ocean.     

Pb-Sr-He isotope and trace element geochemistry of the Cape Verde Archipelago

New lead, strontium and helium isotopic data, together with trace element concentrations, have been determined for basalts from the Cape Verde archipelago (Central Atlantic). Isotopic and chemical variations are observed at the scale of the archipelago and lead to the definition of two distinct groupings, in keeping with earlier studies. The Northern Islands (Santo Antão, São Vicente, São Nicolau and Sal) present Pb isotopic compositions below the Northern Hemisphere Reference Line (NHRL) (cf. Hart, 1984), unradiogenic Sr and relatively primitive ⁴He/³He ratios. In contrast, the Southern Islands (Fogo and Santiago) display Pb isotopes above the NHRL, moderately radiogenic Sr and MORB-like helium signatures. We propose that the dichotomy between the Northern and Southern Islands results from the presence of three isotopically distinct components in the source of the Cape Verde basalts: (1) recycled ∼1.6-Ga oceanic crust (high ²⁰⁶Pb/²⁰⁴Pb, low ⁸⁷Sr/⁸⁶Sr and high ⁴He/³He); (2) lower mantle material (high ³He); and (3) subcontinental lithosphere (low ²⁰⁶Pb/²⁰⁴Pb, high ⁸⁷Sr/⁸⁶Sr and moderately radiogenic ⁴He/³He ratios). The signature of the Northern Islands reflects mixing between recycled oceanic crust and lower mantle, to which small proportions of entrained depleted material from the local upper mantle are added. Basalts from the Southern Islands, however, require the addition of an enriched component thought to be subcontinental lithospheric material instead of depleted mantle. The subcontinental lithosphere may stem from delamination and subsequent incorporation into the Cape Verde plume, or may be remnant from delamination just before the opening of the Central Atlantic. Basalts from São Nicolau reflect the interaction with an additional component, which is identified as oceanic crustal material.     

分步淋洗方法研究碧溪岭榴辉岩Pb同位素组成及其演化

根据大量年代学、地球化学和岩石学等方面的研究,前人对碧溪岭榴辉岩的形成及变质历史有了较明确的认识,但这些研究对超高压变质前后过程中元素和同位素的变化涉及较少。通过分步淋洗方法对碧溪岭榴辉岩中石榴石的Pb同位素研究发现,不同淋洗步骤的Pb同位素组成明显不同,但对不同的石榴石样品以及同一样品用不同的淋洗流程,得到的淋洗规律以及Pb同位素组成变化范围基本一致。不同淋洗步骤的Pb同位素组成构成等时线,给出表面年龄为30亿年左右,与前人报道的碧溪岭地区榴辉岩原岩形成及超高压变质的年龄数据有明显差异。结合前人研究可以判断,这些年龄不具有明确的地质意义,属于假等时线。但分步淋洗结果能反映碧溪岭榴辉岩中Pb同位素的来源可能由地幔组分和上地壳组分混合而成,地幔组分的Pb反映了碧溪岭榴辉岩的原岩是地幔成因的,上地壳组分的Pb表明在榴辉岩快速折返过程中,受到具有上地壳Pb同位素组成的含水流体交代     

He, Sr, Nd, and Pb isotopic constraints on the origin of the Marquesas and other linear volcanic chains

The classic hotspot hypothesis [Morgan, W. J., 1971. Convection plumes in the lower mantle. Nature 230, 42–43], which posits that linear volcanic chains are traces of fixed plumes in the mantle on moving lithospheric plates, was instrumental in elevating the plate tectonics paradigm in the 1960s into a modern Earth Science theory. The hypothesis itself, however, remains conjectural because many of its predictions, particularly the simple age-progressive type of volcanism, are not observed in many linear volcanic chains. As an alternative explanation, it is proposed that linear volcanic chains are formed through magmatism along pre-existing lines of weakness such as transform zones and old sutures, or along cracks created by stresses on lithospheric plates. The Marquesas linear volcanic chain in south-central Pacific has geologic features that are consistent with some of the predictions of both hypotheses. To better constrain the origin of this volcanic chain, we collected major and trace element and Sr, Nd, Pb, and He isotopic data from several Marquesan lavas. Our new analyses combined with literature data classify the samples into the well established tholeiitic to mildly alkalic, low ⁸⁷Sr/⁸⁶Sr, high ¹⁴³Nd/¹⁴⁴Nd, shield-building volcanic phase lava group and highly alkalic, high ⁸⁷Sr/⁸⁶Sr, low ¹⁴³Nd/¹⁴⁴Nd, post-shield phase group. Lead isotopes show generally higher ²⁰⁶Pb/²⁰⁴Pb ratios and suggest evidence of crustal assimilation for the shield-building phase lavas, consistent with the argument that the shield-building phase volcanism has a lithospheric source component. On the other hand, post-shield phase lavas that are predicted to represent the true composition of the mantle source by the hotspot hypothesis have higher ³He/⁴He ratios and these are coupled to other geochemical tracers. Thus our results show that the Marquesas volcanic chain, similar to many other linear volcanic chains, has a high ³He/⁴He component in its mantle source. The presence of such a distinct source component cannot be easily explained by dispersed upper mantle heterogeneities, but provides a powerful constraint for the hotspot origin of many linear volcanic chains.