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1.
埃达克质岩石是高Na、Al和Sr、低Y和HREE以及Nb、Ta亏损的钠质花岗质岩石,奥长花岗岩-英云闪长岩-花岗闪长岩(TTG)是早期(太古宙)大陆壳主要组分,成分与埃达克质岩石相似,这些成分独特的岩石总体上认为是俯冲洋壳、下地壳和拆沉的下地壳中变质玄武岩部分熔融的产物。文中综述我们近年来在变质玄武岩体系相平衡和矿物-熔体微量元素分配实验研究成果:相平衡实验和熔体微量元素特征研究表明,变质玄武岩部分熔融过程中金红石是导致TTG/埃达克岩浆Nb、Ta亏损的必要残留矿物,从而否定了前人“TTG由无金红石的角闪岩熔融产生”的观点;证实金红石仅仅在压力1.5GPa以上才能稳定存在,从而限定TTG/埃达克岩熔体必定产生在大约50km以上,表明TTG/埃达克岩是在相对较深的含金红石榴辉岩相条件下熔融产生的。矿物(石榴子石、角闪石,单斜辉石和金红石)-熔体微量元素分配系数测定和部分熔融模拟结果进一步限定俯冲洋壳和下地壳起源的TTG/埃达克岩浆由含金红石角闪榴辉岩熔融产生,而拆沉下地壳起源的埃达克岩浆的产生要求软流圈地幔高温,由无水或含有少量含水矿物的榴辉岩熔融产生。  相似文献   

2.
王丹  郭敬辉  马旭东 《岩石学报》2021,37(2):341-355
英云闪长岩-奥长花岗岩-花岗闪长岩(TTG)是地球早期大陆地壳最重要的组成部分。TTG的Nb/Ta比值变化不仅与它的成因相关,而且与早期构造环境和地壳分异过程关系紧密。本文选择阴山地块出露的TTG片麻岩及下地壳斜长角闪岩/麻粒岩包体作为研究对象,开展了寄主花岗闪长岩和同源镁铁质包体中的角闪石和黑云母的原位微区矿物的微量元素分析工作,以及TTG与非同源斜长角闪岩包体的全岩主微量元素分析工作。矿物化学研究结果表明,花岗闪长岩和同源镁铁质包体的角闪石具有相似的Mg#值,但是两者具有明显不同的Nb/Ta比值。镁铁质包体中的角闪石更富Cr、Ta,Nb/Ta比值为30~50;TTG岩石中的角闪石Cr和Ta含量偏低,但具有更高的Nb/Ta比值(38~70)。TTG和镁铁质包体中的角闪石Cr含量与Nb/Ta具有较好的负相关关系。全岩地球化学分析结果揭示,TTG片麻岩的具有高Nb/Ta比值(13~65,平均值31),斜长角闪岩和麻粒岩包体具有变化的Nb/Ta比值(10~56)。太古宙绿岩带中玄武质岩石的Nb/Ta平均值为~15,阴山地块斜长角闪岩和麻粒岩包体具有高的Nb/Ta比值,反映了这些代表基性下地壳的岩石经历了部分熔融作用或后期的交代作用,使其Nb/Ta比值发生改变。研究区具有高Nb/Ta比值的TTG可能来源于高Nb/Ta比值基性下地壳部分熔融,并继承了源区高Nb/Ta比值的特征。通过本文研究揭示,高Nb/Ta比值的TTG并非一定形成于俯冲带洋壳榴辉岩相部分熔融,下地壳富角闪石和黑云母的岩石部分熔融是形成高Nb/Ta比值TTG的一种重要途径。  相似文献   

3.
Nb,Ta的硅酸盐地球质量不平衡问题争论由来已久,备受关注。近年来研究发现,含金红石的榴辉岩Nb/Ta往往高于球粒陨石值(Nb/Ta=17.5),暗示其可能是平衡地球Nb亏损的独立储库。而洋壳玄武岩部分熔融实验表明Ta比Nb更倾向进入金红石晶格,这意味着作为俯冲洋壳部分熔融残留相的榴辉岩Nb/Ta不可能高于原岩。为了解释地质观察和实验结果之间的矛盾,系统分析了中国大陆科学钻探工程(CCSD)主孔、先导孔及附近地表榴辉岩的矿物微量元素。结果发现:榴辉岩中的Nb,Ta主要存在于金红石之中,其他矿物中含量极少;Nb,Ta之间存在着强烈分异(Nb/Ta=5.3~96.2),并总体上具有超球粒陨石的特征;韭闪石和多硅白云母的Nb/Ta平均分别为48.6,21.8,显示了很强的Nb,Ta分异能力;其他矿物如石榴石、绿辉石、绿帘石、磷灰石等的Nb、Ta含量及Nb/Ta都很低,对Nb-Ta分异不造成影响。认为导致Nb-Ta分异的不是金红石,而应出现在洋壳俯冲过程中金红石相出现之前的脱水和部分熔融阶段。富含Ti的角闪石(韭闪石)和白云母可能对Nb-Ta分异起到了决定性的作用。等金红石相出现之后,由于其对Nb,Ta的绝对控制作用,此前阶段的分异结果便被固定在金红石中而继承下来。因此,含金红石的榴辉岩常常表现出超球粒陨石Nb/Ta的特征,与金红石不能有效地分异Na,Ta的实验结果之间并不矛盾。在不均匀的上地幔中含金红石的榴辉岩是可能的超球粒陨石Nb/Ta储库之一。  相似文献   

4.
利用LA-ICP-MS对CCSD-MH超高压榴辉岩中金红石进行了详细的原位微区微量元素组成分析.金红石中高场强元素Nb和Ta含量主要受全岩Nb、Ta和TiO2含量控制, Zr、Hf含量比较稳定基本不受全岩含量影响.粒间金红石中, 同一颗粒金红石核部Zr含量系统高于边部, 而边部则出现了明显的Pb和Sr富集特征.CCSD-MH榴辉岩中金红石与全岩的Nb/Ta比值呈现明显的不一致性.全岩Nb/Ta比值明显低于金红石且与全岩TiO2含量负相关, 而金红石的Nb/Ta比值与全岩Nb、Ta含量和Nb/Ta比值没有明显的相关关系.金红石和全岩之间非完全耦合的Nb/Ta组成表明, 金红石并非形成于原岩的结晶过程中而是在超高压变质作用过程中形成, 尽管金红石是榴辉岩中Nb、Ta含量的主要载体矿物, 但金红石的Nb/Ta比值并不一定能完全代表全岩的特征, 而与全岩Nb、Ta和TiO2的含量有关.粒间金红石核部Zr含量所记录的温度与粒径之间具有明显的正相关性, 反映金红石中的Zr在其形成后没有封闭.粒间金红石所表现出的明显的边部富集Pb和Sr的特征, 反映了后期流体活动对金红石组成的影响.这些研究结果为金红石中Zr在高温下的扩散作用和后期流体活动的影响提供了重要证据, 这可能是利用金红石Zr含量地质温度计计算的苏鲁-大别榴辉岩变质温度(598~827℃) 偏低的主要原因.   相似文献   

5.
南迦巴瓦地区广泛出露的中下地壳变基性岩部分熔融形成的层状混合岩和淡色花岗岩,为研究部分熔融过程中榍石的地球化学行为对熔体的微量元素组成的影响提供了良好的机会。相对于源岩或熔融残留体,淡色体亏损Ti、V、REE、Y、Nb、Ta、U等元素,与混合岩中榍石的微量元素特征互补。混合岩、淡色体和榍石微量元素特征表明南迦巴瓦角闪岩部分熔融形成的淡色体的微量元素特征主要受控于榍石的地球化学行为。角闪岩脱水部分熔融过程中,由于长英质熔体的低Ti溶解度,榍石以未熔残留体形式存在于暗色体中,导致熔体亏损Ti、REE、Nb、Ta、V、U等元素和Sr/Y比值相对升高。关键元素在榍石和熔体之间的配分系数受熔体成分影响明显。角闪岩中变质榍石DNb/Ta<1,因此变质榍石残留导致熔体Nb/Ta相对于源岩升高;而高Si-Al花岗质熔体中榍石DNb/Ta>1,因此与高Si-Al熔体平衡的榍石的分离(转熔或结晶分异)将导致熔体Nb/Ta比值相对源岩降低。榍石在部分熔融过程中的微量元素效应为理解变基性岩部分熔融产生熔体的地球化学特征提供新的认识。  相似文献   

6.
基性岩高温-超高温变质作用与TTG质岩成因   总被引:10,自引:6,他引:4  
魏春景  关晓  董杰 《岩石学报》2017,33(5):1381-1404
变质基性岩在高温-超高温下部分熔融可以形成TTG(英云闪长质-奥长花岗质-花岗闪长质)质熔体,有关熔融反应机理、熔体地球化学特征以及太古宙TTG质岩石成因问题备受国内外学者关注。本文基于对相关实验岩石学研究的总结,结合基性岩高温-超高温相平衡的模拟计算,分析了变质基性岩(斜长角闪岩)深熔变质反应过程、P-T条件及其与TTG质岩石成因的联系。变质基性岩高温-超高温深熔作用主要受角闪石脱水熔融反应控制。在1.0GPa以下的无石榴石域,角闪石分解反应主要为:角闪石=单斜辉石+斜方辉石+斜长石+熔体(R1),该反应为多变滑动反应,以斜方辉石出现(800℃)和角闪石消失(1000~1100℃)为标志,其滑动温度范围超过200~300℃。实验岩石学确定的斜长角闪岩开始熔融或缺流体固相线大致相当于斜方辉石出现温度。实际上角闪石脱水熔融反应是从饱和水固相线开始的,反应为:角闪石+石英=单斜辉石+斜长石+熔体(R1a),开始有黑云母参与熔融反应,但该反应对熔体贡献有限。在1.0GPa以上的石榴石域,不同实验所确定的石榴角闪岩缺流体固相线温度主要介于800~900℃之间,固相线表现为正斜率、负斜率、或者为与压力无关的直线等不同结果。相平衡模拟计算表明在石榴石稳定域角闪石脱水熔融反应为较陡的负斜率,分为两部分:当有斜长石存在时,反应为角闪石+斜长石+石英=石榴石+单斜辉石+熔体(R2),低温部分有白云母、绿帘石参与反应。该反应从饱和水固相线(约630℃)开始,到角闪石消失(超过1000℃),滑动温度范围可超过400℃,跨越石榴角闪岩亚相与角闪高压麻粒岩亚相范围;在斜长石消失后角闪石脱水熔融反应为角闪石+石英=石榴石+单斜辉石+熔体(R2a),低温部分有绿帘石、白云母参与熔融反应,该反应从饱和水固相线(约650℃)开始,到角闪石消失(超过900℃),滑动温度范围可超过200~300℃。角闪石脱水熔融反应形成的无水残余物形成麻粒岩和榴辉岩,无水麻粒岩的峰期温度会超过1000℃,由于降温过程中的退变质演化,如超固相线下滞留熔体与残余物之间发生的深熔反应的逆反应,以及在亚固相线下离子交换反应,导致大多数麻粒岩只记录缺流体固相线组合与退变质温度。基性岩部分熔融的熔体成分取决于全岩成分、P-T条件及熔融程度。当熔融程度很低时(如小于5%)可形成富钾花岗质熔体,随着熔融程度增加,熔体成分可转变为奥长花岗质(如5%~20%)和英云闪长质(如大于20%),部分熔融的熔体成分受全岩成分影响很大,只有相对富钾的基性岩才能形成花岗闪长质到石英二长质熔体。太古宙TTG质岩石表现出富Sr、低Y、Yb、Nb、Ta、Ti以及稀土分馏程度高等地球化学特征,要求部分熔融压力较高,残余物中有石榴石(及金红石)存在。争论的焦点是部分熔融究竟发生在石榴角闪岩亚相(及角闪高压麻粒岩亚相),还是发生在榴辉岩相。对此,不同实验给出的不同结论应该与源岩地球化学特征不同有关。考虑到TTG质岩石的可能源岩如太古宙科马提岩和玄武岩地球化学特征的多样性,TTG质岩石本身地球化学特征上的差异也许不能完全指示熔融发生的P-T条件。综合实验岩石学和相平衡模拟结果,本文确定TTG质岩石是由基性岩在角闪石和石榴石共同稳定域由角闪石脱水熔融反应R2和R2a在角闪高压麻粒岩亚相和角闪榴辉岩亚相形成的,P-T条件为1.0~2.5GPa和800~1000/1100℃。角闪高压麻粒岩亚相相对应的地热梯度为15~25℃/km,角闪榴辉岩亚相对应的地热梯度为10~15℃/km。TTG质岩石形成的构造环境不能简单对应发生在显生宙的洋壳热俯冲带、碰撞造山带和洋底高原等。  相似文献   

7.
奥长花岗岩-英云闪长岩-花岗闪长岩岩套(TTG),是地球上最古老(太古宙)陆壳的最主要组成,通常认为是俯冲的玄武质洋壳或玄武质下地壳部分熔融产生的.目前,变质玄武岩残留矿物(石榴子石、角闪石、单斜辉石和金红石)与中酸性熔体之间微量元素分配系数的研究相对有限,这对于理解早期大陆壳的起源和生长机制无疑是十分不利的.  相似文献   

8.
金红石边缘形成榍石冠状边结构在变质中-基性岩中普遍存在,是金红石与退变质流体携带的SiO_2与CaO作用的结果,反应形成的榍石微量元素特征受到金红石和流体的共同影响。雅鲁藏布江缝合带中角闪岩LZ06-04在抬升过程经历近等温降压退变质作用,石榴子石分解导致同一样品中含石榴子石部分与不含石榴子石部分的退变质流体成分的差异。两种流体分别与金红石反应,对应形成的榍石具有相似的Nb、Ta含量和Nb/Ta比值特征,但截然不同的REE特征。榍石的Nb、Ta来源于金红石,残余金红石与含水流体再平衡Nb、Ta的分配系数增大,且D_(Nb)~(Rt/Fluid)≥D_(Ta)~(Rt/Fluid);虽然Nb和Ta在含水流体中都表现为不活动元素,但相对于Nb,Ta在含水流体中活动性较高。榍石的Zr-Hf体系特征受到锆石、石榴子石等矿物的综合影响,并且Zr-Hf在含水流体中表现出比Nb-Ta更高的活动性。榍石的REE特征受流体中REE特征、榍石与流体配分系数以及共生矿物的影响。在岩浆或变质体系,榍石形成过程中,REE富集矿物(如石榴子石、锆石、褐帘石、独居石、磷灰石等)形成或分解将影响榍石的REE分布特征或形成REE环带结构。含水流体中金红石退变质形成榍石反应的进行受流体中TiO_2、CaO和SiO_2活度的影响。因此榍石常见于钙碱性岩浆岩、富Ca基性变质岩和矽卡岩中。流体中CaO活度的变化影响榍石的形成,进而影响Ti、Nb、Ta在流体中的运移能力。俯冲板片产生流体在交代上覆富Ca地幔楔物质过程中形成榍石残留同样可以造成部分熔融体具有亏损HFSE特征。  相似文献   

9.
北京西山东岭台组粗面质火山岩地球化学:下地壳熔融成因   总被引:13,自引:2,他引:11  
北京西山东岭台组粗面岩表现出LREE富集和HREE平坦的稀土配分型式 ,富集LILE (Ba、K和Sr)、和亏损Nb Ta、Th U和Ti,Sr Nd同位素组成富集 (87Sr/ 86Sr(t) =0 .70 6 38~ 0 .70 6 72 ,Nd(t) = 1 6 .3~ - 1 5 .7)。结合所表现出的明显Nb/Ta分馏和高的Zr/Sm比值 ,认为它们来源于大陆下地壳含石榴子石的角闪岩部分熔融作用而成 ,主要的残留相为石榴子石 +斜长石±角闪石±辉石。根据地壳岩石熔融实验研究结果 ,西山地区东岭台组粗面岩的熔融要求有外来的热源参与 ,与区域上同时代发生的玄武岩浆底侵作用具时空上的密切联系 ;这些岩石所显示的高Sr和Ba特征也暗示至少有部分底侵的玄武质岩石参与了部分熔融作用  相似文献   

10.
在1.5GPa,950℃,恒温101h条件下对华北北缘太古宙地体中的斜长角闪岩块状样品进行了脱水部分熔融实验,实验产物组合为Hb+Cpx+Gt+Gl,获得的熔体为花岗闪长质成分。利用LA-ICP-MS测试了矿物和熔体的微量元素,获得该体系内各矿物/熔体的微量元素分配系数。角闪石、单斜辉石和石榴石的分配系数与前人在类似条件下的实验结果基本一致。这说明无论实验的初始物质是粉末状还是块状,对元素的分配没有太大的影响。各矿物的REE分配系数对离子半径的拟合曲线很好地符合晶格应变弹性模型。整体特征上,角闪石、单斜辉石和石榴石的LILE,LREE分配系数较低,而HREE的分配系数较高,石榴石具有强烈富集HREE的特征。由此,造成实验熔体表现出LILE、LREE富集而HREE亏损的特征。残留相中无金红石,使得熔体中没有明显的Nb、Ta负异常。熔体的主-微量元素特征符合华北北缘中生代埃达克质岩石的基本特征,进一步支持了该类岩石"可能起源于古老下地壳的部分熔融"的成因模式。  相似文献   

11.
A mantle value of 17.5 for Nb/Ta appears well established; less well established are crustal values of 11–12, although it appears that Nb/Ta for crustal-derived melts is less than mantle Nb/Ta, demonstrating fractionation of these two elements during crustal evolution, and suggesting that Nb/Ta variation may be indicative of a particular chemical process within the crust-mantle system.

Experimental studies on silicate and carbonatitic liquids at high pressure indicate that, although silicate minerals such as garnet, amphibole and clinopyroxene do fractionate Nb and Ta, the partition coefficients (D's) for both elements are very low. Thus involvement of these minerals may explain relatively small changes in Nb/Ta, but appears inadequate to explain the crust-mantle variation. However, high-quality data for Nb, Ta may be used to provide information on mantle melting or metasomatic processes (e.g., amphibole in the source region decreases Nb/Ta in derived melts, while carbonatitic metasomatism will increase Nb/Ta in affected mantle). Titanate minerals have high D's for Nb and Ta, and do fractionate these elements (e.g., DNb/DTa rutile/liquid of 0.5–0.8), and their involvement in crystal fractionation would increase Nb/Ta in derivative liquids. In contrast, DNb/DTa for rutile/fluid is 1.25, so that rocks affected by fluid equilibrated with residual rutile will show a decrease in Nb/Ta

Some Archaean gneisses appear to have high Nb/Ta, and may be a complementary component to that part of the crust which has a relatively low Nb/Ta, such as crustal-derived magmas (e.g., A- ad I-type granites and silicic volcanics). Within the crustal system pegmatites are known to have extremely high and variable Nb, Ta contents, often with low Nb/Ta. A fluid is generally considered to be involved in the generation of these rocks. Thus it is possible that fluid/melt partitioning may be the key to fractionating Nb and Ta, with preference for Ta in the fluid, and enrichment of Ta relative to Nb into the mid-upper crustal system, as the crust evolved, through upward movement of fluid.  相似文献   


12.
During the evolution of the Earth, distinct geochemical reservoirs with different Nb/Ta ratios have developed. Archean granitoids of the tonalite–trondhjemite–granodiorite (TTG) suite, which represent the Earth’s early continental crust, show larger Nb/Ta variations than any other Earth reservoir. This implies that significant Nb–Ta fractionation must have occurred during early crust formation, while the underlying mechanism behind is still unclear. Here, we present a new model on how Nb may be fractionated from Ta during partial melting of subducted oceanic crust. Our data show that Nb/Ta ratios in melts derived from rutile- and titanite-bearing eclogite are largely controlled by the modal relative abundances of rutile and titanite in the source. High modal ratios of titanite over rutile generate melts with very high Nb/Ta (>60), whereas low modal titanite/rutile produces melts with much lower Nb/Ta (≤30). Very low Nb/Ta (<16) occur when all Ti-phases are consumed at very high degrees of melting. As the modal ratio of titanite to rutile is a function of pressure, the Nb/Ta of melts is a function of melting depth. Our new model helps to explain the extreme variation of Nb/Ta observed in many TTGs and thus how Nb and Ta were fractionated during the early evolution of the Earth. Furthermore, the model also indicates that simple one-stage melting models for mafic crust are not sufficient to explain the formation of TTGs.  相似文献   

13.
Fractionation between Nb and Ta, elements generally regarded as geochemical ‘identical twins’, is a key to deciphering the formation of the continental crust (CC). Here we show that Nb/Ta of rutile grains in eclogitic rocks from the Chinese Continental Scientific Drilling (CCSD) project are remarkably heterogeneous but overall subchondritic at core depths of 100–700 m, and are less variable and mainly suprachondritic at core depths of 700–3025 m, indicating clear Nb/Ta fractionation across a subducted slab. To understand the potential mechanism of Nb/Ta fractionation within the subducted plate, we analysed by laser ablation ICPMS a thermal migration experiment in which a wet andesite was placed in a large thermal gradient (300°C/cm with ends ranging from 950–350°C) at 0.5Gpa. Results show that Nb, Ta and Ti, driven by the thermal gradient, preferentially migrate by diffusion through supercritical fluids into the cooler end of the experiment (at 650–350°C). Due to contrasting Nb and Ta thermal migration patterns, dramatic fractionation between Nb, Ta, and Ti took place in the cooler end. Experimental results are consistent with the measured Nb, Ta in rutile from CCSD drillhole samples. We consider that major fractionation between Nb, Ta must occur before rutile appears, most likely during the prograde blueschist to amphibole–eclogite transformation, when Ti is also mobile. Before rutile appears, partitioning between Ti‐rich dominant minerals such as amphiboles and fluids in the hotter region where dehydration preferentially occurs, produces Nb–Ta–Ti‐rich fluids with subchondritic Nb/Ta, and dehydration residues with suprachondritic Nb/Ta. Meanwhile, owing to evolution of the thermal gradient within the subducting slab, thermal migration of Nb, Ta, and Ti in aqueous fluids result in Nb, Ta, and Ti enrichment in the cooler region and depletion in the hotter region. As a result of high‐pressure metamorphism, hydrous rutile‐rich eclogites with overall subchondritic Nb/Ta form in the cooler region, whereas relatively anhydrous rutile‐poor eclogites with suprachondritic Nb/Ta form in the hotter region. Subsequently, partial melting of hydrous rutile‐rich eclogites with initial subchondritic Nb/Ta at deeper levels transfers overall subchondritic Nb/Ta coupled with Nb, Ta, and Ti depletion characteristics to the CC, leaving dry rutile‐poor eclogites with suprachondritic Nb/Ta and rutile‐rich residual eclogites with overall, heterogeneous subchondritic Nb/Ta as a complementary reservoir to the CC.  相似文献   

14.
A wide range of trace elements have been analysed in mantle xenoliths (whole rocks, clinopyroxene and amphibole separates) from alkaline lavas in the Eastern Carpathians (Romania), in order to understand the process of metasomatism in the subcontinental mantle of the Carpatho-Pannonian region. The xenoliths include spinel lherzolites, harzburgites and websterites, clinopyroxenites, amphibole veins and amphibole clinopyroxenites. Textures vary from porphyroclastic to granoblastic, or equigranular. Grain size increases with increasing equilibrium temperature of mineralogical assemblages and results from grain boundary migration. In peridotites, interstitial clinopyroxenes (cpx) and amphiboles resulted from impregnation and metasomatism of harzburgites or cpx-poor lherzolites by small quantities of a melt I with a melilitite composition. Clinopyroxenites, amphibole veins and amphibole clinopyroxenites are also formed by metasomatism as a result of percolation through fracture systems of large quantities of a melt II with a melanephelinite composition. These metasomatic events are marked by whole-rock enrichments, relative to the primitive mantle (PM), in Rb, Th and U associated in some granoblastic lherzolites and in clinopyroxene and amphibole veins with enrichments in LREE, Ta and Nb. Correlations between major element whole-rock contents in peridotites demonstrate that the formation of interstitial amphibole and clinopyroxene induced only a slight but variable increase of the Ca/Al ratio without apparent modifications of the initial mantle composition. Metasomatism is also traced by enrichments in the most incompatible elements and the LREE. The Ta, Nb, MREE and HREE contents remained unchanged and confirm the depleted state of the initial but heterogeneous mantle. Major and trace element signature of clinopyroxene suggests that amphibole clinopyroxenites and some granoblastic lherzolites have been metasomatized successively by melts I and II. Both melts I and II were Ca-rich and Si-poor, somewhat alkaline (Na > K). Melt I differed from melt II in having higher Mg and Cr contents offset by lower Ti, Al, Fe and K contents. Both were highly enriched in all incompatible trace elements relative to primitive mantle, showing positive anomalies in Rb, Ba, Th, Sr and Zr. They contrasted by their Ta, Nb and LREE contents, lower in melt I than in melt II. Melts I and II originate during a two-stage melting event from the same source at high pressure and under increasing temperature. The source assemblage could be that of a metasomatized carbonated mantle but was more likely that of an eclogite of crustal affinity. Genetic relationships between calc-alkaline and alkaline lavas from Eastern Carpathians and these melts are thought to be only indirect, the former originating from partial melting of mantle sources respectively metasomatized by the melts I and II. Received: 17 March 1997 / Accepted: 14 July 1997  相似文献   

15.
This paper reports detailed analyses of Nb and Ta concentrations of 19 eclogite samples and their principal mineral constituents from the main drill hole of the Chinese Continental Scientific Drilling Project (CCSD) and nearby outcrops. We observe highly fractionated and overall suprachondritic Nb/Ta values in minerals, e.g., rutile (4.8–87), titanite (12–62) and amphibole (2.0–67). Amphiboles in amphibolites (retrograded from eclogite) can be classified into two groups: a low Nb/Ta group that bears higher Al contents and is thus of higher pressure origin, and a high Nb/Ta, lower pressure group. The former group was likely formed during subduction; the latter may have formed during exhumation in the presence of rutile and titanite. The significant Nb/Ta fractionation in rutile and other minerals may reflect early dehydration of the subducted slab at shallow depths before the formation of rutile, which occurs at depths ≥50 km. The dehydration, with amphiboles existing as the main Nb–Ta-bearing phase, would lead to Nb/Ta fractionation, i.e., forming subchondritic Nb/Ta ratios in the released fluids and, complementarily, suprachondritic Nb/Ta ratios in the residual phases. While a large proportion of the fluids may escape from the slab to the mantle wedge, considerable amounts of the fluids can be retained in hydrous minerals within the descending slab, thus forming hydrated cold eclogites with subchondritic Nb/Ta characteristics. As subduction continues to depths over 50 km, rutile appears and consequently controls the Nb–Ta budget. In the presence of rutile, melting of the hydrated cold eclogites with very low Nb/Ta ratios would form magmas with negative Nb, Ta anomalies and subchondritic Nb/Ta. Further dehydration of the continuously descending slab results in even more fractionated Nb/Ta ratios in subsequently released fluids and residues, providing a feasible explanation for the large Nb/Ta variation observed in the modern arc magmas and residual eclogites.  相似文献   

16.
Isobaric partial melting experiments were performed on an Fe-free synthetic composition to simulate partial melting of subducted oceanic crust. Nominally anhydrous experiments at 3.0 GPa yielded melts in equilibrium with garnet (13 to 16 mol.% grossular) and aluminous clinopyroxene (14 to 16 wt.% Al2O3). Melt compositions show decreasing Si and alkalis and increasing Ca, Mg, and Ti contents with increasing temperatures. Experiments at 1200 and 1300°C were rutile saturated, whereas experiments at 1400°C contained no residual rutile. We argue that during the initial stages of subduction, accessory rutile is likely to be stable in subsolidus eclogites of average midocean ridge basalt composition and that only large degrees of partial melting will eradicate rutile from an eclogitic source. At 3 GPa, any eclogites with a bulk TiO2 content of ≥1.5 wt.% rutile will produce rutile-saturated partial melts, except at very high degrees of melting. At higher pressures, all bulk Ti may dissolve in clinopyroxene and garnet, leaving no accessory rutile.Trace element partition coefficients for 24 trace elements between clinopyroxene, garnet, and melt were determined by secondary-ion mass spectrometry analysis of experimental run products at 1400°C and 3 GPa. Partition coefficients for the rare earth elements agree well with previous studies and have been evaluated using the lattice strain model. Partitioning data for high-field strength elements indicate complementary DZr/DHf for clinopyroxene and garnet. Partial melting of an eclogitic component of different modal compositions may therefore explain both subchondritic and superchondritic Zr/Hf ratios. Superchondritic Zr/Hf has recently been observed in some ocean island basalts (OIB), and this may be taken as further evidence for components of recycled oceanic crust in OIB. The data also indicate slight Nb/Ta fractionation during partial melting of bimineralic eclogite, which is not, however, sufficient to explain some recently observed Nb/Ta fractionation in island arc rocks. Accessory rutile, however, can explain such fractionation.  相似文献   

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