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大别山超高压变质岩形成深度的同位素限制 总被引：8，自引：0，他引：8
大别山超高压变质岩形成深度是各国地质学家十分关心的问题。它不仅影响对碰撞造山带形成机制和演化过程的认识,而且影响对地球深部状况及地球动力学的研究。该文对大别山超高压变质岩已有同位素资料进行了分析与讨论。大别山榴辉岩的εNd为-6.2~-17,εSr为18~42,且显示明显的Nd同位素的不平衡现象。大别山榴辉岩的氧同位素组成研究表明,这些榴辉岩的原岩在超高压变质前,不同程度地与贫18O的大气降水(或海水)发生过氧同位素交换,且在超高压变质过程中依然保留了这些痕迹。除一个样品外,大别-苏鲁地区的榴辉岩的3He/4He比值都落在0.79×10-7~9.35×10-7范围内,显示陆壳岩石来源He的重要贡献。所有Sr-Nd、O和He同位素研究均表明:超高压变质岩保存着表壳岩石原岩的同位素特征,而未显示变质时受到地幔物质的明显影响。对于超高压变质岩的上述同位素特征,有人认为是由于大别山造山带俯冲和折返的速度太快造成的。由于造山带俯冲和折返的速度太快,表壳岩石原岩变质时来不及与地幔物质发生交换,故没有留下地幔物质参与的痕迹。该研究认为这种解释有些勉强,因为大别造山带俯冲和折返时间至少需要15Ma.在如此长的时间内,在100多公里地幔深处高于700℃的高温下发生超高压变质作用,表壳岩石原岩不可能不与地幔物质发生同位素交换。相反,如果认为大别山超高压变质岩就在地壳内形成,则大别山超高压变质岩同位素的所有特征就很好解释了。 相似文献
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大别—苏鲁高压变质带中榴辉岩的多样性及其成因 总被引：10，自引：0，他引：10
最近的研究表明,大别—苏鲁高压变质带中的榴辉岩是多种多样的。与蓝片岩共生的C类榴辉岩可能由俯冲洋壳经低温高压变质作用(t=523℃,p=1.2—1.5GPa)形成;与片麻岩共生的B类榴辉岩则可能是在陆-陆碰撞过程中由俯冲陆壳中的基性成分岩石经原地高温(超)高压变质作用(t=651—828℃,p=1.2—3.8GPa)形成;侵入于B类柯石英榴辉岩中的脉状榴辉岩(A类)可能是在相对高温高压条件下(t=769℃,p>1.8GPa)由偏超基性岩浆直接结晶出来的。这些不同类型的榴辉岩不是一次简单高压变质事件的产物,表明华北—扬子板块边界经历了漫长而多期次的演化历史。 相似文献
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在西藏拉萨地块的东部,从松多到加兴,在晚古生代石英岩和碳酸岩地层中分布着一条近东西走向的榴辉岩带。尽管受到不同程度的海水蚀变和后期流体/岩浆渗滤的影响,多数松多榴辉岩保存了类似于N-MORB的微量元素地球化学特征,这也与榴辉岩的Sr-Nd同位素系统特征一致。这些榴辉岩经历了压力约为2.6GPa、温度约为650℃的高压变质作用。石榴石-绿辉石-全岩Sm-Nd等时线给出(239±3.5)Ma的等时线年龄,表明在早中生代,拉萨地块内部至少发生过一期洋壳俯冲事件。以松多榴辉岩为代表的洋壳俯冲事件同时表明带状基墨里大陆的形成有可能是一系列微陆块碰撞拼贴而成。 相似文献
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羌塘中部高压变质带的形成过程 总被引：1，自引：1，他引：0
羌塘中部高压变质带由榴辉岩、石榴石白云母片岩和蓝片岩等组成,与蛇绿混杂岩、晚古生代浅变质地层岩片等共同构成了龙木错-双湖板块缝合带这一构造混杂岩带,是伴随古特提斯洋闭合的深俯冲作用及后期构造作用的产物。通过对其野外地质特征、不同岩石类型岩石学、矿物学以及同位素年代学等的研究,确认榴辉岩和石榴石白云母片岩在早期分别经历了各自的形成过程,在榴辉岩形成之后的折返过程中二者共同构成了高压变质带,并且在折返过程中榴辉岩发生蓝片岩相退变质作用,同时导致了带内蓝片岩的形成。同位素年代学研究结果表明,龙木错-双湖板块缝合带闭合过程中的榴辉岩相变质作用发生于240Ma左右,折返过程中的蓝片岩相退变质作用及蓝片岩的形成应在220～200Ma,高压变质带最终在214Ma之前抬升出露地表。 相似文献
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含柯石英的苏鲁-大别榴辉岩是高压-超高压变质带的产物.依据榴辉岩的总体展布方向、岩石特征、高压-超高压变质作用及退变质作用的温压条件,可划分为NEE向胶东高压-超高压变质带、NNE向郯庐高压-超高压变质带和SEE向大别高压-超高压变质带.榴辉岩的同位素年龄值指示这3个带是主压应力方向不同、形成时期不同、发展和终止时期也各不相同的3个高压-超高压变质带.NEE向胶东高压-超高压变质带主要形成于700～900 Ma的晋宁期,终止于200 Ma左右的印支期;SEE向大别高压-超高压变质带主要形成于400～500 Ma的加里东期,终止于250 Ma左右的印支期;NNE向郯庐高压-超高压变质带初期曾经与胶东高压-超高压变质带是一个带,最早形成于900 Ma左右的晋宁期,但其最重要的形成期是200 Ma左右的印支期,55 Ma左右的喜马拉雅期该带进入推覆造山阶段.胶东、大别和早期的郯庐高压-超高压变质带的主压应力方向都是近SN向,印支期之后的郯庐高压-超高压变质带主压应力方向转变为近EW向. 相似文献
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大别山超高压变质榴辉岩的氦同位素组成及对其形成环境的制约 总被引：6，自引：0，他引：6
大别山地区榴辉岩全岩的3He/4 He值分布在0 .0 13×10 - 6 ～0 .76 0×10 - 6 之间,平均0 .2 0 0×10 - 6 ,榴辉岩中石榴子石单矿物的3He/4 He值与其全岩的3He/4 He值基本一致。在3He—4 He分布图上榴辉岩的氦同位素数据点远离地幔氦的分布范围,而位于大气氦与地壳氦的过渡部位。采用真空压碎方法对榴辉岩中石榴子石和绿辉石的氦同位素组成进行了分析,也未找到地幔氦的明显踪迹。结合大别—苏鲁地区榴辉岩中极低的δ1 8O值、εNd(0 )值等地球化学特征,提出大别—苏鲁地区超高压变质榴辉岩可能是在地壳中形成的,并未曾俯冲至10 0多千米的地幔深度。榴辉岩的3He/4 He值与围岩类型密切相关,榴辉岩的δ1 8O值与围岩的δ1 8O值同步变化,以及含柯石英大理岩、片麻岩和硬玉石英岩等非基性超高压变质岩和脉状榴辉岩的发现,均证明榴辉岩与其围岩一起经历了超高压变质过程,榴辉岩及其围岩在变质过程中未发生明显的位移,即榴辉岩是原地成因的。 相似文献
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苏鲁超高压变质带东海青龙山高压正片麻岩中白云母的^40Ar／^39Ar年代学研究 总被引：7，自引：1，他引：7
作为东海青龙山榴辉岩围岩的高压变质的正片麻岩，其白云母的常规^40Ar／^39Ar年龄和Rb—Sr、Sm—Nd年龄一致，激光微区Ar同位素分析表明，白云母的Ar同位素分布也是均匀的。由此得出的初步结论是：①高压变质的正片麻岩中的白云母中不含过剩Ar，这类矿物可以作为^40Ar／^39Ar同位素测年的对象；②青龙山榴辉岩中的白云母含大量过剩氩，而作为其围岩的超高压正片麻岩中的白云母却不含过剩氩，这一事实证明了榴辉岩中白云母的过剩氩不是来自围岩，而是榴辉岩自身继承的。 相似文献
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本文总结了近年来有关高压-超高压变质电气石的研究成果,并在此基础上指出未来该领域的重点研究方向.电气石是一种分布广泛的矿物.实验证明其稳定存在的温度大于850℃,压力大于4 GPa.由于较慢的空间扩散作用、复杂的成分替代关系和较高的环境敏感度,电气石可以保存完好的生长环带.这有助于我们分析同位素演化、变质流体成分、岩石变质历史等.高压-超高压电气石结构化学研究表明电气石结构中的某些元素含量(如Al和F含量)和矿物的形成温度具有很好的相关性.根据不同的硼同位素来源,高压-超高压变质电气石的生长模型可以分为A型电气石、B型电气石和C型电气石.通过分析出露在全球各地的代表性高压-超高压变质电气石,其特征总体表现为:①多为镁电气石;②X晶位具有很高的占位率(＞0.8 pfu);③化学结构中硼元素具有过量特征(3.2～3.3 pfu);④Ti、Mn、Li、Cl含量很低;⑤硼同位素成分的变化范围为:-16％ ＜δ11B＜+ 1‰.未来高压-超高压变质电气石的研究重点应该放在电气石晶体化学和变质p-t条件的关系、电气石-流体之间微量元素的分异作用以及含硼矿物组合的相平衡模拟等. 相似文献
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本文对榴辉岩部分熔融过程中不同同位素体系是否存在分馏这一当前研究热点进行了综述。榴辉岩作为研究洋陆俯冲、超高压变质以及壳幔相互作用的主要岩石类型,其部分熔融与地壳增生、板片折返过程以及俯冲隧道中元素的迁移分配等具有紧密的联系。作为典型的高压-超高压变质岩石,榴辉岩可通过俯冲带将壳源信息携带至地幔深部,影响地幔的化学组成,并可在大洋玄武岩中得以表现。近些年,随着仪器分析技术的发展,实验研究和理论计算均表明榴辉岩部分熔融过程中稳定同位素可以产生显著的分馏。作为常见的放射性成因子体同位素和传统稳定同位素Sr-Nd-Hf-O被广泛应用于源区示踪、岩浆混合以及结晶分异等过程。但目前有研究指出,在非平衡熔融过程中,熔体和源区的Sr-Nd-Hf-O同位素可发生解耦,导致二者的同位素组成不均一。另外,通过研究榴辉岩及其熔融产物的金属稳定同位素特征,发现榴辉岩部分熔融过程中,由于石榴石效应,会造成Ca、Mg、Fe、Li等金属稳定同位素的分馏。因此,当利用稳定同位素示踪榴辉岩熔体的源区时,需要考虑其分馏的影响。 相似文献
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Sune G. Nielsen Helen M. Williams William L. Griffin Norman Pearson 《Geochimica et cosmochimica acta》2009,73(24):7387-6704
Cratonic eclogites are inferred to originate either from subducted ocean crust or mantle melts accreted onto the roots of continents. These models have different implications for the growth of continents, but it is currently difficult to determine the origin of individual eclogite suites.Upper ocean crust altered at low temperatures and marine sediments both display high thallium (Tl) concentrations and strongly fractionated Tl isotope signatures relative to the ambient upper mantle. In this study we carry out the first examination of the suitability of Tl isotopes as a tracer for an ocean-crust origin of cratonic eclogites. We have analysed the Tl isotope composition of clinopyroxene and garnet in six eclogites from the Kaalvallei and Bellsbank kimberlite pipes in South Africa. Minerals were pre-cleaned with an HCl leaching technique and the leachates display variably light Tl isotope ratios. These most likely reflect low-temperature hydrothermal alteration occurring after eruption of the kimberlite that carried the eclogites to the surface.The leached mineral pairs all display identical Tl isotope ratios, strongly suggesting that the source of the analysed Tl is identical for each mineral pair. It is, however, not possible to exclude the possibility that the analysed Tl originates from kimberlitic material that was not removed by the cleaning procedure.Only one of the six samples exhibits a Tl isotope composition different from ambient mantle. Assuming that the Tl isotope signatures indeed represent the eclogite minerals and not any form of contamination, the Tl isotope composition in this sample is consistent with containing a minor component (<3%) of ocean crust altered at low temperatures.Thallium isotopes may become one of the most sensitive indicators for the presence of low-T altered ocean crust because of the stark contrast in Tl concentration and isotopic composition between the mantle and altered ocean crust. In fact, no other chemical or isotopic tracer could have provided an indication that any of the samples studied here had a subduction origin. However, much work is still required before it becomes clear if Tl isotope measurements are a viable means to establish the origin of cratonic eclogites. 相似文献
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分步淋洗方法研究碧溪岭榴辉岩Pb同位素组成及其演化 总被引：1，自引：0，他引：1
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 相似文献
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稀有气体同位素示踪成矿古流体研究进展 总被引：13，自引：0，他引：13
稀有气体(特别是He、Ar)是一种研究成矿古流体来源的灵敏示踪剂。地球不同圈层的稀有气体同位素具有不同的特征同位素比值。测试样品流体包裹体中的稀有气体同位素值,从测试值中排除掉包裹体形成后各种后生过程对流体初始同位素组成的影响。把得到的结果与前人研究总结的特征值进行比较分析,可以示踪成矿流体来源,从而探讨各种矿床的成矿机制与成矿作用。归纳了近年来用稀有气体同位素来示踪成矿流体的研究进展,概括了其在不同类型矿床中的应用现状,并指出当前该方法存在的问题及发展趋势。 相似文献
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CCSD中HP-UHP岩石稀有气体同位素地球化学及其对板块折返过程的示踪意义 总被引：1，自引：0，他引：1
利用高真空气相质谱系统测定了CCSD中HP-UHP变质岩中主要造岩矿物流体包裹体的稀有气体同位素组成,得出其3He/4He为(0.004~0.775)×10-6,相应R/Ra为0.003~0.553,40Ar/36Ar变化较大,为316.2~11358.8,高于大气40Ar/36Ar(295.5);20Ne/22Ne和21Ne/22Ne分别为9.47~12.4和0.026~0.051,而134Xe/132Xe和136Xe/132Xe分别为0.376~0.484和0.324~0.416,均高于其相应大气值。CCSD中HP-UHP岩石主要造岩矿物的He-Ar、Xe和Ne等同位素组成清楚显示其中流体包裹体主要由地壳变质流体和少量大气饱和水组成,而深源地幔流体组分很低,其中He主要来自地壳,Ar主要由壳源放射性成因40Ar*和少量(平均32.6%)大气Ar混合组成,少量Ne和Xe可能来自地幔。CCSD中HP-UHP岩石具有F40Ar相似文献
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稀有气体（特别是He、Ar）是一种研究成矿古流体来源的灵敏示踪剂。地球不同圈层的稀有气体同位素具有不同的特征同位素比值。测试样品流体包裹体中的稀有气体同位素值，从测试值中排除掉包裹体形成后各种后生过程对流体初始同位素组成的影响。把得到的结果与前人研究总结的特征值进行比较分析，可以示踪成矿流体来源，从而探讨各种矿床的成矿机制与成矿作用。归纳了近年来用稀有气体同位素来示踪成矿流体的研究进展，概括了其在不同类型矿床中的应用现状，并指出当前该方法存在的问题及发展趋势。 相似文献
17.
Snyder Gregory A.; Taylor Lawrence A.; Crozaz Ghislaine; Halliday Alex N.; Beard Brian L.; Sobolev Vladimir N.; Sobolev Nikolai V. 《Journal of Petrology》1997,38(1):85-113
Owing to the association with diamonds, eclogite xenoliths havereceived disproportionate attention given their low abundancein kimberlites. Several hypotheses have been advanced for theorigin of eclogite xenoliths, from the subduction and high-pressuremelting of oceanic crust, to cumulates and liquids derived fromthe upper mantle. We have amassed a comprehensive data set,including major- and trace-element mineral chemistry, carbonisotopes in diamonds, and Rb–Sr, Sm–Nd, Re–Os,and oxygen isotopes in ultrapure mineral and whole-rock splitsfrom eclogites of the Udachnaya kimberlite pipe, Yakutia, Russia.Furthermore, eclogites from two other Yakutian kimberlite pipes,Mir and Obnazhennaya, have been studied in detail and offercontrasting images of eclogite protoliths. Relative to eclogitesfrom southern Africa and other Yakutian localities, Udachnayaeclogites are notable in the absence of chemical zoning in mineralgrains, as well as the degree of light rare earth element (LREE)depletion and unradiogenic Sr; lack of significant oxygen, sulfur,and carbon isotopic variation relative to the mantle; and intermineralradiogenic isotopic equilibration. Several of these eclogitescould be derived from ancient, recycled, oceanic crust, butmany others exhibit no evidence for an oceanic crustal protolith.The apparent lack of stable-isotope variation in the Udachnayaeclogites could be due to the antiquity of the samples and consequentlack of deep oceanic and biogenically diverse environments atthat time. Those eclogites that are interpreted to be non-recycledhave compositions characteristic of Group A eclogites from otherlocalities that also have been interpreted as being directlyfrom the mantle. At least two separate and diverse isotopicreservoirs are suggested by Nd isotopic whole-rock reconstructions.Most samples were derived from typical depleted mantle. However,two groups of three samples each indicate both enriched mantleand possible ultra-depleted mantle present beneath Yakutia duringthe late Archean and early Proterozoic. The vast majority ofeclogites studied from the Obnazhennaya pipe also exhibit characteristicsof Group A eclogites and are probably derived directly fromthe mantle. However, the eclogites from the Mir kimberlite aremore typical of other eclogites world-wide and show convincingevidence of a recycled, oceanic crustal affinity. We concurwith the late Ted Ringwood that eclogites can be formed in avariety of ways, both within the mantle and from oceanic crustalresidues. KEY WORDS: diamonds; eclogite xenoliths; isotopic composition; REE; Yakutia 相似文献
18.
大别造山带中镁铁质——超镁铁质岩石和榴辉岩有关问题的讨论 总被引：21，自引：3，他引：18
根据近年来积累的文献资料及研究讨论指出：（１）大别山造带镁铁质－－超镁铁质岩石可分成两大类;一类以任家湾、童家冲、祝家铺道士冲、青山、沙河等辉石辉长岩类为代表,它们具有相同的牲和成岩年龄,可能与华北、华南地块聚敛碰产生的岛弧或大陆岩浆岩有关;另一类以铙拔寨,大化坪、碧溪岭和毛屋岩体为代表,虽然它们的成岩年龄均在前寒武纪,但却有着不同的成岩时代和成岩环境。（２）大别造山带榴辉岩等多属异地来源,具有不 相似文献
19.
A crustal origin for eclogites and a mantle origin for garnet peridotites: Strontium isotopic evidence from clinopyroxenes 总被引：1，自引：0，他引：1
Hannes K. Brueckner 《Contributions to Mineralogy and Petrology》1977,60(1):1-15
Strontium isotopic data suggest that the classic eclogite-facies rocks of western south Norway described by Eskola (1921) formed from several parental materials in a variety of environments. Mineral separates from essentially basic, bi-minerallic (clinopyroxene and garnet) eclogites that occur as lens-shaped masses within high grade gneisses (country rock eclogites) have Sr87/Sr86 values that range from 0.704 for fine-grained varieties to 0.716 for coarse-grained, orthopyroxene-bearing varieties. These high, varied ratios contrast with the very low, restricted ratios (0.701 to 0.704) of similar minerals from ultrabasic, garnet-clinopyroxene-orthopyroxene-olivine assemblages (garnet peridotites) that occur as lenses within large peridotite bodies. The eclogite-facies metamorphism that generated the garnet peridotites may have occurred in the mantle. However, the metamorphism that generated at least the more radiogenic country-rock eclogites must have occurred in the crust. The high Sr87/Sr86 ratios of these eclogites could be generated either by forming them from crustal parental rocks or by contaminating mantle-derived parental rocks with radiogenic strontium from the country rocks. If this contamination occurred after intrusion and before eclogite-facies metamorphism, a rather contrived history must be postulated that involves intrusion, contamination accompanied by hydration, subsequent dehydration, and finally eclogite-facies metamorphism. These processes could have occurred within the long, complicated history of the enclosing country rocks. Alternatively, if the contamination occurred during eclogite-facies metamorphism, the presence of some hydrous fluid appears to be required to transport the radiogenic strontium from the enclosing country rocks. The eclogites with the highest Sr87/Sr86 ratios are also the most coarse-grained and it is possible that the presence of some intergranular fluid enabled these eclogites to recrystallize to a much larger grain size than would have been possible in a totally anhydrous environment. The garnet peridotites and fine-grained country rock eclogites may have formed from mantle material in the crust but escaped contamination by radiogenic strontium as a result of their position in a dry environment in the crust.Lamont-Doherty Geological Observatory Contribution No. 2443 相似文献
20.
Origins of Xenolithic Eclogites and Pyroxenites from the Central Slave Craton, Canada 总被引：5，自引：0，他引：5
Aulbach Sonja; Pearson Norman J.; O'Reilly Suzanne Y.; Doyle Buddy J. 《Journal of Petrology》2007,48(10):1843-1873
Major- and trace-element and Sr–Nd–Hf isotopic compositionsof garnet and clinopyroxene in kimberlite-borne eclogite andpyroxenite xenoliths were used to establish their origins andevolution in the subcontinental lithospheric mantle beneaththe central Slave Craton, Canada. The majority of eclogitescan be assigned to three groups (high-Mg, high-Ca or low-Mgeclogites) that have distinct trace-element patterns. Althoughpost-formation metasomatism involving high field strength element(HFSE) and light rare earth element (LREE) addition has partiallyobscured the primary compositional features of the high-Mg andhigh-Ca eclogites, trace-element features, such as unfractionatedmiddle REE (MREE) to heavy REE (HREE) patterns suggestive ofgarnet-free residues and low Zr/Sm consistent with plagioclaseaccumulation, could indicate a subduction origin from a broadlygabbroic protolith. In this scenario, the low REE and smallpositive Eu anomalies of the high-Mg eclogites suggest moreprimitive, plagioclase-rich protoliths, whereas the high-Caeclogites are proposed to have more evolved protoliths withhigher (normative) clinopyroxene/plagioclase ratios plus trappedmelt, consistent with their lower Mg-numbers, higher REE andabsence of Eu anomalies. In contrast, the subchondritic Zr/Hfand positive slope in the HREE of the low-Mg eclogites are similarto Archaean second-stage melts and point to a previously depletedsource for their precursors. Low ratios of fluid-mobile to lessfluid-mobile elements and of LREE to HREE are consistent withdehydration and partial melt loss for some eclogites. The trace-elementcharacteristics of the different eclogite types translate intolower Nd for high-Mg eclogites than for low-Mg eclogites. Withinthe low-Mg group, samples that show evidence for metasomaticenrichment in LREE and HFSE have lower Nd and Hf than a samplethat was apparently not enriched, pointing to long-term evolutionat their respective parent–daughter ratios. Garnet andclinopyroxene in pyroxenites show different major-element relationshipsfrom those in eclogites, such as an opposite CaO–Na2Otrend and the presence of a CaO–Cr2O3 trend, independentof whether or not opx is part of the assemblage. Therefore,these two rock types are probably not related by fractionationprocesses. The presence of opx in about half of the samplesprecludes direct crystallization from eclogite-derived melts.They probably formed from hybridized melts that reacted withthe peridotitic mantle. KEY WORDS: eclogites; pyroxenite xenoliths; mantle xenoliths; eclogite trace elements; eclogite Sr isotopes; eclogite Hf isotopes; eclogite Nd isotopes 相似文献