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1.
超高压变质岩的塑性流变学   总被引:1,自引:1,他引:0  
钟增球  索书田 《现代地质》2007,21(2):203-212
岩石流变作用是大陆造山作用的基本特征,超高压岩石的形成和折返过程也是大陆深俯冲带内物质的复杂流变过程。要深入理解大陆造山带的造山作用和大陆壳岩石的深俯冲和折返动力学过程,必须对大陆地壳及地幔岩石的流变学进行深入研究。岩石圈流变学的主要研究内容主要包括流变学分层性、变形分解和应变局部化及大陆壳岩石部分熔融作用的流变学效应等。应用岩石圈流变学的基本原理和方法,分析了大别-苏鲁超高压变质带中超高压变质岩的塑性流变特点,探讨了超高压变质岩形成和折返过程的塑性流变学。  相似文献   

2.
自20世纪80年代在大陆地壳岩石中发现柯石英和金刚石等超高压变质矿物以来,大陆深俯冲和超高压变质作用就成为了固体地球科学研究的前沿和热点领域之一。经过三十余年的研究,已经在大陆地壳的俯冲深度、深俯冲岩石变质P-T-t轨迹、俯冲地壳岩石的折返机制、深俯冲岩石的原岩性质、大陆碰撞过程中的熔/流体活动与元素活动性、俯冲隧道内部不同类型壳幔相互作用、碰撞后岩浆岩的成因、大陆碰撞造山带成矿作用等方面取得了许多重要成果。本文重点对大陆俯冲带超高压岩石部分熔融和不同类型壳幔相互作用近十年来的研究进展进行回顾和总结,并对存在的相关科学问题和未来的研究方向进行了展望。深俯冲大陆地壳的部分熔融主要出现在两个阶段:折返的初期阶段和碰撞后阶段,前者产生了碱性熔体,后者产生了钙碱性熔体。大陆俯冲带壳幔相互作用有两种类型,涉及地幔楔与两种俯冲带流体的交代反应:一是来自深俯冲陆壳的变质脱水/熔融,二是来自先前俯冲古洋壳的变质脱水/熔融。  相似文献   

3.
超高压变质岩中柯石英-石英相变动力学研究的评述   总被引:2,自引:0,他引:2  
含柯石英超高压变质岩的发现是陆过 幔深部俯冲的岩石学语气也揭示了深部变质深种物折返地表的可能性。超高压变质岩的开 折返机制是当前地球科学中最有挑战性的前沿课题之一,具有深刻的大陆动力学意义。  相似文献   

4.
追溯和重塑超高压变质岩由100多千米地幔深度折返至上地壳及地表的过程,对理解会聚板块边缘及大陆碰撞带的运动学和动力学是极为重要的.主要依据构造学、岩石学、地球化学和可利用的地质年代学资料,结合区域多期变形分析,大别-苏鲁区超高压变质岩的折返过程至少可分解出4个大的阶段.块状榴辉岩记录了三叠纪(约250~230 Ma)大陆壳岩石的深俯冲/碰撞作用.超高压变质岩早期迅速折返发生于超高压峰期变质作用(P>3.1~4.0 GPa,T≈800±50 ℃)之后,处于地幔深度和柯石英稳定域,相当于区域D2变形期阶段.分别与区域变形期D3、D4和D5对应的折返过程,以及后成合晶、冠状体等卸载不平衡结构发育和减压部分熔融作用2个中间性构造热事件,均发生在地壳层次. 网络状剪切带在折返过程的不同阶段和不同层次均有发育,标志着在超高压变质带内的变质和变形分解作用曾重复进行.着重指出,超高压变质岩的折返,主要是由大陆壳的深俯冲/碰撞和伸展作用控制的构造过程,且受到俯冲带内、带外诸多因素的约束,其中水流体就起关键作用.   相似文献   

5.
大别地块超高压变质省的构造变形研究   总被引:9,自引:0,他引:9  
索书田 《地学前缘》1999,6(4):255-262
构造解析的基本目的是建立构造事件造成的地质体几何学、运动学、动力学和流变学。大陆碰撞造山带内含柯石英及微粒金刚石等矿物组合的超高压(UHP) 变质岩的形成和折返,是极为复杂的地球动力学过程。与世界上已知大多数超高压变质带相似,中国大别地块内超高压变质省现今观察到的主体构造形式,主要是在碰撞或超高压变质峰期后伸展体制下形成的。通过对大别超高压变质省内伸展组构及挤压( 碰撞) 组构的鉴别、分析,结合有关超高压变质带构造学研究领域的简略综述指出,在揭示超高压变质带的形成及折返动力学过程中,构造解析的思维和工作方法是行之有效的  相似文献   

6.
ThereisanunanimousunderstandingthattheUHPmetamorphisminDabie-SuluareaswasformedduringtheTri-assiccollisioneventbetweentheYangtzeandNorthChinacratons(Congetal.,l994$Zhouetal-,l996;Liouetal.,l994)-Eclogiteisthemostimportantrocktypeamongtheul-trahigh-pressure(UHP)metamorphicrocks.Accordingtotheiroccurrencethereare3typesofeclogites:typeIisen-clavesinultramaficintrusionsandasmembersinthelayeredmafic-ultramaficcomplex(Jahnl998);typeIispodsorlay-ersinthehighlymetamorphicsupracrustals(mainlying…  相似文献   

7.
张泽明  董昕  贺振宇  向华 《岩石学报》2013,29(5):1713-1726
喜马拉雅造山带是印度与亚洲大陆碰撞作用的产物,正在进行造山作用,是研究板块构造的天然实验室.高压和超高压变质岩分布在喜马拉雅造山带的核部.这些变质岩具有不同的形成条件、形成时间和形成过程,为印度与亚洲碰撞带的几何学、运动学和动力学提供了重要的限定.含柯石英的超高压变质岩产出在喜马拉雅造山带的西段,它们形成在古新世与始新世之间(53~46Ma),为印度大陆西北边缘高角度超深俯冲作用的产物,并经历了快速俯冲与快速折返过程.在约5 Myr内,超高压变质岩从>100km的地幔深度折返到了中地壳深度,且仅仅叠加角闪岩相退变质作用.高压榴辉岩产出在喜马拉雅造山带中段,形成时间约为45Ma,为印度大陆低角度深俯冲作用的产物,经历了至少20Myr的长期折返过程,叠加麻粒岩相退变质作用和部分熔融.高压麻粒岩产出在喜马拉雅造山带的东端,是印度大陆东北缘近平俯冲作用的产物,峰期变质作用时间约为35Ma,经历了约20Myr的长期折返过程,叠加了麻粒岩相和角闪岩相退变质作用,并伴随有多期部分熔融.因此,喜马拉雅造山带的变质作用具有明显的时间与空间变化,显示出大陆深俯冲与折返过程的差异性,以及大陆碰撞造山带形成机制的多样性.  相似文献   

8.
桐柏-大别山区高压变质相的构造配置   总被引:18,自引:3,他引:15  
作为华北和扬子陆块间的碰撞造山带桐柏大别山区以发育高压、超高压变质带为特征,从南到北变质相从低级到高级,代表俯冲带深度不同的变质产物,整体形成高压变质相系列。不过现今各变质相岩石的分布极受后期地壳规模的伸展构造控制,大别杂岩的穹隆作用更使高压变质相带的空间分布复杂化。超高压变质岩今日多呈大小不等的块体嵌布于相对低压的大别杂岩之内,造山带根部物质的热软化,使许多深层地幔物质得以像挤牙膏一样挤出于大别杂岩内。它们之中广泛发育着减压退变质的显微结构,与大别杂岩内一些麻粒岩相表壳岩所保存的减压退变质证迹一样,同是挤出作用和碰撞后隆升的构造证迹。高压相系的发育使南桐柏山和大别山迥然不同于桐商( 商丹) 断裂以北的北秦岭北淮阳变质带。新近发表的同位素年代学(40Ar 39 Ar) 资料:316 ~434 Ma ,已证明北秦岭是古生代变质带,它与桐柏- 大别印支期碰撞造山带差异甚大。这两个变质地温梯度差异甚大的变质地体的拼合,说明华北和扬子陆块碰撞的主缝合带是商丹- 桐商断裂带  相似文献   

9.
《Gondwana Research》2014,25(2):494-508
Large segments of the continental crust are known to have formed through the amalgamation of oceanic plateaus and continental fragments. However, mechanisms responsible for terrane accretion remain poorly understood. We have therefore analysed the interactions of oceanic plateaus with the leading edge of the continental margin using a thermomechanical–petrological model of an oceanic-continental subduction zone with spontaneously moving plates. This model includes partial melting of crustal and mantle lithologies and accounts for complex rheological behaviour including viscous creep and plastic yielding. Our results indicate that oceanic plateaus may either be lost by subduction or accreted onto continental margins. Complete subduction of oceanic plateaus is common in models with old (> 40 Ma) oceanic lithosphere whereas models with younger lithosphere often result in terrane accretion. Three distinct modes of terrane accretion were identified depending on the rheological structure of the lower crust and oceanic cooling age: frontal plateau accretion, basal plateau accretion and underplating plateaus.Complete plateau subduction is associated with a sharp uplift of the forearc region and the formation of a basin further landward, followed by topographic relaxation. All crustal material is lost by subduction and crustal growth is solely attributed to partial melting of the mantle.Frontal plateau accretion leads to crustal thickening and the formation of thrust and fold belts, since oceanic plateaus are docked onto the continental margin. Strong deformation leads to slab break off, which eventually terminates subduction, shortly after the collisional stage has been reached. Crustal parts that have been sheared off during detachment melt at depth and modify the composition of the overlying continental crust.Basal plateau accretion scrapes oceanic plateaus off the downgoing slab, enabling the outward migration of the subduction zone. New incoming oceanic crust underthrusts the fractured terrane and forms a new subduction zone behind the accreted terrane. Subsequently, hot asthenosphere rises into the newly formed subduction zone and allows for extensive partial melting of crustal rocks, located at the slab interface, and only minor parts of the former oceanic plateau remain unmodified.Oceanic plateaus may also underplate the continental crust after being subducted to mantle depth. (U)HP terranes are formed with peak metamorphic temperatures of 400–700 °C prior to slab break off and subsequent exhumation. Rapid and coherent exhumation through the mantle along the former subduction zone at rates comparable to plate tectonic velocities is followed by somewhat slower rates at crustal levels, accompanied by crustal flow, structural reworking and syndeformational partial melting. Exhumation of these large crustal volumes leads to a sharp surface uplift.  相似文献   

10.
Diamondiferous rocks from the Kokchetav Massif, Kazakhstan, represent deeply subducted continental crust. In order to constrain the age of ultra high pressure (UHP) metamorphism and subsequent retrogression during exhumation, zircons from diamondiferous gneisses and metacarbonates have been investigated by a combined petrological and isotopic study. Four different zircon domains were distinguished on the basis of transmitted light microscopy, cathodoluminescence, trace element contents and mineral inclusions. Mineral inclusions and trace element characteristics of the zircon domains permit us to relate zircon growth to metamorphic conditions. Domain 1 consists of rounded cores and lacks evidence of UHP metamorphism. Domain 2 contains diamond, coesite, omphacite and titanian phengite inclusions providing evidence that it formed at UHP metamorphic conditions (P>43 kbar; T~950 °C). Domain 3 is characterised by low-pressure mineral inclusions such as garnet, biotite and plagioclase, which are common minerals in the granulite-facies overprint of the gneisses (P~10 kbar; T~800 °C). This multi-stage zircon growth during cooling and exhumation of the diamondiferous rocks can be best explained by zircon growth from Zr-saturated partial melts present in the gneisses. Domain 4 forms idiomorphic overgrowths and the rare earth element pattern indicates that it formed without coexisting garnet, most probably at amphibolite-facies conditions (P~5 kbar; T~600 °C). The metamorphic zircon domains were dated by SHRIMP ion microprobe and yielded ages of 527LJ, 528NJ and 526LJ Ma for domains 2, 3 and 4 respectively. These indistinguishable ages provide evidence for a fast exhumation beyond the resolution of SHRIMP dating. The mean age of all zircons formed between UHP metamorphic conditions and granulite-facies metamorphism is 528Dž Ma, indicating that decompression took place in less than 6 Ma. Hence, the deeply subducted continental crust was exhumed from mantle depth to the base of the crust at rates higher than 1.8 cm/year. We propose a two-stage exhumation model to explain the obtained P-T-t path. Fast exhumation on top of the subducted slab from depth >140 to ~35 km was driven by buoyancy and facilitated by the presence of partial melts. A period of near isobaric cooling was followed by a second decompression event probably related to extension in a late stage of continental collision.  相似文献   

11.
大别山高压-超高压变质期后伸展构造格局   总被引:15,自引:0,他引:15  
钟增球  索书田 《地球科学》1998,23(3):225-229
大别山高压、超高压变质期后构造格架的最显著特征是以罗田片麻岩穹隆为核部的多层伸展拆离滑脱带的发育,并由它们将超高压变质单元、高压变质单元和蓝闪-绿片岩单元分隔成垂向叠置的席状岩片,类似于变质核杂岩的基本结构样式。这种伸展构造格架制约了高压、超高压岩石的展布,而在较大榴辉岩体中保存的缩短或挤压组构则是以高压、超高压变质作用为标志的陆-陆碰撞事件的记录。正确地区分挤压组构与伸展组构是识别大别山带内高压  相似文献   

12.
A series of 2D petrological–thermomechanical numerical experiments was conducted to: (i) characterize the variability of exhumation mechanisms of ultrahigh pressure metamorphic (UHPM) rocks during collision of spontaneously moving plates and (ii) study the possible geodynamic effects of melting at ultrahigh pressure conditions for the exhumation of high‐temperature–ultrahigh pressure metamorphic (HT–UHPM) rocks. To this end, the models include fluid‐ and melt‐induced weakening of rocks. Five distinct modes of exhumation of (U)HPM rocks associated with changes in several parameters in the models of plate collision and continent subduction are identified as follows: vertical crustal extrusion, large‐scale crustal stacking, shallow crustal delamination, trans‐lithospheric diapirism, and channel flow. The variation in exhumation mechanisms for (U)HPM rocks in numerical models of collision driven by spontaneously moving plates contrasts with the domination of the channel flow mode of exhumation in a majority of the published results from numerical models of collision that used a prescribed plate convergence velocity and/or did not include fluid‐ and melt‐induced weakening of rocks. This difference in the range of exhumation mechanisms suggests that the prescribed convergence velocity condition and the neglect of fluid‐ and melt‐related weakening effects in the earlier models may inhibit development of several important collisional processes found in our experiments, such as slab breakoff, vertical crustal extrusion, large‐scale stacking, shallow crustal delamination and relamination, and eduction of the continental plate. Consequently, the significance of channel flow for the exhumation of UHPM rocks may have been overstated based on the results of the earlier numerical experiments. In addition, the results from this study extend over a larger proportion of the high‐temperature range of P–T conditions documented from UHPM rocks, including those retrieved from HT–UHPM rocks, than the results of experiments from previous numerical models. In particular, the highest peak metamorphic temperatures (up to 1000 °C) are recorded in the case of the vertical crustal extrusion model in which subducted continental crust is subjected to a period of prolonged heating by asthenospheric mantle abutting the continental side of the vertically hanging slab. Nonetheless, some extreme temperature conditions which have been suggested for the Kokchetav and Bohemian massifs, perhaps up to 1100–1200 °C, are still to be achieved in experiments using numerical models.  相似文献   

13.
The distribution of rare earth elements was analyzed in the Early Cambrian diamondiferous calcsilicate rocks and gneisses, calciphyres, and marbles of the Kumdy-Kol deposit. These data were compared with the lithogeochemical characteristics of the sedimentary assemblages of weakly metamorphosed Late Precambrian graphite-bearing sedimentary rocks of the Kokchetav metamorphic belt. The obtained results allowed us to suppose that the protoliths of the Kumdy-Kol rocks were compositionally similar to the Late Precambrian graphite-bearing terrigenous-carbonate and sand-shale sequences of the continental shelf of the Kokchetav microcontinent, some of which were transformed in a subduction zone into diamondiferous rocks.  相似文献   

14.
After the discovery of metamorphic coesite in crustal rocks from the Western Alps (Italy) and the Western gneiss region (Norway) in the mid 1980s of the last century, metamorphic diamond was observed only a few years later “in situ” in the Kokchetav Massif (Kazakhstan). Findings of such coesite- and diamond-bearing ultrahigh pressure metamorphic (UHP) rocks with protoliths formed or embedded in crustal levels and subsequently experienced PT-conditions within or even higher than the coesite stability field have dramatically changed our geodynamic view of orogenetic processes. These occurrences provide evidence that crustal rocks were subducted into mantle depths and exhumed to the surface. Recent studies even suggest continental subduction to depths exceeding 300 km. These rocks have been extensively studied and many new and important observations have been made. Thus far, more than 350 papers have been published on various aspects of Kokchetav UHP rocks.The Kokchetav Massif of northern Kazakhstan is part of one of the largest suture zones in Central Asia and contains slices of HP and UHP metamorphic rocks. Classical UHP rocks mainly occur in the Kumdy Kol, Barchi Kol and Kulet areas, and include a large variety of lithologies such as calcsilicate rocks, eclogite, gneisses, schists, marbles of various compositions, garnet–pyroxene–quartz rocks, and garnet peridotite. Most of them contain microdiamonds; some of which reach a grain size of 200 μm. Most diamond grains show cuboid shapes but in rare cases, diamonds within clinozoisite gneiss from Barchi Kol occur as octahhedral form. Microdiamonds contain highly potassic fluid inclusions, as well as solid inclusions like carbonates, silicates and metal sulfides, which favour the idea of diamond formation from a C–O–H bearing fluid. Nitrogen isotope data and negative δ13C values of Kokchetav diamonds indicate a metasedimentary origin.PT-estimates of Kokchetav UHP rocks yield peak metamorphic conditions of at least 43 kbar at temperatures of about 950–1000 °C. Some zircon separates show inherited Proterozoic cores and 537–530 Ma UHP metamorphic mantle zones. Several Ar–Ar-ages on micas scatter around 529–528 and 521–517 Ma and reflect different stages of the exhumation history. Migmatization occurred during exhumation at about 526–520 Ma.Isotopic studies on calcsilicate rocks confirm a metasedimentary origin: δ18O values of garnet and clinopyroxene of a layered calcsilicate rock rule out the possibility having a primitive mantle protolith. Similar studies on eclogites indicate their basaltic protolith having experienced water–rock interaction prior to UHP metamorphism.A number of unique mineralogical findings have been made on Kokchetav UHP rocks. K-feldspar exsolutions in clinopyroxene demonstrate that potassium can be incorporated into the cpx-structure under upper mantle pressures. Other significant observations are coesite exsolutions in titanite, quartz-rods in cpx, the discovery of K-tourmaline as well as new minerals like kokchetavite, a hexagonal polymorph of K-feldspar and kumdykolite, an orthorhombic polymorph of albite.The Kokchetav UHP rocks represent a unique and challenging stomping ground for geoscientists of various disciplines. From crystallography, petrology and geochemistry to geophysics and geodynamics/geotectonics – it concerns all who are interested in the diverse metamorphic processes under upper mantle conditions.  相似文献   

15.
大别山碰撞造山带的地球动力学   总被引:33,自引:4,他引:33  
王清晨  林伟 《地学前缘》2002,9(4):257-265
大别山碰撞造山带的形成和其中超高压变质岩的形成折返具有统一的动力学过程。对大别山超高压变质岩形成 -折返的研究表明 ,大别山的超高压变质作用是冷大陆地壳被前导洋壳下拽而持续俯冲的结果。超高压变质岩的折返是多阶段的。第一阶段 (2 30~ 2 10Ma)在低地温梯度 (约10℃ /km)下发生同俯冲折返 ;第二阶段 (2 10~ 170Ma)的折返由深俯冲板片的断离引发 ,浮力开始起作用 ;第三阶段 (170~ 12 0Ma) ,以区域性岩浆活动、穹隆伸展构造活动和深剥蚀沉积为特征。从分析超高压变质岩的形成折返过程入手 ,以侏罗纪末作为时间参照点 ,以合肥盆地的侏罗系顶界作为当时的地理参照点 ,根据不同岩石单元中岩石的形成深度和碰撞造山中的位移状态 ,可把大别山碰撞造山带划分为原位系统、准原位系统、异位系统和热穹隆改造系统等结构单位。陆陆碰撞造山带形成的物理学前提是俯冲陆壳物质的低密度 ,而最终形成造山带的直接动力学过程则是深俯冲板片的断离及其引发的一系列近垂向运动的地质过程。  相似文献   

16.
桐柏-大别-苏鲁UHP和HP变质带的结构及流变学演化   总被引:8,自引:0,他引:8  
在岩石圈流变学基本原理指导下,运用现代构造解析学方法,在不同尺度上差别和分析了桐柏-大别-苏鲁UHP和HP变质带内深俯冲,同碰撞构造及UHP和HP岩石折返过程中的变形特征,重点讨论同碰撞形成的高角度网结状榴辉岩切带阵列,高角闪岩相剪切及有关变形组合以及碰撞期后伸展韧性薄化变形样式,强调指出不同地壳层次和物理条件下变形分解作用的重要性,而且,在UHP和HP变质带内最有效的应变体制是剪切作用,并在三维空间上形成不同格式的剪切带网状系统,以构造学记录为主线,结合已有可利用的岩石学,变质作用pT轨迹和同位素年代学资料,提出一个UHP和HP变质带尺度上的流变学演化模式,其中,UHP和HP变质岩石由地幔深度折返到地壳表层,经历了楔状挤出,碰撞期后地壳韧性薄化及晚造山伸展塌陷,揭顶作用等多个阶段的动力学过程。  相似文献   

17.
INTRODUCTIONUptonowthereisinagreementonthetectonic-dynamicbackgroundoftheformationofUHPmetamorphicrocks,i.e.,theUHPMrocksareproductsofobliquecollisionbe-tweentheYangtzeandSinokoreancratonsinIndosinianstage(Jahn,1998lWangandCong,l998,1996;Lietal.,l997,l996iHackeretal.,l996ILiouet.al.,l9961Okay;Sen-gor,l993,CongandWang,l994;Sengor,1993).Buthowthesemetamorphicrocksareformedatmantledepthexhumedbacktothesurfacesorapidlyisstillastandingproblem-TheexhumationofUHPMrocksisacomplextectoni…  相似文献   

18.
High‐ to ultrahigh‐pressure (HP‐UHP) metamorphic rocks that resulted from deep continental subduction and subsequent exhumation in the Sulu orogenic belt, China, have experienced multiphase deformation and metamorphic overprint during its long journey to the mantle and return to the surface. HP‐UHP shear zones are strain‐localized weak zones on which the UHP slab is transported over long distances. HP‐UHP shear zones are well exposed along a 200‐km belt in the Sulu UHP metamorphic belt. The shear zones lie structurally below the UHP rocks and above the non‐UHP rocks, suggesting the early exhumation of the UHP rocks by thrusting. The large area distribution, HP‐UHP nature, high strain and structural association of the shear zones with the UHP rocks suggest that the shear zones are probably a regional detachment developed during the early stage of exhumation of the UHP rocks. Kinematic indicators suggest top‐to‐the N–NW motion of the UHP slab during the exhumation, which, combined with isotope signature in Mesozoic igneous rocks, leads us to the interpretation that the subduction polarity is the North China plate down to the south rather than the Yangtze plate down to the north in the Sulu region.  相似文献   

19.
Ultrahigh-pressure(UHP) metamorphic rocks are distinctive products of crustal deep subduction,and are mainly exposed in continental subduction-collision terranes. UHP slices of continental crust are usually involved in multistage exhumation and partial melting, which has obvious influence on the rheological features of the rocks, and thus significantly affect the dynamic behavior of subducted slices. Moreover,partial melting of UHP rocks have significant influence on element mobility and related isotope behavior within continental subduction zones, which is in turn crucial to chemical differentiation of the continental crust and to crust-mantle interaction.Partial melting can occur before, during or after the peak metamorphism of UHP rocks. Post-peak decompression melting has been better constrained by remelting experiments; however, because of multiple stages of decompression, retrogression and deformation, evidence of former melts in UHP rocks is often erased. Field evidence is among the most reliable criteria to infer partial melting. Glass and nanogranitoid inclusions are generally considered conclusive petrographic evidence. The residual assemblages after melt extraction are also significant to indicate partial melting in some cases. Besides field and petrographic evidence, bulk-rock and zircon trace-element geochemical features are also effective tools for recognizing partial melting of UHP rocks. Phase equilibrium modeling is an important petrological tool that is becoming more and more popular in P-T estimation of the evolution of metamorphic rocks; by taking into account the activity model of silicate melt, it can predict when partial melting occurred if the P-T path of a given rock is provided.UHP silicate melt is commonly leucogranitic and peraluminous in composition with high SiO_2,low MgO, FeO, MnO, TiO_2 and CaO, and variable K_2 O and Na_2 O contents. Mineralogy of nanogranites found in UHP rocks mainly consists of plagioclase + K-feldspar + quartz, plagioclase being commonly albite-rich.Trace element pattern of the melt is characterized by significant enrichment of large ion lithophile elements(LILE), depletion of heavy rare earth elements(HREE) and high field strength elements(HFSE),indicating garnet and rutile stability in the residual assemblage. In eclogites, significant Mg-isotope fractionation occurs between garnet and phengite; therefore, Mg isotopes may become an effective indicator for partial melting of eclogites.  相似文献   

20.
Ultra high-pressure (UHP) eclogites from Sulu region (China) represent mafic components of the continental crust, which were first subducted to mantle depths greater than 100 km and then exhumed to the earth's surface. Detailed investigation of microstructures, chemical compositions, petrofabrics and seismic properties of the UHP eclogites can provide important information on the operating deformation mechanisms and rheology of subducted continental crust and on the origin of seismic reflections within the upper mantle. We present here results from field, optical and TEM observations, electron back-scattered diffraction (EBSD) measurements and numerical computations of the seismic properties of UHP eclogites collected from fresh surface outcrops at the drill site (Maobei, Donghai County, Jiangsu Province) of the Chinese Continental Scientific Drilling Program (CCSD). Two types of eclogites have been distinguished: Type-1 (coarse-grained) eclogites deformed by recovery-accommodated dislocation creep at the peak metamorphic conditions, and Type-2 (fine-grained) eclogites which are composed of reworked Type-1 materials during recrystallization-accommodated dislocation creep in shear zones which were active during the exhumation of the UHP metamorphic rocks. Both garnet and omphacite in these eclogites deformed plastically and the flow strength contrast between these two constituent minerals is apparently much less than an order of magnitude under the UHP metamorphic conditions. Plasticity of eclogites under UHP conditions can effectively facilitate channeled flow along the interplate shear zone. The preservation of the relict crustal materials within the continental lithosphere may produce regionally extensive, strong, seismic reflections in the upper mantle. This may explain the origin of mantle reflections observed in many areas of the world.  相似文献   

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