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1.
The Carpathian–Pannonian Region contains Neogene to Quaternary magmatic rocks of highly diverse composition (calc-alkaline, shoshonitic and mafic alkalic) that were generated in response to complex microplate tectonics including subduction followed by roll-back, collision, subducted slab break-off, rotations and extension. Major element, trace element and isotopic geochemical data of representative parental lavas and mantle xenoliths suggests that subduction components were preserved in the mantle following the cessation of subduction, and were reactivated by asthenosphere uprise via subduction roll-back, slab detachment, slab-break-off or slab-tearing. Changes in the composition of the mantle through time are evident in the geochemistry, supporting established geodynamic models.Magmatism occurred in a back-arc setting in the Western Carpathians and Pannonian Basin (Western Segment), producing felsic volcaniclastic rocks between 21 to 18 Ma ago, followed by younger felsic and intermediate calc-alkaline lavas (18–8 Ma) and finished with alkalic-mafic basaltic volcanism (10–0.1 Ma). Volcanic rocks become younger in this segment towards the north. Geochemical data for the felsic and calc-alkaline rocks suggest a decrease in the subduction component through time and a change in source from a crustal one, through a mixed crustal/mantle source to a mantle source. Block rotation, subducted roll-back and continental collision triggered partial melting by either delamination and/or asthenosphere upwelling that also generated the younger alkalic-mafic magmatism.In the westernmost East Carpathians (Central Segment) calc-alkaline volcanism was simultaneously spread across ca. 100 km in several lineaments, parallel or perpendicular to the plane of continental collision, from 15 to 9 Ma. Geochemical studies indicate a heterogeneous mantle toward the back-arc with a larger degree of fluid-induced metasomatism, source enrichment and assimilation on moving north-eastward toward the presumed trench. Subduction-related roll-back may have triggered melting, although there may have been a role for back-arc extension and asthenosphere uprise related to slab break-off.Calc-alkaline and adakite-like magmas were erupted in the Apuseni Mountains volcanic area (Interior Segment) from15–9 Ma, without any apparent relationship with the coeval roll-back processes in the front of the orogen. Magmatic activity ended with OIB-like alkali basaltic (2.5 Ma) and shoshonitic magmatism (1.6 Ma). Lithosphere breakup may have been an important process during extreme block rotations (60°) between 14 and 12 Ma, leading to decompressional melting of the lithospheric and asthenospheric sources. Eruption of alkali basalts suggests decompressional melting of an OIB-source asthenosphere. Mixing of asthenospheric melts with melts from the metasomatized lithosphere along an east–west reactivated fault-system could be responsible for the generation of shoshonitic magmas during transtension and attenuation of the lithosphere.Voluminous calc-alkaline magmatism occurred in the Cãlimani-Gurghiu-Harghita volcanic area (South-eastern Segment) between 10 and 3.5 Ma. Activity continued south-eastwards into the South Harghita area, in which activity started (ca. 3.0–0.03 Ma, with contemporaneous eruption of calc-alkaline (some with adakite-like characteristics), shoshonitic and alkali basaltic magmas from 2 to 0.3 Ma. Along arc magma generation was related to progressive break-off of the subducted slab and asthenosphere uprise. For South Harghita, decompressional melting of an OIB-like asthenospheric mantle (producing alkali basalt magmas) coupled with fluid-dominated melting close to the subducted slab (generating adakite-like magmas) and mixing between slab-derived melts and asthenospheric melts (generating shoshonites) is suggested. Break-off and tearing of the subducted slab at shallow levels required explaining this situation.  相似文献   

2.
斑岩Cu-Mo-Au矿床:新认识与新进展   总被引：59，自引：0，他引：59  
侯增谦 《地学前缘》2004,11(1):131-144
斑岩型矿床作为一种最重要的铜钼和铜金矿床类型一直得到人们的普遍重视 ,近些年来又取得了重要研究进展 ,主要体现在 5个方面 :①岛弧和陆缘弧是斑岩型矿床产出的重要环境 ,但大陆碰撞造山带也具有产出斑岩型矿床的巨大潜力。按矿床产出的构造环境 ,可以分为弧造山型斑岩矿床和碰撞造山型斑岩矿床 ;②弧造山型含矿斑岩主要为钙碱性和高钾钙碱性 ,而碰撞造山型含矿斑岩则主要为高钾钙碱性和橄榄安粗质 (shoshonitic)。两种环境的含矿斑岩多具有埃达克岩 (adakite)岩浆亲合性 ,但前者主要来源于俯冲的大洋板片 ,后者主要来源于碰撞加厚的下地壳。大洋板片的部分熔融缘于俯冲角度的平缓化 ,而加厚下地壳的熔融起因于俯冲大陆板片的断离 (slabbreakoff) ;③在弧造山环境 ,大洋俯冲板片的膝折 (kink)或撕裂 (slabtear)不仅导致俯冲角度变缓 ,而且引起弧地壳耦合变形 ,产生切弧断裂 ,控制斑岩铜系统的时空分布。俯冲板片撕裂引发软流圈上涌 ,诱发大洋板片熔融 ,产生含矿岩浆 ;④在碰撞造山环境 ,大陆俯冲板片的裂离导致软流圈上涌 ,向下地壳注入新生物质 ,并诱发下地壳物质熔融 ,产生含矿岩浆。碰撞后地壳伸展形成横切碰撞带的正断层系统 ,为斑岩侵位提供运移通道 ,并导致岩浆流体大量分凝和铜钼金淀积。不论  相似文献   

3.
俯冲带部分熔融   总被引：3，自引：3，他引：0  
张泽明  丁慧霞  董昕  田作林 《岩石学报》2020,36(9):2589-2615
俯冲带是地幔对流环的下沉翼,是地球内部的重要物理与化学系统。俯冲带具有比周围地幔更低的温度,因此,一般认为俯冲板片并不会发生部分熔融,而是脱水导致上覆地幔楔发生部分熔融。但是,也有研究认为,在水化的洋壳俯冲过程中可以发生部分熔融。特别是在下列情况下,俯冲洋壳的部分熔融是俯冲带岩浆作用的重要方式。年轻的大洋岩石圈发生低角度缓慢俯冲时,洋壳物质可以发生饱和水或脱水熔融,基性岩部分熔融形成埃达克岩。太古代的俯冲带很可能具有与年轻大洋岩石圈俯冲带类似的热结构,俯冲的洋壳板片部分熔融可以形成英云闪长岩-奥长花岗岩-花岗闪长岩。平俯冲大洋高原中的基性岩可以发生部分熔融产生埃达克岩。扩张洋中脊俯冲可以导致板片窗边缘的洋壳部分熔融形成埃达克岩。与俯冲洋壳相比,俯冲的大陆地壳具有很低的水含量,较难发生部分熔融,但在超高压变质陆壳岩石的折返过程中可以经历广泛的脱水熔融。超高压变质岩在地幔深部熔融形成的熔体与地幔相互作用是碰撞造山带富钾岩浆岩的可能成因机制。碰撞造山带的加厚下地壳可经历长期的高温与高压变质和脱水熔融,形成S型花岗岩和埃达克质岩石。  相似文献   

4.
We need to understand chemical recycling at convergent margins and how chemical interactions between subducted slab and the overlying mantle wedge affect mantle evolution and magmagenesis. This requires distinguishing contributions from recycled individual subducted components as well as those contributed by the mantle. We do this by examining magmatic products generated at different depths above a subduction zone, in an intra-oceanic arc setting. The Guguan cross-chain in the intra-oceanic Mariana arc overlies subducted Jurassic Pacific plate lithosphere at depths of ~125--230 km and erupts mostly basalt. Basalts from rear-arc volcanoes are more primitive than those from the magmatic front, in spite of being derived by lower degrees of melting of less-depleted mantle. Rear-arc magmas also show higher temperatures and pressures of equilibration. Coexisting mineral compositions become more MORB- or OIB-like with increasing height above the subduction zone. Trace element and isotopic variations indicate that the subduction component in cross-chain lavas diminishes with increasing depth to the subduction zone, except for water contents. There is little support for the idea that melting beneath the Mariana Trough back-arc basin depleted the source region of arc magmas, but melting to form rear-arc volcanoes may have depleted the source of magmatic front volcanoes. Enrichments in rear-arc lavas were not caused by sediment melting; the data instead favor an OIB-type mantle that has been modestly affected by subduction zone fluids. Our most important conclusion is that sediment fluids or melts are not responsible for the K--h relationship and other cross-chain chemical and isotopic variations. We speculate that an increasing role for supercritical fluids released from serpentinites interacting with modestly enriched mantle might be responsible for cross-chain geochemical and isotopic variations. Electronic Supplementary Material Supplementary material is available for this article at and is accessible for authorized users.  相似文献   

5.
Petrogenesis and tectonic setting of the Roman Volcanic Province, Italy   总被引：11，自引：0，他引：11  
L. Beccaluva  P. Di Girolamo  G. Serri 《Lithos》1991,26(3-4):191-221
The volcanism in the Roman Province of Italy can be modelled by the partial melting of heterogeneously enriched mantle sources. The heterogeneity was created by materials derived from a subducted slab which can still be traced geophysically beneath the central Apennines.

New petrographical and chemical data are presented for the high-K calc-alkaline and the shoshonitic volcanics of the Campania region. Primary magmas are present only locally. The existence of spatial zonation in the volcanism of Campania is documented for the first time. The shoshonitic, leucite-basanitic and leucititic volcanics of the Phlegraean Fields-Procida-Ischia and the Somma-Vesuvius areas are, at similar degrees of evolution, about two times richer in Nb and Ba than those of northwestern Campania and the Latium part of the Roman Province. Accordingly, distinct north-western and south-eastern subprovinces can be defined. The evaluation of enrichment factors, that is the abundance ratio between the average contents of each element in the relatively primitive lavas of the low K- and the high K suites, shows that the mantle sources prior to K-metasomatism were different in the two sub-provinces of the Roman Province. In the north-western one, they resembled the sources of ocean-island tholeiites and moderately enriched MOR-basalts. In the south-east they were similar to those of ocean island alkaline lavas and enriched MORB's.

Modelling based on K, P, Ce, Sr, Rb, Ba, Th, Sm, Eu, Gd, Y, Nb and 87Sr/86Sr was carried out. It indicates that the range of mantle sources of the volcanics in northwestern Campania and Latium can be modelled by the addition of 3 to 20% of materials derived by partial melting of carbonaceous pelites to a Sr-enriched mantle wedge comparable to the Honolulu mantle source least enriched in Nb.

The production of Sr-enriched mantle wedge requires either the action of fluids produced by dehydration of subducted oceanic crust, or a small amount of metasomatism caused by the presence of carbonatite melts.

The near absence of Ti, Ta, Nb, Yb and the highly fractionated REE in the metasomatizing component requires the presence of residual garnet and accessory Ti-rich minerals during the partial melting of the subducted sediments. The writers propose that the mantle wedge overlying the subducted slab was hybridized by melts produced by partial fusion of subducted material derived from the continental crust, probably sediments. This process played a dominant role in the generation of the mantle sources from which the high-K calc-alkaline, shoshonitic, leucite-basanitic and leucititic magmas of the Roman Province were derived.  相似文献   


6.
The magmatic arc of the Fuegian Andes is composed mostly of Upper Mesozoic to Cenozoic calc-alkaline plutons and subordinated lavas. To the rear arc, however, isolated mid-Cretaceous monzonitic plutons and small calc-alkaline dykes and sills crop out. This calc-alkaline unit (the Ushuaia Peninsula Andesites, UPA) includes hornblende-rich, porphyritic quartz meladiorites, granodiorites, andesites, dacites and lamprophyres. Radiometric dating and cross-cutting relationships indicate that UPA is younger than the monzonitic suite. The geochemistry of UPA is medium to high K, with high LILE (Ba 500–2000 ppm, Sr 800–1400 ppm), HFSE (Th 7–23 ppm, Nb 7–13 ppm, Ta 0.5–1.1 ppm) and LREE (La 16–51 ppm) contents, along with relatively low HREE (Yb 1.7–1.3 ppm) and Y (9–19 ppm). The similar mineralogy and geochemistry of all UPA rocks suggest they evolved from a common parental magma, by low pressure crystal fractionation, without significant crustal assimilation. A pure Rayleigh fractionation model indicates that 60–65% of crystal fractionation of 60% hornblende + 34% plagioclase + 4% clinopyroxene + 1% Fe-Ti oxide, apatite and sphene (a paragenesis similar of UPA mafic rocks) can explain evolution from lamprophyres to dacites. The UPA has higher LILE, HFSE and LREE, and lower HREE and Y than the calc-alkaline plutons and lavas of the volcanic front. The HREE and Y are lower than in the potassic plutons as well. High concentrations of Th, Nb, Ta, Zr, Hf, LREE and Ce/Pb, and low U/Th, Ba/Th ratios in UPA, even in the least differentiated samples, suggest contributions from subducted sediments to the mantle source. On the other hand, relatively low HREE and Y, high LREE/HREE (La/Yb 11–38) ratios and Nb-Ta contents can be interpreted as mantle metasomatism by partial melts of either subducted garnetiferous oceanic sediment or basalt as well. Additionally, high LILE content in UPA, similar to the potassic plutons, suggests also a mantle wedge previously metasomatized by potassic parental magmas in their route to crustal levels. Therefore, UPA represents a unique suite in the Fuegian arc generated in a multiple hybridized source. UPA generation is related to a transition from normal to flat subduction which additionally caused the widening and landward migration of the magmatic arc, as well as crustal deformation. Rear-arc magmatism endured ca. 22 m.y.; afterwards, calc-alkaline magmatism remained at the volcanic front.  相似文献   

7.
本文对藏南冈底斯带中段的花岗岩类和角闪辉长岩进行了锆石U-Pb年代学和全岩地球化学分析,据此阐明了岩体的形成机制与演化过程,并探讨了成岩时的大地构造背景。分析结果显示,研究区内花岗岩类和角闪辉长岩体的LA-ICPMS锆石U-Pb定年结果为41~55Ma,为始新世早-中期岩浆活动的产物,代表了区内岩体的成岩年龄。在地球化学组成上,花岗岩类属于钙碱性到高钾钙碱性系列,均富集轻稀土(LREE)和大离子亲石元素(LILE)(Rb、Ba和K),强烈亏损Nb、Ta、P等高场强元素(HFSE),具有弧型岩浆岩的地球化学组成。此外,花岗岩类的铝饱和指数(A/CNK)小于1.1,属于准铝质到弱过铝质的I型花岗岩。角闪辉长岩为石榴橄榄岩部分熔融的产物,并在后期侵位的过程中遭受到了壳源物质的混染。综合分析表明,研究区内的岩体形成于初始碰撞向主碰撞的转化阶段。始新世早期(～50Ma)新特提斯洋板片的断离引起软流圈物质上涌,导致岩石圈地幔发生部分熔融形成基性岩浆,随后基性岩浆底侵至下地壳并诱发下地壳发生部分熔融形成花岗岩质岩浆,最后经过岩浆混合作用形成始新世早-中期冈底斯地区的花岗岩类。  相似文献   

8.
We use published and new trace element data to identify element ratios which discriminate between arc magmas from the supra-subduction zone mantle wedge and those formed by direct melting of subducted crust (i.e. adakites). The clearest distinction is obtained with those element ratios which are strongly fractionated during refertilisation of the depleted mantle wedge, ultimately reflecting slab dehydration. Hence, adakites have significantly lower Pb/Nd and B/Be but higher Nb/Ta than typical arc magmas and continental crust as a whole. Although Li and Be are also overenriched in continental crust, behaviour of Li/Yb and Be/Nd is more complex and these ratios do not provide unique signatures of slab melting. Archaean tonalite-trondhjemite-granodiorites (TTGs) strongly resemble ordinary mantle wedge-derived arc magmas in terms of fluid-mobile trace element content, implying that they did not form by slab melting but that they originated from mantle which was hydrated and enriched in elements lost from slabs during prograde dehydration. We suggest that Archaean TTGs formed by extensive fractional crystallisation from a mafic precursor. It is widely claimed that the time between the creation and subduction of oceanic lithosphere was significantly shorter in the Archaean (i.e. 20 Ma) than it is today. This difference was seen as an attractive explanation for the presumed preponderance of adakitic magmas during the first half of Earth's history. However, when we consider the effects of a higher potential mantle temperature on the thickness of oceanic crust, it follows that the mean age of oceanic lithosphere has remained virtually constant. Formation of adakites has therefore always depended on local plate geometry and not on potential mantle temperature.  相似文献   

9.
Herv Martin 《Lithos》1993,30(3-4):373-388
The petrographic and chemical composition of magmatic rocks generated during the Archaean appears to be different from that of post-Archaean rocks. Komatiites are widespread before 2.5 Ga and rarely occur afterwards. In addition the Archaean continental crust is primarily TTG (Tonalitic, Trondhjemitic and Granodioritic) in composition, exhibiting typical trondhjemitic differentiation trends; whereas modern equivalents are granodioritic to granitic following classical calc-alkaline differentiation trends. This distinction becomes more prominent when rare-earth elements (REE) are taken into account: Archaean TTG are Yb-poor (YbN < 8.5) and have high (La/Yb) ratios (5 < (La/Yb)N < 150), in comparison, the post-2.5 Ga granitoids, emplaced in subduction-zone geodynamic environments have high Yb content (4.5N<20) with very low (La/Yb)N ratios ( 20). Theoretical calculations and experimental petrology have shown that the TTG can be produced by partial melting of an Archaean tholeiite transformed into garnet-bearing amphibolite. Consequently, the low heavy REE content of the TTG is explained by the influence of both residual garnet and hornblende in their source. After 2.5 Ga the role of these minerals in calc-alkaline magma genesis becomes progressively less important, which is interpreted in terms of a cooling Earth model.

In modern subduction zone environments the subducted oceanic slab is relatively “old and cold” and the geothermal gradient along the Benioff plane in low (ca. 10°C/km). Consequently, the down-going lithosphere undergoes dehydration before partial melting is able to occur. The liberated fluids are light REE and LILE-enriched and ascend into the overlying mantle wedge where they induced partial fusion. The produced magmas separate from their mantle source region leaving a residue mainly composed of olivine and pyroxenes. Mantle derived magmas typically exhibit high Yb contents due to low KDYb values for olivine and pyroxenes. During the Archaean, the subducted lithosphere was relatively “young and hot” providing high geothermal gradients along the Benioff zone. Thus, partial melting of the subducted slab was possible at lower temperatures before dehydration would take place. Garnet and hornblende are the main residual phases accounting for the low Yb contents of the Archaean TTG.

This model can be tested using a modern analogue of Archaean-like subduction processes. In south Chile an oceanic ridge has subducted and all thermodynamic calculations indicate that this creates locally high geothermal gradients along the Benioff zone. Thus in very small areas, Archaean-like environments may be simulated in modern subduction zones. The modern andesites produced in this environment show Archaean geochemical characteristics with low YbN (<5), whereas the majority of andesites along the Andean arc have modern patterns with YbN ranging from 8 to more than 17. This conclusion was generalised to all young subducted lithospheres all over the world.

In conclusion, it appears that since the Archaean there has been a change in the site of continental crust genesis. The location of calc-alkaline magma source in subduction-zone environments has migrated through time from the subducted slab to the mantle wedge. This is a direct consequence of the progressive cooling of the Earth.  相似文献   


10.
Compositionally, high-Nb basalts are similar to HIMU (high U/Pb) ocean island basalts, continental alkaline basalts and alkaline lavas formed above slab windows. Tertiary alkaline basaltic lavas from eastern Jamaica, West Indies, known as the Halberstadt Volcanic Formation have compositions similar to high-Nb basalts (Nb > 20 ppm). The Halberstadt high-Nb basalts are divided into two compositional sub-groups where Group 1 lavas have more enriched incompatible element concentrations relative to Group 2. Both groups are derived from isotopically different spinel peridotite mantle source regions, which both require garnet and amphibole as metasomatic residual phases. The Halberstadt geochemistry demonstrates that the lavas cannot be derived by partial melting of lower crustal ultramafic complexes, metasomatised mantle lithosphere, subducting slabs, continental crust, mantle plume source regions or an upper mantle source region composed of enriched and depleted components. Instead, their composition, particularly the negative Ce anomalies, the high Th/Nb ratios and the similar isotopic ratios to nearby adakite lavas, suggests that the Halberstadt magmas are derived from a compositionally variable spinel peridotite source region(s) metasomatised by slab melts that precipitated garnet, amphibole, apatite and zircon. It is suggested that high-Nb basalts may be classified as a distinct rock type with Nb > 20 ppm, intraplate alkaline basalt compositions, but that are generated in subduction zones by magmatic processes distinct from those that generate other intraplate lavas.  相似文献   

11.
During the Neogene, a magmatic change from calc-alkaline to alkaline types occurred in all the regions surrounding the western Mediterranean. This change has been studied in Oranie (western Algeria). In this area, potassic to shoshonitic calc-alkaline andesites (with La/Nb ratios in the range 4–6) were mainly erupted between 12 and 9 Ma. They were followed (between 10 and 7 Ma) by basalts displaying geochemical features which are transitional between calc-alkaline and alkaline lavas (La/Nb=1–1.7). After a ca. 3-Ma quiescence period, volcanic activity resumed, with the eruption of OIB-type alkaline basalts (La/Nb=0.5–0.6), from 4 to 0.8 Ma. A combined geochemical approach, using incompatible elements and Sr, Nd and O isotopes, allows us to conclude that the transitional basalts derived from the melting of a heterogeneous mantle source, at the boundary between lithosphere and asthenosphere. We propose that melting of a previously subduction-modified lithospheric mantle occurred between 12 and 10 Ma, in response to the upwelling of hot asthenosphere flowing up into an opening gap above a detached sinking slab. As a result, calc-alkaline magmas were formed. From 10 to 7 Ma, the transitional basalts were generated through melting of the boundary mantle zone between the lithosphere and the upwelling asthenosphere. During that stage, the contribution of the lithospheric source was still predominant. Then, as sinking of the oceanic slab progressed, the increasing uprise of the asthenosphere led to the formation and emplacement (from 4 to 0.8 Ma) of typical within-plate alkaline basalts derived from a plume-modified asthenospheric mantle.  相似文献   

12.
钨的地球化学性质与华南地区钨矿成因   总被引：2，自引：1，他引：2  
在地球演化早期的强还原条件下,钨表现为中等亲铁元素,因此地球中 90%的钨进入地核。在地幔和地壳的演化过程中,钨是极度不相容亲石元素,从而导致钨元素在地壳中的丰度约是地幔丰度的250倍。钨在岩浆熔体中主要以钨酸的形式迁移,在成矿热液中主要以氟、硼化合物或其络合物的形式运移。钨的矿化需要其在部分熔融、岩浆演化和晚期热液等各阶段逐渐富集。中国是世界上钨矿产资源最丰富的国家,约占世界总储量的60%以上,其中绝大多数矿床产在华南地区,与华南大规模的中生代岩浆活动具有密切的时空联系。微量元素特征(高Rb/Sr和K/Rb比值,低Nb/Ta和Zr/Hf比值)显示它们往往经历了强烈的岩浆分异,这可能与这些花岗岩通常具有高挥发分含量(如F)有关。岩浆中高的F含量对钨的富集和矿化十分重要,它可以降低熔体固相线、粘度和密度,有利于提高岩浆的结晶分异程度,因而使得高度不相容的钨元素在岩浆演化过程和后期热液阶段的富集与矿化。富挥发分岩浆的形成可能与俯冲板块后撤,软流圈物质上涌导致的多硅白云母等富F矿物的高温分解有关。研究表明,华南南岭地区侏罗纪的钨矿化花岗岩主要形成于太平洋板块的俯冲后撤,而华南南部晚白垩世钨成矿作用与新特提斯洋的俯冲后撤有关。  相似文献   

13.
Distribution of the Neogene calc-alkaline magmatism of the Carpathian arc is directly related in space and time to the kinematics of the two major terranes of the Intracarpathian area (Alcapa, Tisia-Getia) along the south-eastern border of the European plate. In the West Carpathians and adjacent areas, the volcanic activity occurred between 20–11 Ma, with large volumes of both acidic and intermediate rocks, generally distributed randomly, sometimes transversally to the orogenic belt and as rare small occurrences along the Flysch belt. In the East Carpathians, the volcanic rocks are distributed along the northern margin of the Zemplin block, the north–easternmost part of the Alcapa and eastward along the front of the Getic block, at the contact with European plate. Between Tokaj-Slanské-Vihorlat up to northern Cãlimani Mountains, the magmatism occurred between 14–9 Ma, and along the Cãlimani-Harghita chain between 9–0.2 Ma. The calc-alkaline magmatic rocks of the Apuseni Mountains are located in the interior of the Tisia block and occurred between 14–9 Ma. The generation of the calc-alkaline magmatism is considered here as the result of complex interplay between plate roll-back and lithospheric detachment tectonic processes and the break-off of the subducted plate, mostly in a post-collisional setting. (1) The magmatites of the Western Carpathians and the Pannonian basin were generated in direct relation to subduction roll-back processes, over the downgoing slab, during the period of lateral extrusion and back-arc extension. In this area, characterized by maximum crustal shortening, we can infer further delamination processes to explain the generation of magmas. (2) The magmatic rocks from the northern sector of the East Carpathians (Tokaj-Slanské-Vihorlat up to the Northern Cãlimani Mountains), resulted after subduction roll-back processes and an almost simultaneous break-off of the descending plate all along the arc segment during main clockwise rotation of the Intracarpathian terranes. (3) In the eastern sector of the East Carpathians (Cãlimani up to Harghita Mountains), the magmatic rocks were generated through partial melting of the subducted slab followed by gradual break-off of the subducted plate along strike (north to south). (4) The Apuseni Mts. magmatic activity resulted in transtensional tectonic regime by decompressional melting of lithospheric mantle, during the translation and rotation of Tisia-Getia block.  相似文献   

14.
江西会昌盆地晚白垩世喷发的站塘安山岩,其形成与晚中生代岩石圈伸展和玄武质岩浆的底侵作用有关。这些岩石是高Na(6.59%～8.46%Na2O)、高Al的奥长花岗质岩石,具有与埃达克岩相似的高Sr和Ba、低Y和HREE、高Sr/Y和La/Yb比等特点。与埃达克岩相比,它们的Na2O较高而CaO较低,其εNd(t)值-2.3～-3.8和87Sr/86Sr初始比值0.707～0.708也与具大洋同位素组成特征的埃达克岩有明显区别。这些化学的和同位素特征,表明它们并非消减板片部分熔融的产物。站塘埃达克质岩浆可能源自底侵玄武质下地壳,其异常的高Na和低Ca特点反映其源岩成分的特殊性。因其成分与由实验产生的富碱玄武岩部分熔融体组成相当,因此,我们认为站塘高钠安山质岩浆可能是富碱玄武质岩石部分熔融的产物。  相似文献   

15.
A. Yu. Martynov 《Petrology》2013,21(5):471-488
Geochemical data obtained on volcanic rocks produced during the early evolutionary stages in Kunashir Island provide insight into certain important aspect of the evolution of the subduction system. The mafic lavas of all age intervals exhibit clearly pronounced across-arc geochemical zoning, which implies that these rocks were produced in the environment of a subducted oceanic slab. The high Ba/Th and U/Th ratios of basalts from the frontal zones suggest that an important role in magma generation was played by a low-temperature aqueous fluid. The arc lavas of the Early Miocene, Pliocene, and Pliocene-Pleistocene episodes in the evolution of the island arc system provide evidence of the melting of subducted sediments, which testifies, when considered together with the calculated P-T conditions under which the high-Mg basalts were derived, that backarc tectono-magmatic processes affected subduction-related magmatic generation. Active mantle diapirism and volcanic activity in the opening Kurile Basin resulted in the heating of the suprasubduction mantle in the rear zone, the involvement of the upper sedimentary layer of the oceanic slab in the process of melting, and the eventual generation of basaltic magmas with unusual geochemical characteristics.  相似文献   

16.
东天山卡拉塔格泥盆纪岩浆岩地球化学特征及成因   总被引：1，自引：0，他引：1  
文中对卡拉塔格地区泥盆纪岩浆岩进行了系统的岩相学、岩石地球化学研究,探讨其成因及形成构造背景。卡拉塔格地区泥盆纪火山岩主要为安山岩,并被同期一套成分连续的侵入体,包括辉长岩、闪长岩、石英闪长岩、二长岩等侵入。其中,辉长岩为钙碱性低钾系列准铝质岩石,具有较高的Al2O3含量(18.76%~19.06%)和Mg#(57.28~69.37),具有正Eu异常;闪长岩、石英闪长岩、二长岩和安山岩为钙碱性高钾钙碱性系列的准铝质弱过铝质岩石,也具有较高的Al2O3含量(15.02%~17.43%)和Mg#(53.67~72.91),具有较弱的Eu负异常或无Eu异常。这些岩浆岩都具有较低的初始Sr值(0.703 11~0.705 18)以及较高的εNd(t)值(5.36~7.72),均富集轻稀土和大离子亲石元素Rb、Ba、K等,亏损重稀土和高场强元素Ta、Nb、Ti等,都具有岛弧岩浆岩的特征。相似的岩石地球化学特征显示它们可能为同源岩浆活动的产物,可能是由俯冲洋壳形成的流体交代地幔楔岩石发生部分熔融而形成。泥盆纪岩浆岩形成于康古尔洋向卡拉麦里洋俯冲的岛弧背景。  相似文献   

17.
Dirk Küster  Ulrich Harms 《Lithos》1998,45(1-4):177-195
Potassic metaluminous granitoids with enrichments of HFS elements constitute part of widespread post-collisional magmatism related to the Late Neoproterozoic Pan-African orogeny in northeastern Africa (Sudan, Ethiopia, Somalia) and Madagascar. The plutons were emplaced between 580 and 470 Ma and comprise both subsolvus and hypersolvus biotite–granite, biotite–hornblende–granite, quartz–monzonite and quartz–syenite. Pyroxene-bearing granitoids are subordinate. Basic dikes and enclaves of monzodioritic composition are locally associated with the granitoid plutons. Granitoids emplaced in pre-Neoproterozoic crust have Sri-ratios between 0.7060 and 0.7236 and Nd(t) values between −15.8 and −5.6 while those emplaced in, or close to the contact with, juvenile Neoproterozoic crust have lower Sri-ratios (0.7036–0.7075) and positive Nd(t) values (4.6). However, it is unlikely that the potassic granitoids represent products of crustal melting alone. The association with basic magmas derived from subduction-modified enriched mantle sources strongly suggests that the granitoids represent hybrid magmas produced by interaction and mixing of mantle and crust derived melts in the lower crust. The most intense period of this potassic granitoid magmatism occurred between 585 and 540 Ma, largely coeval with HT granulite facies metamorphism in Madagascar and with amphibolite facies retrogression in northeastern Africa (Somalia, Sudan). Granitoid magmatism and high-grade metamorphism are probably both related to post-collisional lithospheric thinning, magmatic underplating and crustal relaxation. However, the emplacement of potassic granites continued until about 470 Ma and implies several magmatic pulses associated with different phases of crustal uplift and cooling. The potassic metaluminous granites are temporally and spatially associated with post-collisional high-K calc-alkaline granites with which they share many petrographical, geochemical and isotopical similarities, except the incompatible element enrichments. The resemblance indicates a strongly related petrogenesis of both granite associations.  相似文献   

18.
位于青藏高原南部的冈底斯岩浆弧形成于中生代新特提斯大洋岩石圈的长期俯冲过程中,而且在印度与亚洲大陆碰撞过程中叠加了强烈的新生代岩浆作用,是世界上典型的复合型大陆岩浆弧,已经成为研究汇聚板块边缘岩浆作用和大陆地壳生长与再造的天然实验室。基于对现有研究成果的总结,我们将冈底斯岩浆弧的岩浆构造演化划分为5个阶段：第1阶段发生在晚白垩世之前,以新特提斯洋岩石圈长期正常俯冲和钙碱性弧岩浆岩的发育为特征;第2阶段发生在晚白垩世时期,以活动的新特提斯洋中脊发生俯冲和强烈的岩浆作用与显著的新生地壳生长为特征;第3阶段发生在晚白垩世晚期,以残余的新特提斯大洋岩石圈俯冲和正常弧型岩浆作用为特征;第4阶段发生在古新世至中始新世,以印度与亚洲大陆碰撞、俯冲的新特提斯洋岩石圈回转和断离,及其诱发的幔源岩浆作用、新生和古老地壳的强烈再造为特征;第5阶段为发生在晚渐新世到中中新世的后碰撞阶段,深俯冲印度岩石圈的回转和断离,或加厚岩石圈地幔的对流移去导致了加厚下地壳的部分熔融和埃达克质岩石的广泛发育,同时伴随幔源钾质超钾质岩浆作用。冈底斯弧岩浆作用与岩浆成分的系统时空变化很好地记录了从新特提斯洋俯冲到印度亚洲大陆碰撞的完整构造演化过程。  相似文献   

19.
玛里雅蛇绿岩位于新疆准噶尔西缘达拉布特断裂东侧的弧前增生楔内,形成于石炭纪,出露岩石类型齐全,其中硅质岩与火山岩相间出露,多表现为非构造接触。地球化学特征表明,它们大致可以分为四个系列:(1)A系列为岛弧英安岩,Th强烈富集,可能有洋壳沉积物参与,高场强元素Nb亏损,与洋壳的俯冲有关;(2)M系列与典型洋中脊玄武岩的稀土元素配分模式一致,不过Ba强烈富集,可能受到俯冲流体的影响;(3)E系列位于地幔序列N-MORB和E-MORB之间,表明它可能是地幔岩浆的混合产物,未受到地幔岩浆源区之外物质的影响;(4)O系列与典型的洋岛玄武岩基本一致,只是Ta、La和Th含量略偏低,但都处于地幔序列范围内,可能与其他岩浆源有轻微的混合。这种岩浆特征与智利洋中脊俯冲环境下所产生的岩浆特征一致;由于西准噶尔晚古生代仍然发生俯冲消减,因此推测玛里雅蛇绿岩可能形成于洋中脊俯冲环境。  相似文献   

20.
The Banda arc of eastern Indonesia manifests the collision of a continent and an intra-oceanic island arc. The presently active arc is located on what appears to be oceanic crust whereas the associated subduction trench is underlain by continental crust.Recent lavas from the Banda arc are predominantly andesitic and range from tholeiitic in the north through calc-alkaline to high-K calc-alkaline varieties in the southern islands. Defining this regular geochemical variation are significant increases in the abundances of K (2,600–21,000 ppm), Rb (10–90 ppm), Cs (0.5–7.0 ppm), and Ba (100–1,000 ppm) from tholeiitic to high-K calc-alkaline lavas. 87Sr/86Sr ratios in the tholeiites are relatively low, from 0.7045 to 0.7047. In the calc-alkaline lavas, 87Sr/86Sr ratios range from 0.7052 to 0.7095, and in the high-K calc-alkaline lavas from 0.7065 to 0.7080. There is no correlation between 87Sr/86Sr and major and trace element abundances, even among lavas from the same volcano. Late Cenozoic cordierite — bearing lavas from Ambon, north of the presently active arc, are highly enriched in K, Rb and Cs, which together with 87Sr/86Sr ratios of approximately 0.715 is consistent with their derivation from partial melting of pelitic material in the locally — thick crust.The high 87Sr/86Sr ratios in the Recent calc-alkaline lavas are interpreted to result from mixing of a sialic component with a mantle derived component. The most likely cause is subduction and subsequent melting of either sea-floor sediments or continental crust. However, it is probably unrealistic to model this type of deep contamination by simple two-component mixing. Such contamination implies that the volcanic rocks from the Banda arc are at least partly a manifestation of melting at or near the Benioff seismic zone. Temperatures of at least 750–800 ° C at the top of the subducted lithospheric slab at depths of approximately 150 km are also implied; temperatures very close to the solidus of hydrous basalt (eclogite) at such pressure. It is concluded that partial melting of the crustal component of the subducted lithospheric slab may play a significant role in island arc petrogenesis.This paper is the result of a cooperative project with the Geological Survey of Indonesia, Ministry of Mines and Energy  相似文献   

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