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对南秦岭北大巴山地区广泛分布的一套基性岩墙群中的辉绿岩进行采样,并进行了锆石U-Pb年代学、全岩地球化学分析。结果显示,岩石形成年龄为435~433 Ma,为早志留世晚期岩浆活动产物。这些辉绿岩具低硅、高碱、高钛的碱性岩特征。岩石微量及稀土元素具板内玄武岩特征,轻稀土元素相对富集,轻重稀土元素分异明显,富集不相容元素Ba、Nb、Ta,而K、Y、Yb相对亏损;K及Rb的负异常表明岩石源区残留角闪石或金云母,部分熔融模拟结果显示岩石起源于尖晶石角闪石岩高程度部分熔融。综合地球化学特征及前人研究结果,认为北大巴山地区在早古生代处于大规模伸展裂陷背景下,岩石圈的拉张诱发了低熔点的交代岩石圈地幔熔融,进而形成了这条碱性岩浆带。 相似文献
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山西繁峙新生代玄武岩地幔源区及成因探讨:元素及Sr-Nd-Pb-Hf同位素地球化学证据 总被引：1，自引：1，他引：0
山西省繁峙玄武岩位于华北克拉通重力梯度带附近,是华北克拉通中部新生代玄武岩重要组成部分。前人全岩K-Ar测年结果为26.3~24.3Ma。对繁峙地区苏孟庄和应县两地玄武岩的地球化学特征研究表明,其微量元素和同位素均具有类OIB特征,即富集不相容元素,轻、重稀土元素分馏明显((La/Yb)N=8.42~21.60),不存在Sr、Eu负异常,Sr同位素比值(87Sr/86Sr=0.703848~0.704870)较低,Nd(143Nd/144Nd=0.512617~0.513057)和Hf(176Hf/177Hf=0.282873~0.283001)同位素比值较高,Pb同位素比值分别为206Pb/204Pb=17.2~17.9,207Pb/204Pb=15.3~15.4和208Pb/204Pb=37.5~37.9。结合岩相学特征和主量元素特征,我们推断繁峙新生代玄武岩是软流圈低程度部分熔融结果,并存在岩石圈物质的加入,岩浆上升时在岩石圈地幔条件下的岩浆房内经历了以橄榄石、单斜辉石为主的分离结晶作用,岩浆因快速上升而地壳混染程度甚低。苏孟庄碱性玄武岩具有较深的熔融深度和较低的熔融程度,而应县亚碱性玄武岩熔融深度较浅,熔融程度较高。结合重力梯度带附近其他地区的新生代玄武岩的研究,我们推测重力梯度带附近新生代的火山活动可能起源于西部软流圈地幔向东流动越过重力梯度带时的减压部分熔融,该地区广泛分布的断裂带为岩浆上涌提供了通道。本文为中国东部新生代玄武质火山活动的岩石成因学研究提供了新的视角。 相似文献
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内蒙古阿巴嘎旗地区新生代玄武岩基本特征及成因 总被引：9，自引：0，他引：9
内蒙古阿巴嘎旗及其以北地区新生代玄武岩是更新世中心式火山活动产生的大陆溢流玄武岩,该区玄武岩以高碱、富钛、贫铝为特征,属于钠质碱性玄武岩系列.源区是软流圈上地幔,玄武岩是部分熔融和分离结晶两种作用的结果.地幔橄榄岩部分熔融产生玄武质岩浆,部分原始地幔岩浆未经变异沿构造通道直接喷出地表形成碧玄岩、碱性橄榄玄武岩;部分原始地幔岩浆在上升过程中因停顿,原始地幔岩浆发生橄榄石分离结晶作用,部分橄榄石从岩浆中析出,最终岩浆喷出地表形成橄榄拉斑玄武岩.研究该区新生代玄武岩基本特征,探讨岩浆起源和岩石产生的构造环境对认识该区岩石圈地幔和软流圈性质具有重要意义. 相似文献
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中国东部新生代玄武岩的地球化学：Ⅰ.主元素和微量元素组成：岩石成因… 总被引：17，自引：8，他引：17
所研究的玄武岩包括拉斑玄武岩、碱性玄武岩、苦橄粗玄岩和钾质玄武岩。主元素和微量元素的组成变化表明，中国东部玄武岩既是不同深度地幔部分熔融的产物，又经历了岩浆结晶分层作用。强不相容元素比值的变化特征显然与岩石圈地幔交代作用有关。软流圈地幔的上涌并导致上覆不均一的岩石圈地幔的部分熔融是形成中国东部新生代玄武岩的主要机制。 相似文献
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大麻坪地区二辉橄榄岩部分熔融实验研究 总被引：1，自引：0，他引：1
本文以采自大麻坪地区汉诺坝玄武岩中的二辉橄榄岩包体为初始实验物料,在压力1.0～3.0 GPa、温度1350～1550℃条件下进行了部分熔融实验,对实验产物进行了岩相学研究和电子探针成分分析。二辉橄榄岩在1350℃开始熔融,在实验的温度压力范围内,熔融程度为10%～30%。随熔融程度的升高,部分熔融后残余岩石倾向于向富镁、低铁、低钙、低硅的趋势演化,而部分熔融产生的熔体则倾向于富镁、富铁、低铝、低硅的趋势演化。在岩石化学图解上本次实验中二辉橄榄岩部分熔融产生的熔体化学组成与汉诺坝地区拉斑玄武岩的组成相近。随熔融程度升高,熔体具有从苦橄质→玄武质演化的趋势。 相似文献
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柳泉地区是苏北地区煌斑岩的集中分布区,与之相伴的还有金伯利岩和橄榄玄武玢岩。通过研究该区煌斑岩的岩石学及岩石地球化学特征,进一步探讨其岩石成因及构造环境。研究表明:柳泉地区煌斑岩为同源岩浆演化的产物,整体属于钾质碱性煌斑岩,具有低硅、富铁镁钛的特点,大离子亲石元素和轻稀土元素相对富集,高场强元素和重稀土元素相对亏损。柳泉地区煌斑岩形成于中—新生代太平洋板块俯冲、岩石圈减薄的构造背景下,起源于深75～100 km、受俯冲沉积物改造形成的富集岩石圈地幔源区,经含角闪石石榴石二辉橄榄岩部分熔融,并沿构造薄弱带上侵至地壳浅部形成的。 相似文献
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《矿物学报》2019,(6)
通过对滇东北码口地区峨眉山玄武岩的矿物学和岩石地球化学特征研究,对其成因以及母岩浆起源做出了合理的解释。该玄武岩SiO2的含量为48.88%～52.80%,为基性熔岩。在TAS图解中大部分样品点落入碱性玄武岩中,小部分为亚碱性玄武岩。其镁指数I(Mg~#)平均值为0.45%,比原始岩浆的0.67%～0.70%低,表明原始岩浆经历了一定分异;相对富集轻稀土而亏损重稀土(LREE/HREE=6.69～8.07),轻重稀土发生了轻微分异作用,可见轻微的负铕异常(δEu=0.72～0.93);在蛛网图中可见K、P和Sr等元素不同程度上的亏损,Ti/Y比值(Ti/Y含量为490.06～627.77)该玄武岩属于高钛玄武岩。研究表明,码口地区玄武岩为下地幔石榴石地幔橄榄岩部分熔融产物,形成于板块拉张环境,与地幔活动有关,在成岩过程中遭受地壳物质混染,并且发生了橄榄石、斜长石和单斜辉石的分离结晶作用。 相似文献
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本文选取冈底斯带东段加查县东北部丝波绒曲复式岩体为对象,对其进行了岩相学、地质年代学、岩石地球化学以及Sr-Nd-Hf同位素组成的综合研究,据此探讨了该复式岩体的成因及其对构造演化的启示。研究结果表明,该复式岩体由早侏罗世辉长岩-花岗岩杂岩(188～185Ma)和始新世花岗质岩石(～47Ma)构成,两期花岗质岩石中普遍发育塑变形态的镁铁质包体。早侏罗世杂岩由角闪辉长岩和英云闪长岩组成,角闪辉长岩中的主要铁镁矿物为角闪石,它们为一套钙碱性弧岩浆岩组合,具有亏损的Sr-Nd-Hf同位素组成。始新世花岗质岩石主要为二长花岗岩-花岗闪长岩,它们较早侏罗世英云闪长岩更为富碱,属钙碱性-高钾钙碱性I型花岗岩,其同位素组成也较早侏罗世英云闪长岩富集。综合分析表明,该区早侏罗世复合辉长岩-花岗岩的形成受控于新特提斯洋板片北向俯冲的构造背景,角闪辉长岩起源于受俯冲板片脱水交代的上覆地幔楔的部分熔融,共生的英云闪长岩则为同期幔源岩浆底侵诱发初生地壳部分熔融产生的长英质岩浆与幔源岩浆不同程度混合的产物。始新世花岗岩的形成受控于新特提斯洋板片断离的构造背景,是由具"弧"型地球化学特征的初生地壳再造的产物,并有少量印度陆壳富集组分参与成岩。 相似文献
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埃达克质岩的构造背景与岩石组合 总被引：6，自引：1，他引：5
本文介绍了埃达克质岩形成的构造背景与岩石组合。埃达克质岩可以形成于不同的构造背景并与不同类型的岩石同时出现：1）火山弧环境中常出现埃达克质岩一高镁安山岩-富Nb玄武质岩组合,它的形成可能与板片熔融以及熔体一地幔橄榄岩的相互作用有关;2）大陆活动碰撞造山带环境（如羌塘）中埃达克质岩常与同期钾质或橄榄玄粗质岩共生,这可能与俯冲陆壳熔融和俯冲陆壳熔体交代的地幔橄榄岩熔融有关;3）造山带伸展垮塌环境（如大别山）中埃达克质岩会伴随有镁铁质一超镁铁质岩浆出露,增厚下地壳产生埃达克质岩浆后的榴辉岩质残留体拆沉进入地幔,与地幔橄榄岩的混合可能形成后期镁铁质一超镁铁质岩浆的源区;4）大陆板内伸展环境中埃达克质岩常与同期橄榄玄粗质的岩石共生,增厚、拆沉下地壳,以及富集地幔的熔融或岩浆混合在岩石的成因中发挥了重要作用。 相似文献
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Volcanism and orogenic belts — The origin of andesites 总被引：2，自引：0，他引：2
A.L. Boettcher 《Tectonophysics》1973,17(3):223-240
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强烈亏损重稀土元素的中酸性火成岩(或埃达克质岩)与Cu、Au成矿作用 总被引：33，自引：4，他引：33
文中概述了强烈亏损重稀土元素的中酸性火成岩(或埃达克质岩)的研究历史、现状和意义,列出了扬子地块东部、青藏高原以及新疆北部与铜金成矿有关的同类岩石的一些特征,重点分析了当前强烈亏损重稀土元素的中酸性火成岩(或埃达克质岩)的研究中所存在的问题,并提出了一些初步的设想。强烈亏损重稀土元素的中酸性火成岩(或埃达克质岩)不仅具有重要的地球动力学意义(可能与俯冲、拆沉、底侵、板片窗或地幔交代等深部过程有关),而且具有极其重要的Cu、Au成矿意义。俯冲洋壳熔融形成的埃达克岩及其成矿作用已有相当深入的研究,但是来自大陆内部的强烈亏损重稀土元素的中酸性火成岩的成因、岩石组合及其成矿作用是否类似于俯冲洋壳熔融形成的埃达克岩,还需要深入的研究。一些强烈亏损重稀土元素的中酸性火成岩(或埃达克质岩)的所表现出的高钾特征很可能与高压(>1 GPa)条件下的熔融或源岩的高钾有关。文中提出了一个有别于俯冲洋壳熔融+埃达克岩+Cu、Au成矿的新工作模型——拆沉洋壳或下地壳熔融+强烈亏损重稀土元素的中酸性火成岩(或埃达克质岩)+Cu、Au成矿。拆沉洋壳或下地壳熔融形成熔体的Fe_2O_3对地幔的交代(氧化)作用可能是Cu、Au从地幔迁出并最终成矿的一个重要原因,但是增厚下地壳环境中流体的作用也不? 相似文献
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Simple mixing as the major control of the evolution of volcanic suites in the Ecuadorian Andes 总被引：8，自引：0，他引：8
Pierre Schiano M. Monzier J.-P. Eissen H. Martin K. T. Koga 《Contributions to Mineralogy and Petrology》2010,160(2):297-312
Examination of an extensive major and trace element database for about 700 whole rocks from the Ecuadorian Andes reveals series
of local trends typified by three volcanoes: Iliniza and Pichincha from the Western Cordillera and Tungurahua from the Eastern
Cordillera. These local trends are included in a more scattered global trend that reflects typical across-arc chemical variations.
The scatter of the global trend is attributed to greater crustal contributions or decreasing melt fractions. Trace element
modelling shows that the local trends are consistent with mixing, and not with any fractional crystallization or progressive
melting dominated processes. These local trends are extendable to include samples from other Ecuadorian volcanoes, suggesting
that mixing processes are dominant throughout the region. Mixing model using trace and major element analyses identifies two
end-members: low-silica, basaltic and high-silica, dacitic magmas. It also shows that mixing occurred between magmas after
their segregation, rather than earlier mixing between the solid sources prior to melting. As a consequence, there must exist
efficient magma-mixing processes that can overcome the obstacles to mixing magmas with contrasting physical properties, and
can produce series of hybrid liquids over regional-scale. Model calculations show that estimated silicic end-members are primary
magmas and are not co-magmatic derivatives of the corresponding mafic end-members. Lavas of Ecuadorian volcanoes are likely
originated from magmas of contrasting origins, such as basaltic magmas generated by fluxed melting of peridotites in the mantle
wedge and dacitic, adakite-type magmas originating from the slab or the mafic lower crust. 相似文献
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Early Paleozoic magmatism of the Tannuola terrane located in the northern Central Asian Orogenic Belt is important to understanding the transition from subduction to post-collision settings. In this study, we report in situ zircon U-Pb ages, whole rock geochemistry, and Sr-Nd isotopic data from the mafic and granitic rocks of the eastern Tannuola terrane to better characterize their petrogenesis and to investigate changing of the tectonic setting and geodynamic evolution. Zircon U-Pb ages reveal three magmatic episodes for about 60 Ma from ∼510 to ∼450 Ma, that can be divided into the late Cambrian (∼510–490 Ma), the Early Ordovician (∼480–470 Ma) and the Middle-Late Ordovician (∼460–450 Ma) stages. The late Cambrian episode emplaced the mafic, intermediate and granitic rocks with volcanic arc affinity. The late Cambrian mafic rocks of the Tannuola terrane may originate from melting of mantle source that contain asthenosphere and subarc enriched mantle metasomatized by melts derived from sinking oceanic slab. Geochemical and isotopic compositions indicate the late Cambrian intermediate-granitic rocks are most consistent with an origin from a mixed source including fractionation of mantle-derived magmas and crustal-derived components. The Early Ordovician episode reveal bimodal intrusions containing mafic rocks and adakite-like granitic rocks implying the transition from a thinner to a thicker lower crust. The Early Ordovician mafic rocks are formed as a result of high degree melting of mantle source including dominantly depleted mantle and subordinate mantle metasomatized by fluid components while coeval granitic rocks were derived from partial melting of the high Sr/Y mafic rocks. The latest Middle-Late Ordovician magmatic episode emplaced high-K calc-alkaline ferroan granitic rocks that were formed through the partial melting the juvenile Neoproterozoic sources.These three episodes of magmatism identified in the eastern Tannuola terrane are interpreted as reflecting the transition from subduction to post-collision settings during the early Paleozoic. The emplacement of voluminous magmatic rocks was induced by several stages of asthenospheric upwelling in various geodynamic settings. The late Cambrian episode of magmatism was triggered by the slab break-off while subsequent Early Ordovician episode followed the switch to a collisional setting with thickening of the lower crust and the intrusion of mantle-induced bimodal magmatism. During the post-collisional stage, the large-scale lithospheric delamination provides the magma generation for the Middle-Late Ordovician granitic rocks. 相似文献
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冀东地区位于华北克拉通北缘,学术界对该地区新太古代岩浆作用的成因模式及构造背景一直存在争议,因此对冀东青龙-双山子地区的新太古代变质表壳岩及侵入岩进行了系统的同位素年代学及岩石地球化学研究.锆石LA-MC-ICP-MS U-Pb年代学结果显示变安山岩的形成时代为2 576 Ma,辉长闪长岩-英云闪长岩-石英闪长岩的侵入时代为2 484~2 535 Ma.岩石地球化学特征显示,较早期的变安山岩部分属高镁安山岩类,源自俯冲板片脱水流体交代地幔楔的部分熔融;而稍晚的侵入岩类为具有埃达克质岩石特征的镁闪长岩类,源区具有熔体交代地幔楔部分熔融的特征;整体构成高镁安山岩-埃达克质镁闪长岩组合.结合区域上的同位素年代学及地球化学报道,冀东青龙-双山子地区新太古代应处于活动大陆边缘构造背景. 相似文献
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藏南冈底斯带中段始新世岩浆作用的厘定及其大地构造意义 总被引：7，自引：0，他引：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
19.
Ioan Seghedi Hilary Downes Szabolcs Harangi Paul R.D. Mason Zoltn Pcskay 《Tectonophysics》2005,410(1-4):485-499
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
20.
The conditions of magma formation were reconstructed on the basis of characteristic features of the evolution of the Kurile-Kamchatka island-arc system, structural and chemical zoning patterns of volcanic complexes, and available published data on peridotite and basalt melting and stability of hydrous minerals. It was shown that the volcanic arc of the Sredinnyi Range of Kamchatka occurs now at the final stage of subduction, whereas subduction beneath the volcanic arc of eastern Kamchatka began at the end of the Miocene, after its jump into the present-day position. The volcanism of Southern Kamchatka and the Kuriles has occurred under steady-state subduction conditions since the Miocene and is represented by typical island-arc magmas. The latter are generated in a mantle wedge, where the melting of water-saturated peridotite occurs in a high-temperature zone under the influence of fluid. The formation of the frontal and rear volcanic zones was related to the existence of two levels of water release from various hydrous minerals. During the initial and final stages of subduction, as well as in the zone of Kamchatka—Aleutian junction, partial melting is possible in the upper part of the subducted slab in contact with a hotter mantle material compared with the mantle in a steady-state regime. This is responsible for the coexistence of predominant typical island-arc rocks, rocks with intraplate geochemical signatures, and highly magnesian rocks, including adakites. 相似文献