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1.
南秦岭耀岭河群裂谷型火山岩锆石U—Pb年代学 总被引：24，自引：6，他引：24
南秦岭耀岭河群以变质基性火山岩为主,夹少量酸性火山岩和碎屑岩。基性火山岩和凝灰岩的TIMS法锆石U-Pb同位素年龄分别为808Ma±6Ma和746Ma±2Ma,表明耀岭河群主体形成于南华纪,西峡-淅川一带所谓的“武当岩群”明显年轻于中元古代武当岩群,应该属于耀岭河群。耀岭河群大陆裂谷型火山岩是全球Rodinia超大陆在新元古代晚期南华纪裂解过程中的产物,反映秦岭造山带和Rodinia超大陆的形成演化密切相关。 相似文献
2.
南秦岭东段耀岭河群、陨西群、武当山群火山岩和基性岩墙群岩石成因 总被引：13，自引：3，他引：10
南秦岭东段新元古代中-晚期(676～833 Ma)耀岭河群、陨西群、武当群火山岩和基性岩墙群产生于大陆板内裂谷环境.根据岩石地球化学数据,南秦岭东段新元古代中-晚期裂谷基性熔岩和基性岩墙总体上属于低Ti/Y(<500)岩浆类型.元素和同位素数据表明,南秦岭东段新元古代中-晚期裂谷基性熔岩和基性岩墙的化学变化不是由一个共同的母岩浆结晶分异作用所产生,它们极有可能是源于地幔柱源(εNd(t)≈ 5,Mg#≈0.7,La/Nb≈0.7).大陆地壳或大陆岩石圈混染作用对于南秦岭东段新元古代中-晚期裂谷基性熔岩和基性岩墙的形成有重要贡献.我们的研究揭示,南秦岭东段新元古代中-晚期火山岩和基性岩墙存在空间上的地球化学变化.它们总体上是产生于幔源石榴子石稳定区.而西北部镇安地区耀岭河群基性熔岩的母岩浆则是形成于幔源尖晶石-石榴子石过渡带.碱性熔岩是产生于部分熔融程度较低(<10%)的条件下,拉斑玄武质熔岩是产生于部分熔融程度较高(10%～30%)的条件下.武当山地区的武当山群和耀岭河群基性熔岩的母岩浆经受了浅层位辉长岩质(cpx plag ± ol)分离作用,而其他地区基性熔岩和基性岩墙的化学演化则是受控于单斜辉石(cpx)±橄榄石(ol)分离作用. 相似文献
3.
南秦岭武当山群变质酸性火山岩锆石U-Pb年代学 总被引：4，自引：0，他引：4
对武当山群3个变质酸性火山岩样品的锆石U-Pb定年结果表明,武当山群变质酸性火山岩形成年龄为675.2±3.1 Ma,说明武当山群存在新元古代南华纪的地层组成.武当山群变质变形复杂,具多期岩浆活动,可能由不同时代火山岩和少量沉积岩组成,部分变质火山岩具有与耀岭河群火山岩和侵入到武当山群中的基性侵入岩相似的形成年龄,指示了武当山群变质酸性火山岩可能与基性侵入岩群和耀岭河群火山岩存在成因联系.基于现有同位素定年数据,武当山群火山岩数据具有年龄跨度大(太古宙至中生代)的显著特征,但总的趋势是新近取得的年龄数据多数比早期获得的数据要年轻. 相似文献
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5.
扬子克拉通北缘碎屑沉积岩地球化学特征及意义 总被引：3，自引：0，他引：3
通过系统研究扬子克拉通北缘西乡-碑坝小区后太古代变质沉积岩的主量元素、微量元素和Nd同位素组成,得出如下结论:(1)扬子北缘中、晚元古代三花石组杂砂岩的εNd(t),分别为 2.72和 0.69,TDM分别为1.40Ga和1.57Ga,与扬子北缘同时期西乡群火山岩具有相近的Nd同位素组成,扬子克拉通北缘新元古代存在的岛弧物质控制着该区中、晚元古代沉积物源的地球化学组成,后河群碎屑物质对火地垭群沉积岩有一定的影响;(2)扬子克拉通北缘古生代沉积物源区以再旋回沉积物源为主,并随时间变化对再旋回沉积物源的接受逐渐加强,沉积源区的长英质物质逐渐增多,分异程度越来越高;西乡-碑坝小区从寒武纪-志留纪沉积物源很可能是扬子克拉通基底崆岭群和基性火山岩等风化剥蚀后混合的产物,本区从晚泥盆世开始,其沉积物源区与秦岭群片麻岩的风化剥蚀有明显的关系;(3)扬子北缘西乡-碑坝小区从晚二叠世到早侏罗世碎屑沉积岩的εNd(t)比早古生代碎屑沉积岩的明显偏大,结合微量元素数据分析,这与晚二叠世峨眉山玄武岩的多次喷发(火山灰)和风化剥蚀作用有关. 相似文献
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碧口群火山岩性质及形成环境 总被引：1，自引：0，他引：1
中元古代—新元古代碧口群火山岩系分布在扬子地块北缘、秦岭造山带南侧。碧口群火山岩系具大陆裂谷火山岩特点,形成于大陆裂谷作用构造环境。火山岩系特征为：① 具双峰式火山岩组合,火山岩系由基性火山岩（细碧岩及细碧质凝灰岩）及酸性火山岩（石英角斑岩及石英角斑质凝灰岩）组成。② 基性火山岩包括两个岩浆系列的岩石,即碱性玄武岩浆系列及拉斑玄武岩浆系列。③ 火山岩富集LREE及LIL。微量元素及同位素（SmNd,RbSr）研究表明,基性火山岩形成于相似于洋岛玄武岩源的地幔柱源,酸性火山岩为地壳重熔的产物。扬子地块北缘分布有碧口群、西乡群等中元古代—新元古代大陆火山岩系,表明在这一时期大陆裂谷拉张火山作用发育,成为秦岭地壳的主要增生成壳期。 相似文献
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扬子北缘晋宁期望江山基性岩体的地球化学特征及其构造背景 总被引：11，自引：2，他引：11
钐 钕同位素定年和系统的元素 同位素地球化学研究表明 ,位于扬子克拉通北缘的望江山基性岩体形成于约 785± 88Ma的晋宁期 ,并具有陆内裂谷环境岩浆作用的地球化学属性 ,与时代为 0 95～ 0 .90Ga、具岛弧型火山岩特征的西乡群明显不同 ,标志该地区于新元古代经历了由洋壳消减的大陆边缘向陆内裂谷转变的构造演化。 相似文献
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<正>武当地块南接扬子板块北缘,西南与北大巴山加里东褶皱带相邻,是卷入南秦岭构造带中的前震旦纪浅变质过渡基底地块。该区域地层主要为新元古界武当山群和耀岭河群、震旦系陡山沱组和灯影组以及古生代地层。区内中酸性岩浆岩相对贫乏,但广泛发育基性岩脉。目前对武当地块岩浆岩的年代学研究报道的几乎均为新元古代或古生代年龄,这与东、西秦岭及大别-苏鲁造山带记录的大量中生代年龄数据截然不同。例如,周鼎武等[1-2]获得武当地块中基性岩墙年龄为782±164 Ma(Sm-Nd等时线)和694±21 Ma(角闪石40Ar/39Ar);胡建民等[3-4]则认为这些所谓基性岩墙实 相似文献
9.
扬子克拉通北缘元古宙基底同位素地质年代学和地壳增生历史：Ⅱ．火地垭群 总被引：1，自引：0，他引：1
扬子克拉通地壳的生成始于太古宙，但依据目前的研究成果，其主体形成于元古宙，对位于扬子克拉通北缘，分布在碑坝地区重要的基底岩系之一的火地垭群铁船山组火山岩进行了Ｓｍ－Ｎｄ和Ｒｂ－Ｓｒ同位素地球化学研究．同位素年代学数据表明，铁船山组岩系形成于约（１６６８５）Ｍａ的中元古代，并源于高亏损的地幔岩浆库（ｄ（ｔ）７．５３．１０），且其亏损地幔模式年龄ＴＤＭ（（１．６８±０．１０）Ｇａ）与Ｓｍ－Ｎｄ等时年龄是一致的．Ｒｂ－Ｓｒ同位素年代学揭示出在新元古代早期（约（８６０±１２）Ｍａ的晋宁期）铁船山组岩系受到了构造热事件的改造．该事件与区内大规模的基性－超基性和碱性、中－酸性岩浆活动的同时出现在时间上是一致的．这些晋宁期岩浆作用有着以下共同特征：（１）岩浆源于亏损程度大为降低的岩浆库；（２）模式年龄ＴＤＭ与铁船山组火山岩的形成时代相近．在本区的西乡地区，同为中元古代形成的西乡群底部的白勉峡组火山岩与其周围的晋宁期基性－超基性和碱性、中－酸性岩浆岩在年代学特征、岩浆库性质和亏损地幔模式年龄等多方面与碑坝地区铁船山组火山岩及其周围晋宁期岩浆岩的特征是类似的．这些同位素地球化学特征所揭示的区内地壳增生和晋宁期构造历史进一 相似文献
10.
祁连山带及邻区前寒武纪深变质基底的时代和组成 总被引：3，自引：0，他引：3
根据变泥砂质岩石和壳源花岗质岩石的地质、年代学、地球化学和Nd同位素组成研究，主要结论为：①祁连造山带深变质基底主要由变泥砂质岩石和花岗岩组成，其主体形成于0．8－0．6Ga（晋宁期）；②大多数变砂质岩石和花岗岩具有较强的负铕和负钡异常，tDM和εNd(1.0Ga）分别为1.87-2.26Ga和8.54-4.06，显示出较高的成熟度；③花岗质岩石为典型的陆－陆碰撞的产物，可能与全球新元古代Rodinia超大陆形成事件有关。本文还对祁连造山带及邻区深变质基底的构造归属进行了研究，认为祁连－柴北缘地体和阿拉善－敦煌地体在晋宁期以前相互分离，分属华北克拉通和扬子地台不同的板块体系。祁连造山带和秦岭造山带至少在晋宁期就有相同或相似的地质深化历史。 相似文献
11.
俯冲到地幔深度的地壳物质不可避免地在板片-地幔界面与地幔楔发生相互作用，由此形成的超镁铁质交代岩就是造山带镁铁质火成岩的地幔源区.因此，造山带镁铁质火成岩为研究俯冲地壳物质再循环和壳-幔相互作用提供了重要研究对象.为了揭示俯冲陆壳物质再循环的机制和过程，对大别造山带碰撞后安山质火山岩开展了元素和同位素地球化学研究.这些安山质火山岩的SIMS锆石U-Pb年龄为124±3~130±2 Ma，表明其形成于早白垩世.此外，残留锆石的U-Pb年龄为中新元古代和三叠纪，分别对应于大别-苏鲁造山带超高压变火成岩的原岩年龄和变质年龄.它们具有岛弧型微量元素特征、富集的Sr-Nd-Hf同位素组成，以及变化的且大多不同于正常地幔的锆石δ18O值.这些元素和同位素特征指示，这些安山质火山岩是交代富集的造山带岩石圈地幔部分熔融的产物.在三叠纪华南陆块俯冲于华北陆块之下的过程中，俯冲华南陆壳来源的长英质熔体交代了上覆华北岩石圈地幔楔橄榄岩，大陆俯冲隧道内的熔体-橄榄岩反应产生了富沃、富集的镁铁质地幔交代岩.这种地幔交代岩在早白垩世发生部分熔融，就形成了所观察到的安山质火山岩.因此，碰撞造山带镁铁质岩浆岩的地幔源区是通过大陆俯冲隧道内板片-地幔相互作用形成的，而加入地幔楔中长英质熔体的比例决定了这些镁铁质岩浆岩的岩石化学和地球化学成分. 相似文献
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The Orós belt is a metamorphosed and deformed supracrustal sequence whose deposition started at ca. 1.8 Ga. The volcanic rocks form an essentially bimodal association with a predominance of felsic volcanics. Mafic volcanics show geochemical and Nd isotopic differences which point to separate origins for each type. The mafic rocks are either chemically similar to EMORBs or are transalkaline types, enriched in LILE and LREE and relatively depleted in HFSE but with different isotopic signatures. One mafic type is associated with dominant andesites in a suite which could have evolved by an AFC process involving a Transamazonian-age source rock which later produced some of the overlying felsic volcanics. The rhyolites have variable geochemical signatures, all typical of anatectic products derived from continental crustal rocks. Sedimentary rocks are dominated by pelitic types of different provenances, accompanied by minor arenites and lesser carbonate rocks and calc-silicates. The depositional environment of the supracrustal sequence was continental, and a number of lines of evidence suggest that a rift environment probably developed during relaxation following the Transamazonian orogeny. The most abundant igneous rocks are felsic plutonics, emplaced nearly 100 Ma after the volcanic activity, but whose geochemical signature is similar to that of most of the rhyolites. These are cut by more alkaline anorogenic intrusives. The volcano-sedimentary sequence was intruded at ca. 0.9 Ga by a mafic-ultramafic sill. All deformation and metamorphism occurred during the Brasiliano orogeny, which was accompanied by the intrusion of syn-tectonic granites.The Orós belt, therefore, represents an intracontinental ensialic late Paleoproterozoic volcano-sedimentary basin initially related to strain relaxation of the crust. With subsequent collapse and development of faults, the anorogenic alkaline granites intruded at ca. 1.7 Ga. Based on the data available on this province, the Orós belt forms a part of a series of supracrustal belts of different ages, which were consolidated and welded in the Brasiliano orogeny.Within the Borborema Province, supracrustal sequences with ages of ≈ 2.0-1.9 Ga, ≈ 1.8-1.7 Ga (Orós), ≈ 1.1-1.0 Ga, and ≈ 0.6 Ga are presently known. All were aglutinated or amalgamated to neighboring blocks during the Brasiliano orogenic cycle. 相似文献
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华北克拉通中元古代裂解事件:以渣尔泰-白云鄂博-化德裂谷带岩浆与沉积作用研究为例 总被引：9，自引：7，他引：2
华北克拉通存在三个主要的中元古代裂谷带,从南到北分别为熊耳裂谷带、燕辽裂谷带以及渣尔泰-白云鄂博-化德裂谷带。其中熊耳群中火山岩的峰期年龄为1780~1750Ma,其上还有形成于被动大陆边缘的五佛山群、汝阳群以及官道口群。中北部的燕辽裂谷带包括长城系、蓟县系和青白口系,其中长城系团山子组和大红峪组火山岩的年龄分别为~1640Ma和1626~1622Ma,蓟县系高于庄组、雾迷山组和铁岭组凝灰岩的年龄分别为1560Ma、1485Ma和1437Ma,而下马岭组凝灰岩年龄为1366~1380Ma。北缘渣尔泰-白云鄂博-化德裂谷带中渣尔泰群书记沟组玄武岩年龄为1743Ma,阿古鲁沟组酸性火山岩年龄为~810Ma,白云鄂博群尖山组中基性火山岩年龄为1728Ma,化德群比鲁特组火山碎屑岩年龄为1515Ma。中元古代岩浆事件除了裂谷带中的火山作用外,还包括三期基性岩墙群(~1780Ma太行-吕梁岩墙群、~1730Ma密云岩墙群和~1620Ma泰山岩墙群)以及1.76Ga到1.65Ga非造山岩浆组合(斜长岩-环斑花岗岩体-A型花岗岩)。中元古代中期,华北克拉通北缘发育了基性岩席(墙)、A型花岗岩以及碳酸岩脉,双峰式岩浆作用说明华北北缘在中元古代中期经历了裂谷作用,与哥伦比亚超大陆的最终裂解有关,并且与白云鄂博巨型REE-Nb-Fe矿床的形成具有成因上的联系。华北克拉通北部两个裂谷带中的地层具有可以对比的层序以及时代,而中元古代中期辉绿岩墙、A型花岗岩以及碳酸岩脉可以与其它克拉通同时期的非造山岩浆作用对比,证明华北克拉通经历了哥伦比亚超大陆的最终裂解。古地磁数据已经证明在哥伦比亚超大陆时期Siberia、Laurentia、Baltica、Amazion以及华北克拉通是连接在一起的,而北缘中元古代中期大陆裂谷相关岩浆岩的发现也说明它是与另一个古大陆相连的。华北克拉通南缘熊耳火山岩的构造背景到底是大陆裂谷还是大陆边缘弧则关系着其是与另一个克拉通相连还是面向大海,这需要我们进一步深入研究。 相似文献
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系统收集并总结了武当地块与扬子陆核区(崆岭地区)已发表的新元古代沉积岩中碎屑锆石的U-Pb年代学数据,对二者的相互关系进行分析,并讨论了扬子克拉通北缘新元古代时期的构造演化过程及特征。对前人发表的年代学数据进行的统计和对比结果表明,武当地块沉积岩中碎屑锆石年龄谱记录了~710Ma和~2.5Ga的年龄峰值,同时缺乏3.0Ga年龄的锆石,表明其沉积物质来源可能并非扬子陆核区,其在新元古代之前可能作为一个独立的微陆块与扬子陆核区(崆岭地区)分离开来,二者于新元古代中期发生碰撞拼合而成为一个整体。 相似文献
15.
Ling Wenli Gao Shan Cheng Jianping Zhang Benren Faculty of Earth Sciences China University of Geosciences Wuhan Zheng Haifei Department of Geology Peking University Beijing 《中国地质大学学报(英文版)》1998,9(2)
ＴｈｅＹａｎｇｔｚｅａｎｄＮｏｒｔｈＣｈｉｎａｃｒａｔｏｎｓ（ｓｍＹＣａｎｄＮＣＣ）ａｒｅｔｗｏｏｆｔｈｅｍａｉｎｃｏｎｓｔｉｔｕｅｎｔｐａｒｔｓｏｆｔｈｅｃｏｎｔｉｎｅｎｔｉｎＣｈｉ－ｎａ,ａｎｄｃｏｎｎｅｃｔｗｉｔｈｔｈｅｆａｍｏｕｓＱｉｎｌｉｎ... 相似文献
16.
We trace source variations of active margin granitoids which crystallised intermittently over ~300 Ma in varying kinematic regimes, by combining zircon Lu-Hf isotopic data from Early Palaeozoic to Early Jurassic igneous and metaigneous rocks in the Mérida Andes, Venezuela and the Santander Massif, Colombia, with new whole rock Rb/Sr and Sm-Nd isotopic data, and quartz O isotopic data. These new data are unique in South America because they were obtained from discrete magmatic and metamorphic zircon populations, providing a high temporal resolution dataset, and compare several isotopic systems on the same samples. Collectively, these data provide valuable insight into the evolution of the isotopic structure of the continental crust in long-lived active margins.Phanerozoic active margin-related granitoids in the Mérida Andes and the Santander Massif yield zircon Lu-Hf model ages ranging between 0.77 Ga and 1.57 Ga which clearly define temporal trends that can be correlated with changes in tectonic regimes. The oldest Lu-Hf model ages of >1.3 Ga are restricted to granitoids which formed during Barrovian metamorphism and crustal thickening between ~499 Ma and ~473 Ma. These granitoids yield high initial 87Sr/86Sr ratios, suggesting that evolved, Rb-rich middle to upper crust was the major source of melt. Granitoids and rhyolites which crystallised during subsequent extension between ~472 Ma and ~452 Ma yield younger Lu-Hf model ages of 0.80 Ga–1.3 Ga and low initial 87Sr/86Sr ratios, suggesting that they were derived from much more juvenile, Rb-poor sources such as mafic lower crust and mantle-derived melts. The rapid change in magmatic sources at ~472 Ma can be attributed either to reduced crustal assimilation during extension, or a short pulse of crustal growth by addition of juvenile material to the continental crust. Between ~472 Ma and ~196 Ma Lu-Hf model ages remain mostly constant between ~1.0 and ~1.2 Ga. The large scatter and the absence of definite trends in initial 87Sr/86Sr ratios suggest that both mafic, Rb-poor, and evolved Rb-rich sources were important precursors of active margin magmas in Colombia and Venezuela throughout the Palaeozoic to the Early Jurassic.Previous studies have shown that the genesis of arc magmas may be stimulated by heat advection to the crust during the underplating of mantle derived melt, but the absence of permanent younging trends in Lu-Hf model ages from ~472 Ma to ~196 Ma suggests that very little new crust was generated during this period in the studied region. An overwhelming majority of the analysed igneous rocks yield zircon Lu-Hf model ages of >1 Ga which may be accounted for by documented local crustal end members of 1 Ga–1.6 Ga, and do not require contributions from the depleted mantle. Therefore, recycling of ~1 Ga and older crust was a dominant process in the north-western corner of Gondwana between ~472 Ma and ~196 Ma.This study shows that whole rock Sm-Nd and zircon Lu-Hf data can be interpreted similarly regarding the age of the source regions, whereas Rb-Sr and O isotope data from the same rocks yield valuable information regarding the geochemical nature of the source. 相似文献
17.
Neoproterozoic Mafic Dykes and Basalts in the Southern Margin of Tarim, Northwest China: Age, Geochemistry and Geodynamic Implications 总被引：4，自引：0，他引：4
<正>Neoproterozoic rifting-related mafic igneous rocks are widely distributed both in the northern and southern margins of the Tarim Block,NW China.Here we report the geochronology and systematic whole-rock geochemistry of the Neoproterozoic mafic dykes and basalts along the southern margin of Tarim.Our zircon U-Pb age,in combination with stratigraphic constraint on their emplacement ages,indicates that the mafic dykes were crystallized at ca.802 Ma,and the basalt, possibly coeval with the ca.740 Ma volcanic rocks in Quruqtagh in the northern margin of Tarim. Elemental and Nd isotope geochemistry of the mafic dykes and basalts suggest that their primitive magma was derived from asthenospheric mantle(OIB-like) and lithospheric mantle respectively,with variable assimilation of crustal materials.Integrating the data supplied in the present study and that reported previously in the northern margin of Tarim,we recognize two types of mantle sources of the Neoproterozoic mafic igneous rocks in Tarim,namely the matasomatized subcontinental lithospheric mantle(SCLM) in the northern margin and the long-term enriched lithospheric mantle and asthenospheric mantle in the southern margin.A comprehensive synthesis of the Neoproterozoic igneous rocks throughout the Tarim Block led to the recognition of two major episodes of Neoproterozoic igneous activities at ca.820-800 Ma and ca.780-740 Ma,respectively.These two episodes of igneous activities were concurrent with those in many other Rodinian continents and were most likely related to mantle plume activities during the break-up of the Rodinia. 相似文献
18.
We report the results of a SIMS U-Pb study of 112 zircons from breccia samples from the Apollo 14 and 17 landing sites. Zircon occurs in the breccia matrices as rounded, irregular shaped, broken and rarely euhedral grains and as constituent minerals in a variety of lithic clasts ranging in composition from ultra-mafic and mafic rocks to highly evolved granophyres. Crystallisation of zircon in magmatic rocks is governed by the zirconium saturation in the melt. As a consequence, the presence of zircon in mafic rocks on the Moon implies enrichment of their parent melts in the KREEP component. Our SIMS results show that the ages of zircons from mafic to ultramafic clasts range from ca. 4.35 Ga to ca. 4.00 Ga demonstrating multiple generations of KREEPy mafic and ultramafic magmas over this time period. Individual zircon clasts in breccia matrices have a similar age range to zircons in igneous clasts and all represent zircons that have been incorporated into the breccia from older parents. The age distributions of zircons from breccias from both the Apollo 14 and Apollo 17 landing sites are essentially identical in the range 4.35-4.20 Ga. However, whereas Apollo 14 zircons additionally show ages from 4.20 to 3.90 Ga, no zircons from Apollo 17 samples have primary ages less than ca. 4.20 Ga. Also, in contrast to previous suggestions that the magmatism in the lunar crust is continuous our results show that the zircon age distribution is uneven, with distinct peaks of magmatic activity at ca. 4.35 Ga, ca. 4.20 Ga in Apollo 14 and 17 and a possible third peak in zircons from Apollo 14 at ca. 4.00 Ga. To explain the differences in the zircon age distributions between the Apollo 14 and 17 landing sites we propose that episodes of KREEP magmatism were generated from a primary reservoir, and that this reservoir contracted over time towards the centre of Procellarum KREEP terrane. We attribute the peaks in KREEP magmatism to impact induced emplacement of KREEP magma from a primary mantle source or to a progressive thermal build-up in the mantle source until the temperature exceeds the threshold for generation of KREEP magma, which is transported into the crust by an unspecified possibly plume-like process. 相似文献
19.
前人通过滇西三江带内岩浆记录精细刻画了古特提斯洋分支洋——哀牢山洋的形成及演化历史,然而区域沉积记录是如何响应哀牢山洋俯冲及闭合过程的,目前仍未得到深入研究。我们通过对哀牢山构造带北段点苍山变质杂岩内三叠纪至侏罗纪3件沉积岩样品中255颗碎屑锆石进行U-Pb定年、微量元素及Hf同位素分析,结合区域已有研究,恢复哀牢山洋末期演化的区域沉积响应。结果表明,变质砂岩DC1801、片岩DC1703和碳酸盐岩DC1702中最年轻岩浆锆石群加权平均年龄分别为~180 Ma、~247 Ma和~254 Ma,结合其接触关系以及区域地层对比,约束其最大沉积年龄分别为侏罗纪早期(DC1801)和三叠纪早期(DC1702和DC1703)。不同时期碎屑沉积岩物源分析表明三叠纪碎屑沉积岩(DC1703)主要源自哀牢山构造带内部近源的多期岩浆物质(~0.8 Ga、~0.45 Ga和~0.25 Ga)、冈瓦纳裂解前印度大陆内部多期再循环的格林威尔晚期(~0.95 Ga)和泛非期(~0.6 Ga)岩浆物质贡献。侏罗纪碎屑沉积岩(DC1801)物质主要源自思茅地块内部印支期岩浆活动,而~0.45 Ga、~0.8 Ga和~0.95 Ga等时期的碎屑物质贡献比例明显降低。同一沉积盆地同时代碳酸盐岩与陆源碎屑岩中碎屑锆石结构大体相似,但碳酸盐岩中代表多期循环的远源物质的年龄所占比例却降低。点苍山碎屑沉积岩锆石Hf同位素组成随时间变化证实了哀牢山洋闭合时间为~247 Ma,而在点苍山变质地体南段发育的海相碳酸盐岩与陆源碎屑岩(片岩)的沉积组合记录了哀牢山洋末期演化至闭合过程。碎屑锆石Eu/Eu*异常揭示了区域地壳自~247 Ma哀牢山洋闭合至~235 Ma的加厚过程,三叠纪至侏罗纪碎屑沉积物源的转化可能与哀牢山洋闭合引发的沉积区抬升有关。 相似文献
20.
祥山和于埠变质辉长岩是胶北地块上古元古代变质镁铁质岩石的典型代表,辉长岩侵入古元古代荆山群野头组,产有"祥山式"岩浆熔离型铁矿,成矿的专属性指示辉长岩属于层状侵入体类型,形成于大陆伸展构造背景。在祥山变质辉长岩中获得了1851±9Ma的变质年龄,在于埠变质辉长岩中获得了2052±23Ma的锆石U-Pb成岩年龄和1834±5Ma的变质年龄。~2.05Ga的岩浆结晶锆石的εHf(t)值均为正值(+1.87~+3.64),一阶段Hf模式年龄(tDM)为2292~2381Ma(平均为2327Ma),指示于埠变质辉长岩源自古元古代中期的亏损地幔。于埠变质辉长岩的成岩年龄制约了荆山群野头组的沉积上限,荆山群中至少有一部分形成于2.2~2.05Ga之间,沉积于大陆裂谷-稳定大陆边缘的构造环境。祥山和于埠变质辉长岩中有少量斜长花岗岩与之伴生,这些斜长花岗岩具有类似于大洋斜长花岗岩的岩石特征,低K、Ti、Sr,高Na、Yb,形成于低压背景;从斜长花岗岩中获得了1848±8Ma和1873±5Ma的锆石U-Pb年龄,斜长花岗岩中的锆石Th/U比值较低(0.01~0.29),具有初始熔体中结晶锆石特征。结合斜长花岗岩的地球化学特征,推测它们是辉长岩部分熔融的产物,并指示~1.87Ga已由挤压构造体制转变为伸展构造体制。综合前人研究成果,胶北地块已识别出2.18~2.15Ga、~2.10Ga、~2.05Ga的三期双峰式岩浆岩构造组合,指示2.2~2.05Ga期间总体为伸展构造背景。因此建议胶-辽-吉活动带的形成演化过程划分为两个阶段,早期为大陆裂解-稳定陆缘演化阶段(2.2~2.0Ga),沉积了巨量的陆缘碎屑岩-碳酸盐岩建造;晚期为俯冲-碰撞造山阶段(2.0~1.85Ga),胶-辽-吉活动带褶皱造山。 相似文献