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1.
对蚌埠隆起区中生代不同时期的花岗岩中6个岩体的锆石LA-MC-ICP MS原位Hf同位素的研究,据此限定它们的岩浆源区和重建华北克拉通东南部的构造格架。结果表明,中生代不同时期的花岗岩中岩浆锆石的初始Hf同位素组成(ε_(Hf)(t))可以分成两组:第一组的女山(130Ma)和西庐山花岗岩(130Ma)的ε_(Hf)(t)值分别为-18.4和-16.1;第二组的曹山(110Ma)、锥山二长花岗岩(110Ma)和蚂蚁山花岗岩(110Ma)以及淮光花岗闪长岩(130Ma)的ε_(Hf)(t)值分别为-22.3、-23.1和-21.1以及-28.1,这些岩浆锆石低的ε_(Hf)(t)值表明它们可能来源于古老的大陆下地壳。女山和西庐山岩体中早古生代—新元古代继承锆石具有低的ε_(Hf)(t)值(-2.3~-7.7)和1.52Ga~1.79Ga的Hf同位素两阶段模式年龄,表明它们的岩浆源区主要以扬子克拉通下地壳物质为主。曹山、锥山和蚂蚁山以及淮光岩体中岩浆锆石的Hf同位素两阶段模式年龄为1.89Ga~2.58Ga,结合淮光岩体中古元古代继承锆石和3400Ma捕获锆石中低的ε_(Hf)(t)值(-5.7~-6.8,-0.6、-0.9)和古老的Hf同位素两阶段模式年龄(2.44Ga~2.80Ga,3.7Ga),表明它们主要来源于华北克拉通下地壳物质的部分熔融。淮光和女山岩体中古元古代—新太古宙继承锆石中正的ε_(Hf)(t)值(0.3~6.7)以及高的ε_(Hf)(t)值(16.9~21.7)的存在,暗示形成这些古老继承锆石的初始物质中有幔源物质的涉入。蚌埠隆起区深部地壳中扬子克拉通基底物质的存在暗示扬子克拉通可能沿着郯庐断裂带向西或北西方向俯冲于华北克拉通之下。  相似文献   

2.
基底古老地层的研究可以为探索地球早期陆壳形成与演化历史提供重要支持,胶东地区是华北克拉通变质基底重要的出露区之一,在胶北地体的西缘有一套高成熟度的古老石英岩-山阳村石英岩,前人将其划归古元古代粉子山群的小宋组,但缺乏明确的年代学限定。本文对山阳村石英岩的碎屑锆石进行U-Pb年代学和Hf同位素分析,获得年龄谱的最大峰值为2501±16Ma,且是最小峰值年龄。与古元古的粉子山群和中元古的芝罘群的碎屑锆石年龄谱均不同。综合年龄谱特征、野外产状以及岩石组合,本文认为山阳村石英岩是新太古代的岩石建造,建议为其单独建立新太古代岩石地层单位。结合本次研究及前人工作本文认为应将原粉子山群小宋组划到太古代归属胶东岩群。山阳村石英岩中,~2.5Ga锆石Hf同位素εHf(t)0且从下方靠近亏损地幔演化线并在~2.7Ga地壳演化线附近分布,显示其原岩来自~2.7Ga新生地壳的重熔;ca.2.7~3.0Ga的锆石Hf同位素εHf(t)0且在~3.1Ga地壳演化线附近,意味着其母岩的源区为~3.1Ga的新生地壳,且在ca.2.7~3.0Ga发生了持续的地壳再熔融;3.0Ga碎屑锆石的Hf同位素εHf(t)0,源区岩石形成于更古老陆壳物质的再循环。已知的胶北地块3.0Ga锆石的Hf同位素特征暗示华北克拉通在4.1Ga前就存在地壳,而且在~4.1Ga发生了重熔。  相似文献   

3.
第五春荣  孙勇  王倩 《岩石学报》2012,28(11):3520-3530
定量地给出大陆地壳生长速率以及生长量随时间的演化是研究大陆地壳形成与演化的核心问题之一.近年来,利用沉积岩和沉积物中碎屑锆石的U-Pb年龄和Hf同位素组成已成为目前研究大陆地壳生长和演化最为简捷、有效的工具.本文对来自华北克拉通西部泾河和洛河河沙中的187颗碎屑锆石进行Hf同位素组成分析,并结合已有的资料来探讨华北克拉通地壳的生长和演化规律.结果显示:随着地质历史变化,华北克拉通地壳生长呈阶段性特点.如在中太古代中期-新太古代末期(3.0 ~2.5Ga)地壳生长速率较快,大约已有60%现今大陆地壳形成.此后,陆壳呈较稳定速率增长,到新元古代晚期(600Ma)基本己形成现存大陆地壳.表明现今的大陆主要生长于太古宙和元古宙,而显生宙陆壳的增生量可以忽略不计.根据河流碎屑锆石和前寒武纪岩石中锆石的U-Pb年龄、两阶段模式年龄(t DM2C和tNC2C)和εHf(t)所获得华北克拉通早前寒武纪地壳演化曲线,本文提出~2.7Ga和~2.5Ga分别曾经为华北克拉通太古宙岩浆作用最活跃时期,也是地壳快速生长时期,表明华北克拉通在新太古代曾发生过两期明显的地壳生长.  相似文献   

4.
位于华北克拉通东缘的胶北地体,被普遍认为是胶-辽-吉带的西南组成部分,经历了多期岩浆-变质热事件,而晚太古宙末期约2.5Ga的岩浆事件是该区最强的岩浆事件;为了确定该期岩浆热事件的性质,本文选取2件形成于约2.5Ga的英云闪长质片麻岩及花岗质片麻岩开展锆石Hf同位素测试分析;总计69个锆石Hf同位素分析点的结果显示,它们均具有正的εHf(t)值,在10.71到3.0之间,平均为6.02,两阶段锆石Hf模式年龄主要分布于2.6~2.9Ga之间,平均为2747Ma,明显大于锆石的207Pb/206Pb年龄,表明约2.5Ga的TTG及花岗质片麻岩主要源于2.6~2.9Ga新生地壳的重熔或再造;另外,一些锆石具有极正的εHf(t)值,它们的锆石Hf模式年龄与U-Pb年龄相近,这暗示在约2.5Ga有亏损地幔物质加入地壳,并发生了即时重熔;根据本次研究获得的锆石Hf同位素数据,结合前人的Nd同位素结果,我们认为胶北地体内约2.5Ga的岩浆活动可能主要表现为与地幔岩浆低侵作用有关的新生地壳的重熔或再造,约2.9Ga和2.7~2.8Ga是胶北地体地壳生长的两个时期,并且与华北克拉通大部分地区一样,2.7~2.8Ga是胶北地体新生地壳形成最重要的时期。  相似文献   

5.
中国西秦岭碎屑锆石U-Pb年龄及其构造意义   总被引:5,自引:1,他引:4  
西秦岭是北接华北克拉通、西接祁连与柴达木、南接松潘—甘孜地块的东秦岭造山带的西延。文中研究了该区从前寒武纪到三叠纪的碎屑沉积岩。这些碎屑沉积岩中分离出的锆石由LA-ICPMS(激光剥蚀等离子体质谱)进行了U-Pb定年。全岩Nd亏损地幔模式年龄类似于扬子克拉通年龄,主要分布于1.55~1.98Ga,峰值为1.81Ga,而与华北克拉通主要为古元古代与太古宙的模式年龄形成明显的对比。泥盆系中的碎屑锆石930~730Ma的U-Pb年龄指示其与扬子克拉通具亲缘性。930~730Ma是源区地壳的强烈增长阶段。二叠系—三叠系的碎屑沉积岩主体以含老于1600Ma的碎屑锆石为特征。碎屑锆石U-Pb年龄与Sm-Nd同位素组成指示此时华北克拉通南缘的基底岩石成为二叠系—三叠系碎屑沉积岩的重要物源。扬子克拉通在三叠纪时与华北克拉通拼接。西秦岭二叠系—三叠系碎屑沉积岩含有高达50%的华北克拉通南缘的基底岩石。  相似文献   

6.
对登封地区嵩山群五指岭组二云石英片岩和石英岩中碎屑锆石进行了LA-ICP-MS U-Pb年代学和原位Hf同位素分析,为探讨华北克拉通南缘太古宙地壳生长和再造提供了制约。结果显示,碎屑锆石多数呈自形–半自形,发育振荡生长环带,结合相对高的Th/U比值(0.07~1.87),暗示它们多数为岩浆成因。二云石英片岩和石英岩中碎屑锆石具有类似的年龄和Hf同位素组成,它们的207Pb/206Pb谐和年龄分别介于2879~2027 Ma和3346~1903 Ma之间,峰期年龄分别为2524 Ma和2528 Ma。~2.5 Ga锆石的εHf(t)值多数为正值,介于+0.10~+9.22之间,tDM2C变化于3028~2453 Ma之间,4颗碎屑锆石的εHf(t)值为负值,变化于-1.68~-0.03之间,tDM2C介于3132~3032 Ma之间。根据上述结果并结合相邻地区的相关研究资料,表明嵩山群沉积于古元古代晚期,五指岭组中碎屑锆石的物源主要为华北克拉通南缘~2.5 Ga具有新生地壳属性的结晶基底物质。华北克拉通南缘存在中–新太古代时期的地壳生长,同时发育中太古代古老地壳物质的再造。  相似文献   

7.
华北克拉通五台群LA-ICP-MS锆石U-Pb年龄和Hf同位素特征   总被引:2,自引:0,他引:2  
通过对五台群石咀亚群金刚库组4个典型样品的LA-ICP-MS锆石U-Pb年龄和Hf同位素研究,对五台群的形成时代及华北克拉通新太古代—古元古代期间的地壳演化进行了探讨。锆石U-Pb同位素测定结果表明,侵入金刚库组中的片麻状花岗岩锆石的U-Pb年龄为2548Ma,因此五台群的上限年龄约为2.5Ga;金刚库组黑云母石英片岩和片麻状石英闪长岩的原岩锆石U-Pb年龄分别为2663Ma和2636Ma,因此五台群的下限年龄约为2.7Ga。五台群的地质年龄为2.5~2.7Ga,属于新太古代。锆石Hf同位素研究结果表明,黑云母石英片岩和片麻状石英闪长岩的二阶段Hf模式年龄(tDM2)均为2.8Ga左右,指示2.8Ga左右是五台山区乃至整个华北克拉通地壳生长的重要时期;片麻状花岗岩tDM2平均为2.57Ga,与锆石结晶年龄非常接近,表明2.5Ga左右也是华北克拉通地壳的主要增生期。地壳的增长是幕式的,2.8Ga和2.5Ga都是华北克拉通地壳生长时期。  相似文献   

8.
报道了五台地区一个晚太古代片麻状富钾花岗岩的锆石U-Pb年龄为2509±7.4Ma.该年龄与前人获得的年代学数据一起,进一步限定了晚太古期间五台-吕梁地区与俯冲有关的弧岩浆活动的年代框架.为了探讨晚太古宙-古元古代不同类型的花岗岩的源区性质和演化,特别是当时的陆壳增生机制和古老陆壳性质,本文在锆石U-Pb年代学的基础上对相应的锆石进行了细致的Hf同位素原位测量.结果表明,晚太古代片麻状花岗岩可能代表发育在古老克拉通(东部陆块?)上的弧岩浆作用产物.碰撞后(1.8 Ga)花岗岩的形成与加厚的造山带发生垮塌性伸展有关,后者导致幔源物质底侵,并引起下地壳物质的部分熔融而形成花岗质岩石.这些壳源花岗质岩浆再以不同比例与幔源岩浆混合而形成吕梁-五台地区成分复杂的碰撞后岩浆岩(花岗质为主).锆石Hf同位素还表明,吕梁-五台地区可能存在老于2.7Ga的古老克拉通物质(2.9Ga?),虽然目前还没有发现这么老的碎屑锆石.  相似文献   

9.
本文报道了华北克拉通西部武川西乌兰不浪地区太古宙变质基底的锆石SHRIMP年龄和Hf同位素组成。一个片麻状奥长花岗岩样品的锆石具核边结构,核部岩浆锆石和边部变质锆石的207Pb/206Pb加权平均年龄分别为2692±17Ma和2528±16Ma。对9个样品进行了锆石Hf同位素分析。新太古代早期(2692~2697Ma)片麻状奥长花岗岩(2个样品)的岩浆锆石的εHf(t)、tDM1(Hf)和tDM2(Hf)分别为4.78~8.83、2646~2780Ma和2632~2845Ma;新太古代二辉麻粒岩(2个样品)中的捕获锆石的εHf(t)、tDM1(Hf)和tDM2(Hf)分别为-2.30~8.62、2543~2954Ma和2529~3189Ma;新太古代变质深成岩(4个样品)的岩浆锆石的εHf(t)、tDM1(Hf)和tDM2(Hf)分别为-2.60~8.09、2529~2880Ma和2538~3089Ma;古元古代蓝晶石榴长英质片麻岩(1个样品)的碎屑锆石的εHf(t)、tDM1(Hf)和tDM2(Hf)分别为1.52~6.59、2432~2774Ma和2498~2925Ma。结合前人研究结果,可得出如下结论和认识:1)该区存在新太古代早期片麻状奥长花岗岩,太古宙岩石在新太古代晚期普遍遭受高级变质作用影响;2)新太古代早期为该区地壳形成主要时期,新太古代晚期则主要表现为陆壳物质再循环;3)作为阴山地块的典型代表,固阳-武川地区与华北克拉通东部太古宙基底十分类似,可能表明华北克拉通在新太古代晚期已成为统一的整体。  相似文献   

10.
中国最老岩石和锆石   总被引:18,自引:12,他引:6  
在中国大陆的许多地区都已发现大于3.4Ga的锆石和岩石.鞍山是全球仅有几个存在≥3.8Ga岩石的地区之一.它们以不大的规模存在于白家坟、东山、深沟寺杂岩中,由糜棱岩化奥长花岗岩、条带状奥长花岗岩和变质石英闪长岩组成.近年来,在鞍山地区还发现了许多3.7~3.6Ga岩石和锆石.锆石Hf同位素组成表明鞍山地区在3.8~3.6Ga期间存在周期性的地幔添加和陆壳形成.除鞍山外,在中国许多地区的不同类型岩石中也获得了≥3.4Ga锆石,虽然它们大多数都是碎屑和残余成因.(1)华北克拉通冀东铬云母石英岩中3.85~3.55Ga碎屑锆石:(2)华北克拉通信阳中生代火山岩长英质麻粒岩中3.66Ga岩浆锆石;(3)华南克拉通宜昌地区杨子地块新元古代砂岩中3.80Ga碎屑锆石(一颗);(4)华南克拉通华夏地块新元古代一古生代变质沉积岩中3.76~3.6Ga碎屑锆石;(5)西北地区塔里木地块阿克塔什塔格地区古元古代片麻状花岗岩中3.6Ga残余锆石;(6)西秦岭奥陶纪变质火山岩中4.08Ga捕掳锆石(一颗);(7)西藏普兰地区奥陶纪石英岩中4.1Ga碎屑锆石(一颗,有3.61Ga增生边).一些古老锆石有高达4.1~4.0Ga的Hf同位素模式年龄.在中国,>3.4Ga地壳物质的比例以往被低估了,发现冥古宙和始太古代物质的可能性仍然存在,它们将对中国早期陆壳演化提供新的制约.  相似文献   

11.
By the analysis of the published zircon U-Pb ages and Hf isotope data, this paper firstly presents a comprehensive review about the staggered growth and reworking of early Precambrian continental crust in Alxa Block. The results show that the ancient crustal remnants of Alxa Block was formed in Meso-Paleo Archean, which was recorded by 3.0~3.6 Ga detrital zircons and Hf model ages. The early crustal growth of Alxa Block could be traced back to early Paleo-archean. Currently, the oldest zircon U-Pb age is about 3.6 Ga. Analogous to the other places of North China Craton, the Alxa Block underwent two-stage crustal growth at 2.7~2.9 Ga and 2.5~2.6 Ga respectively, and the former might be wider. The ~2.5 Ga (TTG) tectono-magmatic event, which represents the North China continent’s cratonization, also existed in Alxa Block. The corresponding zircon Hf isotope data indicate that the TTGs were mainly derived by melting of 2.7~2.9 Ga juvenile crust, possibly by mixing with a certain ancient crust, and a small portion was produced by instant reworking of 2.5~2.6 Ga juvenile crust. Proceeding to Paleo-proterozoic, the Alxa Block underwent multi-stage tectono-magmatic events, approximately peaked at 2.30~2.35 Ga, 2.15~2.17 Ga, 2.00~2.10 Ga, 1.95~1.98 Ga and ~1.90 Ga. The continental crust was mainly formed by reworking of 2.7~2.9 Ga and 2.5~2.6 Ga juvenile crust, simultaneously by a fraction of ~2.1 Ga juvenile crust. In Paleo-proterozoic, not only the Archean crustal reworking but also the juvenile crustal growth existed in Alxa Block.  相似文献   

12.
古老锆石和岩石的发现,是探索地球早期地质演化的关键.为进一步揭示扬子陆块基底物质组成和早期地壳形成演化,采用LA-ICP-MS锆石微区U-Pb测年,对扬子陆块西南缘禄丰地区东川群变质砂岩进行了年代学研究,发现3 822±21 Ma的古老碎屑锆石.这是目前在扬子陆块获得的第2颗>3.8 Ga的古老锆石,也是目前在该地区发现的最老锆石.变质砂岩碎屑物质主要包括4个峰值年龄(~2 320 Ma、~2 162 Ma、~2 036 Ma和~1 915 Ma),2颗最年轻的锆石年龄基本限定了东川群早期最大沉积时限,与区域上火山岩时代相吻合.另外还包含少量中-晚太古代(2.6~2.9 Ga)和始太古代(3.7~3.8 Ga)的碎屑物质.Hf同位素组成显示这些碎屑锆石具有不同成因,其中2 674~3 822 Ma的碎屑锆石总体具有正的εHf(t)值和2.9~3.9 Ga的两阶段模式年龄,暗示扬子陆块在冥古宙-古太古代时期就有一定规模的新生陆壳分布.古元古代(1.9~2.4 Ga)的岩浆活动除有少量古元古代(2.3~2.4 Ga)新生地壳组分熔融外,大多为太古宙(2.5~3.7 Ga)古老地壳部分熔融.中元古代更多表现为古老地壳的熔融和物质再循环.研究结果为深化扬子陆块早前寒武纪地质演化认识提供了新资料.   相似文献   

13.
锆石U-Pb定年及Hf同位素测定结果表明,鄂尔多斯盆地周缘的华北板块北缘、兴蒙造山系及扬子板块—秦岭—大别—苏鲁造山带等构造单元系统具有明显不同的形成与演化历史。华北板块北缘锆石年龄平均值为1 837Ma,最强烈的岩浆活动出现于2 200~1 800Ma,该期锆石约占全部的40%;次为强烈的岩浆活动在2 800~2 200Ma,其众数在全部锆石中约占30%;1 500~1 200Ma、500~100Ma这两个阶段形成的锆石在全区所占比例各约为15%。华北板块北缘最突出的特征是基本不含1000~700 Ma期间形成的锆石,>3 000Ma的锆石在全区分布极为有限。锆石Hf同位素亏损地幔模式年龄表明华北板块北缘平均值为2.55Ga,较U-Pb平均年龄老,说明2 200~1 800Ma期间形成的锆石含有较多的古老地壳再循环组分。Hf亏损地幔模式年龄最强峰值约为2.8Ga,与全岩Nd亏损地幔模式年龄的峰值相一致,Hf模式年龄为3.0~2.25Ga的颗粒占全部的近95%,证明华北板块北缘的地壳增生主要在太古宙至古元古代期间。Hf同位素亏损地幔模式年龄>3.0Ga的锆石颗粒所占比例不到0.1%,另外近5%锆石的模式年龄分布于中元古代。晚古生代—中生代所形成的锆石均是先存地壳组分,尤其是中元古代增生地壳的熔融作用形成。兴蒙造山系中锆石U-Pb年龄平均值为497Ma,最强峰分布于石炭纪(约320Ma),石炭纪—二叠纪末(350~250Ma)形成的锆石所占比例达30%以上。新元古代至早古生代(600~440Ma)形成的锆石占全部锆石的55%以上,而中元古代末—新元古代期间(1 200~600Ma)形成的锆石在全区仅占4%。中元古代以前形成的锆石非常有限,说明该区最早形成的地壳组分在兴蒙造山系的形成过程中较充分地参与到后期的岩浆作用过程中。兴蒙造山系中锆石相应的Hf同位素亏损地幔模式年龄平均为1.13Ga,明显较相应的U-Pb年龄老,最强峰值出现于约0.6Ga。Hf亏损地幔模式年龄为0.7~0.28Ga的颗粒在兴蒙造山系所占比例达57%,证明该区最强烈的地壳增生发生于新元古代至古生代期间。Hf同位素亏损地幔模式年龄分布于1.5~0.7Ga的锆石在全区约占38%,说明此期间也是该区地壳较强烈的增生期。Hf亏损地幔模式年龄大于1.5Ga的锆石所占比例不到5%,古生代以后兴蒙造山系也基本没有明显的地壳增生。扬子与秦岭—大别—苏鲁造山带构造单元中的锆石U-Pb年龄平均为799Ma,年龄为1 300~750Ma的锆石在全部锆石中约占70%。晚古生代—燕山期形成的锆石约占20%。年龄在3500~2 650Ma、2 118~1 680Ma的锆石在该区各约占5%。结合扬子与秦岭—大别—苏鲁造山带平均为1.56Ga的Nd亏损地幔模式年龄特征,说明1 300~750Ma期间该区较强烈的岩浆作用事件中有较多的古老地壳组分加入其中。锆石U-Pb年龄及Hf同位素组成均说明鄂尔多斯盆地周缘各构造单元具有不同的形成演化历史。地壳是幕式增长的,但各构造单元每幕发生的时间、强度存在明显差别。因此,由盆地中不同时代地层中碎屑锆石U-Pb年龄及Hf同位素组成及全岩Nd同位素特征的系统研究可反演盆地物源供给与周围构造单元之间的关系。  相似文献   

14.
Discoveries of >4 Ga old zircon grains in the northwest Yilgarn of Western Australia led to the conclusion that evolved crust formed on the Earth within the first few 100 Ma after accretion. Little is known, however, about the fate of the first crust that shaped early Earth's surface. Here we report combined solution and laser-ablation Lu–Hf–U–Pb isotope analyses of early Archean and Hadean detrital zircon grains from different rocks of the Narryer Gneiss Complex (NGC), Yilgarn Craton, Western Australia. The zircons show two distinct groups with separate evolutionary trends in their Hf isotopes. The majority of the zircon grains point to separation from a depleted mantle reservoir at ∼3.8–3.9 Ga. The second Hf isotope trend implies reworking of older Hadean zircon grains. The major trend starting at 3.8–3.9 Ga defined by the Hf isotopes corresponds to a Lu/Hf that is characteristic for felsic crust and consequently, the primary sources for these zircons presumably had a chemical composition characteristic of continental crust. Reworked Hadean crust appears to have evolved with a similar low Lu/Hf, such that the early crust was probably evolved with respect to Lu–Hf distributions. The co-variation of Hf isotopes vs. age in zircon grains from Mt. Narryer and Jack Hills zircon grains implies a similar crustal source for both sediments in a single, major crustal domain. Age spectra and associated Hf isotopes in the zircon grains strongly argue for ongoing magmatic reworking over hundreds of millions of years of the felsic crustal domain in which the zircon grains formed. Late-stage metamorphic zircon grains from the Meeberrie Gneiss unit yield a mean U–Pb age of 3294.5 ± 3.2 Ma with initial Hf isotopes that correspond to the evolutionary trend defined by older NGC zircon grains and overlap with other detrital zircon grains, proving their genetic relationship. This ‘Meeberrie event’ is interpret here as the last reworking event in the precursor domain before final deposition. The continuous magmatic activity in one crustal domain during the Archean is recorded by the U–Pb ages and Hf isotope systematics of zircon grains and implies reworking of existing crust. We suspect that the most likely driving force for such reworking of crustal material is ongoing crustal collision and subduction. A comparison of Hf isotope signatures of zircon grains from other Archean terranes shows that similar trends are recognised within all sampled Archean domains. This implies either a global trend in crustal growth and reworking, or a genetic connection of Archean terranes in close paleo-proximity to each other. Notably, the Archean Acasta gneiss (Canada) shows a similar reworking patterns to the Yilgarn Craton of Hadean samples implying either a common Hadean source or amalgamation at the Hadean–Archean transition.  相似文献   

15.
对扬子陆块三峡地区黄牛岩剖面莲沱组顶部砂岩中的120颗碎屑锆石进行了U-Pb定年和Lu-Hf同位素分析.结果显示,黄牛岩剖面莲沱组中碎屑锆石的年龄谱具有~880~800 Ma、~2 000 Ma、~2 500 Ma及~2 700 Ma的峰值,其中最年轻的碎屑锆石年龄为724±8 Ma.结合前人对该地区莲沱组顶部凝灰岩开展的年代学工作,将莲沱组顶部砂岩沉积时代限定为724~714 Ma.莲沱组砂岩沉积时间与其中最年轻的碎屑锆石U-Pb年龄接近,反映了其源区地壳物质的快速再循环.碎屑锆石Hf同位素两阶段模式年龄(TDM2)集中在~3.7~3.1 Ga、~2.5~2.0 Ga和~1.3~1.0 Ga,反映其物源区存在古-中太古代、古元古代以及中元古代末期的初生地壳生长.对比近年来三峡地区不同剖面莲沱组砂岩中已报道的碎屑锆石年龄和Hf同位素数据,黄牛岩剖面的莲沱组碎屑锆石年龄和Hf同位素组成与之以北的王丰岗剖面均存在明显差异,说明莲沱组沉积期两者的陆源物质供给区有较大差别.   相似文献   

16.
扬子陆核的生长和再造:锆石U-Pb年龄和Hf同位素研究   总被引:5,自引:2,他引:5  
张少兵  郑永飞 《岩石学报》2007,23(2):393-402
对宜昌三峡附近崆岭杂岩中混合岩、片麻岩和变沉积岩以及莲沱砂岩进行了锆石U-Pb和Hf-O同位素研究,研究结果深化了我们对扬子陆核生长和再造的认识。在莲沱砂岩中发现了老达3.8Ga的碎屑锆石,说明扬子陆块可能存在这个年龄的地壳物质;其Hf同位素组成指示初生地壳生长出现在4.0Ga。崆岭杂岩中混合岩和片麻岩的U-Pb年龄表明,在3.2~3.3Ga和2.9~3.0Ga有两期重要的岩浆活动,指示扬子陆核可能于中太古代就开始形成。锆石Hf同位素研究则指示,其原岩至少从3.5Ga就开始从亏损地幔分异出来。混合岩和变沉积岩中所记录的1.9~2.0Ga变质事件,是扬子陆核再造并发生克拉通化的主要时期。而广泛分布于扬子陆块周边的新元古代岩浆活动不仅导致了许多太古宙和古元古宙地壳重熔,而且引起了初生地壳的快速再造。  相似文献   

17.
赵燕  第五春荣  孙勇  朱涛  王洪亮 《岩石学报》2013,29(5):1698-1712
敦煌杂岩位于塔里木克拉通的东部,探寻和研究其中的早前寒武纪地质体对于探讨敦煌地块早前寒武纪地壳的形成和演化及其构造归属等问题具有重要的意义.甘肃敦煌水峡口地区的敦煌杂岩主要由英云闪长质片麻岩、花岗闪长质片麻岩以及表壳岩石组成.利用LA-ICP-MS锆石U-Pb定年方法测得水峡口英云闪长片麻岩和花岗片麻岩原岩的形成年龄分别为2561±16Ma和2510±22Ma,确证了在敦煌杂岩中存在太古宙岩石.此外,还获得斜长角闪岩的变质年龄为1806±14Ma,推测其原岩岩浆可能来自古老岩石圈地幔的部分熔融.根据已有的资料提出在古元古代晚期(1.80 ~ 1.85Ga)敦煌杂岩经历了一期较广泛的变质作用.锆石Hf同位素显示~2.5Ga的岩石年龄在敦煌地块代表新太古代晚期重要地壳生长时期,而~1.8Ga的构造-热事件则是以古老地壳物质循环再造为主.这些资料显示敦煌地块和华北克拉通在早前寒武纪经历了类似的地壳形成和演化过程,且共同记录了全球性的Columbia碰撞造山事件信息.  相似文献   

18.
How the earth's crust formed and evolved during the Precambrian times is one of the key questions to decipher the evolution of the early Earth. As one of the few cratons containing well-preserved Eoarchean to Neoarchean basement on Earth, the North China Craton is an ideal natural laboratory to unravel the early crustal evolution. It is controversial whether the Archean tectonothermal events in this area represents reworking or growth of the continental crust. To solve this issue, we have compelled field-based mapping, zircon U–Pb dating by SHRIMP RG and LA–ICP–MS U–Pb, zircon SHRIMP SI oxygen and LA–MC–ICP–MS Hf isotope, and whole-rock Nd–O isotope analyses from the Archean granitoids in northern Liaoning, North China Craton. On the basis of zircon U–Pb isotopic dating and measured geological section investigation, two distinct magmatic suites as enclaves in the Jurassic granites are recognized, viz. a newly discovered 3.0 Ga crustal remnant and a 2.5 Ga granitoid. The Mesoarchean zircons from the 3.0 Ga granodioritic gneisses exhibit heterogeneous Hf isotopic compositions, with the most radiogenic analysis (εHf(t) = +3.8) following the depleted mantle evolution array and the most unradiogenic εHf(t) extending down to −3.4. This implies that both ancient continental crust at least as old as 3.4 Ga and depleted mantle contributed to the magma source of the protoliths of the Mesoarchean gneisses. The εHf(t) values of the Neoarchean zircons from these gneisses overlap the 3.4–3.0 Ga zircon evolution trend, indicating that the ancient crustal materials have been reworked during the late Neoarchean. The Neoarchean zircons from the 2.5 Ga granitoids have a relatively small variation in the Hf isotope and are mainly plotted in the 3.0–2.8 Ga zircon evolution field. However, taking all the εHf(t) values of the Neoarchean zircons into the consideration, we find that the Hf model age of the Neoarchean zircon does not represent the time of crustal growth or reworking but are artifacts of magma mixing. The interaction between the magmas derived from the ancient crustal materials and the depleted mantle is also supported by zircon O isotopic data and Hf–O isotopic modeling of the Neoarchean granitoids. Both Mesoarchean and late Neoarchean tectonothermal events involved synchronous crustal growth and reworking, which may be applicable to other parts of the world.  相似文献   

19.
We present results of study of the trace-element and Lu–Hf isotope compositions of zircons from Paleoproterozoic high-grade metasedimentary rocks (paragneisses) of the southwestern margin of the Siberian craton (Irkut terrane of the Sharyzhalgai uplift). Metamorphic zircons are represented by rims and multifaceted crystals dated at ~ 1.85 Ga. They are depleted in either LREE or HREE as a result of subsolidus recrystallization and/or synchronous formation with REE-concentrating garnet or monazite. In contrast to the metamorphic zircons, the detrital cores are enriched in HREE and have high (Lu/Gd)n ratios, which is typical of igneous zircon. The weak positive correlation between 176Lu/177Hf and 176Hf/177Hf in the zircon cores evidences that their Hf isotope composition evolved through radioactive decay in Hf = the closed system. Therefore, the isotope parameters of these zircons can give an insight into the provenance of metasedimentary rocks. The Paleoproterozoic detrital zircon cores from paragneisses, dated at ~ 2.3–2.4 and 2.0–1.95 Ga, are characterized by a wide range of εHf values (from + 9.8 to –3.3) and model age T C 2.8–2.0 Ga. The provenance of these detrital zircons included both rocks with juvenile isotope Hf parameters and rocks resulted from the recycling of the Archean crust with a varying contribution of juvenile material. Zircons with high positive εHf values were derived from the juvenile Paleoproterozoic crustal sources, whereas the lower εHf and higher T C values for zircons suggest the contribution of the Archean crustal source to the formation of their magmatic precursors. Thus, at the Paleoproterozoic stage of evolution of the southwestern margin of the Siberian craton, both crustal recycling and crustal growth through the contribution of juvenile material took place. On the southwestern margin of the Siberian craton, detrital zircons with ages of ~ 2.3–2.4 and 1.95–2.0 Ga are widespread in Paleoproterozoic paragneisses of the Irkut and Angara–Kan terranes and in terrigenous rocks of the Urik–Iya graben, which argues for their common and, most likely, proximal provenances. In the time of metamorphism (1.88–1.85 Ga), the age of Paleoproterozoic detrital zircons (2.4–2.0 Ga), and their Lu–Hf isotope composition (εHf values ranging from positive to negative values) the paragneisses of the southwestern margin of the Siberian craton are similar to the metasedimentary rocks of the Paleoproterozoic orogenic belts of the North China Craton. In the above two regions, the sources of detrital zircons formed by both the reworking of the Archean crust and the contribution of juvenile material, which is evidence for the crustal growth in the period 2.4–2.0 Ga.  相似文献   

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