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1.
新疆西准噶尔克拉玛依岩体以及周围地层中存在着大量暗色闪长玢岩岩墙,是岩浆物质贯入3组走向不同的裂隙形成的。对其中一个闪长玢岩岩墙样品进行锆石LA-ICP-MS年代学测试,得到303.1±1.2Ma的锆石206Pb/238U加权平均年龄,对从该闪长玢岩中分离出的角闪石进行Ar-Ar年代学测试,得到312.1±2.8Ma的坪年龄(1120~1400℃)和313.6±6.9Ma的反等时线年龄。对该闪长玢岩岩墙附近的含角闪石黑云母二长花岗岩进行的锆石LA-ICP-MS年代学测试,获得其206Pb/238U加权平均年龄为319.0±1.0Ma。对侵入石炭纪地层的一个花岗斑岩岩脉样品进行锆石LA-ICP-MS年代学测试,得到了315.3±1.0Ma的206Pb/238U加权平均年龄。上述年代学测试结果表明克拉玛依市以西地区的暗色岩墙形成时代是石炭纪末期,不是前人所说的二叠纪。在这些岩墙形成之前,该区在石炭纪晚期还发育以克拉玛依岩体及附近酸性岩脉为代表的花岗质岩浆活动。上述围岩和岩墙的年代学资料揭示出该区闪长玢岩岩墙所占据的裂隙形成时代在315~303Ma之间,为新疆西准噶尔地区晚古生代地球动力学背景及岩浆活动的深入研究,提供了时间方面的约束。  相似文献   

2.
中亚造山带西部西准噶尔地区红山花岗岩体内部发育多期似岩墙状安山质暗色条带,LA-ICP-MS锆石U-Pb同位素定年和岩石化学与同位素分析表明,它们具有不同的形成年龄、相同的源区和相似的形成过程。其中,具有不规则状或环状形态的暗色条带,其锆石U-Pb年龄为319.1±2.9 Ma和313.3±2.4 Ma,远大于红山岩体花岗岩锆石结晶年龄(305~301Ma),可能是红山岩体侵位过程中所捕掳的围岩;具有线性展布特征的安山质暗色条带,其锆石U-Pb年龄为295±2Ma,形成于红山岩体侵位之后,构成伸展岩墙群。红山岩体中的安山质暗色条带和线状岩墙群具有相似的岩石化学组成,富SiO_2(56.48%~63.09%)、MgO(3.56%~6.31%),具有高的Mg#值(51.74~62.40)及Na_2O/K_2O值(1.34~3.43);球粒陨石标准化稀土元素(REE)配分模式呈明显的右倾型,富集轻稀土元素(LREE)和大离子亲石元素(LILE)Rb、K、Ba、U、Sr,亏损高场强元素(HFSE)Th、Nb、Ce、P和重稀土元素,具较弱的负铕异常;其同位素组成特征为(~(87 )Sr/~(86 )Sr)i=0.703295~0.703620,(~(143) Nd/~(144) Nd)i=0.512612~0.512618,εNd(t)=6.91~7.62,(~(206) Pb/~(204) Pb)t为17.6883~17.9876,(~(207) Pb/~(204) Pb)t为15.5313~15.5686,(~(208)Pb/~(204)Pb)t为37.4460~38.0581。它们具有与赞岐岩类似的地球化学特征,总体表现出与弧岩浆作用相关的地球化学特征,可能具有共同的物质来源,为准噶尔洋板片俯冲消减后同一地幔源区在不同阶段的产物。其中,形成于弧岩浆作用时期的赞岐岩(319~313 Ma),构成与岛弧花岗岩类伴生的环状似岩墙状安山质暗色条带;形成于后造山伸展岩浆作用晚期的赞岐岩(~295Ma),构成与达拉布特左行走滑作用相关的陆内伸展岩墙群。安山质暗色条带(岛弧火山作用)、红山岩体(后造山伸展)和线状岩墙群(陆内伸展)记录了西准噶尔红山地区洋陆转换的全过程。  相似文献   

3.
基性岩墙群对探讨岩石圈伸展过程、时空演化及深部动力学等方面具有重要意义。为了厘定东准噶尔琼河坝地区岩墙群的形成时代、源区地幔性质、成岩构造背景、岩石成因及其与区域上的其他岩浆作用的成因关系,揭示东准噶尔古生代的地球动力学背景,对侵入到绿石沟岩体花岗岩中的暗色岩墙群进行了遥感卫星影像解译,并从野外地质、岩石学、矿物学、年代学、锆石Hf-O同位素和地球化学等方面进行了系统研究。绿石沟岩体中岩墙存在闪长玢岩和辉绿玢岩岩墙的岩石组合,它们的锆石LA-ICP-MS和SHRIMP U-Pb定年结果表明,闪长玢岩、辉绿玢岩岩墙形成时代分别为346±1 Ma和~332 Ma。辉绿玢岩岩墙的锆石εHf(t)值为+10. 2~+15. 4,对应的二阶段Hf模式年龄为0. 35~0. 67 Ga,其锆石δ18O值主要变化范围为5. 00‰~6. 41‰。这些同位素特征表明其具有亏损地幔源区的物质组成。矿物学研究表明,辉绿玢岩岩墙中的角闪石为浅闪石、铁浅闪石,其结晶温度范围为896~984℃,压力为41~88 MPa,对应结晶深度约1. 54~3. 31 km;辉石为透辉石,辉石-熔体平衡时的岩浆温度为1 092~1 099℃,压力为500~630 MPa,推测形成辉绿玢岩辉石岩浆房的存储深度为16. 5~20. 8 km。东准噶尔琼河坝地区大量中基性岩墙构成的岩墙群可作为区域伸展构造的重要标志,结合前人对该区构造背景认识,认为琼河坝地区在早石炭世时可能处于后碰撞伸展拉张环境,这为探讨东准噶尔乃至中亚造山带西段的古生代的地球动力学环境演变提供了新依据。  相似文献   

4.
萨吾尔地区位于西准噶尔东北缘,广泛发育晚古生代中酸性侵入岩和火山岩以及少量基性侵入岩,这些岩浆岩的年代学研究对于限制西准噶尔地区石炭纪构造环境具有重要的意义。本文通过研究萨吾尔地区科克托别岩体的岩相学特征、锆石SHRIMP U-Pb年龄以及地球化学特征,探讨该岩体构造背景以及成因机制,为进一步论证西准噶尔地区石炭纪构造环境提供佐证。科克托别岩体包括中粗粒辉长岩、细粒辉长岩和闪长岩,在野外露头显示细粒辉长岩以脉状侵入中粗粒辉长岩中,细粒辉长岩中包裹有中粗粒辉长岩包体,中粗粒辉长岩与闪长岩之间呈渐变过渡接触关系,说明科克托别岩体是不同期次岩浆侵位形成的杂岩体,早期岩浆侵入形成中粗粒辉长岩和闪长岩,晚期岩浆上侵就位于中粗粒辉长岩构造裂隙中形成细粒辉长岩。科克托别岩体中细粒辉长岩锆石SHRIMP U-Pb年龄为323.2±6.2Ma,表明岩体形成于早石炭世晚期。该岩体成岩年龄晚于该地区蛇绿岩套岩石年龄,也晚于岛弧火山岩年龄以及含斑岩矿床侵入岩年龄,与该地区I型花岗岩年龄相似,而明显早于碰撞后A型花岗岩和双峰式火山岩的形成年龄,说明科克托别岩体可能形成于同碰撞构造环境中。不同岩相的岩石主量元素之间的相关关系以及微量元素配分型式相似性说明它们为同源岩浆结晶分异的产物。岩相学和地球化学特征表明岩体初始岩浆可能为软流圈地幔与上覆交代地幔相互作用形成,板片断离可能为软流圈地幔的上涌起到重要作用。  相似文献   

5.
新疆西准噶尔拉巴花岗岩地球化学特征及年代学研究   总被引:4,自引:0,他引:4  
新疆西准噶尔玛依勒地区的拉巴岩体侵入于下石炭统包古图组中,由花岗闪长岩、石英闪长岩、英云闪长岩、花岗岩组成,以花岗岩为主。其中花岗岩和花岗闪长岩属钙碱性、高钾钙碱性系列,为偏铝质至过铝质岩石,并具有轻稀土-大离子亲石元素富集、Nb-Ta-Ti等高场强元素亏损的地球化学特征。该岩体两个代表样品的锆石La-ICP-MS法206Pb/238U加权平均年龄分别为287±5Ma和295.1±2.3Ma,表明岩体的结晶年龄为早二叠世,与西准噶尔地区后碰撞花岗岩的时代(年龄峰值310~295Ma)相近。综合岩体的地质、地球化学特征和区域地质特征,认为拉巴花岗岩体为准噶尔地区后碰撞阶段伸展期的岩浆活动产物。  相似文献   

6.
老山口铁铜金矿区位于准噶尔北缘的喀拉通克—卡拉先格尔成矿带南段,矿化与岩浆侵入活动有关。本文利用LA-ICP-MS锆石U-Pb定年方法对老山口铁铜金矿区的中粒闪长岩、正长岩、黑云母闪长岩和闪长玢岩进行了年代学研究,获得其年龄分别为353.8±1.9Ma、366.3±1.9Ma、3±2.3Ma和379.7±3Ma,表明矿区存在三期岩浆活动。其中黑云母闪长岩和闪长玢岩的年龄,在误差范围内一致,它们可能为中泥盆世同源岩浆演化的产物,且岩体侵入时代与准噶尔洋俯冲阶段花岗岩及卡拉先格尔斑岩铜矿带含矿斑岩年龄较一致,表明其可能是板块俯冲阶段的产物。闪长岩和正长岩的年龄分别为353.8±1.9Ma和366.3±1.9Ma,与东准噶尔北部青格里河下游一带后碰撞花岗岩类和布尔根一带后造山伸展A型花岗岩的年龄接近,而地球化学特征却存在差异,说明老山口正长岩和闪长岩体是俯冲晚期阶段的产物。根据地质特征,老山口铁铜金矿的形成与闪长岩及闪长玢岩侵入有关,因此岩体年龄也限定了矿区存在两期铁铜金矿化,即379Ma左右和354Ma左右。  相似文献   

7.
西准噶尔萨尔托海花岗岩株锆石U-Pb年代学及地质意义   总被引:1,自引:0,他引:1  
新疆西准噶尔萨尔托海蛇绿岩与下石炭统呈逆冲断层接触,后被达尔布特走滑断层所改造,是西准噶尔地区时代最新、规模最大的蛇绿混杂岩带。萨尔托海岩株侵入于萨尔托海蛇绿混杂岩带之中,岩体岩性为肉红色二长花岗岩。对花岗岩样品进行测年,新获得LA-ICPMS锆石U-Pb年龄(309±3)Ma(2σ),代表了花岗岩结晶时代,较区域花岗岩基如庙尔沟、加甫萨尔苏等岩体的形成时代略老。综合蛇绿岩及区域岩体时代和岩石学特征等,认为该年龄限定了蛇绿岩侵位时代上限,揭示其属区域伸展背景的产物,标志着区域俯冲作用已经结束。因此,西准噶尔地区至少在309 Ma以后不存在俯冲作用,该认识有助于理解新疆北部多期次岩浆活动的时限和性质。  相似文献   

8.
对新疆西准噶尔南部地区与早古生代蛇绿岩紧密伴生的业姆奇花岗岩体岩石学、岩石地球化学、同位素年代学进行研究,认为业姆奇花岗岩为低钾(拉斑)系列,岩石地球化学特征具板内靠近岛弧区域特征。通过对二长花岗岩LA-ICP-MS锆石U-Pb测年,获得比较准确的年龄数据539.7±2.6Ma,表明其形成时代为早寒武世,该侵入岩作为西准噶尔地区最老的岩浆活动产物,代表了在诺丁尼亚统一大陆形成之后早期裂解阶段古洋盆初期的地质记录。  相似文献   

9.
纸房花岗岩体位于新疆东准噶尔卡拉麦里构造带北侧。该岩体侵入的最新地层为中—上奥陶统荒草坡群,并被晚志留世及早泥盆世地层不整合覆盖。对纸房花岗岩进行锆石SHRIMP U-Pb定年,获得的206Pb/238U加权平均年龄为(463±7)~(436±4)Ma,表明该岩体形成于晚奥陶世—早志留世,是早古生代岩浆活动的产物。对已有的区域地质资料、岩体侵位时代及其与围岩接触关系进行综合分析后认为,纸房花岗岩体的形成时代大致对应于卡拉麦里构造带内区域性角度不整合的形成时间,推测该岩体为早古生代造山过程中形成的花岗质岩石。高Sr、低Yb、弱的Eu负异常等地球化学特征也显示其为埃达克型同造山花岗岩。纸房地区早古生代同造山花岗岩的存在为东准噶尔卡拉麦里构造带早古生代造山作用的确认提供了证据。  相似文献   

10.
西准噶尔北部萨吾尔地区晚古生代火山岩浆作用强烈,其形成构造环境一直是争议的焦点。塔斯特岩体作为区内最重要的复式岩体,主要由辉长岩、花岗闪长岩、二长花岗岩和钾长花岗岩组成,对其中的辉长岩进行LA-ICP-MS锆石U-Pb定年,206Pb/238U年龄加权平均值为345.3±2.3Ma(MSWD=1.8),说明塔斯特岩体形成于早石炭世中期。岩石地球化学特征显示,样品里特曼指数δ平均值为3.04,A/CNK(0.76~0.85)1.1,属于准铝质钙碱性岩石,岩石富集大离子亲石元素,而高场强元素和重稀土元素相对亏损,无明显的Eu异常,与西准噶尔地区后碰撞花岗岩类地球化学特征相似。综合研究认为,该辉长岩形成于后碰撞构造环境,可能是后碰撞阶段挤压-伸展转变期的产物。塔斯特辉长岩年龄是目前西准噶尔地区最老的后碰撞岩浆岩锆石年龄,表明西准噶尔地区在早石炭世中期已处于后碰撞构造环境,为西准噶尔地区后碰撞构造-岩浆演化下限的厘定提供了新的证据。  相似文献   

11.
高精度LA-ICP-MS锆石U-Pb测年结果表明,黄羊山岩浆混合花岗岩加权平均~(206)Pb/~(238)U年龄为311±12Ma,首次获得闪长质微细粒包体加权平均~(206)Pb/~(238)U年龄为300±6Ma,在误差范围内完全一致,均属于晚石炭世,前者代表黄羊山岩浆混合花岗岩成岩年龄,后者代表暗色闪长质微粒包体的形成年龄,表明两者是同时代形成的,属于300Ma前后准噶尔周边地区后碰撞岩浆活动的产物.岩石地球化学研究表明,寄主岩石具有高硅、低铝、贫钙镁、富碱和高分异的特征,寄主岩石、包体和辉绿岩脉成分均落在了混合趋势线上,寄主岩富集Rb和Th等大离子亲石元素及Zr、Hf等高场强元素,亏损Ba、Sr、Ta和Ti等元素,δEu值(为0.01)极低,具有低的~(87)Sr/~(86)Sr初始比值和高正的ε_(Nd)(t)值.黄羊山碱性花岗岩是在后碰撞拉张的构造背景下,幔源岩浆发生底垫作用,由于幔源岩浆底垫作用,下地壳温度升高而熔融形成酸性壳源岩浆,部分幔源岩浆沿着地壳中的深断裂带上涌,发生不同程度壳幔混合形成的,其中闪长质微细粒包体就是基性的幔源岩浆和酸性的壳源岩浆不同程度的混合的记录者,研究区的辉绿岩脉是幔源岩浆直接分异演化的产物.  相似文献   

12.
东准噶尔卡拉麦里黄羊山花岗岩岩石成因探讨   总被引:3,自引:0,他引:3  
黄羊山花岗岩体是卡拉麦里造山带典型的后碰撞花岗岩体, 发育大量闪长质微细粒包体。黄羊山花岗岩具有高硅(72.21%~77.36%)、低铝(9.00%~12.93%)、贫钙镁(CaO: 0.20%~1.21%; MgO: 0.03%~0.44%)、富碱(Na2O+K2O: 7.43%~9.02%)以及高分异(SI=0.28~3.47, DI=76.45~95.99)的特征。强烈富集LILE和HFSE (Zr+ Nb+Ce+Y=260.01 μg/g~797.83 μg/g), Ga含量高(10000×Ga/Al=3.95~5.69), 属于A型花岗岩类。岩石学和岩相学(包体细粒淬冷边, 反向脉, 复合包体以及寄主岩石和包体中斜长石斑晶在形态、成分、光性上的一致性等)、岩石地球化学(Y/Nb=2.77~6.82, La/Nb=0.91~4.33, Ba/Nb=0.13~37.86等)、Sr和Nd同位素(ISr多数在0.7031~0.7041, εNd(t)在5.2~7.1之间)以及LA-ICP-MS锆石U-Pb测年(寄主岩石为311±12 Ma, 包体为300±6 Ma)综合研究显示, 黄羊山花岗岩是壳-幔源岩浆混合成因。从晚石炭世到二叠世, 东准噶尔地区进入后碰撞构造演化阶段, 在后碰撞构造阶段, 早期的俯冲板片断离, 软流圈减压熔融, 玄武质岩浆底侵至下地壳底部, 底侵基性岩浆带来的巨大热量, 导致地壳物质熔融, 形成大规模的花岗质岩浆, 两种岩浆发生了不同程度的混合, 其中闪长质微细粒包体就是基性的幔源岩浆和酸性的壳源岩浆不同程度混合的产物。  相似文献   

13.
周丽云  王瑜  王娜 《地质通报》2015,34(203):400-418
分布于中国东北完达山地区的饶河花岗岩岩体中暗色矿物和斑晶钾长石定向排列,呈北北东走向,其中透镜状闪长质捕掳体近水平排列,局部具有左行剪切的特点。岩体中发育石香肠状石英脉,表明岩体在侵位过程中受到左行剪切作用的影响或制约。对出露的花岗岩进行LA-ICP-MS锆石U-Pb定年,获得年龄121±1Ma和119±1Ma,表明该岩浆流动形成于早白垩世。同时对围岩辉长岩、侵入岩体中的正长岩脉和辉绿岩脉进行锆石U-Pb年龄分析,分别获得160±1Ma、109±2Ma、124±1Ma的年龄结果。根据各样品中继承锆石的特征,围岩辉长岩的年龄数据很集中,不存在古老锆石的年龄信息。岩浆流动岩体及岩脉中都有太古宙、元古宙等各时代的锆石年龄数据,可能表明完达山地区在约120Ma之前已完成古太平洋板块的俯冲拼贴,饶河岩体形成于走滑环境下的陆内变形,为同构造侵入岩。  相似文献   

14.
新疆东准噶尔地区地处阿尔泰、准噶尔和东天山等山系和构造单元的结合部位, 是研究中亚造山带(或称北亚造山区)构造演化的关键地区。以往的研究多集中于东准噶尔的岩石组合和地球化学组成, 相对缺乏构造变形尤其是中小尺度构造变形的研究。初步研究发现东准噶尔分布着大量的中基性暗色岩墙, 它们是后期岩浆侵入到前期构造裂隙中的产物, 可以从时空两个方面为构造裂隙的研究提供制约。本文结合地质资料和高分辨率遥感影像解译, 在琼河坝岛弧带中的和尔赛岩体(早泥盆世)中识别出来了874个暗色岩墙(晚石炭世-早二叠世)片段, 它们的走向以北西西-南东东向为主, 另外还有少数北东-南西和北西-南东走向的岩墙。通过岩墙的宏观变形特征可以推测, 北西西-南东东走向的岩墙形成于压张性裂隙之中, 北西-南东走向的岩墙形成于左行张剪裂隙之中, 北东-南西走向的岩墙形成于右行压剪裂隙之中。这些裂隙形成时平面最大主应力为北西西-南东东方向。结合岩体和岩墙的时代, 本文认为在晚泥盆世-早石炭世期间, 和尔赛岩体由于受到北西西-南东东方向的区域挤压作用而产生相应的裂隙, 可能标志着洋盆结束后碰撞作用的发生, 而晚石炭世-早二叠世暗色岩墙的普遍发育可能是后碰撞岩浆活动的标志。  相似文献   

15.
This work carried out systematic geological field investigation, petrography observation, zircon geochronology and whole rock geochemistry on Late Paleozoic intrusions in the Xingxingxia region near the Xinjiang-Gansu provincial boundary, western China, aiming to constrain the Late Paleozoic tectonic framework of the Xingxingxia region and the final closure time of South Tianshan Ocean in the East Tianshan. The Xingxingxia area is located in the east part of the Tianshan orogen, and adjacent to the north of the Tarim Basin. The Late Paleozoic magma activities in the Xingxingxia region can be mainly divided into three stages. The first stage includes intrusive magma activities under a collision setting between Late Ordovician to the Late Devonian. The second stage is intrusive magma activities under a subduction setting during(304±3)–(278±3) Ma, and the third stage involves intrusive magma activities under a collision and post-collision setting during(268±5)–(259.9±2.6) Ma. The final suture zone of South Tianshan Ocean should be between the Central Tianshan Block and South Tianshan accretionary complex. Based on previous work, both the first stage magma activities(i.e., intrusive magmatic activities between the Late Ordovician to Late Devonian) and the Hongliuhe ophiolitic complex indicate a close event between Central Tianshan Block and South Tianshan Accretionary Complex. The 304±3 Ma dioritic metamorphic gneiss of the XingX ingxia complex and the 278±3 Ma diorite are all island arc calc-alkaline rocks, the 289±3 Ma gabbro is island arc tholeiitic gabbro formed by magma from metasomatic enrichment mantle. All these results indicate that the second stage of magmatic activities is under a subduction setting. The third stage magma activities i.e. the granitic magma activities of(268±5)–(259.9±2.6) Ma occurred at a transitional setting from compressional to post-collision extensional tectonic setting. Thus, around(268±5)–(260±3) Ma, the final closure of the South Tianshan Ocean occurred and the Tianshan orogen shifted into the intracontinental evolution stage. During and after the closure process, a wide range of metamorphism and large dextral strike-slip faults developed.  相似文献   

16.
The Zhongchuan district is an important component of the metallogenic belt in the Western Qinling. The Zhongchuan granite pluton occurring in the centre of the Zhongchuan metallogenic area has been poorly constrained, though the Triassic granite in Western Qinling has been well documented. In‐situ zircon U–Pb ages, Hf isotopic compositions and whole‐rock geochemical data are presented for host granite and mafic microgranular enclaves (MMES) from the Zhongchuan pluton, in order to constrain its sources, petrogenesis and tectonic setting of the pluton. The distribution of major, trace and rare earth elements apparently reflect exchange between the MMES and the host granitic rocks mainly due to interactions between coeval felsic host magma and mafic magma. The zircon U–Pb age of host granite (231.6 ± 1.5 to 235.8 ± 2.3 Ma) has overlapping uncertainty with that of the MMES (236.6 ± 1.3 Ma), establishing that the mafic and felsic magmas were coeval. The Hf isotopic composition of the MMES (εHf(t) = −13.4 to 4.0) is distinct from the host granite (εHf(t) = −15.7 to 0.0), indicating that both enriched subcontinental lithosphere mantle (SCLM) and crustal sources contributed to their origin. The zircons have two‐stage Hf model ages of 1064 to 1798 Ma for the host granite and 858 to 1747 Ma for the MMES. This suggests that the granitic pluton was likely derived from partial melting of a Late Mesoproterozoic crust, with subsequent interaction with the SCLM‐derived mafic magmas in tectonic affinity to the South China Block. Copyright © 2012 John Wiley & Sons, Ltd.  相似文献   

17.
The Sausfjellet pluton is made up of two intrusive units emplaced into high-grade metamorphic rocks of the Helgeland Nappe Complex of the Uppermost Allochthon in the Norwegian Caledonides. The eastern part of the pluton intruded marble and less voluminous calc-silicate and pelitic rocks. The western half is hosted predominantly by semi-pelitic migmatite with intercalated marble. Remelting of the migmatite during pluton emplacement occurred in a thermal aureole as much as 1000 m wide. The early gabbroic unit forms the southeastern part of the body; it consists of hornblende-bearing to hornblende-rich gabbro and diorite which is thought to have crystallized from an H2O-rich andesitic parental magma. The younger dioritic unit underlies the central and western parts of the pluton, as well as a zone as much as 200 m wide that separates the rest of the pluton from its host rocks (herein the “annular zone”). The interior or central zone of the dioritic unit is pyroxene diorite that is locally interlayered with anorthosite. The western and annular zones are, by comparison, mineralogically heterogeneous. They range from diorite to quartz monzonite and from biotite-bearing two- and three-pyroxene assemblages to biotite–hornblende assemblages. Neither rock type nor mafic assemblage is correlated with position in the pluton or proximity to a contact. Stoped blocks of a distinctive coarse-grained diorite, as well as pyroxene-rich calc-silicates, are present in the gabbroic unit and the central zone of the dioritic unit. The few stoped blocks observed in the western zone of the dioritic unit are predominantly quartz-rich gneiss. Chemical variation in the central zone of the dioritic unit is interpreted to result from accumulation of pyroxenes+plagioclase from an H2O-poor andesitic parent. These rocks have approximately constant δ18O of +6.6±0.2‰ and lack evidence of in situ assimilation. Heterogeneities in the western and annular zones of the dioritic unit are reflected in variable, anomalously enriched incompatible element contents and in δ18O, which ranges from +6.7‰ to +8.6‰. Petrologic models indicate that the magma parental to the central zone could also be parental to the western and annular zones. If so, evolution of the western and annular zone magma was by crystal accumulation and assimilation of metapelitic host rocks. As much as 20% of the mass of the western and annular zones can be ascribed to assimilated material, which apparently entered the magma by stoping. Therefore, the asymmetrical zoning of the pluton is due to differences in host rock compositions and the relative ability of the magma to assimilate its host rocks.  相似文献   

18.
《Gondwana Research》2006,9(4):567-574
The Puttetti alkali syenite pluton in southern India belongs to the suite of felsic magmatic intrusives emplaced during the Late Neoprotrozoic-Cambrian time during the final phase of amalgamation of the Gondwana supercontinent. In this study, we evaluate the cooling history of this pluton based on various isotopic systems. We present whole-rock Pb-Pb data on the syenite which yields an isochron age of 508±25Ma. Three phlogopite separates from the syenite pluton give K-Ar ages of 454.0±9.0, 448.5±8.9 and 445.6±8.8 Ma indicating cooling age at temperatures of ∼415°C. U-Pb analyses of zircons from this syenite yielded an age of 572±2 Ma in a previous study. With U-Pb closure temperatures >800 o C, this age probably indicates the timing of emplacement of the Puttetti pluton. Collectively, we estimate from the isotopic age data and respective closure temperatures that the syenite body cooled at about 3.2 o C/Ma from about 800 o C to about 415 o C. The markedly low cooling rate of the syenite pluton, absence of chilled margin effects, and common occurrence of pyroxene, feldspar, phlogopite and zircons megacrysts in the rock indicate that the host granulites were at high temperatures during the emplacement of the syenite magma. The cooling history of Puttetti syenite estimated in this study is closely comparable with the 3–4 o C/Ma cooling rate estimated for a granite pluton in a previous study from Madagascar. Our study suggests protracted cooling rates for the late Pan-African intrusives emplaced within the Gondwana crust, with a long residence history in a hot crust bore they were exhumed to shallower levels.  相似文献   

19.
With aim of providing constraints on the Late Paleozoic tectonic evolution of the southern Central Asian Orogenic Belt(CAOB),an integrated study was conducted on the geochronological and geochemical data for dioritic,granitic and diabase dykes from the Aqishan-Yamansu belt in the eastern Tianshan,NW China.Zircon U-Pb dating indicates that the dioritic and granitic dykes were both emplaced in the Late Carboniferous(~311 Ma and^315 Ma).The dioritic dykes show adakitic characteristics and have high Na2 O and positiveεHf(t)values(+12 to+17),which suggest an origin from partial melts of a subducted oceanic slab.The granitic dykes have high SiO2 and K2 O contents and are characterized by en riched light rare earth elements(LREE)and slightly flat heavy rare earth elements(HREE),with negative Eu and Nb-Ta-Ti anomalies.These dykes are alkali-calcic and show geochemical features of highly fractionated Itype granites.Their positiveεHf(t)values(+16 to+17)suggest that they were derived from a juvenile accreted oceanic crustal sou rce.The coeval diabase dykes have low SiO2 and K2 O contents but high TiO2,MgO and Mg#(54-59).They are enriched in LREE and show characteristics of enriched mid-ocean ridge basalts(E-MORB).The relatively high Ba/Th,slightly low Th/Ta ratios,and negative Nb-Ta anomalies imply a mantle source metasomatised by slab-derived fluids.Thus,these basic dykes were generated likely by partial melting of the upwelling asthenosphere mantle with a slight influence of slab-derived fluids.Therefore,we suggest that the formation of these Late Carboniferous dykes were triggered by a post-collisional slab breakoff and the Aqishan-Yamansu belt was a continental arc formed by southdipping subduction of the Kangguer oceanic plate.  相似文献   

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