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1.
刘淑娟 《河北地质》2007,(4):21-22,27
西石门-李家庄金矿区位于河北省灵寿县西北部山区,产于山西断隆五台台拱阜平穹褶束Ⅳ级构造单元中,区内出露地层为太古界阜平群团泊口组,以片麻岩为主,矿体赋存于太古界阜平群团泊口组片麻岩、二长浅粒岩等的石英脉及蚀变岩中。  相似文献   

2.
关鸿  徐平 《岩石学报》1998,14(4):460-470
利用激光探针等离子体质谱方法研究了阜平杂岩中几种不同类型片麻岩中的锆石样品。实验结果显示,对于较简单的锆石群,其207Pb-206Pb数据分布的峰值年龄给出与常规锆石铅的TIMS方法一致的结果;通过分析大量的锆石颗粒,可以弥补TIMS方法分析数据较少的缺陷,从而给出更全面的年龄分布特征。对于具有多期混合的锆石,以及具有继承铅、多期增生历史的锆石,通过对一个样品中多个颗粒的分析以及对单个颗粒的不同位置的分析,可区分出不同期次地质事件的信息,从而为阜平杂岩的形成、变质演化历史提供了年代学依据。研究结果为阜平杂岩中大量发育的灰片麻岩给出约2.5Ga的岩浆活动年龄信息,出露面积较小的角闪斜长片麻岩给出了约2.7Ga的年龄信息,同时还给出了约2.2Ga和约1.9Ga的两期变质事件年龄信息  相似文献   

3.
太行山太古代阜平群中刚玉矽线石型矿床,产于太古界阜平群地层中,矿体顶板围岩是长英质片麻岩.长英质片麻岩系流纹岩的变质岩.刚玉矽线石矿体系沉积变质而成.局部地段刚玉产出,除与原岩铝过饱和程度有关外,并与混合岩过程中钾交代作用有明显关系.含矿岩系的变质强度达到了矽线石角闪岩亚相.  相似文献   

4.
阜平地区位于河北省西部,太行山脉的中段。该处出露的岩层主要是太古宙阜平群。1963年马杏垣教授等在太古宙变质杂岩体构造特征的重要阐述中,曾指出阜平是一个片麻岩穹窿。1965年马杏垣等又对中国东部区域变质作用早于24亿年前后的变质岩系的构造变动类型及形成条件进行了广泛的讨论。其中对阜平穹窿作了专门的阐述。以后,河  相似文献   

5.
<正>1研究区地质概况研究区大地构造位置属华北地台山西台背斜太行隆起带东侧的阜平隆起区,出露地层为太古宙阜平群中、高级变质岩系,是华北地台变质结晶基底的一部分,岩性主要为黑云斜长片麻岩、斜长角闪岩、角闪斜长片麻岩、含矽线石的钾长浅粒岩、大理岩等。其上为元古宇至侏罗系及新生界的盖层。区内构造比较发育,主要为震旦纪阜平造山运动SN方向的挤压应力形成的近EW向展布复向斜、复背斜,一系列与褶  相似文献   

6.
位于华北克拉通中部造山带的阜平杂岩是研究华北克拉通演化历史的理想对象之一。阜平杂岩由一系列高角闪岩相至麻粒岩相变质和多期强烈变形的岩石组成,包括灰色片麻岩、麻粒岩、角闪岩、细粒片麻岩和大理岩,可以分为四个岩性单元:阜平灰色片麻岩、龙泉关眼球状片麻岩、湾子表壳岩和南营花岗片麻。本研究分析了大约200颗来自湾子表壳岩中碎屑锆石的U-Pb年龄和Hf同位素组成。其中锆石变质增生边给出1.82~1.84Ga,对应华北克拉通的最终拼合事件。除了小部分继承锆石具有2.5Ga到2.9Ga的继承年龄外,大部分岩浆锆石给出2.10Ga和2.51Ga两组年龄。这些结果表明湾子表壳岩来源于2.5Ga的阜平TTG片麻岩和2.0~2.1Ga的南营花岗片麻岩,沉积年龄在1.84~2.10Ga之间。所有年龄在2.51Ga的锆石都具有正的εHf初始值( 1.4~ 10.9),指示了一个重要的地壳增生事件发生在2.5Ga,大量的新生岩浆从亏损地幔涌入地壳中。Hf同位素数据还表明年龄在2.8Ga岩石是源区下地壳的重要组成部分,这跟东部陆块的Nd同位素组成相一致。年龄在2.1Ga的岩石εHf初始值为-4.9到 6.1,本文解释为其形成于先成地壳的再...  相似文献   

7.
吕鹏  曲永贵 《吉林地质》1999,18(1):32-38
大山片麻岩的原财为奥长化岗石,呈不规则状侵入柳树河子片麻岩中,年龄27亿年左右,太古代阜平运动晚期侵位的。侵位与当时区域上大规模的韧性剪切作用密切相关。由于剪切带各相关位置的位移量的差异,形成空间,给岩浆被动就位了有利场所,形成大山片麻岩古深成岩体。  相似文献   

8.
五台山早元古代碰撞造山带初步认识   总被引:36,自引:5,他引:36       下载免费PDF全文
五台山地区分布着复杂的变质杂岩。过去人们把这些变质岩作为地层分成群组段。龙泉关剪切构造岩的发现突破了这种传统观念。野外工作中发现所谓五台群主要包含了三个蛇绿混杂带;阜平群和恒山群的主要成分是灰片麻岩,它们构成两个太古代陆块的基底。五台地区的花岗岩类由代表弧环境的双花岗岩带的I型和S型花岗岩组成,它们与变质的钙碱性火山岩代表了古代的岩浆弧。滹沱群的豆村和东冶亚群以及过去划入阜平群和五台群的某些变沉积岩是阜平陆块被动大陆边缘的沉积。滹沱群的郭家寨亚群则是前陆盆地的磨拉石沉积。因此可以认为,这是一个由恒山仰冲陆块、北台-车厂弧和阜平俯冲陆块构成的碰撞造山带,碰撞时间大致是距今2050Ma。闭合的弧前大洋和弧后盆地形成了三条蛇绿混杂带。  相似文献   

9.
阜平(超)群是华北克拉通中段变质基底的代表性“地层”。阜平柳树黑云斜长片麻岩常规微量锆石U-pb法(2800-150^+230)Ma的年龄,既是阜平(超)群底部可能为中太古代、也是华北克拉通变质基底为一统太古宙的主要年龄依据。然而,阜平(超)群传统的地层、年龄和性质一直不断地受到后续研究者质疑,现已为许多文献证实不是有序的群级地层而是中-下地壳性质的杂岩。阜平杂岩种类繁多,除了一些学者提出的构造成  相似文献   

10.
本文收集了阜平杂岩新太古代早期-古元古代晚期基底岩石的岩石地球化学、锆石U-Pb年代学、同位素地球化学和变质作用资料,以期对阜平杂岩早寒武纪演化历史进行初步总结.阜平新太古代早期~2.7 Ga片麻岩原岩为英云闪长岩,具有TTG质片麻岩的地球化学特征;其锆石εHf(t)具有较高的正值(+5.44~+7.50),单阶段模式年龄为2 745~2 824 Ma,表明新太古代早期为阜平杂岩强烈的地壳生长时期.新太古代晚期片麻岩的时代集中于2 543~2 484 Ma,主要岩石类型为英云闪长岩-奥长花岗岩-花岗闪长岩(TTG),同时区域内还存在二长花岗岩.TTG质片麻岩的εNd(t)值为-1.64~+0.96,单阶段模式年龄为2.76~3.04 Ga;锆石εHf(t)值为-1.9~+7.91,单阶段和两阶段模式年龄分别为2 546~2 888 Ma和2 548~3 119 Ma.这些TTG岩石主要为新太古代早期岩石的部分熔融,并有少量中太古代地壳物质参与.近于同期具有岛弧性质的辉长岩和变质作用暗示阜平杂岩新太古代晚期可能经历了俯冲和弧-陆或陆-陆碰撞.古元古代中期(2.1~2.0 Ga)阜平地区花岗质岩浆活动强烈.该阶段花岗岩具有A型花岗岩特征,与同期的火山-沉积岩系形成于华北克拉通古元古代中期伸展的陆内裂谷环境中.阜平杂岩中基性麻粒岩包体记录的变质作用时代为1.89~1.85 Ga,并具有顺时针演化的P-T轨迹,其代表了古元古代晚期裂谷闭合的陆内造山过程,表明华北最终克拉通化.   相似文献   

11.
Abstract Grey gneisses are tonalitic intrusive rocks that have Archaean characteristics and tectonic significance. Archaean grey gneisses in North China may be classified into two types: the Zunhua type and the Hengshan type. Grey gneisses of the Zunhua type alternate with basic granulites, forming a bimodal migmatitic suite. The rock is characterized by complex mineral composition, highly varied REE patterns and positive Eu anomaly and originated from autochthonous or partly autochthonous deep - level migmatization with a high degree (30% ±) of fusion. As the sub - stratum in the root of the early - stage high - grade greenstone belt, they prevented basic rocks from sinking. Grey gneisses of the Hengshan type are characterized by a relatively distinct intrusion form, large - amplitude upward emplacement, rather simple mineral composition, only slight changes of REE patterns and absence of Eu anomaly. The rock is a product of subduction and underthrusting of the high - grade greenstone belt and then fusion and emplacement with a low degree (15% ±) of fusion. In this paper an attempt is made to furnish important information about palaeoplate tectonics and early crustal evolution by means of a study of grey gneisses.  相似文献   

12.
塔里木巴楚小海子正长岩杂岩体的岩石成因探讨   总被引:6,自引:4,他引:2  
位荀  徐义刚 《岩石学报》2011,27(10):2984-3004
巴楚小海子正长岩杂岩体是二叠纪塔里木大火成岩省的重要组成部分.SIMS锆石U-Pb定年显示其形成于279.7±2.0Ma,与本区辉绿岩脉和石英正长斑岩岩脉近于同时侵位.根据矿物学特征,小海子正长岩体可分为铁橄榄石正长岩和角闪正长岩两类.前者主要由碱性长石、铁橄榄石、单斜辉石、角闪石和少量石英、斜长石组成,后者主要由碱性长石、角闪石、黑云母和少量的石英、斜长石组成.小海子正长岩体为铁质、碱性系列,轻稀土相对富集,重稀土亏损,具有明显的Eu正异常,无Nb、Ta负异常,相对低的(87Sr/86Sr);(0.7033 ~0.7038)和正的εNd(t)值(+3.1~+3.8),暗示它们来自亏损的地幔源区,没有地壳物质的加入.主微量和同位素地球化学分析,暗示巴楚小海子正长岩的母岩浆为碱性的幔源玄武质岩浆经橄榄石、单斜辉石分离结晶后的残余熔体,并且含有堆晶的碱性长石.这种含有碱性长石堆晶的熔体,在相对还原的条件下结晶,形成铁橄榄石正长岩;在相对氧化的条件下结晶,并经过不同程度斜长石的分离结晶形成角闪正长岩.  相似文献   

13.
英云闪长岩-奥长花岗岩和花岗闪长岩(简称TTG)是太古宙高级变质地体的主要物质组成,对深入理解早期大陆生长及其机制具有重要的科学意义。目前,人们对其成因过程与机制仍有不同认识。本文以怀安陆块中广泛分布的TTG片麻岩为例,探讨其成因演化和机制。研究区位于华北克拉通中北部,主要由新太古代英云闪长岩及少量奥长花岗岩、花岗闪长岩组成。我们从该区识别出富硅富重稀土和负铕异常的低铝奥长花岗质片麻岩,形成时代与广泛分布的高铝TTG质片麻岩一致(锆石SHRIMP U-Pb年龄2.53Ga)。岩石地球化学数据显示,低铝奥长花岗质片麻岩的主量元素具有富SiO 2(76%~79%),低Al2O3(11.01%~12.61%)、CaO(1.27%~1.59%)、MgO(0.74%~0.24%)和Mg#(18~53)等特征,而广泛分布的高铝TTG岩系的主量元素含量变化大,例如,SiO 2=63%~77%、Al2O3=13.2%~17.77%、CaO=1.8%~5.78%、MgO=0.18%~3.84%和Mg#=35~64。微量元素方面,低铝奥长花岗质片麻岩具有Eu/Eu*负异常(除1个样品为弱正异常1.38外,其余样品分布在0.59~0.44),富集重稀土((La/Yb)N=4~7,(Gd/Yb)N=0.36~1.27),而高铝TTG岩系从弱负铕异常到正异常(Eu/Eu*=0.8~5.35),轻重稀土分馏明显((La/Yb)N=10~103、(Gd/Yb)N=1.97~5.72)。在微量蛛网图中二者的区别除重稀土明显存在区别外,低铝奥长花岗质片麻岩显示出Ba、Sr的相对亏损,而高铝TTG岩系则相反。二者Lu/Hf比值差异明显,低铝奥长花岗质片麻岩变化在0.1~0.16,而高铝TTG岩系变化在0.01~0.07。在Lu/Hf与相关元素以及SiO 2与相关元素哈克图解中,二者差异更加明显,表明它们之间不存在直接的成因联系。综合锆石U-Pb、Lu-Hf同位素特征以及岩石地球化学特征,我们认为低铝奥长花岗质片麻岩是低压下由新太古代新生基性地壳物质低程度部分熔融而成,源区残留矿物相以辉石+斜长石为主,岩浆可能存在过独居石的分异作用。高铝TTG岩系主要由新生基性地壳在相对高压下部分熔融而成,源区残留相以石榴石+辉石+角闪石以及无或少量斜长石为特征。岩浆经历过角闪石和辉石分离结晶作用,铕正异常增大的现象可能与斜长石堆晶有关。本区同时形成高铝和低铝TTG岩系的机制还需深入研究。俯冲机制、地幔柱机制以及二者共同作用等机制均能解释TTG的成因。依据本区同期还形成大量辉长质-闪长质岩浆和稍晚(2.5~2.45Ga)形成的钾质花岗岩类岩浆的侵入活动,我们认为本区高铝和低铝TTG岩系分别来自底侵作用导致的下地壳不同深度不同程度的部分熔融有关。引起底侵作用的机制可能与地幔柱或地幔柱与板块俯冲共同作用有关。  相似文献   

14.
阜平杂岩中的浅色体主要分为2种类型,早期浅色体基本沿片麻理分布,较富钾长石(微斜长石)、石英,贫斜长石,形成于低水深熔或压溶条件下,水含量较低,局部脱水但尚未达到整体脱水的程度;晚期浅色体切割现有的片麻理,较富斜长石、石英,贫钾长石,形成于有水熔融条件下,平阳奥长花岗岩的出现即与晚期浅色体相对应。南营片麻岩、南营浅色花岗片麻岩的地球化学性质与其他片麻岩具有明显的不一致性。浅色体的稀土元素配分型式较复杂,根据对元素相对富集或亏损的分析得知,大多数浅色体的形成受围岩成分的控制,从早期浅色体向晚期浅色体发展,稀土元素含量向LREE相对亏损、HREE相对富集的方向转化,某些微量元素有明显的继承性。与地球化学特征相比,矿物组合的确定对浅色体阶段的归属判定更为重要。阜平杂岩变质演化不是简单的进变质脱水反应,其水分含量的变化十分复杂,对其深入研究有助于更好地了解该区地质和构造的演化过程。  相似文献   

15.
阜平地区麻粒岩的P—T路径研究   总被引:3,自引:0,他引:3  
阜平麻粒岩分布于阜平大柳树和坊时一带的原阜平超群下亚群索家庄组花岗质片麻碉中,以不同规模的透镜体,似层状体产出。麻粒岩主要由石榴石、单斜辉石、斜方辉石、角闪石和斜长石等矿物组成,含有少量的石英。根据岩石的矿物组合和结构特征可将其变质作用演化上个阶段;①石榴石中的角闪石、斜长石、单斜辉石等变质矿物包体代表峰前阶段;②粗粒平衡共生的角闪石、单斜辉石、石榴石、斜长石±紫苏辉石±石英等代表了峰期变质阶段;③ 石榴石变斑晶后生合品反应边中外侧细粒斜方辉石、斜长石和石英集合体代表了峰后变质阶段;④ 后生合晶反应边中内侧角闪石、斜长石等,代表了晚期退化变质阶段。这四个变质阶段演化的P-T条件依次为:峰前阶段636℃、0.824GPa.峰期阶段751℃~ 833℃、0.854~ 1.085GPa,峰后阶段670℃~ 740℃、 0.55~0.70GPa,退化变质阶段665℃、0.727GPa.构成了一条顺时针的P-T路径,反映了该变质区从早期褶皱增厚到晚期构造抬升的地质动力学过程。  相似文献   

16.
工作中重点对河北平山小觉地区阜平岩群两类角闪质岩石深熔作用的地球化学进行了研究。一类为厚层状斜长角闪岩,相邻新生浅色体常量元素组成上向TTG花岗质岩石方向转化,稀土和高场强元素含量明显降低,轻重稀土分离程度增高,tDM减小,εNd(t0)增大。另一类为与黑云变粒岩-片麻岩互层的条带状、石香肠状斜长角闪岩,相邻新生浅色体与之存在不同的地球化学关系:(1)稀土总量相对增高,轻重稀土分离程度有所降低;(2)稀土总量和轻重稀土分离程度都有明显增高。后者Nd同位素组成与斜长角闪岩也存在很大区别。这些现象可用熔融母岩、形成条件等差异得到合理的解释。  相似文献   

17.
The Garland Peak Syenite (GPS) of the Red Hill complex, New Hampshire, consists predominantly of amphibole, oligoclase, perthite, and quartz; amphiboles have homogeneous kaersutite cores with strongly zoned rims ranging in composition from pargasite to hastingsite to hornblende. The thin section scale association of kaersutite, an amphibole that typically crystallizes in silica-undersaturated magmas, with quartz suggests that the GPS magma experienced substanital changes in magmatic composition, including silica activity, during its crystallization history. Kaersutite-bearing camptonites are also associated with the Red Hill complex. The camptonite amphiboles are very similar in composition to the core kaersutites in the GPS, suggesting that the earliest GPS liquid may have had camptonitic affinities. In order to elucidate the process where-by silica-undersaturated magmas differentiate to saturation, amphiboles in these rocks were analyzed by electron and ion microprobe techniques. Amphiboles show a progressive increase in REE abundances from the camptonites to the GPS kaersutite cores to the GPS pargasite/hastingsite/hornblende rims. The systematic change in REE concentrations, and the variations in V, Ti, Sr versus Zr, Eu/Eu0 and La/Yb versus Ce, suggest a possible differentiation relationship for the amphiboles and imply that the GPS was derived from magmas similar to camptonites. Rimward depletions in Sr, Ti, V, and Eu/Eu0, and the increase in La/Yb values suggest that parental camptonites fractionated plagioclase, magnetite, and amphibole to produce the silica-oversaturated GPS. Bulk-rock modelling agrees with the trace element record preserved in the amphiboles, that plagioclase, magnetite, and amphibole fractionation caused silica saturation. Minor pegmatitic patches occur in the GPS. Ferrohornblendes in the pegmatites have REE abundances distinct from the other GPS amphiboles, and this difference may be due to open system processes.  相似文献   

18.
The Chakradharpur Granite—Gneiss complex (CKPG) is exposed as an elliptical body within the arcuate metamorphic belt sandwiched between the Singhbhum Granite in the south and the Chotonagpur Granite—Gneiss to the north. It consists of an older bimodal suite of grey gneiss and amphibolites, intruded by a younger unit of pegmatitic granite. The bimodal suite represents the basement to the enveloping metasediments.The average major-element chemistry of the grey gneiss conforms to the definition of trondhjemite and includes both low-Al2O3 and high-Al2O3 types. The amphibolites can be grouped into a low-MgO and a high-MgO type. Rocks of the younger unit range in composition from granodiorite to quartz monzonite. The two granitic units also differ significantly in their Rb, Sr and Ba contents, and in the REE distribution pattern. The grey gneiss shows a highly fractionated REE pattern and a distinct positive Eu anomaly, with Eu/Eu* values increasing with increase in SiO2 %. In samples of the younger granite, the REE pattern is less fractionated, with higher HREE abundance relative to the grey gneiss and usually shows a negative Eu anomaly. The two types of REE patterns in amphibolites are interpreted to represent the two broad groups identified on the basis of major element chemistry.On the basis of chemical data, a two-stage partial melting model for the genesis of grey gneiss is suggested, involving separation of hornblende and varying amounts of plagioclase in the residual phase. Varying amounts of plagioclase in the residuum result in the wide range of Al2O3 content of the partial melt from which the trondhjemites crystallised. Residual hornblende produces the highly fractionated REE pattern, but a relatively higher HREE content of the trondhjemites compared to those produced by separation of garnet in the residual phase. The high level of Ba together with moderate levels of Sr in the trondhjemites can also be explained by plagioclase in the residue, whose effectiveness in partitioning Ba compared to Sr is lower. Of the two groups of amphibolites, the low-MgO type shows relative depletion of LREE compared to the high-MgO type. It contains varying amounts of plagioclase and is tentatively suggested to represent the residue. The other group, with a slightly fractionated REE pattern (CeN/ YbN = 2.01), is generally considered to represent the source material for the trondhjemites. This may have been generated by 5–15% partial melting of mantle peridotites, containing higher concentrations of LIL elements than those which produced average Precambrian tholeiites. This first phase of partial melting resulted in the slightly fractionated REE pattern of these amphibolites. Derivation of the younger granitic unit from the trondhjemites can be ruled out on the basis of REE data alone. REE data suggest partial melting of metasediments to be the origin of these rocks. It is also possible that deeply buried volcanic rocks, similar to calc-alkaline components of greenstone belts, are the parent for this component.  相似文献   

19.
华北克拉通中部造山带南段崤山地区太华群变质杂岩中的TTG质片麻岩具较宽范围的Si O2(63.00%~73.13%)、Al2O3(14.22%~19.38%)和较低的Mg O(0.42%~1.62%)、Cr(4.7~19.2μg/g)和Ni(2.28~16.3μg/g),显示低Yb(0.54~1.16μg/g)、Y(5.49~11.6μg/g)以及高(La/Yb)N(22.4~47.7)和Sr/Y(12.4~84.3)的特征。其稀土元素配分曲线具明显Eu负异常,在微量元素蛛网图上显示显著的Nb-Ta、Ti负异常。崤山TTG片麻岩的原岩形成于新太古代晚期(~2.52 Ga)的加厚下地壳部分熔融,源区残留石榴子石及角闪石,斜长石结晶分异作用降低了岩浆体系的Sr含量和Sr/Y值。绝大部分继承锆石的形成时代(2544±8 Ma)接近于TTG岩浆结晶年龄,表明加厚下地壳源区物质组成相对较年轻。另外,崤山TTG质片麻岩具有正的岩浆锆石εHf(t)值(0.39~4.76)以及略低的继承锆石εHf(t)值(-1.88~3.05),与登封群新太古代TTG相似,均明显高于鲁山太华群新太古代早期TTG。因此,崤山TTG片麻岩具有明显的新生地壳组分,暗示了显著的地壳生长,可能与华北克拉通中部造山带南段新太古代活动大陆边缘增生造山过程相关。  相似文献   

20.
Rare earth element (REE) concentrations have been determined (by the INAA method) for the c. 2,800 m.y. old Nûk gneisses from the Buksefjorden region, southern West Greenland. Samples include dioritic to granodioritic gneisses and synplutonic mafic dykes; a Malene metagabbro and Qôrqut granite were analysed for comparisons.The early Nûk gneisses, diorites and tonalites, have mildly fractionated REE patterns which are interpreted as resulting from partial melting of garnetbearing amphibolite or granulite. Early Nûk trondhjemitic gneisses possess downward convex patterns with prominent positive Eu anomalies; they may be related to the diorites and tonalites by the separation of hornblende in a residue of partial melting or fractional crystallization. Most of the later Nûk grey gneisses have extremely fractionated linear patterns which were derived from a source very rich in garnet, possibly eclogite. REE patterns measured in the late Nûk Ilivertalik granite complex are mildly fractionated but with a high overall abundance consistent with an origin by partial melting of mafic lower crustal material. Two sets of synplutonic mafic dykes have strongly fractionated patterns similar to those found in alkali basalts.The geochemical variations suggest that the igneous precursors of the Nûk gneisses were not cogenetic, but were derived from widely differing sources.  相似文献   

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