南秦岭佛坪地区麻粒岩相岩石锆石U—Pb年龄

对南秦岭佛坪地区麻粒岩相岩石中锆石的特征进行了详细的研究和U-Pb同位素年龄测定。中酸性麻粒岩中3个变质成因锆石的~(256)Pb/~(238)U表面年龄统计权重平均值(谐和年龄)为221.4±3.6Ma,是这些变质锆石较为准确的生成年龄;该样品4个锆石颗粒组成的不一致线上、下交点年龄分别为822±272Ma和218±14Ma;石榴夕线黑云片麻岩中4个锆石颗粒构成的不一致线的上下交点年龄分别为2283±162Ma和271±15Ma。两个样品的数据点均比较靠近下交点而远离上交点,其上交点年龄不具明确地质意义。综合各方面因素,认为麻粒岩相峰变质作用时代为印支期—海西晚期(220～270Ma左右),这是迄今为止秦岭地区所报道过的最年轻的麻粒岩地质体。     

南天山榆树沟麻粒岩相构造岩研究

榆树沟麻粒岩相构造岩宏观上呈糜棱岩带和糜棱岩化带产出,发育强烈流变叶理;微观上主要造岩矿物发育各种塑性变形显微构造。变形过程中同种造岩矿物的动态重结晶新晶与塑变残斑（残晶） 之间化学成分变化不明显, 表明在变形期间水活度低,以位错蠕变为主。该构造岩形成于深地壳麻粒岩相变质的晚期阶段,是地体在早期阶段于下地壳底部－上地幔顶部发生高压麻粒岩相变质作用后因构造抬升进入深地壳麻粒岩相环境下发生退变质和强烈韧性剪切变形的产物, 其形成后经历了快速的构造折返过程。     

"旧地重游",再次认识与评价:开拓铂族元素新资源的重要途径

简略介绍了几种在90年代报导或发现的工业铂族金属矿床,它们之中有一些是已知矿床重新认识和评价的新成果。     

冀西北石榴角闪二辉麻粒岩早期高压变质矿物组合的确定及其形成的温压条件——来自锆石中矿物包裹体的信息

采用激光拉曼、阴极发光和电子探针技术,确认冀西北石榴角闪二辉麻粒岩锆石中保存早期高压变质包体矿物组合:石榴石(Grt)+单斜辉石(Cpx)+斜长石(Pl)+石英(Qtz)+金红石(Rt)、单斜辉石(Cpx)+斜长石(Pl)+石英(Qtz)和石榴石(Grt)+单斜辉石(Cpx)+斜长石(Pl)+石英(Qtz)。其中少量锆石具有继承性锆石的核,而多数锆石则形成于高压麻粒岩相变质阶段。利用TWQ方法限定石榴角闪二辉麻粒岩锆石中所保存的高压包体矿物组合的变质温度条件为750～820℃,压力为1.07～1.40 GPa。该项研究成果对于如何识别高压麻粒岩以及深入研究其成因机制均具有重要的科学意义。     

Origin of 1.8 Ga zircons in Post Eocene mafic dikes in the Roshtkhar area,NE Iran

The Roshtkhar area is located in the Khaf-Kashmar-Bardaskan volcano-plutonic belt to the northeastern Iran along the regional E–W trending Dorouneh Fault, northeastern of the Lut Block. There are several outcrops of subvolcanic rocks occurring mainly as dikes in the area, which intruded into Cenozoic intrusive rocks. We present U–Pb dating of zircons from a diabase dike and syenite rock using LA-ICP-MS that yielded an age of 1778 ± 10 Ma for the dike, indicating this Cenozoic dike has zircon xenocrysts inherited from deeper sources; and 38.0 ± 0.5 Ma, indicating an Late Eocene crystallization age for the syenite. Geochemically, the dikes typical of high-K calc-alkaline to shoshonitic magmas. Petrographic observations and major and trace element variations suggest that diabase melts underwent variable fractionation of clinopyroxene, olivine, and Fe-Ti oxides and minor crustal contamination during the differentiation process. Primitive mantle-normalized multi-element diagrams display enrichment in LILE, such as Rb, Ba, Th, U, and Sr compared to HFSE, as well as negative anomalies of Nb, Ta, P, and Ti, suggesting derivation from subduction-modified mantle. Chondrite-normalized REE plots show moderately LREE enriched patterns (<3.83 La_N/Yb_N <8.27), and no significant Eu anomalies. Geochemical modelling using Sm/Yb versus La/Yb and La/Sm ratios suggests a low-degree of batch melting (~1–3%) of a phlogopite-spinel peridotite source to generate the mafic dikes. The geochemical signatures suggest that the Roshtkhar mafic dikes cannot be related directly to subduction and likely resulted from melting of upper mantle in an extensional setting where the heat flow was provided from deeper levels. These dikes presumably derived the zircon xenocrysts from the assimilation of upper crust of Gondwanian basement. Processes responsible for partial melting of metasomatized lithospheric mantle and post-collision magmatism in NE Iran was triggered by heating due to asthenospheric upwelling in an extensional setting.     

北大巴山花栎村镁铁质岩地球化学、年代学及其构造环境制约

北大巴山岚皋花栎村镁铁质岩为一套辉绿岩、辉长辉绿岩、辉绿玢岩和辉长岩组合,主要组成矿物为单斜辉石、长石,副矿物主要为铁钛氧化物等。镁铁质岩地球化学特征表现为高TiO_2(2.26%~7.30%)、TFe_2O_3(11.17%~17.0%)、较低的MgO(2.96%~5.52%)及较高的全碱含量(K_2O+Na_2O=3.07%~6.76%),属于典型的碱性辉长岩系列,Mg~#值(36~42)较高,表明岩体来源于高度演化的岩浆。微量元素特征显示富集大离子亲石元素Ba、Pb,稀土元素配分曲线显示明显的轻稀土元素富集特征(La_N/Yb_N=9.34~13.05),微量和稀土元素综合显示似洋岛玄武岩的地球化学特征。花栎村镁铁质岩LA-ICP-MS锆石年龄为436.9±2.4Ma,与相邻地区岩体形成年代一致,综合限定北大巴山地区岩浆活动时代为早志留世。岩体表现为EMⅠ、EMⅡ和少量HIMU的混和富集地幔源区特征及地幔柱源区特征,地幔动力学分析表明,早志留世或之前北大巴山地区可能存在一期与俯冲相关的弧后拉张作用导致下部岩浆上涌侵位,最终完成该区岩浆作用。     

闽东南基性岩脉形成的构造应力场地质意义

闽东南沿海地处长乐-南澳构造带内,发育晚中生代以来的基性岩脉(岩群),其几何形态和产状记录着区域应力场活动。通过对漳浦赤湖和东山海边基性岩脉的几何形态和产状的分析,推测长乐-南澳带在白垩纪为左旋韧性剪切带,古新世转变成左行脆性剪切带。长乐-南澳带的左旋走滑活动,是由古太平洋板块朝NW斜向俯冲引起的。晚白垩世以来,闽东南应力场性质为剪切与拉张相互变换,指示地壳拉张不是连续的,而是分期次;晚白垩世以来大洋板块属于低应力型俯冲,拉张是东南部主构造。     

Synplutonic mafic dykes from late Archaean granitoids in the Eastern Dharwar Craton,southern India

We present a first overview of the synplutonic mafic dykes (mafic injections) from the 2.56–2.52 Ga calcalkaline to potassic plutons in the Eastern Dharwar Craton (EDC). The host plutons comprise voluminous intrusive facies (dark grey clinopyroxene-amphibole rich monzodiorite and quartz monzonite, pinkish grey porphyritic monzogranite and grey granodiorite) located in the central part of individual pluton, whilst subordinate anatectic facies (light grey and pink granite) confined to the periphery. The enclaves found in the plutons include highly angular screens of xenoliths of the basement, rounded to pillowed mafic magmatic enclaves (MME) and most spectacular synplutonic mafic dykes. The similar textures of MME and adjoining synplutonic mafic dykes together with their spatial association and occasional transition of MME to dismembered synplutonic mafic dykes imply a genetic link between them. The synplutonic dykes occur in varying dimension ranging from a few centimeter width upto 200 meters width and are generally dismembered or disrupted and rarely continuous. Necking of dyke along its length and back veining of more leucocratic variant of the host is common feature. They show lobate as well as sharp contacts with chilled margins suggesting their injection during different stages of crystallization of host plutons in magma chamber. Local interaction, mixing and mingling processes are documented in all the studied crustal corridors in the EDC. The observed mixing, mingling, partial hybridization, MME and emplacement of synplutonic mafic dykes can be explained by four stage processes: (1) Mafic magma injected during very early stage of crystallization of host felsic magma, mixing of mafic and felsic host magma results in hybridization with occasional MME; (2) Mafic magma introduced slightly later, the viscosities of two magmas may be different and permit only mingling where by each component retain their identity; (3) When mafic magma injected into crystallizing granitic host magma with significant crystal content, the mafic magma is channeled into early fractures and form dismembered synplutonic mafic dykes and (4) Mafic injections enter into largely crystallized (>80% crystals) granitic host results in continuous dykes with sharp contacts. The origin of mafic magmas may be related to development of fractures to mantle depth during crystallization of host magmas which results in the decompression melting of mantle source. The resultant hot mafic melts with low viscosity rise rapidly into the crystallizing host magma chamber where they interact depending upon the crystallinity and viscosity of the host. These hot mafic injections locally cause reversal of crystallization of the felsic host and induce melting and resultant melts in turn penetrate the crystallizing mafic body as back veining. Field chronology indicates injection of mafic magmas is synchronous with emplacement of anatectic melts and slightly predates the 2.5 Ga metamorphic event which affected the whole Archaean crust. The injection of mafic magmas into the crystallizing host plutons forms the terminal Archaean magmatic event and spatially associated with reworking and cratonization of Archaean crust in the EDC.     

华北克拉通晚前寒武纪镁铁质岩墙群K－Ar年龄及地质意义

华北克拉通腹地山西地块内广泛发育大规模的晚前寒武纪镁铁质岩墙群。通过对晋北地区新平堡镁铁质岩墙群９个样品的Ｋ－Ａｒ年龄等时线分析，这些岩墙可能形成于１４３０Ｍａ．从山西各地所采集的６４个镁铁质岩墙群样品的Ｋ－Ａｒ表观年龄统计分析可见，华北克拉通腹地内广泛发育的镁铁质岩墙群主要形成于中元古代１０００～１８００Ｍａ间，活动高峰期在１２００～１６００Ｍａ。     

超高温麻粒岩中尖晶石成分、结构特征和矿物反应的指示意义:以阿尔泰造山带超高温尖晶石-斜方辉石-石榴石麻粒岩为例

超高温变质作用的研究已成为世界上热门的地球科学领域之一,其中斜方辉石+夕线石+石英、假蓝宝石+石英、尖晶石+石英、大隅石+石英以及富铝斜方辉石等标型矿物组合和特征可以指示岩石经历了超高温变质作用(温度>900℃),这对查明地球深部下地壳的物质组成和构造演化具有重要意义。初次对产于世界上不同地区超高温麻粒岩尖晶石+石英共生等的标型矿物组合、不同赋存状态的尖晶石ZnO含量、XZn[Zn/(Mg+Fe2++Zn)]、XMg等进行分析和对比,认为不同地区不同赋存状态的尖晶石,其ZnO含量、XZn和XMg有所不同,但总的来说,超高温麻粒岩尖晶石中ZnO质量分数多数低于2.5%,但个别特殊的有高达近15%。尖晶石中XZn较低且尖晶石与石英共生,可以作为超高温变质的证据之一。通过对阿尔泰南缘超高温尖晶石-斜方辉石-石榴石麻粒岩中尖晶石成分及ZnO含量分析,得出与石英共生的尖晶石ZnO质量分数约为2.50%,且有与XFe成正比的变化趋势,而与钛铁矿共生的尖晶石ZnO质量分数约为1.85%,虽然两者含量稍有不同,但与世界上超高温麻粒岩中多数尖晶石ZnO含量相比都相近。结合其他特征矿物组合,可以确定该岩石中尖晶石与石英共生组合可以作为阿尔泰地区发生超高温变质作用的证据。通过对阿尔泰南缘与尖晶石-石英有关的变质反应期次划分等的初步研究,认为变质期次可划分为峰期变质和退变质两期,推测峰期的温度条件可达到1000℃,且该超高温麻粒岩可能经历了顺时针p-T演化轨迹。该超高温麻粒岩在阿尔泰造山带的出现,可能与古生代时期发生的古亚洲洋俯冲、西伯利亚板块和哈萨克斯坦—准噶尔板块碰撞造山作用过程有关。