“地球动力学”的研究现状与展望——第32届国际地质大会研究成果综述

第32届国际地质大会通过按地域和构造作用过程等形式划分11个专题会场,展示了地球动力学的研究成果。其成果主要包括特提斯域构造演化及其不同阶段的块体裂解、拼合及后期改造的细节过程,地质历史中的超大陆分布和成因,俯冲—碰撞带深部构造和变质机制,安第斯山(Andes)缓倾角平坦式俯冲过程及其地壳变形和岩浆作用的响应,显微构造对动力作用过程的影响和控制,地壳和上地幔熔融、流变学和动力学意义,大洋岩石圈构造与演化,大陆地盾区构造和再活动,稳定大陆区地震,空间大地测量学和现代板块运动等方面。这些研究成果充分显示了地球动力学研究具有多学科、多手段(如古地磁、超深钻、地球物理、大地测量和GPS等)、多尺度(宏观、微观)和多时期、全面、综合、并逐步接近定时、定位和定量地探索和研究的特点,它从地球(主要为上地幔和地壳)的组成、结构构造入手,逐步认识地球(主要为地球岩石圈)的演化和动力学。     

西天山艾肯达坂组火山岩系同位素定年及其构造意义

西天山艾肯达坂地区较好发育了艾肯达坂纽红色陆相火山岩建造．它不整合在下石炭统大哈拉军山组之上,未经变形和变质，属于陆陆碰撞晚期的橄榄安粗岩系，其年龄确定是厘定从碰撞造山向陆内构造演化的关键。因此,通过16件新获得的钾氩年龄测值，确定艾肯达坂组火山岩系形成在260Ma～270Ma之间，属早二叠世，而不是过去认为的石炭纪；西天山的陆陆碰撞应在二叠纪末结束,此后进入陆内造山阶段。     

Crustal Electrical Conductivity Structure of Southern Tibet from Magnetoteiluric Survey

Two superwide bands of frequency magnetotelluric (MT) profiles (Yadong-Xuegula,Jilong-Cuoqin) across the Yaluzangbu suture were deployed along the west-east direction, for the research into the electrical conductivity structure in the shallow and deep crust along the west-east and north-south directions in the southern part of Tibet plateau. The main characters of the dectrical conductivity structure in this region are: (1) large-scale high resistive bodies exist near the Yaluzangbu suture surface, which extends to the maximum depth of more than 30 km. They are the reflection of the Gangdise granite; (2) small-scale conductive bodies exist in the southern part of the Yaluzangbu suture,and large-scale ones under the suture and in the northern part; (3) conductive bodies widely spread in the crust along the profiles. They are discontinuous, mainly decline to the north and become larger in scale, steeper near the suture, deeper gradually from south to north; (4) under the Yaluzangbu suture,the conductive bodies become larger in scale, more conductive gradually from west to east. These important dectrical characters are caused possibly by the India plate subduction to the north. The variation in characters of the large-scale conductive bodies from west to east may be the proof that the plate collision might cause substantial movement along the west-cast direction.     

宇宙地球厅

宇宙是由许许多多的银河系类星系组成。银河系是由成千上万颗恒星和行星组成，地球所在的太阳系只是银河系的一部分。银河系充满了未知的迷，最令人感兴趣的，那就是地球是怎样形成的?又是怎样演化的?宇宙地球厅将为您解开这个迷。     

Numerical Modeling of Basin-Range Tectonics Related to Continent-Continent Collision

Continent-continent collision is the most important driving mechanism for the occurrence of various geological processes in the continental lithosphere. How to recognize and determine continent-continent collision,especially its four-dimensional temporal-spatial evolution, is a subject that geological communities have long been concerned about and studied. Continent-continent collision is mainly manifested by strong underthrnsting (subduction) of the underlying block along an intracontinental subduction zone and continuous obduction (thrusting propagation) of the overlying block along the intracontinental subduction zone, the occurrence of a basin-range tectonic framework in a direction perpendicular to the subduction zone and the flexure and disruption of the Moho. On the basis of numerical modeling, the authors discuss in detail the couplings between various amounts and rates of displacement caused by basin subsidence, mountain uplift and Moho updoming and downflexure during obduction (thrusting propagation) and subduction and the migration pattern of basin centers. They are probably indications or criteria for judgment or determination of continent-continent collision.     

苏北榴辉岩Sm-Nd等时线同位素年龄及地质意义

采用Sm-Nd同位素定年方法，测得江苏北部新沂地区踢球山榴辉岩岩体时代为221.6±8.4 Ma,Sm-Nd年龄被看作为踢球山超高压变质之后板块折返过程中的高压榴辉岩相重结晶阶段年龄。中朝板块与扬子板块碰撞时代主要发生在晚三叠世。     

内蒙古黄花滩铜镍矿区辉长岩LA-ICP-MS锆石U-Pb定年及地球化学特征

在乌拉特后旗—达茂旗—四子王旗一带的内蒙古中部地区分布着超基性-酸性连续岩浆系列,开展其岩体年代学、地球化学研究可为内蒙古中部地区与超基性-基性岩有关的铜镍矿成矿规律研究提供基础地质资料,还可以推断岩浆侵位时期的区域大地构造背景。本文以达茂旗黄花滩铜镍矿区出露的辉长岩为研究对象,采用LA-ICP-MS仪器对无裂隙、高透明度、阴极发光均匀、环带清晰的锆石进行U-Pb定年,获得岩体加权平均年龄为262.4±1.1 Ma,并利用XRF和ICP-MS进行岩石地球化学分析显示黄花滩辉长岩具有后碰撞拉伸环境下的岩浆特征。综合前人相关研究认为,内蒙古中部地区于中二叠世晚期(255~275 Ma)已经进入后碰撞构造阶段,而古亚洲洋在该区域的闭合应发生在晚二叠世前(~285 Ma),此结论丰富了古亚洲洋闭合时间上限及中晚二叠世期间内蒙古中部地区构造背景方面的证据。     

从藏南陆-陆碰撞带深部结构构造演化探讨斑岩铜矿的成岩成矿问题

本文以INDEPTH项目对印度大陆与欧亚大陆碰撞带深部成像结果为基础,从构造演化角度探讨藏南陆-陆碰撞带冈底斯斑岩铜矿带的成矿作用问题。深部探测给出的碰撞带深部结构与侯增谦等地质学家提出的深部结构有较大的异同,如何协调起来以深化对藏南陆-陆碰撞条件下成矿作用的认识,这是本文讨论的中心。藏南碰撞带成矿实际上是在新特提斯大洋岩石圈俯冲形成的冈底斯岩浆弧成矿作用的基础上,再经过陆-陆碰撞挤压强烈改造后的再成矿。碰撞带的深部结构构造演化的特点是:(1)新特提斯大洋岩石圈板块向北连续俯冲了约120 Ma,形成的冈底斯陆缘火山岩浆弧带,这导致了陆缘带地壳增厚并含有大量的地幔岩浆流体物质(如南美安第斯成矿带那样);(2)在印度大陆与冈底斯陆缘弧接近碰撞时,在对挤中新特提斯大洋洋壳与大洋岩石圈地幔发生向上挤出与向下拆沉,并使部分洋壳残片和大洋岩石圈物质保存在中上地壳内;(3)两大陆岩石圈碰撞对接后,印度岩石圈地幔加深达70~80 km并沿地壳底部向北推进,并将加厚地壳内大量的成矿物质、钙碱性岩浆,洋壳及新生的下地壳,以及部分地幔物质从地壳底部将其围限起来,成为后期再成矿的物质基础;(4)查明了碰撞带深部壳/幔间产生了一层中间速度层(相当于MASH层),在中上地壳部位出现一层巨大的部分熔融层;(5)在碰撞挤压下冈底斯带内产生多组断裂构造,大型逆冲断裂系与背冲断裂,并引发了含矿岩浆的再活动,并在浮力(下地壳内)和挤压力作用下多次活动上升生成斑岩型铜矿床;(6)成矿后地表遭受过强烈的风化剥蚀作用,使矿床出露地表。