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1.
GEOCHEMISTRY OF THE PLIOCENE SHOSHONITIC ROCKS FROM OIYUG BASIN, CENTRAL TIBET  相似文献   

2.
揭示地质现象的本质与核心   总被引:8,自引:0,他引:8  
青藏高原的形成与演化是举世瞩目的现代地学前缘 ,岩石圈结构及其演变对于探讨高原隆升及其资源环境效应具有重要意义。多年来 ,对于青藏高原岩石圈结构的认识主要基于地球物理探测结果和地质研究 ,尚未发现深达地幔的物质。我们在西昆仑地区康西瓦新生代火山岩中首次发现了以含金云母方辉橄榄岩为主的深源包体 ,其主要组成矿物为橄榄石和斜方辉石 ,含有少量单斜辉石、尖晶石和金云母。橄榄岩具有平衡粒状变晶结构 ,部分橄榄石颗粒仍保留有扭折带。电子探针分析结果表明 ,尖晶石的x(Cr) /x(Cr +Al)变化为 2 5%~ 8% ,属于尖晶石铬铁矿系列。根据CarrollWebb和Wood(1986 )提出的温压图解 ,橄榄岩形成压力大致为16 0 0MPa ,约相当于深度 56km。据此 ,认为康西瓦新生代玄武岩中产出的橄榄岩包体系岩浆活动过程中从岩石圈地幔携带上来的幔源物质 ,对于探讨青藏高原北部的岩石圈结构及其演化具有重要意义。  相似文献   

3.
TWO TYPES OF CENOZOIC HIGH-K MAGMATINSM IN EASTERN TIBET:IMPLICATIONS FOR THE NATURE OF MANTLE SOURCES1 ArnaudNO ,VidalP ,TapponnierP ,etal.ThehighK2 OvolcanismofnorthwesternTibet:geochemistryandtectonicim plications[J] :EarthPlanetSciLett,1991,11:351~ 36 7. 2 DengW .CenozoicvolcanicrocksinthenorthernNgaridistrictoftheTibet Discussionontheconcurrentsubduction[J] .Ac taPetrolSinica ,1989( 3) :1~ 11. 3 HarrisonTM ,LeloupPH ,RyersonFJ,…  相似文献   

4.
Kohistan Sequence has been considered as island arc formed during the subduction of oceanic lithosphere at the leading edge of northward moving Indian continent.. Sedimentary sequences indicate that formation of the intra\|oceanic Kohistan arc began in early Cretaceous time. The isotopic data demonstrate the involvement of enriched, DUPAL type mantle, suggesting that Kohistan arc was formed at or south of the present equator (Khan et al., 1997). The Intra oceanic phase of Kohistan lasted until sometime between 102 and 85 Ma, when Kohistan collided with Asia. From this time until collision with India about 50 Ma ago, Kohistan existed as Andean\|type margin. This paleomagnetic study is from the volcanic and plutonic rocks exposed in Gupis\|Shamran area (west of Gilgit) in northern part of the Kohistan arc. According to geochronological data these rocks were formed 61~55Ma ago (Treloar et al., 1989), when Kohistan was existing as Andean\|type margin. Seven to nine samples were collected from nine sites of Shamran volcanics (58±1)Ma and from five sites of Pingal, Gupis, and Yasin plutons (Ar\|Ar hornblende ages ranges from 61~52Ma). On the basis of one Rb\|Sr age of (59±2)Ma from these plutons, the above\|mentioned Ar/Ar ages may be regarded as reasonable intrusion ages of these plutons (Searle, 1991).  相似文献   

5.
岩溶动力系统中的生物作用机理初探   总被引:24,自引:1,他引:24  
岩溶动力系统是地球表层系统的重要组成部分。生物是地球表层系统中最活跃的地质营力之一 ,它在岩溶动力系统中扮演着重要的角色。地质历史时期 ,生物圈大气圈界面上 ,生物通过植物的光合同化、动植物分泌 ,使大气圈中的CO2 不断转移到碳酸盐岩中 ,形成岩溶发育的物质基础 ,并成为全球最大的碳库 ;生物圈水圈界面上 ,生物形成的生物 (微 )环境改变了水循环的强度和方向 ,并影响岩溶发育 ;生物圈岩石圈界面上 ,生物通过生物物理、生物化学过程 ,殖居碳酸盐岩之上 ,并以之为生存依托 ,生物的新陈代谢过程使碳酸盐岩岩石圈活化 ,使其积极参与全球碳循环。  相似文献   

6.
MAIN CENTRAL THRUST ZONE IN THE KATHMANDU AREA, CENTRAL NEPAL, AND ITS TECTONIC SIGNIFICANCE1 AritaK ,LallmeyerRD ,TakasuA .TectonothermalevolutionoftheLesserHimalaya ,Nepal:constraintsfrom 4 0 Ar/3 9AragesfromtheKathmandunappe[J].TheIslandArc ,1997,6 :372~ 384. 2 RaiSM ,GuillotS ,LeFortP ,etal.Pressure temperatureevolutionintheKathmanduandGosainkundregions ,CentralNepal[J].JourAsianEarthSci ,1998,16 :2 83~ 2 98. 3 SchellingD ,KArita .…  相似文献   

7.
CHRONOSTRATIGRAPHY,SEDIMENTATION AND EVOLUTION OF THE XIGAZE FOREARC BASIN: IMPLICATIONS FOR DYNAMIC EVOLUTION OF THE YARLUNG ZANGBO SUTURE ZONE1 All埁greCJ,CourtillotV ,TapponnierP ,etal.StructureandevolutionoftheHimalaya Tibetorogenicbelt[J] .Nature,1984 ,30 7:17~ 2 2 . 2 CoulonC ,MaluskiH ,BollingerC ,etal.MesozoicandCenozoicvolcanicrocksfromcentralandsouthernTibet:3 9Ar 40 Ardating ,petrotogicalcharacteristicsandgeodyn…  相似文献   

8.
9.
ULTRAMAFIC XENOLITHS FROM A KAMAFUGITE LAVA IN CENOZOIC VOLCANIC FIELD OF WEST QINLING, CHINA AND ITS GEOLOGICAL IMPLICATION  相似文献   

10.
HETEROGENEITY OF THE LITHOSPHERE IN TIBETAN PLATEAU ON THE CONSTRAINTS OF MAGMATISM  相似文献   

11.
SIGNIFICANCE AND CHARACTERISTICS OF OPHIOLITE SUITE IN LAJI SHAN, SOUTHERN QILIAN MOUNTAINS, QINGHAI PROVINCE,CHINAthedoctoralprogramofhighereducation (970 49119)  相似文献   

12.
CENOZOIC VOLCANISM AND LITHOSPHERETECTONIC EVOLUTION IN NORTH TIBET  相似文献   

13.
As a widely‐developed mineral in various types of rocks, pyrite features important geological information such as temperature and pressure during its formation and evolution (An et al., 2014; An et al., 2018). It is an important geological formation for studying the origins of rocks, mineralization, and deposits (Xue et al., 2014; An et al., 2016). The study of the genesis of gold deposits is a research hotspot in current geology and mineral deposits not only because of high economic value, but also because of important practical significance (An et al., 2017; Yang et al., 2014). Shandong Zhaoyuan, as the third largest gold production area in the world, has important research significance of the origin and generation of gold‐bearing minerals (Xue et al., 2014; Wen et al., 2014). In this study, pyrite from augen granite (figure 1a), syenite (figure 1b), basite (figure 1c) and gold ore (figure 1d) at Zhaoyuan gold deposit Shandong Province, was selected as the research object. The morphological and structural micro‐fabrics were analysed by polarized light microscopy (PLM) and Raman spectroscopy to reveal the source and process of gold further.  相似文献   

14.
Pb, Sr AND Nd-ISOTOPIC COMPOSITIONS OF PALEO AND NEO-TETHYAN OCEANIC CRUSTS IN THE EASTERN TETHYAN DOMAIN: IMPLICATION FOR THE INDIAN OCEAN-TYPE ISOTOPIC SIGNATURE  相似文献   

15.
Diamonds have been discovered in mantle peridotites and chromitites of six ophiolitic massifs along the 1300 km‐long Yarlung‐Zangbo suture (Bai et al., 1993; Yang et al., 2014; Xu et al., 2015), and in the Dongqiao and Dingqing mantle peridotites of the Bangong‐Nujiang suture in the eastern Tethyan zone (Robinson et al., 2004; Xiong et al., 2018). Recently, in‐situ diamond, coesite and other UHP mineral have also been reported in the Nidar ophiolite of the western Yarlung‐Zangbo suture (Das et al., 2015, 2017). The above‐mentioned diamond‐bearing ophiolites represent remnants of the eastern Mesozoic Tethyan oceanic lithosphere. New publications show that diamonds also occur in chromitites in the Pozanti‐Karsanti ophiolite of Turkey, and in the Mirdita ophiolite of Albania in the western Tethyan zone (Lian et al., 2017; Xiong et al., 2017; Wu et al., 2018). Similar diamonds and associated minerals have also reported from Paleozoic ophiolitic chromitites of Central Asian Orogenic Belt of China and the Ray‐Iz ophiolite in the Polar Urals, Russia (Yang et al., 2015a, b; Tian et al., 2015; Huang et al, 2015). Importantly, in‐situ diamonds have been recovered in chromitites of both the Luobusa ophiolite in Tbet and the Ray‐Iz ophiolite in Russia (Yang et al., 2014, 2015a). The extensive occurrences of such ultra‐high pressure (UHP) minerals in many ophiolites suggest formation by similar geological events in different oceans and orogenic belts of different ages. Compared to diamonds from kimberlites and UHP metamorphic belts, micro‐diamonds from ophiolites present a new occurrence of diamond that requires significantly different physical and chemical conditions of formation in Earth's mantle. The forms of chromite and qingsongites (BN) indicate that ophiolitic chromitite may form at depths of >150‐380 km or even deeper in the mantle (Yang et al., 2007; Dobrthinetskaya et al., 2009). The very light C isotope composition (δ13C ‐18 to ‐28‰) of these ophiolitic diamonds and their Mn‐bearing mineral inclusions, as well as coesite and clinopyroxene lamallae in chromite grains all indicate recycling of ancient continental or oceanic crustal materials into the deep mantle (>300 km) or down to the mantle transition zone via subduction (Yang et al., 2014, 2015a; Robinson et al., 2015; Moe et al., 2018). These new observations and new data strongly suggest that micro‐diamonds and their host podiform chromitite may have formed near the transition zone in the deep mantle, and that they were then transported upward into shallow mantle depths by convection processes. The in‐situ occurrence of micro‐diamonds has been well‐demonstrated by different groups of international researchers, along with other UHP minerals in podiform chromitites and ophiolitic peridotites clearly indicate their deep mantle origin and effectively address questions of possible contamination during sample processing and analytical work. The widespread occurrence of ophiolite‐hosted diamonds and associated UHP mineral groups suggests that they may be a common feature of in‐situ oceanic mantle. The fundamental scientific question to address here is how and where these micro‐diamonds and UHP minerals first crystallized, how they were incorporated into ophiolitic chromitites and peridotites and how they were preserved during transport to the surface. Thus, diamonds and UHP minerals in ophiolites have raised new scientific problems and opened a new window for geologists to study recycling from crust to deep mantle and back to the surface.  相似文献   

16.
东南沿海地区第四纪大陆岩石圈地幔的特征   总被引:5,自引:0,他引:5  
东南沿海地区新生代玄武岩中的橄榄岩包体来自年轻的大陆岩石圈地幔 ,该岩石圈地幔在岩石学、矿物组成、痕量元素以及Sr Nd同位素组成等各方面具有很大差异。这些差异反映了它们来自不同的地幔过程。南海张开与地幔热柱有关 ,南海扩张后第四纪形成的火山岩携至地表的包体更多保留了地幔热柱的信息。橄榄岩包体的矿物成分与深海橄榄岩类似 ,相对贫Opx而富Ol;在痕量元素上 ,表现为强不相容元素的富集 ,其配分模式类似于其寄主岩 ;Nd同位素强烈亏损 ,显示出比MORB源区更亏损的特征。大陆岩石圈地幔经历了来自地幔深处的贫SiO2 熔体的进一步改造。  相似文献   

17.
造山带超高压变质流体中气体组成及成藏条件初探   总被引:3,自引:1,他引:3  
传统的油气地质研究和勘探开发几乎都是集中在盆地,而造山带作为板(陆)块的碰撞、会聚带,为无机成因气形成和释放的有利场所,是天然气地质理论研究的一个新领域。本文利用激光拉曼探针技术对大别造山带超高压变质岩中流体包裹体进行了成分分析,结果表明超高压变质流体中不仅含有CO2(>50%)、H2、N2、H2S等,还有高含量的幔源烃类气(CH4等,含量最高达23.6mol%)。同时,超高压变质带中还发育有浅层碳酸盐岩及其它含碳岩石经动力变质作用可形成大量的CO2气。大别超高压变质带中具有无机成因气成藏的可能条件,带内广泛发育的推覆构造、韧性断层及糜棱岩可以作为无机成因气成藏的圈、盖和保存条件。本文成果可为油气地质研究和勘探开发提供新的思路、方向和领域。  相似文献   

18.
滇西南澜沧县老厂浅水相“老厂组”时代之订正   总被引:4,自引:3,他引:1  
方宗杰  肖荫文 《地层学杂志》1999,23(4):248-256,T002
对澜沧县老厂水库东侧公路剖面开展系统的生物地层学研究,证实西盟至竹塘公路13~14km 区段属Eostaffella 带,12.5~13km 区段属Pseudostaffella 带。所谓的浅水相“老厂组”和冬瓜林火山岩的时代应修正为早石炭世德坞阶至晚石炭世滑石板阶,宜归入平掌组的范畴。确认老厂矿区存在有两套不同时代、不同构造背景的火山岩  相似文献   

19.
INDIA/ASIA CONVERGENCE AND HIMALAYAN SHORTENING   总被引:1,自引:0,他引:1  
INDIA/ASIA CONVERGENCE AND HIMALAYAN SHORTENING  相似文献   

20.
深层气理论分析和深层气潜势研究   总被引:9,自引:3,他引:9  
近年来的一些文献表述深层气时在"深层"和"深部"名词概念上容易造成不必要的费解。就沉积层而言,宜将生油主带(生油窗)作为"深"的界限,从此界限开始到基底以上地层范围的天然气统统称为"深层气";就整个地球而言,宜将沉积层结晶基底和该基底以下的天然气统统称为"深部气"。当然,还应更多地注意来源于深部"深生浅储"的"深层气"。深层气的形成与地壳烃类形成的垂直分带性有关。在一定的历史时期和一定的沉积盆地油气形成分带性理论对勘探实践发挥了一定的指导作用,随着油气地质科研和勘探实践的发展,人们逐渐发现了油气形成分带性理论中油相消失和气相生成带开始门限指标的局限性。不同盆地有不同深度的生油主带,因而也有不同深度范围生气主带(干气带)。腐泥型有机质的演化需要更高的活化能,而需更高的温度和更大的深度,其生气主带深于腐殖型有机质源岩层的位置。生气主带有机质演化受多种因素控制,其中温度、深度和时间是重要因素,引起深层温度升高的条件有地球动力和深部热流等。古生界以前的重大生物地质事件为深层气形成准备了有机质及其演化条件,从物质基础上讲,深层气有巨大的资源潜势。油气形成的地球动力学观点及其他新观点为研究深层气提供了新的思路,岩石圈的烃类资源远未枯竭,被发现和开采的资源仅是其中的一部分,更多的需在深部去发掘。  相似文献   

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