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1.
朱文斌  王玺  葛荣峰 《地质学报》2021,95(1):124-138
地体构造是对板块构造理论的发展和补充,它受控于全球板块动力学体系,因此不能将地体与板块割裂开来去研究。其相对于刚性板块的小规模、多样性和广泛性,对了解全球板块的离散和大陆的拼贴增生过程具有十分重要意义。地体构造无处不在,它不仅存在于中、新生代陆缘造山带中,也存在于古老造山带中,一些古老的克拉通实际上也是由不同的地体拼合而成的。地体的运动包括聚合、离散和走滑三种方式,地体的增生作用是聚合的主要表现形式,并导致大陆的生长扩大,而地体的离散作用联合增生作用,决定了现代大陆的轮廓。分析地体聚合和离散的过程,可以发现有两种不同的模式,即单向聚合-离散和多向聚合-离散,它们对应了不同的地球动力学过程。地体的单向聚合-离散可以由大洋的俯冲增生或大陆汇聚碰撞而导致,但在这个过程中,大洋向大陆的单向俯冲起到了主导作用。地体的多向离散和聚合与岩石圈的裂解与汇聚有密切联系,从全球构造演化的格局来看,岩石圈裂解与汇聚的方向本身具有多向性,这就导致了一些微陆块地体与具洋壳性质的地体一同发生多向离散和聚合。地体的单向离散和聚合会因构造变动而转变为多向离散和聚合,俯冲板片回转与海沟后撤会导致俯冲带弯曲和俯冲方向的改变,这是引起上述转变的原因。  相似文献   
2.
尾亚—天湖地区位于新疆中亚造山带东南部的中天山地块内,晚古生代—中生代岩浆活动强烈,产出了战略性关键矿产尾亚钒铁磁铁矿。在详细岩相学观察的基础上,对尾亚、天湖和沙泉子南岩体中的角闪石和黑云母进行了电子探针(EMPA)测试分析,限定了3个岩体结晶的温压条件、氧逸度、含水量和含铁指数等要素,为解析中天山地块的岩浆-成矿物化条件及其区域找矿勘查工作提供参考。测试结果表明,该区花岗岩类中的角闪石富镁、钙、钠,贫钾,属于钙角闪石族;黑云母有高镁、钛、铝、钾和低硅、钠的特征为镁质黑云母。角闪石和黑云母的化学成分揭示其寄主岩浆为钙碱性造山带岩系,具有壳幔混源的特征,推测可能是板块俯冲背景下由地幔楔与大陆地壳物质混熔形成。根据角闪石-黑云母矿物温压计,估算出沙泉子南石英闪长岩的结晶温度为651~753 ℃,压力为31~79 MPa,尾亚二长花岗岩和钾长花岗岩的结晶温度为762~833 ℃,压力为85~215 MPa,天湖花岗闪长岩的结晶温度为668~812 ℃,压力为31~117 MPa。3个岩体岩浆结晶时的氧逸度lgf(O2)范围为-15.7~-9.4,而且在角闪石结晶时岩浆具有较高的含水量。综合分析,认为该区的花岗岩类具有高温、低压、高氧逸度、富水和高含铁指数的特点,有利于Fe等成矿元素在流体中富集,具有良好的铁矿成矿条件。进一步利用角闪石-黑云母压力计,计算了花岗岩类岩体的侵位深度,从而估算出岩体的剥蚀程度处于2.2~5.5 km,且区域的隆升剥蚀量差异明显;结合现有的矿产地表展布特征,推测天湖岩体一带深部仍具有较好的铁矿找矿潜力。  相似文献   
3.
李先棋  涂向衡  杜彦强  李琼仙 《云南地质》2011,30(2):130-133,140
从干树金矿赋存于怒江构造带高黎贡山岩群变质岩系中,有两个明显的次级矿化带,具多期次成矿作用特点:前期可能为沉积变质赋矿,后期为剪切(构造热液)成矿。晚期在浅部风化淋滤富集。剪切作用形成的金矿是主体。  相似文献   
4.
胶北地体早前寒武纪重大岩浆事件、陆壳增生及演化   总被引:4,自引:4,他引:0  
刘建辉  刘福来  丁正江  刘平华  王舫 《岩石学报》2015,31(10):2942-2958
早前寒武纪重大岩浆事件是早期陆壳增生及演化的主要地质作用。本文通过系统总结最近几年胶北地体早前寒武纪重大岩浆事件代表性岩石的岩相学、锆石U-Pb年代学、岩石地球化学及锆石Hf同位素研究的最新成果,厘定出太古宙~2.9Ga、2.7Ga及2.5Ga三期以TTGs岩浆事件为代表的陆壳增生事件。这些TTGs具有典型太古宙高铝TTGs的地球化学特征及正的εHf(t)值,锆石Hf模式年龄主要集中在ca.3.2~2.7Ga。两种不同的构造模式被用来理解胶北太古宙TTGs(陆壳)的成因:(1)加厚基性下地壳的部分熔融;(2)俯冲洋壳的部分熔融。根据胶北TTGs在时间上呈事件性侵位,空间上呈面状分布,以及相对较低的Mg#、Cr及Ni含量,前者可能更适合胶北TTGs的成因。确定了胶北古元古代2.2~2.0Ga黑云母/角闪石二长花岗片麻岩及~1.8Ga以二长(正长)花岗岩为代表的多期陆壳重熔事件。综合这些研究结果,初步总结出胶北早前寒武纪陆壳形成及演化历史:1)2.9Ga,主要为基性地壳(洋壳)的增生,并可能存在规模有限的、被剥蚀殆尽的太古宙早期陆壳;2)在~2.9Ga、~2.7Ga及~2.5Ga,由于地幔(热)柱上涌,ca.3.3~2.7Ga新生的加厚基性玄武质下地壳发生事件性部分熔融,并伴随有早期陆壳的重熔,形成主要由TTGs及少量陆壳重熔型(高钾)花岗岩组成的太古宙陆壳;3)ca.2.2~2.0Ga,可能由于地幔物质上涌,陆壳伸展,形成裂谷,陆壳物质重熔,形成ca.2.2~2.0Ga花岗质岩石;4)ca.1.95~1.85Ga,发生强烈的挤压碰撞构造作用,裂谷闭合,卷入挤压作用的物质发生高角闪岩相到高压麻粒岩相变质;5)~1.8Ga,地幔物质上涌,陆壳伸展减薄,陆壳物质重熔,形成~1.8Ga花岗岩。  相似文献   
5.
滇西镇康放羊山Cu-Pb-Zn多金属矿床是保山地块发现的首个富铜的铅锌多金属矿床。为探讨其成矿流体来源和矿床成因,对该矿床开展了流体包裹体和C-O同位素研究。结果表明,阶段Ⅱ主要发育富液相包裹体,均一温度和盐度(NaCleq,质量分数)集中在240~300℃和8.0%~18.0%;阶段Ⅲ以含CO2和子矿物包裹体为特征,均一温度和盐度的两个峰值为360~400℃、16.0%~24.0%和240~320℃、4.0%~14.0%;阶段Ⅳ以富液相和纯液相包裹体为主,均一温度和盐度降低至220~340℃和8.0%~14.0%。C-O同位素分析结果(δ13CV-PDB值为-5.88‰~-2.37‰,δ18OV-SMOW值为8.18‰~12.79‰)显示成矿流体主要来源于岩浆热液,在迁移过程中受到围岩溶解作用的影响。综合研究认为,放羊山矿床阶段Ⅱ和阶段Ⅲ的成矿流体主要来源于大陆碰撞形成的中高温、中高盐度、富CO2岩浆热液,在阶段Ⅲ晚期和阶段Ⅳ受到中低温、低盐度大气降水的影响;矿床为受构造控制明显的中高温热液矿床,预测在矿区深部有望找到矽卡岩型矿体。  相似文献   
6.
青藏高原岩石圈三维电性结构   总被引:3,自引:0,他引:3       下载免费PDF全文
本文报道通过综合大地电磁调查数据研究青藏高原岩石圈三维电阻率模型的初步成果.大地电磁法调查区域已经覆盖了高原大部分面积,为全区三维电阻率成像研究打下了可靠的基础.对多个测区大地电磁数据进行精细的同化处理和反演成像,取得了青藏高原可靠的岩石圈三维电阻率结构图像.成像的区域为28°N—35°N,80°E—104°E.三维反演计算时采用的网格尺寸为20km×20km,垂直方向不等间距剖分为26层.结果表明,青藏高原现今岩石圈电阻率扰动主要反映印度克拉通对亚欧大陆板块俯冲引起的热流体运动和大陆碰撞和拆离产生的构造.在岩石圈地幔,察隅地块、喜马拉雅地块和拉萨地块东部联成统一的高电阻率地块,它们反映了向北东俯冲的印度克拉通.雅鲁藏布江、班公—怒江和金沙江缝合带都有明显的低电阻率异常,表明岩石圈深处有热流体活动.雅鲁藏布江、班公—怒江和金沙江缝合带都有明显的低电阻率异常,也表明它们的岩石圈还有流体活动.青藏高原东部的低阻区沿100°E向地幔下方扩大,反映了金沙江断裂带有切穿岩石圈的趋势.地幔电阻率平面扰动的模式显示,青藏高原东西部的地体碰撞拼合形式和方向是不同的.在青藏高原西部,羌塘、拉萨和喜马拉雅等地体从北到南碰撞拼合.在青藏高原东部,羌塘—拉萨、察隅、印支、雅安和扬子等地体多方向拆离拼合,在地壳造成不正交的拆离带和压扭构造系.从高阻-低阻区的分布看,东部的地体拼合有地幔的根源,今后还会进一步发展.察隅地块岩石圈对青藏高原东部的楔入,使其北部和东部地块的岩石圈发生拆离撕裂,也造成热流体上涌的低电阻率异常.  相似文献   
7.
In the Cleaverville area of Western Australia, the Regal, Dixon Island, and Cleaverville Formations preserve a Mesoarchean lower‐greenschist‐facies volcano‐sedimentary succession in the coastal Pilbara Terrane. These formations are distributed in a rhomboidal‐shaped area and are unconformably overlain by two narrowly distributed shallow‐marine sedimentary sequences: the Sixty‐Six Hill and Forty‐Four Hill Members of the Lizard Hills Formation. The former member is preserved within the core of the Cleaverville Syncline and the latter formed along the northeast‐trending Eighty‐Seven Fault. Based on the metamorphic grade and structures, two deformation events are recognized: D1 resulted in folding caused by a collisional event, and D2 resulted in regional sinistral strike‐slip deformation. A previous study reported that the Cleaverville Formation was deposited at 3020 Ma, after the Prinsep Orogeny (3070–3050 Ma). Our SHRIMP U–Pb zircon ages show that: (i) graded volcaniclastic–felsic tuff within the black shale sequence below the banded iron formation in the Cleaverville Formation yields an age of (3 114 ±14) Ma; (ii) the youngest zircons in sandstones of the Sixty‐Six Hill Member, which unconformably overlies pillow basalt of the Regal Formation, yield ages of 3090–3060 Ma; and (iii) zircons in sandstones of the Forty‐Four Hill Member show two age peaks at 3270 Ma and 3020 Ma. In this way, the Cleaverville Formation was deposited at 3114–3060 Ma and was deformed at 3070–3050 Ma (D1). Depositional age of the Cleaverville Formation is at least 40–90 Myr older than that proposed in previous studies and pre‐dates the Prinsep Orogeny (3070–3050 Ma). After 3020 Ma, D2 resulted in the formation of a regional strike‐slip pull‐apart basin in the Cleaverville area. The lower‐greenschist‐facies volcano‐sedimentary rocks are distributed only within this basin structure. This strike‐slip deformation was synchronous with crustal‐scale sinistral shear deformation (3000–2930 Ma) in the Pilbara region.  相似文献   
8.
The Woniusi flood basalts from the Baoshan terrane, SW China, represent a signi?cant eruption of volcanic rocks which were linked to the Late Paleozoic rifting of the Cimmeria from the northern margin of East Gondwana. However, the precise mechanism for the formation and propagation of the rifting is still in debate. Here we report 40Ar/39Ar dating, whole-rock geochemistry, and Sr–Nd–Pb isotopes for the Woniusi basalts from the Baoshan terrane of SW China, with the aim of assessing if a mantle plume was related to the formation of the continent Cimmeria. 40Ar/39Ar dating of the Woniusi basalts yielded ages of 279.3 ± 1.1 Ma and 273.9 ± 1.5 Ma, indicating they were emplaced during the Early Permian. Whole-rock geochemistry shows that these basalts have subalkaline tholeiitic af?nity, low TiO2 (1.2–2.2 wt%), and fractionated chondrite-normalized LREE and nearly ?at HREE patterns [(La/Yb)N = 2.86–5.77; (Dy/Yb)N = 1.21–1.49] with noticeable negative Nb and Ta anomalies on the primitive mantle-normalized trace element diagram. The ?Nd(t) values (?4.76 to +0.92) and high (206Pb/204Pb)i (18.40?18.66) along with partial melt modeling indicates that the basalts were likely derived from a sub-continental lithospheric mantle (SCLM) source metasomatized by subduction-related processes. On the basis of a similar emplacement age to the Panjal basalts and Qiangtang mafic dykes and flood basalts in the Himalayas, combined with a tectonic reconstruction of Gondwana in the Early Permian, we propose that the large-scale eruption of these basalts and dykes was related to an Early Permian mantle plume that possibly initiated the rifting on the northern margin of East Gondwana.  相似文献   
9.

In its type area around Narooma, the Narooma Terrane in the Lachlan Orogen comprises the Wagonga Group, which consists of the Narooma Chert overlain by the argillaceous Bogolo Formation. Conodonts indicate that the lower, largely massive (ribbon chert) part of the Narooma Chert ranges in age from mid-Late Cambrian to Darriwilian-Gisbornian (late Middle to early Late Ordovician). The upper Narooma Chert consists of shale, containing Eastonian (Late Ordovician) graptolites, interbedded with chert. Where not deformed by later faulting, the boundary between the Narooma Chert and Bogolo Formation is gradational. At map scale, the Narooma Terrane consists of a stack of imbricate thrust slices caught between two thrust faults that juxtaposed the terrane against the coeval Adaminaby Superterrane in Early Silurian time. These slices are best defined where Narooma Chert is thrust over Bogolo Formation. The soles of such slices contain multiply foliated chert. Late extensional shear bands indicate a strike-slip component to the faulting. The Narooma Terrane, with chert overlain by muddy ooze, is interpreted to be an oceanic terrane that accumulated remote from land for ~50 million years. The upward increase in the terrigenous component at the top of the Wagonga Group (shale, argillite, siltstone and sandstone of the upper Narooma Chert and Bogolo Formation) records approach of the terrane to the Australian sector of the Gondwana margin. Blocks of chert, argillite and sandstone reflect extensional/strike-slip disruption of the terrane as it approached the transform trench along the Gondwana-proto-Pacific plate boundary. Blocks of basalt and basalt breccia represent detritus from a seamount that was also entering the trench. There is no evidence that the Narooma Terrane or the adjacent Adaminaby Group formed in an accretionary prism/ subduction complex.  相似文献   
10.
We report new zircon U–Pb age, Hf isotopic, and major and trace element data for rhyolites from the Duolong Ore Concentration Area of the Southern Qiangtang Terrane. Building on previous studies, we constrain the tectonic setting and propose a model to explain the geodynamics and crustal growth during regional magmatism in the Early Cretaceous. The analysed rhyolites yield laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) zircon U–Pb ages of 115 and 118 Ma. The rocks are K-rich (K2O = 6.66–9.93 wt.%; K2O/Na2O = 8.2–19.7 wt.%), alkaline and peraluminous (A/CNK = 1.02–1.46), and are characterized by high SiO2 contents (72.8–78.8 wt.%) similar to highly fractionated I-type granites. Fractionation of Fe–Ti oxides, plagioclase, hornblende, Ti-bearing phases, apatite, monazite, allanite and zircon contributed to the variations in major and trace element chemistry. High K2O contents are likely due to partial melting of the continental crust. The samples have positive zircon εHf(t) values ranging from +7.1 to +11.2. These features, together with young zircon Hf crustal model ages of 489–721 Ma, indicate that the K-rich rhyolites were derived from juvenile lower crust with an input of a mantle-derived component. We suggest that the Early Cretaceous K-rich rhyolites formed in a continental arc setting during northward subduction of Bangong Co–Nujiang oceanic lithosphere. Basaltic magma underplating was responsible for vertical crustal growth, triggered by slab roll-back in the Duolong Ore Concentration Area in the Early Cretaceous.  相似文献   
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