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1.
Preservation/exhumation of ultrahigh-pressure subduction complexes   总被引:14,自引:0,他引:14  
W.G. Ernst   《Lithos》2006,92(3-4):321-335
Ultrahigh-pressure (UHP) metamorphic terranes reflect subduction of continental crust to depths of 90–140 km in Phanerozoic contractional orogens. Rocks are intensely overprinted by lower pressure mineral assemblages; traces of relict UHP phases are preserved only under kinetically inhibiting circumstances. Most UHP complexes present in the upper crust are thin, imbricate sheets consisting chiefly of felsic units ± serpentinites; dense mafic and peridotitic rocks make up less than  10% of each exhumed subduction complex. Roundtrip prograde–retrograde PT paths are completed in 10–20 Myr, and rates of ascent to mid-crustal levels approximate descent velocities. Late-stage domical uplifts typify many UHP complexes.

Sialic crust may be deeply subducted, reflecting profound underflow of an oceanic plate prior to collisional suturing. Exhumation involves decompression through the PT stability fields of lower pressure metamorphic facies. Scattered UHP relics are retained in strong, refractory, watertight host minerals (e.g., zircon, pyroxene, garnet) typified by low rates of intracrystalline diffusion. Isolation of such inclusions from the recrystallizing rock matrix impedes back reaction. Thin-aspect ratio, ductile-deformed nappes are formed in the subduction zone; heat is conducted away from UHP complexes as they rise along the subduction channel. The low aggregate density of continental crust is much less than that of the mantle it displaces during underflow; its rapid ascent to mid-crustal levels is driven by buoyancy. Return to shallow levels does not require removal of the overlying mantle wedge. Late-stage underplating, structural contraction, tectonic aneurysms and/or plate shallowing convey mid-crustal UHP décollements surfaceward in domical uplifts where they are exposed by erosion. Unless these situations are mutually satisfied, UHP complexes are completely transformed to low-pressure assemblages, obliterating all evidence of profound subduction.  相似文献   

2.
We have used a coupled thermo-mechanical finite-element (FE) model of crustal deformation driven by mantle/oceanic subduction to demonstrate that the tectonic evolution of the Lachlan Fold Belt (LFB) during the Mid-Palaeozoic (Late Ordovician to Early Carboniferous) can be linked to continuous subduction along a single subduction zone. This contrasts with most models proposed to date which assume that separate subduction zones were active beneath the western, central and eastern sections of the Lachlan Orogen. We demonstrate how the existing data on the structural, volcanic and erosional evolution of the Lachlan Fold Belt can be accounted for by our model. We focus particularly on the timing of fault movement in the various sectors of the orogen. We demonstrate that the presence of the weak basal decollement on which most of the Lachlan Fold Belt is constructed effectively decouples crustal structures from those in the underlying mantle. The patterns of faulting in the upper crust appears therefore to be controlled by lateral strength contrasts inherited from previous orogenic events rather than the location of one or several subduction zones. The model also predicts that the uplift and deep exhumation of the Wagga-Omeo Metamorphic Belt (WOMB) is associated with the advection of this terrane above the subduction point and is the only tectonic event that gives us direct constraints on the location of the subduction zone. We also discuss the implications of our model for the nature of the basement underlying the present-day orogen.  相似文献   
3.
山东南墅地区孔兹岩系变质矿物的成因及演化   总被引:3,自引:0,他引:3  
南墅地区孔兹岩系的变质矿物具有多成因、多世代的特征 ,其经历三阶段五幕的变质作用 ,形成了以Sil+Gt +Cord +Bi +Kf +Pl+Q为代表的共生矿物组合。通过对主要变质矿物成因及演化特征的分析 ,结合温压计估算 ,确定该区孔兹岩系峰期变质作用温度为 70 0~ 75 0℃ ,压力为 0 .6~0 .7GPa ,变质程度达角闪麻粒岩相。确立 pTt轨迹具顺时针演化特点 ,反映一种陆 -陆碰撞造山带式构造演化模式。  相似文献   
4.
Garnet‐bearing peridotite lenses are minor but significant components of most metamorphic terranes characterized by high‐temperature eclogite facies assemblages. Most peridotite intrudes when slabs of continental crust are subducted deeply (60–120 km) into the mantle, usually by following oceanic lithosphere down an established subduction zone. Peridotite is transferred from the resulting mantle wedge into the crustal footwall through brittle and/or ductile mechanisms. These ‘mantle’ peridotites vary petrographically, chemically, isotopically, chronologically and thermobarometrically from orogen to orogen, within orogens and even within individual terranes. The variations reflect: (1) derivation from different mantle sources (oceanic or continental lithosphere, asthenosphere); (2) perturbations while the mantle wedges were above subducting oceanic lithosphere; and (3) changes within the host crustal slabs during intrusion, subduction and exhumation. Peridotite caught within mantle wedges above oceanic subduction zones will tend to recrystallize and be contaminated by fluids derived from the subducting oceanic crust. These ‘subduction zone peridotites’ intrude during the subsequent subduction of continental crust. Low‐pressure protoliths introduced at shallow (serpentinite, plagioclase peridotite) and intermediate (spinel peridotite) mantle depths (20–50 km) may be carried to deeper levels within the host slab and undergo high‐pressure metamorphism along with the enclosing rocks. If subducted deeply enough, the peridotites will develop garnet‐bearing assemblages that are isofacial with, and give the same recrystallization ages as, the eclogite facies country rocks. Peridotites introduced at deeper levels (50–120 km) may already contain garnet when they intrude and will not necessarily be isofacial or isochronous with the enclosing crustal rocks. Some garnet peridotites recrystallize from spinel peridotite precursors at very high temperatures (c. 1200 °C) and may derive ultimately from the asthenosphere. Other peridotites are from old (>1 Ga), cold (c. 850 °C), subcontinental mantle (‘relict peridotites’) and seem to require the development of major intra‐cratonic faults to effect their intrusion.  相似文献   
5.
The Inner Arc of the Central Andes, broadly corresponding to the Eastern Cordillera, is the location of a rich Tertiary and Triassic Sn–W–(Ag-base metal) metallogenic province, commonly referred to as the Bolivian tin belt. We propose that the Tertiary metallogeny, which generated most of the tin ores, was a direct consequence of discrete “collisions” between the South American plate and the Nazca slab and sub-slab mantle, during the ongoing Andean orogeny. Evidence supporting this proposal include: (1) the coincidence of the tin province and the Inner Arc in a marked “hump” in the Andean orogen, which may represent tectonic indentation; (2) the symmetry of the tin province with respect to the Bolivian orocline, the axis of which corresponds to the direction of highest compression; (3) the relative symmetry of the magmatism and tin mineralization with respect to this axis; (4) the concurrent timing of mineralization and compressional pulses; (5) the similar host rock geochemistry and ore lead isotope data, testifying to a common crustal reservoir; and (6) the striking similarity of the igneous suites, associated with the ore deposits to those from “typical” collisional orogens. A number of studies have called upon a persistent tin anomaly to explain the metallogeny of the region. We propose, instead, that the latter is better explained by periodic compressional interaction between the Farallon/Nazca oceanic plate and the South American continent. This led to the generation of peraluminous magmas, which during fractional crystallization exsolved the fluids responsible for the voluminous Sn–W mineralization.  相似文献   
6.
Coupled thermal‐mechanical models are used to investigate interactions between metamorphism, deformation and exhumation in large convergent orogens, and the implications of coupling and feedback between these processes for observed structural and metamorphic styles. The models involve subduction of suborogenic mantle lithosphere, large amounts of convergence (≥ 450 km) at 1 cm yr?1, and a slope‐dependent erosion rate. The model crust is layered with respect to thermal and rheological properties — the upper crust (0–20 km) follows a wet quartzite flow law, with heat production of 2.0 μW m?3, and the lower crust (20–35 km) follows a modified dry diabase flow law, with heat production of 0.75 μW m?3. After 45 Myr, the model orogens develop crustal thicknesses of the order of 60 km, with lower crustal temperatures in excess of 700 °C. In some models, an additional increment of weakening is introduced so that the effective viscosity decreases to 1019 Pa.s at 700 °C in the upper crust and 900 °C in the lower crust. In these models, a narrow zone of outward channel flow develops at the base of the weak upper crustal layer where T≥600 °C. The channel flow zone is characterised by a reversal in velocity direction on the pro‐side of the system, and is driven by a depth‐dependent pressure gradient that is facilitated by the development of a temperature‐dependent low viscosity horizon in the mid‐crust. Different exhumation styles produce contrasting effects on models with channel flow zones. Post‐convergent crustal extension leads to thinning in the orogenic core and a corresponding zone of shortening and thrust‐related exhumation on the flanks. Velocities in the pro‐side channel flow zone are enhanced but the channel itself is not exhumed. In contrast, exhumation resulting from erosion that is focused on the pro‐side flank of the plateau leads to ‘ductile extrusion’ of the channel flow zone. The exhumed channel displays apparent normal‐sense offset at its upper boundary, reverse‐sense offset at its lower boundary, and an ‘inverted’ metamorphic sequence across the zone. The different styles of exhumation produce contrasting peak grade profiles across the model surfaces. However, P–T–t paths in both cases are loops where Pmax precedes Tmax, typical of regional metamorphism; individual paths are not diagnostic of either the thickening or the exhumation mechanism. Possible natural examples of the channel flow zones produced in these models include the Main Central Thrust zone of the Himalayas and the Muskoka domain of the western Grenville orogen.  相似文献   
7.
8.
程丰  彭景臻  王林  郭召杰 《地质学报》2023,97(9):2927-2938
盆山耦合研究在大地构造和地球动力学研究中占有重要地位。地貌负载引起的大陆岩石圈挠曲与沉积盆地沉降是盆山耦合的一种重要体现方式。本论文聚焦于挤压背景下大陆岩石圈挠曲盆地与造山带的耦合过程,系统梳理了单个或者多个地貌负载的几何形态、挠曲盆地几何形态以及岩石圈有效弹性厚度(Te)三者之间的数学关系。在此基础上,论文介绍了岩石圈挠曲模拟方法在恢复岩石圈刚性程度、造山带演化过程以及盆地沉积沉降方面的具体应用。结合古环境分析与岩石圈挠曲模拟实验,本文提出了一种定量恢复造山带古海拔的新方法。有别于基于温度、压力以及动植物分布与海拔之间关系所建立的传统古高度计,该方法强调在海侵时期地貌负载与沉积盆地间的高度差即为造山带的古海拔。该方法的提出为重建中亚以及其他曾受海侵影响并与岩石圈挠曲相关造山带的古海拔提供了新的思路。论文最后介绍了岩石圈挠曲模拟在定量分析造山带与盆地演化的研究过程中存在的问题与不足,并提出了在探究沉积盆地基底属性、重建岩石圈挠曲相关造山带古海拔以及有关挠曲模拟软件开发方面的新展望。  相似文献   
9.
滕霞  张建新 《岩石学报》2020,36(10):2963-2982
超高温(≥900℃)变质作用发生在自太古代以来的各个地质历史时期,目前极可能也正发生在青藏高原地壳深部。同时,它也是以冈瓦纳为代表的超大陆在最终拼合时的显著标识,这一关联指示了超高温变质作用与碰撞造山带的密切关系。本文总结了东冈瓦纳内与泛非造山作用有关的典型超高温变质岩的分布、岩石学特征、峰期变质条件、P-T轨迹及形成时代,并简要介绍我们在柴达木地块西段新识别出的泛非期超高温变质作用的基本特征。结合东冈瓦纳超高温变质作用特征和造山带热模拟研究的新进展,本文获得以东冈瓦纳超高温变质作用为代表的碰撞造山带超高温变质作用的几点认识:1)东冈瓦纳麻粒岩地块中的超高温变质岩和普通麻粒岩记录了相似的变质年龄、P-T轨迹以及呈过渡变化的峰期温度,两者可能是同一构造事件的产物,共同组成一个高温-超高温变质岩单元;2)超高温变质作用在东冈瓦纳内部持续了至少超过30Myr,但未见呈大规模的同期或近同期基性岩岩浆出露,指示此处需要的长期热源不是地幔来源岩浆;3)虽然数值模拟能成功呈现加厚地壳被放射元素衰变热加热至超高温条件的情况,且加热及持续时间与东冈瓦纳超高温变质约束的结果相当,但是模拟中需要的高生热值暗示,在自然界中,完全只靠放射性元素衰变生热或许不能让碰撞造山带内达到超高温条件;4)碰撞造山带经历了长期的构造演化,这一过程中,造山带内地壳不太可能同时达到超高温变质条件,这一特征可能反映在P-T-t轨迹的差异上,对这些轨迹的系统研究有助于对超高温变质作用的构造-热过程的理解。  相似文献   
10.
赣江断裂带中生代的演化及其地球动力学背景   总被引:17,自引:9,他引:8       下载免费PDF全文
梁兴  吴根耀 《地质科学》2006,41(1):64-80
赣江断裂带是江西省境内醒目的北北东向平移断裂构造带,由一系列北北东向、北东向和北西向断裂束组成,表现为一个大规模的左行走滑脆性剪切带并兼具伸展断陷和右旋走滑的成份。赣江断裂带在重力、航磁异常呈现为显著的梯度带,是一条晚中生代的岩浆岩带,控制了以鄱阳盆地为代表的一系列白垩纪-古近纪沉积盆地的形成与发育。该带在中生代的演化可分为早-中侏罗世压扭、晚侏罗早-白垩世左行平移和晚白垩世上盘斜落的右行平移3个阶段。在侏罗纪以来太平洋板块对欧亚大陆斜向俯冲的大背景下,赣江断裂带的形成和演化与华南广为发育的燕山期陆内造山作用密切相关,北北东向断裂的发育则直接受郯庐断裂早白垩世左行走滑活动控制,因而表现出“北强南弱”和“北早南晚”的特点。白垩纪时赣江断裂的活动方式与郯庐断裂一致,可认为是后者的南延。  相似文献   
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