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1.
This contribution emphasizes first-order structural and metamorphic characters of Precambrian accretionary orogens to understand the kinematics and thermomechanical state of the continental lithosphere in convergent settings involving massive juvenile magmatism. We define a new class of orogens, called ultra-hot orogens (UHO), in which the weakest type of lithosphere on Earth is deformed. UHO are characterized by (1) distributed shortening and orogen-scale flow combining vertical and horizontal longitudinal advection, under long-lasting convergence, (2) homogeneous thickening by combined downward movements of supracrustal units and three-dimensional mass redistribution in the viscous lower crust, and (3) steady-state, negligible topography and relief leveled by syn-shortening erosion and near-field sedimentation. The flow analysis of UHO provides clues to understanding crustal kinematics beneath high plateaus and suggests that the seismic reflectivity pattern of hot orogens is an image of the layering produced by lateral flow of the lower crust and associated syn-kinematic plutonism.In between the UHO and the modern cold orogens (CO), developed by shortening of lithosphere bearing a stiff upper mantle, two classes of orogens are defined. Hot orogens (HO, representative of Cordilleran and wide mature collisional belts) share flow pattern characteristics with UHO, but involve a less intense magmatic activity and develop high topographies driving their collapse. Mixed-hot orogens (MHO, representative of magmatic arcs and Proterozoic collisional belts) are orogens made of UHO-type juvenile crust and display CO-like structure and kinematics. This classification points to the fundamental link between the presence of a stiff lithospheric mantle and strain localization along major thrusts in convergent settings. A high Moho temperature (> 900 °C), implying thinning of the lithospheric mantle, enhances three-dimensional flow of the lithosphere in response to convergence. Overall, this classification of orogens emphasizes the space and time variability of uppermost mantle temperature in controlling plate interactions and continental growth. 相似文献
2.
Kent C. Condie 《Tectonophysics》1984,105(1-4)
Metamorphic mineral assemblages suggest the existence of variable geotherms and lithospheric thicknesses beneath late Archean continental crust. Archean granite-greenstone terranes reflect steep geotherms (50–70°C/km) while high-grade terranes reflect moderate geotherms similar to present continental crust with high heat flow (25–40°C/km). Corresponding lithosphere thicknesses for each terrane during the late Archean are 35–50 km and 50–75 km, respectively.Early Archean ( 3.0 b.y.) greenstones differ from late Archean ( 2.7 b.y.) greenstones by the rarity or absence of andesite and graywacke and the relative abundance of pelite, quartzite, and komatiite. Mature clastic sediments in early greenstones reflect shallow-water, stable-basin deposition. Such rocks, together with granite-bearing conglomerate and felsic volcanics imply the existence of still older granitic source terranes. The absence or rarity of andesite in early greenstones reflects the absence of tectonic conditions in which basaltic and tonalitic magmas are modified to produce andesite.A model is presented in which early Archean greenstones form at the interface between tonalite islands and oceanic lithosphere, over convective downcurrents; high-grade supracrustals form on stable continental edges or interiors; and late Archean greenstones form in intracontinental rifts over mantle plumes. 相似文献
3.
Irina M. Artemieva 《Tectonophysics》2006,416(1-4):245
This paper reports a new 1° × 1° global thermal model for the continental lithosphere (TC1). Geotherms for continental terranes of different ages (> 3.6 Ga to present) constrained by reliable data on borehole heat flow measurements (Artemieva, I.M., Mooney, W.D. 2001. Thermal structure and evolution of Precambrian lithosphere: a global study. J. Geophys. Res 106, 16387–16414.), are statistically analyzed as a function of age and are used to estimate lithospheric temperatures in continental regions with no or low-quality heat flow data (ca. 60% of the continents). These data are supplemented by cratonic geotherms based on electromagnetic and xenolith data; the latter indicate the existence of Archean cratons with two characteristic thicknesses, ca. 200 and > 250 km. A map of tectono-thermal ages of lithospheric terranes complied for the continents on a 1° × 1° grid and combined with the statistical age relationship of continental geotherms (z = 0.04 t + 93.6, where z is lithospheric thermal thickness in km and t is age in Ma) formed the basis for a new global thermal model of the continental lithosphere (TC1). The TC1 model is presented by a set of maps, which show significant thermal heterogeneity within continental upper mantle, with the strongest lateral temperature variations (as large as 800 °C) in the shallow mantle. A map of the depth to a 550 °C isotherm (Curie isotherm for magnetite) in continental upper mantle is presented as a proxy to the thickness of the magnetic crust; the same map provides a rough estimate of elastic thickness of old (> 200 Ma) continental lithosphere, in which flexural rigidity is dominated by olivine rheology of the mantle.Statistical analysis of continental geotherms reveals that thick (> 250 km) lithosphere is restricted solely to young Archean terranes (3.0–2.6 Ga), while in old Archean cratons (3.6–3.0 Ga) lithospheric roots do not extend deeper than 200–220 km. It is proposed that the former were formed by tectonic stacking and underplating during paleocollision of continental nuclei; it is likely that such exceptionally thick lithospheric roots have a limited lateral extent and are restricted to paleoterrane boundaries. This conclusion is supported by an analysis of the growth rate of the lithosphere since the Archean, which does not reveal a peak in lithospheric volume at 2.7–2.6 Ga as expected from growth curves for juvenile crust.A pronounced peak in the rate of lithospheric growth (10–18 km3/year) at 2.1–1.7 Ga (as compared to 5–8 km3/year in the Archean) well correlates with a peak in the growth of juvenile crust and with a consequent global extraction of massif-type anorthosites. It is proposed that large-scale variations in lithospheric thickness at cratonic margins and at paleoterrane boundaries controlled anorogenic magmatism. In particular, mid-Proterozoic anorogenic magmatism at the cratonic margins was caused by edge-driven convection triggered by a fast growth of the lithospheric mantle at 2.1–1.7 Ga. Belts of anorogenic magmatism within cratonic interiors can be caused by a deflection of mantle heat by a locally thickened lithosphere at paleosutures and, thus, can be surface manifestations of exceptionally thick lithospheric roots. The present volume of continental lithosphere as estimated from the new global map of lithospheric thermal thickness is 27.8 (± 7.0) × 109 km3 (excluding submerged terranes with continental crust); preserved continental crust comprises ca. 7.7 × 109 km3. About 50% of the present continental lithosphere existed by 1.8 Ga. 相似文献
4.
Oceanic arcs are commonly cited as primary building blocks of continents, yet modern oceanic arcs are mostly subducted. Also, lithosphere buoyancy considerations show that oceanic arcs (even those with a felsic component) should readily subduct. With the exception of the Arabian–Nubian orogen, terranes in post-Archean accretionary orogens comprise < 10% of accreted oceanic arcs, whereas continental arcs compose 40–80% of these orogens. Nd and Hf isotopic data suggest that accretionary orogens include 40–65% juvenile crustal components, with most of these (> 50%) produced in continental arcs.Felsic igneous rocks in oceanic arcs are depleted in incompatible elements compared to average continental crust and to felsic igneous rocks from continental arcs. They have lower Th/Yb, Nb/Yb, Sr/Y and La/Yb ratios, reflecting shallow mantle sources in which garnet did not exist in the restite during melting. The bottom line of these geochemical differences is that post-Archean continental crust does not begin life in oceanic arcs. On the other hand, the remarkable similarity of incompatible element distributions in granitoids and felsic volcanics from continental arcs is consistent with continental crust being produced in continental arcs.During the Archean, however, oceanic arcs may have been thicker due to higher degrees of melting in the mantle, and oceanic lithosphere would be more buoyant. These arcs may have accreted to each other and to oceanic plateaus, a process that eventually led to the production of Archean continental crust. After the Archean, oceanic crust was thinner due to cooling of the mantle and less melt production at ocean ridges, hence, oceanic lithosphere is more subductable. Widespread propagation of plate tectonics in the late Archean may have led not only to rapid production of continental crust, but to a change in the primary site of production of continental crust, from accreted oceanic arcs and oceanic plateaus in the Archean to primarily continental arcs thereafter. 相似文献
5.
中国大地构造几个重大问题的探讨 总被引：9，自引：1，他引：9
中国大地构造需要研究的重大问题甚多 ,文中选择了其中的 4个加以讨论。首先是大地构造发展演化的动力学理论。现在流行的按密度差、温度差建立的地幔对流、拆沉作用、地幔柱理论 ,阐明不了中国大陆岩石圈、大陆造山带的组成、结构与演化。我们的研究成果表明 ,任何一个自然形成的系统 ,其运动与演化的能源 (或力源 )都来源于它的自身 ;它内部的变形和结构几何学特征 ,也是它自身运动的结果。为此特提出在地球自转速度变化制约下的多层扭动涡旋甩出说———核幔壳“风暴”所引发的热核反应是地球发展与演化惟一的、统一的动力来源。第二 ,地槽、板块是涡旋甩出构造体系中的一种运动方式、一种造山模式。此外 ,我们根据秦岭和其它造山带所总结出来的抽拉逆冲岩片构造 (或抽拉构造 )也是大陆岩石圈板块或壳块内部的一种新的运动方式 ,它是继地槽学说、板块构造理论以后一种新的造山模式。文中较详细地介绍了抽拉构造理论的基本特征。第三 ,中国大陆岩石圈在中—新生代时期、在陆相沉积盆地形成以后、在抽拉构造体制作用下所形成的 (陆内 )造山带以及它们之间的残留陆相 (或海相 )沉积盆地 ,是中国大地构造的基本特征。陆内造山作用是中国大陆划时代的造山作用 ,所形成的造山带是中国大陆最重要的造山带。? 相似文献
6.
Accretionary orogens throughout space and time represent extremely fertile settings for the formation and preservation of a wide variety of mineral deposit types. These range from those within active magmatic arcs, either in continental margin or intra-oceanic settings, to those that develop in a variety of arc-flanking environments, such as fore-arcs and back-arcs during deformation and exhumation of the continental margin. Deposit types also include those that form in more distal, far back-arc and foreland basin settings. The metallogenic signature and endowment of individual accretionary orogens are, at a fundamental level, controlled by the nature, composition and age of the sub-continental lithosphere, and a complex interplay between formational processes and preservational forces in an evolving Earth. Some deposit types, such as orogenic gold and volcanic massive sulfide (VMS) deposits, have temporal patterns that mimic the major accretionary and crustal growth events in Earth history, whereas others, such as porphyry Cu–Au–Mo and epithermal Au–Ag deposits, have largely preservational patterns. The presence at c. 3.4 Ga of (rare) orogenic gold deposits, whose formation necessitates some form of subduction–accretion, provides strong evidence that accretionary processes operated then at the margins of continental nuclei, while the widespread distribution of orogenic gold and VMS deposits at c. 2.7–2.6 Ga reflects the global distribution of accretionary orogens by this time. 相似文献
7.
大陆内部变形在很大程度受制于大陆岩石圈流变侧向不均一性,而温度(地热梯度)是影响地壳和地幔岩石流变性质的主导因素。由热引起的地壳/地幔岩石材料的热弱化是弱化的主要途径,为陆内变形准备了物质条件。在构造外力(板块相关的或非相关的)的作用下,这些受到热弱化的岩石材料极易发生变形,导致岩石圈内部的造山带和变形带的形成。文章试图在广泛的国内外文献搜集和综合分析基础上,介绍由生热元素(heat producing elements)聚集产生的地壳/地幔(岩石)热弱化以及随后地幔下降流构造力作用造成的大陆内部应变局部化和陆内构造变形。这些地幔下降流是由大陆岩石圈地幔重力(瑞利 泰勒型)不稳定性发育引起的。 相似文献
8.
Xenolith evidence for polybaric melting and stratification of the upper mantle beneath South China 总被引：2，自引：0，他引：2
Mantle xenoliths from Hainan and Qilin, South China have been studied to constrain the nature of the upper mantle and mantle processes beneath a continental margin. The extremely low Ti (160–245 ppm) contents in clinopyroxenes from some spinel lherzolites, indicative of high degrees of partial melting are inconsistent with the relatively high clinopyroxene modes (7.4–13%) in these samples. This inconsistency could be due to polybaric melting that started in the garnet stability field, then, after the breakdown of garnet to pyroxene and spinel, continued in the spinel stability field. Polybaric melting, due to adiabatic decompression of upwelling mantle, would leave a residual mantle in which the degree of depletion decreases with depth. The predicted stratified lithospheric mantle is evidenced by the negative correlation between the forsterite content in olivine and the equilibration temperature, proportional to the depth in the lithosphere from which the xenolith was derived. The lower part of the lithospheric mantle beneath South China consists predominantly of fertile and moderately depleted peridotites, which are either devoid of LREE enrichment, or show the trace element signature of incipient metasomatism, and plot within the Phanerozoic mantle domain. In contrast, the upper part of the mantle contains harzburgite and cpx-poor lherzolite, which are strongly affected by metasomatism of melt/fluid of highly variable composition. The anomalously high orthopyroxene mode (up to 47%) makes some of these refractory samples compositionally similar to the Proterozoic/Archean mantle. Their low equilibrium temperature (800–900 °C) points to the presence of old lithospheric relicts in the uppermost mantle beneath South China. Such lithosphere architecture may have resulted from partial replacement of Archean–Proterozoic lithosphere by asthenosphere that rose adiabatically subsequent to lithospheric thinning during the Cenozoic. 相似文献
9.
Archean plate tectonics, rise of Proterozoic supercontinentality and onset of regional, episodic stagnant-lid behavior 总被引：3，自引：1，他引：2
Intense devolatilization and chemical-density differentiation attended late-stage accretion of the primitive Earth; it lessened after crystallization of a magma mush ocean during continued cooling. By 4.3Ga, shallow seas were present, so surface temperatures had fallen far below the 1300, 1120, and 950°C low-pressure solidi of peridotite, basalt, and granite, respectively. At temperatures less than about half their solidi, such materials existed as lithosphere in the near-surface Hadean realm. Stagnant-lid convection probably did not occur because massive heat transfer necessitated vigorous crust–mantle overturn in the early, hot Earth. Instead, bottom-up mantle convection, including voluminous plume ascent, efficiently rid the planet of heat, but lessened over time. Plate thickening and broadening is reflected in the post-Hadean rock record. Stages of geologic evolution included: (a) 4.5–4.4Ga, early, chaotic magma mush ocean overturn and ephemeral lithospheric platelets; (b) 4.4–2.7Ga, growth of oceanic and diminutive continental plates, obliterated by return mantle flow prior to 4.0Ga, but the latter enlarging and gradually accumulating as largely submarine, sutured, sialic crust-capped lithospheric collages; (c) 2.7–1.0Ga, progressive assembly of old shields and younger orogenic belts into supercratonal plates characterized by continental freeboard, sedimentary differentiation, and episodic glaciation during transpolar drift, as well as onset of regionally, temporally limited stagnant-lid convection beneath supercontinents; (d) 1.0Ga-present, modern, laminar-flowing asthenospheric cells capped by giant, stately moving plates. Restriction of komatiitic lavas to the Archean, and of multicycle sediments, most ophiolite complexes ± alkaline igneous rocks, and high-pressure and ultrahigh-pressure metamorphic belts to progressively younger Proterozoic–Phanerozoic orogens reflects increasingly negative buoyancy of the cooler oceanic lithosphere. Attending supercontinent assembly, density instabilities of thickening oceanic plates increasingly began to dominate overturn of the suboceanic mantle as cold, top-down convection. Scales and dynamics of hot asthenospheric upwelling versus lithospheric foundering and asthenospheric return flow (bottom-up versus top-down) changed gradually over geologic time in response to planetary thermal relaxation. 相似文献
10.
The disturbance of mechanical and thermal equilibria in the upper shell of the Earth as a result of mantle or local within-plate
processes related to periodic tectonic activity gives rise to the formation of convective flows in the low-viscosity asthenosphere.
These flows affect the lithosphere and create domains of subsidence and uplift, which can continue to develop long after the
cessation of active periods. If the density of the lithosphere does not decrease with depth, then small-scale flows increase
uplift in zones of compression of the continental lithosphere and create domains of extension at their margins. In our opinion,
small-scale convection is the main geodynamic factor that forms foredeeps. The results of detailed numerical modeling of foredeep
formation at the margins of adjoining orogens are presented in the current paper. In order to set the initial conditions for
the stage of continental collision, the precollision stages of the foldbelt evolution are considered, including the stage
of trough formation on the thinned continental crust or on the oceanic lithosphere and the stage of sedimentary basin formation;
depending on the degree of extension, this can be an inner sea or a passive continental margin. Such initial conditions were
used in modeling of the compression stage (continental collision), when the orogen-foredeep system is formed. The parameters
of the model and the tectonic processes are chosen so as to bring the results of numerical computation in line with the data
on the Greater Caucasus and northern Forecaucasus, including the thickness of the crustal layers and sedimentary cover, structure
of the foredeeps, rate of tectonic subsidence, heat flow, etc. Comparison of the numerical modeling results with the formation
history of the Caucasus foredeeps confirms that the first stage of regional compression of the Greater Caucasus took place
before the deposition of the Maikop sediments. At least three compression stages followed: 16.6–15.8 Ma (Tarchanian), 14.3–12.3
Ma (Konkian-early Sarmatian), and 7.0–5.2 Ma (Pontian). The next stage of regional compression is apparently occurring at
present. 相似文献
11.
Composition and age of tertiary sills and dykes, Jameson Land Basin, East Greenland: relation to regional flood volcanism 总被引：1，自引：0，他引：1
The Paleozoic–Mesozoic Jameson Land Basin (East Greenland) is intruded by a sill complex and by a swarm of ESE trending dykes. Together with dykes of the inner Scoresby Sund fjord, they form a regional Early Tertiary intrusive complex located 200–400 km inland of the East Greenland rifted continental margin. Most of the intrusive rocks in the Jameson Land Basin are geochemically coherent and consist of evolved plagioclase–augite–olivine saturated, uncontaminated high-Ti basalt with 48.5–50.2 wt.% SiO2, 2.2–3.2 wt.% TiO2, 5.1–7.4 wt.% MgO, 9–17 ppm Nb and La/YbN=2.8–3.6. Minor tholeiitic rock types are: (a) low-Ti basalt (49.7 wt.% SiO2, 1.7 wt.% TiO2, 6.8 wt.% MgO, 2.6 ppm Nb and La/YbN=0.5) akin to oceanic basalts; (b) very-high-Ti basalt (48.6 wt.% SiO2, 4.1 wt.% TiO2, 5.1 wt.% MgO and 21 ppm Nb); and (c) plagioclase ultraphyric basalt. The tholeiitic dolerites are cut by alkali basalt (43.7–47.3 wt.% SiO2, 4.1–5.1 wt.% TiO2, 4.9–6.2 wt.% MgO, 29–46 ppm Nb and La/YbN=16–17) sills and dykes.Modelling of high-field-strength and rare-earth elements indicate that the high-Ti basalts formed from 6–10% melting of approximately equal proportions of garnet- and spinel-bearing mantle of slightly depleted composition beneath thick continental lithosphere. Conversely, dolerite intrusions and flood basalts of similar compositional kindred from adjacent but more rift-proximal occurrences in Northeast Greenland formed from shallower melting of dominantly spinel-bearing mantle beneath extended and thinned continental lithosphere. These variations in lithospheric thickness suggest the continent–ocean transition of the East Greenland rifted volcanic margin is sharp and narrow.40Ar–39Ar dating and paleomagnetism show that the high-Ti dolerites were emplaced at 53–52 Ma (most likely during C23r) and hence surprisingly postdate the main flood volcanism by 2–5 Ma and the inception of seafloor spreading between Greenland and Europe by 1–2 Ma. The formation of tholeiitic and alkaline magmas emplaced into the Jameson Land Basin corroborates to the importance of post-breakup magmatism along the East Greenland volcanic rifted margin. Upwelling of the ancestral Iceland mantle plume under central Greenland at 53–52 Ma (rather than under the active rift), perhaps accompanied by a failed attempt to shift the rift zone westward towards the plume axis, may have triggered post-breakup continental magmatism of the Jameson Land Basin and the inner Scoresby Sund region, along preexisting structural lineaments. 相似文献
12.
中生代华北燕山造山带是陆内造山作用的典型,但长期来对造山作用的动力学机制存在多种分歧观点。本文尝试将岩石圈不同深度的构造整合在一起,探索陆内造山作用的主因。本文拟从燕山带中生代构造运动的基本特征入手,选择集宁-承德基底岩石圈断裂带作为先存构造薄弱带,结合不同深度层次的地质作用:①地表的断陷盆地及其火山-沉积岩建造;②断块构造的差异隆升;③固态流变和地热活动;④幔源或者壳幔混溶的火山岩,论证先存构造薄弱带的活化现象。在此基础上,通过幔源熔-流体的交代作用讨论了岩石圈强度的弱化,结合岩石圈结构的层析成像研究,得到初步结论:地幔底辟体上涌是华北克拉通中生代构造活化的重要背景。不排除不同板块间相互作用的影响。最后,从与国外典型的陆内造山带的对比中,进一步认识到:深部地幔物质上涌和上部岩石圈物质的均衡调整,是陆内造山与陆缘造山的本质区别。 相似文献
13.
George Helffrich 《Tectonophysics》2006,416(1-4):23
Small-scale seismic heterogeneity exists at different levels in the lower mantle, and is detected by methods that analyze scattered–not direct–energy from natural and artificial sources. Its vertical distribution, association with subduction, and its ≤ 10-km characteristic scale length strongly suggest that it is chemical/petrological in nature and originally created by melting and differentiation during mid-ocean ridge formation. What is of interest is that the scale lengths of both upper and lower mantle seismic heterogeneity are similar, which supports the view of a common origin explored here. Unlike the lower mantle however, which is broadly homogeneous in structure, the upper mantle contains things that trap and impede the dispersal and re-mixing of heterogeneity: continental crust, lithosphere and cratonic roots. These probably control the depths, the longevity and the age of heterogeneities at shallow mantle levels, and suggest that heterogeneities observed in continental mantle lithosphere are probably old, trapped by the process that grows continental roots. Alternatively, if crustal heterogeneity is controlled by the details of a magmatic process, it must either be somehow continually renewed, for which there is no recognizable surface expression, or it must be depleted over time and the present is a time when, by luck, we may still witness it. 相似文献
14.
Effects of buoyancy and mechanical layering on collisional deformation of continental lithosphere: Results from physical modeling 总被引：1，自引：0，他引：1
We use two suites of lithospheric-scale physical experiments to investigate the manner in which deformation of the continental lithosphere is affected by both (1) variations of lithospheric density (quantified by the net buoyant mass per area in the lithospheric mantle layer, MB), and (2) the degree of coupling between the crust and lithospheric mantle (characterized by a modified Ampferer ratio, Am). The dynamics of the experiments can be characterized with a Rayleigh–Taylor type ratio, CLM. Models with a positively buoyant lithospheric mantle layer (MB > 0 and CLM > 0) result in distributed root formation and a wide deformation belt. In contrast, models with a negatively buoyant lithospheric mantle layer strongly coupled to the crust (MB < 0, 0 > CLM > ≈ − 0.2, and Am > ≈ 10− 3) exhibit localized roots and narrow deformation belts. Syncollisional delamination of the model lithospheric mantle layer and a wide deformation belt is exhibited in models with negatively buoyant lithospheric mantle layers weakly coupled to the crust (MB < 0, CLM < 0, and Am < ≈ 10− 3). Syncollisional delamination of the continental lithosphere may initiate due to buoyancy contrasts within the continental plate, instead of resulting from wedging by the opposing plate. Rayleigh–Taylor instabilities dominate the style of deformation in models with a negatively buoyant lithospheric mantle layer strongly coupled to the crust and a slow convergence rate (MB < 0 and CLM > ≈ − 0.2). The degree of coupling (Am) between the model crust and lithospheric mantle plays a lesser role in both the style of lower-lithospheric deformation and the width of the crustal deformed zone with increasing density of the lithospheric mantle layer. 相似文献
15.
An intrinsic feature of Cordillera-style orogenic systems is a spatial trend in the radiogenic isotopic composition of subduction-related magmatism. Magmatism is most isotopically juvenile near the trench and becomes increasingly evolved landward. A compilation of radiogenic isotopic data from the central Andes, U.S. Cordillera, and Tibet (the most well-studied examples of modern and ancient Cordilleran systems) demonstrate such spatial trends are long-lived and persist throughout the life of these continental subduction margins. The consistency of the isotopic trend through time in magmatic products is surprising considering the plethora of orogenic processes that might be expected to alter them. In addition to longevity, spatial isotopic trends encompass a broad spectrum of geochemical compositions that represent diverse petrogenetic and geodynamic processes. The two end-members of the spatial isotopic trends are represented by melts sourced within isotopically juvenile asthenospheric mantle and melts sourced from isotopically evolved continental lithospheric mantle and/or lower crust. Mantle lithosphere generally thins toward the magmatic arc and trench in Cordilleran orogens because sub-lithospheric processes such as delamination, subduction erosion, and subduction ablation, operate to thin or remove the continental mantle lithosphere. With time, magmatic additions may impart the isotopic composition of the mantle source on the lower crust, giving rise to an isotopically homogenous deep lithosphere. The results of this analysis have significant implications for interpreting temporal and spatial shifts in isotopic composition within Cordilleran orogens and suggest that the continental mantle lithosphere may be a significant source of magmatism in orogenic interiors. 相似文献
16.
大陆岩石圈研究进展 总被引：5，自引：0，他引：5
从地震学、地球化学、岩石学等不同学科的角度,对大陆岩石圈研究进展做了简要介绍。不同学科的最新研究成果表明,岩石圈在热状态、化学成分和力学行为等方面具有高度非均匀性。这不仅表现为岩石圈性质和结构随深度的变化,而且还反映在不同时代、大陆与海洋以及克拉通和造山带岩石圈结构特征的显著差异上。性质和结构的差异体现了岩石圈形成和长期演化过程的复杂性。我们认为,不同岩石圈块体之间、岩石圈与深部对流地幔之间普遍存在着相互作用。这种相互作用被认为是稳定克拉通岩石圈遭受改造甚至破坏的深部机制,同时还是地球深、浅部物质交换的重要方式,因而显著影响着地球深部的对流和地表的构造过程。值得注意的是,由于岩石圈本身定义的模糊性及其厚度的不确定性,地震活动与岩石圈强度之间的关系以及大陆岩石圈演化的规律性等问题仍有待于进一步的研究和探索。 相似文献
17.
Lithospheric controls on the formation of provinces hosting giant orogenic gold deposits 总被引：10，自引：0，他引：10
Frank P. Bierlein David I. Groves Richard J. Goldfarb Benoit Dubé 《Mineralium Deposita》2006,40(8):874-886
Ages of giant gold systems (>500 t gold) cluster within well-defined periods of lithospheric growth at continental margins, and it is the orogen-scale processes during these mainly Late Archaean, Palaeoproterozoic and Phanerozoic times that ultimately determine gold endowment of a province in an orogen. A critical factor for giant orogenic gold provinces appears to be thickness of the subcontinental lithospheric mantle (SCLM) beneath a province at the time of gold mineralisation, as giant gold deposits are much more likely to develop in orogens with subducted oceanic or thin continental lithosphere. A proxy for the latter is a short pre-mineralisation crustal history such that thick SCLM was not developed before gold deposition. In constrast, orogens with protracted pre-mineralisation crustal histories are more likely to be characterised by a thick SCLM that is difficult to delaminate, and hence, such provinces will normally be poorly endowed. The nature of the lithosphere also influences the intrinsic gold concentrations of potential source rocks, with back-arc basalts, transitional basalts and basanites enriched in gold relative to other rock sequences. Thus, segments of orogens with thin lithosphere may enjoy the conjunction of giant-scale fluid flux through gold-enriched sequences. Although the nature of the lithosphere plays the crucial role in dictating which orogenic gold provinces will contain one or more giant deposits, the precise siting of those giants depends on the critical conjunction of a number of province-scale factors. Such features control plumbing systems, traps and seals in tectonically and lithospherically suitable terranes within orogens. 相似文献
18.
Paleoproterozoic supercontinent: Origin and evolution of accretionary and collisional orogens exemplified in Northern cratons 总被引：1，自引：0，他引：1
M. V. Mints 《Geotectonics》2007,41(4):257-280
The evolution of the North American, East European, and Siberian cratons is considered. The Paleoproterozoic juvenile associations concentrate largely within mobile belts of two types: (1) volcanic-sedimentary and volcanic-plutonic belts composed of low-grade metamorphic rocks of greenschist to low-temperature amphibolite facies and (2) granulite-gneiss belts with a predominance of high-grade metamorphic rocks of high-temperature amphibolite to ultrahigh-temperature granulite facies. The first kind of mobile belt includes paleosutures made up of not only oceanic and island-arc rock associations formed in the process of evolution of relatively short-lived oceans of the Red Sea type but also peripheral accretionary orogens consisting of oceanic, island-arc, and backarc terranes accreted to continental margins. The formation of the second kind of mobile belt was related to the activity of plumes expressed in vigorous heating of the continental crust; intraplate magmatism; formation of rift depressions filled with sediments, juvenile lavas, and deposits of pyroclastic flows; and metamorphism of lower and middle crustal complexes under conditions of granulite and high-temperature amphibolite facies that, in addition, spreads over the fill of rift depressions. The evolution of mobile belts pertaining to both types ended with thrusting in a collisional setting. Five periods are recognized in Paleoproterozoic history: (1) origin and development of a superplume in the mantle that underlay the Neoarchean supercontinent; this process resulted in separation and displacement of the Fennoscandian fragment of the supercontinent (2.51–2.44 Ga); (2) a period of relatively quiet intraplate evolution complicated by locally developed plume-and plate-tectonic processes (2.44–2.0 (2.11) Ga); (3) the origin of a new superplume in the subcontinental mantle (2.0–1.95 Ga); (4) the complex combination of intense global plume-and plate-tectonic processes that led to the partial breakup of the supercontinent, its subsequent renascence and the accompanying formation of collisional orogens in the inner domains of the renewed Paleoproterozoic supercontinent, and the emergence of accretionary orogens along some of its margins (1.95–1.75 (1.71) Ga); and (5) postorogenic and anorogenic magmatism and metamorphism (<1.75 Ga). 相似文献
19.
论全球性中-新生代陆内造山作用与造山带 总被引：29，自引：4，他引：25
对不同类型造山作用与造山带的深入剖析,在现代地学研究中占有重要的位置。迄今对造山带类型划分以及陆内（ 板内） 造山带是否存在及其形成机制问题,尚有不同认识。文章在阐明造山带分类准则的基础上,将全球性中－ 新生代造山带划分为陆缘型、陆间型与陆内型三大类。对陆内造山带则划分出发育在前寒武纪古克拉通基础上、发育在前中生代陆缘、陆间造山带基础上两种类型。文内还对全球性中－ 新生代陆内造山作用与造山带的展布特点、形成机制及其大陆动力学意义进行概括论述 相似文献
20.
超越板块构造——我国构造地质学要做些什么? 总被引：25，自引：1，他引：24
对近十年来全球构造学和构造地质学的重要进展进行了简要评述.30年前建立的全球构造理论改变了人们对地球及其演化的认识.作为固体地球统一理论的板块构造主要涉及刚性板块边界之间的变形、地震活动和火山作用.至今还没有完整理论阐明板块运动的驱动力和地幔对流机制.板块边界和板内变形等许多问题仍然无法回答.大陆岩石圈和大洋岩石圈在成分、厚度和力学强度方面有明显的差别, 因此现有板块构造不完全适合于大陆构造.大陆地壳和地幔流变学的综合研究是认识大陆构造和超越板块构造的最佳途径.流变学是大陆造山带几何学和动力学的桥梁.大陆岩石圈对构造作用、重力作用和热作用的响应在很大程度上取决于其流变强度.岩石圈流变性质是岩石圈分层和塑性流动的主导因素.大量透入性变形和巨型大陆造山带内部构造显示非刚性特征.大陆构造和力学行为主要由地壳强度而不是地幔强度所控制.从大陆岩石圈多层性和力学强度不均匀性表征看, 现在是抛弃传统“三明治”构造模式的时候了.面对地球系统科学和地球动力学新思维发展趋势, 多学科综合研究大陆构造(造山带)和加速高水平构造地质学人才的培养是我国构造地质学发展的最紧迫任务 相似文献