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1IntroductionThe northern segment of the South LancangjiangBelt refers to the terrain about200km east of theYunxian-Lingcang granite in the South LancangjiangBelt(Fig.1).During the seventh Five-Year Plan peri-od,Mo Xuanxue et al.(1993)undertook the resear…  相似文献   

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《Gondwana Research》2001,4(3):319-328
Examination of Landsat TM images, reconnaissance field traverses and the published geological maps from the Eastern Ghats Mobile Belt (EGMB), India, reveal a network of major ductile shear zones both within and at the margins. These shear zones are characterized by mylonitic foliation, grain size reduction, metamorphic retrogression, stretching lineations and distinct signatures of alkaline, anorthositic and granitic magmatism. These shear zones divide the EGMB into distinct terranes, which are heterogeneously deformed with extensive tracts of foliated mylonitic gneisses and ultramylonites. The main gneissic foliation in all the terranes is refolded in near non-coaxial manner generally about the axis subparallel to the elongation of the terrane.Structural history in each terrane is distinct in the orientation of stretching lineations, attitude of gneissosity and early fold axial planes, lithological assemblages and available geochronological data. It is possible to recognise nine large terranes within the EGMB and the characteristics of each terrane have been described. The terrane distribution in the EGMB could well fit a thrust tectonic, allochthonous model of amalgamation and accretion. Different terranes could be different thrust nappes or allochthonous tectonic sheets representing tectono-stratigraphic terranes.  相似文献   

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The formation of the Tongyu gold deposit, controlled by regional polyphase deformation-metamorphism.is closely related to the regional composite antiform-shear slip fracture zone. Late-stage reworking of theTaihua Group accounts for the enrichment of ore substances. It is a typical syntectonic gold deposit. The formation and evolution of the deposit involved four stages: (Ⅰ) the state of preparation of ore sub-stances, in which primary source beds originated: (Ⅱ) the stage of remobilization of ore substances, in whichregional progressive metamorphism and migmatization and thermodynamic-chemical differentiation led toremobilization of gold and its initial local concentration: (Ⅲ) the stage of gold deposit formation, in which re-gional folding produced concordant and cross shear-slip fractures and under the dynamic action gold was sepa-rated and migrated in a certain direction and concentrated to form a gold deposit: (Ⅳ) the stage ofsuperpositon, reworking and exposure of orebodies, in which the block uplifted and the deposit againunderwent reworking through faulting and mechanical differentiation.Thermodynamic mineralization played adominant role in the formation of the deposit.  相似文献   

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The 100-km diameter Popigai impact crater (astrobleme), which formed 35.7?Ma ago as a result of the collision of an ordinary chondrite asteroid, was discovered in the 1970s. The impact site was studied in detail for nearly two decades, and various geological investigations were performed there. They included drilling of numerous wells (about 850), geophysical surveys, and investigations of impact breccias and impactites. This research was generally performed in connection with the identification of the unique resource of industrial impact diamonds, which were found in impact rocks for the first time in the world. The extensive research data acquired over 20–30 years include geological maps, collections of rock samples and thin sections, core samples, etc. All these materials are stored in the Russian Research Geological Institute in St Petersburg. Although a lot of data on the Popigai crater have already been published, the available materials and new analytical methods offer the opportunity to obtain some new data on mechanisms of rock-forming processes during an impact event, to improve existing geological models, and to compare in detail all these features to those established in other large craters on the Earth. Modelling of the physical processes of impact cratering has been extended and new data contribute significantly to the study of impact cratering and other problems of comparative planetology. In particular, many different hypotheses of rock-forming mechanisms are tested, especially those of impact melting of various target lithologies, homogenisation of huge volumes of melt products, and their mode of ejection, deposition, cooling, etc.  相似文献   

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<正>Objective The tectonic characteristics and evolution of the Paleoproterozoic Jiao-Liao-Ji belt have been extensively studied in recent decades(Fig.1 a).Two main models have been proposed for the formation of this belt:a continental-or arc-continent collisional belt,and the opening and closure of an intra-continental rift.The main reasons for these ongoing debates are own to the complex composition,including metamorphosed volcano-sedimentary rocks,multiple pulses of granitic magmatism,meta-mafic intrusions,and tectonometamorphic history.In addition,earlier work focused on the geochronology and metamorphic evolution,whereas the  相似文献   

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Experiments on water-rock interaction were carried out on wall-rock samples fromtheMobin gold deposit,Southwest Hunan,China ,with the aim of determining the optimum physical and chemical conditions for the mobilization of gold in solution.Results indicate that gold is most easily mobilized from the wall rock-tuffaceous slate of the Mobin Deposit.Mobi-lization is optimized if fluids are neutral to slightly alkaline and contain both chlorine and sul-phur ions at the concentration and composition of about[0.25M(NH4)2 1M NaCl].The amount of gold leached from the tuffaceous slate increases with temperature although the effect decreases above about 200℃.  相似文献   

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The Chañarcillo Basin is an Early Cretaceous extensional basin in northern Chile (27–29°S). The folding style of the syn-rift successions along the eastern side of the basin reveals an architecture consisting of a NNE-trending anticline “Tierra Amarilla Anticlinorium”, associated with the inversion of the Elisa de Bordos Fault. A set of balanced cross sections and palinspastic restorations across the basin show that a partially inverted “domino-style” half-graben as the structural framework is most appropriate for reproducing the deformation observed at the surface. This inverted system provides a 9–14 km shortening in the basin. The ages of the synorogenic deposits preserved next to the frontal limb of the “Tierra Amarilla Anticlinorium” suggest that basin inversion occurred close to the “K–T” boundary (“K–T” phase of Andean deformation). We propose that tectonic inversion is the fundamental deformation mechanism, and that it emphasizes the regional importance of inherent Mesozoic extensional systems in the evolution of the northern Chilean Andes.  相似文献   

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ABSTRACT

In many Precambrian provinces, the understanding about the tectonic history is restrained by the limited exposure of rocks so that aerogeophysical data can provide information below the surface cover of sediments, soil, and water to build a tectonic model of the region. However, the tectonic evolution of cratons and shear zones is very complex due to scarce aerogeophysical and geological data. The integrated observation of geology, aerogammaspectrometry, and aeromagnetometry of the Brazilian Shield, states of Santa Catarina, Paraná, and southern São Paulo, is enhanced by a 2011 high-resolution aerogeophysical survey. The Ponta Grossa and Florianópolis dike swarms show two sets of linear high magnetic signal. Peralkaline–carbonatitic complexes are observed in all images, e.g. Jacupiranga, Tunas, and Anitápolis. Three main geotectonic provinces are apparent in the shield. The Dom Feliciano Belt has two domains in terms of radioelements K, Th, and U. This belt includes granitic rocks of the Florianópolis Batholith, Brusque Group schists, and Itajaí Basin of sedimentary and volcanic rocks. The Luís Alves Craton has mostly the Santa Catarina Granulitic Complex and other gneisses. The craton has patches of high emission rates and extends to the northeastern extreme of the studied area with a high-contrast magnetic signal in most of the unit. The Ribeira Belt also has high in gammaspectrometric images, although less homogeneous than the Dom Feliciano Belt. This belt contains granitic complexes, gneisses, and schists and has a low magnetic signal with patches of high analytical signal amplitude. Shear zones delimit different geotectonic units, but are also significant in the Ribeira Belt. The Luís Alves Craton is the most complex unit, as seen in ternary K + eTh + eU images, requiring the future discrimination of small features. This novel study of the Brazilian Shield based on new geophysical data supports the classification of the proposed main geotectonic units.  相似文献   

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Generally, arc-related or subduction-related mafic magmas are formed during or slightly postdate subduction, and characterized by depletion in high field strength elements (HFSEs) relative to the large ion lithophile elements (LILEs) and light rare-earth elements (LREEs). Combining with mineral chemistry and Sr–Nd isotopes, these geochemical characteristics were usually used to define an arc setting, especially for some ancient arcs that had been strongly modified by later tectonic activities. However, we report an exceptional case from the northern part of the Triassic Yidun Arc Belt, eastern Tibetan Plateau. The Ganluogou gabbro (∼152 Ma) occurs as several intrusive bodies. Its mineral assemblage is olivine (chrysolite), plagioclase (anorthite), clinopyroxene (diopside), amphibole (edenite and pargasite) and phlogopite. Whole rock geochemistry shows low SiO2 (42.87–46.99 wt.%), total rear earth elements (ΣREE = 22.8–28.4 ppm), Na2O + K2O (0.92–1.34 wt.%), and high Al2O3, MgO and FeO contents. It has small variations of initial 87Sr/86Sr ((87Sr/86Sr)i = 0.7053–0.7055) and εNd(t) values (−4.8 to −1.8). All the samples exhibit enrichment in LILEs including Th and U, but strongly depleted in HFSEs, including Nb, Ta, Zr and Hf. For the mineral chemistry, there are two type amphiboles. Amp(I) show higher V, Sc, Cr, Sr, Nb and Zr contents, but lower Th and U contents than those of Amp(II). Their REE patterns range from convex shape without Eu anomaly to LREE-enriched pattern with weak positive Eu anomaly. We suggest that Amp(I) was crystallized from a liquid that was mainly buffered by olivine, clinopyroxene and plagioclase, while Amp(II) crystallized from later melt that was mainly buffered by olivine. Based on clinopyroxene chemistry, compositions of coexisting olivine and plagioclase, and whole rock Sr–Nd isotopes, the parental magma of the Ganluogou gabbro is interpreted as a tholeiitic arc-affinity magma, which might be derived from an N-MORB mantle that had been metasomatised by slab-derived melts in the late Triassic (237–206 Ma). Thus, the Ganluogou gabbro provides an example that magmas exhibiting arc-affinity could in fact be formed in a post-orogenic extensional setting.  相似文献   

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Lithium isotope geochemistry is increasingly being used to trace deep-earth processes, reflecting the observed large variation of Li isotope ratios in mantle-derived rocks, including peridotite xenoliths associated with ancient continents. We briefly review the Li isotopic compositions of major geochemical reservoirs, the assumed mechanisms of Li isotopic fractionation, and, in particular, the origins of isotopically light Li in mantle-derived rocks based on the latest developments in Li isotope geochemistry. Comparison of Li isotope data with existing Sr-Nd isotope ratios reflects the subduction-recycling of ancient oceanic crust and the reappearance of Li in volcanic rocks. This circulation may play an important role in generating the isotopically light-Li component in the mantle – perhaps the enriched mantle end member defined by the Sr-Nd isotopic compositions of oceanic basalts.  相似文献   

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The Neoarchaean Epoch nickel sulphide (NiS) deposit, discovered in 1970 and subsequently mined from 1972 to 1998, has been previously interpreted to be a magmatic ore system. However, on the basis of field, petrographic and analytical data obtained during the initial exploration and evaluation stages, integrated with limited new analytical data (SEM and ore microscopy), we propose that the Epoch NiS may be of hydrothermal origin. Key features that have prompted a re-appraisal of the genesis of the Epoch mineralisation, include: a) ore lenses are irregularly distributed along foliation fabrics of the host talc-carbonate rocks and as such no relationship to basal ultramafic/mafic units; b) the thickness of the ore lenses are highly variable from tens of centimetres to several metres; c) ore mineralogy is characterised by dominant millerite–pyrite–chalcopyrite assemblages; and d) high Pd/Pt ratios. Although our hydrothermal model is somewhat speculative, we suggest that on present evidence there is little doubt that the Epoch NiS lacks the features of typical magmatic sulphide deposits. More geochemical and isotopic data are needed to test our model.  相似文献   

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Gold deposits such as the Aketishikan, Togetobie, Tasbig-Kokeydlas, Kums and Hongshanzui gold deposits in the Nurt area in Altay of Xinjiang were found in Member 3 rhyolite tufflava, fragmental lava and ignimbrite of the Carboniferous Hongshanzui Group. Trace and rare earth elements, sulfur, lead, oxygen and hydrogen isotopes, and geochronological studies indicate that the ore-forming material was mostly supplied by the Carboniferous volcanic rocks through water-rock interaction under a low-to-moderate temperature, and the hydrothermal ore-forming fluid came from meteoric water with some magmatic water input evolved from the granitic magmas. Gold deposits in the Nurt area as well as in the northern Altay might form in multiple stages, and the Yanshanian mineralization period should be paid more attention besides the Variscan mineralization period.  相似文献   

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Two distinct groups of granitoids occur on the eastern side of the Kosciusko Batholith. Those considered to be derivatives of sedimentary source rocks (S‐types) are usually foliated and either contain cordierite or white‐mica secondary after cordierite. The granitoids produced from igneous source material (I‐types) are generally massive and frequently contain hornblende. Geochemical parameters provide the best discriminant between the two groups, I‐types have higher Ca, Al, Na2O/K2O, and Fe2O3/FeO, and lower Fe, Mg, Sc, V, Cr, Co, Ni, Cu, Zn, Ba, Rb, Th, La, Ce, and Y than S‐types of comparable SiO2 values.

The differences between the two groups are not the result of differences in the melt‐forming process but reflect differences in the nature of the source material. Thus the geochemical features of the S‐type granitoids are indicative of their source rocks having been through a process of chemical weathering in a sedimentary cycle. Conversely, the I‐type granitoids were derived from fractionated rocks that had not been involved in weathering processes.  相似文献   

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