scholarly journals BACIA PRECURSORA VERSUS BACIAS OROGÊNICAS: EXEMPLOS DO GRUPO ANDRELÂNDIA COM BASE EM DATAÇÕES U-PB (LA-ICP-MS) EM ZIRCÃO E ANÁLISES LITOQUÍMICAS

2013 ◽  
Author(s):  
Juliane Belém ◽  
Antônio Carlos Pedrosa-Soares ◽  
Carlos Maurício Noce ◽  
Luiz Carlos Da Silva ◽  
Richard Armstrong ◽  
...  

Resultados de datações U-Pb (LA-ICP-MS) sobre zircões e análises litoquímicas de amostras de paragnaisse e xisto do Grupo Andrelândia, coletadas desde sua área-tipo até a região de alto grau metamórfico do sistema orogênico Araçuaí-Ribeira, evidenciam que esta extensa unidade estratigráfica inclui representantes de bacia precursora de margem continental passiva, representada pelo Grupo Andrelândia Inferior (paragnaisse de Madre de Deus, Seqüência Carrancas), com idade máxima em ca. 950 Ma e fontes sedimentares diversificadas, datadas do Toniano ao Neoarqueano; e de bacias orogênicas, representadas pela Unidade Santo Antônio do Grupo Andrelândia Superior e paragnaisses de alto grau metamórfico da região de Ubá-Carangola, com idade máxima em torno de 640 Ma e extrema concentração de áreas-fontes neoproterozóicas. As análises litoquímicas apontam para larga predominância de fontes sedimentares situadas em arcos magmáticos, mas a amostra que melhor indica a bacia precursora (o paragnaisse de Madre de Deus, Seqüência Carrancas) tem assinatura similar a depósitos de margem continental passiva. Amostras de paragnaisse migmatítico revelam a idade de ca. 565 Ma para o clímax metamórfico-anatético na zona de fronteira Araçuaí-Ribeira. Destaca-se que o Grupo Andrelândia Superior, na forma como é representado em mapas atuais, incluiria pelo menos duas bacias orogênicas, i.e., uma, na Faixa Brasília e, outra, no sistema Araçuaí-Ribeira.Palavras-chave: geocronologia U-Pb, litoquímica, Grupo Andrelândia ABSTRACT: PRECURSOR BASIN VERSUS OROGENIC BASINS: EXAMPLES FROM THE ANDRELÂNDIA GROUP BASED ON ZIRCON U-Pb (LA-ICP-MS) AND LITHOCHEMICAL ANALYSIS. Results from zircon U-Pb (LA-ICP-MS) and lithochemical analysis on samples from the Andrelândia Group, collected from its type-area to the high grade core of the Araçuaí-Ribeira orogenic system, suggest that this extensive stratigraphic unit includes a precursor passive margin basin, represented by the Lower Andrelândia Group (Madre de Deus paragneiss, Carrancas sequence), with maximum depositional age around 950 Ma and diversified sediment sources dated from the Tonian to Neoarchean; and orogenic basin(s), represented by the Santo Antônio unit of the Upper Andrelândia Group and high grade paragneisses of the Ubá-Carangola region, with a maximum depositional age around 640 Ma and provenance extremely restricted to Neoproterozoic sources. Lithochemical analysis point to a large predominance of sediment sources located in magmatic arcs, but the sample representing the precursor basin shows signature similar to passive margin deposits. High grade paragneisses reveal the age of ca. 565 Ma to the metamorphic-anatectic climax in the Araçuaí-Ribeira boundary zone. It is important to notice that the Upper Andrelândia Group, as represented in current maps, includes at least two orogenic basins, i.e., the older, to the west, in the Brasília belt, and the younger, to the east, in the Araçuaí-Ribeira system.Keywords: U-Pb geochronology, lithochemistry, Andrelândia Group.

2013 ◽  
Author(s):  
Tatiana Gonçalves-Dias ◽  
Antônio Carlos Pedrosa-Soares ◽  
Ivo Antônio Dussin ◽  
Fernando Flecha de Alkmim ◽  
Fabrício Andrade Caxito ◽  
...  

O Complexo Jequitinhonha, situado no nordeste de Minas Gerais, é uma das unidades metassedimentares mais extensas do Orógeno Araçuaí. Na área-tipo, situada na região de Jequitinhonha -Almenara, este complexo consiste de paragnaisse peraluminoso (kinzigítico) migmatizado, com intercalações de quartzito, grafita gnaisse e rocha calcissilicática. Os dados isotópicos U-Pb (LA-ICP-MS) de 80 grãos detríticos de zircão de uma amostra de quartzito, coletada em corte da BR-367 cerca de 12 km a SW de Almenara, permitem identificar seis principais intervalos de idades, cujas médias das modas sugerem as seguintes fontes de sedimentos: o embasamento São Francisco-Congo (2541 ± 8 Ma e 2044 ± 6 Ma), o sistema Espinhaço-Chapada Diamantina (1819 ± 6 Ma, 1487 ± 5 Ma e 1219 ± 3 Ma) e o sistema de rifteamento Noqui-Zadiniano-Mayumbiano-Salto da Divisa (956 ± 4 Ma). A idade máxima de sedimentação em 898 ± 8 Ma é dada pelo zircão mais novo. Os espectros de idades desta amostra do Complexo Jequitinhonha e de rochas do Grupo Macaúbas são muito similares, indicando correlação entre estas unidades. Contudo, no Complexo Jequitinhonha inexiste evidência de glaciação. Assim, o Complexo Jequitinhonha na área-tipo é interpretado como depósito de margem passiva da bacia precursora do Orógeno Araçuaí, mais novo que a glaciação Macaúbas e, portanto, equivalente às formações Chapada Acauã Superior e Ribeirão da Folha.Palavras-chave: Complexo Jequitinhonha, geocronologia U-Pb, Orógeno AraçuaíABSTRACT: MAXIMUM SEDIMENTATION AGE AND PROVENANCE OF THE JEQUITINHONHA COMPLEX IN THE TYPE-AREA (ARAÇUAÍ OROGEN): FIRST U-PB (LA-ICP-MS) DATA FROM DETRITAL ZIRCON GRAINS.The Jequitinhonha Complex is one of the most extensive metasedimentary units of the Araçuaí Orogen. In the type-area, located in the Jequitinhonha-Almenara region, this complex includes migmatized peraluminous (kinzigitic) paragneiss with intercalations of quartzite, graphite gneiss and calcsilicate rock. U-Pb (LA-ICP-MS) data from 80 detrital zircon grains extracted from a quartzite sample, collected in a BR-367 road cut around 12 km SW from Almenara, yielded six main age intervals, which mode mean values suggest the following sediment sources: the São Francisco-Congo basement (2541 ± 8 Ma and 2044 ± 6 Ma), the Espinhaço-Chapada Diamantina system (1819 ± 6 Ma, 1487 ± 5 Ma and 1219 ± 3 Ma), and the Noqui-Zadinian-Mayumbian-Salto da Divisa rift system (956 ± 4 Ma). The maximum sedimentation age of 898 ± 8 Ma is constrained by the youngest zircon grain. Spectra of detrital zircon ages for this sample of the Jequitinhonha Complex and rocks of the Macaúbas Group are very similar and suggest a correlation between these units. However, this complex shows no evidence of glaciation. Therefore, the Jequitinhonha Complex in its type-area is interpreted as a passive margin deposit of the precursor basin of the Araçuaí Orogen, younger than the Macaúbas glaciation and, thus, equivalent of the Upper Chapada Acauã and Ribeirão da Folha formations.Keywords: Jequitinhonha Complex, U-Pb geochronology, Araçuaí Orogen


1971 ◽  
Vol 35 ◽  
pp. 22-23
Author(s):  
T Frisch

The area mapped by the writer is situated to the west of Fiskenæsset and lies in the boundary zone between granulite and amphibolite facies rocks (see Kalsbeek, this report). In the north a creamy- to pink-weathering gneiss, commonly containing hypersthene and biotite is the chief rock type. In the south small-folded, pale-grey weathering biotite-hornblende gneisses are predominant. Amphibolite is of common occurrence in layers, pods and agmatite. The areal extent of the anorthosite-pyribolite complex as previously outlined by reconnaissance mapping (Ghisler & Windley, 1967) was confirmed in general but modified in detail. Additional occurrences of rocks belonging to the complex were found.


1994 ◽  
Vol 131 (2) ◽  
pp. 191-200 ◽  
Author(s):  
G. Warrington ◽  
J. C. W. Cope ◽  
H. C. Ivimey-Cook

AbstractIn 1967 the Somerset coastline near Watchet was proposed as the type area of the basal (Planorbis) chronozone of the Hettangian Stage and thus of the Jurassic System. Neither at that time nor subsequently, however, has a type locality and section been nominated from those available in the area. There is urgent need to select a Global Stratotype Section and Point (GSSP) for the base of the Hettangian, and of the Jurassic System. The cliff forming the headland at the west side of St Audrie's Bay, three kilometres east of Watchet, Somerset, is here proposed as the type locality and section, with the base of the Hettangian Stage, at the base of the Planorbis Chronozone, being placed at the horizon currently recognized as that at which ammonites of the genus Psiloceras appear. In this section the base of the Planorbis Chronozone corresponds with the base of the Psiloceras planorbis Biozone. The proposal of this section is conditioned by the availability of comprehensive litho- and biostratigraphic information, and the ability of the section to fulfil International Commission on Stratigraphy (ICS) requirements for a candidate GSSP.


2013 ◽  
Vol 150 (6) ◽  
pp. 1103-1126 ◽  
Author(s):  
DETA GASSER ◽  
ARILD ANDRESEN

AbstractThe tectonic origin of pre-Devonian rocks of Svalbard has long been a matter of debate. In particular, the origin and assemblage of pre-Devonian rocks of western Spitsbergen, including a blueschist-eclogite complex in Oscar II Land, are enigmatic. We present detrital zircon U–Pb LA-ICP-MS data from six Mesoproterozoic to Carboniferous samples and one U–Pb TIMS zircon age from an orthogneiss from Oscar II Land in order to discuss tectonic models for this region. Variable proportions of Palaeo- to Neoproterozoic detritus dominate the metasedimentary samples. The orthogneiss has an intrusion age of 927 ± 3 Ma. Comparison with detrital zircon age spectra from other units of similar depositional age within the North Atlantic region indicates that Oscar II Land experienced the following tectonic history: (1) the latest Mesoproterozoic sequence was part of a successor basin which originated close to the Grenvillian–Sveconorwegian orogen, and which was intruded byc. 980–920 Ma plutons; (2) the Neoproterozoic sediments were deposited in a large-scale basin which stretched along the Baltoscandian margin; (3) the eclogite-blueschist complex and the overlying Ordovician–Silurian sediments probably formed to the north of the Grampian/Taconian arc; (4) strike-slip movements assembled the western coast of Spitsbergen outside of, and prior to, the main Scandian collision; and (5) the remaining parts of Svalbard were assembled by strike-slip movements during the Devonian. Our study confirms previous models of complex Caledonian terrane amalgamation with contrasting tectonic histories for the different pre-Devonian terranes of Svalbard and particularly highlights the non-Laurentian origin of Oscar II Land.


2015 ◽  
Vol 186 (4-5) ◽  
pp. 331-351 ◽  
Author(s):  
Alexandra Afilhado ◽  
Maryline Moulin ◽  
Daniel Aslanian ◽  
Philippe Schnürle ◽  
Frauke Klingelhoefer ◽  
...  

Abstract Geophysical data acquired on the conjugate margins system of the Gulf of Lion and West Sardinia (GLWS) is unique in its ability to address fundamental questions about rifting (i.e. crustal thinning, the nature of the continent-ocean transition zone, the style of rifting and subsequent evolution, and the connection between deep and surface processes). While the Gulf of Lion (GoL) was the site of several deep seismic experiments, which occurred before the SARDINIA Experiment (ESP and ECORS Experiments in 1981 and 1988 respectively), the crustal structure of the West Sardinia margin remains unknown. This paper describes the first modeling of wide-angle and near-vertical reflection multi-channel seismic (MCS) profiles crossing the West Sardinia margin, in the Mediterranean Sea. The profiles were acquired, together with the exact conjugate of the profiles crossing the GoL, during the SARDINIA experiment in December 2006 with the French R/V L’Atalante. Forward wide-angle modeling of both data sets (wide-angle and multi-channel seismic) confirms that the margin is characterized by three distinct domains following the onshore unthinned, 26 km-thick continental crust : Domain V, where the crust thins from ~26 to 6 km in a width of about 75 km; Domain IV where the basement is characterized by high velocity gradients and lower crustal seismic velocities from 6.8 to 7.25 km/s, which are atypical for either crustal or upper mantle material, and Domain III composed of “atypical” oceanic crust. The structure observed on the West Sardinian margin presents a distribution of seismic velocities that is symmetrical with those observed on the Gulf of Lion’s side, except for the dimension of each domain and with respect to the initiation of seafloor spreading. This result does not support the hypothesis of simple shear mechanism operating along a lithospheric detachment during the formation of the Liguro-Provencal basin.


2021 ◽  
pp. 32-44
Author(s):  
Alexander Tolstov ◽  
Vladimir Cherenkov ◽  
Leonid Baranov

The northeastern Siberian platform (Republic of Sakha, Yakutia) hosts the Udzhinskaya province of alkaline ultrabasic massifs with carbonatites as final phases of magmatic system evolution; they form i ts central carbonatite core and are characterized by elevated Fe, Al and P concentrations. They also contain a complex of rare and rare-earth elements. Crust of laterite weathering of up to 400 m thick is present within the massifs. Phosphate, Nb, Y, Sc and TR content in crust of carbonatite weathering is much higher compared to unaltered rock differences. Their maximum values are in the sequence of specific sedimentary deposits f ormed a s denudation products of ore-bearing carbonatite crust precipitated in minor lake depressions and due to their intensive chemogenic transformation in hot humid climate. They are unique high-grade ores, with no world analogs in terms of mineral potential. Sometimes, these rocks are their natural concentrates averaging (in weight %) 7,21 Nb2O5, 0,578 Y2O3, 0,045 Sc2O3 and 10,16 TR2O3. The rocks composing the ore-bearing sequence show distinct evidence of sedimentary genesis: well-pronounced layered texture and facial zoning, presence of carbonized vegetable detrite and bacteriomorphic aggregates. Therefore, it is reasonable to regard a set of these formations as an independent stratigraphic unit, Tomtor sequence. Geological data suggest that it formed 340-280 Ma. Tomtor sequence can be an important prospecting criteria in prospecting for rare and rare-earth elements.


Minerals ◽  
2019 ◽  
Vol 9 (4) ◽  
pp. 244 ◽  
Author(s):  
Keyser ◽  
Ciobanu ◽  
Cook ◽  
Feltus ◽  
Johnson ◽  
...  

Zirconium is an element of considerable petrogenetic significance but is rarely found in hematite at concentrations higher than a few parts-per-million (ppm). Coarse-grained hematite ore from the metamorphosed Peculiar Knob iron deposit, South Australia, contains anomalous concentrations of Zr and has been investigated using microanalytical techniques that can bridge the micron- to nanoscales to understand the distribution of Zr in the ore. Hematite displays textures attributable to annealing under conditions of high-grade metamorphism, deformation twins (r~85˚ to hematite elongation), relict magnetite and fields of sub-micron-wide inclusions of baddeleyite as conjugate needles with orientation at ~110˚/70˚. Skeletal and granoblastic zircon, containing only a few ppm U, are both present interstitial to hematite. Using laser-ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) spot analysis and mapping, the concentration of Zr in hematite is determined to be ~260 ppm on average (up to 680 ppm). The Zr content is, however, directly attributable to nm-scale inclusions of baddeleyite pervasively distributed throughout the hematite rather than Zr in solid solution. Distinction between nm-scale inclusions and lattice-bound trace element substitutions cannot be made from LA-ICP-MS data alone and requires nanoscale characterization. Scandium-rich (up to 0.18 wt. % Sc2O3) cores in zircon are documented by microprobe analysis and mapping. Using high-angle annular dark field scanning transmission electron microscopy imaging (HAADF-STEM) and energy-dispersive spectrometry STEM mapping of foils prepared in-situ by focused ion beam methods, we identify [011]baddeleyite epitaxially intergrown with [22.1]hematite. Lattice vectors at 84–86˚ underpinning the epitaxial intergrowth orientation correspond to directions of r-twins but not to the orientation of the needles, which display a ~15˚ misfit. This is attributable to directions of trellis exsolutions in a precursor titanomagnetite. U–Pb dating of zircon gives a 206Pb/238U weighted mean age of 1741 ± 49 Ma (sensitive high-resolution ion microprobe U–Pb method). Based on the findings presented here, detrital titanomagnetite from erosion of mafic rocks is considered the most likely source for Zr, Ti, Cr and Sc. Whether such detrital horizons accumulated in a basin with chemical precipitation of Fe-minerals (banded iron formation) is debatable, but such Fe-rich sediments clearly included detrital horizons. Martitization during the diagenesis-supergene enrichment cycle was followed by high-grade metamorphism during the ~1.73–1.69 Ga Kimban Orogeny during which martite recrystallized as granoblastic hematite. Later interaction with hydrothermal fluids associated with ~1.6 Ga Hiltaba-granitoids led to W, Sn and Sb enrichment in the hematite. By reconstructing the evolution of the massive orebody at Peculiar Knob, we show how application of complimentary advanced microanalytical techniques, in-situ and on the same material but at different scales, provides critical constraints on ore-forming processes.


1990 ◽  
Vol 27 (10) ◽  
pp. 1382-1393 ◽  
Author(s):  
Jean Michel Bertrand ◽  
Emmanuel Ferraz Jardim de Sá

The reconstruction of Early Proterozoic crustal evolution and geodynamic environments, in Africa and South America, is incomplete if cratonic areas alone are studied. If the presence of high-grade gneisses is considered as a first clue to past collisional behaviour, 2 Ga high-grade gneisses are more abundant within the Pan-African–Brasiliano mobile belts than in the intervening pre-Late Proterozoic cratons. The West African craton and the Guiana–Amazonia craton consist of relatively small Archaean nuclei and widespread low- to medium-grade volcanic and volcanoclastic formations intruded by Early Proterozoic granites. By contrast, 2 Ga granulitic assemblages and (or) nappes and syntectonic granites are known in several areas within the Pan-African–Brasiliano belts of Hoggar–Iforas–Air, Nigeria, Cameroon, and northeast Brazil. Nappe tectonics have been also described in the Congo–Chaillu craton, and Early Proterozoic reworking of older granulites may have occurred in the São Francisco craton. The location of the Pan-African–Brasiliano orogenic belts is probably controlled by preexisting major structures inherited from the Early Proterozoic. High-grade, lower crustal assemblages 2 Ga old have been uplifted or overthrust and now form polycyclic domains in these younger orogenic belts, though rarely in the cratons themselves. The Congo–Chaillu and perhaps the São Francisco craton are exceptional in showing controversial evidence of collisional Eburnian–Transamazonian assemblages undisturbed during Late Proterozoic time.


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