Heilbron, M; Almeida, J.; Tupinambá, M.; Duarte, B.P.; Valladares, C.; Schmitt, R.; Nogueira, J.R.; Valeriano, C.; Ragatky, D.; Eirado, L.G.; Palermo, N.; Geraldes, M.
TEKTOS/Faculdade de Geologia-UERJ. Rua São Francisco Xavier 524, 4-andar, Bloco A. Rio de Janeiro - RJ, Brasil. heilbron@uerj ABSTRACT Key-words: Ribeira belt, SE-Brazil, Western Gondwana, Brasiliano Collage TECTONIC SUBDIVISION The southern tip of the São Francisco craton (SFC) is bordered by the Brasília belt at the western side and by the Ribeira belt at the eastern side. The southern part of the Brasília Orogen has an overall NNW-SSE trend and is subdivided in nappes with tectonic movement to E or ESE, towards the SFC or tangent along its southern border. These nappes result from an early collisional stage (collision I, ca. 630-625 Ma, Trouw et al., 2000, Campos Neto, 2000) On the eastern side, the NE-SW trending Ribeira Orogen results from the interaction between the SFC with microplates to the SE and with the southwestern part of the Congo Craton. Two collisional stages (Collision II, ca. 580 Ma and Collision III, ca. 520 Ma) result on the docking of four northwest vergent terranes (Occidental, Paraíba do Sul, Oriental and Cabo Frio, Heilbron et al. 2000).
NEOPROTEROZOIC SUCCESSIONS: PRECURSOR BASINS OF THE RIBEIRA OROGEN Andrelândia Megasequence of the Occidental terrane: AMS The AMS represent the Neoproterozoic passive margin sucession of the São Francisco paleocontinent. The sucession is subdivided in two sequences (Carrancas, Serra do Turvo), that grade laterally to distal pelagic facies that is virtually indistinguishable (Ribeiro et al., 2003). From bottom to top, the Carrancas Sequence is composed of banded paragneisses with amphibolites, quartzite and grey phyllite intercalations; greenish muscovite-quartzite with minor schist intercalations; and grey graphitic phyllites and schists with quartzite intercalations. The Serra do Turvo Sequence overlaps both the Carrancas Sequence and the basement. The lower part is composed of biotite phyllites and plagioclase-biotite-garnet schists/ gneisses with dropstones of basement fragments. The upper part contains similar schists and gneisses, with a stratified appearance due to intercalations of amphibolite, quartzite, garnet-rich metachert and calcsilicate rocks. The paleoenvironment interpretation points to deposition in a passive margin basin with shelf deposits grading to more distal deep marine turbidites with transitions to ocean floor sediments and igneous rocks (Paciullo et al., 2000). The chemistry of the AMS amphibolites indicates a transition from continental to transitional oceanic environment, with TDM model ages of 1.20 and 1.05 Ga. U-Pb data from detrital zircons reveal essentially Paleoproterozoic sources, with subordinate Archean and Mesoproterozoic contribution (Valladares et al., 2001). The age of the youngest detrital zircon (ca. 900 Ma, Valeriano et al., 2004) and the metamorphic ages of the Brasília (ca. 630-580 Ma) and Ribeira (ca. 605-560 Ma) orogens constrain the depositional age of the MAS
Metasedimentary Units of the Paraíba do Sul and Oriental Terranes The metasediments that outcrop in the Paraíba do Sul and Oriental terranes comprise a succession of pelitic and psammitic rocks, with carbonatic and calc-silicate intercalations. The metasediments from the Paraíba do Sul Terrane are essentially composed of two main lithotypes: psammitic biotite gneisses and pelitic sillimanite-biotite gneisses. Garnet and tourmaline are common especially in the pelitic gneisses. Centimetric to metric lenses of calc-silicate rock, sillimanite quartz schist, garnet rich metachert and impure marble are frequent. Distinct metasedimentary successions occur in the three structural domains of the Oriental Terrane. It is possible that the metasedimentary successions of the Oriental Terrane represent a carbonate passive margin of a continent opposed to the SFP. The successions were intruded by Neoproterozoic magmatic arc rocks showing the transition from passive to active margin as a consequence of the initiation of subduction (Heilbron & Machado, 2003). Migmatitic garnet-biotite gneisses with lenses of dolomitic olivine marble and calcsilicate rocks occur in the Cambuci Domain. Lenses of basic rocks, metamorphosed to garnet-diopside granulites are also abundant. The leucosomes of the migmatites are locally charnockitic in composition. U-Pb data from detrital zircons indicate sources from the basement and from a Neoproterozoic magmatic arc (Heilbron & Machado, 2003). In the Costeiro Domain peraluminous gneisses, rich in garnet, sillimanite and locally containing cordierite are predominant. This succession contains many intercalations of up to about 10 m thick of impure quartzite, banded biotite gneisses, calcsilicate rocks and amphibolites. Detrital zircon ages from the quartzites indicate sources from Archean to Neoproterozoic (Valladares et al., 2001). The metasedimentary succession of the Italva Domain includes banded biotite gneisses, calcitic marbles, amphibolites and amphibole schists. The succession is interpreted as representing a shelf environment with basaltic volcanism, now metamorphosed to amphibolite facies. The U-Pb zircon age of ca. 840 Ma, from amphibolite, is the best estimate for the depositional age of this succession (Heilbron and Machado, 2003). Búzios-Palmital Sucession of the Cabo Frio terraneThe Búzios succession is composed of sillimanite-kyanite-garnet-biotite gneisses with K-feldspar and abundant intercalations of calc-silicate layers and amphibolite lenses and layers. Sillimanite-garnet-biotite gneisses with intercalations of calcsilicate rocks and garnet quartzites predominantly compose the Palmital Succession. U-Pb (SHRIMP) ages of detrital zircon from this succession showed the following sources: Archean (ca. 2.5 Ga); Paleoproterozoic (ca. 2.0 Ga); and Neoproterozoic (ca. 1.0 Ga and ca. 800-600 Ma; Schmitt et al., 2003). The lithological composition, available geochronological data and geographic position of the successions, all point to deposition in a Neoproterozoic back-arc basin related to the arc (Heilbron & Machado, 2003). NEOPROTEROZOIC-CAMBRIAN CONVERGENCEThe region described here shows clearly the diachronous nature of the different stages of the Brasiliano Orogeny, both in the Ribeira and the southern Brasília orogens. It results from the progressive collision of the following continents: Paranapanema, SF-Congo, Oriental and Cabo Frio. In both orogens, subduction of oceanic lithosphere leads to the formation of continental volcanic arcs. The collisional stage in the southern Brasília Orogen took place around ca. 630 Ma (Collision I), whereas in the Ribeira Orogen it happened at ca. 580-560 Ma (Collision II). Collision II affected also the southern extreme of the recently structured Brasília Orogen, leading to the complex Zone of Interference between the two orogens. Finally, a third collision (Collision III) took place between the Cabo Frio and Oriental terranes at ca. 520-510 Ma.
Subduction of the Adamastor OceanMagmatic arc rocks that testify pre-collisional subduction in the Ribeira Orogen are located in the Oriental Terrane. The subduction was probably towards E-SE producing the Rio Negro Magmatic Arc. Only the plutonic portion of this arc is preserved; it is composed of calc-alkaline tonalitic to granitic orthogneisses with associated gabbros. They intruded into paragneisses of the Costeiro Domain that probably represent the distal (turbiditic) part of the passive margin of the Oriental Terrane paleocontinent. Geochemical and isotopic data suggest at least two stages for the development of this arc: ca. 790 Ma and ca. 635-620 Ma. Important features of this arc are that the Pb isotopic data reveal the absence of a Paleoproterozoic or older inheritance and that the Nd data indicate two groups of rocks with contrasting levels of crustal contamination. U-Pb data suggest that the arc was a source area for the sediments of the Cambuci Domain (fore-arc basin?) and for the younger units of the Costeiro Domain (back-arc?), demonstrating that the sedimentation was coeval with the subduction process.Collision
II: ca. 590-560 Ma
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