Mineralogia e Petrologia de xenólitos mantélicos da Província Kimberlitica de Juína, MT

Estudos petrográficos, mineralógicos e isotópicos (radiogênicos (Sm/Nd) realizados em xenólitos mantélicos registrados em kimberlitos de Juína sugerem que o manto superior abaixo dessa região é composicionalmente estratificado e composto principalmente de peridotitos e eclogitos. Entre os xenólitos encontrados, peridotitos são os mais abundantes e representados por granada peridotitos e granada \'+OU-\'espinélio peridotitos. Granada \'+OU-\' espinélio peridotitos exibem texturas equigranulares e intensa silicificação substituindo olivina e ortopiroxênio por quartzo criptocristalino, assim podendo ser subdivididos em granada \'+OU-\' espinélio peridotitos com assinatura de eclogitos (GEPE) e granada \'+OU-\' espinélio peridotitos silicificado (GEPS). GEPE exibem abundantes agulhas de rutilos incluídas em clinopiroxênios(CPX) e granadas(GRT). Nestes xenólitos ocorrem os CPX com os maiores conteúdos de \'AL IND.2\'\'O IND.3\' e as GRT com os menores teores de CaO de todos os peridotitos. GEPE apresentam elevado conteúdo de elementos incompatíveis, e (até 2.313 vezes ao do manto primitivo) e enriquecimento em ETRs leves nos CPX, com [\'La/Yb] IND.N\'\'>OU=\'1. São caracterizados por equilíbrio em temperaturas (881 a 907°C) e pressões (26 a 33 kbar) relativamente baixas. Mostram valores negativos de \'\'épsilon\'IND. Nd\'(-11,06) e idade modelo (\'T IND.DM\') de 1.884 Ma. GEPS representam os xenólitos mais abundantes dos peridotitos. Contêm menores inclusões de rutilo e forte modificação por processo de silicificação. Apresenta CPX com maior conteúdo de MgO e enriquecimento nos incompatíveis e ETRs [\'La/Yb] IND.N\'\'>OU=\'1, e GRT com conteúdo intermediário de \'Cr IND.2\'\'O IND.3\' e empobrecimento em ETRs pesados [\'Dy/Yb] IND.N\' OU=\'1. Are characterized by balance in temperature (881 to 907°C) and pressures (26 to 33 kbar) relatively low. Show negative values of \'\'épsilon\'IND. Nd\' ( -11.06) and age model (TDM) of 1,884 Ma. GEPS represent the most abundant xenoliths of peridotite. Contain rutile inclusions and strong minor modification by silicification process. Presents more MgO content CPX and enrichment in incompatible and ETRs [\'La/Yb] IND.N\'\'>OR=\'1, and GRT intermediate content of Cr2O3 and impoverishment in heavy ETRs [\'Dy/Yb] IND.N\' < 1, compared to others. Were equilibradoss in temperatures and pressures respectively between 1077 the 1353° C 50 to 63 and kbares. Show negative values of \'épsilon\'Nd (-8.35 to -11.31) and age model (TDM) of 1,842 the 1114 Ma. Garnet peridotite with textures 1 and 2 (GPT1 and GPT2) exhibit severe deformation textures, with formation of neoblastos of olivine. GPT1 shows more enriched in olivine porfiroclasto and lower contents of garnet, with higher CaO content in the CPX, while the GRT GPT2 is more enriched in TiO2. GT1 and GT2 have the smallest contents of incompatible elements (ETRL ~ 10 times the chondrite) of peridotite. The equilibrium temperatures and pressures were between 1084 and 1473 ºC, and 37 to 58 kbars for GPT1, respectively, and 1263 to 1408°C and 40 to 60 Kbars for GPT2. Show negative values of \'épsilon\'Nd (-3.24) and age model (TDM) of 1,242 Ma.The high content of incompatible elements, with enrichment of light in CPX and ETRs impoverishment in GRT, suggests that the xenoliths represent a enriched mantle source type, with negative \'épsilon\'Nd and Sm/Nd < 1. It could be inferred that these were formed by igneous fractionation peridotite in the upper mantle, then lithosphere for GEPS and GEPE and asthenosphere for GPT1 and GPT2, being basaltic liquid extraction residue (e.g. Group volcanic Roosevelt). Metasomatized peridotite (MARID) represent the crystallization of metasomatic minerals (Modal) and anomalous enrichment of trace elements and ETRs, and it could be associated with a concomitant with the event source carbonatitic-kimberlitic. Xenoliths of eclogite are rare and they can be divided into three groups: i)bi-minerálicos Eclogite (EB), ii) Orthopyroxene-rutile eclogite (ORE); and iii) Sanidinequartz-coesite eclogite (SQC). The modal content of garnet increases of the ORE for EB to SQC. In this same sense is an increase of grossularite molecule in garnet and Al2O3 in clinopyroxene. EB and ORE present chemical composition of group. A or Group I eclogite. SQC have composition similar to group B or II. Exhibit isotopic variables from positive reasons \'épsilon\'Nd + 0.16 (ORE) until negative values high \'épsilon\'Nd -13.03 (EB), and age model (TDM) between 1166 to 1648 Ma.The internal isochrone CPX and GRT, and two whole rock eclogites (EB and ORE) presented a crystallization age and/or recrystallization of 200 Ma, corroborating the hypothesis that the eclogite were formed by the subduction of oceanic crust (Proto) at the bottom of the supercontinent of Gondwana during the Mesozoic.However, do not rule out the hypothesis that the eclogite (EB and ORE) could be considered cumulus of high-pressure igneous and/or melting basaltic liquid residue during mesoproterozoics events.The megacristais suite (LICPX) features low Cr content, with affinity to eclogite. Can be interpreted as formed during the co-precipitation of low chromium clinopyroxene and picroilmenite, below temperatures between1264° C and 1308° C in a liquid proto-kimberlitic