Geological, geophysical and morphological study of the circular structure of SÃo Miguel do Tapuio , Piaui , Brazil

Detalhes bibliográficos
Autor(a) principal: Jackson Alves Martins
Data de Publicação: 2016
Tipo de documento: Tese
Idioma: por
Título da fonte: Biblioteca Digital de Teses e Dissertações da UFC
Texto Completo: http://www.teses.ufc.br/tde_busca/arquivo.php?codArquivo=17050
Resumo: The SÃo Miguel do Tapuio Circular Structure (SMTCS) is a remarkable geomorphological feature with 20 km diameter recognized in Mesopaleozoic sandstones of ParnaÃba Basin (Piauà State, Brazil). Studies concerning the origin of the SMTCS are divided between an endogenous origin and other caused by a meteoritic impact. In this study, we performed an extensive bibliographic research, analysis of the previous cartographic studies, field geology and laboratory works (remote sensing, geophysics, topography, petrography and geochronology). The remote sensing data were used to delineate the superficial morphological configuration of the structure, its diameter and compartments, as well as the ring pattern of drainage and the multi-directional pattern of the relief. The information of gravimetric and topographic surveys shows the shallow nature of SMTCS with ~ 1.4 km depth, there is a strong correlation with the theoretical model of the complex type impact structures, there are no regional anomalies associated with a non-outcropping igneous body and the positive Bouguer anomaly observed in one of the profiles is consistent with the observed gravity anomalies in large craters. The petrographic studies did not allow us any identification of typical structural or textural features of a clear impact origin. However, it was found features that could vaguely be regarded as shatter cones and also indicative of micro-deformational features of meteoritic impact (Planar Fractures (PFs), Feather Features (FFs) and Healed Fractures (HFs)), possibly associated with an inferior position to the strongest deformation zone of the structure. The structure core sandstones thermal metamorphism characterizes intense recrystallization and elimination of all previous matrix. They have thrust listric faults with steep dip converging to the structure central point and suggest to be penetrative in shallow subsurface character, highlighting the remarkable correlation with the 2D Euler deconvolution products. The geochronological results from U-Pb not allowed to find the ages of possible isotopic imbalances that could possibly be related to SMTCS (< 400 Ma), but marked the crystallization ages of the zircons and their source areas, with Paleoproterozoic influence (~2200-1800Ma), Upper Mesoproterozoic (~1200-900 Ma) and Neoproterozoic (~800-550 Ma). Finally, it was concluded that although it was not found unequivocal petrographic-mineralogical features of impact processes, all the evidence and characteristics obtained in this research suggests an exogenous source for SMTCS. The current surface may represent the lower portion of an ancient crater, in this related to an astrobleme.
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spelling info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/doctoralThesisGeological, geophysical and morphological study of the circular structure of SÃo Miguel do Tapuio , Piaui , BrazilEstudo geolÃgico, geofÃsico e morfolÃgico da estrutura circular de SÃo Miguel do Tapuio, PiauÃ, Brasil2016-04-28Raimundo Mariano Gomes Castelo Branco13240005387http://buscatextual.cnpq.br/buscatextual/visualizacv.jsp?id=K4781605D2Josà de AraÃjo Nogueira Neto13957791391http://lattes.cnpq.br/0273671687486902Mariano de Franca Alencar Neto77832884304http://lattes.cnpq.br/3538573584743629Christiano Magini52365751415http://lattes.cnpq.br/1966952635205319MARCELO HENRIQUE LEÃO SANTOS 84209143120http://lattes.cnpq.br/543538060818110162031082353 http://lattes.cnpq.br/4286714933399280Jackson Alves MartinsUniversidade Federal do CearÃPrograma de PÃs-GraduaÃÃo em GeologiaUFCBRGeologia regional GeofÃsica GeocronologiaSensoriamento remotoBacia do ParnaÃbaAstroblemaSensoriamento remotoGeofÃsica GeocronologiaGEOLOGIAThe SÃo Miguel do Tapuio Circular Structure (SMTCS) is a remarkable geomorphological feature with 20 km diameter recognized in Mesopaleozoic sandstones of ParnaÃba Basin (Piauà State, Brazil). Studies concerning the origin of the SMTCS are divided between an endogenous origin and other caused by a meteoritic impact. In this study, we performed an extensive bibliographic research, analysis of the previous cartographic studies, field geology and laboratory works (remote sensing, geophysics, topography, petrography and geochronology). The remote sensing data were used to delineate the superficial morphological configuration of the structure, its diameter and compartments, as well as the ring pattern of drainage and the multi-directional pattern of the relief. The information of gravimetric and topographic surveys shows the shallow nature of SMTCS with ~ 1.4 km depth, there is a strong correlation with the theoretical model of the complex type impact structures, there are no regional anomalies associated with a non-outcropping igneous body and the positive Bouguer anomaly observed in one of the profiles is consistent with the observed gravity anomalies in large craters. The petrographic studies did not allow us any identification of typical structural or textural features of a clear impact origin. However, it was found features that could vaguely be regarded as shatter cones and also indicative of micro-deformational features of meteoritic impact (Planar Fractures (PFs), Feather Features (FFs) and Healed Fractures (HFs)), possibly associated with an inferior position to the strongest deformation zone of the structure. The structure core sandstones thermal metamorphism characterizes intense recrystallization and elimination of all previous matrix. They have thrust listric faults with steep dip converging to the structure central point and suggest to be penetrative in shallow subsurface character, highlighting the remarkable correlation with the 2D Euler deconvolution products. The geochronological results from U-Pb not allowed to find the ages of possible isotopic imbalances that could possibly be related to SMTCS (< 400 Ma), but marked the crystallization ages of the zircons and their source areas, with Paleoproterozoic influence (~2200-1800Ma), Upper Mesoproterozoic (~1200-900 Ma) and Neoproterozoic (~800-550 Ma). Finally, it was concluded that although it was not found unequivocal petrographic-mineralogical features of impact processes, all the evidence and characteristics obtained in this research suggests an exogenous source for SMTCS. The current surface may represent the lower portion of an ancient crater, in this related to an astrobleme.A Estrutura Circular de SÃo Miguel do Tapuio (ECSMT) à uma notÃvel e marcante anomalia geomorfolÃgica com diÃmetro de ~20 km, registrada nos arenitos mesopaleozoicos da Bacia do ParnaÃba, Estado do PiauÃ, Brasil. Os estudos que consideram a gÃnese da ECSMT dividem-se entre uma origem endÃgena e uma de impacto meteorÃtico. No presente estudo foram realizados trabalhos envolvendo a anÃlise bibliogrÃfica e cartografia existentes, de campo e laboratoriais (sensoriamento remoto, gravimetria, topografia, petrografia e geocronologia). Os trabalhos de sensoriamento remoto serviram para delinear em detalhe a configuraÃÃo morfolÃgica superficial, o diÃmetro total e compartimentos, bem como o padrÃo de drenagem anelar e multidirecional dos lineamentos de relevo. As informaÃÃes dos levantamentos gravimÃtrico e topogrÃfico serviram para mostrar o carÃter raso da ECSMT com ~1,4 km de profundidade, que existe forte correlaÃÃo com o modelo teÃrico de estruturas de impacto do tipo complexa, que nÃo existem anomalias regionais associadas a um corpo Ãgneo nÃo aflorante e que a anomalia Bouguer positiva observada em um dos perfis à compatÃvel com as anomalias gravimÃtricas observadas em grandes crateras. Os trabalhos petrogrÃficos nÃo permitiram encontrar feiÃÃes estruturais e texturais que pudessem ser seguramente interpretadas como de choque. Entretanto, foram encontradas feiÃÃes que lembram "shatter cones" e ainda feiÃÃes microdeformacionais indicativas de impacto meteorÃtico (Planar Fractures (PFs), Feather Features (FFs) e Healed Fractures (HFs)), possivelmente associadas a uma posiÃÃo inferior à zona de mais intensa deformaÃÃo da estrutura. O metamorfismo termal observado nos metarenitos do nÃcleo da estrutura caracteriza intensa recristalizaÃÃo e eliminaÃÃo de matriz previa. Os mesmos apresentam falhas lÃstricas com mergulho Ãngreme e convergindo para ponto central da estrutura e sugerem serem penetrativas em carÃter raso subsuperficial, com destaque para a notÃvel correlaÃÃo com os produtos de deconvoluÃÃo de Euler 2D. Os resultados geocronolÃgicos atravÃs do U-Pb nÃo permitiram encontrar idades relacionadas à possÃveis desequilÃbrios isotÃpicos que eventualmente poderiam ser correlacionados à ECSMT (< 400 Ma), e sim marcaram Ãs idades de cristalizaÃÃo dos zircÃes e suas Ãreas fontes, com influÃncia paleoproterozÃica (~2200 a 1800 Ma), mesoproterozoico superior (~1200 â 900 Ma) e neoproterozoico (~800 a 550 Ma). Desta forma, conclui-se, que embora nÃo tenham sido encontradas feiÃÃes inequÃvocas dos processos de impacto, todas as caracterÃsticas observadas e levantadas nesta pesquisa sÃo compatÃveis com estruturas de impacto jà confirmadas, atribuindo assim uma origem exÃgena para a ECSMT. A atuaÃÃo dos processos erosivos pode representar hoje um nÃvel inferior da superfÃcie da cratera inicial, tratando-se de um astroblema.CoordenaÃÃo de AperfeÃoamento de Pessoal de NÃvel Superior http://www.teses.ufc.br/tde_busca/arquivo.php?codArquivo=17050application/pdfinfo:eu-repo/semantics/openAccessporreponame:Biblioteca Digital de Teses e Dissertações da UFCinstname:Universidade Federal do Cearáinstacron:UFC2019-01-21T11:30:25Zmail@mail.com -
dc.title.en.fl_str_mv Geological, geophysical and morphological study of the circular structure of SÃo Miguel do Tapuio , Piaui , Brazil
dc.title.alternative.pt.fl_str_mv Estudo geolÃgico, geofÃsico e morfolÃgico da estrutura circular de SÃo Miguel do Tapuio, PiauÃ, Brasil
title Geological, geophysical and morphological study of the circular structure of SÃo Miguel do Tapuio , Piaui , Brazil
spellingShingle Geological, geophysical and morphological study of the circular structure of SÃo Miguel do Tapuio , Piaui , Brazil
Jackson Alves Martins
Geologia regional
GeofÃsica
Geocronologia
Sensoriamento remoto
Bacia do ParnaÃba
Astroblema
Sensoriamento remoto
GeofÃsica
Geocronologia
GEOLOGIA
title_short Geological, geophysical and morphological study of the circular structure of SÃo Miguel do Tapuio , Piaui , Brazil
title_full Geological, geophysical and morphological study of the circular structure of SÃo Miguel do Tapuio , Piaui , Brazil
title_fullStr Geological, geophysical and morphological study of the circular structure of SÃo Miguel do Tapuio , Piaui , Brazil
title_full_unstemmed Geological, geophysical and morphological study of the circular structure of SÃo Miguel do Tapuio , Piaui , Brazil
title_sort Geological, geophysical and morphological study of the circular structure of SÃo Miguel do Tapuio , Piaui , Brazil
author Jackson Alves Martins
author_facet Jackson Alves Martins
author_role author
dc.contributor.advisor1.fl_str_mv Raimundo Mariano Gomes Castelo Branco
dc.contributor.advisor1ID.fl_str_mv 13240005387
dc.contributor.advisor1Lattes.fl_str_mv http://buscatextual.cnpq.br/buscatextual/visualizacv.jsp?id=K4781605D2
dc.contributor.referee1.fl_str_mv Josà de AraÃjo Nogueira Neto
dc.contributor.referee1ID.fl_str_mv 13957791391
dc.contributor.referee1Lattes.fl_str_mv http://lattes.cnpq.br/0273671687486902
dc.contributor.referee2.fl_str_mv Mariano de Franca Alencar Neto
dc.contributor.referee2ID.fl_str_mv 77832884304
dc.contributor.referee2Lattes.fl_str_mv http://lattes.cnpq.br/3538573584743629
dc.contributor.referee3.fl_str_mv Christiano Magini
dc.contributor.referee3ID.fl_str_mv 52365751415
dc.contributor.referee3Lattes.fl_str_mv http://lattes.cnpq.br/1966952635205319
dc.contributor.referee4.fl_str_mv MARCELO HENRIQUE LEÃO SANTOS
dc.contributor.referee4ID.fl_str_mv 84209143120
dc.contributor.referee4Lattes.fl_str_mv http://lattes.cnpq.br/5435380608181101
dc.contributor.authorID.fl_str_mv 62031082353
dc.contributor.authorLattes.fl_str_mv http://lattes.cnpq.br/4286714933399280
dc.contributor.author.fl_str_mv Jackson Alves Martins
contributor_str_mv Raimundo Mariano Gomes Castelo Branco
Josà de AraÃjo Nogueira Neto
Mariano de Franca Alencar Neto
Christiano Magini
MARCELO HENRIQUE LEÃO SANTOS
dc.subject.por.fl_str_mv Geologia regional
GeofÃsica
Geocronologia
Sensoriamento remoto
Bacia do ParnaÃba
Astroblema
Sensoriamento remoto
GeofÃsica
Geocronologia
topic Geologia regional
GeofÃsica
Geocronologia
Sensoriamento remoto
Bacia do ParnaÃba
Astroblema
Sensoriamento remoto
GeofÃsica
Geocronologia
GEOLOGIA
dc.subject.cnpq.fl_str_mv GEOLOGIA
dc.description.sponsorship.fl_txt_mv CoordenaÃÃo de AperfeÃoamento de Pessoal de NÃvel Superior
dc.description.abstract.por.fl_txt_mv The SÃo Miguel do Tapuio Circular Structure (SMTCS) is a remarkable geomorphological feature with 20 km diameter recognized in Mesopaleozoic sandstones of ParnaÃba Basin (Piauà State, Brazil). Studies concerning the origin of the SMTCS are divided between an endogenous origin and other caused by a meteoritic impact. In this study, we performed an extensive bibliographic research, analysis of the previous cartographic studies, field geology and laboratory works (remote sensing, geophysics, topography, petrography and geochronology). The remote sensing data were used to delineate the superficial morphological configuration of the structure, its diameter and compartments, as well as the ring pattern of drainage and the multi-directional pattern of the relief. The information of gravimetric and topographic surveys shows the shallow nature of SMTCS with ~ 1.4 km depth, there is a strong correlation with the theoretical model of the complex type impact structures, there are no regional anomalies associated with a non-outcropping igneous body and the positive Bouguer anomaly observed in one of the profiles is consistent with the observed gravity anomalies in large craters. The petrographic studies did not allow us any identification of typical structural or textural features of a clear impact origin. However, it was found features that could vaguely be regarded as shatter cones and also indicative of micro-deformational features of meteoritic impact (Planar Fractures (PFs), Feather Features (FFs) and Healed Fractures (HFs)), possibly associated with an inferior position to the strongest deformation zone of the structure. The structure core sandstones thermal metamorphism characterizes intense recrystallization and elimination of all previous matrix. They have thrust listric faults with steep dip converging to the structure central point and suggest to be penetrative in shallow subsurface character, highlighting the remarkable correlation with the 2D Euler deconvolution products. The geochronological results from U-Pb not allowed to find the ages of possible isotopic imbalances that could possibly be related to SMTCS (< 400 Ma), but marked the crystallization ages of the zircons and their source areas, with Paleoproterozoic influence (~2200-1800Ma), Upper Mesoproterozoic (~1200-900 Ma) and Neoproterozoic (~800-550 Ma). Finally, it was concluded that although it was not found unequivocal petrographic-mineralogical features of impact processes, all the evidence and characteristics obtained in this research suggests an exogenous source for SMTCS. The current surface may represent the lower portion of an ancient crater, in this related to an astrobleme.
A Estrutura Circular de SÃo Miguel do Tapuio (ECSMT) à uma notÃvel e marcante anomalia geomorfolÃgica com diÃmetro de ~20 km, registrada nos arenitos mesopaleozoicos da Bacia do ParnaÃba, Estado do PiauÃ, Brasil. Os estudos que consideram a gÃnese da ECSMT dividem-se entre uma origem endÃgena e uma de impacto meteorÃtico. No presente estudo foram realizados trabalhos envolvendo a anÃlise bibliogrÃfica e cartografia existentes, de campo e laboratoriais (sensoriamento remoto, gravimetria, topografia, petrografia e geocronologia). Os trabalhos de sensoriamento remoto serviram para delinear em detalhe a configuraÃÃo morfolÃgica superficial, o diÃmetro total e compartimentos, bem como o padrÃo de drenagem anelar e multidirecional dos lineamentos de relevo. As informaÃÃes dos levantamentos gravimÃtrico e topogrÃfico serviram para mostrar o carÃter raso da ECSMT com ~1,4 km de profundidade, que existe forte correlaÃÃo com o modelo teÃrico de estruturas de impacto do tipo complexa, que nÃo existem anomalias regionais associadas a um corpo Ãgneo nÃo aflorante e que a anomalia Bouguer positiva observada em um dos perfis à compatÃvel com as anomalias gravimÃtricas observadas em grandes crateras. Os trabalhos petrogrÃficos nÃo permitiram encontrar feiÃÃes estruturais e texturais que pudessem ser seguramente interpretadas como de choque. Entretanto, foram encontradas feiÃÃes que lembram "shatter cones" e ainda feiÃÃes microdeformacionais indicativas de impacto meteorÃtico (Planar Fractures (PFs), Feather Features (FFs) e Healed Fractures (HFs)), possivelmente associadas a uma posiÃÃo inferior à zona de mais intensa deformaÃÃo da estrutura. O metamorfismo termal observado nos metarenitos do nÃcleo da estrutura caracteriza intensa recristalizaÃÃo e eliminaÃÃo de matriz previa. Os mesmos apresentam falhas lÃstricas com mergulho Ãngreme e convergindo para ponto central da estrutura e sugerem serem penetrativas em carÃter raso subsuperficial, com destaque para a notÃvel correlaÃÃo com os produtos de deconvoluÃÃo de Euler 2D. Os resultados geocronolÃgicos atravÃs do U-Pb nÃo permitiram encontrar idades relacionadas à possÃveis desequilÃbrios isotÃpicos que eventualmente poderiam ser correlacionados à ECSMT (< 400 Ma), e sim marcaram Ãs idades de cristalizaÃÃo dos zircÃes e suas Ãreas fontes, com influÃncia paleoproterozÃica (~2200 a 1800 Ma), mesoproterozoico superior (~1200 â 900 Ma) e neoproterozoico (~800 a 550 Ma). Desta forma, conclui-se, que embora nÃo tenham sido encontradas feiÃÃes inequÃvocas dos processos de impacto, todas as caracterÃsticas observadas e levantadas nesta pesquisa sÃo compatÃveis com estruturas de impacto jà confirmadas, atribuindo assim uma origem exÃgena para a ECSMT. A atuaÃÃo dos processos erosivos pode representar hoje um nÃvel inferior da superfÃcie da cratera inicial, tratando-se de um astroblema.
description The SÃo Miguel do Tapuio Circular Structure (SMTCS) is a remarkable geomorphological feature with 20 km diameter recognized in Mesopaleozoic sandstones of ParnaÃba Basin (Piauà State, Brazil). Studies concerning the origin of the SMTCS are divided between an endogenous origin and other caused by a meteoritic impact. In this study, we performed an extensive bibliographic research, analysis of the previous cartographic studies, field geology and laboratory works (remote sensing, geophysics, topography, petrography and geochronology). The remote sensing data were used to delineate the superficial morphological configuration of the structure, its diameter and compartments, as well as the ring pattern of drainage and the multi-directional pattern of the relief. The information of gravimetric and topographic surveys shows the shallow nature of SMTCS with ~ 1.4 km depth, there is a strong correlation with the theoretical model of the complex type impact structures, there are no regional anomalies associated with a non-outcropping igneous body and the positive Bouguer anomaly observed in one of the profiles is consistent with the observed gravity anomalies in large craters. The petrographic studies did not allow us any identification of typical structural or textural features of a clear impact origin. However, it was found features that could vaguely be regarded as shatter cones and also indicative of micro-deformational features of meteoritic impact (Planar Fractures (PFs), Feather Features (FFs) and Healed Fractures (HFs)), possibly associated with an inferior position to the strongest deformation zone of the structure. The structure core sandstones thermal metamorphism characterizes intense recrystallization and elimination of all previous matrix. They have thrust listric faults with steep dip converging to the structure central point and suggest to be penetrative in shallow subsurface character, highlighting the remarkable correlation with the 2D Euler deconvolution products. The geochronological results from U-Pb not allowed to find the ages of possible isotopic imbalances that could possibly be related to SMTCS (< 400 Ma), but marked the crystallization ages of the zircons and their source areas, with Paleoproterozoic influence (~2200-1800Ma), Upper Mesoproterozoic (~1200-900 Ma) and Neoproterozoic (~800-550 Ma). Finally, it was concluded that although it was not found unequivocal petrographic-mineralogical features of impact processes, all the evidence and characteristics obtained in this research suggests an exogenous source for SMTCS. The current surface may represent the lower portion of an ancient crater, in this related to an astrobleme.
publishDate 2016
dc.date.issued.fl_str_mv 2016-04-28
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
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dc.publisher.initials.fl_str_mv UFC
dc.publisher.country.fl_str_mv BR
publisher.none.fl_str_mv Universidade Federal do CearÃ
dc.source.none.fl_str_mv reponame:Biblioteca Digital de Teses e Dissertações da UFC
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