A Method to Refine the Palinspastic Restoration of Late Proterozoic Avalonian-Cadomian Belt
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Assembly, Configuration, and Break-Up History of Rodinia
Author's personal copy Available online at www.sciencedirect.com Precambrian Research 160 (2008) 179–210 Assembly, configuration, and break-up history of Rodinia: A synthesis Z.X. Li a,g,∗, S.V. Bogdanova b, A.S. Collins c, A. Davidson d, B. De Waele a, R.E. Ernst e,f, I.C.W. Fitzsimons g, R.A. Fuck h, D.P. Gladkochub i, J. Jacobs j, K.E. Karlstrom k, S. Lu l, L.M. Natapov m, V. Pease n, S.A. Pisarevsky a, K. Thrane o, V. Vernikovsky p a Tectonics Special Research Centre, School of Earth and Geographical Sciences, The University of Western Australia, Crawley, WA 6009, Australia b Department of Geology, Lund University, Solvegatan 12, 223 62 Lund, Sweden c Continental Evolution Research Group, School of Earth and Environmental Sciences, University of Adelaide, Adelaide, SA 5005, Australia d Geological Survey of Canada (retired), 601 Booth Street, Ottawa, Canada K1A 0E8 e Ernst Geosciences, 43 Margrave Avenue, Ottawa, Canada K1T 3Y2 f Department of Earth Sciences, Carleton U., Ottawa, Canada K1S 5B6 g Tectonics Special Research Centre, Department of Applied Geology, Curtin University of Technology, GPO Box U1987, Perth, WA 6845, Australia h Universidade de Bras´ılia, 70910-000 Bras´ılia, Brazil i Institute of the Earth’s Crust SB RAS, Lermontova Street, 128, 664033 Irkutsk, Russia j Department of Earth Science, University of Bergen, Allegaten 41, N-5007 Bergen, Norway k Department of Earth and Planetary Sciences, Northrop Hall University of New Mexico, Albuquerque, NM 87131, USA l Tianjin Institute of Geology and Mineral Resources, CGS, No. -
A History of Proterozoic Terranes in Southern South America: from Rodinia to Gondwana
+ MODEL GEOSCIENCE FRONTIERS -(-) (2011) 1e9 available at www.sciencedirect.com China University of Geosciences (Beijing) GEOSCIENCE FRONTIERS journal homepage: www.elsevier.com/locate/gsf REVIEW A history of Proterozoic terranes in southern South America: From Rodinia to Gondwana C. Casquet a,*, C.W. Rapela b, R.J. Pankhurst c, E.G. Baldo d, C. Galindo a, C.M. Fanning e, J.A. Dahlquist d, J. Saavedra f a Departamento de Petrologıa y Geoquımica, IGEO (Universidad Complutense, CSIC), 28040 Madrid, Spain b Centro de Investigaciones Geologicas (CONICET-UNLP), 1900 La Plata, Argentina c Visiting Research Associate, British Geological Survey, Keyworth, Nottingham NG12 5GG, United Kingdom d CICTERRA (CONICET-UNC), 5000 Cordoba, Argentina e Research School of Earth Sciences, The Australian National University, Canberra, Australia f Instituto de Agrobiologıa y Recursos Naturales CSIC, 37071 Salamanca, Spain Received 3 August 2011; accepted 8 November 2011 KEYWORDS Abstract The role played by Paleoproterozoic cratons in southern South America from the Mesopro- Paleoproterozoic; terozoic to the Early Cambrian is reconsidered here. This period involved protracted continental amal- Cratons; gamation that led to formation of the supercontinent Rodinia, followed by Neoproterozoic continental Grenvillian; break-up, with the consequent opening of Clymene and Iapetus oceans, and finally continental Neoproterozoic rifting; re-assembly as Gondwana through complex oblique collisions in the Late Neoproterozoic to Early SW Gondwana assembly Cambrian. The evidence for this is based mainly on a combination of precise U-Pb SHRMP dating and radiogenic isotope data for igneous and metamorphic rocks from a large area extending from the Rio de la Plata craton in the east to the Argentine Precordillera in the west and as far north as Arequipa in Peru. -
The Making and Unmaking of a Supercontinent: Rodinia Revisited
Tectonophysics 375 (2003) 261–288 www.elsevier.com/locate/tecto The making and unmaking of a supercontinent: Rodinia revisited Joseph G. Meerta,*, Trond H. Torsvikb a Department of Geological Sciences, University of Florida, 241 Williamson Hall, PO Box 11210 Gainesville, FL 32611, USA b Academy of Sciences (VISTA), c/o Geodynamics Center, Geological Survey of Norway, Leif Eirikssons vei 39, Trondheim 7491, Norway Received 11 April 2002; received in revised form 7 January 2003; accepted 5 June 2003 Abstract During the Neoproterozoic, a supercontinent commonly referred to as Rodinia, supposedly formed at ca. 1100 Ma and broke apart at around 800–700 Ma. However, continental fits (e.g., Laurentia vs. Australia–Antarctica, Greater India vs. Australia– Antarctica, Amazonian craton [AC] vs. Laurentia, etc.) and the timing of break-up as postulated in a number of influential papers in the early–mid-1990s are at odds with palaeomagnetic data. The new data necessitate an entirely different fit of East Gondwana elements and western Gondwana and call into question the validity of SWEAT, AUSWUS models and other variants. At the same time, the geologic record indicates that Neoproterozoic and early Paleozoic rift margins surrounded Laurentia, while similar-aged collisional belts dissected Gondwana. Collectively, these geologic observations indicate the breakup of one supercontinent followed rapidly by the assembly of another smaller supercontinent (Gondwana). At issue, and what we outline in this paper, is the difficulty in determining the exact geometry of the earlier supercontinent. We discuss the various models that have been proposed and highlight key areas of contention. These include the relationships between the various ‘external’ Rodinian cratons to Laurentia (e.g., Baltica, Siberia and Amazonia), the notion of true polar wander (TPW), the lack of reliable paleomagnetic data and the enigmatic interpretations of the geologic data. -
U-Pb Geochronologic Evidence for the Evolution of the Gondwanan Margin of the North-Central Andes
U-Pb geochronologic evidence for the evolution of the Gondwanan margin of the north-central Andes David M. Chew† Urs Schaltegger Department of Mineralogy, University of Geneva, Rue des Maraîchers 13, 1205 Geneva, Switzerland Jan Košler Department of Earth Science, University of Bergen, Allegaten 41, N-5007 Bergen, Norway Martin J. Whitehouse Laboratory for Isotope Geology, Swedish Museum of Natural History, S-104 05 Stockholm, Sweden Marcus Gutjahr Institute for Isotope Geology and Mineral Resources, ETH-Zentrum, Clausiusstrasse 25, CH-8092 Zürich, Switzerland Richard A. Spikings Aleksandar Miškovi´c Department of Mineralogy, University of Geneva, Rue des Maraîchers 13, 1205 Geneva, Switzerland ABSTRACT zircon overgrowths from amphibolite-facies limited because they are either obscured by later schists, which reveals metamorphic events tectonic events along the convergent margin or We investigated the Neoproterozoic–early at ca. 478 and ca. 312 Ma and refutes the buried by the ubiquitous volcanic cover. Paleozoic evolution of the Gondwanan mar- previously assumed Neoproterozoic age for This problem is particularly acute in the gin of the north-central Andes by employing orogeny in the Peruvian Eastern Cordillera. north-central Andes, where Precambrian base- U-Pb zircon geochronology in the Eastern The presence of an Ordovician magmatic ment is not exposed for over 2000 km along Cordilleras of Peru and Ecuador using a and metamorphic belt in the north-central strike, from 15°S in Peru to 2°S in Colombia. combination of laser-ablation–inductively Andes demonstrates that Famatinian meta- This corresponds to the distance between the coupled plasma–mass spectrometry detrital morphism and subduction-related mag- northern extent of the Arequipa-Antofalla base- zircon analysis and dating of syn- and post- matism were continuous from Patagonia ment (Fig. -
From Rodinia to Gondwana
A history of Proterozoic terranes in southern South America: From Rodinia to Gondwana C. Casquet a,*, c.w. Rapela b, R.J. Pankhurst c, E.G. Baldo d, C. Galindo a, C.M. Fanning e, J.A. Dahlquist d, J. Saavedra f a Departamento de Petrologia y Geoquimica, ICEO (Universidad Complutense, CSIC), 28040 Madrid, Spain b Centra de Investigaciones Geologicas (CONICET-UNLP), 1900 La Plata, Argentina C 'Visiting Research Associate, British Geological SUlVey, Keyworth, Nottingham NG12 SCC, United Kingdom d CICTERRA (CONICET-UNC), 5000 Cordoba, Argentina e Research School of Earth Sciences, The Australian National University, Canberra, Australia f Instituto de Agrobiologia y Recursos Naturales CSIC, 37071 Salamanca, Spain KEYWORDS Abstract The role played by Paleoproterozoic cratons in southern South America from the Mesopro Paleoproterozoic; terozoic to the Early Cambrian is reconsidered here. This period involved protracted continental amal Cratons; gamation that led to formation of the supercontinent Rodinia, followed by N eoproterozoic continental Grenvillian; break-up, with the consequent opening of Clymene and Iapetus oceans, and finally continental Neoproterozoic rifting; re-assembly as Gondwana through complex oblique collisions in the Late Neoproterozoic to Early SW Gondwana assembly Cambrian. The evidence for this is based mainly on a combination of precise U-Pb SHRMP dating and radiogenic isotope data for igneous and metamorphic rocks from a large area extending from the Rio de la Plata craton in the east to the Argentine Precordillera in the west and as far north as Arequipa in Peru. Our interpretation of the paleogeograpbical and geodynamic evolution invokes a hypothetical Paleoproterozoic block (MARA) embracing basement ultimately older than 1.7 Ga in the Western Sierras 1. -
Archean Evolution of the Southern São Francisco
ARCHEAN EVOLUTION OF THE SOUTHERN SÃO FRANCISCO CRATON (SE BRAZIL) i ii FUNDAÇÃO UNIVERSIDADE FEDERAL DE OURO PRETO Reitor Cláudia Aparecida Marliére de Lima Vice-Reitor Hermínio Arias Nalini Júnior Pró-Reitor de Pesquisa e Pós-Graduação Sérgio Francisco de Aquino ESCOLA DE MINAS Diretor Issamu Endo Vice-Diretor José Geraldo Arantes de Azevedo Brito DEPARTAMENTO DE GEOLOGIA Chefe Luis Antônio Rosa Seixas iii EVOLUÇÃO CRUSTAL E RECURSOS NATURAIS iv CONTRIBUIÇÕES ÀS CIÊNCIAS DA TERRA - VOL. 349 TESE DE DOUTORAMENTO ARCHEAN EVOLUTION OF THE SOUTHERN SÃO FRANCISCO CRATON (SE BRAZIL) Capucine Albert Orientador Dr. Cristiano de Carvalho Lana Co-orientador Dr. Federico Farina Tese apresentada ao Programa de Pós-Graduação em Evolução Crustal e Recursos Naturais do Departamento de Geologia da Escola de Minas da Universidade Federal de Ouro Preto como requisito parcial à obtenção do Título de Doutor, Área de Concentração: Tectônica, Petrogênese e Recursos Minerais OURO PRETO 2017 v vii viii Acknowledgements Many people have contributed toward the realization of this project, bringing their geological knowledge, financial or logistic support and moral encouragements, and I have every person to acknowledge and thank for their contribution, whether small or big. Thank you! Cristiano, I am indebted to you for providing me with the opportunity to do research, and for all your support throughout the years. I am particularly grateful for your enthusiasm, your trust, and your availability. Thank you for the time and effort you dedicate to your students, providing us with the opportunity to be involved in scientific discussions, and for letting us follow our own research interests and ideas. -
Back Matter (PDF)
Index Page numbers in italic denote figures. Page numbers in bold denote tables. Accra Plains Migmatite, correlation with Me´dio Coreau´ Bafia Group 86 domain 102–103, 114 Bahia–Gabon continental bridge 153, 154 Adamastor ocean Baixo Araguaia Supergroup 174, 299 closure 260, 265, 269, 270, 271, 271, 273 geochronology 184, 189, 190, 191 subduction 229, 231 Baltica Adamawa fault 92 palaeogeography 13–16, 14, 15, 17,22–23 Adamawa–Yade´ domain 85, 85, 87, 88,90–91 palaeomagnetic poles 10, 11 Afagados do Ingrazeira fault 72 Bambui Group 165, 201, 206 A´ gua Clara domain 241, 242 Bandeirinha Formation 36, 36, 37 A´ guas Belas–Caninde´ suite 80, 81 Bangweulu block 33, 43–45 Akanyaru Supergroup 33, 41–43, 45 Baoule´ –Mossi domain 142–144 Albian gap 379, 382, 384, 392 Barro Alto complex 204 Ale´m Paraı´ba shear zone 222 basalt, Brazilian margin 373 Algodo˜es Unit 53 basins Alto Moxoto´ terrane 72, 77, 92 sag Alto Pajeu´ terrane 72, 73, 77, 78, 92 Espirito Santo Basin 379 Amazonia Sa˜o Francisco craton 33, 34, 35–36, 39 palaeogeography 13–16, 14, 15, 16, 17, 21, 22–23 salt, Brazilian margin 366–370, 367, 375 palaeomagnetic poles 12,13 sedimentary Amazonian craton 102 Borborema Province 56 geochronology 177, 189, 191 Garupi Belt 141 Andrelaˆndia Group 164, 202, 205, 217 Parana´ –Cape–Karoo 319–337 Angola craton 4, 5, 223, 224, 225–226 rift, Brazilian margin, uplifted flanks 383–387 correlation with Cabo Frio terrane 292 Sa˜o Francisco–Congo craton 33–46 Apiaı´ terrane 214, 218, 221, 222–223, 229 Sa˜o Luı´s craton 140, 141 Apparent Polar Wander Path -
From Rodinia to Gondwana
GEOSCIENCE FRONTIERS 3(2) (2012) 137e145 available at www.sciencedirect.com China University of Geosciences (Beijing) GEOSCIENCE FRONTIERS journal homepage: www.elsevier.com/locate/gsf GSF REVIEW A history of Proterozoic terranes in southern South America: From Rodinia to Gondwana C. Casquet a,*, C.W. Rapela b, R.J. Pankhurst c, E.G. Baldo d, C. Galindo a, C.M. Fanning e, J.A. Dahlquist d, J. Saavedra f a Departamento de Petrologıa y Geoquımica, IGEO (Universidad Complutense, CSIC), 28040 Madrid, Spain b Centro de Investigaciones Geologicas (CONICET-UNLP), 1900 La Plata, Argentina c Visiting Research Associate, British Geological Survey, Keyworth, Nottingham NG12 5GG, United Kingdom d CICTERRA (CONICET-UNC), 5000 Cordoba, Argentina e Research School of Earth Sciences, The Australian National University, Canberra, Australia f Instituto de Agrobiologıa y Recursos Naturales CSIC, 37071 Salamanca, Spain Received 3 August 2011; accepted 8 November 2011 Available online 3 December 2011 KEYWORDS Abstract The role played by Paleoproterozoic cratons in southern South America from the Mesopro- Paleoproterozoic; terozoic to the Early Cambrian is reconsidered here. This period involved protracted continental amal- Cratons; gamation that led to formation of the supercontinent Rodinia, followed by Neoproterozoic continental Grenvillian; break-up, with the consequent opening of Clymene and Iapetus oceans, and finally continental Neoproterozoic rifting; re-assembly as Gondwana through complex oblique collisions in the Late Neoproterozoic to Early SW Gondwana assembly Cambrian. The evidence for this is based mainly on a combination of precise U-Pb SHRMP dating and radiogenic isotope data for igneous and metamorphic rocks from a large area extending from the Rio de la Plata craton in the east to the Argentine Precordillera in the west and as far north as Arequipa in Peru. -
Palaeozoic Amalgamation of Central Europe: an Introduction and Synthesis of New Results from Recent Geological and Geophysical Investigations
Downloaded from http://sp.lyellcollection.org/ by guest on September 28, 2021 Palaeozoic amalgamation of Central Europe: an introduction and synthesis of new results from recent geological and geophysical investigations J. A. WINCHESTER 1, T. C. PHARAOH 2 & J. VERNIERS 3 1School of Earth Sciences and Geography, Keele University, Staffs ST5 5BG, UK; j. a. winchester@esci, keele.ac, uk 2British Geological Survey, Kingsley Dunham Centre, Keyworth, Notts NG12 5GG, UK 3Laboratorium voor Palaontologie, Krijgslaan 281/$8, B 9000, Gent, Belgium Abstract: Multidisciplinary studies undertaken within the EU-funded PACE Network have permitted a new 3-D reassessment of the relationships between the principal crustal blocks abutting Baltica along the Trans-European Suture Zone (TESZ). The simplest model indicates that accretion was in three stages: end-Cambrian accretion of the Bruno- Silesian, Lysogdry and Matopolska terranes; late Ordovician accretion of Avalonia, and early Carboniferous accretion of the Armorican Terrane Assemblage (ATA), which had coalesced during Late Devonian - Early Carboniferous time. All these accreted blocks contain similar Neoproterozoic basement indicating a peri-Gondwanan origin: Palaeozoic plume-influenced metabasite geochemistry in the Bohemian Massif in turn may explain their progressive separation from Gondwana before their accretion to Baltica, although separation of the Bruno-Silesian and related blocks from Baltica during the Cambrian is contentious. Inherited ages from both the Bruno-Silesian crustal block and Avalonia contain a 1.5 Ga 'Rondonian' component arguing for proximity to the Amazonian craton at the end of the Neoproterozoic: such a component is absent from Armorican terranes, which suggests that they have closer affinities with the West African craton. -
Archean Crust and Metallogenic Zones in the Amazonian Craton Sensed by Satellite Gravity Data Received: 3 September 2018 J
www.nature.com/scientificreports OPEN Archean crust and metallogenic zones in the Amazonian Craton sensed by satellite gravity data Received: 3 September 2018 J. G. Motta 1, C. R. de SOUZA FILHO1, E. J. M. Carranza 2 & C. Braitenberg 3 Accepted: 17 January 2019 The formation of ore deposits has been extensively studied from a shallow crust perspective. In Published: xx xx xxxx contrast, the association of mineral systems with deep crustal structure of their host terranes remains relatively undisclosed, and there is evidence that processes throughout the lithosphere are coupled for their evolution. The current debate centers on the control of the regional deep crustal architecture in focusing and transferring fuids between geochemical reservoirs. Defning such architecture is not unequivocal, and involves combining indirect information in order to constrain its physical properties and evolution. Herein, based on evidence from satellite gravity, constrained by airborne potential feld data (gravity and magnetics), we provide an example on how the lithosphere geometry controlled the location of copper and gold systems in the world-class Archean Carajás Mineral Province (Amazonian Craton, South America). Validation with information from passive seismic (wave speeds, crustal and lithospheric thickness) and geochronologic data (model, crystallization ages, and Neodymium isotope ratio determinations) portrays a signifcantly enlarged, poly-phase, Archean crust that exerted geometric control on the location of the mineral systems within and adjacent to the province during tectonic quiescence and switches. This new geologic scenario impacts the understanding of the Amazonian Craton. Synergy between multi-source data, as experimented here, can provide robust models efciently and, conceivably, help to unveil similar terrains elsewhere. -
Supercontinent Reconstruction the Palaeomagnetically Viable, Long
Geological Society, London, Special Publications The palaeomagnetically viable, long-lived and all-inclusive Rodinia supercontinent reconstruction David A. D. Evans Geological Society, London, Special Publications 2009; v. 327; p. 371-404 doi:10.1144/SP327.16 Email alerting click here to receive free email alerts when new articles cite this service article Permission click here to seek permission to re-use all or part of this article request Subscribe click here to subscribe to Geological Society, London, Special Publications or the Lyell Collection Notes Downloaded by on 21 December 2009 © 2009 Geological Society of London The palaeomagnetically viable, long-lived and all-inclusive Rodinia supercontinent reconstruction DAVID A. D. EVANS Department of Geology & Geophysics, Yale University, New Haven, CT 06520-8109, USA (e-mail: [email protected]) Abstract: Palaeomagnetic apparent polar wander (APW) paths from the world’s cratons at 1300–700 Ma can constrain the palaeogeographic possibilities for a long-lived and all-inclusive Rodinia supercontinent. Laurentia’s APW path is the most complete and forms the basis for super- position by other cratons’ APW paths to identify possible durations of those cratons’ inclusion in Rodinia, and also to generate reconstructions that are constrained both in latitude and longitude relative to Laurentia. Baltica reconstructs adjacent to the SE margin of Greenland, in a standard and geographically ‘upright’ position, between c. 1050 and 600 Ma. Australia reconstructs adja- cent to the pre-Caspian margin of Baltica, geographically ‘inverted’ such that cratonic portions of Queensland are juxtaposed with that margin via collision at c. 1100 Ma. Arctic North America reconstructs opposite to the CONgo þ Sa˜o Francisco craton at its DAmaride–Lufilian margin (the ‘ANACONDA’ fit) throughout the interval 1235–755 Ma according to palaeomag- netic poles of those ages from both cratons, and the reconstruction was probably established during the c. -
Significance of the Nova Brasilndia Metasedimentary Belt In
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Bern Open Repository and Information System (BORIS) TECTONICS, VOL. 23, TC6004, doi:10.1029/2003TC001563, 2004 Significance of the Nova Brasilaˆndia metasedimentary belt in western Brazil: Redefining the Mesoproterozoic boundary of the Amazon craton Eric Tohver,1,2 Ben van der Pluijm,1 Klaus Mezger,3 Eric Essene,1 Jaime Scandolara,4 and Gilmar Rizzotto4 Received 18 July 2003; revised 6 July 2004; accepted 16 September 2004; published 7 December 2004. [1] The Nova Brasilaˆndia metasedimentary belt belts in sedimentary environment, metamorphic grade, (NBMB) of western Brazil marks a fundamental and timing of deformation, signify that these two belts crustal boundary in the Amazon craton. The are not geologically continuous. The ‘‘Grenvillian’’ metasedimentary rocks of the NBMB (calc-silicates, deformation recorded by the NBMB belt marks the metapelites, quartzites, metabasites) contrast strongly final docking of the Amazon craton and Paragua with the older, polycyclic granitoid rocks of the craton within the Rodinia framework. The Aguapeı´ adjacent Amazon craton. Aeromagnetic anomalies belt, in contrast, seems to record only limited indicate that the belt is continuous for at least deformation internal to the Paragua craton. INDEX 1000 km in an E-W direction, although the TERMS: 8102 Tectonophysics: Continental contractional orogenic easternmost extent of the NBMB is covered by belts; 3660 Mineralogy and Petrology: Metamorphic petrology; the Cretaceous sediments of the Parecis Formation. 1035 Geochemistry: Geochronology; 8025 Structural Geology: Additional geologic evidence suggests that the belt Mesoscopic fabrics; 9360 Information Related to Geographic extends along an E-W trend for 2000 km.