Proterozoic accretionary belts of the Amazonian Craton Umberto G. Cordani Institute of Geosciences University of Sao Paulo, Brazil.

Slides:



Advertisements
Similar presentations
THE HIGHEST CENTRAL ANDES Victor A. Ramos Laboratorio de Tectónica Andina Universidad de Buenos Aires.
Advertisements

Department of Industry and Resources Geological Survey of Western Australia Tectonic evolution and mineralization of the Australian Proterozoic Ian M.
This is a computer model of the thermal structure of a subduction zone (convergence at 6 cm/year) showing how cool rocks of the slab pass to great depths,
Accretionary growth of Paleoproterozoic Fennoscandia: results from deep seismic experiments BABEL, FIRE and SVEKALAPKO Annakaisa Korja University of Helsinki.
ISOSTASY Removal of material from the top will induce uplift at the surface. Removal of material from the bottom will produce subsidence. Thus, in the.
Surface geology of the Japanese Islands Shigeru Otoh (Graduate School of Science and Engineering, University of Toyama) International Workshop on KamLAND.
大陸地殼演化 Genesis and evolution of the continental crust I. Introduction - Principal topics to be covered: 1.Characteristics, ages and compositions of the.
Crustal Deformation and Mountain Building
Evolution of Continental Crust Chapter 10. Hypsographic Curve.
4. Formation and Deformation of the Continental Crust
Growth of the Continental Crust Lecture 48. Age of the Crust The oceanic crust is ephemeral; its mean age is 60 Ma and, with the exception of possible.
Classroom presentations to accompany Understanding Earth, 3rd edition prepared by Peter Copeland and William Dupré University of Houston Chapter 21 Deformation.
Passive margins and their terminal collisions through Earth history Dwight Bradley U.S. Geological Survey Dwight Bradley U.S. Geological Survey.
Deep seismic reflection profiling of Archean cratons Arie J. van der Velden Frederick A. Cook Outline: - Locations of available profiles - Causes of reflectivity:
Proterozoic Evolution of the Western Margin of the Wyoming Craton: Implications for the Tectonic and Magmatic Evolution of the Northern Rockies Southwest.
Did plate tectonic begin in Early Archean times? Hugh Smithies Martin Van Kranendonk Dave Champion Geological Survey of Western Australia.
Time Scale Age of Oldest Rocks: 4.0 Ga 2.5 Ga EoArchean NeoArchean.
Proterozoic Making the Modern World Myrs 2500 Myr 1600 Myr 1000 Myr.
Plate Tectonics in the Archean On Archean granites, greenstones, cratons and tectonics: does the evidence demand a verdict? M. J. de Wit (1998) Nick Cowan.
THE PRIMORDIAL EARTH Hadean and Archean Eons Evolution of Early Life Most likely anaerobic bacteria Were heterotrophs consumed simple organic compounds.
Announcements: Final Exam Monday, Dec. 16, 11-1 this room.
Rodinia, Rifting, Iapetus and the Great American Bank
2) Super Continent cyclisity (?) and Wilson cycle tectonics
Walter D. Mooney, Ph.D. US Geological Survey Menlo Park, California USA Lecture #1: Evolution of the Early Earth IPRCC and SinoProbe Short.
BEFORE PANGAEA EPSC 510 // PRESENTATION 1.
Heat flow and heat production in the Canadian Shield Jean-Claude Mareschal, GEOTOP-UQAM-McGill, with a little help from my friends… Claude Jaupart, Clement.
Total Heat Loss of the Earth and Heat Production in the Continental Crust Makoto Yamano Earthquake Research Institute, University of Tokyo, Japan.
The internal structure of the Earth The internal structure of the Earth 1 The Tectonic Cycle The Earth’s crust.
GLOBAL TOPOGRAPHY. CONTINENTAL & OCEANIC LITHOSPHERE.
David Foster - University of Florida Paul Mueller - University of Florida David Mogk - Montana State University David Foster - University of Florida Paul.
Iron Ore Group, Eastern Indian Craton Asish Basu University of Rochester New York
Geological History of the Earth. Hadeon Eon No rocks because the Earth was molten.
GEO-4840 TECTONICS-S05 PART 1: LECTURES [ Wed (16) ] 19/1 - 09/3 PART 2: STUDENT PROJECTS [ Presentations ] 13/4 PART 3: FIELD TEACHING [ Corsica.
Archean Plate Tectonics: Isotopic Evidence from Samples of the Lithospheric Mantle to the Upper Crust Steven B Shirey Department of Terrestrial Magnetism.
Precambrian Earth History—The Proterozoic Eon
Precambrian Geology.  Comprises 88% of geologic time  Precambrian has 2 Eons  Geology hard to Study...  Preserved rocks are metamorphosed  Very few.
GEO-4840 TECTONICS-s06 PART 1: Lectures [ Mondays 8-12 ] 23/1 - 06/3 PART 2: Student projects [ Essay and presentation ] Weeks PART 3: Field teaching.
Archean Rocks Best, Chapter 15A.
Earth History GEOL 2110 The Cryptozoic (Precambrian) SuperEon
How and why does subduction occur? zConvergence yOne plate sinks beneath the other yDense oceanic crust sinks into mantle.
What can xenoliths tell us? Roberta L. Rudnick Geochemistry Laboratory Department of Geology University of Maryland Roberta L. Rudnick Geochemistry Laboratory.
Penrose Conference – June 2006 High-Mg Magmatism Through Time: Implications for Plate Tectonics C.M. Lesher Mineral Exploration Research Centre Department.
Plate Tectonics  Lithosphere – the earth’s crust 1) The Earth’s crust is not a continuous, solid rock layer 2) The crust is broken up into smaller units.
Major tectonic processes illustrated with examples from the Geology of Norway Intro and overview of the Late Proterozoic to Permian tectonic evolution.
Thermal modelling of crustal stacking and exhumation during the Paleoproterozoic orogenic growth of the Fennosscandian Shield I.T. Kukkonen 1, A. Korja.
J. Toro, West Virginia University, USA
Content 1.Geology of Isua (3.8Ga), Greenland, (1) presence of accretionary complex (horizontal stress field same as today), 2.(2) presence of water >1000m,
Plate Tectonics. OVERVIEW Defining Plate Tectonics Review of Earth’s Layers Focus: Crust & Asthenosphere Evolution of Plate Tectonic Theory Visual Evidence.
GY111 Physical Geology Evolution of the Continents.
Crustal Features 8.9B relate plate tectonics to the formation of crustal features.
Mesoproterozoic Ferroan Magmatism in the Southwestern USA
Lecture Outlines Physical Geology, 14/e
Lecture Outlines Physical Geology, 10/e
Mountain Building “Tectonic Forces at Work”
Goals (and conclusions)
The anatomy of continents
CCFS-Macquarie University, University of WA, Geological Survey WA
Carla Braitenberg Department of Mathematics and Geosciences
Mesoproterozoic orangeite of Karelia (Kostomuksha-Lentiira): evidence for composition of mantle lithosphere Alexey Kargin, Anna Nosova, Yulia Larionova,
Ocean-Ocean Subduction Zones System
Warm-Up: March 18, 2016 Write down everything you know about plate tectonics.
HISTORY OF THE CONTINENTS
1 The Tectonic Cycle The internal structure of the Earth
Chapter 10.
12.2 Features of Plate Tectonics
Crust-Mantle Relationships
Plate Tectonics.
Department of Earth Sciences University of Windsor
Phil Thurston Laurentian University
The Wyoming Province: A Unique Archean Craton
Presentation transcript:

Proterozoic accretionary belts of the Amazonian Craton Umberto G. Cordani Institute of Geosciences University of Sao Paulo, Brazil

TECTONIC EVOLUTION OF THE AMAZONIAN CRATON IN THE PROTEROZOIC -- The SW part of the Amazonian craton was formed by continuous amalgamation of magmatic arcs, largely juvenile, the roots of which are now exhumed. - Accretionary belts, driven by subduction, formed a very large domain, at least 2700 km long and about 1300 km wide -- Duration of the process is about 700 m.y., starting at 2.0 Ga. An ocean basin was closed, to the SW of a large continent formed by the Guyana Shield plus the West African craton. -- The units decrease in age from NE to SW, and lithologies are practically only granitic (s.l.). Basement was not detected.

EARTH THERMAL EVOLUTION Layered mantle convection Subduction slabs restricted to upper mantle Whole-mantle convection Oceanic lithosphere down to lower mantle SUPERPLUMES AVALANCHES SUPERCONTINENT CYCLE

PALEOPROTEROZIC Woopmay Orogen ARCHEAN Slave Craton

INTRA-OCEANIC MAGMATIC ARCS WITHIN ACCRETIONARY BELTS Absence of continental basement rocks Stacking, “Soft-collision” and accretion processes Positive or slightly negative on granitoids Sm-Nd model ages similar or slightly older than radiometric ages of rocks (U-Pb on Zircon)  Nd

Províncias tectônicas da parte NW do Craton Amazônico

Províncias tectônicas da parte SW do Craton Amazônico

VENTUARI-TAPAJÓS and RIO NEGRO-JURUENA MAGMATIC ARCS Predominantly granitoid material, deformed and undeformed Archean basement not detected Radiometric ages roughly between 2.0 and 1.5 Ga, decreasing from NE to SW Post-orogenic volcanic-sedimentary basins with similar or slightly younger ages. Sm – Nd model ages always younger than 2.1 Ga from slightly negative to about (+3)  Nd (T)

Reconstrução da posição relativa de Laurentia, Baltica, Amazonia e Australia há 1.65 Ga. Y-M=Yavapai-Mazatzal Lb=Labradorian G=Gothian R-J=Rio Negro-Juruena (a) - Pesonen et al (2001) (b) - Modelo alternativo (c) - Ahäll & Larson (2000) e Geraldes et al. (2001)

RONDONIAN-SAN IGNACIO PROVINCE and SUNSAS BELT

RONDONIAN-SAN IGNACIO PROVINCE Presence of Paleoproterozoic basement Large metamorphic belts of Mesoproterozoic age Volcanic-sedimentary units of Meso-Neoproterozoic age Juvenile magmatic arcs (Pensamiento complex and related rocks) Radiometric ages between 1.3 and 1.5 Ga Sm – Nd model ages between 1.7 and 2.2 Ga between (-3) and (+2)  Nd (T) U-Pb radiometric ages between 1.4 and 1.5 Ga Sm – Nd model ages between 1.5 and 1.7 Ga about (+4)  Nd (T)

MAIN CONCLUSIONS -- The SW part of the Amazonian craton was formed by continuous amalgamation of magmatic arcs, largely juvenile, the roots of which are now exhumed. - Accretionary belts, driven by subduction, formed a very large domain, at least 2700 km long and about 1300 km wide -- Duration of the process is about 700 m.y., starting at 2.0 Ga. An ocean basin was closed, to the SW of a large continent formed by the Guyana Shield plus the West African craton. -- The units decrease in age from NE to SW, and lithologies are practically only granitic (s.l.). Basement was not detected.