Rodinia to Gondwana: the Geodynamic Map of Gondwana Supercontinent Assembly
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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. -
Proterozoic East Gondwana: Supercontinent Assembly and Breakup Geological Society Special Publications Society Book Editors R
Proterozoic East Gondwana: Supercontinent Assembly and Breakup Geological Society Special Publications Society Book Editors R. J. PANKHURST (CHIEF EDITOR) P. DOYLE E J. GREGORY J. S. GRIFFITHS A. J. HARTLEY R. E. HOLDSWORTH A. C. MORTON N. S. ROBINS M. S. STOKER J. P. TURNER Special Publication reviewing procedures The Society makes every effort to ensure that the scientific and production quality of its books matches that of its journals. Since 1997, all book proposals have been refereed by specialist reviewers as well as by the Society's Books Editorial Committee. If the referees identify weaknesses in the proposal, these must be addressed before the proposal is accepted. Once the book is accepted, the Society has a team of Book Editors (listed above) who ensure that the volume editors follow strict guidelines on refereeing and quality control. We insist that individual papers can only be accepted after satis- factory review by two independent referees. The questions on the review forms are similar to those for Journal of the Geological Society. The referees' forms and comments must be available to the Society's Book Editors on request. Although many of the books result from meetings, the editors are expected to commission papers that were not pre- sented at the meeting to ensure that the book provides a balanced coverage of the subject. Being accepted for presentation at the meeting does not guarantee inclusion in the book. Geological Society Special Publications are included in the ISI Science Citation Index, but they do not have an impact factor, the latter being applicable only to journals. -
Balkatach Hypothesis: a New Model for the Evolution of the Pacific, Tethyan, and Paleo-Asian Oceanic Domains
Research Paper GEOSPHERE Balkatach hypothesis: A new model for the evolution of the Pacific, Tethyan, and Paleo-Asian oceanic domains 1,2 2 GEOSPHERE, v. 13, no. 5 Andrew V. Zuza and An Yin 1Nevada Bureau of Mines and Geology, University of Nevada, Reno, Nevada 89557, USA 2Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, California 90095-1567, USA doi:10.1130/GES01463.1 18 figures; 2 tables; 1 supplemental file ABSTRACT suturing. (5) The closure of the Paleo-Asian Ocean in the early Permian was accompanied by a widespread magmatic flare up, which may have been CORRESPONDENCE: avz5818@gmail .com; The Phanerozoic history of the Paleo-Asian, Tethyan, and Pacific oceanic related to the avalanche of the subducted oceanic slabs of the Paleo-Asian azuza@unr .edu domains is important for unraveling the tectonic evolution of the Eurasian Ocean across the 660 km phase boundary in the mantle. (6) The closure of the and Laurentian continents. The validity of existing models that account for Paleo-Tethys against the southern margin of Balkatach proceeded diachro- CITATION: Zuza, A.V., and Yin, A., 2017, Balkatach hypothesis: A new model for the evolution of the the development and closure of the Paleo-Asian and Tethyan Oceans criti- nously, from west to east, in the Triassic–Jurassic. Pacific, Tethyan, and Paleo-Asian oceanic domains: cally depends on the assumed initial configuration and relative positions of Geosphere, v. 13, no. 5, p. 1664–1712, doi:10.1130 the Precambrian cratons that separate the two oceanic domains, including /GES01463.1. the North China, Tarim, Karakum, Turan, and southern Baltica cratons. -
Geologic History of Siletzia, a Large Igneous Province in the Oregon And
Geologic history of Siletzia, a large igneous province in the Oregon and Washington Coast Range: Correlation to the geomagnetic polarity time scale and implications for a long-lived Yellowstone hotspot Wells, R., Bukry, D., Friedman, R., Pyle, D., Duncan, R., Haeussler, P., & Wooden, J. (2014). Geologic history of Siletzia, a large igneous province in the Oregon and Washington Coast Range: Correlation to the geomagnetic polarity time scale and implications for a long-lived Yellowstone hotspot. Geosphere, 10 (4), 692-719. doi:10.1130/GES01018.1 10.1130/GES01018.1 Geological Society of America Version of Record http://cdss.library.oregonstate.edu/sa-termsofuse Downloaded from geosphere.gsapubs.org on September 10, 2014 Geologic history of Siletzia, a large igneous province in the Oregon and Washington Coast Range: Correlation to the geomagnetic polarity time scale and implications for a long-lived Yellowstone hotspot Ray Wells1, David Bukry1, Richard Friedman2, Doug Pyle3, Robert Duncan4, Peter Haeussler5, and Joe Wooden6 1U.S. Geological Survey, 345 Middlefi eld Road, Menlo Park, California 94025-3561, USA 2Pacifi c Centre for Isotopic and Geochemical Research, Department of Earth, Ocean and Atmospheric Sciences, 6339 Stores Road, University of British Columbia, Vancouver, BC V6T 1Z4, Canada 3Department of Geology and Geophysics, University of Hawaii at Manoa, 1680 East West Road, Honolulu, Hawaii 96822, USA 4College of Earth, Ocean, and Atmospheric Sciences, Oregon State University, 104 CEOAS Administration Building, Corvallis, Oregon 97331-5503, USA 5U.S. Geological Survey, 4210 University Drive, Anchorage, Alaska 99508-4626, USA 6School of Earth Sciences, Stanford University, 397 Panama Mall Mitchell Building 101, Stanford, California 94305-2210, USA ABSTRACT frames, the Yellowstone hotspot (YHS) is on southern Vancouver Island (Canada) to Rose- or near an inferred northeast-striking Kula- burg, Oregon (Fig. -
Upper Mantle P and S Wave Velocity Structure of the Kalahari Craton And
RESEARCH LETTER Upper Mantle P and S Wave Velocity Structure of the 10.1029/2019GL084053 Kalahari Craton and Surrounding Proterozoic Key Points: • Thick cratonic lithosphere extends Terranes, Southern Africa beneath the Rehoboth Province and Kameron Ortiz1, Andrew Nyblade1,5 , Mark van der Meijde2, Hanneke Paulssen3 , parts of the northern Okwa Terrane 4 4 5 2,6 and Magondi Belt Motsamai Kwadiba , Onkgopotse Ntibinyane , Raymond Durrheim , Islam Fadel , • The northern edge of the greater and Kyle Homman1 Kalahari Craton lithosphere lies along the northern boundary of the 1Department of Geosciences, Pennsylvania State University, University Park, PA, USA, 2Faculty for Geo‐information Rehoboth Province and Magondi Science and Earth Observation (ITC), University of Twente, Enschede, Netherlands, 3Department of Earth Sciences, Belt 4 • Cratonic mantle lithosphere Faculty of Geosciences, Utrecht University, Utrecht, Netherlands, Botswana Geoscience Institute, Lobatse, Botswana, 5 6 beneath the Okwa Terrane and School of Geosciences, The University of the Witwatersrand, Johannesburg, South Africa, Geology Department, Faculty Magondi Belt may have been of Science, Helwan University, Ain Helwan, Egypt chemically altered by Proterozoic magmatic events Abstract New broadband seismic data from Botswana and South Africa have been combined with Supporting Information: existing data from the region to develop improved P and S wave velocity models for investigating the • Supporting Information S1 upper mantle structure of southern Africa. Higher craton‐like velocities are imaged beneath the Rehoboth Province and parts of the northern Okwa Terrane and the Magondi Belt, indicating that the Correspondence to: northern edge of the greater Kalahari Craton lithosphere lies along the northern boundary of these A. Nyblade, terranes. -
Locating South China in Rodinia and Gondwana: a Fragment of Greater India Lithosphere?
Locating South China in Rodinia and Gondwana: A fragment of greater India lithosphere? Peter A. Cawood1, 2, Yuejun Wang3, Yajun Xu4, and Guochun Zhao5 1Department of Earth Sciences, University of St Andrews, North Street, St Andrews KY16 9AL, UK 2Centre for Exploration Targeting, School of Earth and Environment, University of Western Australia, 35 Stirling Highway, Crawley, WA 6009, Australia 3State Key Laboratory of Isotope Geochemistry, Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, Guangzhou 510640, China 4State Key Laboratory of Biogeology and Environmental Geology, Faculty of Earth Sciences, China University of Geosciences, Wuhan 430074, China 5Department of Earth Sciences, University of Hong Kong, Pokfulam Road, Hong Kong, China ABSTRACT metamorphosed Neoproterozoic strata and From the formation of Rodinia at the end of the Mesoproterozoic to the commencement unmetamorphosed Sinian cover (Fig. 1; Zhao of Pangea breakup at the end of the Paleozoic, the South China craton fi rst formed and then and Cawood, 2012). The Cathaysia block is com- occupied a position adjacent to Western Australia and northern India. Early Neoproterozoic posed predominantly of Neoproterozoic meta- suprasubduction zone magmatic arc-backarc assemblages in the craton range in age from ca. morphic rocks, with minor Paleoproterozoic and 1000 Ma to 820 Ma and display a sequential northwest decrease in age. These relations sug- Mesoproterozoic lithologies. Archean basement gest formation and closure of arc systems through southeast-directed subduction, resulting is poorly exposed and largely inferred from the in progressive northwestward accretion onto the periphery of an already assembled Rodinia. presence of minor inherited and/or xenocrys- Siliciclastic units within an early Paleozoic succession that transgresses across the craton were tic zircons in younger rocks (Fig. -
Assembling Laurentia—Integrated Theme Sessions on Tectonic Turning Points
Assembling Laurentia—Integrated Theme Sessions on Tectonic Turning Points Michael L. Williams, Dept. of Geosciences, University of Massachusetts, Amherst, Massachusetts 01003, USA, [email protected]; Dawn A. Kellett, Geological Survey of Canada–Atlantic Division, Natural Resources Canada/Government of Canada, 1 Challenger Drive, Dartmouth, Nova Scotia B2Y 4A2, Canada, [email protected]; Basil Tikoff*, Dept. of Geoscience, University of Wisconsin– Madison, 1215 W. Dayton Street, Madison, Wisconsin 53706, USA, [email protected]; Steven J. Whitmeyer, Dept. of Geology and Environmental Science, James Madison University, 801 Carrier Drive, MSC 6903, Harrisonburg, Virginia 22807, USA, [email protected] The North American continent records the headlined by a Pardee Symposium, which and the broader implications of, these changes, evolution of tectonic processes and tectonic will provide an overview of the tectonic evo- and to widen the scope of investigation environments from the earliest Archean to lution of Laurentia and an introduction to the beyond a particular boundary or regional geo- modern times. The continent hosts a rich concept of key “Turning Points.” Seven logical event to the scale of Laurentia itself. Archean (and possibly Hadean) record, at related topical sessions, under the general The time slices for the topical sessions are as least three great Proterozoic orogenic belts, heading “Assembling Laurentia,” will span follows (with brief explanations from each and a wide range of Phanerozoic tectonic, the GSA meeting. -
Pan-African Orogeny 1
Encyclopedia 0f Geology (2004), vol. 1, Elsevier, Amsterdam AFRICA/Pan-African Orogeny 1 Contents Pan-African Orogeny North African Phanerozoic Rift Valley Within the Pan-African domains, two broad types of Pan-African Orogeny orogenic or mobile belts can be distinguished. One type consists predominantly of Neoproterozoic supracrustal and magmatic assemblages, many of juvenile (mantle- A Kröner, Universität Mainz, Mainz, Germany R J Stern, University of Texas-Dallas, Richardson derived) origin, with structural and metamorphic his- TX, USA tories that are similar to those in Phanerozoic collision and accretion belts. These belts expose upper to middle O 2005, Elsevier Ltd. All Rights Reserved. crustal levels and contain diagnostic features such as ophiolites, subduction- or collision-related granitoids, lntroduction island-arc or passive continental margin assemblages as well as exotic terranes that permit reconstruction of The term 'Pan-African' was coined by WQ Kennedy in their evolution in Phanerozoic-style plate tectonic scen- 1964 on the basis of an assessment of available Rb-Sr arios. Such belts include the Arabian-Nubian shield of and K-Ar ages in Africa. The Pan-African was inter- Arabia and north-east Africa (Figure 2), the Damara- preted as a tectono-thermal event, some 500 Ma ago, Kaoko-Gariep Belt and Lufilian Arc of south-central during which a number of mobile belts formed, sur- and south-western Africa, the West Congo Belt of rounding older cratons. The concept was then extended Angola and Congo Republic, the Trans-Sahara Belt of to the Gondwana continents (Figure 1) although West Africa, and the Rokelide and Mauretanian belts regional names were proposed such as Brasiliano along the western Part of the West African Craton for South America, Adelaidean for Australia, and (Figure 1). -
Paleozoic 3: Alabama in the Paleozoic
UNIVERSITY OF SOUTH ALABAMA GY 112: Earth History Paleozoic 3: Alabama in the Paleozoic Instructor: Dr. Douglas W. Haywick Last Time The Paleozoic Part 2 1) Back to Newfoundland 2) Eastern Laurentian Orogenies (Appalachians) 3) Other Laurentian Orogenies (Antler, Ouachita) (web notes 25) Laurentia (Paleozoic North America) Even though this coastline of Laurentia was a passive continental margin, a plate tectonic boundary was rapidly approaching… A B A B Laurentia (Paleozoic North America) The resulting Taconic Orogeny first depressed the seafloor Laurentia (localized transgression) and A Island arc then pushed previously deposited passive continental B margin sediments up into thrust fault mountains. Baltica There was only minimal metamorphism and igneous A intrusions. B Middle Ordovician Laurentia (Paleozoic North America) Laurentia Baltica Middle Ordovician Laurentia (Paleozoic North America) Laurentia Baltica Middle Ordovician Laurentia (Paleozoic North America) The next tectonic event (the Acadian Orogeny) was caused Laurentia by the approach of Baltica A B Baltica A B Baltica Baltica Late Ordovician Laurentia (Paleozoic North America) The Acadian Orogeny was more extensive and more intense (metamorphism and A lots of igneous intrusions) B A B Early Devonian Laurentia (Paleozoic North America) The Acadian Orogeny was more extensive and more intense (metamorphism and lots of igneous intrusions) Early Devonian Laurentia (Paleozoic North America) Lastly, along comes Gondwanna and…. …well you get the idea. A B B A B Mississippian Laurentia (Paleozoic North America) Lastly, along comes Gondwanna and…. …well you get the idea. A B B A B Pennsylvannian Suture zone Laurentia (Paleozoic North America) Lastly, along comes Gondwanna and…. …well you get the idea. -
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 Saharides and Continental Growth During the Final Assembly of Gondwana-Land
Reconstructing orogens without biostratigraphy: The Saharides and continental growth during the final assembly of Gondwana-Land A. M. Celâl S¸ engöra,b,1, Nalan Lomc, Cengiz Zabcıb, Gürsel Sunalb, and Tayfun Önerd aIstanbul_ Teknik Üniversitesi (ITÜ)_ Avrasya Yerbilimleri Enstitüsü, Ayazaga˘ 34469 Istanbul,_ Turkey; bITÜ_ Maden Fakültesi, Jeoloji Bölümü, Ayazaga˘ 34469 Istanbul,_ Turkey; cDepartement Aardwetenschappen, Universiteit Utrecht, 3584 CB Utrecht, The Netherlands; and dSoyak Göztepe Sitesi, Üsküdar 34700 Istanbul,_ Turkey Contributed by A. M. Celâl S¸ engör, October 3, 2020 (sent for review July 17, 2020; reviewed by Jonas Kley and Leigh H. Royden) A hitherto unknown Neoproterozoic orogenic system, the Sahar- identical to those now operating (the snowball earth and the ab- ides, is described in North Africa. It formed during the 900–500-Ma sence of land flora were the main deviating factors), yet the interval. The Saharides involved large subduction accretion com- dominantly biostratigraphy-based methods used to untangle oro- plexes occupying almost the entire Arabian Shield and much of genic evolution during the Phanerozoic are not applicable Egypt and parts of the small Precambrian inliers in the Sahara in- to them. cluding the Ahaggar mountains. These complexes consist of, at least by half, juvenile material forming some 5 million km2 new Method of Reconstructing Complex Orogenic Evolution in continental crust. Contrary to conventional wisdom in the areas the Neoproterozoic without Biostratigraphy: Example of the they occupy, -
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.