New Directions in Wilson Cycle Concepts: Supercontinent and Tectonic Rock Cycles
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Two Contrasting Phanerozoic Orogenic Systems Revealed by Hafnium Isotope Data William J
ARTICLES PUBLISHED ONLINE: 17 APRIL 2011 | DOI: 10.1038/NGEO1127 Two contrasting Phanerozoic orogenic systems revealed by hafnium isotope data William J. Collins1*(, Elena A. Belousova2, Anthony I. S. Kemp1 and J. Brendan Murphy3 Two fundamentally different orogenic systems have existed on Earth throughout the Phanerozoic. Circum-Pacific accretionary orogens are the external orogenic system formed around the Pacific rim, where oceanic lithosphere semicontinuously subducts beneath continental lithosphere. In contrast, the internal orogenic system is found in Europe and Asia as the collage of collisional mountain belts, formed during the collision between continental crustal fragments. External orogenic systems form at the boundary of large underlying mantle convection cells, whereas internal orogens form within one supercell. Here we present a compilation of hafnium isotope data from zircon minerals collected from orogens worldwide. We find that the range of hafnium isotope signatures for the external orogenic system narrows and trends towards more radiogenic compositions since 550 Myr ago. By contrast, the range of signatures from the internal orogenic system broadens since 550 Myr ago. We suggest that for the external system, the lower crust and lithospheric mantle beneath the overriding continent is removed during subduction and replaced by newly formed crust, which generates the radiogenic hafnium signature when remelted. For the internal orogenic system, the lower crust and lithospheric mantle is instead eventually replaced by more continental lithosphere from a collided continental fragment. Our suggested model provides a simple basis for unravelling the global geodynamic evolution of the ancient Earth. resent-day orogens of contrasting character can be reduced to which probably began by the Early Ordovician12, and the Early two types on Earth, dominantly accretionary or dominantly Paleozoic accretionary orogens in the easternmost Altaids of Pcollisional, because only the latter are associated with Wilson Asia13. -
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. -
Map of How Earth Would Have Looked If Supercontinent Gondwana Had Broken up Differently
Map of How Earth Would Have Looked if Supercontinent Gondwana Had Broken Up Differently UK EDITION FRIDAY, 14TH MARCH, 2014 News Business Economy Technology Sport Entertainment & Arts Viewpoint Video Science Map of How Earth Would Have IBTIMES TV Looked if Supercontinent Gondwana Had Broken Up Differently By Hannah Osborne March 3, 2014 10:23 GMT + Recreation of Banksy Marks 3 Years of Syrian Crisis How Earth would have looked if rift had split continent differently. Sascha Brune/Christian Heine http://www.ibtimes.co.uk/map-how-earth-would-have-looked-if-supercontinent-gondwana-had-broken-differently-1438639[14/03/2014 12:00:17 pm] Map of How Earth Would Have Looked if Supercontinent Gondwana Had Broken Up Differently A map showing what Earth would have looked like had the supercontinent Gondwana broken up differently has been created by researchers. The map looks at how the world would be completely different if the South Atlantic and West African rift had split, instead of the rift that emerged along the Equatorial Atlantic margins. Geoscientists at the University of Sydney and the GFZ German Research Centre for Geosciences used sophisticated plate tectonic and 2D numerical modelling to create the map. The Gondwana supercontinent broke up 130 million years ago leading to the creation of South America and Africa. However, for millions of years before this, the southern continents of Why advertise with us South America, Africa, Antarctica, Australia, and India were united as Gondwana. READ MORE It is still unclear why Gondwana fragmented, but it is understood if first split along the East Africa coast in a western and eastern part, before South America separated. -
Geology: Ordovician Paleogeography and the Evolution of the Iapetus Ocean
Ordovician paleogeography and the evolution of the Iapetus ocean Conall Mac Niocaill* Department of Geological Sciences, University of Michigan, 2534 C. C. Little Building, Ben A. van der Pluijm Ann Arbor, Michigan 48109-1063. Rob Van der Voo ABSTRACT thermore, we contend that the combined paleomagnetic and faunal data ar- Paleomagnetic data from northern Appalachian terranes identify gue against a shared Taconic history between North and South America. several arcs within the Iapetus ocean in the Early to Middle Ordovi- cian, including a peri-Laurentian arc at ~10°–20°S, a peri-Avalonian PALEOMAGNETIC DATA FROM IAPETAN TERRANES arc at ~50°–60°S, and an intra-oceanic arc (called the Exploits arc) at Displaced terranes occur along the extent of the Appalachian-Cale- ~30°S. The peri-Avalonian and Exploits arcs are characterized by Are- donian orogen, although reliable Ordovician paleomagnetic data from Ia- nigian to Llanvirnian Celtic fauna that are distinct from similarly aged petan terranes have only been obtained from the Central Mobile belt of the Toquima–Table Head fauna of the Laurentian margin, and peri- northern Appalachians (Table 1). The Central Mobile belt separates the Lau- Laurentian arc. The Precordillera terrane of Argentina is also charac- rentian and Avalonian margins of Iapetus and preserves remnants of the terized by an increasing proportion of Celtic fauna from Arenig to ocean, including arcs, ocean islands, and ophiolite slivers (e.g., Keppie, Llanvirn time, which implies (1) that it was in reproductive communi- 1989). Paleomagnetic results from Arenigian and Llanvirnian volcanic units cation with the peri-Avalonian and Exploits arcs, and (2) that it must of the Moreton’s Harbour Group and the Lawrence Head Formation in cen- have been separate from Laurentia and the peri-Laurentian arc well tral Newfoundland indicate paleolatitudes of 11°S (Table 1), placing them before it collided with Gondwana. -
Wilson Cycle Guide
Wilson Cycle Description Lynn S. Fichter and Eric Pyle Department of Geology and Environmental Science James Madison University Layout of this Guide For each stage represented in this Wilson Cycle, several pieces of information are provided: Description of Process: a description of the forces acting on a particular location, and the results of those forces; Composition: the particular rock types that result from these forces, including chemical make up, major minerals present, and texture (grain size and orientation), expressed in photographs, verbal descriptions, and categorical graphs; Specific Locations, Present and Past: the map locations of examples of the environment, with current and past locations represented. Stage A: Stable Continental Craton Description of Process: This stage represents the basis of all existing continents, showing in a simplified fashion both continental crust and adjacent oceanic crust, both of which lie over the mantle. You will notice that the continental crust is considerably thicker than the ocean crust. Continental crust is less dense than oceanic crust (approximately 2.7 g/cm3 vs. 3.3 g/cm3), and so “rides” higher over the mantle. Continental crust is also more rigid that oceanic crust. Furthermore, the development of continental crust involves considerable thickening. Composition: This diagram represents considerable simplification, in that the internal structure has not been shown, but is represented as a crystalline “basement” for the continent. This basement material represents a variety of rock types, including granites and diorites, gneisses and schists, and various sedimentary rocks. Taken as a whole, the average composition of the basement rock is the same as a granodiorite – enriched in sodium, potassium and silica-rich minerals, such as alkali feldspar, sodium plagioclase, and quartz, and depleted in iron/magnesium, silica poor minerals, such as olivine, pyroxene, and amphibole. -
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. -
Connecting the Deep Earth and the Atmosphere
In Mantle Convection and Surface Expression (Cottaar, S. et al., eds.) AGU Monograph 2020 (in press) Connecting the Deep Earth and the Atmosphere Trond H. Torsvik1,2, Henrik H. Svensen1, Bernhard Steinberger3,1, Dana L. Royer4, Dougal A. Jerram1,5,6, Morgan T. Jones1 & Mathew Domeier1 1Centre for Earth Evolution and Dynamics (CEED), University of Oslo, 0315 Oslo, Norway; 2School of Geosciences, University of Witwatersrand, Johannesburg 2050, South Africa; 3Helmholtz Centre Potsdam, GFZ, Telegrafenberg, 14473 Potsdam, Germany; 4Department of Earth and Environmental Sciences, Wesleyan University, Middletown, Connecticut 06459, USA; 5DougalEARTH Ltd.1, Solihull, UK; 6Visiting Fellow, Earth, Environmental and Biological Sciences, Queensland University of Technology, Brisbane, Queensland, Australia. Abstract Most hotspots, kimberlites, and large igneous provinces (LIPs) are sourced by plumes that rise from the margins of two large low shear-wave velocity provinces in the lowermost mantle. These thermochemical provinces have likely been quasi-stable for hundreds of millions, perhaps billions of years, and plume heads rise through the mantle in about 30 Myr or less. LIPs provide a direct link between the deep Earth and the atmosphere but environmental consequences depend on both their volumes and the composition of the crustal rocks they are emplaced through. LIP activity can alter the plate tectonic setting by creating and modifying plate boundaries and hence changing the paleogeography and its long-term forcing on climate. Extensive blankets of LIP-lava on the Earth’s surface can also enhance silicate weathering and potentially lead to CO2 drawdown (cooling), but we find no clear relationship between LIPs and post-emplacement variation in atmospheric CO2 proxies on very long (>10 Myrs) time- scales. -
Magmatic Records of the Late Paleoproterozoic to Neoproterozoic 14 Extensional and Rifting Events in the North China Craton: a Preliminary Review
Magmatic Records of the Late Paleoproterozoic to Neoproterozoic 14 Extensional and Rifting Events in the North China Craton: A Preliminary Review Shuan-Hong Zhang and Yue Zhao Abstract The North China Craton (NCC) is characterized by multistages of extensional and continental rifting and deposition of thick marine or interactive marine and terrestrial clastic and carbonate platform sediments without angular unconformity during Earth’s middle age of 1.70–0.75 Ga. Factors controlling these multistages of extensional and continental rifting events in the NCC can be either from the craton itself or from the neighboring continents being connected during these periods. Two large igneous provinces including the ca. 1.32 Ga mafic sill swarms in Yanliao rift (aulacogen) in the northern NCC and the ca. 0.92–0.89 Ga Xu-Huai–Dalian–Sariwon mafic sill swarms in southeastern and eastern NCC, have recently been identified from the NCC. Rocks from these two large igneous provinces exhibit similar geochemical features of tholeiitic compositions and intraplate characteristics. Formation of these two large igneous provinces was accompanied by pre-magmatic uplift as indicated by the field relations between the sills and their hosted sedimentary rocks. The Yanliao and Xu-Huai–Dalian–Sariwon large igneous provinces represent two continental rifting events that have led to rifting to drifting transition and breakup of the northern margin of the NCC from the Columbia (Nuna) supercontinent and the southeastern margin of the NCC from the Rodinia supercontinent, respectively. As shown by the ca. 200 Ma Central Atlantic Magmatic Province related to breakup of the Pangea supercontinent and initial opening of the Central Atlantic Ocean and the ca. -
Pannotia to Pangaea: Neoproterozoic and Paleozoic Orogenic Cycles in the Circum-Atlantic Region: a Celebration of the Career of Damian Nance
Downloaded from http://sp.lyellcollection.org/ by guest on September 27, 2021 Pannotia to Pangaea: Neoproterozoic and Paleozoic Orogenic Cycles in the Circum-Atlantic Region: A celebration of the career of Damian Nance J. Brendan Murphy1,2*, Robin A. Strachan3 and Cecilio Quesada4 1Department of Earth Sciences, St Francis Xavier University, Antigonish, Nova Scotia, B2G 2W5, Canada 2Earth Dynamics Research Group, the Institute for Geoscience Research (TIGeR), School of Earth and Planetary Sciences, Curtin University, WA 6845, Australia 3School of the Environment, Geography and Geosciences, University of Portsmouth, Portsmouth PO1 3QL, UK 4Instituto Geológico y Minero de España (IGME), C/Ríos Rosas, 23, 28003 Madrid, Spain JBM, 0000-0003-2269-1976 *Correspondence: [email protected] Special Publication 503 celebrates the career of between tectonic events and biogeochemical cycles, R. Damian Nance. It features 27 articles, with more as exemplified in the late Neoproterozoic–Early than 110 authors based in 18 different countries. Cambrian by the amalgamation of Gondwana span- The wide range of topics presented in this volume ning a time interval characterized by dramatic climate mirrors the breadth and depth of Damian’s contribu- swings, profound changes in the chemistry of the tions, interests and expertise. Like Damian’s papers, oceans and atmosphere, and the evolution of multi- the contributions range from the predominantly con- cellular animals (see Hoffman 1991; Hoffman et al. ceptual to detailed field work, but all are targeted at 1998; Narbonne 2010; Knoll 2013). understanding important tectonic processes. Their As reconstructions became more refined, scope not only varies in scale from global to regional several authors proposed that Gondwana was part to local, but also in the range of approaches required of a larger entity called Pannotia that included Lau- to gain that understanding. -
A History of Supercontinents on Planet Earth
By Alasdair Wilkins Jan 27, 2011 2:31 PM 47,603 71 Share A history of supercontinents on planet Earth Earth's continents are constantly changing, moving and rearranging themselves over millions of years - affecting Earth's climate and biology. Every few hundred million years, the continents combine to create massive, world-spanning supercontinents. Here's the past and future of Earth's supercontinents. The Basics of Plate Tectonics If we're going to discuss past and future supercontinents, we first need to understand how landmasses can move around and the continents can take on new configurations. Let's start with the basics - rocky planets like Earth have five interior levels: heading outwards, these are the inner core, outer core, mantle, upper mantle, and the crust. The crust and the part of the upper mantle form the lithosphere, a portion of our planet that is basically rigid, solid rock and runs to about 100 kilometers below the planet's surface. Below that is the asthenosphere, which is hot enough that its rocks are more flexible and ductile than those above it. The lithosphere is divided into roughly two dozen major and minor plates, and these plates move very slowly over the almost fluid-like asthenosphere. There are two types of crust: oceanic crust and continental crust. Predictably enough, oceanic crust makes up the ocean beds and are much thinner than their continental counterparts. Plates can be made up of either oceanic or continental crust, or just as often some combination of the two. There are a variety of forces pushing and pulling the plates in various directions, and indeed that's what keeps Earth's crust from being one solid landmass - the interaction of lithosphere and asthenosphere keeps tearing landmasses apart, albeit very, very slowly. -
Back to the Future II: Tidal Evolution of Four Supercontinent Scenarios
Earth Syst. Dynam., 11, 291–299, 2020 https://doi.org/10.5194/esd-11-291-2020 © Author(s) 2020. This work is distributed under the Creative Commons Attribution 4.0 License. Back to the future II: tidal evolution of four supercontinent scenarios Hannah S. Davies1,2, J. A. Mattias Green3, and Joao C. Duarte1,2,4 1Instituto Dom Luiz (IDL), Faculdade de Ciências, Universidade de Lisboa, Campo Grande, 1749-016, Lisbon, Portugal 2Departamento de Geologia, Faculdade de Ciências, Universidade de Lisboa, Campo Grande, 1749-016, Lisbon, Portugal 3School of Ocean Sciences, Bangor University, Askew St, Menai Bridge LL59 5AB, UK 4School of Earth, Atmosphere and Environment, Monash University, Melbourne, VIC 3800, Australia Correspondence: Hannah S. Davies ([email protected]) Received: 7 October 2019 – Discussion started: 25 October 2019 Revised: 3 February 2020 – Accepted: 8 February 2020 – Published: 20 March 2020 Abstract. The Earth is currently 180 Myr into a supercontinent cycle that began with the break-up of Pangaea and which will end around 200–250 Myr (million years) in the future, as the next supercontinent forms. As the continents move around the planet they change the geometry of ocean basins, and thereby modify their resonant properties. In doing so, oceans move through tidal resonance, causing the global tides to be profoundly affected. Here, we use a dedicated and established global tidal model to simulate the evolution of tides during four future supercontinent scenarios. We show that the number of tidal resonances on Earth varies between one and five in a supercontinent cycle and that they last for no longer than 20 Myr.