When and How Did Plate Tectonics Begin? Theoretical and Empirical Considerations
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Ocean Trench
R E S O U R C E L I B R A R Y E N C Y C L O P E D I C E N T RY Ocean trench Ocean trenches are long, narrow depressions on the seafloor. These chasms are the deepest parts of the ocean—and some of the deepest natural spots on Earth. G R A D E S 5 - 12+ S U B J E C T S Earth Science, Geology, Geography, Physical Geography C O N T E N T S 11 Images, 1 Video, 2 Links For the complete encyclopedic entry with media resources, visit: http://www.nationalgeographic.org/encyclopedia/ocean-trench/ Ocean trenches are long, narrow depressions on the seafloor. These chasms are the deepest parts of the ocean—and some of the deepest natural spots on Earth. Ocean trenches are found in every ocean basin on the planet, although the deepest ocean trenches ring the Pacific as part of the so-called “Ring of Fire” that also includes active volcanoes and earthquake zones. Ocean trenches are a result of tectonic activity, which describes the movement of the Earth’s lithosphere. In particular, ocean trenches are a feature of convergent plate boundaries, where two or more tectonic plates meet. At many convergent plate boundaries, dense lithosphere melts or slides beneath less-dense lithosphere in a process called subduction, creating a trench. Ocean trenches occupy the deepest layer of the ocean, the hadalpelagic zone. The intense pressure, lack of sunlight, and frigid temperatures of the hadalpelagic zone make ocean trenches some of the most unique habitats on Earth. -
0 Master's Thesis the Department of Geosciences And
Master’s thesis The Department of Geosciences and Geography Physical Geography South American subduction zone processes: Visualizing the spatial relation of earthquakes and volcanism at the subduction zone Nelli Metiäinen May 2019 Thesis instructors: David Whipp Janne Soininen HELSINGIN YLIOPISTO MATEMAATTIS-LUONNONTIETEELLINEN TIEDEKUNTA GEOTIETEIDEN JA MAANTIETEEN LAITOS MAANTIEDE PL 64 (Gustaf Hällströmin katu 2) 00014 Helsingin yliopisto 0 Tiedekunta/Osasto – Fakultet/Sektion – Faculty Laitos – Institution – Department Faculty of Science The Department of Geosciences and Geography Tekijä – Författare – Author Nelli Metiäinen Työn nimi – Arbetets titel – Title South American subduction zone processes: Visualizing the spatial relation of earthquakes and volcanism at the subduction zone Oppiaine – Läroämne – Subject Physical Geography Työn laji – Arbetets art – Level Aika – Datum – Month and year Sivumäärä – Sidoantal – Number of pages Master’s thesis May 2019 82 + appencides Tiivistelmä – Referat – Abstract The South American subduction zone is the best example of an ocean-continent convergent plate margin. It is divided into segments that display different styles of subduction, varying from normal subduction to flat-slab subduction. This difference also effects the distribution of active volcanism. Visualizations are a fast way of transferring large amounts of information to an audience, often in an interest-provoking and easily understandable form. Sharing information as visualizations on the internet and on social media plays a significant role in the transfer of information in modern society. That is why in this study the focus is on producing visualizations of the South American subduction zone and the seismic events and volcanic activities occurring there. By examining the South American subduction zone it may be possible to get new insights about subduction zone processes. -
Initiation of Plate Tectonics in the Hadean: Eclogitization Triggered by the ABEL Bombardment
Accepted Manuscript Initiation of plate tectonics in the Hadean: Eclogitization triggered by the ABEL Bombardment S. Maruyama, M. Santosh, S. Azuma PII: S1674-9871(16)30207-9 DOI: 10.1016/j.gsf.2016.11.009 Reference: GSF 514 To appear in: Geoscience Frontiers Received Date: 9 May 2016 Revised Date: 13 November 2016 Accepted Date: 25 November 2016 Please cite this article as: Maruyama, S., Santosh, M., Azuma, S., Initiation of plate tectonics in the Hadean: Eclogitization triggered by the ABEL Bombardment, Geoscience Frontiers (2017), doi: 10.1016/ j.gsf.2016.11.009. This is a PDF file of an unedited manuscript that has been accepted for publication. As a service to our customers we are providing this early version of the manuscript. The manuscript will undergo copyediting, typesetting, and review of the resulting proof before it is published in its final form. Please note that during the production process errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain. ACCEPTED MANUSCRIPT MANUSCRIPT ACCEPTED P a g e ‐|‐1111‐‐‐‐ ACCEPTED MANUSCRIPT ‐ 1‐ Initiation of plate tectonics in the Hadean: 2‐ Eclogitization triggered by the ABEL 3‐ Bombardment 4‐ 5‐ S. Maruyama a,b,*, M. Santosh c,d,e , S. Azuma a 6‐ a Earth-Life Science Institute, Tokyo Institute of Technology, 2-12-1, 7‐ Ookayama-Meguro-ku, Tokyo 152-8550, Japan 8‐ b Institute for Study of the Earth’s Interior, Okayama University, 827 Yamada, 9‐ Misasa, Tottori 682-0193, Japan 10‐ c Centre for Tectonics, Resources and Exploration, Department of Earth 11‐ Sciences, University of Adelaide, SA 5005, Australia 12‐ d School of Earth Sciences and Resources, China University of Geosciences 13‐ Beijing, 29 Xueyuan Road, Beijing 100083, China 14‐ e Faculty of Science, Kochi University, KochiMANUSCRIPT 780-8520, Japan 15‐ *Corresponding author. -
And Post-Collision Calc-Alkaline Magmatism in the Qinling Orogenic Belt, Central China, As Documented by Zircon Ages on Granitoid Rocks
Journal of the Geological Societv. London, Vol. 153, 1996, pp. 409-417. Palaeozoic pre- and post-collision calc-alkaline magmatism in the Qinling orogenic belt, central China, as documented by zircon ages on granitoid rocks F. XUE'.*,',A. KRONER', T. REISCHMANN' & F. LERCH' 'Institut fiir Geowissenschaften, Universitat Mainz, 55099 Mainz, Germany 'Department of Geology, Northwest University, 710069 Xi'an, China .'Present address: Department of Geophysical Sciences, The University of Chicago, 5734 South Ellis Avenue, Chicago, IL 60637, USA Abstract: Basedon large-scale reconnaissance mapping, we identifiedtwo calc-alkaline plutonic assemblagesfrom the northern Qinling orogenic belt.central China. The older assemblage of intrusions. closely associated and deformed coevally with their host volcanic arc sequences, seems to represent the fractionation product of basaltic arc magma. It therefore predates the collision of the North China Block with the Central Qinling island-arc system that developed in a SW Pacific-type oceanic domain south of the North China Block. Single-zircon zo7Pb/2'"Pb evaporation dating yielded early to middle Ordovician ages for this assemblage. with a relatively small range from 487.2 f 1.1 to 470.2 f 1.3 Ma. Intrusions of the younger assemblage are largely undeformed and truncate structures shown in rocks of theolder assemblage. They are interpreted as post-collisional calc-alkaline granitoids.Single zircon dating provided an age of 401.8 f 0.8 Mafor the younger assemblage. consistentwith earlier work that defines an age range from c. 420 to 395Ma. Our datafavour a tectonicmodel involving formation and amalgamation of islandarc and microcontinent terranes between ca. 490 and 470 Ma ago to create the Central Qinling Zone which subsequently collided with theNorth China Block prior to c. -
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. -
Coastal and Marine Ecological Classification Standard (2012)
FGDC-STD-018-2012 Coastal and Marine Ecological Classification Standard Marine and Coastal Spatial Data Subcommittee Federal Geographic Data Committee June, 2012 Federal Geographic Data Committee FGDC-STD-018-2012 Coastal and Marine Ecological Classification Standard, June 2012 ______________________________________________________________________________________ CONTENTS PAGE 1. Introduction ..................................................................................................................... 1 1.1 Objectives ................................................................................................................ 1 1.2 Need ......................................................................................................................... 2 1.3 Scope ........................................................................................................................ 2 1.4 Application ............................................................................................................... 3 1.5 Relationship to Previous FGDC Standards .............................................................. 4 1.6 Development Procedures ......................................................................................... 5 1.7 Guiding Principles ................................................................................................... 7 1.7.1 Build a Scientifically Sound Ecological Classification .................................... 7 1.7.2 Meet the Needs of a Wide Range of Users ...................................................... -
Extrusive and Intrusive Magmatism Greatly Influence the Tectonic Mode of Earth-Like Planets
EPSC Abstracts Vol. 11, EPSC2017-945, 2017 European Planetary Science Congress 2017 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2017 Extrusive and Intrusive Magmatism Greatly Influence the Tectonic Mode of Earth-Like Planets D. Lourenco, P. J. Tackley, A. Rozel and M. Ballmer Institute of Geophysics, Department of Earth Sciences, ETH Zurich, Switzerland ([email protected] / Fax: +41 44 633 1065) Abstract reported in [3], we use thermo-chemical global mantle convection numerical simulations to Plate tectonics on Earth-like planets is typically systematically investigate the effect of plutonism, in modelling using a strongly temperature-dependent conjugation with eruptive volcanism. Results visco-plastic rheology. Previous analyses have reproduce the three common tectonic/convective generally focussed on purely thermal convection. regimes usually obtained in simulations using a However, we have shown that the influence of visco-plastic rheology: stagnant-lid (a one-plate compositional heterogeneity in the form of planet), episodic (where the lithosphere is unstable continental [1] or oceanic [2] crust can greatly and frequently overturns into the mantle), and influence plate tectonics by making it easier (i.e. it mobile-lid (similar to plate tectonics). At high occurs at a lower yield stress or friction coefficient). intrusion efficiencies, we observe and characterise a Here we present detailed results on this topic, in new additional regime called “plutonic-squishy lid”. particular focussing on the influence of intrusive vs. This regime is characterised by a set of strong plates extrusive magmatism on the tectonic mode. separated by warm and weak regions generated by plutonism. Eclogitic drippings and lithospheric delaminations often occur around these weak regions. -
1 John A. Tarduno
JOHN A. TARDUNO January, 2016 Professor of Geophysics Tel: 585-275-5713 Department of Earth and Environmental Sciences Fax: 585-244-5689 University of Rochester, Rochester, NY 14627 Email: [email protected] USA http://www.ees.rochester.edu/people/faculty/tarduno_john Academic Career: 2005-present Professor of Physics and Astronomy, University of Rochester, Rochester, NY. 2000-present Professor of Geophysics, University of Rochester, Rochester, NY. 1998-2006 Chair, Department of Earth and Environmental Sciences 1996 Associate Professor of Geophysics, University of Rochester, Rochester, NY. 1993 Assistant Professor of Geophysics, University of Rochester, Rochester, NY. 1990 Assistant Research Geophysicist, Scripps Institution of Oceanography, La Jolla, Ca. 1989 National Science Foundation Postdoctoral Fellow, ETH, Zürich, Switzerland 1988 JOI/USSAC Ocean Drilling Fellow, Stanford University, Stanford, Ca. 1987 Ph.D. (Geophysics), Stanford University, Stanford, Ca. 1987 M.S. (Geophysics) Stanford University, Stanford Ca. 1983 B.S. (Geophysics) Lehigh University, Bethlehem Pa. Honors and Awards: Phi Beta Kappa (1983) Fellow, Geological Society of America (1998) JOI/USSAC Distinguished Lecturer (2000-2001) Goergen Award for Distinguished Achievement and Artistry in Undergraduate Teaching (2001) Fellow, American Association for the Advancement of Science (2003) American Geophysical Union/Geomagnetism and Paleomagnetism Section Bullard Lecturer (2004) Fellow, John Simon Guggenheim Foundation (2006-2007) Edward Peck Curtis Award for -
The Rock and Fossil Record the Rock and Fossil Record the Rock And
TheThe RockRock andand FossilFossil RecordRecord Earth’s Story and Those Who First Listened . 426 Apply . 427 Internet Connect . 428 When on Earth? . 429 Activity . 430 MathBreak . 434 Internet Connect 432, 435 Looking at Fossils . 436 QuickLab . 438 Internet Connect . 440 Time Marches On . 441 QuickLab . 443 Internet Connect . 445 Chapter Lab . 446 Chapter Review . 449 TEKS/TAKS Practice Tests . 451, 452 Feature Article . 453 Time Stands Still Pre-Reading Questions Sealed in darkness for 49 million years, this beetle still shimmers with the same metallic hues that once helped it hide among ancient plants. This rare fossil 1. How do scientists study was found in Messel, Germany. In the same rock formation, the Earth’s history? scientists have found fossilized crocodiles, bats, birds, and 2. How can you tell the age frogs. A living stag beetle (above) has a similar form and of rocks and fossils? color. Do you think that these two beetles would live in 3. What natural or human similar environments? What do you think Messel, Germany, events have caused mass was like 49 million years ago? In this chapter, you will extinctions in Earth’s learn how scientists answer these kinds of questions. history? 424 Chapter 16 Copyright © by Holt, Rinehart and Winston. All rights reserved. MAKING FOSSILS Procedure 1. You and three or four of your classmates will be given several pieces of modeling clay and a paper sack containing a few small objects. 2. Press each object firmly into a piece of clay. Try to leave an imprint showing as much detail as possible. -
Volcanism in a Plate Tectonics Perspective
Appendix I Volcanism in a Plate Tectonics Perspective 1 APPENDIX I VOLCANISM IN A PLATE TECTONICS PERSPECTIVE Contributed by Tom Sisson Volcanoes and Earth’s Interior Structure (See Surrounded by Volcanoes and Magma Mash for relevant illustrations and activities.) To understand how volcanoes form, it is necessary to know something about the inner structure and dynamics of the Earth. The speed at which earthquake waves travel indicates that Earth contains a dense core composed chiefly of iron. The inner part of the core is solid metal, but the outer part is melted and can flow. Circulation (movement) of the liquid outer core probably creates Earth’s magnetic field that causes compass needles to point north and helps some animals migrate. The outer core is surrounded by hot, dense rock known as the mantle. Although the mantle is nearly everywhere completely solid, the rock is hot enough that it is soft and pliable. It flows very slowly, at speeds of inches-to-feet each year, in much the same way as solid ice flows in a glacier. Earth’s interior is hot both because of heat left over from its formation 4.56 billion years ago by meteorites crashing together (accreting due to gravity), and because of traces of natural radioactivity in rocks. As radioactive elements break down into other elements, they release heat, which warms the inside of the Earth. The outermost part of the solid Earth is the crust, which is colder and about ten percent less dense than the mantle, both because it has a different chemical composition and because of lower pressures that favor low-density minerals. -
Stagnant Lid Tectonics: Perspectives from Silicate Planets, Dwarf Planets, Large Moons, and Large Asteroids
Geoscience Frontiers 9 (2018) 103e119 HOSTED BY Contents lists available at ScienceDirect China University of Geosciences (Beijing) Geoscience Frontiers journal homepage: www.elsevier.com/locate/gsf Research Paper Stagnant lid tectonics: Perspectives from silicate planets, dwarf planets, large moons, and large asteroids Robert J. Stern a,*, Taras Gerya b, Paul J. Tackley b a Geosciences Department, University of Texas at Dallas, Richardson, TX 75083-0688, USA b Department of Earth Sciences, ETH-Zurich, 8092 Zurich, Switzerland article info abstract Article history: To better understand Earth’s present tectonic styleeplate tectonicseand how it may have evolved from Received 7 November 2016 single plate (stagnant lid) tectonics, it is instructive to consider how common it is among similar bodies Received in revised form in the Solar System. Plate tectonics is a style of convection for an active planetoid where lid fragment 22 May 2017 (plate) motions reflect sinking of dense lithosphere in subduction zones, causing upwelling of Accepted 16 June 2017 asthenosphere at divergent plate boundaries and accompanied by focused upwellings, or mantle plumes; Available online 1 July 2017 any other tectonic style is usefully called “stagnant lid” or “fragmented lid”. In 2015 humanity completed a50þ year effort to survey the 30 largest planets, asteroids, satellites, and inner Kuiper Belt objects, Keywords: “ ” Stagnant lid which we informally call planetoids and use especially images of these bodies to infer their tectonic Solar system activity. The four largest planetoids are enveloped in gas and ice (Jupiter, Saturn, Uranus, and Neptune) Plate tectonics and are not considered. The other 26 planetoids range in mass over 5 orders of magnitude and in Planets diameter over 2 orders of magnitude, from massive Earth down to tiny Proteus; these bodies also range Moons widely in density, from 1000 to 5500 kg/m3. -
Is Plate Tectonics Needed to Evolve Technological Species on Exoplanets?
Geoscience Frontiers 7 (2016) 573e580 HOSTED BY Contents lists available at ScienceDirect China University of Geosciences (Beijing) Geoscience Frontiers journal homepage: www.elsevier.com/locate/gsf Research paper Is plate tectonics needed to evolve technological species on exoplanets? Robert J. Stern Geoscience Department, University of Texas at Dallas, Richardson, TX 75080, USA article info abstract Article history: As we continue searching for exoplanets, we wonder if life and technological species capable of Received 23 September 2015 communicating with us exists on any of them. As geoscientists, we can also wonder how important is the Received in revised form presence or absence of plate tectonics for the evolution of technological species. This essay considers this 18 November 2015 question, focusing on tectonically active rocky (silicate) planets, like Earth, Venus, and Mars. The Accepted 4 December 2015 development of technological species on Earth provides key insights for understanding evolution on Available online 29 December 2015 exoplanets, including the likely role that plate tectonics may play. An Earth-sized silicate planet is likely Keywords: to experience several tectonic styles over its lifetime, as it cools and its lithosphere thickens, strengthens, Plate tectonics and becomes denser. These include magma ocean, various styles of stagnant lid, and perhaps plate Exoplanets tectonics. Abundant liquid water favors both life and plate tectonics. Ocean is required for early evolution Planetary science of diverse single-celled organisms, then colonies of cells which specialized further to form guts, ap- Intelligent life pendages, and sensory organisms up to the complexity of fish (central nervous system, appendages, eyes). Large expanses of dry land also begin in the ocean, today produced above subduction zones in juvenile arcs and by their coalescence to form continents, although it is not clear that plate tectonics was required to create continental crust on Earth.