Lithospheric Strength and Its Relationship to the Elastic and Seismogenic Layer Thickness
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D6 Lithosphere, Asthenosphere, Mesosphere
200 Chapter d FAMILIAR WORLD The Present is the Key to the Past: HUGH RANCE d6 Lithosphere, asthenosphere, mesosphere < plastic zone > The terms lithosphere and asthenosphere stem from Joseph Barell’s 1914-15 papers on isostasy, entitled The Strength of the Earth's Crust, in the Journal of Geology.1 In the 1960s, seismic studies revealed a zone of rock weakness worldwide near the top of the upper part of the mantle. This zone of weakness is called the asthenosphere (Gk. asthenes, weak). The asthenosphere turned out to be of revolutionary significance for historical geology (see Topic d7, plate tectonic theory). Within the asthenosphere, rock behaves plastically at rates of deformation measured in cm/yr over lineal distances of thousands of kilometers. Above the asthenosphere, at the same rate of deformation, rock behaves elastically and, being brittle, it can break (fault). The shell of rock above the asthenosphere is called the lithosphere (Gk. lithos, stone). The lithosphere as its name implies is more rigid than the asthenosphere. It is important to remember that the names crust and lithosphere are not synonyms. The crust, the upper part of the lithosphere, is continental rock (granitic) in some places and is oceanic rock (basaltic) elsewhere. The lower part of lithosphere is mantle rock (peridotite); cooler but of like composition to the asthenosphere. The asthenosphere’s top (Figure d6.1) has an average depth of 95 km worldwide below 70+ million year old oceanic lithosphere.2 It shallows below oceanic rises to near seafloor at oceanic ridge crests. The rigidity difference between the lithosphere and the asthenosphere exists because downward through the asthenosphere, the weakening effect of increasing temperature exceeds the strengthening effect of increasing pressure. -
Asthenosphere–Lithospheric Mantle Interaction in an Extensional Regime
Chemical Geology 233 (2006) 309–327 www.elsevier.com/locate/chemgeo Asthenosphere–lithospheric mantle interaction in an extensional regime: Implication from the geochemistry of Cenozoic basalts from Taihang Mountains, North China Craton ⁎ Yan-Jie Tang , Hong-Fu Zhang, Ji-Feng Ying State Key Laboratory of Lithospheric Evolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, P.O. Box 9825, Beijing 100029, PR China Received 25 July 2005; received in revised form 27 March 2006; accepted 30 March 2006 Abstract Compositions of Cenozoic basalts from the Fansi (26.3–24.3 Ma), Xiyang–Pingding (7.9–7.3 Ma) and Zuoquan (∼5.6 Ma) volcanic fields in the Taihang Mountains provide insight into the nature of their mantle sources and evidence for asthenosphere– lithospheric mantle interaction beneath the North China Craton. These basalts are mainly alkaline (SiO2 =44–50 wt.%, Na2O+ K2O=3.9–6.0 wt.%) and have OIB-like characteristics, as shown in trace element distribution patterns, incompatible elemental (Ba/Nb=6–22, La/Nb=0.5–1.0, Ce/Pb=15–30, Nb/U=29–50) and isotopic ratios (87Sr/86Sr=0.7038–0.7054, 143Nd/ 144 Nd=0.5124–0.5129). Based on TiO2 contents, the Fansi lavas can be classified into two groups: high-Ti and low-Ti. The Fansi high-Ti and Xiyang–Pingding basalts were dominantly derived from an asthenospheric source, while the Zuoquan and Fansi low-Ti basalts show isotopic imprints (higher 87Sr/86Sr and lower 143Nd/144Nd ratios) compatible with some contributions of sub- continental lithospheric mantle. The variation in geochemical compositions of these basalts resulted from the low degree partial melting of asthenosphere and the interaction of asthenosphere-derived magma with old heterogeneous lithospheric mantle in an extensional regime, possibly related to the far effect of the India–Eurasia collision. -
Seismic Velocity Structure of the Continental Lithosphere from Controlled Source Data
Seismic Velocity Structure of the Continental Lithosphere from Controlled Source Data Walter D. Mooney US Geological Survey, Menlo Park, CA, USA Claus Prodehl University of Karlsruhe, Karlsruhe, Germany Nina I. Pavlenkova RAS Institute of the Physics of the Earth, Moscow, Russia 1. Introduction Year Authors Areas covered J/A/B a The purpose of this chapter is to provide a summary of the seismic velocity structure of the continental lithosphere, 1971 Heacock N-America B 1973 Meissner World J i.e., the crust and uppermost mantle. We define the crust as 1973 Mueller World B the outer layer of the Earth that is separated from the under- 1975 Makris E-Africa, Iceland A lying mantle by the Mohorovi6i6 discontinuity (Moho). We 1977 Bamford and Prodehl Europe, N-America J adopted the usual convention of defining the seismic Moho 1977 Heacock Europe, N-America B as the level in the Earth where the seismic compressional- 1977 Mueller Europe, N-America A 1977 Prodehl Europe, N-America A wave (P-wave) velocity increases rapidly or gradually to 1978 Mueller World A a value greater than or equal to 7.6 km sec -1 (Steinhart, 1967), 1980 Zverev and Kosminskaya Europe, Asia B defined in the data by the so-called "Pn" phase (P-normal). 1982 Soller et al. World J Here we use the term uppermost mantle to refer to the 50- 1984 Prodehl World A 200+ km thick lithospheric mantle that forms the root of the 1986 Meissner Continents B 1987 Orcutt Oceans J continents and that is attached to the crust (i.e., moves with the 1989 Mooney and Braile N-America A continental plates). -
Essentials of Geology
INSTRUCTOR’S MANUAL AND TEST BANK Essentials of Geology Fourth Edition Stephen Marshak Instructor’s Manual by John Werner SEMINOLE STATE COLLEGE OF FLORIDA Test Bank by Jacalyn Gorczynski TEXAS A&M UNIVERSITY– CORPUS CHRISTI Heather L. Lehto ANGELO STATE UNIVERSITY Daniel Wynne SACRAMENTO COMMUNITY COLLEGE B W • W • NORTON & COMPANY • NEW YORK • LONDON —-1 —0 —+1 5577-50734_ch00_2P.indd77-50734_ch00_2P.indd iiiiii 110/5/120/5/12 55:41:41 PPMM W. W. Norton & Company has been in de pen dent since its founding in 1923, when William Warder Norton and Mary D. Herter Norton fi rst published lectures delivered at the People’s Institute, the adult education division of New York City’s Cooper Union. The Nortons soon expanded their program beyond the Institute, publishing books by celebrated academics from America and abroad. By mid- century, the two major pillars of Norton’s publishing program— trade books and college texts— were fi rmly established. In the 1950s, the Norton family transferred control of the company to its employees, and today— with a staff of four hundred and a comparable number of trade, college, and professional titles published each year— W. W. Norton & Company stands as the largest and oldest publishing house owned wholly by its employees. Copyright © 2013, 2009, 2007, 2004 by W. W. Norton & Company, Inc. All rights reserved. Printed in the United States of America. Associate Editor, Supplements: Callinda Taylor. Project Editor: Thom Foley. Production Manager: Benjamin Reynolds. Editorial Assistant, Supplements: Paula Iborra. Composition and project management: Westchester Publishing Ser vices. Art by CodeMantra and Precision Graphics. -
Controls of Subduction Geometry, Location of Magmatic Arcs, and Tectonics of Arc and Back-Arc Regions
Controls of subduction geometry, location of magmatic arcs, and tectonics of arc and back-arc regions TIMOTHY A. CROSS Exxon Production Research Company, P.O. Box 2189, Houston, Texas 77001 REX H. PILGER, JR. Department of Geology, Louisiana State University, Baton Rouge, Louisiana 70803 ABSTRACT States), intra-arc extension (for example, convergence rate, direction and rate of the Basin and Range province), foreland absolute upper-plate motion, age of the de- Most variation in geometry and angle of fold and thrust belts, and Laramide-style scending plate, and subduction of aseismic inclination of subducted oceanic lithosphere tectonics. ridges, oceanic plateaus, or intraplate is caused by four interdependent factors. island-seamount chains. It is crucial to Combinations of (1) rapid absolute upper- INTRODUCTION recognize that, in the natural system of the plate motion toward the trench and active Earth, the major factors may interact and, overriding of the subducted plate, (2) rapid Since Luyendyk's (1970) pioneer attempt therefore, are interdependent variables. De- relative plate convergence, and (3) subduc- to relate subduction-zone geometry to some pending on the associations among them, in tion of intraplate island-seamount chains, fundamental aspect(s) of plate kinematics a historical and spatial context, their aseismic ridges, and oceanic plateaus and dynamics, subsequent investigations effects on the geometry of subducted litho- (anomalously low-density oceanic litho- have suggested an increasing variety and sphere can be additive, or by contrast, one sphere) cause low-angle subduction. Under complexity among possible controls and variable can act in opposition to another conditions of low-angle subduction, the resultant configurations of subduction variable and result in total or partial cancel- upper surface of the subducted plate is in zones. -
Planet Earth in Cross Section by Michael Osborn Fayetteville-Manlius HS
Planet Earth in Cross Section By Michael Osborn Fayetteville-Manlius HS Objectives Devise a model of the layers of the Earth to scale. Background Planet Earth is organized into layers of varying thickness. This solid, rocky planet becomes denser as one travels into its interior. Gravity has caused the planet to differentiate, meaning that denser material have been pulled towards Earth’s center. Relatively less dense material migrates to the surface. What follows is a brief description1 of each layer beginning at the center of the Earth and working out towards the atmosphere. Inner Core – The solid innermost sphere of the Earth, about 1271 kilometers in radius. Examination of meteorites has led geologists to infer that the inner core is composed of iron and nickel. Outer Core - A layer surrounding the inner core that is about 2270 kilometers thick and which has the properties of a liquid. Mantle – A solid, 2885-kilometer thick layer of ultra-mafic rock located below the crust. This is the thickest layer of the earth. Asthenosphere – A partially melted layer of ultra-mafic rock in the mantle situated below the lithosphere. Tectonic plates slide along this layer. Lithosphere – The solid outer portion of the Earth that is capable of movement. The lithosphere is a rock layer composed of the crust (felsic continental crust and mafic ocean crust) and the portion of the mafic upper mantle situated above the asthenosphere. Hydrosphere – Refers to the water portion at or near Earth’s surface. The hydrosphere is primarily composed of oceans, but also includes, lakes, streams and groundwater. -
On the Thermodynamics of Listric Faults
Earth Planets Space, 56, 1111–1120, 2004 On the thermodynamics of listric faults Klaus Regenauer-Lieb1,2, Bruce Hobbs2, and Alison Ord2 1Johannes Gutenberg-Universitat¨ Mainz, Geophysics and Geodynamics, 55099 Mainz, Germany 2CSIRO Exploration and Mining Perth (ARRC), PO Box 1130, Bentley WA 6102, Australia (Received June 15, 2004; Revised November 21, 2004; Accepted December 4, 2004) We investigate a novel fully coupled thermal-mechanical numerical model of the crust in order to trace the physics of interaction of its brittle and ductile layers. In a unified approach these layers develop in a natural transition as a function of the state variables pressure, deviatoric stress, temperature and strain-rate. We find that the main storage of elastic energy lies in the domain where brittle and ductile strain-rates overlap so that shear zones are attracted to this zone of maximum energy dissipation. This dissipation appears as a local heat source (shear heating). The brittle-ductile transition zone evolves through extreme weakening by thermo-mechanical feedback. The physics of the weakening process relies on repeated breaching of a critical energy flux threshold for feedback within this sub-horizontal brittle-ductile flow layer, thus developing unstable slipping events at post- and pre-seismic strain-rates. The width- and the temperature domain of the feedback layer is controlled by the activation enthalpy Q of the material. For olivine rheology (Q ∼ 500 kJ/mol) the layer can be extremely thin <500 m and adheres to the 875 K isotherm. For quartz (Q ∼ 135 kJ/mol) the width of the feedback layer fans out into multiple interacting ductile faults covering a temperature domain of 450–600 K. -
The Distribution of Water in the Continental Lithospheric Mantle and Its Implications for the Stability of Continents
Invited Review Geology November 2013 Vol.58 No.32: 38793889 doi: 10.1007/s11434-013-5949-1 The distribution of water in the continental lithospheric mantle and its implications for the stability of continents XIA QunKe* & HAO YanTao CAS Key Laboratory of Crust-Mantle Materials and Environments, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China Received January 14, 2013; accepted May 14, 2013; published online July 11, 2013 The lithospheric mantle is one of the key layers controlling the stability of continents. Even a small amount of water can influence many chemical and physical properties of rocks and minerals. Consequently, it is a pivotal task to study the distribution of water in the continental lithosphere. This paper presents a brief overview of the current state of knowledge about (1) the occurrence of water in the continental lithospheric mantle, (2) the spatial and temporal variations of the water content in the continental litho- spheric mantle, and (3) the relationship between water content and continent stability. Additionally, suggestions for future re- search directions are briefly discussed. water, nominally anhydrous minerals, continental lithospheric mantle, continent stability Citation: Xia Q K, Hao Y T. The distribution of water in the continental lithospheric mantle and its implications for the stability of continents. Chin Sci Bull, 2013, 58: 38793889, doi: 10.1007/s11434-013-5949-1 The lithospheric mantle is the lowermost part of continental continental lithospheric mantle is tightly related to its vis- plates; its viscosity contrast with the underlying astheno- cosity and stability [23,25–28]. -
Plate Tectonics
Plate tectonics tive motion determines the type of boundary; convergent, divergent, or transform. Earthquakes, volcanic activity, mountain-building, and oceanic trench formation occur along these plate boundaries. The lateral relative move- ment of the plates typically varies from zero to 100 mm annually.[2] Tectonic plates are composed of oceanic lithosphere and thicker continental lithosphere, each topped by its own kind of crust. Along convergent boundaries, subduction carries plates into the mantle; the material lost is roughly balanced by the formation of new (oceanic) crust along divergent margins by seafloor spreading. In this way, the total surface of the globe remains the same. This predic- The tectonic plates of the world were mapped in the second half of the 20th century. tion of plate tectonics is also referred to as the conveyor belt principle. Earlier theories (that still have some sup- porters) propose gradual shrinking (contraction) or grad- ual expansion of the globe.[3] Tectonic plates are able to move because the Earth’s lithosphere has greater strength than the underlying asthenosphere. Lateral density variations in the mantle result in convection. Plate movement is thought to be driven by a combination of the motion of the seafloor away from the spreading ridge (due to variations in topog- raphy and density of the crust, which result in differences in gravitational forces) and drag, with downward suction, at the subduction zones. Another explanation lies in the different forces generated by the rotation of the globe and the tidal forces of the Sun and Moon. The relative im- portance of each of these factors and their relationship to each other is unclear, and still the subject of much debate. -
The Mid-Lithospheric Discontinuity Caused by Channel Flow in the Cratonic Lithosphere
The Mid-Lithospheric Discontinuity caused by channel flow in the cratonic lithosphere Haibin Yang *a, b, Irina M. Artemieva c,d,e, Hans Thybo e,f,g a. School of Earth Sciences, University of Melbourne, Melbourne, Australia b. Research School of Earth Sciences, Australian National University, Canberra, Australia c. Department of Geophysics, Stanford University, Stanford, CA 94305, USA d. Section of Oceanic Dynamics, GEOMAR Helmholtz Center for Ocean Research, Kiel 24148, Germany e. State Key Laboratory of Geological Processes and Mineral Resources, School of Earth Sciences, China University of Geosciences, Wuhan, China f. Eurasia Institute of Earth Science, Istanbul Technical University, Maslak, 34469 Istanbul, Turkey g. Centre for Earth Evolution and Dynamics (CEED), University of Oslo, Blindern, 0316 Oslo, Norway Corresponding author: Haibin Yang Email: [email protected] This is a non-peer reviewed preprint submitted to EarthArXiv. 1 Abstract Stable cratons with a thick (> 200 km) and cold lithosphere form rheologically strong plates that move atop a ductile asthenospheric mantle. Various types of seismic observations show the presence of a potentially rheologically weak zone at depths of ca. 80 – 150 km termed the Mid-Lithosphere Discontinuity (MLD). While various mechanisms may explain the MLD, the dynamic processes leading to the seismic observations are unclear. We propose that the MLD can be caused by channel flow in the lower lithosphere, triggered by negative Rayleigh-Taylor instabilities at cratonic margins in the Archean, when the mantle was hotter than at present. Presence of a chemically distinct, low-density cratonic lithospheric root is required to initiate the process. Numerical modeling shows that the top of the channel flow creates a shear zone at a depth comparable to the globally observed seismic MLD. -
Variations in Wedge Earthquake Distribution Along the Strike Underlain by Thermally Controlled Hydrated Megathrusts
applied sciences Article Variations in Wedge Earthquake Distribution along the Strike Underlain by Thermally Controlled Hydrated Megathrusts Rui Qu 1,2 , Yingfeng Ji 1,2,* and Weiling Zhu 1,3,* 1 State Key Laboratory of Tibetan Plateau Earth System, Resources and Environment (TPESRE), Institute of Tibetan Plateau Research, Chinese Academy of Sciences, Beijing 100101, China; [email protected] 2 College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China 3 Department of Geophysics, Yunnan University, Kunming 650091, China * Correspondence: [email protected] (Y.J.); [email protected] (W.Z.) Featured Application: Resource and environmental effects. Abstract: Accretionary wedge earthquakes usually occur in the overriding crust close to the trench or above the cold nose of the mantle wedge. However, the mechanism and temperature properties related to the slab dip angle remain poorly understood. Based on 3D thermal models to estimate the subduction wedge plate temperature and structure, we investigate the distribution of wedge earthquakes in Alaska, which has a varying slab dip angle along the trench. The horizontal distance of wedge-earthquake hypocenters significantly increases from the Aleutian Islands to south–central Alaska due to a transition from steep subduction to flat subduction. Slab dehydration inside the subducted Pacific plate indicates a simultaneous change in the distances between the intraslab metamorphic fronts and the Alaskan Trench at various depths, which is associated with the flattening Citation: Qu, R.; Ji, Y.; Zhu, W. of the Pacific plate eastward along the strike. The across-arc width of the wedge-earthquake source Variations in Wedge Earthquake zone is consistent with the across-arc width of the surface high topography above the fully dehydrated Distribution along the Strike megathrust, and the fluid upwelling spontaneously influences wedge seismotectonics and orogenesis. -
Origin and Evolution of Asthenospheric Layers
Two mechanisms of formation of asthenospheric layers L. Czechowski and M. Grad Institute of Geophysics, Faculty of Physics, University of Warsaw Ul. Pasteura 5, 02-093 Warszawa, Poland Phone: +48 22 5532003 E-mail: [email protected] Corresponding author: Leszek Czechowski: [email protected] The theory of plate tectonics describes some basic global tectonic processes as a result of motion of lithospheric plates. The boundary between lithosphere and asthenosphere (LAB) is defined by a difference in response to stress. Position of LAB is determined by: (i) the ratio (melting temperature)/( temperature) and (ii) an invariant of the stress tensor. We consider the role of these both factors for origin and decay of asthenosphere. We find that the asthenosphere of shear stress origin could be a transient, time-dependent feature. Key words: asthenosphere, evolution, LAB, origin of asthenosphere 1. Introduction The plate tectonics theory describes some of the basic tectonic processes on the Earth as motion of lithospheric plates. The plates are moved by large-scale thermal convection in the mantle. The lithosphere is mechanically resistant. Its thickness varies from ~50 to ~250 km. The lithosphere is underlain by the asthenosphere. The boundary between the lithosphere and the asthenosphere (LAB) is defined by a difference in response to stress: the asthenosphere deforms viscously. The bulk of asthenosphere is not melted (1), but at the deformation rate typical for the mantle convection (about 10-14 s-1) it behaves as a fluid with the viscosity η of about 5 1019 kg m-1 s-1. The mantle below has higher effective viscosity (e.g.