The African Plate: a History of Oceanic Crust Accretion and Subduction Since the Jurassic
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The Mediterranean Region—A Geological Primer
160 Article by William Cavazza1 and Forese Carlo Wezel2 The Mediterranean region—a geological primer 1 Dept. of Earth and Geoenvironmental Sciences, Univ. of Bologna, Italy. [email protected] 2 Institute of Environmental Dynamics, University of Urbino, Italy. [email protected] The last twenty-five years of geological investigation of the Mediterranean region have disproved the traditional Introduction notion that the Alpine-Himalayan mountain ranges Many important ideas and influential geological models have been originated from the closure of a single, albeit complex, developed based on research undertaken in the Mediterranean oceanic domain—the Tethys. Instead, the present-day region. For example, the Alps are the most studied orogen in the geological configuration of the Mediterranean region is world, their structure has been elucidated in great detail for the most part and has served as an orogenic model applied to other collisional the result of the creation and ensuing consumption of orogens. Ophiolites and olistostromes were defined and studied for two major oceanic basins—the Paleotethys and the the first time in this region. The Mediterranean Sea has possibly the Neotethys—and of additional smaller oceanic basins highest density of DSDP/ODP sites in the world, and extensive within an overall regime of prolonged interaction research on its Messinian deposits and on their on-land counterparts has provided a spectacular example for the generation of widespread between the Eurasian and the African-Arabian plates. basinal evaporites. Other portions of this region are less well under- In greater detail, there is still some debate about exactly stood and are now the focus of much international attention. -
Iberian Plate-Kinematics in Paleomagnetic and Mantle Reference Frames, Gondwana Research (2016), Doi: 10.1016/J.Gr.2016.03.006
ÔØ ÅÒÙ×Ö ÔØ Cretaceous slab break-off in the Pyrenees: Iberian plate-kinematics in paleo- magnetic and mantle reference frames Reinoud L.M. Vissers, Douwe J.J. van Hinsbergen, Douwe G. van der Meer, Wim Spakman PII: S1342-937X(16)30053-3 DOI: doi: 10.1016/j.gr.2016.03.006 Reference: GR 1599 To appear in: Gondwana Research Received date: 21 September 2015 Revised date: 2 March 2016 Accepted date: 3 March 2016 Please cite this article as: Vissers, Reinoud L.M., van Hinsbergen, Douwe J.J., van der Meer, Douwe G., Spakman, Wim, Cretaceous slab break-off in the Pyrenees: Iberian plate-kinematics in paleomagnetic and mantle reference frames, Gondwana Research (2016), doi: 10.1016/j.gr.2016.03.006 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 Cretaceous slab break-off in the Pyrenees: Iberian plate- kinematics in paleomagnetic and mantle reference frames Reinoud L.M. Vissers1, Douwe J.J. van Hinsbergen1, Douwe G. van der Meer1,2, Wim Spakman1,3 1 Department of Earth Sciences, Utrecht University, Budapestlaan 4, Utrecht 3584 CD, Netherlands 2 Nexen Petroleum UK Ltd, 97 Oxford Road, Uxbridge, Middlesex UB8 1LU, UK 3 Center for Earth Evolution and Dynamics (CEED), University of Oslo, Sem Saelands vei 24, NO-0316 Oslo, Norway corresponding author: Reinoud L.M. -
India-Asia Collision and the Cenozoic Slowdown of the Indian Plate
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 115, B03410, doi:10.1029/2009JB006634, 2010 Click Here for Full Article India-Asia collision and the Cenozoic slowdown of the Indian plate: Implications for the forces driving plate motions Alex Copley,1 Jean-Philippe Avouac,1 and Jean-Yves Royer2 Received 21 May 2009; revised 12 August 2009; accepted 25 September 2009; published 17 March 2010. [1] The plate motion of India changed dramatically between 50 and 35 Ma, with the rate of convergence between India and Asia dropping from 15 to 4 cm/yr. This change is coincident with the onset of the India-Asia collision, and with a rearrangement of plate boundaries in the Indian Ocean. On the basis of a simple model for the forces exerted upon the edges of the plate and the tractions on the base of the plate, we perform force balance calculations for the precollision and postcollision configurations. We show that the observed Euler poles for the Indian plate are well explained in terms of their locations and magnitudes if (1) the resistive force induced by mountain building in the Himalaya-Tibet area is 5–6 Â 1012 N/m, (2) the net force exerted upon the Indian plate by subduction zones is similar in magnitude to the ridge-push force (2.5 Â 1012 N/m), and (3) basal tractions exert a resisting force that is linearly proportional to the plate velocity in the hot spot reference frame. The third point implies an asthenospheric viscosity of 2–5 Â 1019 Pa s, assuming a thickness of 100–150 km. -
Readingsample
The TRANSMED Atlas. The Mediterranean Region from Crust to Mantle Geological and Geophysical Framework of the Mediterranean and the Surrounding Areas Bearbeitet von William Cavazza, François M. Roure, Wim Spakman, Gerard M. Stampfli, Peter A. Ziegler 1. Auflage 2004. Buch. xxiii, 141 S. ISBN 978 3 540 22181 4 Format (B x L): 19,3 x 27 cm Gewicht: 660 g Weitere Fachgebiete > Physik, Astronomie > Angewandte Physik > Geophysik Zu Inhaltsverzeichnis schnell und portofrei erhältlich bei Die Online-Fachbuchhandlung beck-shop.de ist spezialisiert auf Fachbücher, insbesondere Recht, Steuern und Wirtschaft. Im Sortiment finden Sie alle Medien (Bücher, Zeitschriften, CDs, eBooks, etc.) aller Verlage. Ergänzt wird das Programm durch Services wie Neuerscheinungsdienst oder Zusammenstellungen von Büchern zu Sonderpreisen. Der Shop führt mehr als 8 Millionen Produkte. Chapter 1 The Mediterranean Area and the Surrounding Regions: Active Processes, Remnants of Former Tethyan Oceans and Related Thrust Belts William Cavazza · François Roure · Peter A. Ziegler Abstract 1.1 Introduction The Mediterranean domain provides a present-day geo- From the pioneering studies of Marsili – who singlehand- dynamic analog for the final stages of a continent-conti- edly founded the field of oceanography with the publi- nent collisional orogeny. Over this area, oceanic lithos- cation in 1725 of the Histoire physique de la mer, a scien- pheric domains originally present between the Eurasian tific best-seller of the time (Sartori 2003) – to the tech- and African-Arabian plates have been subducted and par- nologically most advanced cruises of the R/V JOIDES tially obducted, except for the Ionian basin and the south- Resolution, the Mediterranean Sea has represented a cru- eastern Mediterranean. -
1. the Western Iberia Margin: a Geophysical and Geological Overview1
Whitmarsh, R.B., Sawyer, D.S., Klaus, A., and Masson, D.G. (Eds.), 1996 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 149 1. THE WESTERN IBERIA MARGIN: A GEOPHYSICAL AND GEOLOGICAL OVERVIEW1 L.M. Pinheiro,2 R.C.L. Wilson,3 R. Pena dos Reis,4 R.B. Whitmarsh,5 A. Ribeiro6 ABSTRACT This paper presents a general overview of the geology and geophysics of western Iberia, and in particular of the western Portuguese Margin. The links between the onshore and offshore geology and geophysics are especially emphasized. The west Iberia Margin is an example of a nonvolcanic rifted margin. The Variscan basement exposed on land in Iberia exhibits strike- slip faults and other structural trends, which had an important effect on the development, in time and space, of subsequent rift- ing of the continental margin and even perhaps influences the present-day offshore seismicity. The margin has had a long tec- tonic and magmatic history from the Late Triassic until the present day. Rifting first began in the Late Triassic; after about 70 Ma, continental separation began in the Tagus Abyssal Plain. Continental breakup then appears to have progressively migrated northwards, eventually reaching the Galicia Bank segment of the margin about 112 Ma. Although there is onshore evidence of magmatism throughout the period from the Late Triassic until 130 Ma and even later, this was sporadic and of insignificant vol- ume. Important onshore rift basins were formed during this period. Offshore, the record is complex and fragmentary. An ocean/ continent transition, over 150 km wide, lies beyond the shelf edge and is marked on its western side by a peridotite ridge and thin oceanic crust characterized by seafloor spreading anomalies. -
Greater India Basin Hypothesis and a Two-Stage Cenozoic Collision Between India and Asia
Greater India Basin hypothesis and a two-stage Cenozoic collision between India and Asia Douwe J. J. van Hinsbergena,b,1, Peter C. Lippertc,d, Guillaume Dupont-Nivete,f,g, Nadine McQuarrieh, Pavel V. Doubrovinea,b, Wim Spakmani, and Trond H. Torsvika,b,j,k aPhysics of Geological Processes, University of Oslo, Sem Sælands vei 24, NO-0316 Oslo, Norway; bCenter for Advanced Study, Norwegian Academy of Science and Letters, Drammensveien 78, 0271 Oslo, Norway; cDepartment of Geosciences, University of Arizona, Tucson, AZ 85721; dDepartment of Earth and Planetary Sciences, University of California, Santa Cruz, CA 95064; eGéosciences Rennes, Unité Mixte de Recherche 6118, Université de Rennes 1, Campus de Beaulieu, 35042 Rennes Cedex, France; fPaleomagnetic Laboratory Fort Hoofddijk, Department of Earth Sciences, University of Utrecht, Budapestlaan 17, 3584 CD, Utrecht, The Netherlands; gKey Laboratory of Orogenic Belts and Crustal Evolution, Ministry of Education, Peking University, Beijing 100871, China; hDepartment of Geology and Planetary Science, University of Pittsburgh, Pittsburgh, PA 15260; iDepartment of Earth Sciences, University of Utrecht, Budapestlaan 4, 3584 CD, Utrecht, The Netherlands; jCenter for Geodynamics, Geological Survey of Norway, Leiv Eirikssons vei 39, 7491 Trondheim, Norway; and kSchool of Geosciences, University of the Witwatersrand, WITS 2050, Johannesburg, South Africa Edited by B. Clark Burchfiel, Massachusetts Institute of Technology, Cambridge, MA, and approved March 29, 2012 (received for review October 19, 2011) Cenozoic convergence between the Indian and Asian plates pro- (Fig. 2; SI Text) as well as with an abrupt decrease in India–Asia duced the archetypical continental collision zone comprising the convergence rates beginning at 55–50 Ma, as demonstrated by Himalaya mountain belt and the Tibetan Plateau. -
Himalaya - Southern-Tibet: the Typical Continent-Continent Collision Orogen
237 Himalaya - Southern-Tibet: the typical continent-continent collision orogen When an oceanic plate is subducted beneath a continental lithosphere, an Andean mountain range develops on the edge of the continent. If the subducting plate also contains some continental lithosphere, plate convergence eventually brings both continents into juxtaposition. While the oceanic lithosphere is relatively dense and sinks into the asthenosphere, the greater sialic content of the continental lithosphere ascribes positive buoyancy in the asthenosphere, which hinders the continental lithosphere to be subducted any great distance. Consequently, a continental lithosphere arriving at a trench will confront the overriding continent. Rapid relative convergence is halted and crustal shortening forms a collision mountain range. The plane marking the locus of collision is a suture, which usually preserves slivers of the oceanic lithosphere that formerly separated the continents, known as ophiolites. The collision between the Indian subcontinent and what is now Tibet began in the Eocene. It involved and still involves north-south convergence throughout southern Tibet and the Himalayas. This youthful mountain area is the type example for studies of continental collision processes. The Himalayas Location The Himalayas form a nearly 3000 km long, 250-350 km wide range between India to the south and the huge Tibetan plateau, with a mean elevation of 5000 m, to the north. The Himalayan mountain belt has a relatively simple, arcuate, and cylindrical geometry over most of its length and terminates at both ends in nearly transverse syntaxes, i.e. areas where orogenic structures turn sharply about a vertical axis. Both syntaxes are named after the main peaks that tower above them, the Namche Barwa (7756 m) to the east and the Nanga Parbat (8138 m) to the west, in Pakistan. -
REGIONAL GEOGRAPHY of AFRICA. Uganda Certificate of Education
REGIONAL GEOGRAPHY OF AFRICA. Uganda Certificate of Education. GEOGRAPHY Code: 273/2, Paper 2 2 hours 30 minutes PART I : THE REST OF AFRICA. INSTRUCTIONS TO CANDIDATES: This paper consists of two sections: Part I Rest of Africa. Answer two questions from part I @ question carry 25marks. Any additional question (s) answered will not be marked. Four questions are set and a candidate is required to answer only two questions. This region covers 50% of paper 273/2. 1) Download and print out a hard copy then copy this notes in a fresh book for Rest of Africa paper2. 2) If You need a copy of this work organized by the teacher for Rest of Africa. Call 0775 534057 for a book of Africa and it will be delivered. Emihen – Utec 1 SIZE, SHAPE AND POSITION. POSITION OF AFRICA. Africa is one of the largest continents of the world. It’s the second to the largest landmass combined of Eurasia i.e. Europe and Asia continents. LOCATION: Africa lies between latitudes 37.51’N just West of Cape Blanc in Tunisia to Cape Aghulhas at Latitude 34.51’S a distance of 8,000kms. Africa also lies between Cape Ras Hagun 51.50’E and Cape Verde 17.32’W. SIZE: Africa covers land area of about 30,300,300km2. THE SHAPE: Africa’s shape is unbalanced; with her northern part being bulky and wide, while the southern part being thinner and narrower in appearance. Emihen-Utec 2 The Latitude EQUATOR divides the continent into TWO HALVES, there being approximately; 3800kms between the Cape Agulhas in the south and Equator while between Tunisia and Equator in the North is 4,100kms. -
Late Paleozoic and Mesozoic Evolution of the Lhasa Terrane in the Xainza MARK Area of Southern Tibet
Tectonophysics 721 (2017) 415–434 Contents lists available at ScienceDirect Tectonophysics journal homepage: www.elsevier.com/locate/tecto Late Paleozoic and Mesozoic evolution of the Lhasa Terrane in the Xainza MARK area of southern Tibet ⁎ Suoya Fana,b, , Lin Dinga, Michael A. Murphyb, Wei Yaoa, An Yinc a Key Laboratory of Continental Collision and Plateau Uplift, Institute of Tibetan Plateau Research, Chinese Academy of Sciences, Beijing 100101, China b Department of Earth and Atmospheric Sciences, University of Houston, Houston, TX 77204, USA c Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA 90095-1567, USA ARTICLE INFO ABSTRACT Keywords: Models for the Mesozoic growth of the Tibetan plateau describe closure of the Bangong Ocean resulting in Lhasa terrane accretion of the Lhasa terrane to the Qiangtang terrane along the Bangong-Nuijiang suture zone (BNSZ). Shortening However, a more complex history is suggested by studies of ophiolitic melanges south of the BNSZ “within” the Foreland basin Lhasa terrane. One such mélange belt is the Shiquanhe-Namu Co mélange zone (SNMZ) that is coincident with Suture zone the Geren Co-Namu Co thrust (GNT). To better understand the structure, age, and provenance of rocks exposed Provenance along the SNMZ we conducted geologic mapping, sandstone petrography, and U-Pb zircon geochronology of Geochronology rocks straddling the SNMZ. The GNT is north-directed and places Paleozoic strata against the Yongzhu ophiolite and Cretaceous strata along strike. A gabbro in the Yongzhu ophiolite yielded a U-Pb zircon age of 153 Ma. Detrital zircon age data from Permian rocks in the hanging wall suggests that the Lhasa terrane has affinity with the Himalaya and Qiangtang, rather than northwest Australia. -
The Plate Tectonics of Cenozoic SE Asia and the Distribution of Land and Sea
Cenozoic plate tectonics of SE Asia 99 The plate tectonics of Cenozoic SE Asia and the distribution of land and sea Robert Hall SE Asia Research Group, Department of Geology, Royal Holloway University of London, Egham, Surrey TW20 0EX, UK Email: robert*hall@gl*rhbnc*ac*uk Key words: SE Asia, SW Pacific, plate tectonics, Cenozoic Abstract Introduction A plate tectonic model for the development of SE Asia and For the geologist, SE Asia is one of the most the SW Pacific during the Cenozoic is based on palaeomag- intriguing areas of the Earth$ The mountains of netic data, spreading histories of marginal basins deduced the Alpine-Himalayan belt turn southwards into from ocean floor magnetic anomalies, and interpretation of geological data from the region There are three important Indochina and terminate in a region of continen- periods in regional development: at about 45 Ma, 25 Ma and tal archipelagos, island arcs and small ocean ba- 5 Ma At these times plate boundaries and motions changed, sins$ To the south, west and east the region is probably as a result of major collision events surrounded by island arcs where lithosphere of In the Eocene the collision of India with Asia caused an the Indian and Pacific oceans is being influx of Gondwana plants and animals into Asia Mountain building resulting from the collision led to major changes in subducted at high rates, accompanied by in- habitats, climate, and drainage systems, and promoted dis- tense seismicity and spectacular volcanic activ- persal from Gondwana via India into SE Asia as well -
Lhasa Terrane in Southern Tibet Came from Australia
Lhasa terrane in southern Tibet came from Australia Di-Cheng Zhu1*, Zhi-Dan Zhao1, Yaoling Niu1,2,3, Yildirim Dilek4, and Xuan-Xue Mo1 1State Key Laboratory of Geological Processes and Mineral Resources, and School of Earth Science and Resources, China University of Geosciences, Beijing 100083, China 2School of Earth Sciences, Lanzhou University, Lanzhou 730000, China 3Department of Earth Sciences, Durham University, Durham DH1 3LE, UK 4Department of Geology, Miami University, Oxford, Ohio 45056, USA ABSTRACT REGIONAL GEOLOGY AND DETRITAL The U-Pb age and Hf isotope data on detrital zircons from Paleozoic metasedimentary rocks ZIRCON ANALYSES ε in the Lhasa terrane (Tibet) defi ne a distinctive age population of ca. 1170 Ma with Hf(t) values The Lhasa terrane is one of the three large identical to the coeval detrital zircons from Western Australia, but those from the western east-west−trending tectonic belts in the Tibetan Qiangtang and Tethyan Himalaya terranes defi ne an age population of ca. 950 Ma with a similar Plateau. It is located between the Qiangtang ε Hf(t) range. The ca. 1170 Ma detrital zircons in the Lhasa terrane were most likely derived from and Tethyan Himalayan terranes, bounded by the Albany-Fraser belt in southwest Australia, whereas the ca. 950 Ma detrital zircons from both the Bangong-Nujiang suture zone to the north the western Qiangtang and Tethyan Himalaya terranes might have been sourced from the High and the Indus–Yarlung Zangbo suture zone to Himalaya to the south. Such detrital zircon connections enable us to propose that the Lhasa the south, respectively (Fig. -
Classic Localities Explained: the Eastern French Pyrenees – from Mountain Belt to Foreland Basin
The eastern French Pyrenees: from mountain belt to foreland basin Item Type Article Authors Satterfield, Dorothy; Rollinson, Hugh; Suthren, Roger Citation Satterfield, D., Rollinson, H., and Suthren, R. (2019). 'The eastern French Pyrenees: from mountain belt to foreland basin'. Geology Today: Localities explained 23, pp. 1-34. DOI 10.1111/gto.12291 Publisher Wiley Journal Geology Today Download date 28/09/2021 21:45:49 Item License http://onlinelibrary.wiley.com/termsAndConditions#vor Link to Item http://hdl.handle.net/10545/624573 Satterfield et al. – Classic Localities – French Pyrenees Classic localities explained: The Eastern French Pyrenees – from Mountain Belt to Foreland Basin Dorothy Satterfield, Hugh Rollinson and Roger Suthren Environmental Science, University of Derby, Kedleston Road, Derby, UK. DE22 1GB [email protected] Abstract The Pyrenees are a young mountain belt formed as part of the larger Alpine collision zone. This excursion explores the development of the Pyrenean Mountain Belt in southern France, from its early extensional phase in the mid-Cretaceous and subsequent collisional phase, through its uplift and erosion in the Late Cretaceous and again in the Eocene, which led to the development of the Aquitaine-Languedoc foreland basin. One of the complexities of the Pyrenean Belt is that thrusting, uplift and erosion during the Pyrenean orogeny exposed older Variscan basement rocks in the central core of the mountains, rocks which were metamorphosed during an earlier event in the late Carboniferous. Thus, this orogenic belt also tells the story of an earlier collision between Laurussia in the north and Gondwana in the south at ca 300 Ma, prior to the onset of the Pyrenean events at ca.