Ridge Subduction, and Feedback Controls on the Andean Margin Developmentat the Chile Triple Junction Area (45-48Øs)
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Cenozoic Changes in Pacific Absolute Plate Motion A
CENOZOIC CHANGES IN PACIFIC ABSOLUTE PLATE MOTION A THESIS SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI`I IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF SCIENCE IN GEOLOGY AND GEOPHYSICS DECEMBER 2003 By Nile Akel Kevis Sterling Thesis Committee: Paul Wessel, Chairperson Loren Kroenke Fred Duennebier We certify that we have read this thesis and that, in our opinion, it is satisfactory in scope and quality as a thesis for the degree of Master of Science in Geology and Geophysics. THESIS COMMITTEE Chairperson ii Abstract Using the polygonal finite rotation method (PFRM) in conjunction with the hotspot- ting technique, a model of Pacific absolute plate motion (APM) from 65 Ma to the present has been created. This model is based primarily on the Hawaiian-Emperor and Louisville hotspot trails but also incorporates the Cobb, Bowie, Kodiak, Foundation, Caroline, Mar- quesas and Pitcairn hotspot trails. Using this model, distinct changes in Pacific APM have been identified at 48, 27, 23, 18, 12 and 6 Ma. These changes are reflected as kinks in the linear trends of Pacific hotspot trails. The sense of motion and timing of a number of circum-Pacific tectonic events appear to be correlated with these changes in Pacific APM. With the model and discussion presented here it is suggested that Pacific hotpots are fixed with respect to one another and with respect to the mantle. If they are moving as some paleomagnetic results suggest, they must be moving coherently in response to large-scale mantle flow. iii List of Tables 4.1 Initial hotspot locations . -
Geodetic Determination of Relative Plate Motion and Crustal Deformation Across the Scotia-South America Plate Boundary in Eastern Tierra Del Fuego
Article Geochemistry 3 Volume 4, Number 9 Geophysics 19 September 2003 1070, doi:10.1029/2002GC000446 GeosystemsG G ISSN: 1525-2027 AN ELECTRONIC JOURNAL OF THE EARTH SCIENCES Published by AGU and the Geochemical Society Geodetic determination of relative plate motion and crustal deformation across the Scotia-South America plate boundary in eastern Tierra del Fuego R. Smalley, Jr. Center for Earthquake Research and Information, University of Memphis, 3876 Central Avenue, Ste. 1, Memphis, Tennessee 38152, USA ([email protected]) E. Kendrick and M. G. Bevis School of Ocean, Earth and Space Technology, University of Hawaii, 1680 East West Road, Honolulu, Hawaii 96822, USA ([email protected]; [email protected]) I. W. D. Dalziel and F. Taylor Institute of Geophysics, Jackson School of Geosciences, University of Texas at Austin, 4412 Spicewood Springs Road, Building 600, Austin, Texas 78759, USA ([email protected]; [email protected]) E. Laurı´a Instituto Geogra´fico Militar de Argentina, Cabildo 381, 1426 Buenos Aires, Argentina ([email protected]) R. Barriga Instituto Geogra´fico Militar de Chile, Nueva Santa Isabel 1640, Santiago, Chile ([email protected]) G. Casassa Centro de Estudios Cientı´ficos, Avda. Arturo Prat 514, Casilla 1469, Valdivia, Chile ([email protected]) E. Olivero and E. Piana Centro Austral de Investigaciones Cientı´ficas, Av. Malvinas Argentinas s/n, Caja de Correo 92, 9410 Ushuaia, Tierra del Fuego, Argentina ([email protected]; [email protected]) [1] Global Positioning System (GPS) measurements provide the first direct measurement of plate motion and crustal deformation across the Scotia-South America transform plate boundary in Tierra del Fuego. -
Chapter 4 Tectonic Reconstructions of the Southernmost Andes and the Scotia Sea During the Opening of the Drake Passage
123 Chapter 4 Tectonic reconstructions of the Southernmost Andes and the Scotia Sea during the opening of the Drake Passage Graeme Eagles Alfred Wegener Institute, Helmholtz Centre for Marine and Polar Research, Bre- merhaven, Germany e-mail: [email protected] Abstract Study of the tectonic development of the Scotia Sea region started with basic lithological and structural studies of outcrop geology in Tierra del Fuego and the Antarctic Peninsula. To 19th and early 20th cen- tury geologists, the results of these studies suggested the presence of a submerged orocline running around the margins of the Scotia Sea. Subse- quent increases in detailed knowledge about the fragmentary outcrop ge- ology from islands distributed around the margins of the Scotia Sea, and later their interpretation in light of the plate tectonic paradigm, led to large modifications in the hypothesis such that by the present day the concept of oroclinal bending in the region persists only in vestigial form. Of the early comparative lithostratigraphic work in the region, only the likenesses be- tween Jurassic—Cretaceous basin floor and fill sequences in South Geor- gia and Tierra del Fuego are regarded as strong enough to be useful in plate kinematic reconstruction by permitting the interpretation of those re- gions’ contiguity in mid-Mesozoic times. Marine and satellite geophysical data sets reveal features of the remaining, submerged, 98% of the Scotia 124 Sea region between the outcrops. These data enable a more detailed and quantitative approach to the region’s plate kinematics. In contrast to long- used interpretations of the outcrop geology, these data do not prescribe the proximity of South Georgia to Tierra del Fuego in any past period. -
Earth's Tectonic Plates
Copyright © Glencoe/McGraw-Hill, a division of the McGraw-Hill Companies, Inc. Teaching TransparencyTeaching Master49 Transparency Tectonic Plates Earth’s MASTER 49 5.4 North American 1.8 Eurasian Plate Juan Plate 2.3 Divergent 3.7 de Fuca 5.4 boundary Plate Caribbean Philippine Convergent Plate 2.3 Arabian Plate boundary Cocos Plate 9.2 Plate 2.5 Pacific Plate Ridge axis 10.0 3.0 2.0 Transform African Plate 2.0 17.2 6.0 Earth theEnvironment, andtheUniverse Science:Geology, 10.5 boundary Nazca South American 6.2 Plate Plate Subduction zone TEACHING TRANSPARENCY Indian-Australian Plate 7.1 11.1 16.8 1.7 Zones of extension 4.1 within continents 10.3 6.0 1.3 7.3 3.7 3.3 Uncertain plate 7.7 7.5 7.2 boundary Antarctic Plate 5.0 Rate of movement 5.7 (cm/y) Use withChapter17 Section 17.3 97 Name Class Date WORKSHEET 49 TEACHING TRANSPARENCY Use with Chapter 17 Earth’s Tectonic Plates Section 17.3 1. In what direction is the Pacific Plate moving? 2. Are the Pacific Plate and the Antarctic Plate moving toward each other, away from each other, or past each other? Explain your answer. 3. What type of boundary separates the South American Plate from the Nazca Plate? Explain your answer. 4. Describe the relative motion between the North American Plate and the Pacific Plate. 5. Between which plates is the relative motion the fastest? 6. Would you predict that, over time, the distance between New York and Miami will increase, decrease, or stay the same? Explain your answer. -
Uplift of Quaternary Shorelines in Eastern Patagonia: Darwin Revisited
Uplift of Quaternary shorelines in Eastern Patagonia: Darwin revisited Kevin Pedoja, Vincent Regard, Laurent Husson, Joseph Martinod, Benjamin Guillaume, Enrique Fucks, Maximiliano Iglesias, Pierre Weill To cite this version: Kevin Pedoja, Vincent Regard, Laurent Husson, Joseph Martinod, Benjamin Guillaume, et al.. Uplift of Quaternary shorelines in Eastern Patagonia: Darwin revisited. Geomorphology, Elsevier, 2011, 127 (3-4), pp.121-142. 10.1016/j.geomorph.2010.08.003. insu-00610899 HAL Id: insu-00610899 https://hal-insu.archives-ouvertes.fr/insu-00610899 Submitted on 6 Mar 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Distributed under a Creative Commons Attribution| 4.0 International License Uplift of quaternary shorelines in eastern Patagonia: Darwin revisited Kevin Pedoja a,⁎, Vincent Regard b,c,d, Laurent Husson e,f, Joseph Martinod b,c,d, Benjamin Guillaume g, Enrique Fucks h, Maximiliano Iglesias i, Pierre Weill a a Laboratoire de Morphodynamique Continentale et Côtière, CNRS, Université de Caen, 14000 Caen, France b Université de Toulouse ; UPS (OMP) ; LMTG ; 14 Av Edouard Belin, F-31400 Toulouse, France c IRD ; LMTG ; F-31400 Toulouse, France d CNRS ; LMTG ; F-31400 Toulouse, France e CNRS UMR 6118, Géosciences Rennes, 35042 Rennes, France f CNRS UMR 6112, Laboratoire de Planétologie et Géodynamique de Nantes, France g Dip. -
West Antarctica: Tectonics and Paleogeography
Chapter 2 West Antarctica: Tectonics and Paleogeography The origin of West Antarctica (WANT) can be traced back to the Terra Australis orogenesis that began between 520 Ma and 510 Ma—shortly after the terminal suturing of Gondwana (Boger 2011). The onset of this event was responsible for the termination of passive margin sedimentation along much of the Pacific margin of Gondwana and marks the beginning of widespread and broadly coeval deforma- tion and arc-type plutonism. It also began a long-lived process of accretion that added much of the crust that defines eastern Australia, West Antarctica (domain 5 of Boger 2011, Fig. 2.1), and western South America (Cawood 2005, 2009). Post-Gondwana accretionary growth—the Terra Australis and Gondwanide Orogenies—The suturing of the West Gondwana and Australo–Antarctic plates along the Kuunga Orogen brought to an end the long-lived process of convergence between the pre-collision components of Gondwana. The result was a reconfigura- tion of the early to middle Cambrian plate system and the consequent transfer of ocean floor consumption from between the pre-Gondwana cratons to the outboard Pacific margin of newly formed Gondwana supercontinent (Cawood2005 ). This led to the establishment of the accretionary Terra Austrais Orogen (Cawood 2005), a general name given to the orogenic belt that stretched continuously from north- ern South America to northern Australia and which began in the early to middle Cambrian and lasted until the late Carboniferous. In Antarctica Terra Australis (Ross) orogenesis also deformed and variably metamorphosed the pre-Gondwana passive margin (Fig. 2.2). The Gondwana supercontinent underwent a sequential fragmentation over approximately 165 Ma. -
Crustal Faults in the Chilean Andes: Geological Constraints and Seismic Potential
Andean Geology 46 (1): 32-65. January, 2019 Andean Geology doi: 10.5027/andgeoV46n1-3067 www.andeangeology.cl Crustal faults in the Chilean Andes: geological constraints and seismic potential *Isabel Santibáñez1, José Cembrano2, Tiaren García-Pérez1, Carlos Costa3, Gonzalo Yáñez2, Carlos Marquardt4, Gloria Arancibia2, Gabriel González5 1 Programa de Doctorado en Ciencias de la Ingeniería, Pontificia Universidad Católica de Chile, Avda. Vicuña Mackenna 4860, Macul, Santiago, Chile. [email protected]; [email protected] 2 Departamento de Ingeniería Estructural y Geotécnica, Pontificia Universidad Católica de Chile, Avda. Vicuña Mackenna 4860, Macul, Santiago, Chile. [email protected]; [email protected]; [email protected] 3 Departamento de Geología, Universidad de San Luis, Ejercito de Los Andes 950, D5700HHW San Luis, Argentina. [email protected] 4 Departamento de Ingeniería Estructural y Geotécnica y Departamento de Ingeniería de Minería, Pontificia Universidad Católica de Chile. Avda. Vicuña Mackenna 4860, Macul, Santiago, Chile. [email protected] 5 Departamento de Ciencias Geológicas, Universidad Católica del Norte, Angamos 0610, Antofagasta, Chile. [email protected] * Corresponding author: [email protected] ABSTRACT. The Chilean Andes, as a characteristic tectonic and geomorphological region, is a perfect location to unravel the geologic nature of seismic hazards. The Chilean segment of the Nazca-South American subduction zone has experienced mega-earthquakes with Moment Magnitudes (Mw) >8.5 (e.g., Mw 9.5 Valdivia, 1960; Mw 8.8 Maule, 2010) and many large earthquakes with Mw >7.5, both with recurrence times of tens to hundreds of years. By contrast, crustal faults within the overriding South American plate commonly have longer recurrence times (thousands of years) and are known to produce earthquakes with maximum Mw of 7.0 to 7.5. -
19. Analysis and Correlation of Volcanic
Jørgensen, B.B., D’Hondt, S.L., and Miller, D.J. (Eds.) Proceedings of the Ocean Drilling Program, Scientific Results Volume 201 19. ANALYSIS AND CORRELATION OF VOLCANIC ASH IN MARINE SEDIMENTS FROM THE PERU MARGIN, OCEAN DRILLING PROGRAM LEG 201: EXPLOSIVE VOLCANIC 1 CYCLES OF THE NORTH-CENTRAL ANDES D. Hart2 and D.J. Miller3 ABSTRACT Although land studies have identified major volcanic centers of his- 1Hart, D., and Miller, D.J., 2006. toric eruptions within the Central Andes, the tephrachronologic record Analysis and correlation of volcanic is disturbed by the high erosion rates in this arid region. Owing to ero- ash in marine sediments from the Peru sion, studies of volcanic cyclicity based on subaerial deposits offer an margin, Ocean Drilling Program Leg incomplete record of the frequency and episodicity of eruptions since 201: explosive volcanic cycles of the north-central Andes. In Jørgensen, the Miocene. However, volcanic material commonly occurs in marine B.B., D’Hondt, S.L., and Miller, D.J. sediment as discrete ash fall layers and/or disseminated ash accumula- (Eds.), Proc. ODP, Sci. Results, 201, 1–43 tions. A detailed investigation of cores from three sites offshore Peru [Online]. Available from World Wide drilled during Ocean Drilling Program (ODP) Leg 201 has been con- Web: <http://www-odp.tamu.edu/ ducted to determine the occurrence of volcanic ash layers and ash accu- publications/201_SR/VOLUME/ CHAPTERS/122.PDF>. [Cited YYYY- mulations within marine sediments along the Peru shelf. These sites MM-DD] were previously occupied during ODP Leg 112, which suffered from 2Department of Geology and poor and/or disturbed core recovery. -
1028-2 Holocene Sediments from the Southern Chile Trench a Record Of
Journal of the Geological Society Holocene sediments from the Southern Chile Trench: a record of active margin magmatism, tectonics and palaeoseismicity Bianca Heberer, Georg Röser, Jan H. Behrmann, Meinert Rahn and Achim Kopf Journal of the Geological Society 2010; v. 167; p. 539-553 doi:10.1144/0016-76492009-015 Email alerting click here to receive free email alerts when new articles cite this article service Permission click here to seek permission to re-use all or part of this article request Subscribe click here to subscribe to Journal of the Geological Society or the Lyell Collection Notes Downloaded by National Centre University on 10 May 2010 © 2010 Geological Society of London Journal of the Geological Society, London, Vol. 167, 2010, pp. 539–553. doi: 10.1144/0016-76492009-015. Holocene sediments from the Southern Chile Trench: a record of active margin magmatism, tectonics and palaeoseismicity BIANCA HEBERER1*, GEORG RO¨ SER2, JAN H. BEHRMANN3, MEINERT RAHN4 &ACHIMKOPF5 1Department of Geography and Geology, University of Salzburg, Hellbrunner Strasse 34, 5020 Salzburg, Austria 2Anders Estenstads Veg 22, 7046 Trondheim, Norway 3IFM-GEOMAR, Wischofstrasse 1–3, 24148 Kiel, Germany 4ENSI, 5232 Villigen-ENSI, Switzerland 5RCOM, Universita¨t Bremen, Leobener Strasse, 28539 Bremen, Germany *Corresponding author (e-mail: [email protected]) Abstract: Sedimentology, petrography and the provenance of Holocene sediments from the Southern Chile Trench (36–478S) were investigated in an integrated approach combining description of a collection of gravity cores, measurements of physical properties, quantitative X-ray petrography and modal analysis. The sediments studied were trench hemipelagic sediments, fan deposits, and more distal hemipelagic sediments from the Nazca Plate. -
LA-ICPMS U–Pb Igneous and Detrital Zircon Ages from the Chile Triple Junction and the Taitao Peninsula, Chilean Patagonia
Geochemical Journal, Vol. 47, pp. 149 to 165, 2013 Shallow-depth melt eduction due to ridge subduction: LA-ICPMS U–Pb igneous and detrital zircon ages from the Chile Triple Junction and the Taitao Peninsula, Chilean Patagonia RYO ANMA1* and YUJI ORIHASHI2 1Faculty of Life and Environmental Sciences, University of Tsukuba, Ten-nodai 1-1-1, Tsukuba, Ibaraki 305-8572, Japan 2Earthquake Research Institute, The University of Tokyo, Yayoi 1-1-1, Bunkyo-ku, Tokyo 113-0032, Japan (Received April 25, 2012; Accepted January 26, 2013) To understand the processes of melt eduction in a ridge subduction zone, we performed U–Pb dating on zircons sepa- rated from igneous and sedimentary rocks that were newly dredged from the Chile Triple Junction area and from volcanic rocks collected from the Taitao peninsula, southern Chile. The youngest fraction of the U–Pb age population was used to estimate the age of magmatism or sedimentation. Our new results indicate that the fore-arc region became volcanically active over a period of ~0.4 m.y., after obduction of the Taitao ophiolite (~5.7 to 5.2 Ma) from the west and after granite intrusions related to ridge subduction at ~6 Ma. Fore-arc volcanism produced ejecta of basaltic to dacitic compositions and migrated from offshore (~5.3 Ma) to inland (~4.6 Ma) along the Chile Margin Unit that trends northeast–southwest. The volcanism further extended east to produce the dacitic volcanic plug of Pan de Azucar (~4.3 Ma) and lavas in Fjord San Pedro (~2.9 Ma). The migration took place at a rate of ~2.3 cm/y to ~5.3 cm/y. -
Miocene to Late Quaternary Patagonian Basalts (46–478S): Geochronometric and Geochemical Evidence for Slab Tearing Due to Active Spreading Ridge Subduction
Journal of Volcanology and Geothermal Research 149 (2006) 346–370 www.elsevier.com/locate/jvolgeores Miocene to Late Quaternary Patagonian basalts (46–478S): Geochronometric and geochemical evidence for slab tearing due to active spreading ridge subduction Christe`le Guivel a,*, Diego Morata b, Ewan Pelleter c,d, Felipe Espinoza b, Rene´ C. Maury c, Yves Lagabrielle e, Mireille Polve´ f,g, Herve´ Bellon c, Joseph Cotten c, Mathieu Benoit c, Manuel Sua´rez h, Rita de la Cruz h a UMR 6112 bPlane´tologie et Ge´odynamiqueQ, Universite´ de Nantes, 2 rue de la Houssinie`re, 44322 Nantes, France b Departamento de Geologı´a. Fac. Cs. Fı´sicas y Matema´ticas, Universidad de Chile, Plaza Ercilla 803, Santiago, Chile c UMR 6538 bDomaines oce´aniquesQ, UBO-IUEM, place Nicolas-Copernic, 29280 Plouzane´, France d CRPG-CNRS UPR A2300, BP 20, 54501 Vandoeuvre-les-Nancy, France e UMR 5573, Dynamique de la Lithosphe`re, Place E. Bataillon, case 60, 34095, Montpellier Cedex 5, France f LMTG-OMP, 14 Avenue E. Belin, 31400 Toulouse, France g IRD-Departamento de Geologia de la Universidad de Chile, Chile h Servicio Nacional de Geologı´a y Minerı´a, Avda. Santa Marı´a 0104, Santiago, Chile Received 18 May 2005; received in revised form 29 August 2005; accepted 14 September 2005 Abstract Miocene to Quaternary large basaltic plateaus occur in the back-arc domain of the Andean chain in Patagonia. They are thought to result from the ascent of subslab asthenospheric magmas through slab windows generated from subducted segments of the South Chile Ridge (SCR). We have investigated three volcanic centres from the Lago General Carrera–Buenos Aires area (46–478S) located above the inferred position of the slab window corresponding to a segment subducted 6 Ma ago. -
Paper Is Divided Into Two Parts
Earth-Science Reviews 140 (2015) 72–107 Contents lists available at ScienceDirect Earth-Science Reviews journal homepage: www.elsevier.com/locate/earscirev Geologic and kinematic constraints on Late Cretaceous to mid Eocene plate boundaries in the southwest Pacific Kara J. Matthews a,⁎, Simon E. Williams a, Joanne M. Whittaker b,R.DietmarMüllera, Maria Seton a, Geoffrey L. Clarke a a EarthByte Group, School of Geosciences, The University of Sydney, NSW 2006, Australia b Institute for Marine and Antarctic Studies, University of Tasmania, TAS 7001, Australia article info abstract Article history: Starkly contrasting tectonic reconstructions have been proposed for the Late Cretaceous to mid Eocene (~85– Received 25 November 2013 45 Ma) evolution of the southwest Pacific, reflecting sparse and ambiguous data. Furthermore, uncertainty in Accepted 30 October 2014 the timing of and motion at plate boundaries in the region has led to controversy around how to implement a Available online 7 November 2014 robust southwest Pacific plate circuit. It is agreed that the southwest Pacific comprised three spreading ridges during this time: in the Southeast Indian Ocean, Tasman Sea and Amundsen Sea. However, one and possibly Keywords: two other plate boundaries also accommodated relative plate motions: in the West Antarctic Rift System Southwest Pacific fi Lord Howe Rise (WARS) and between the Lord Howe Rise (LHR) and Paci c. Relevant geologic and kinematic data from the South Loyalty Basin region are reviewed to better constrain its plate motion history during this period, and determine the time- Late Cretaceous dependent evolution of the southwest Pacific regional plate circuit. A model of (1) west-dipping subduction Subduction and basin opening to the east of the LHR from 85–55 Ma, and (2) initiation of northeast-dipping subduction Plate circuit and basin closure east of New Caledonia at ~55 Ma is supported.