The Proto-Andean Margin of Gondwana: an Introduction
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Kinematic Reconstruction of the Caribbean Region Since the Early Jurassic
Earth-Science Reviews 138 (2014) 102–136 Contents lists available at ScienceDirect Earth-Science Reviews journal homepage: www.elsevier.com/locate/earscirev Kinematic reconstruction of the Caribbean region since the Early Jurassic Lydian M. Boschman a,⁎, Douwe J.J. van Hinsbergen a, Trond H. Torsvik b,c,d, Wim Spakman a,b, James L. Pindell e,f a Department of Earth Sciences, Utrecht University, Budapestlaan 4, 3584 CD Utrecht, The Netherlands b Center for Earth Evolution and Dynamics (CEED), University of Oslo, Sem Sælands vei 24, NO-0316 Oslo, Norway c Center for Geodynamics, Geological Survey of Norway (NGU), Leiv Eirikssons vei 39, 7491 Trondheim, Norway d School of Geosciences, University of the Witwatersrand, WITS 2050 Johannesburg, South Africa e Tectonic Analysis Ltd., Chestnut House, Duncton, West Sussex, GU28 OLH, England, UK f School of Earth and Ocean Sciences, Cardiff University, Park Place, Cardiff CF10 3YE, UK article info abstract Article history: The Caribbean oceanic crust was formed west of the North and South American continents, probably from Late Received 4 December 2013 Jurassic through Early Cretaceous time. Its subsequent evolution has resulted from a complex tectonic history Accepted 9 August 2014 governed by the interplay of the North American, South American and (Paleo-)Pacific plates. During its entire Available online 23 August 2014 tectonic evolution, the Caribbean plate was largely surrounded by subduction and transform boundaries, and the oceanic crust has been overlain by the Caribbean Large Igneous Province (CLIP) since ~90 Ma. The consequent Keywords: absence of passive margins and measurable marine magnetic anomalies hampers a quantitative integration into GPlates Apparent Polar Wander Path the global circuit of plate motions. -
A Dangling Slab, Amplified Arc Volcanism, Mantle Flow and Seismic Anisotropy in the Kamchatka Plate Corner
AGU Geodynamics Series Volume 30, PLATE BOUNDARY ZONES Edited by Seth Stein and Jeffrey T. Freymueller, p. 295-324 1 A Dangling Slab, Amplified Arc Volcanism, Mantle Flow and Seismic Anisotropy in the Kamchatka Plate Corner Jeffrey Park,1 Yadim Levin,1 Mark Brandon,1 Jonathan Lees,2 Valerie Peyton,3 Evgenii Gordeev ) 4 Alexei Ozerov ,4 Book chapter in press with "Plate Boundary Zones," edited by Seth Stein and Jeffrey Freymuller Abstract The Kamchatka peninsula in Russian East Asia lies at the junction of a transcurrent plate boundary, aligned with the western Aleutian Islands, and a steeply-dipping subduction zone with near-normal convergence. Seismicity patterns and P-wave tomography argue that subducting Pacific lithosphere terminates at the Aleutian junction, and that the downdip extension (>150km depth) of the slab edge is missing. Seismic observables of elastic anisotropy (SKS splitting and Love-Rayleigh scattering) are consistent \Vith asthenospheric strain that rotates from trench-parallel beneath the descending slab to trench-normal beyond its edge. Present-day arc volcanism is concentrated near the slab edge, in the Klyuchevskoy and Sheveluch eruptive centers. Loss of the downdip slab edge, whether from thermo-convective or ductile instability, and subsequent "slab-window" mantle return flow is indicated by widespread Quaternary volcanism in the Sredinny Range inland of Klyuchevskoy and Sheveluch, as well as the inferred Quaternary uplift of the central Kamchatka depression. The slab beneath Klyuchevskoy has shallower dip (35°) than the subduction zone farther south (55°) suggesting a transient lofting of the slab edge, either from asthenospheric flow or the loss of downdip load. -
Redalyc.Sr, C and O Isotope Composition of Marbles from The
Geologica Acta: an international earth science journal ISSN: 1695-6133 [email protected] Universitat de Barcelona España Murra, J.A.; Baldo, E.G.; Galindo, C.; Casquet, C.; Pankhurst, R.J.; Rapela, C.W.; Dahlquist, J. Sr, C and O isotope composition of marbles from the Sierra de Ancasti, Eastern Sierras Pampeanas, Argentina: age and constraints for the Neoproterozoic-Lower Paleozoic evolution of the proto- Gondwana margin Geologica Acta: an international earth science journal, vol. 9, núm. 1, marzo, 2011, pp. 79-92 Universitat de Barcelona Barcelona, España Available in: http://www.redalyc.org/articulo.oa?id=50522124008 How to cite Complete issue Scientific Information System More information about this article Network of Scientific Journals from Latin America, the Caribbean, Spain and Portugal Journal's homepage in redalyc.org Non-profit academic project, developed under the open access initiative Geologica Acta, Vol.9, Nº 1, March 2011, 79-92 DOI: 10.1344/105.000001645 Available online at www.geologica-acta.com Sr, C and O isotope composition of marbles from the Sierra de Ancasti, Eastern Sierras Pampeanas, Argentina: age and constraints for the Neoproterozoic–Lower Paleozoic evolution of the proto-Gondwana margin 1 1 2 2 3 4 1 J.A. MURRA E.G. BALDO C. GALINDO C. CASQUET R.J. PANKHURST C.W. RAPELA J. DAHLQUIST 1 CICTERRA (Universidad Nacional de Córdoba - Conicet) Av. Vélez Sarsfield 1611, 5016 Córdoba, Argentina. Murra E-mail: [email protected] Baldo E-mail: [email protected] Dahlquist E-mail: [email protected] 2 Departamento. Petrología y Geoquímica Facultad de Ciencias Geológicas, Inst. -
Arc Dacite Genesis Pathways: Evidence from Mafic Enclaves and Their Hosts in Aegean Lavas ⁎ G.F
Lithos 95 (2007) 346–362 www.elsevier.com/locate/lithos Arc dacite genesis pathways: Evidence from mafic enclaves and their hosts in Aegean lavas ⁎ G.F. Zellmer a,b, , S.P. Turner c a Institute of Earth Sciences, Academia Sinica, 128 Academia Road, Section 2, Nankang, Taipei 11529, Taiwan, ROC b Lamont-Doherty Earth Observatory, 61 Route 9W, Palisades, New York 10964, USA c GEMOC, Department of Earth and Planetary Sciences, Macquarie University, Sydney, NSW 2109, Australia Received 4 January 2006; accepted 17 August 2006 Available online 25 September 2006 Abstract Mafic enclaves are commonly found in intermediate arc magmas, and their occurrence has been linked to eruption triggering by pre-eruptive magma mixing processes. New major, trace, Sr–Nd and U–Th isotope data of rocks from Nisyros in the Aegean volcanic arc are presented here. Pre-caldera samples display major and trace element trends that are consistent with fractionation of magnetite and apatite within intermediate compositions, and zircon within felsic compositions, and preclude extensive hybrid- ization between mafic and felsic magmas. In contrast, post-caldera dacites form a mixing trend towards their mafic enclaves. In terms of U-series isotopes, most samples show small 238U excesses of up to ∼10%. Mafic enclaves have significantly higher U/Th ratios than their dacitic host lavas, precluding simple models that relate the mafic and felsic magmas by fractionation or aging alone. A more complicated petrogenetic scenario is required. The post-caldera dacites are interpreted to represent material remobilized from a young igneous protolith following influx of fresh mafic magma, consistent with the U–Th data and with Sr–Nd isotope constraints that point to very limited (b10%) assimilation of old crust at Nisyros. -
The Evolution of the Island Arc of Japan and the Formation of Granites in the Circum-Pacific Belt
JOURNALOF GEOMAGNETISMAND GEOELECTRICITY VOL. 23, No. 3, 4, 1971 The Evolution of the Island Arc of Japan and the Formation of Granites in the Circum-Pacific Belt Naoto KAWAI, Tadashi NAKAJIMA and Kimio HIROOKa+ Department of Material Physics, Faculty of Engineering Science, Osaka University, Osaka, Japan (Received April 27, 1971) Abstract From a palaeomagnetic study and radiometric investigation of Cretaceous intrusive rocks it was recently suggested that the Palaeozoic basin formed in the northeastern Japan was severely deformed at the end of Mesozoic era. This resulted in a narrowing and shortening of the entire length of the Japanese islands. The northeastern block moved southwestward by approximately 200km and southwestern northeastward by 150km, whereas the middle block remained relative- ly unmoved but was compressed between the two blocks. As the compressional forces increased, first the Palaeozoic sediments of the central block were uplifted, and subsequently the "median line" was formed. Along the latter line, the northern half of the southern block moved eastward relative to the southern half. A strong uniaxial stress superimposed upon a hydrostatic one oc- curred associated with the relative movement. The sediments as the results recrystallized to form the three major metamorphic belts. During and after these movements, the compressed zone in the middle of the island was push- ed to the east to form a great warp in the island. Such a simple model of a bend accompanied by a tension crack as predicted by Kawai, Ito and Kume several years ago was reconsidered. The contraction of the basin was finally related to the eastward drift of Asian continent upon the Creta- ceous Pacific sea floor. -
A New Record Ofrodinia Break-Up in the Western Sierras Pampeanas of Argentina
A-type magmatism in the sierras ofMaz and Espinal: A new record ofRodinia break-up in the Western Sierras Pampeanas of Argentina Fernando CoIomboa,,,, Edgardo G.A. BaIdoa, Cesar Casquetb, RobertJ. PankhurstC, Carmen Galindob, CarIos W. RapeIa d, Juan A. DahIquista, C. Mark Fanninge a Departamento de Geologfa - FCEFyN, Universidad NacionaI de Cordoba, Wlez Sarsfield 1611, X5016GCA Cordoba, Argentina b Departamento de Petrologfa y Geoquimica, Universidad Complutense, 28040 Madrid, Spain C British Geological Survey, Keyworth, Nottingham NG12 5GG, England, United Kingdom d Centro de Investigaciones Geologicas, Universidad Nacional de La Plata, 1900 La Plata, Argentina e Research School of Earth Sciences, The Australian National University, Canberra, Australia A BST RAC T Two orthogneisses have been recognized in the sierras of Espinal and Maz (Wes tern Sierras Pampeanas, NWArgentina) that were emplaced within a Grenvillian metasedimentary sequence. Microcline, plagio clase and quartz are the main rock-forming minerals, with accessory zircon, apatite-(CaF), magnetite, biotite (Fe/(Fe + Mg) = 0.88-0.91). ferropargasite (Fetotal/(Fetotal + Mg) = 0.88-0.89), titanite (with up to 3 1.61 wt% Y203) and an REE-rich epidote. REE-poor epidote and zoned garnet (Ca and Fe + -rich) are meta Keywords: morphic minerals, while muscovite, carbonates and chlorite are secondary phases. Texture is mylonitic. Rodinia Two representative samples are classified as granite (from Sierra de Espinal) and granodiorite/tonalite U-Pb SHRIMP dating Anorogenic magmatism (from Sierra de Maz) on the grounds of immobile trace elements. Some trace element contents are rather Mesoproterozoic high (Zr: 603 and 891 ppm, Y: 44 and 76 ppm, 10,000 x Ga/AI: 2.39-3.89) and indicate an affiliation with Western Sierras Pampeanas A-type granites (more specifically, the A2 group). -
Early Evolution of the Proto-Andean Margin of South America
Early evolution of the Proto-Andean margin of South America C. W. Rapela Centro de Investigaciones Geológicas, Universidad Nacional de La Plata, Calle 1 No. 644, 1900 La Plata, Argentina R. J. Pankhurst British Antarctic Survey, Cambridge CB30ET, United Kingdom C. Casquet Departamento de Petrología y Geoquímica, Universidad Complutense, 28040 Madrid, Spain E. Baldo J. Saavedra CSIC, Instituto de Agrobiología y Recursos Naturales, 37071 Salamanca, Spain C. Galindo Departamento de Petrología y Geoquímica, Universidad Complutense, 28040 Madrid, Spain ABSTRACT INTRODUCTION From a detailed study of a 500 km transect in the Sierras Pampeanas, central-west Argen- The evolution of the Gondwana margin pro- tina, two pre-Silurian tectono-magmatic episodes are recognized and defined, each culminating posed here is based on new geochemical, isotopic, in micro-continental collisions against the proto-Andean margin of Gondwana. The Pampean petrological, and sedimentological data from a orogeny started in Early Cambrian time with short-lived subduction, indicated by ca. 535 Ma 500 km traverse across the Eastern Sierras Pam- calc-alkaline granitoids. Following Pampean terrane collision, burial to granulite facies condi- peanas and Precordillera (Fig. 1). Pre-Silurian tions (ca. 9 kbar) generated widespread migmatites and ca. 520 Ma highly peraluminous gran- metamorphic and magmatic history is inferred ites in the Eastern Sierras Pampeanas. After brief quiescence, a second major episode, the from (1) dating by conventional U-Pb on abraded Famatinian orogeny, started with subduction ca. 490 Ma, forming a wide continental arc and zircons, U-Pb SHRIMP analyses, and whole-rock ensialic backarc basin. This heralded the approach of Laurentia to Gondwana, during which Rb-Sr and K-Ar, (2) thermo-barometry based on the Precordillera terrane separated from the southern Appalachian region, finally colliding with microprobe mineral analyses, and (3) Nd and Sr Gondwana in Silurian–Devonian time. -
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. -
Exploring Submarine Arc Volcanoes Steven Carey University of Rhode Island, [email protected]
University of Rhode Island DigitalCommons@URI Graduate School of Oceanography Faculty Graduate School of Oceanography Publications 2007 Exploring Submarine Arc Volcanoes Steven Carey University of Rhode Island, [email protected] Haraldur Sigurdsson University of Rhode Island Follow this and additional works at: https://digitalcommons.uri.edu/gsofacpubs Terms of Use All rights reserved under copyright. Citation/Publisher Attribution Carey, S., and H. Sigurdsson. 2007. Exploring submarine arc volcanoes. Oceanography 20(4):80–89, https://doi.org/10.5670/ oceanog.2007.08. Available at: https://doi.org/10.5670/oceanog.2007.08 This Article is brought to you for free and open access by the Graduate School of Oceanography at DigitalCommons@URI. It has been accepted for inclusion in Graduate School of Oceanography Faculty Publications by an authorized administrator of DigitalCommons@URI. For more information, please contact [email protected]. This article has This been published in or collective redistirbution of any portion of this article by photocopy machine, reposting, or other means is permitted only with the approval of The approval portionthe ofwith any permitted articleonly photocopy by is of machine, reposting, this means or collective or other redistirbution SP ec I A L Iss U E On Ocean E X P L O R ATIO N Oceanography , Volume 20, Number 4, a quarterly journal of The 20, Number 4, a quarterly , Volume O ceanography Society. Copyright 2007 by The 2007 by Copyright Society. ceanography Exploring O ceanography Society. All rights All reserved. Society. ceanography O Submarine Arc Volcanoes or Th e [email protected] Send Society. ceanography to: correspondence all B Y S T even C A R E Y an D H A R A LDUR SIGURD ss O N Three quarters of Earth’s volcanic activ- although a significant part of arc volca- tion of tsunamis (Latter, 1981). -
Viscous Volcanos 2016 Grades 6-8 (Earth Science)
2016 Deepwater Exploration of the Marianas Viscous Volcanoes Focus Serpentine mud volcanoes Grade Level 6-8 (Earth Science) Focus Question What are serpentine mud volcanoes and how are they different from magma volcanoes? Learning Objectives • Students will describe mud volcanoes, contrast them with magma volcanoes, and explain how these structures, the Mariana Islands, and the Mariana Trench are related to the motion of tectonic plates. Materials For each serpentine mud volcano model: q Plastic tubing, approximately 1/4” outer diameter, 1/8” inside diameter q 2-liter plastic soda bottle q Fast-setting epoxy glue q Air-cure modeling clay, approximately 500 ml q Fine sand, table salt, or finely ground coffee q Drill and drill bit to match outside diameter of plastic tubing For each sediment-derived mud volcano model: q 2-liter plastic soda bottle q Cardboard or acrylic disk, diameter slightly smaller than soda bottle diameter q Fine sand or clay q Drill and drill bits, 3/8” and 1/2” For each magma volcano model: q Modeling materials, depending upon techniques chosen (see Learning Procedure, Step 1d and Step 4. Image captions/credits on Page 2. Audio-Visual Materials q (Optional) Interactive whiteboard Teaching Time If you need assistance with this document, please contact NOAA 1 Two or three 45-minute class periods Fisheries at (808) 725-5000. www.oceanexplorer.noaa.gov Viscous Volcanos 2016 Grades 6-8 (Earth Science) Seating Arrangement Groups of two to four students Maximum Number of Students 30 Key Words Mariana Arc Serpentine Mud volcano Mariana Trench Magma volcano Tectonic plate Images from Page 1 top to bottom: This Google Earth map shows the operating area of the 2016 Deepwater Background Information Exploration of the Marianas Expedition. -
A History of Proterozoic Terranes in Southern South America: from Rodinia to Gondwana
+ MODEL GEOSCIENCE FRONTIERS -(-) (2011) 1e9 available at www.sciencedirect.com China University of Geosciences (Beijing) GEOSCIENCE FRONTIERS journal homepage: www.elsevier.com/locate/gsf REVIEW A history of Proterozoic terranes in southern South America: From Rodinia to Gondwana C. Casquet a,*, C.W. Rapela b, R.J. Pankhurst c, E.G. Baldo d, C. Galindo a, C.M. Fanning e, J.A. Dahlquist d, J. Saavedra f a Departamento de Petrologıa y Geoquımica, IGEO (Universidad Complutense, CSIC), 28040 Madrid, Spain b Centro de Investigaciones Geologicas (CONICET-UNLP), 1900 La Plata, Argentina c Visiting Research Associate, British Geological Survey, Keyworth, Nottingham NG12 5GG, United Kingdom d CICTERRA (CONICET-UNC), 5000 Cordoba, Argentina e Research School of Earth Sciences, The Australian National University, Canberra, Australia f Instituto de Agrobiologıa y Recursos Naturales CSIC, 37071 Salamanca, Spain Received 3 August 2011; accepted 8 November 2011 KEYWORDS Abstract The role played by Paleoproterozoic cratons in southern South America from the Mesopro- Paleoproterozoic; terozoic to the Early Cambrian is reconsidered here. This period involved protracted continental amal- Cratons; gamation that led to formation of the supercontinent Rodinia, followed by Neoproterozoic continental Grenvillian; break-up, with the consequent opening of Clymene and Iapetus oceans, and finally continental Neoproterozoic rifting; re-assembly as Gondwana through complex oblique collisions in the Late Neoproterozoic to Early SW Gondwana assembly Cambrian. The evidence for this is based mainly on a combination of precise U-Pb SHRMP dating and radiogenic isotope data for igneous and metamorphic rocks from a large area extending from the Rio de la Plata craton in the east to the Argentine Precordillera in the west and as far north as Arequipa in Peru. -
53. Petrologic Evolution of the Mariana Arc and Back-Arc Basin System— a Synthesis of Drilling Results in the South Philippine Sea1
53. PETROLOGIC EVOLUTION OF THE MARIANA ARC AND BACK-ARC BASIN SYSTEM— A SYNTHESIS OF DRILLING RESULTS IN THE SOUTH PHILIPPINE SEA1 James H. Natland, Deep Sea Drilling Project, Scripps Institution of Oceanography, La Jolla, California and John Tarney, Department of Geology, University of Leicester, LEI 7RH, United Kingdom ABSTRACT The results of Deep Sea Drilling Project Leg 60 pertaining to the petrologic evolution of the Mariana Trough and Mariana arc are summarized in Part I. The rocks recovered at five principal sites are exceptionally diverse, including gabbros and calc-alkalic andesites derived from the West Mariana Ridge; fresh and hydrothermally altered basalts in the Mariana Trough; and interbedded boninites and arc tholeiites in the forearc region between the modern arc and the trench. Part I outlines the stratigraphy, alteration, and petrology of these rock suites and summarizes hypotheses on their origin. Part II integrates these results with those of previous DSDP legs in the region, and with island sampling, to present a composite 40-m.y. history of the Mariana arc system. Arc volcanism began in the Eocene, probably as a result of a change to the west in the motion of the Pacific plate. A north-south-trending fracture zone was transformed into a trench-subduction complex, trapping a portion of the Pacific plate in the Philippine Sea. The crust of this basin, drilled in Hole 447 (Leg 59), has the composition of typical ocean floor basalt. The earliest Eocene arc was built up dominantly of arc tholeiite and boninitic lavas, with lesser calc-alkalic lavas, based on the results of Leg 60 drilling at Sites 458 and 459 in the forearc region; Leg 59, Site 448, on the Palau-Kyushu Ridge; and exposures on the islands of Palau, Guam, and Saipan.