A Tectonic Reconstruction of Accreted Terranes Along
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Review of the Geology and Paleontology of the Ellsworth Mountains, Antarctica
U.S. Geological Survey and The National Academies; USGS OF-2007-1047, Short Research Paper 107; doi:10.3133/of2007-1047.srp107 Review of the geology and paleontology of the Ellsworth Mountains, Antarctica G.F. Webers¹ and J.F. Splettstoesser² ¹Department of Geology, Macalester College, St. Paul, MN 55108, USA ([email protected]) ²P.O. Box 515, Waconia, MN 55387, USA ([email protected]) Abstract The geology of the Ellsworth Mountains has become known in detail only within the past 40-45 years, and the wealth of paleontologic information within the past 25 years. The mountains are an anomaly, structurally speaking, occurring at right angles to the Transantarctic Mountains, implying a crustal plate rotation to reach the present location. Paleontologic affinities with other parts of Gondwanaland are evident, with nearly 150 fossil species ranging in age from Early Cambrian to Permian, with the majority from the Heritage Range. Trilobites and mollusks comprise most of the fauna discovered and identified, including many new genera and species. A Glossopteris flora of Permian age provides a comparison with other Gondwana floras of similar age. The quartzitic rocks that form much of the Sentinel Range have been sculpted by glacial erosion into spectacular alpine topography, resulting in eight of the highest peaks in Antarctica. Citation: Webers, G.F., and J.F. Splettstoesser (2007), Review of the geology and paleontology of the Ellsworth Mountains, Antarctica, in Antarctica: A Keystone in a Changing World – Online Proceedings of the 10th ISAES, edited by A.K. Cooper and C.R. Raymond et al., USGS Open- File Report 2007-1047, Short Research Paper 107, 5 p.; doi:10.3133/of2007-1047.srp107 Introduction The Ellsworth Mountains are located in West Antarctica (Figure 1) with dimensions of approximately 350 km long and 80 km wide. -
Two Contrasting Phanerozoic Orogenic Systems Revealed by Hafnium Isotope Data William J
ARTICLES PUBLISHED ONLINE: 17 APRIL 2011 | DOI: 10.1038/NGEO1127 Two contrasting Phanerozoic orogenic systems revealed by hafnium isotope data William J. Collins1*(, Elena A. Belousova2, Anthony I. S. Kemp1 and J. Brendan Murphy3 Two fundamentally different orogenic systems have existed on Earth throughout the Phanerozoic. Circum-Pacific accretionary orogens are the external orogenic system formed around the Pacific rim, where oceanic lithosphere semicontinuously subducts beneath continental lithosphere. In contrast, the internal orogenic system is found in Europe and Asia as the collage of collisional mountain belts, formed during the collision between continental crustal fragments. External orogenic systems form at the boundary of large underlying mantle convection cells, whereas internal orogens form within one supercell. Here we present a compilation of hafnium isotope data from zircon minerals collected from orogens worldwide. We find that the range of hafnium isotope signatures for the external orogenic system narrows and trends towards more radiogenic compositions since 550 Myr ago. By contrast, the range of signatures from the internal orogenic system broadens since 550 Myr ago. We suggest that for the external system, the lower crust and lithospheric mantle beneath the overriding continent is removed during subduction and replaced by newly formed crust, which generates the radiogenic hafnium signature when remelted. For the internal orogenic system, the lower crust and lithospheric mantle is instead eventually replaced by more continental lithosphere from a collided continental fragment. Our suggested model provides a simple basis for unravelling the global geodynamic evolution of the ancient Earth. resent-day orogens of contrasting character can be reduced to which probably began by the Early Ordovician12, and the Early two types on Earth, dominantly accretionary or dominantly Paleozoic accretionary orogens in the easternmost Altaids of Pcollisional, because only the latter are associated with Wilson Asia13. -
Office of Polar Programs
DEVELOPMENT AND IMPLEMENTATION OF SURFACE TRAVERSE CAPABILITIES IN ANTARCTICA COMPREHENSIVE ENVIRONMENTAL EVALUATION DRAFT (15 January 2004) FINAL (30 August 2004) National Science Foundation 4201 Wilson Boulevard Arlington, Virginia 22230 DEVELOPMENT AND IMPLEMENTATION OF SURFACE TRAVERSE CAPABILITIES IN ANTARCTICA FINAL COMPREHENSIVE ENVIRONMENTAL EVALUATION TABLE OF CONTENTS 1.0 INTRODUCTION....................................................................................................................1-1 1.1 Purpose.......................................................................................................................................1-1 1.2 Comprehensive Environmental Evaluation (CEE) Process .......................................................1-1 1.3 Document Organization .............................................................................................................1-2 2.0 BACKGROUND OF SURFACE TRAVERSES IN ANTARCTICA..................................2-1 2.1 Introduction ................................................................................................................................2-1 2.2 Re-supply Traverses...................................................................................................................2-1 2.3 Scientific Traverses and Surface-Based Surveys .......................................................................2-5 3.0 ALTERNATIVES ....................................................................................................................3-1 -
Petrological and Geochemical Characteristics of Metamorphic and Igneous Units from the Allochthonous Madre De Dios Terrane, Southern Chile ⁎ F.A
Petrological and geochemical characteristics of metamorphic and igneous units from the allochthonous Madre de Dios Terrane, Southern Chile ⁎ F.A. Sepúlveda a, , F. Hervé a, M. Calderón a, J.P. Lacassie b,c a Departamento de Geología, Facultad de Ciencias Físicas y Matemáticas, Universidad de Chile, Casilla 13518, Correo 21, Santiago, Chile b Paleoproterozoic Mineralization Research Group, Department of Geology, University of Johannesburg, Auckland Park, Johannesburg, 2006, South Africa c SERNAGEOMIN, Av. Santa María 0104, Providencia, Santiago, Chile Abstract The Denaro Complex, part of the Madre de Dios Terrane is composed of metamorphosed pillow basalts, metahyaloclastites, banded metalliferous and radiolarian metacherts, metapelites and redeposited calcareous metasandstones. The basaltic rocks show primary textures, minerals and structures. They are foliated especially in the vicinities of thrust faults, interpreted to have developed during the accretion of the terrane to the Gondwana margin. Composition of relic primary augite and chromite crystals plots into the MORB field of tectonic discriminant diagrams, as do the analyses of whole rock geochemistry, which indicates that these rocks are akin to volcanic rocks erupted along a constructive plate margin (N- and E-type MORBs), probably in a spreading axis-centered oceanic plateau or ridge. The metamorphic assemblages of pumpellyite–actinolite facies bear witness of metamorphism in a frontal accretionary wedge at elevated P and low T conditions, probably related to the Late Triassic–Early Jurassic Chonide event, which has been recognized elsewhere in the Patagonian Andes. Keywords: Metamorphism; Terrane accretion; Pumpellyite–actinolite facies; Seamount subduction; Frontal accretion 1. Introduction The rocks which crop out at the Madre de Dios archipelago (50°–50°50'S), referred to by Hervé and Mpodozis (2005) as 1.1. -
(Ordovícico) En El Segmento Andino Central Del Orógeno Terra Australis
XII Congreso Geológico Chileno Santiago, 22-26 Noviembre, 2009 S9_011 La tectónica acrecional oclóyica (Ordovícico) en el segmento andino central del orógeno Terra Australis Astini R.A.1, Martina F.1 1Laboratorio de Análisis de Cuencas, CICTERRA-Universidad Nacional de Córdoba, Av. Velez Sarsfield 1611, 2º piso, of. 7, X5016GCA Córdoba, Argentina. [email protected] En el marco del orógeno acrecional de Terra Australis [1] se reconocen intervalos temporales con acreción de terrenos e interrupción momentánea de la subducción que afectan diferencialmente al margen protoandino y permiten reconocer segmentos con características e historias contrastadas en los Andes. Sobre la base de una revisión conceptual y bibliográfica y de nuevos estudios estratigráficos, geoquímicos e isotópicos en la región del antepaís andino central se propone un mecanismo acrecional alternativo para la etapa de orogénesis ordovícica, que es la de mayor extensión que haya afectado al margen proto-pacífico antes de la orogenia gondwánica, con que finaliza la historia acrecional paleozoica. Dentro de la etapa de orogénesis oclóyica se propone separar la colisión del terreno de Precordillera [2] en el segmento andino central entre 27°30’ y 36°30’ LS aproximadamente (~1000 km de longitud), de la acreción de un bloque alargado (sliver o ribbon terrane) de basamento mesoproterozoico de mucho mayor extensión longitudinal (superior los 2000 km) (Fig. 1) que, de alguna manera, ha sido denominado Occidentalia [3]. Este último incluiría en los Andes Centrales a los terrenos de basamento mesoproterozoico correspondientes a las Sierras Pampeanas Occidentales, ubicados al oeste del cinturón de Famatina y su continuación septentrional en la Puna Catamarqueña (afloramientos de Casadero Grande) y en los terrenos de Arequipa-Antofalla. -
Geologists of Russian Origin in Latin America
REVISTA DEL MUSEO DE LA PLATA 2018, Volumen 3, Número 2: 223-295 Geologists of Russian origin in Latin America P. Tchoumatchenco1 , A.C. Riccardi 2 , †M. Durand Delga3 , R. Alonso 4 , 7 8 M. Wiasemsky5 , D. Boltovskoy 6 , R. Charrier , E. Minina 1Geological Institute, Bulgarian Academy of Sciences Acad. G. Bonchev Str. Bl. 24, 1113 Sofia, Bulgaria, [email protected] 2Museo de La Plata, Facultad de Ciencias Naturales y Museo, Universidad Nacional de La Plata, Argentina, [email protected] 3Passed away August19, 2012 4Universidad Nacional de Salta, Argentina, [email protected] 581, Chemin du Plan de Charlet, F-74190 Passy, France, [email protected] 6Dep. Ecologia, Genetica y Evolucion, Fac. Ciencias Exactas y Naturales, Univ. de Buenos Aires, Argentina, [email protected] 7History of Geology Group, Sociedad Geológica de Chile, Santiago de Chile, [email protected] 8State Geological Museum “V.I.Vernadsky”, Mohovaya ul. 11/11, Moscow 125009, Russian Federation, [email protected] REVISTA DEL MUSEO DE LA PLATA / 2018, Volumen 3, Número 2: 223-295 / ISSN 2545-6377 ISSN 2545-6377 UNIVERSIDAD NACIONAL DE LA PLATA - FACULTAD DE CIENCIAS NATURALES Y MUSEO Revista del Museo de La Plata 2018 Volumen 3, Número 2 (Julio-Diciembre): 223-295 Geologists of Russian origin in Latin America P. Tchoumatchenco1, A.C. Riccardi2, †M. Durand Delga3, R. Alonso4, M. Wiasemsky5, D. Boltovskoy6, R. Charrier7, E. Minina8 1 Geological Institute, Bulgarian Academy of Sciences Acad. G. Bonchev Str. Bl. 24, 1113 Sofia, Bulgaria, [email protected] 2 Museo de La Plata, Facultad de Ciencias Naturales y Museo, Universidad Nacional de La Plata, Argentina, [email protected] 3 Passed away August19, 2012 4 Universidad Nacional de Salta, Argentina, [email protected] 5 81, Chemin du Plan de Charlet, F-74190 Passy, France, [email protected] 6 Dep. -
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. -
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. -
Zootaxa, the Youngest Rostroconch Mollusc from North America
Zootaxa 2603: 61–64 (2010) ISSN 1175-5326 (print edition) www.mapress.com/zootaxa/ Correspondence ZOOTAXA Copyright © 2010 · Magnolia Press ISSN 1175-5334 (online edition) The youngest rostroconch mollusc from North America, Minycardita capitanensis n. sp. MICHAEL J. VENDRASCO1, RICHARD D. HOARE2 & GORDEN L. BELL, JR3 1Department of Biological Science, California State University, Fullerton, Fullerton, CA 92834-6850, USA. E-mail: [email protected] 2Department of Geology, Bowling Green State University, Bowling Green, OH 43403, USA. E-mail: [email protected] 3Guadalupe Mountains National Park, 400 Pine Canyon Drive, Salt Flat, TX 79847, USA. E-mail: [email protected] Rostroconchs are an extinct class of mollusc that lived worldwide through most or all of the Paleozoic Era (Runnegar 1978). They were most diverse in the early Paleozoic (Pojeta 1985), perhaps due to a lower rate of evolution in the rostroconch clade that survived the end-Ordovician mass extinction event (Wagner 1997). Rostroconchs have a univalved larval shell and a pseudo-bivalved adult shell. Their ecology appears to have ranged from infaunal to rarely epifaunal, and from deposit to suspension feeding (Pojeta et al. 1972, Pojeta & Runnegar 1976, Runnegar 1978, Pojeta 1987). A single but well-preserved, essentially complete rostroconch specimen was recovered from the region surrounded by the famous Capitan Reef of the Permian of West Texas (Newell et al. 1953). In particular, the specimen is from the upper scaphopod bed of the Reef Trail Member of the Bell Canyon Formation exposed in the Guadalupe Mountains National Park (Rigby & Bell 2005: fig. 2). The fusulinid biostratigraphic zonal indicator Paraboultonia splendens Skinner & Wilde, 1954 occurs both below the upper scaphopod bed and above it, indicating that this horizon was deposited during the latest Guadalupian (late middle Permian) (Rigby & Bell 2006), and thus is the youngest known deposit in North America to contain a rostroconch. -
Mesh-Based Tectonic Reconstruction: Andean Margin Evolution Since the Cretaceous
Mesh-based tectonic reconstruction: Andean margin evolution since the Cretaceous Tomas P. O'Kane, Gordon S. Lister Journal of the Virtual Explorer, Electronic Edition, ISSN 1441-8142, volume 43, paper 1 In: (Eds.) Stephen Johnston and Gideon Rosenbaum, Oroclines, 2012. Download from: http://virtualexplorer.com.au/article/2011/297/mesh-based-tectonic-reconstruction Click http://virtualexplorer.com.au/subscribe/ to subscribe to the Journal of the Virtual Explorer. Email [email protected] to contact a member of the Virtual Explorer team. Copyright is shared by The Virtual Explorer Pty Ltd with authors of individual contributions. Individual authors may use a single figure and/or a table and/or a brief paragraph or two of text in a subsequent work, provided this work is of a scientific nature, and intended for use in a learned journal, book or other peer reviewed publication. Copies of this article may be made in unlimited numbers for use in a classroom, to further education and science. The Virtual Explorer Pty Ltd is a scientific publisher and intends that appropriate professional standards be met in any of its publications. Journal of the Virtual Explorer, 2012 Volume 43 Paper 1 http://virtualexplorer.com.au/ Mesh-based tectonic reconstruction: Andean margin evolution since the Cretaceous Tomas P. O'Kane Research School of Earth Sciences, The Australian National University, Canberra 0200 Australia. Email: [email protected] Gordon S. Lister Research School of Earth Sciences, The Australian National University, Canberra 0200 Australia. Abstract: In this contribution we demonstrate an example of what can be described as mesh-based tectonic reconstruction. -
4 Three-Dimensional Density Model of the Nazca Plate and the Andean Continental Margin
76 4 Three-dimensional density model of the Nazca plate and the Andean continental margin Authors: Andrés Tassara, Hans-Jürgen Götze, Sabine Schmidt and Ron Hackney Paper under review (September 27th, 2005) by the Journal of Geophysical Research Abstract We forward modelled the Bouguer anomaly in a region encompassing the Pacific ocean (east of 85°W) and the Andean margin (west of 60°W) between northern Peru (5°S) and Patagonia (45°S). The three-dimensional density structure used to accurately reproduce the gravity field is simple. The oceanic Nazca plate is formed by one crustal body and one mantle lithosphere body overlying a sub-lithospheric mantle, but fracture zones divide the plate into seven along-strike segments. The subducted slab was modelled to a depth of 410 km, has the same structure as the oceanic plate, but it is subdivided into four segments with depth. The continental margin consists of one upper-crustal and one lower-crustal body without lateral subdivision, whereas the mantle has two bodies for the lithosphere and two bodies for the asthenosphere that are separated across-strike by the downward prolongation of the eastern limit of active volcanism. We predefined the density for each body after studying its dependency on composition of crustal and mantle materials and pressure-temperature conditions appropriate for the Andean setting. A database containing independent geophysical information constrains the geometry of the subducted slab, locally the Moho of the oceanic and continental crusts, and indirectly the lithosphere-asthenosphere boundary (LAB) underneath the continental plate. Other geometries, especially that of the intracrustal density discontinuity (ICD) in the continental margin, were not constrained and are the result of fitting the observed and calculated Bouguer anomaly during the forward modelling.