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The San Bias Pluton: an Example of Carboniferous Plutonism in the Sierras Pampeanas, Argentina
The San BIas Pluton: An example of Carboniferous plutonism in the Sierras Pampeanas, Argentina l.A. Dahlquist a.*, R.l. Pankhurst b, c.w. Rapela e, C. Casquet d, C.M. Fanning e, P. Alasino f, M. Baez g a UNdeC-CRlLAR-CONICET, Entre Ríos y Mendoza, 5301 Anillaco, La Rioja, Argentina b NERC lsotope Geosciences Laboratory, British Geological Survey, Keyworth, Nottingham, NG12 5GG, UK e Centro de Investigaciones Geológicas, Universidad Nacional de La Plata-CONICET, Calle / No. 644, /900 La Plata, Argentina d Universidad Complutense de Madrid, Facultad de Geología, Dpto. de Petrología y Geoquímica, 28040 Madrid, España e Research School of Earth Sciences, The Australian National University, Mills Road, Canberra, ACT 0200, Australia f CRlLAR-CONICET, Entre Ríos y Mendoza, 5301 Anillaco, La Rioja, Argentina g INSUGEO-UNT, Miguel Litio 205, 4000 S.M. de Tucumán, Argentina Abstraet New geoehronologieal and geoehemieal data are reported for the San BIas Pluton (SBP), in the northwestern Sierra de Velaseo, Sierras Pampeanas, whieh intrudes Ordovieian granitoids developed during the Famatinian orogeny. A precise Carboniferous age of 340 ± 3 Ma is established by U-Pb dating of zireon using a sensitive high-resolution ion mieroprobe (SHRIMP). The SBP illustrates several petrologieal and geoehemieal eharaeteristies of previously reported Carboniferous granitoids in the Sierras Pampeanas. Their generation is eonsistent with a regional reheating of the erust at approximately 342 Ma, whieh resulted in the forn1ation of relatively large amounts of granitie melts that were emplaeed in higher erustallevels along master fractures (older master shear zones ofLower Paleozoie age). The SBP can be ehemieally defined as a typieal A-type granitoid related to posteollisonal or postorogenie magmatism. -
Radiogenic Heat Production in Granitoids from the Sierras De Córdoba, Argentina
Pleitavino et al. Geotherm Energy (2021) 9:16 https://doi.org/10.1186/s40517-021-00198-9 RESEARCH Open Access Radiogenic heat production in granitoids from the Sierras de Córdoba, Argentina M. Pleitavino1,2* , M. E. Carro Pérez1,3,4 , E. García Aráoz1,4 and M. A. Cioccale1 *Correspondence: [email protected] Abstract 1 Facultad de Ciencias One of the most important processes of heat generation from the Earth’s interior is Exactas, Físicas y Naturales, Universidad Nacional de the radioactive decay of isotopes. The main hosts of the major radiogenic elements Córdoba, Av. Vélez Sarsfeld U, Th and K in the crust are granitoids. The Sierras de Córdoba are formed of dissimilar 1611, X5016CGA Córdoba, granitic intrusions emplaced by a series of magmatic events that occurred during Argentina Full list of author information the Paleozoic. The diferent granitoids are classifed as A-type, I-type, and S-type, and is available at the end of the there is also a magmatic expression corresponding to the Famatinian period which article exhibits TTG-type characteristics. In this work, the geochemical concentrations of the radiogenic elements of the granitic intrusions making up the Sierras de Córdoba were compiled in a single database. The radiogenic heat production of the Sierras de Córdoba granitoids was evaluated, making this the frst study of radiogenic heat gen- eration in the area. The radiogenic heat production showed variability for the diferent events, with the highest values found in Achalian magmatism and early Carboniferous magmatism, which are represented by A-type granitoids. The Capilla del Monte pluton has the highest heat production rate, with a value of 4.54 1.38 µW/m3. -
Basement Composition and Basin Geometry Controls on Upper-Crustal Deformation in the Southern Central Andes (30–36° S)
Geol. Mag.: page 1 of 17 c Cambridge University Press 2016 1 doi:10.1017/S0016756816000364 Basement composition and basin geometry controls on upper-crustal deformation in the Southern Central Andes (30–36° S) ∗ ∗ ∗ JOSÉ F. MESCUA †, LAURA GIAMBIAGI , MATÍAS BARRIONUEVO , ∗ ∗ ANDRÉS TASSARA‡, DIEGO MARDONEZ , MANUELA MAZZITELLI ∗ & ANA LOSSADA ∗ Instituto Argentino de Nivología, Glaciología y Ciencias Ambientales (IANIGLA), Centro Científico Tecnológico Mendoza, CONICET. Av. Ruiz leal s/n Parque General San Martín, Mendoza (5500) Argentina ‡Departamento de Ciencias de la Tierra, Universidad de Concepción, Victor Lamas 1290, Barrio Universitario, Concepción, Casilla 160-C, Chile (Received 13 December 2015; accepted 5 April 2016) Abstract – Deformation and uplift in the Andes are a result of the subduction of the Nazca plate below South America. The deformation shows variations in structural style and shortening along and across the strike of the orogen, as a result of the dynamics of the subduction system and the features of the upper plate. In this work, we analyse the development of thin-skinned and thick-skinned fold and thrust belts in the Southern Central Andes (30–36° S). The pre-Andean history of the area determined the formation of different basement domains with distinct lithological compositions, as a result of terrane accretions during Palaeozoic time, the development of a widespread Permo-Triassic magmatic province and long-lasting arc activity. Basin development during Palaeozoic and Mesozoic times produced thick sedimentary successions in different parts of the study area. Based on estimations of strength for the different basement and sedimentary rocks, calculated using geophysical estimates of rock physical properties, we propose that the contrast in strength between basement and cover is the main control on structural style (thin- v. -
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. -
IV. Northern South America EIA/ARI World Shale Gas and Shale Oil Resource Assessment
IV. Northern South America EIA/ARI World Shale Gas and Shale Oil Resource Assessment IV. NORTHERN SOUTH AMERICA SUMMARY Northern South America has prospective shale gas and shale oil potential within marine- deposited Cretaceous shale formations in three main basins: the Middle Magdalena Valley and Llanos basins of Colombia, and the Maracaibo/Catatumbo basins of Venezuela and Colombia, Figure IV-1. The organic-rich Cretaceous shales (La Luna, Capacho, and Gacheta) sourced much of the conventional gas and oil produced in Colombia and western Venezuela, and are similar in age to the Eagle Ford and Niobrara shale plays in the USA. Ecopetrol, ConocoPhillips, ExxonMobil, Shell, and others have initiated shale exploration in Colombia. Colombia’s petroleum fiscal regime is considered attractive to foreign investment. Figure IV-1: Prospective Shale Basins of Northern South America Source: ARI 2013 May 17, 2013 IV-1 IV. Northern South America EIA/ARI World Shale Gas and Shale Oil Resource Assessment For the current EIA/ARI assessment, the Maracaibo-Catatumbo Basin was re-evaluated while new shale resource assessments were undertaken on the Middle Magdalena Valley and Llanos basins. Technically recoverable resources (TRR) of shale gas and shale oil in northern South America are estimated at approximately 222 Tcf and 20.2 billion bbl, Tables IV-1 and IV- 2. Colombia accounts for 6.8 billion barrels and 55 Tcf of risked TRR, while western Venezuela has 13.4 billion barrels and 167 Tcf. Eastern Venezuela may have additional potential but was not assessed due to lack of data. Colombia’s first publicly disclosed shale well logged 230 ft of over-pressured La Luna shale with average 14% porosity. -
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. -
Gondwanide Continental Collision and the Origin of Patagonia 3 4 R.J
1 2 Gondwanide continental collision and the origin of Patagonia 3 4 R.J. Pankhurst1*, C.W. Rapela2, C.M. Fanning3, M. Márquez4 5 6 1. Visiting Research Associate, NERC Isotope Geosciences Laboratory, British Geological Survey, 7 Keyworth, Nottingham NG12 5GG, U.K. 8 2. Centro de Investigaciones Geológicas, CONICET-UNLP, Calle 1 No. 644, 1900 La Plata, Argentina 9 3. Research School of Earth Sciences, The Australian National University, Mills Road, Canberra, ACT 200, 10 Australia 11 4. Universidad Nacional de la Patagonia San Juan Bosco, Departamento de Geología, Kilómetro 4, 12 9000 Comodoro Rivadavia, Argentina. 13 14 *Corresponding author. Tel.: +44 115 9363263; fax.: +44 115 9363302. 15 E-Mail addresses: [email protected] (R.J. Pankhurst), [email protected] (C.W. Rapela), 16 [email protected] (C.M. Fanning), [email protected] (M. Márquez). 17 18 Abstract 19 A review of the post-Cambrian igneous, structural and metamorphic history of 20 Patagonia, largely revealed by a five-year programme of U–Pb zircon dating (32 samples), 21 geochemical and isotope analysis, results in a new Late Palaeozoic collision model as the 22 probable cause of the Gondwanide fold belts of South America and South Africa. 23 In the northeastern part of the North Patagonian Massif, Cambro-Ordovician 24 metasediments with a Gondwana provenance are intruded by Mid Ordovician granites 25 analogous to those of the Famatinian arc of NW Argentina; this area is interpreted as 26 Gondwana continental crust at least from Devonian times, probably underlain by 27 Neoproterozoic crystalline basement affected by both Pampean and Famatinian events, 28 with a Cambrian rifting episode previously identified in the basement of the Sierra de la 29 Ventana. -
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. -
The Taconic Orogeny in Newfoundland: a Three-Stage Process
atlantic geology . volume 43 . 2007 83 geochronology and isotope geology, indicated that this model was incomplete. We will present new evidence that the Taconic orogeny comprises three separate accretionary events starting in the Late Cambrian and finishing in the Late Ordovician. Taconic 1 is represented by ca. 495 Ma west-directed obduc- tion of the ca. 510 Ma Lushs Bight oceanic Tract onto the peri- Laurentian Dashwoods microcontinent. Subduction is inferred to have initiated at a spreading centre abandoned during an inboard ridge jump responsible for separation of Dashwoods from Laurentia. Partial subduction of the buoyant Dashwoods forced subduction to step back into the Humber seaway, which led to formation of the ca. 490 Ma Baie Verte oceanic tract (BVOT). Dextral oblique closure of the Humber seaway first formed the Notre Dame arc (489–477 Ma) built on Dashwoods and the coeval Snooks Arm arc built on the BVOT, followed by their collision with Laurentia (Taconic 2) and each other. The obliquity of convergence induced large-scale translations of continental ribbons of the Laurentian margin from the lati- tude of Labrador to central Newfoundland. After a magmatic gap of c. 7–10 my, the Notre Dame arc records a voluminous flare-up of predominantly tonalite magmatism (464–459 Ma) during the waning stages of Taconic 2. Magmatism overlaps with strong deformation and comprises both arc and non-arc- like tonalite. We relate this flare-up to break-off of the oceanic lithosphere of the downgoing Laurentian slab. Taconic 3 is rep- resented by 455–450 Ma collision between a peri-Laurentian arc terrane and the peri-Gondwanan Popelogan-Exploits arc and their composite accretion to Laurentia. -
New Studies of Uranium Deposits Related to Granites in Argentina
NEW STUDIES OF URANIUM DEPOSITS RELATED TO GRANITES IN ARGENTINA J. ÁLVAREZ, L. LÓPEZ, F. PARRA, C. BELLO, P. ANZIL, M. SALVATORE, L. SCARLATTA, P. FERREYRA, S. MIYNO, E. FELKAI Comisión Nacional de Energía Atómica (CNEA), Buenos Aires, Argentina R. LIRA CONICET- FCEFyN-UNC, Córdoba, Argentina A. HANLY International Atomic Energy Agency, Vienna, Austria M. CUNEY, J. MERCADIER Université de Lorraine, Nancy, France 1. INTRODUCTION At present, the Comisión Nacional de Energía Atómica, in cooperation with the National University of Córdoba, is carrying out the project entitled Melallogenesis of Granite-Related Uranium Deposits in Argentina within the framework of an IAEA coordinated research project which is Geochemical and Mineralogical Characterization of Uranium and Thorium Deposits. This paper briefly describes the specific objectives and activities in progress as part of this research project, which has been underway since 2015 [1]. This project aims to focus on the characterization of the Devonian–Lower Carboniferous magmatic and hydrothermal systems related to granitoids of the Pampean Ranges and to relate these processes to uranium metallogeny. Therefore, several metallogenetic studies have been carried out in order to improve the geological, structural, geochemical and mineralogical characterization of uranium deposits related to granites. To this end, efforts have been made to define those felsic igneous rocks that have played the most relevant role as uranium sources, including successive fractionation in the different magmatic complexes and characterize the relationship between magmatic uranium enrichment and hydrothermal deposits, and alteration and uranium mobility. 2. DESCRIPTION AND RESULTS The scientific scope of this paper specifically covers four areas of uranium mineralization where granite- related (endogranitic) hosts have been described: Sala Grande, Don Alberto and Los Riojanos are enclosed in the Achala Batholith, and La Estela is located in the Cerro Áspero–Alpa Corral Batholith [2, 3]. -
The Geology, Paleontology and Paleoecology of the Cerro Fortaleza Formation
The Geology, Paleontology and Paleoecology of the Cerro Fortaleza Formation, Patagonia (Argentina) A Thesis Submitted to the Faculty of Drexel University by Victoria Margaret Egerton in partial fulfillment of the requirements for the degree of Doctor of Philosophy November 2011 © Copyright 2011 Victoria M. Egerton. All Rights Reserved. ii Dedications To my mother and father iii Acknowledgments The knowledge, guidance and commitment of a great number of people have led to my success while at Drexel University. I would first like to thank Drexel University and the College of Arts and Sciences for providing world-class facilities while I pursued my PhD. I would also like to thank the Department of Biology for its support and dedication. I would like to thank my advisor, Dr. Kenneth Lacovara, for his guidance and patience. Additionally, I would like to thank him for including me in his pursuit of knowledge of Argentine dinosaurs and their environments. I am also indebted to my committee members, Dr. Gail Hearn, Dr. Jake Russell, Dr. Mike O‘Connor, Dr. Matthew Lamanna, Dr. Christopher Williams and Professor Hermann Pfefferkorn for their valuable comments and time. The support of Argentine scientists has been essential for allowing me to pursue my research. I am thankful that I had the opportunity to work with such kind and knowledgeable people. I would like to thank Dr. Fernando Novas (Museo Argentino de Ciencias Naturales) for helping me obtain specimens that allowed this research to happen. I would also like to thank Dr. Viviana Barreda (Museo Argentino de Ciencias Naturales) for her allowing me use of her lab space while I was visiting Museo Argentino de Ciencias Naturales. -
GSA TODAY • Radon in Water, P
Vol. 8, No. 11 November 1998 INSIDE • Field Guide Editor, p. 5 GSA TODAY • Radon in Water, p. 10 • Women Geoscientists, p. 12 A Publication of the Geological Society of America • 1999 Annual Meeting, p. 31 Gas Hydrates: Greenhouse Nightmare? Energy Panacea or Pipe Dream? Bilal U. Haq, National Science Foundation, Division of Ocean Science, Arlington, VA 22230 ABSTRACT Recent interest in methane hydrates has resulted from the recognition that they may play important roles in the global carbon cycle and rapid climate change through emissions of methane from marine sediments and permafrost into the atmosphere, and in causing mass failure of sediments and structural changes on the continental slope. Their presumed large volumes are also consid- ered to be a potential source for future exploitation of methane as a resource. Natural gas hydrates occur widely on continental slope and rise, stabilized in place by high hydrostatic pressure and frigid bottom-temperature condi- tions. Change in these conditions, Figure 1. This seismic profile, over the landward side of Blake Ridge, crosses a salt diapir; the profile has either through lowering of sea level or been processed to show reflection strength. The prominent bottom simulating reflector (BSR) swings increase in bottom-water temperature, upward over the diapir because of the higher conductivity of the salt. Note the very strong reflections of may trigger the following sequence of gas accumulations below the gas-hydrate stability zone and the “blanking” of energy above it. Bright events: dissociation of the hydrate at its Spots along near-vertical faults above the diapir represent conduits for gas venting.