The History and Evolution of Payún Matrú Caldera, Mendoza Province, Argentina

Total Page:16

File Type:pdf, Size:1020Kb

The History and Evolution of Payún Matrú Caldera, Mendoza Province, Argentina University of Wollongong Research Online Faculty of Science, Medicine & Health - Honours Theses University of Wollongong Thesis Collections 2012 The History and Evolution of Payún Matrú Caldera, Mendoza Province, Argentina Ryan Manton University of Wollongong Follow this and additional works at: https://ro.uow.edu.au/thsci University of Wollongong Copyright Warning You may print or download ONE copy of this document for the purpose of your own research or study. The University does not authorise you to copy, communicate or otherwise make available electronically to any other person any copyright material contained on this site. You are reminded of the following: This work is copyright. Apart from any use permitted under the Copyright Act 1968, no part of this work may be reproduced by any process, nor may any other exclusive right be exercised, without the permission of the author. Copyright owners are entitled to take legal action against persons who infringe their copyright. A reproduction of material that is protected by copyright may be a copyright infringement. A court may impose penalties and award damages in relation to offences and infringements relating to copyright material. Higher penalties may apply, and higher damages may be awarded, for offences and infringements involving the conversion of material into digital or electronic form. Unless otherwise indicated, the views expressed in this thesis are those of the author and do not necessarily represent the views of the University of Wollongong. Recommended Citation Manton, Ryan, The History and Evolution of Payún Matrú Caldera, Mendoza Province, Argentina, Bachelor of Science (Honours), School of Earth & Environmental Science, University of Wollongong, 2012. https://ro.uow.edu.au/thsci/54 Research Online is the open access institutional repository for the University of Wollongong. For further information contact the UOW Library: [email protected] The History and Evolution of Payún Matrú Caldera, Mendoza Province, Argentina Abstract A petrological and geochemical study was performed on rock samples collected from the retro-arc, Payún Matrú Caldera (36°24' S, 69°11' W) Mendoza Province, western Argentina. The caldera formed between 168 ± 4 ka and 86 ± 1 ka, with volcanic products in the area ranging from Pleistocene to Holocene (Germa et al., 2010). Payún Matrú is located on La Carbonilla Lineament, which also controls the location of at least 300 other volcanic vents. Field work was carried out over five days in late February 2012, 38 hand samples were collected and five trachyte dykes were identified within the northeast quadrant of the caldera’s topographic rim, with their strike and dip noted. Hernando et al. (2012) proposed the formation of a sub-volcanic magma chamber, with magma mixing being a dominant process. They further suggest that the influx of mafic material into the base of the chamber resulted in caldera formation. Germa et al. (2010) propose that the caldera formed from tectonic influences, due ot the regional extensional setting. More evidence was found for the former process within this research project. A comparison between the seven identified rock suites was conducted. From an analysis of petrological thin-sections, it was evident that the chamber had progressively evolved to its most mature state, immediately before caldera formation. The degree and type of dis-equilibrium textures within phenocrysts was noted, as well as the proportion of low- to high-temperature minerals. A comparison between photomicrographs and the major- and trace-element contents was made to determine the conditions in the chamber at a given point in time. A method which utilised digital elevation models to measure the physical attributes of lava flows around Payún Matrú was also used and tested to demonstrate the evolution of melts from the Payún Matrú magma chamber. It was found that the most likely cause of caldera formation was the over- pressuring of a zoned magma chamber, due to an influx of mafic material. This resulted in the eruption of only the evolved upper portion of the chamber, with the lower portion erupting post-caldera. This post- caldera flow eprr esents the most primitive flow, with a flat trace-element plot and a high proportion of ferromagnesian minerals. The chamber environment, post-caldera, is dominated by the crystallisation of mineral assemblages which have a high Al 2O3 content, and large ion-lithophile elements (LILE) such as Sr and Ba are accepted into the mineral assemblage. This is supported by the presence of large, unsieved sanidine phenocrysts in the petrological analysis. The waning of mafic material into the chamber is thought to have occurred after this period. The significance of this project is that it demonstrates the possible mechanisms for large, ash-flow, caldera- forming eruptions. Degree Type Thesis Degree Name Bachelor of Science (Honours) Department School of Earth & Environmental Science Advisor(s) Allan Chivas Keywords Lava, Viscosity, Caldera formation, Payúnia volcanic province This thesis is available at Research Online: https://ro.uow.edu.au/thsci/54 The History and Evolution of Payún Matrú Caldera, Mendoza Province, Argentina By Ryan Manton A thesis submitted in part fulfilment of the requirements of the Honours degree of Bachelor of Science in the School of Earth and Environmental Sciences University of Wollongong, 2012 The information in this thesis is entirely the result of investigations conducted by the author unless otherwise acknowledged, and has not been submitted in part, or otherwise, for any other degree or qualification. Ryan John Manton 9/10/2012 II ABSTRACT A petrological and geochemical study was performed on rock samples collected from the retro-arc, Payún Matrú Caldera (36°24' S, 69°11' W) Mendoza Province, western Argentina. The caldera formed between 168 ± 4 ka and 86 ± 1 ka, with volcanic products in the area ranging from Pleistocene to Holocene (Germa et al., 2010). Payún Matrú is located on La Carbonilla Lineament, which also controls the location of at least 300 other volcanic vents. Field work was carried out over five days in late February 2012, 38 hand samples were collected and five trachyte dykes were identified within the northeast quadrant of the caldera’s topographic rim, with their strike and dip noted. Hernando et al. (2012) proposed the formation of a sub-volcanic magma chamber, with magma mixing being a dominant process. They further suggest that the influx of mafic material into the base of the chamber resulted in caldera formation. Germa et al. (2010) propose that the caldera formed from tectonic influences, due to the regional extensional setting. More evidence was found for the former process within this research project. A comparison between the seven identified rock suites was conducted. From an analysis of petrological thin-sections, it was evident that the chamber had progressively evolved to its most mature state, immediately before caldera formation. The degree and type of dis-equilibrium textures within phenocrysts was noted, as well as the proportion of low- to high-temperature minerals. A comparison between photomicrographs and the major- and trace-element contents was made to determine the conditions in the chamber at a given point in time. A method which utilised digital elevation models to measure the physical attributes of lava flows around Payún Matrú was also used and tested to demonstrate the evolution of melts from the Payún Matrú magma chamber. It was found that the most likely cause of caldera formation was the over-pressuring of a zoned magma chamber, due to an influx of mafic material. This resulted in the eruption of only the evolved upper portion of the chamber, with the lower portion erupting post-caldera. This post-caldera flow represents the most primitive flow, with a flat trace-element plot and a high proportion of ferromagnesian minerals. The chamber environment, post-caldera, is dominated by the crystallisation of mineral assemblages which have a high Al2O3 content, and large ion- lithophile elements (LILE) such as Sr and Ba are accepted into the mineral assemblage. This is supported by the presence of large, unsieved sanidine phenocrysts in the petrological analysis. The waning of mafic material into the chamber is thought to have occurred after this period. The significance of this project is that it demonstrates the possible mechanisms for large, ash-flow, caldera-forming eruptions. III TABLE OF CONTENTS Introduction ........................................................................................................................................... 1 1.1 Location and Background ........................................................................................................... 1 1.2 Previous Field Work around Payún Matrú ................................................................................ 2 1.3 Aims and Objectives ................................................................................................................... 3 1.4 Methodology .............................................................................................................................. 4 Regional Geology .................................................................................................................................. 8 2.1 The Andean Orogeny ................................................................................................................... 8 2.2 The Gondwanide Margin .........................................................................................................
Recommended publications
  • Geologic Map of the Central San Juan Caldera Cluster, Southwestern Colorado by Peter W
    Geologic Map of the Central San Juan Caldera Cluster, Southwestern Colorado By Peter W. Lipman Pamphlet to accompany Geologic Investigations Series I–2799 dacite Ceobolla Creek Tuff Nelson Mountain Tuff, rhyolite Rat Creek Tuff, dacite Cebolla Creek Tuff Rat Creek Tuff, rhyolite Wheeler Geologic Monument (Half Moon Pass quadrangle) provides exceptional exposures of three outflow tuff sheets erupted from the San Luis caldera complex. Lowest sheet is Rat Creek Tuff, which is nonwelded throughout but grades upward from light-tan rhyolite (~74% SiO2) into pale brown dacite (~66% SiO2) that contains sparse dark-brown andesitic scoria. Distinctive hornblende-rich middle Cebolla Creek Tuff contains basal surge beds, overlain by vitrophyre of uniform mafic dacite that becomes less welded upward. Uppermost Nelson Mountain Tuff consists of nonwelded to weakly welded, crystal-poor rhyolite, which grades upward to a densely welded caprock of crystal-rich dacite (~68% SiO2). White arrows show contacts between outflow units. 2006 U.S. Department of the Interior U.S. Geological Survey CONTENTS Geologic setting . 1 Volcanism . 1 Structure . 2 Methods of study . 3 Description of map units . 4 Surficial deposits . 4 Glacial deposits . 4 Postcaldera volcanic rocks . 4 Hinsdale Formation . 4 Los Pinos Formation . 5 Oligocene volcanic rocks . 5 Rocks of the Creede Caldera cycle . 5 Creede Formation . 5 Fisher Dacite . 5 Snowshoe Mountain Tuff . 6 Rocks of the San Luis caldera complex . 7 Rocks of the Nelson Mountain caldera cycle . 7 Rocks of the Cebolla Creek caldera cycle . 9 Rocks of the Rat Creek caldera cycle . 10 Lava flows premonitory(?) to San Luis caldera complex . .11 Rocks of the South River caldera cycle .
    [Show full text]
  • Field Excursion Report 2010
    Presented at “Short Course on Geothermal Drilling, Resource Development and Power Plants”, organized by UNU-GTP and LaGeo, in Santa Tecla, El Salvador, January 16-22, 2011. GEOTHERMAL TRAINING PROGRAMME LaGeo S.A. de C.V. GEOTHERMAL ACTIVITY AND DEVELOPMENT IN SOUTH AMERICA: SHORT OVERVIEW OF THE STATUS IN BOLIVIA, CHILE, ECUADOR AND PERU Ingimar G. Haraldsson United Nations University Geothermal Training Programme Orkustofnun, Grensasvegi 9, 108 Reykjavik ICELAND [email protected] ABSTRACT South America holds vast stores of geothermal energy that are largely unexploited. These resources are largely the product of the convergence of the South American tectonic plate and the Nazca plate that has given rise to the Andes mountain chain, with its countless volcanoes. High-temperature geothermal resources in Bolivia, Chile, Ecuador and Peru are mainly associated with the volcanically active regions, although low temperature resources are also found outside them. All of these countries have a history of geothermal exploration, which has been reinvigorated with recent changes in global energy prices and the increased emphasis on renewables to combat global warming. The paper gives an overview of their main regions of geothermal activity and the latest developments in the geothermal sector are reviewed. 1. INTRODUCTION South America has abundant geothermal energy resources. In 1999, the Geothermal Energy Association estimated the continent’s potential for electricity generation from geothermal resources to be in the range of 3,970-8,610 MW, based on available information and assuming the use of technology available at that time (Gawell et al., 1999). Subsequent studies have put the potential much higher, as a preliminary analysis of Chile alone assumes a generation potential of 16,000 MW for at least 50 years from geothermal fluids with temperatures exceeding 150°C, extracted from within a depth of 3,000 m (Lahsen et al., 2010).
    [Show full text]
  • Neotectonics Along the Eastern Flank of the North Patagonian Icefield, Southern Chile: Cachet and Exploradores Fault Zones
    XII Congreso Geológico Chileno Santiago, 22-26 Noviembre, 2009 S9_053 Neotectonics along the eastern flank of the North Patagonian Icefield, southern Chile: Cachet and Exploradores fault zones Melnick, D.1, Georgieva, V.1, Lagabrielle, Y.2, Jara, J.3, Scalabrino, B.2, Leidich, J.4 (1) Institute of Geosciences, University of Potsdam, 14476 Potsdam, Germany. (2) UMR 5243 Géosciences Montpellier, Université de Montpellier 2, France. (3) Departamento de Ciencias de la Tierra, Universidad de Concepción, Chile. (4) Patagonia Adventure Expeditions, Casilla 8, Cochrane, Chile. [email protected] Introduction In the southern Andes, the North Patagonian Icefield (NPI) is a poorly-known region in terms of geology and neotectonics that marks a major topographic anomaly at the transition between the Austral and Patagonian Andes. The NPI is located immediately east of the Nazca-Antarctic-South America Triple Plate Junction, where the Chile Rise collides against the margin (Fig. 1A). Since 14 Ma, this Triple Junction has migrated northward as a result of oblique plate convergence, resulting in collision and subduction of two relatively short ridge segments in the Golfo de Penas region at 6 and 3 Ma, and at present of one segment immediately north of the Taitao Peninsula [1]. Oblique plate convergence in addition to collision of these ridge segments resulted in the formation of a forearc sliver, the Chiloe block, which is decoupled from the South American foreland by the Liquiñe-Ofqui fault zone. Here we present geomorphic and structural field evidence that indicates neotectonic activity in the internal part of the orogen, along the flanks of the NPI (Fig.
    [Show full text]
  • Eruptive Activity of Planchón-Peteroa Volcano for Period 2010-2011, Southern Andean Volcanic Zone, Chile
    Andean Geology 43 (1): 20-46. January, 2016 Andean Geology doi: 10.5027/andgeoV43n1-a02 www.andeangeology.cl Eruptive activity of Planchón-Peteroa volcano for period 2010-2011, Southern Andean Volcanic Zone, Chile *Felipe Aguilera1, 2, Óscar Benavente3, Francisco Gutiérrez3, Jorge Romero4, Ornella Saltori5, Rodrigo González6, Mariano Agusto7, Alberto Caselli8, Marcela Pizarro5 1 Servicio Nacional de Geología y Minería, Avda. Santa María 0104, Santiago, Chile. 2 Present address: Departamento de Ciencias Geológicas, Universidad Católica del Norte, Avda. Angamos 0610, Antofagasta, Chile. [email protected] 3 Departamento de Geología, Universidad de Chile, Plaza Ercilla 803, Santiago, Chile. [email protected]; [email protected] 4 Centro de Investigación y Difusión de Volcanes de Chile, Proyecto Archivo Nacional de Volcanes, Santiago, Chile. [email protected] 5 Programa de Doctorado en Ciencias mención Geología, Universidad de Chile, Plaza Ercilla 803, Santiago, Chile. [email protected]; [email protected] 6 Departamento de Ciencias Geológicas, Universidad Católica del Norte, Avda. Angamos 0610, Antofagasta, Chile. [email protected] 7 Departamento de Ciencias Geológicas, Universidad de Buenos Aires, Ciudad Universitaria, Pabellón 2, 1428EHA, Buenos Aires, Argentina. [email protected] 8 Laboratorio de Estudio y Seguimiento de Volcanes Activos (LESVA), Universidad Nacional de Río Negro, Roca 1242, (8332) Roca, Argentina. [email protected] * Corresponding author: [email protected] ABSTRACT. Planchón-Peteroa volcano started a renewed eruptive period between January 2010 and July 2011. This eruptive period was characterized by the occurrence of 4 explosive eruptive phases, dominated by low-intensity phreatic activity, which produced almost permanent gas/steam columns (200-800 m height over the active crater).
    [Show full text]
  • Widespread Crater-Related Pitted Materials on Mars: Further Evidence for the Role of Target Volatiles During the Impact Process ⇑ Livio L
    Icarus 220 (2012) 348–368 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Widespread crater-related pitted materials on Mars: Further evidence for the role of target volatiles during the impact process ⇑ Livio L. Tornabene a, , Gordon R. Osinski a, Alfred S. McEwen b, Joseph M. Boyce c, Veronica J. Bray b, Christy M. Caudill b, John A. Grant d, Christopher W. Hamilton e, Sarah Mattson b, Peter J. Mouginis-Mark c a University of Western Ontario, Centre for Planetary Science and Exploration, Earth Sciences, London, ON, Canada N6A 5B7 b University of Arizona, Lunar and Planetary Lab, Tucson, AZ 85721-0092, USA c University of Hawai’i, Hawai’i Institute of Geophysics and Planetology, Ma¯noa, HI 96822, USA d Smithsonian Institution, Center for Earth and Planetary Studies, Washington, DC 20013-7012, USA e NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA article info abstract Article history: Recently acquired high-resolution images of martian impact craters provide further evidence for the Received 28 August 2011 interaction between subsurface volatiles and the impact cratering process. A densely pitted crater-related Revised 29 April 2012 unit has been identified in images of 204 craters from the Mars Reconnaissance Orbiter. This sample of Accepted 9 May 2012 craters are nearly equally distributed between the two hemispheres, spanning from 53°Sto62°N latitude. Available online 24 May 2012 They range in diameter from 1 to 150 km, and are found at elevations between À5.5 to +5.2 km relative to the martian datum. The pits are polygonal to quasi-circular depressions that often occur in dense clus- Keywords: ters and range in size from 10 m to as large as 3 km.
    [Show full text]
  • THE 1:1,000,000 GEOLOGIC MAP of ARSIA MONS, MARS. W. B. Garry1, D. A. Williams2, A. M. Dapremont3 and D. E. Shean4 1NASA Goddard
    Planetary Geologic Mappers Meeting 2018 (LPI Contrib. No. 2066) 7028.pdf THE 1:1,000,000 GEOLOGIC MAP OF ARSIA MONS, MARS. W. B. Garry1, D. A. Williams2, A. M. Dapremont3 and D. E. Shean4 1NASA Goddard Space Flight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771, [email protected], 2School of Earth and Space Exploration, Arizona State University, Tempe, AZ, 85287, 3Earth and Atmospheric Sciences, Georgia Institute of Technology, Atlanta, GA, 30331, 4College of Engineering, University of Washington, Seattle, WA, 98195. Introduction: Arsia Mons, centered at 8.26°S and (MGS) Mars Orbiter Laser Altimeter (MOLA) topogra- 239.1°E, is the southernmost edifice of the three Tharsis phy [15] that reveal morphologic details and spatial re- Montes volcanoes on Mars. Each volcano has a similar, lationships appropriate for our mapping purposes. overall shape and structure [1, 2], but there are distinct Mapping Methods: Mapping was completed in spatial distributions of morphologic features that hint ESRI’s ArcMap™ 10.2. Line work was drawn at map each volcano has a slightly different evolution history scales of ~1:100,000 to ~1:50,000 with vertex spacing [3]. To determine the differences between these three of 500 m and registered to the THEMIS daytime infra- Martian shield volcanoes, we present a series of individ- red base map. The final ArcMap project includes loca- ual geologic maps of Arsia (this map), Pavonis [4], and tion features (points), linear features (lines), geologic Ascraeus Mons [5] based on high-resolution data sets to contacts (lines), and geologic map (polygons). show their similarities and differences.
    [Show full text]
  • Volcanism on Mars
    Author's personal copy Chapter 41 Volcanism on Mars James R. Zimbelman Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC, USA William Brent Garry and Jacob Elvin Bleacher Sciences and Exploration Directorate, Code 600, NASA Goddard Space Flight Center, Greenbelt, MD, USA David A. Crown Planetary Science Institute, Tucson, AZ, USA Chapter Outline 1. Introduction 717 7. Volcanic Plains 724 2. Background 718 8. Medusae Fossae Formation 725 3. Large Central Volcanoes 720 9. Compositional Constraints 726 4. Paterae and Tholi 721 10. Volcanic History of Mars 727 5. Hellas Highland Volcanoes 722 11. Future Studies 728 6. Small Constructs 723 Further Reading 728 GLOSSARY shield volcano A broad volcanic construct consisting of a multitude of individual lava flows. Flank slopes are typically w5, or less AMAZONIAN The youngest geologic time period on Mars identi- than half as steep as the flanks on a typical composite volcano. fied through geologic mapping of superposition relations and the SNC meteorites A group of igneous meteorites that originated on areal density of impact craters. Mars, as indicated by a relatively young age for most of these caldera An irregular collapse feature formed over the evacuated meteorites, but most importantly because gases trapped within magma chamber within a volcano, which includes the potential glassy parts of the meteorite are identical to the atmosphere of for a significant role for explosive volcanism. Mars. The abbreviation is derived from the names of the three central volcano Edifice created by the emplacement of volcanic meteorites that define major subdivisions identified within the materials from a centralized source vent rather than from along a group: S, Shergotty; N, Nakhla; C, Chassigny.
    [Show full text]
  • March 21–25, 2016
    FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk,
    [Show full text]
  • A Structural and Geochronological Study of Tromen Volcano
    Volcanism in a compressional Andean setting: A structural and geochronological study of Tromen volcano (Neuqu`enprovince, Argentina) Olivier Galland, Erwan Hallot, Peter Cobbold, Gilles Ruffet, Jean De Bremond d'Ars To cite this version: Olivier Galland, Erwan Hallot, Peter Cobbold, Gilles Ruffet, Jean De Bremond d'Ars. Vol- canism in a compressional Andean setting: A structural and geochronological study of Tromen volcano (Neuqu`enprovince, Argentina). Tectonics, American Geophysical Union (AGU), 2007, 26 (4), pp.TC4010. <10.1029/2006TC002011>. <insu-00180007> HAL Id: insu-00180007 https://hal-insu.archives-ouvertes.fr/insu-00180007 Submitted on 29 Jun 2016 HAL is a multi-disciplinary open access L'archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destin´eeau d´ep^otet `ala diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publi´esou non, lished or not. The documents may come from ´emanant des ´etablissements d'enseignement et de teaching and research institutions in France or recherche fran¸caisou ´etrangers,des laboratoires abroad, or from public or private research centers. publics ou priv´es. TECTONICS, VOL. 26, TC4010, doi:10.1029/2006TC002011, 2007 Volcanism in a compressional Andean setting: A structural and geochronological study of Tromen volcano (Neuque´n province, Argentina) Olivier Galland,1,2 Erwan Hallot,1 Peter R. Cobbold,1 Gilles Ruffet,1 and Jean de Bremond d’Ars1 Received 28 June 2006; revised 6 February 2007; accepted 16 March 2007; published 2 August 2007. [1] We document evidence for growth of an active [3] In contrast, a context of crustal thickening, where the volcano in a compressional Andean setting.
    [Show full text]
  • Sr–Pb Isotopes Signature of Lascar Volcano (Chile): Insight Into Contamination of Arc Magmas Ascending Through a Thick Continental Crust N
    Sr–Pb isotopes signature of Lascar volcano (Chile): Insight into contamination of arc magmas ascending through a thick continental crust N. Sainlot, I. Vlastélic, F. Nauret, S. Moune, F. Aguilera To cite this version: N. Sainlot, I. Vlastélic, F. Nauret, S. Moune, F. Aguilera. Sr–Pb isotopes signature of Lascar volcano (Chile): Insight into contamination of arc magmas ascending through a thick continental crust. Journal of South American Earth Sciences, Elsevier, 2020, 101, pp.102599. 10.1016/j.jsames.2020.102599. hal-03004128 HAL Id: hal-03004128 https://hal.uca.fr/hal-03004128 Submitted on 13 Nov 2020 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. Copyright Manuscript File Sr-Pb isotopes signature of Lascar volcano (Chile): Insight into contamination of arc magmas ascending through a thick continental crust 1N. Sainlot, 1I. Vlastélic, 1F. Nauret, 1,2 S. Moune, 3,4,5 F. Aguilera 1 Université Clermont Auvergne, CNRS, IRD, OPGC, Laboratoire Magmas et Volcans, F-63000 Clermont-Ferrand, France 2 Observatoire volcanologique et sismologique de la Guadeloupe, Institut de Physique du Globe, Sorbonne Paris-Cité, CNRS UMR 7154, Université Paris Diderot, Paris, France 3 Núcleo de Investigación en Riesgo Volcánico - Ckelar Volcanes, Universidad Católica del Norte, Avenida Angamos 0610, Antofagasta, Chile 4 Departamento de Ciencias Geológicas, Universidad Católica del Norte, Avenida Angamos 0610, Antofagasta, Chile 5 Centro de Investigación para la Gestión Integrada del Riesgo de Desastres (CIGIDEN), Av.
    [Show full text]
  • Tracing a Major Crustal Domain Boundary Based on the Geochemistry of Minor Volcanic Centres in Southern Peru
    7th International Symposium on Andean Geodynamics (ISAG 2008, Nice), Extended Abstracts: 298-301 Tracing a major crustal domain boundary based on the geochemistry of minor volcanic centres in southern Peru Mirian Mamani1, Gerhard Wörner2, & Jean-Claude Thouret3 1 Georg-August University, Goldschmidstr. 1, 37077 Göttingen, Germany ([email protected], [email protected]) 2 Université Blaise Pascal, Clermont Ferrand, France ([email protected]) KEYWORDS : minor volcanic centres, crust, tectonic erosion, Central Andes, isotopes Introduction Geochemical studies of Tertiary to Recent magmatism in the Central Volcanic Zone have mainly focused on large stratovolcanoes. This is because mafic minor volcanic centres and related flows that formed during a single eruption are relatively rare and occur in locally clusters (e.g. Andagua/Humbo fields in S. Peru, Delacour et al., 2007; Negrillar field in N. Chile, Deruelle 1982) or in the back arc region (Davidson and de Silva, 1992). These studies showed that the "monogenetic" lavas are high-K calc-alkaline and their major, trace, and rare elements, as well as Sr-, Nd- and Pb- isotopes data display a range comparable to those of the Central Volcanic Zone composite volcanoes (Delacour et al., 2007). It has been argued that the eruptive products of these minor centers bypass the large magma chamber systems below Andean stratovolcanoes and thus may represent magmas that were derived from a deeper level in the crust (Davidson and de Silva, 1992; Ruprecht and Wörner, 2007). This study represents a continuation of our work to understand the regional variation in erupted magma composition in the Central Andes (Mamani et al., 2008; Wörner et al., 1992).
    [Show full text]
  • Taxonomic Revision of the Chilean Puya Species (Puyoideae
    Taxonomic revision of the Chilean Puya species (Puyoideae, Bromeliaceae), with special notes on the Puya alpestris-Puya berteroniana species complex Author(s): Georg Zizka, Julio V. Schneider, Katharina Schulte and Patricio Novoa Source: Brittonia , 1 December 2013, Vol. 65, No. 4 (1 December 2013), pp. 387-407 Published by: Springer on behalf of the New York Botanical Garden Press Stable URL: https://www.jstor.org/stable/24692658 JSTOR is a not-for-profit service that helps scholars, researchers, and students discover, use, and build upon a wide range of content in a trusted digital archive. We use information technology and tools to increase productivity and facilitate new forms of scholarship. For more information about JSTOR, please contact [email protected]. Your use of the JSTOR archive indicates your acceptance of the Terms & Conditions of Use, available at https://about.jstor.org/terms New York Botanical Garden Press and Springer are collaborating with JSTOR to digitize, preserve and extend access to Brittonia This content downloaded from 146.244.165.8 on Sun, 13 Dec 2020 04:26:58 UTC All use subject to https://about.jstor.org/terms Taxonomic revision of the Chilean Puya species (Puyoideae, Bromeliaceae), with special notes on the Puya alpestris-Puya berteroniana species complex Georg Zizka1'2, Julio V. Schneider1'2, Katharina Schulte3, and Patricio Novoa4 1 Botanik und Molekulare Evolutionsforschung, Senckenberg Gesellschaft für Naturforschung and Johann Wolfgang Goethe-Universität, Senckenberganlage 25, 60325, Frankfurt am Main, Germany; e-mail: [email protected]; e-mail: [email protected] 2 Biodiversity and Climate Research Center (BIK-F), Senckenberganlage 25, 60325, Frankfurt am Main, Germany 3 Australian Tropical Herbarium and Tropical Biodiversity and Climate Change Centre, James Cook University, PO Box 6811, Caims, QLD 4870, Australia; e-mail: [email protected] 4 Jardin Botânico Nacional, Camino El Olivar 305, El Salto, Vina del Mar, Chile Abstract.
    [Show full text]