Chapter 18: Volcanic Activity
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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 . -
Lunar and Planetary Science XXXII (2001) 1509.Pdf
Lunar and Planetary Science XXXII (2001) 1509.pdf TERRESTRIAL ANALOGS FOR MARTIAN VOLCANIC FEATURES SEEN IN MOC IMAGES. L. Keszthelyi and A. S. McEwen, Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona 85721 Introduction: Many of the Mars Orbital Camera lavas. For example, if basaltic lavas are erupted after images include volcanic features whose initially inter- significant cooling and crystallization, their rheology pretation is best made by examining terrestrial analogs. will mimic more evolved lavas [3]. But relatively Channel-fed aa, rubbly pahoehoe sheets, inflated pa- evolved compositions should be expected to cap the hoehoe, and lava tubes have now been observed and Martian shield volcanoes, just as evolved, alkalic lavas evidence for voluminous and widespread mafic pyro- cap the Hawaiian shield volcanoes [4]. Such lavas are clastics continues to mount. After these initial qualita- the natural products of a cooling mantle magma source tive interpretations are made, more quantitative mod- region or a crystallizing basaltic magma chamber. The eling can be effectively applied in future studies. presence of such lavas is not evidence for arc-type vol- Shield volcanoes: The five major shield volcanoes canism. are the most prominent volcanic features on Mars. While highly speculative at this point, the observa- Examination of ~200 MOC images of the Tharsis vol- tions to date suggest that the Martian shield volcanoes canoes, Olympus Mons, and Elysium Mons showed a may be dominantly basaltic but are capped by a layer terrain largely mantled by various types of cover. This of more evolved lavas. Moderate explosive activity is makes interpretation of the volcanic features challeng- usually associated with the eruption of such evolved ing. -
Geology and Mineralization of the Sierra Blanca Peaks, Hudspeth County, Texas W
New Mexico Geological Society Downloaded from: http://nmgs.nmt.edu/publications/guidebooks/31 Geology and mineralization of the Sierra Blanca Peaks, Hudspeth County, Texas W. N. McAnulty, 1980, pp. 263-266 in: Trans Pecos Region (West Texas), Dickerson, P. W.; Hoffer, J. M.; Callender, J. F.; [eds.], New Mexico Geological Society 31st Annual Fall Field Conference Guidebook, 308 p. This is one of many related papers that were included in the 1980 NMGS Fall Field Conference Guidebook. Annual NMGS Fall Field Conference Guidebooks Every fall since 1950, the New Mexico Geological Society (NMGS) has held an annual Fall Field Conference that explores some region of New Mexico (or surrounding states). Always well attended, these conferences provide a guidebook to participants. Besides detailed road logs, the guidebooks contain many well written, edited, and peer-reviewed geoscience papers. These books have set the national standard for geologic guidebooks and are an essential geologic reference for anyone working in or around New Mexico. Free Downloads NMGS has decided to make peer-reviewed papers from our Fall Field Conference guidebooks available for free download. Non-members will have access to guidebook papers two years after publication. Members have access to all papers. This is in keeping with our mission of promoting interest, research, and cooperation regarding geology in New Mexico. However, guidebook sales represent a significant proportion of our operating budget. Therefore, only research papers are available for download. Road logs, mini-papers, maps, stratigraphic charts, and other selected content are available only in the printed guidebooks. Copyright Information Publications of the New Mexico Geological Society, printed and electronic, are protected by the copyright laws of the United States. -
The Volcanic Ash Soils of Chile
' I EXPANDED PROGRAM OF TECHNICAL ASSISTANCE No. 2017 Report to the Government of CHILE THE VOLCANIC ASH SOILS OF CHILE FOOD AND AGRICULTURE ORGANIZATION OF THE UNITED NATIONS ROMEM965 -"'^ .Y--~ - -V^^-.. -r~ ' y Report No. 2017 Report CHT/TE/LA Scanned from original by ISRIC - World Soil Information, as ICSU World Data Centre for Soils. The purpose is to make a safe depository for endangered documents and to make the accrued information available for consultation, following Fair Use Guidelines. Every effort is taken to respect Copyright of the materials within the archives where the identification of the Copyright holder is clear and, where feasible, to contact the originators. For questions please contact [email protected] indicating the item reference number concerned. REPORT TO THE GOVERNMENT OP CHILE on THE VOLCANIC ASH SOILS OP CHILE Charles A. Wright POOL ANL AGRICULTURE ORGANIZATION OP THE UNITEL NATIONS ROME, 1965 266I7/C 51 iß - iii - TABLE OP CONTENTS Page INTRODUCTION 1 ACKNOWLEDGEMENTS 1 RECOMMENDATIONS 1 BACKGROUND INFORMATION 3 The nature and composition of volcanic landscapes 3 Vbloanio ash as a soil forming parent material 5 The distribution of voloanic ash soils in Chile 7 Nomenclature used in this report 11 A. ANDOSOLS OF CHILE» GENERAL CHARACTERISTICS, FORMATIVE ENVIRONMENT, AND MAIN KINDS OF SOIL 11 1. TRUMAO SOILS 11 General characteristics 11 The formative environment 13 ÈS (i) Climate 13 (ii) Topography 13 (iii) Parent materials 13 (iv) Natural plant cover 14 (o) The main kinds of trumao soils ' 14 2. NADI SOILS 16 General characteristics 16 The formative environment 16 tö (i) Climat* 16 (ii) Topograph? and parent materials 17 (iii) Natural plant cover 18 B. -
Chapter 2 Alaska’S Igneous Rocks
Chapter 2 Alaska’s Igneous Rocks Resources • Alaska Department of Natural Resources, 2010, Division of Geological and Geophysical Surveys, Alaska Geologic Materials Center website, accessed May 27, 2010, at http://www.dggs.dnr.state.ak.us/?link=gmc_overview&menu_link=gmc. • Alaska Resource Education: Alaska Resource Education website, accessed February 22, 2011, at http://www.akresource.org/. • Barton, K.E., Howell, D.G., and Vigil, J.F., 2003, The North America tapestry of time and terrain: U.S. Geological Survey Geologic Investigations Series I-2781, 1 sheet. (Also available at http://pubs.usgs.gov/imap/i2781/.) • Danaher, Hugh, 2006, Mineral identification project website, accessed May 27, 2010, at http://www.fremontica.com/minerals/. • Digital Library for Earth System Education, [n.d.], Find a resource—Bowens reaction series: Digital Library for Earth System Education website, accessed June 10, 2010, at http://www.dlese.org/library/query.do?q=Bowens%20reaction%20series&s=0. • Edwards, L.E., and Pojeta, J., Jr., 1997, Fossils, rocks, and time: U.S. Geological Survey website. (Available at http://pubs.usgs.gov/gip/fossils/contents.html.) • Garden Buildings Direct, 2010, Rocks and minerals: Garden Buildings Direct website, accessed June 4, 2010, at http://www.gardenbuildingsdirect.co.uk/Article/rocks-and- minerals. • Illinois State Museum, 2003, Geology online–GeoGallery: Illinois State Museum Society database, accessed May 27, 2010 at http://geologyonline.museum.state.il.us/geogallery/. • Knecht, Elizebeth, designer, Pearson, R.W., and Hermans, Majorie, eds., 1998, Alaska in maps—A thematic atlas: Alaska Geographic Society, 100 p. Lillie, R.J., 2005, Parks and plates—The geology of our National parks, monuments, and seashores: New York, W.W. -
Depth and Degree of Melting of Komatiites
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 97, NO. B4, PAGES 4521-4540, APRIL 10, 1992 Depth and Degree of Melting of Komatiites CLAUDE HERZBERG Departmentof GeologicalSciences, Rutgers University,New Brunswick,New Jersey Mineral PhysicsInstitute, State Universityof New York, StonyBrook, New York High pressuremelting experimentsßhove ." v .......... new constraintsto be placedon the depthand degreeof partial melting of komatiites. Komatiitesfrom GorgonaIsland were formed by relatively low degreesof pseudoinvariantmelting(< 30 %)involving L + O1 + Opx + Cpx + Gt on the solidusat 40 kbar, about 130 km depth. Munro-typekomatiites were separatedfrom a harzburgiteresidue (L + O1 + Opx) at pressuresthat are poorly constrained,but were probablyaround 50 kbar, about 165 km depth;the degreeof partial melting was <40%. Komatiites from the BarbertonMountain Land were formed by high degrees(-50 %) of pseudoinvariantmelting (L + O1 + Gt + Cpx) of fertile mantleperidotitc in the 80- to 100-kbarrange, about 260- to 330- km depth. Secularvariations in the geochemistryof komatiitescould have formed in response to a reductionin the temperatureand pressureof meltingwith time. The 3.5 Ga Barbertonkomatiites and the 2.7 Ga Munro-typekomatiites could have formedin plumesthat were hotterthan the present-daymantle by 500ø and 30(Y',respectively. When excesstemperatures are this size, melting is deeperand volcanismchanges from basalticto komatiitic. The komatiitesfrom Gorgona Island, which are Mesozoic in age, may be representativeof komatiitesthat are predictedto occur in oceanicplateaus of Cretaceousage throughoutthe Pacific [Storey et al., 1991]. 1. INTRODUCTION range of CaO and A1203contents in the 80- to 160-kbar range. A calibration has been made of the effect of pressure on Komatiites are high MgO volcanic rocks that can be CaO/(CaO + A1203)and MgO in komatiiticliquids formed on roughly explained by high degrees of melting of mantle the solidus, and an examinationhas been made of the effect of peridotitc,typically 50 to 100 % [e.g., Vi.ljoenand Vi.ljoen, FeO. -
The Science Behind Volcanoes
The Science Behind Volcanoes A volcano is an opening, or rupture, in a planet's surface or crust, which allows hot magma, volcanic ash and gases to escape from the magma chamber below the surface. Volcanoes are generally found where tectonic plates are diverging or converging. A mid-oceanic ridge, for example the Mid-Atlantic Ridge, has examples of volcanoes caused by divergent tectonic plates pulling apart; the Pacific Ring of Fire has examples of volcanoes caused by convergent tectonic plates coming together. By contrast, volcanoes are usually not created where two tectonic plates slide past one another. Volcanoes can also form where there is stretching and thinning of the Earth's crust in the interiors of plates, e.g., in the East African Rift, the Wells Gray-Clearwater volcanic field and the Rio Grande Rift in North America. This type of volcanism falls under the umbrella of "Plate hypothesis" volcanism. Volcanism away from plate boundaries has also been explained as mantle plumes. These so- called "hotspots", for example Hawaii, are postulated to arise from upwelling diapirs with magma from the core–mantle boundary, 3,000 km deep in the Earth. Erupting volcanoes can pose many hazards, not only in the immediate vicinity of the eruption. Volcanic ash can be a threat to aircraft, in particular those with jet engines where ash particles can be melted by the high operating temperature. Large eruptions can affect temperature as ash and droplets of sulfuric acid obscure the sun and cool the Earth's lower atmosphere or troposphere; however, they also absorb heat radiated up from the Earth, thereby warming the stratosphere. -
Lecture 8: Volcanism
Lecture 8: Volcanism EAS 2200 Introduction to the Earth System Today’s Plan Introduction Melting in the Earth mid-ocean ridges subduction zones mantle plumes Crystallization of igneous rocks Volcanic eruptions Introduction Volcanic eruptions are among the most spectacular natural phenomena. Where does the magma come from? Why does most volcanism occur only in certain areas? What causes eruptions to sometimes be catastrophic and sometimes quiescent? Why is there such a variety of igneous rocks? Where does magma come from? Early ideas: Hot vapors produce melting Burning coals layers provide heat for melting Global layer of molten rock at depth Modern ideas: Decompression melting Flux melting Intrusions of magma into the crust (but this begs the question of the origin of the original magma). Deep burial of low melting point material (rare). Melting of Rock Complex (“multi-phase”) substances progressively melt over a range of temperatures. The lowest temperature at which melt exists (temperature at which melting begins) is known as the solidus. The highest temperature at which solid persists (temperature at which melting is complete) is known as the liquidus. The melting range for most rocks (diference in solidus and liquidus) is several hundred degrees C. In essentially all cases, melting in the Earth is believed to be partial (i.e., liquidus temperature Volcanoes are like Clouds Decompression Melting Solidus temperature of rock decreases with decreasing pressure. Temperature of rising mantle rock also decreases with pressure (adiabatic decompression). Adiabat is steeper than solidus, so that rising mantle rock eventually reaches solidus and Melting and Mantle Convection We can expect melting to occur within hot, rising mantle convection cells. -
Depth of Differentiation Under Osorno Volcano (Chile)
Depth of differentiation under Osorno volcano (Chile) T.Bechona, J. Vander Auweraa, O. Namurb, P. Fugmanna, O. Bollea, L. Larac aUniversity of Liège – Department of Geology bUniversity of Leuven – Department of Earth and Environmental Sciences cSERNAGEOMIN Introduction What is the depth of the magma chamber at Osorno volcanoCredit ? : H. Foucart It matters for : • Understanding differentiation in young arcs. Estimations evidence the major role of arc magmatism in the construction of continental crust (up to 60% : Rudnick and Gao, 2003). • Monitoring a major flank collapse like the one of Mt St Helens in 1980s (USA) 2 Introduction ↑ Ryan et al. (2009) Modified Credit : H. Foucart 3 ↑ After Stern et al 2007, modified by P. Fugmann Method T°C and P (kbar) of last Lee et al 2009 equilibration with mantle Assuming H2O (1%) Assuming P (0-5kbar) and H2O (0-5%) • Whole rock major elements: XRF Putirka 2008 T°C: Wan et al 2007 • Minerals major Coogan et al 2014 elements: microprobe Harrisson et Watson 1984 Depth P (kbar): Putirka 2008 Tassara et Echaurren Neave et Putirka 2017 (km): 2012 Assuming H2O 4 Results Trachy- Trachyte Basaltic- Andesite Trachy- Andesite Trachy- Basalts Basaltic- Basalts Andesites Dacites Andesites 5 Results Trachy- Trachyte Basaltic- Andesite Trachy- Andesite In addition : • Magma compositions results from fractional crystallization (mass balance model +traceTrachy elements- diagrams) Basalts • Dominant mineral phases : Ol + Plag in mafic rocks • Rather low water content (No hydrated phases except in one dacite) Basaltic- Basalts Andesites Dacites Andesites 6 Results ↑ Putirka (2008) 7 Results T°C and P° 8 Discussion P° (kbar) H2O (%wt) 9 ↓ Seismic data from SERNAGEOMIN surveillance (Chile) Discussion W E Sea level 1 Kbar 2 Kbar 3 Kbar 10 Discussion 1-3 Kbar Using crustal model of Tassara and Magma chamber Echaurren (2012) ←↓ P° ~ 11-12 Kbar Last peridotite equilibrium T°C~ 1335°C 11 Discussion N S Crustal 2 disc. -
Three-Dimensional Magmatic Architecture of a Buried Shield Volcano
https://doi.org/10.1130/G47941.1 Manuscript received 22 January 2020 Revised manuscript received 24 August 2020 Manuscript accepted 29 August 2020 © 2020 The Authors. Gold Open Access: This paper is published under the terms of the CC-BY license. Published online 12 October 2020 Inside the volcano: Three-dimensional magmatic architecture of a buried shield volcano Faye Walker1*, Nick Schofield1, John Millett1,2, Dave Jolley1, Simon Holford3, Sverre Planke2,4, Dougal A. Jerram4,5 and Reidun Myklebust6 1 Geology and Petroleum Geology, University of Aberdeen, Aberdeen AB24 3UE, UK 2 Volcanic Basin Petroleum Research, Blindernveien 5, N-0361 Oslo, Norway 3 Australian School of Petroleum, University of Adelaide, Adelaide, South Australia 5000, Australia 4 Centre for Earth Evolution and Dynamics (CEED), University of Oslo, N-0315 Oslo, Norway 5 DougalEARTH Ltd., Solihull B91 3NU, UK 6 TGS, Asker N-1386, Norway ABSTRACT its magma chamber have never been imaged in The nature and growth of magmatic plumbing systems are of fundamental importance detail before. to igneous geology. Traditionally, magma chambers have been viewed as rapidly emplaced Magma chambers have traditionally been bodies of molten rock or partially crystallized “magma mush” connected to the surface viewed as large, long-lived, geometrically sim- by a narrow cylindrical conduit (referred to as the “balloon-and-straw” model). Recent ple bodies of molten rock, which are emplaced data suggest, however, that magma chambers beneath volcanoes are formed incrementally rapidly and slowly crystallize to form plutons through amalgamation of smaller intrusions. Here we present the first high-resolution three- (Glazner et al., 2004; Annen et al., 2015; Jerram dimensional reconstruction of an ancient volcanic plumbing system as a large laccolithic and Bryan, 2018; Sparks et al., 2019). -
Igneous Activity and Volcanism Homework
DATE DUE: Name: Ms. Terry J. Boroughs Geology 300 Section: IGNEOUS ROCKS AND IGNEOUS ACTIVITY Instructions: Read each question carefully before selecting the BEST answer. Use GEOLOGIC vocabulary where applicable! Provide concise, but detailed answers to essay and fill-in questions. TURN IN YOUR 882 –ES SCANTRON AND ANSWER SHEET ONLY! MULTIPLE CHOICE QUESTIONS: 1. Gabbro and Granite a. Have a similar mineral composition b. Have a similar texture c. Answers A. and B. d. Are in no way similar 2. Which of the factors listed below affects the melting point of rock and sediment? a. Composition of the material d. Water content b. The confining pressure e. All of the these c. Only composition of the material and the confining pressure 3. Select the fine grained (aphanitic) rock, which is composed mainly of sodium-rich plagioclase feldspar, amphibole, and biotite mica from the list below: a. Basalt b. Andesite c. Granite d. Diorite e. Gabbro 4. __________ is characterized by extremely coarse mineral grains (larger than 1-inch)? a. Pumice b. Obsidian c. Granite d. Pegmatite 5. Basalt exhibits this texture. a. Aphanitic b. Glassy c. Porphyritic d. Phaneritic e. Pyroclastic 6. Rocks that contain crystals that are roughly equal in size and can be identified with the naked eye and don’t require the aid of a microscope, exhibits this texture: a. Aphanitic b. Glassy c. Porphyritic d. Phaneritic e. Pyroclastic 7. The texture of an igneous rock a. Is controlled by the composition of magma. b. Is the shape of the rock body c. Determines the color of the rock d. -
3D Seismic Imaging of the Shallow Plumbing System Beneath the Ben Nevis 2 Monogenetic Volcanic Field: Faroe-Shetland Basin 3 Charlotte E
ArticleView metadata, text citation and similar papers at core.ac.uk Click here to download Article text Ben Nevis Paperbrought to you by CORE MASTER.docx provided by Aberdeen University Research Archive Plumbing systems of monogenetic edifices 1 3D seismic imaging of the shallow plumbing system beneath the Ben Nevis 2 Monogenetic Volcanic Field: Faroe-Shetland Basin 3 Charlotte E. McLean1*; Nick Schofield2; David J. Brown1, David W. Jolley2, Alexander Reid3 4 1School of Geographical and Earth Sciences, Gregory Building, University of Glasgow, G12 8QQ, UK 5 2Department of Geology and Petroleum Geology, University of Aberdeen AB24 3UE, UK 6 3Statoil (U.K.) Limited, One Kingdom Street, London, W2 6BD, UK 7 *Correspondence ([email protected]) 8 Abstract 9 Reflective seismic data allows for the 3D imaging of monogenetic edifices and their 10 corresponding plumbing systems. This is a powerful tool in understanding how monogenetic 11 volcanoes are fed and how pre-existing crustal structures can act as the primary influence 12 on their spatial and temporal distribution. This study examines the structure and lithology of 13 host-rock as an influence on edifice alignment and provides insight into the structure of 14 shallow, sub-volcanic monogenetic plumbing systems. The anticlinal Ben Nevis Structure 15 (BNS), located in the northerly extent of the Faroe-Shetland Basin, NE Atlantic Margin, was 16 uplifted during the Late Cretaceous and Early Palaeocene by the emplacement of a laccolith 17 and a series of branching sills fed by a central conduit. Seismic data reveals multiple 18 intrusions migrated up the flanks of the BNS after its formation, approximately 58.4 Ma 19 (Kettla-equivalent), and fed a series of scoria cones and submarine volcanic cones.