DOCSLIB.ORG

Shield Volcano

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Shield Volcano Frank Press • Raymond Siever • John Grotzinger • Thomas H. Jordan Understanding Earth Fourth Edition Chapter 6: Volcanism Lecture Slides prepared by Bill Dupré • Peter Copeland Copyright © 2004 by W. H. Freeman & Company 4. …accumulating on the surface to form a Types of Lavas volcano. • Basaltic lavas: low-viscosity mafic lavas, 3. Lavas erupt from typically erupted at 1000o to 1200o C; cool to the magma chamber form basalt. through central and side vents… • Rhyolitic lavas: high-viscosity felsic lavas, typically erupted at 800o to 1200o C; cool to 2. …rises through the lithosphere to form a form rhyolite. magma chamber • Andesitic lavas: intermediate in composition 1. Magma, which and viscosity between mafic and felsic originates in the magmas; cool to form andesite. partially melted Fig. 6.1 asthenosphere… Flood Basalts of the Columbia Plateau Types of Basalts • Flood Basalts: thick, widespread accumulations of basalt, typically fed by fissures • Pahoehoe: a very low viscosity basaltic lava characterized by a ropy texture • Aa: a relatively low viscosity basaltic lava characterized by a jagged, blocky texture • Pillow Basalts: a basaltic lava extruded beneath the water, characterized by glassy pillows filled with crystalline basalt Fig. 6.2 Vesicular Basalt: trapped gases form bubbles (vesicles) Fig. 6.3 Fig. 6.4 Pyroclastic Volcanic Bomb Material: Fragmentary volcanic rocks ejected into the air Fig. 6.5 Fig. 6.6 Volcanic Features Formed by Pyroclastic Flows: Central Eruptions A density flow consisting • Shield Volcanoes of a hot (up to 800o C), • Volcanic domes poisonous mixture of gas and pyroclastic material • Cinder-cones Volcanoes moving downslope at • Composite Volcanoes speed in excess of 200 • Craters km/hr! • Calderas Fig. 6.8 Eruptive Styles and Landforms Mauna Kea Shield Volcano Volcanic Dome Mauna Loa Cinder Cone Volcano Composite Volcano Crater Caldera Fig. 6.9 Fig.6.9.a Shield Volcano Lava Dome Fig. 6.9b Fig.6.9.a Lyn Topinka/USGS Volcanic Dome Cerro Negro Cinder Cone, near Managua, Nicaragua in 1968 Fig. 6.9b Mark Hurd Aerial Surveys Fig. 6.9c Cinder Cone Mt Fujiyama, Japan Fig. 6.9c Raga/The Stock Market Fig. 5.15 Caldera Stages in the Development of Crater Lake Fig. 6.10 Shiprock, Formation of a Diatreme New Mexico Fig. 6.12 Fig. 6.12 Fissure Eruptions Volcanoes along the Laki Fissure A volcanic eruption originating (Iceland) formed in 1783, resulting along an elongate fissure rather in the largest lava than a central vent. flow in recorded history Fig. 6.13 Mt. St. Helens: Before Mt. St. Helens: During Hydrothermal Activity: • The circulation of water through hot Sulfur-encrusted Fumarole volcanic rocks and magma •Forms fumaroles – volcanic vents emitting gases, some charged with dissolved minerals •Forms geysers – heated hydrothermal waters under pressure, that intermittently erupts at the surface • Provides the source for Geothermal Energy. Fig. 6.16 Volcanism Associated with Plate Tectonics Fig. 6.19 Fig. 6.20.
Load more

Recommended publications
  • Geologic Map of the Long Valley Caldera, Mono-Inyo Craters
    DEPARTMENT OF THE INTERIOR TO ACCOMPANY MAP 1-1933 US. GEOLOGICAL SURVEY GEOLOGIC MAP OF LONG VALLEY CALDERA, MONO-INYO CRATERS VOLCANIC CHAIN, AND VICINITY, EASTERN CALIFORNIA By Roy A. Bailey GEOLOGIC SETTING VOLCANISM Long Valley caldera and the Mono-Inyo Craters Long Valley caldera volcanic chain compose a late Tertiary to Quaternary Volcanism in the Long Valley area (Bailey and others, volcanic complex on the west edge of the Basin and 1976; Bailey, 1982b) began about 3.6 Ma with Range Province at the base of the Sierra Nevada frontal widespread eruption of trachybasaltic-trachyandesitic fault escarpment. The caldera, an east-west-elongate, lavas on a moderately well dissected upland surface oval depression 17 by 32 km, is located just northwest (Huber, 1981).Erosional remnants of these mafic lavas of the northern end of the Owens Valley rift and forms are scattered over a 4,000-km2 area extending from the a reentrant or offset in the Sierran escarpment, Adobe Hills (5-10 km notheast of the map area), commonly referred to as the "Mammoth embayment.'? around the periphery of Long Valley caldera, and The Mono-Inyo Craters volcanic chain forms a north- southwestward into the High Sierra. Although these trending zone of volcanic vents extending 45 km from lavas never formed a continuous cover over this region, the west moat of the caldera to Mono Lake. The their wide distribution suggests an extensive mantle prevolcanic basement in the area is mainly Mesozoic source for these initial mafic eruptions. Between 3.0 granitic rock of the Sierra Nevada batholith and and 2.5 Ma quartz-latite domes and flows erupted near Paleozoic metasedimentary and Mesozoic metavolcanic the north and northwest rims of the present caldera, at rocks of the Mount Morrisen, Gull Lake, and Ritter and near Bald Mountain and on San Joaquin Ridge Range roof pendants (map A).
    [Show full text]
  • Volcanic Gases and Aerosols Guidelines Introduction
    IVHHN Gas Guidelines www.ivhhn.org/gas/guidelines.html Volcanic Gases and Aerosols Guidelines The following pages contain information relating to the health hazards of gases and aerosols typically emitted during volcanic activity. Each section outlines the properties of the emission; its impacts on health; international guidelines for concentrations; and examples of concentrations and effects in volcanic contexts, including casualties. Before looking at the emissions data, we recommend that you read the general introduction to volcanic gases and aerosols first. A glossary to some of the terms used in the explanations and guidelines is also provided at the end of this document. Introduction An introduction to the aims and purpose of the Gas and Aerosol Guidelines is given here, as well as further information on international guideline levels and the units used in the website. A brief review of safety procedures currently implemented by volcanologists and volcano observatories is also provided. General Introduction Gas and aerosol hazards are associated with all volcanic activity, from diffuse soil gas emissions to 2- plinian eruptions. The volcanic emissions of most concern are SO2, HF, sulphate (SO4 ), CO2, HCl and H2S, although, there are other volcanic volatile species that may have human health implications, including mercury and other metals. Since 1900, there have been at least 62 serious volcanic-gas related incidents. Of these, the gas-outburst at Lake Nyos in 1986 was the most disastrous, causing 1746 deaths, >845 injuries and the evacuation of 4430 people. Other volcanic-gas related incidents have been responsible for more than 280 deaths and 1120 injuries, and contributed to the evacuation or ill health of >53,700 people (Witham, in review).
    [Show full text]
  • Geologic Storage Formation Classification: Understanding Its Importance and Impacts on CCS Opportunities in the United States
    BEST PRACTICES for: Geologic Storage Formation Classification: Understanding Its Importance and Impacts on CCS Opportunities in the United States First Edition Disclaimer This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference therein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof. The views and opinions of authors expressed therein do not necessarily state or reflect those of the United States Government or any agency thereof. Cover Photos—Credits for images shown on the cover are noted with the corresponding figures within this document. Geologic Storage Formation Classification: Understanding Its Importance and Impacts on CCS Opportunities in the United States September 2010 National Energy Technology Laboratory www.netl.doe.gov DOE/NETL-2010/1420 Table of Contents Table of Contents 5 Table of Contents Executive Summary ____________________________________________________________________________ 10 1.0 Introduction and Background
    [Show full text]
  • 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.
    [Show full text]
  • Satellite Observations of Fumarole Activity at Aluto Volcano, Ethiopia: Implications for Geothermal Monitoring and Volcanic Hazard
    Accepted Manuscript Satellite observations of fumarole activity at Aluto volcano, Ethiopia: Implications for geothermal monitoring and volcanic hazard Mathilde Braddock, Juliet Biggs, Iain M. Watson, William Hutchison, David M. Pyle, Tamsin A. Mather PII: S0377-0273(17)30118-X DOI: doi: 10.1016/j.jvolgeores.2017.05.006 Reference: VOLGEO 6091 To appear in: Journal of Volcanology and Geothermal Research Received date: 24 February 2017 Revised date: 6 May 2017 Accepted date: 7 May 2017 Please cite this article as: Mathilde Braddock, Juliet Biggs, Iain M. Watson, William Hutchison, David M. Pyle, Tamsin A. Mather , Satellite observations of fumarole activity at Aluto volcano, Ethiopia: Implications for geothermal monitoring and volcanic hazard, Journal of Volcanology and Geothermal Research (2017), doi: 10.1016/ j.jvolgeores.2017.05.006 This is a PDF file of an unedited manuscript that has been accepted for publication. As a service to our customers we are providing this early version of the manuscript. The manuscript will undergo copyediting, typesetting, and review of the resulting proof before it is published in its final form. Please note that during the production process errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain. ACCEPTED MANUSCRIPT Satellite observations of fumarole activity at Aluto volcano, Ethiopia: implications for geothermal monitoring and volcanic hazard Mathilde Braddock1*, Juliet Biggs2, Iain M. Watson2, William Hutchison3, David M. Pyle4 and Tamsin A. Mather4 1 School of Earth Sciences, University of Bristol, Wills Memorial Building, Queens Road, Bristol BS8 1RJ, UK 2 COMET, School of Earth Sciences, University of Bristol, Wills Memorial Building, Queens Road, Bristol BS8 1RJ, UK 3 School of Earth and Environmental Sciences, University of St.
    [Show full text]
  • Geothermal Springs, Geysers and Fumaroles
    Sciences Secondary volcanic activities: Geothermal springs, Geysers and Fumaroles Geothermal Springs A geothermal (or hydrothermal) spring is produced by the emergence of geothermally heated groundwater from the Earth's crust. There are geothermal springs in many locations all over the crust of the earth. Geothermal Springs Surface water percolates downward through the rocks below the Earth's surface to high-temperature regions surrounding a magma chamber, either active or recently solidified but still hot. When the water is heated, becomes less dense, and rises Surface water back to the surface along fissures and cracks. Sometimes these features are called "dying volcanoes" because they seem to represent the last stage of volcanic activity as the magma, in depth, cools and hardens. Water percolation Heated water rises up The temperature of hot springs depends on factors such as: •the rate at which water circulates through the underground channels Hot rocks •the amount of heat at depth •the dilution of the heated water by cool ground water near the surface. Geothermal Springs The water issuing from a hot spring is heated by geothermal heat from the Earth's astenosphere. In general, the temperature of rocks increases with depth. The rate of temperature increase is known as the geothermal gradient (it is about 25°C per km). If water percolates deeply enough into the crust, it will be heated as it comes into contact with hot rocks. Warm springs are sometimes the result of hot and cold springs mixing but may also occur outside of volcanic areas. Geysers Geyser are located near active volcanic areas, and the geyser effect is due to the proximity of magma.
    [Show full text]
  • Insights from Fumarole Gas Geochemistry on the Recent Volcanic Unrest of Pico Do Fogo, Cape Verde
    ORIGINAL RESEARCH published: 15 July 2021 doi: 10.3389/feart.2021.631190 Insights from Fumarole Gas Geochemistry on the Recent Volcanic Unrest of Pico do Fogo, Cape Verde Gladys V. Melián 1,2,3*, Pedro A. Hernández 1,2,3, Nemesio M. Pérez 1,2,3, María Asensio-Ramos 1, Eleazar Padrón 1,2,3, Mar Alonso 1,2, Germán D. Padilla 1,2, José Barrancos 1,2, Francesco Sortino 4, Hirochicka Sumino 5, Fátima Rodríguez 1, Cecilia Amonte 1, Sonia Silva 6, Nadir Cardoso 6 and José M. Pereira 7 1Instituto Volcanológico de Canarias (INVOLCAN), La Laguna, Spain, 2Instituto Tecnológico y de Energías Renovables (ITER), Granadilla de Abona, Spain, 3Agencia Insular de la Energía de Tenerife (AIET), Granadilla de Abona, Spain, 4Istituto Nazionale di Geofisica e Vulcanologia - Sezione Roma 2, Roma, Italy, 5Department of General Systems Studies, Graduate School of Arts and Sciences, The University of Tokyo, Komaba, Meguro-ku, Japan, 6Universidade de Cabo Verde (UNICV), Praia, Cape Verde, 7Laboratório de Engenharia Civil of Cape Verde (LEC) Tira - Chapéu, Praia, Cape Verde Edited by: We report the results of the geochemical monitoring of the fumarolic discharges at the Pico Francesco Italiano, do Fogo volcano in Cape Verde from 2007 to 2016. During this period Pico do Fogo National Institute of Geophysics and Volcanology, Italy experienced a volcanic eruption (November 23, 2014) that lasted 77 days, from a new vent Reviewed by: ∼2.5 km from the fumaroles. Two fumaroles were sampled, a low (F1∼100°C) and a Pierpaolo Zuddas, medium (F2∼300°C) temperature. The variations observed in the δ18O and δ2H in F1 and Sorbonne Universités, France F2 suggest different fluid source contributions and/or fractionation processes.
    [Show full text]
  • VOLCANO-TECTONIC HISTORY of CRATER FLAT, SOUTHWESTERN NEVADA, AS SUGGESTED by NEW EVIDENCE from DRILL HOLE USW-VH-1 and VICINITY By
    5)zt.-t"o En-, 6-.-5 f %. _rc . i%: .- 1 - . ~~Open-File Report 82-457 n-File Report 82-457 (.8X/1<~~/I I W II ~~~~~~~~~~~~~~i UNITED STATES V DEPARTMENT OF THE INTERIOR GEOLOGICAL SURVEY VOLCANO-TECTONIC HISTORY OF CRATER FLAT. SOUTHWESTERN NEVADA, AS SUGGESTED BY NEW EVIDENCE FROM DRILL HOLE USW-VH-1 AND VICINITY Open-File Report 82-457 1982 This report is preliminary and has not been reviewed for conformity with U.S. Geological Survey editorial standards. X 0 X 0 0- 0 Prepared by the U.S. Geological Survey C- for the 3 z Nevada Operations Office -4i U.S. Department of Energy z (Memorandum of Understanding DE-AI08-78ET44802) U, I.- -4 Copies of this Open-file Report may be purchased from Open-File Services Section Branch of Distribution U.S. Geological Survey Box 25425, Federal Center Denver, Colorado 80225 PREPAYMENT IS REQUIRED Price information will be published in the monthly listing RNew Publications of the Geological Surveys FOR ADDITIONAL IXNFORAATION CALL: Commercial: (303)234-5888 FTS: 234-5888 Open-File Report 82-457 Open-File Report 82-457 UNITED STATES DEPARTMENT OF THE INTERIOR GEOLOGICAL SURVEY VOLCANO-TECTONIC HISTORY OF CRATER FLAT, SOUTHWESTERN NEVADA, AS SUGGESTED BY NEW EVIDENCE FROM DRILL HOLE USW-VH-1 AND VICINITY By W. J. Carr CONTENTS Page Abstract... ....... .......... ............................... .........................a.. ............1 Introduction,............................................................ 1 Acknowledgments............................................... ...... ........ 3 Drill-hole location and history..................................... 3 Geologic framework of Crater Flat ...................................6 Aeromagnetic anomalies........................ oo..... ... .......... ..................7 Volcano-tectonic history of Crater Flat ....o........o .................. 9 Lithology of drill hole.'.. ............................. o..................... 12 Structural properties of the core..
    [Show full text]
  • Source to Surface Model of Monogenetic Volcanism: a Critical Review
    Downloaded from http://sp.lyellcollection.org/ by guest on September 28, 2021 Source to surface model of monogenetic volcanism: a critical review I. E. M. SMITH1 &K.NE´ METH2* 1School of Environment, University of Auckland, Auckland, New Zealand 2Volcanic Risk Solutions, Massey University, Palmerston North 4442, New Zealand *Correspondence: [email protected] Abstract: Small-scale volcanic systems are the most widespread type of volcanism on Earth and occur in all of the main tectonic settings. Most commonly, these systems erupt basaltic magmas within a wide compositional range from strongly silica undersaturated to saturated and oversatu- rated; less commonly, the spectrum includes more siliceous compositions. Small-scale volcanic systems are commonly monogenetic in the sense that they are represented at the Earth’s surface by fields of small volcanoes, each the product of a temporally restricted eruption of a composition- ally distinct batch of magma, and this is in contrast to polygenetic systems characterized by rela- tively large edifices built by multiple eruptions over longer periods of time involving magmas with diverse origins. Eruption styles of small-scale volcanoes range from pyroclastic to effusive, and are strongly controlled by the relative influence of the characteristics of the magmatic system and the surface environment. Gold Open Access: This article is published under the terms of the CC-BY 3.0 license. Small-scale basaltic magmatic systems characteris- hazards associated with eruptions, and this is tically occur at the Earth’s surface as fields of small particularly true where volcanic fields are in close monogenetic volcanoes. These volcanoes are the proximity to population centres.
    [Show full text]
  • A Unique Volcanic Field in Tharsis, Mars: Monogenetic Cinder Cones and Lava Flows As Evidence for Hawaiian Eruptions
    42nd Lunar and Planetary Science Conference (2011) 1379.pdf A UNIQUE VOLCANIC FIELD IN THARSIS, MARS: MONOGENETIC CINDER CONES AND LAVA FLOWS AS EVIDENCE FOR HAWAIIAN ERUPTIONS. P. Brož1 and E. Hauber2, 1Institute of Geophysics ASCR, v.v.i., Prague, Czech Republic, [email protected], 2Institut für Planetenforschung, DLR, Berlin, Germany, [email protected]. Introduction: Most volcanoes on Mars that have Data: We use images from several cameras, i.e. been studied so far seem to be basaltic shield volca- Context Camera (CTX), High Resolution Stereo Cam- noes, which can be very large with diameters of hun- era (HRSC), and High Resolution Imaging Science dreds of kilometers [e.g., 1] or much smaller with di- Experiment (HiRISE) for morphological analyses. ameters of several kilometers only [2]. Few Viking Topographic information (e.g., heights and slope an- Orbiter-based studies reported the possible existence gles) were determined from single shots of the Mars of cinder cones [3,4] or stratovolcanoes [5-7], and only Orbiter Laser Altimeter (MOLA) in a GIS environ- the advent of higher-resolution data led to the tentative ment, and from stereo images (HRSC, CTX) and de- interpretation of previously unknown edifices as cinder rived gridded digital elevation models (DEM). cones [8] or rootless cones [9]. The identification of Morphometry: For comparison between the cinder cones can constrain the nature of eruption proc- cones and terrestrial morphological analogues (i.e. esses and, indirectly, our understanding of the nature cinder cones [10]) we determined some basic mor- of parent magmas (e.g., volatile content). Here we re- phometric properties and their ratios (e.g., crater di- port on our observation of a unique cluster of possible ameter [WCR] vs.
    [Show full text]
  • 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.
    [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]