Geos 432-4 Volcanic Landforms

Total Page:16

File Type:pdf, Size:1020Kb

Geos 432-4 Volcanic Landforms GEOS 432-4; Volcanic processes and landforms Plate Tectonics and Volcanism Mantle hot spots Oceanic Basaltic Continental Rhyolitic, andesitic, or basaltic Plate tectonics and Volcanism Plate margins Divergent-basaltic Subduction of oceanic plate-andesite 1 Large scale landforms Submarine volcanoes Large scale landforms Basalt plateaus Volcanic Products Gas Lava Tephra 2 Gas Vents Hot springs, geysers, fumaroles, solfataras Hot springs Solfatara, Iceland Geyser, ―Strokkur‖ at Geysir, Iceland 3 1 2 3 4 Mud volcano http://ngm.nationalgeographic.com/ngm/20 08-01/volcano-culture/drowning-in- mud.html 4 Lake Nyos case history http://perso.wanadoo.fr/mhalb/nyos/index.htm Lava Composition Silica content: 35% (basalt) – 75% (rhyolite, obsidian) Viscosity Related to composition-higher silica—more viscous Temp and volatile content also important Volatiles decrease viscosity but degas at surface Basalt 1100-1200 degrees C Lava flows Vesicles AA Aaflow, lava Iceland Pahoehoe lava Aa lava flow 5 Rhylolite/obsidian flow Obsidian Columnar jointing 6 Pillow lavas Tephra Ash—sand size & smaller Lapilli—gravel Blocks (Cold) Bombs (warm) Pumice, 1875 eruption of Askja, Iceland 1875 Snow exposed 7 Pyroclastic eruptions Heimaey, Iceland, 1973 2010 Eruption: Eyjafyallajökull http://www.youtube.com/watch?v=f1ztg0wUqKY Pyroclastic flow or surge High temperature, very fast, very destructive 8 Mt. Pelee, 1902 Town of St. Pierre, Carribean Island of Martinique 30,000 killed Mt. St. Helens, 1980 Lateral Blast Debris flows, Mt. St. Helens 9 Mt St. Helens Lahars Orting, Washington Mt. Rainier Mt. Shasta 10 Armero, Nevado del Ruiz, 1985 23,000 people killed Volcanic landforms ShieldShield volcano volcano Shield volcano L Lava flow Exogenous dome a v a Scoria cone ScoriaScoria cone cone Scoria Scoria cone cone Tuff ring Endogenous dome Ruptured ED Composite (strato) volcano Explosion caldera Maars with tephra Maar with rampart Collapse caldera Gas maar Explosion crater 11 Lava flows—fissure or central vent Young lava flow, Iceland Fissures, Iceland Iceland Lava Cascade, Iceland Fissure, Craters of the Moon 12 Basalt flow Craters of the Moon Miocene basalt flows from fissures- Columbia River Plateau Exogenous domes Spatter cone-Iceland Shield Volcano-Iceland Mauna Loa, as seen from Kilauea Mauna Loa from Kilauea 13 Pyroclastic cones, rings Tuff ring, northern Iceland Scoria cone Tuff cone 14 Tuff Ring, Iceland Lake Myvatn, Iceland 15 Endogenous domes Mt. St. Helens Composite (strato) volcanoes 16 Mt. Fuji Craters, calderas Maar, New Mexico Crater Lake 17 Halemaumau pit crater Summit caldera, Askja Volcano, Iceland Santorini, Greece 18 Miscellaneous IcelandicIcelandic Table Table Mountain Mountain -Tuya Tuya, Iceland Miscellaneous con’t Lava tube Tumuli Volcanic neck Tree mold 19 .
Recommended publications
  • Mud Volcano Eruptions and Earthquakes in the Northern Apennines and Sicily, Italy
    Tectonophysics 474 (2009) 723–735 Contents lists available at ScienceDirect Tectonophysics journal homepage: www.elsevier.com/locate/tecto Mud volcano eruptions and earthquakes in the Northern Apennines and Sicily, Italy Marco Bonini Consiglio Nazionale delle Ricerche, Istituto di Geoscienze e Georisorse, Via G. La Pira 4, I-50121 Florence, Italy article info abstract Article history: The relations between earthquakes and the eruption of mud volcanoes have been investigated at the Pede–Apennine Received 28 November 2008 margin of the Northern Apennines and in Sicily. Some of these volcanoes experiencederuptionsorincreased Received in revised form 1 April 2009 activity in connection with historical seismic events, showing a good correlation with established thresholds of Accepted 20 May 2009 hydrological response (liquefaction) to earthquakes. However, the majority of eruptions have been documented to Available online 25 May 2009 be independent of seismic activity, being mud volcanoes often not activated even when the earthquakes were of suitable magnitude and the epicentre at the proper distance for the triggering. This behaviour suggests that Keywords: fi fl Mud volcanoes paroxysmal activity of mud volcanoes depends upon the reaching of a speci c critical state dictated by internal uid Vents pressure, and implies that the strain caused by the passage of seismic waves can activate only mud volcanoes in near- Earthquakes critical conditions (i.e., close to the eruption). Seismogenic faults, such as the Pede–Apennine thrust, often Eruptions structurally control the fluid reservoirs of mud volcanoes, which are frequently located at the core of thrust-related Northern Apennines folds. Such an intimate link enables mud volcanoes to represent features potentially suitable for recording Sicily perturbations associated with the past and ongoing tectonic activity of the controlling fault system.
    [Show full text]
  • Response of Mud Volcanoes to Earthquakes: Role of Static Strains and Frequency-Dependence of Ground Motion
    IAVCEI 2013 Scientific Assembly - July 20 - 24, Kagoshima, Japan Forecasting Volcanic Activity - Reading and translating the messages of nature for society 1P2_2B-O1 Room A3 Date/Time: July 21 17:00-17:15 Response of mud volcanoes to earthquakes: role of static strains and frequency-dependence of ground motion Michael Manga1, Maxwell Rudolph2, Marco Bonini3 1University of California, Berkeley, USA, 2University of Colorado, Boulder, USA, 3Consiglio Nazionale delle Ricerche, Florence, Italy E-mail: [email protected] Distant earthquakes can trigger the eruption of mud volcanoes. We report observations of the response of the Davis-Schrimpf, California, mud volcanoes to 2 earthquakes and non-response to 4 other earthquakes. We find that eruptions are triggered by dynamic stresses and that the mud volcanoes are more sensitive to long period seismic waves than short period waves with the same amplitude. These observations are consistent with models in which fluid mobility is enhanced by dislodging bubbles by the time-varying flows produced by seismic waves. In the Northern Apennines, Italy, we document responses and non-responses to the May-June 2012 Emilia seismic sequence. Here we find that discharge only increases where dikes under the vents are unclamped by the static stresses produced by the earthquakes. Mud volcanoes can thus respond to static stress changes (if feeder dikes are unclamped) and dynamic stresses produced by seismic waves (possibly by mobilizing bubbles). ©IAVCEI 2013 Scientific Assembly. All rights reserved. 290 IAVCEI
    [Show full text]
  • Explosive Mud Volcano Eruptions and Rafting of Mud Breccia Blocks
    Earth and Planetary Science Letters 555 (2021) 116699 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Explosive mud volcano eruptions and rafting of mud breccia blocks ∗ Adriano Mazzini a,d, , Grigorii Akhmanov b, Michael Manga c, Alessandra Sciarra d, Ayten Huseynova e, Arif Huseynov e, Ibrahim Guliyev e a Centre for Earth Evolution and Dynamics (CEED), University of Oslo, Oslo, Norway b Faculty of Geology, Lomonosov Moscow State University, Moscow, Russian Federation c Department of Earth and Planetary Science, University of California, Berkeley, USA d Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma 1, Italy e Oil and Gas Institute, Azerbaijan National Academy of Sciences, Baku, Azerbaijan a r t i c l e i n f o a b s t r a c t Article history: Azerbaijan hosts the highest density of subaerial mud volcanoes on Earth. The morphologies characterizing Received 6 June 2020 these structures vary depending on their geological setting, frequency of eruption, and transport Received in revised form 11 October 2020 processes during the eruptions. Lokbatan is possibly the most active mud volcano on Earth exhibiting Accepted 26 November 2020 impressive bursting events every ∼5 years. These manifest with impressive gas flares that may reach Available online xxxx 3 more than 100 meters in height and the bursting of thousands of m of mud breccia resulting in Editor: J.-P. Avouac spectacular mud flows that extend for more than 1.5 kilometres. Unlike other active mud volcanoes, Keywords: to our knowledge Lokbatan never featured any visual evidence of enduring diffuse degassing (e.g., Lokbatan mud volcano Azerbaijan active pools and gryphons) at and near the central crater.
    [Show full text]
  • Marine Geology 378 (2016) 196–212
    Marine Geology 378 (2016) 196–212 Contents lists available at ScienceDirect Marine Geology journal homepage: www.elsevier.com/locate/margo Multidisciplinary study of mud volcanoes and diapirs and their relationship to seepages and bottom currents in the Gulf of Cádiz continental slope (northeastern sector) Desirée Palomino a,⁎, Nieves López-González a, Juan-Tomás Vázquez a, Luis-Miguel Fernández-Salas b, José-Luis Rueda a,RicardoSánchez-Lealb, Víctor Díaz-del-Río a a Instituto Español de Oceanografía, Centro Oceanográfico de Málaga, Puerto Pesquero S/N, 29640 Fuengirola, Málaga, Spain b Instituto Español de Oceanografía, Centro Oceanográfico de Cádiz, Muelle Pesquero S/N, 11006 Cádiz, Spain article info abstract Article history: The seabed morphology, type of sediments, and dominant benthic species on eleven mud volcanoes and diapirs Received 28 May 2015 located on the northern sector of the Gulf of Cádiz continental slope have been studied. The morphological char- Received in revised form 30 September 2015 acteristics were grouped as: (i) fluid-escape-related features, (ii) bottom current features, (iii) mass movement Accepted 4 October 2015 features, (iv) tectonic features and (v) biogenic-related features. The dominant benthic species associated with Available online 9 October 2015 fluid escape, hard substrates or soft bottoms, have also been mapped. A bottom current velocity analysis allowed, the morphological features to be correlated with the benthic habitats and the different sedimentary and ocean- Keywords: fl Seepage ographic characteristics. The major factors controlling these features and the benthic habitats are mud ows Mud volcanoes and fluid-escape-related processes, as well as the interaction of deep water masses with the seafloor topography.
    [Show full text]
  • The Goshogake Mud Volcano Field, Tohoku, Northern Japan: an Acidic, High- 1 2 Temperature System Related to Magmatic Volcanism
    49th Lunar and Planetary Science Conference 2018 (LPI Contrib. No. 2083) 1094.pdf THE GOSHOGAKE MUD VOLCANO FIELD, TOHOKU, NORTHERN JAPAN: AN ACIDIC, HIGH- 1 2 TEMPERATURE SYSTEM RELATED TO MAGMATIC VOLCANISM. G. Komatsu , R. Ishimaru , N. Miyake2, K. Kawai3, M. Kobayashi4, and H. Sakuma5, 1International Research School of Planetary Sciences, Un- iversità d'Annunzio, Viale Pindaro 42, 65127 Pescara, Italy ([email protected]), 2Planetary Exploration Research Center, Chiba Institute of Technology, 2-17-1 Tsudanuma, Narashino-shi, Chiba 275-0016, Japan, 3Department of Earth and Planetary Science, University of Tokyo, Hongo 7-3-1, Bunkyo, Tokyo 113-0033, Japan, 4Department of Earth and Planetary Environmental Science, University of Tokyo, Hongo 7-3-1, Bunkyo, Tokyo 113-0033, Japan. 5Research Center for Functional Materials, National Institute for Materials Science, 1-1 Namiki, Tsukuba, 305-0044 Japan. Introduction: Mud volcanism is widespread in We present documentation of the Goshogake mud various geologic settings in the world. Large-scale volcano features, and data from field measurements of mud volcanoes are well known for example along the temperature of emitted watery mud and methane abun- Alpine orogenic belt of the Mediterranean, Caspian dance, as well as from laboratory analyses for pH of and Black Sea regions [e.g., 1, 2, 3, 4, 5]. The most stu- collected watery mud and isotope ratios of water died mud volcanism sites are related to sedimentary phase, mineralogical composition of deposited solid processes at relatively low temperatures. For example, phases, collected gas composition and microbiology in Azerbaijan the temperatures of fluids consisting of [16, 17, 18].
    [Show full text]
  • Special Paper 470 3300 Penrose Place, P.O
    What Is a Volcano? edited by Edgardo Cañón-Tapia Centro de Investigación Científica y de Educacíon Superior de Ensenada Department of Geology Carretera Ensenada-Tijuana No. 3918 Fraccionamiento Zona Playitas Ensenada Baja California Mexico C.P. 22860 Alexandru Szakács Sapientia University Department of Environmental Sciences Cluj-Napoca, Romania and Romanian Academy Institute of Geodynamics Bucharest, Romania Special Paper 470 3300 Penrose Place, P.O. Box 9140 Boulder, Colorado 80301-9140, USA 2010 Downloaded from http://pubs.geoscienceworld.org/books/book/chapter-pdf/960985/front_matter.pdf by guest on 27 September 2021 Copyright © 2010, The Geological Society of America (GSA), Inc. All rights reserved. GSA grants permission to individual scientists to make unlimited photocopies of one or more items from this volume for noncommercial purposes advancing science or education, including classroom use. For permission to make photocopies of any item in this volume for other noncommercial, nonprofit purposes, contact The Geological Society of America. Written permission is required from GSA for all other forms of capture or reproduction of any item in the volume including, but not limited to, all types of electronic or digital scanning or other digital or manual transformation of articles or any portion thereof, such as abstracts, into computer-readable and/or transmittable form for personal or corporate use, either noncommercial or commercial, for-profit or otherwise. Send permission requests to GSA Copyright Permissions, 3300 Penrose Place, P.O. Box 9140, Boulder, Colorado 80301-9140, USA. GSA provides this and other forums for the presentation of diverse opinions and positions by scientists worldwide, regardless of their race, citizenship, gender, religion, or political viewpoint.
    [Show full text]
  • Origins of High-Temperature Fluids in the Goshogake Mud Volcano Field, Tohoku, Northern Japan: Chemical and Isotopic Studies of Gas and Water
    49th Lunar and Planetary Science Conference 2018 (LPI Contrib. No. 2083) 1210.pdf ORIGINS OF HIGH-TEMPERATURE FLUIDS IN THE GOSHOGAKE MUD VOLCANO FIELD, TOHOKU, NORTHERN JAPAN: CHEMICAL AND ISOTOPIC STUDIES OF GAS AND WATER. R. Ishimaru1, N. Miyake1, G. Komatsu2, K. Kawai3, M. Kobayashi4, H. Sakuma5, T. Matsui1 1Planetary Exploration Research Center (PERC), Chiba Institute of Technology (Chitech) (2-17-1 Tsudanuma, Narashino, Chiba 275-0016, Japan; [email protected]), 2International Research School of Planetary Sciences, Università d'Annunzio (Viale Pindaro 42, 65127 Pescara, Italy), 3Department of Earth and Planetary Science, School of Science, University of Tokyo (Hongo 7-3-1, Bunkyo, Tokyo 113-0033, Japan), 4Department of Earth and Planetary Environmental Sci- ence, School of Science, University of Tokyo (Hongo 7-3-1, Bunkyo, Tokyo 113-0033, Japan), 5Reseach Center for Functional Materials, National Institute for Materials Science (1-1 Namiki, Tsukuba, 305-0044 Japan). Introduction: Mud volcanoes occur everywhere Gas sampling and laboratory analysis. Gases were in various geological settings on the Earth [e.g., 1] and, collected with a custom-made sampling device for possibly, on other planetary bodies, such as Mars [e.g., laboratory measurement of the gas species. The com- 2] and Enceladus ocean floor. Their surface terrains position analysis of the gas samples in the chamber are formed by mud ascending and erupting, together was conducted using Gas Chromatography (GS) in the with water and gas, from depths. Therefore, mud vol- laboratory. The GC analyses are made in two ways: cano is one of the most suitable landforms for explor- qualitative and quantitative analyses.
    [Show full text]
  • 1998 Volcanic Activity in Alaska and Kamchatka: Summary of Events and Response of the Alaska Volcano Observatory by Robert G
    1998 Volcanic Activity in Alaska and Kamchatka: Summary of Events and Response of the Alaska Volcano Observatory by Robert G. McGimsey, Christina A. Neal, and Olga Girina Open-File Report 03-423 U.S. Department of the Interior U.S. Geological Survey 1998 Volcanic Activity in Alaska and Kamchatka: Summary of Events and Response of the Alaska Volcano Observatory By Robert G. McGimsey1, Christina A. Neal1, and Olga Girina2 1Alaska Volcano Observatory, 4200 University Dr., Anchorage, AK 99508-4664 2Kamchatka Volcanic eruptions Response Team, Institute of Volcanic Geology and Geochemistry, Piip Blvd., 9 Petropavlovsk-Kam- chatsky, 683006, Russia AVO is a cooperative program of the U.S. Geological Survey, University of Alaska Fairbanks Geophysical Institute, and the Alaska Division of Geological and Geophysical Surveys. AVO is funded by the U.S. Geological Survey Volcano Hazards Program and the State of Alaska Any use of trade, firm, or product names is for descriptive purposes only and does not imply endorsement by the U.S. Government Open-File Report 03-423 U.S. Department of the Interior U.S. Geological Survey TABLE OF CONTENTS Introduction. 1 Reports of volcanic activity, northeast to southwest along Aleutian arc . 4 Shrub Mud Volcano . 4 Augustine Volcano . 6 Becharof Lake Area . 8 Chiginagak Volcano . 10 Shishaldin Volcano. 12 Akutan Volcano . 12 Korovin Volcano . 13 Reports of Volcanic activity, Kamchatka, Russia, North to South . 15 Sheveluch Volcano . 17 Klyuchevskoy Volcano. 19 Bezymianny Volcano . 21 Karymsky Volcano . 23 References. 24 Acknowledgments . 26 Figures 1 A. Map location of historically active volcanoes in Alaska and place names used in this summary .
    [Show full text]
  • Experimental Simulation Reveals That Mud Behaves Like Lava Under Martian Conditions
    50th Lunar and Planetary Science Conference 2019 (LPI Contrib. No. 2132) 1511.pdf EXPERIMENTAL SIMULATION REVEALS THAT MUD BEHAVES LIKE LAVA UNDER MARTIAN CONDITIONS. P. Brož1, O. Krýza1, S.J. Conway2, J. Raack3, M.R. Patel4,5, M.R. Balme4, A. Mazzini6, E. Hauber7 and M.E. Sylvest4 1Institute of Geophysics of the Czech Academy of Science, Prague, Czech Republic, [email protected] 2CNRS UMR-6112 LPG Nantes, France 3Institut für Planetologie, Westfälische Wilhelms- Universität Münster, Germany 4School of Physical Science, STEM, The Open University, Milton Keynes, UK Open University, Milton Keynes, United Kingdom 5Space Science and Technology Department, STFC Rutherford Apple- ton Laboratory, Oxford, UK 6Centre for Earth Evolution and Dynamics (CEED), University of Oslo, Norway 7Institute of Planetary Research, DLR, Berlin, Germany. Abstract: Here we present results of mud experi- ments performed inside a low pressure chamber to in- vestigate the mechanisms of sedimentary volcanism on the cold martian surface. Our results show that mud propagates under the martian environmental properties with a different behavior than on the Earth surface. Results show that Mars low atmospheric pressure and temperatures cause rapid freezing of the mud flow’s surface. This newly formed “protective crust” effects the propagation of the mud flow resulting in a behavior in some aspects similar to the pahoehoe lava flows on Earth. These findings open new scenarios for the inter- pretation of the flow-related morphologies on Mars. Introduction: Ever since the presence of methane in the martian atmosphere was first reported [1,2], mud volcanism has been hypothesized to be the possible release mechanism [3].
    [Show full text]
  • Distribution, Morphology, and Morphometry of Circular Mounds in the Elongated Basin of Northern Terra Sirenum, Mars Ryodo Hemmi and Hideaki Miyamoto*
    Hemmi and Miyamoto Progress in Earth and Planetary Science (2017) 4:26 Progress in Earth and DOI 10.1186/s40645-017-0141-x Planetary Science RESEARCH ARTICLE Open Access Distribution, morphology, and morphometry of circular mounds in the elongated basin of northern Terra Sirenum, Mars Ryodo Hemmi and Hideaki Miyamoto* Abstract An elongated, flat-floored basin, located in the northern part of Terra Sirenum on Mars, holds numerous enigmatic mounds (100 m wide) on the surface of its floor. We investigated their geological context, spatial distribution, morphological characteristics, and morphometric parameters by analyzing a variety of current remote sensing data sets of Mars. Over 700 mounds are identified; mapping of the mounds shows the spatial density of about 21 per 100 km2 and appearances of several clusters, coalescence, and/or alignment. Most of the mounds have smoother surface textures in contrast to the rugged surrounding terrain. Some of the mounds display depressions on their summits, meter-sized boulders on their flanks, and distinct lobate features. We also perform high-resolution topographic analysis on 50 isolated mounds, which reveals that their heights range from 6 to 43 m with a mean of 18 m and average flank slopes of most mounds are below 10°. These characteristics are consistent with the deposition and extension of mud slurries with mud breccia and gases extruded from subsurface, almost equivalent to terrestrial mud volcanism. If so, both abundance of groundwater and abrupt increase in pore fluid pressure are necessary for triggering mud eruption. Absolute crater retention ages suggest that the floor of the basin located among middle Noachian-aged highland terrains has been resurfaced during the Late Hesperian Epoch.
    [Show full text]
  • Volcanism and Volcanoes
    Volcanism and Volcanoes • Volcanism is one of the most impressive displays of Earth’s dynamic internal processes. • From a human perspective, volcanism can be a destructive force causing property damage, injuries, fatalities, and atmospheric changes. • From a geologic perspective, volcanism is a constructive process that builds oceanic Redoubt Volcano. Photograph by W. White, U.S. islands, produces Geological Survey, December 18, 1989 oceanic crust, provides parent material for highly productive soils, and releases the gases that formed Earth’s early atmosphere and surface waters. Why Study Volcanism? • Volcanic eruptions affect the atmosphere, hydrosphere, and biosphere locally and sometimes globally. • Volcanism is a major geologic hazard to a significant portion of Earth’s inhabitants. • Volcanism is responsible for much of Earth’s most spectacular scenery. Augustine Volcano. Photograph by M.E. Yount, U.S. Geological Survey, March 31, 1986. First, you need to know a little about Plate Tectonics.. Text: Figure 4.1, pg 107 http://www.geology.sdsu.edu/how_volcanoes_work/Volcan o_tectonic.html Convergent, Divergent and Transform Boundary http://geomaps.wr.usgs.gov/parks/pltec/pltec3.html younger older DIVERGENT BOUNDARY Divergent Plate Boundary Age of the Atlantic oceanic crust. The crust near the continental margins (blue) is about 200 million years old. It gets progressively younger toward the mid-Atlantic ridge, where oceanic crust is forming today. Courtesy of NOAA http://www.geology.sdsu.edu/how_volcanoes_work/Volcan o_tectonic.html Pillow basalts on the south Pacific seafloor -- Courtesy of NOAA. http://www.geology.sdsu.edu/how_volcanoes_work/Volcano_tectonic.html Transform Boundary…earthquakes Convergent Plate Boundary • The Pacific Ring of Fire • the most volcanically active belt on Earth • subduction zone…large ocean trenches Island Arc Volcanic Arc http://www.geology.sdsu.edu/how_volcanoes_work/Volcano_tectonic.html Intraplate Volcanism Mantle plumes on earth Hotspot Volcanism http://www.geology.sdsu.edu/ Figure 4.4 pg.
    [Show full text]
  • HYDROVOLCANIC (TUFF) RINGS and CONES from PHREATOMAGMATIC EXPLOSIVE ERUPTIONS on MARS P. Brož1,2 and E. H
    44th Lunar and Planetary Science Conference (2013) 2430.pdf AMENTHES CONES, MARS: HYDROVOLCANIC (TUFF) RINGS AND CONES FROM PHREATOMAGMATIC EXPLOSIVE ERUPTIONS ON MARS P. Brož1,2 and E. Hauber3, 1Institute of Geo- physics ASCR, v.v.i., Prague, Czech Republic, [email protected], 2 Institute of Petrology and Structural Geology, Charles University, Czech Republic 3Institute of Planetary Research, DLR, Berlin, Germany, [email protected]. Introduction: Mars was volcanically active Skinner and Tanaka conclude that an origin as mud throughout most, if not all, of its history [e.g., 1-4], and volcanoes best explains their formation [15]. An igne- volcanism played a significant role in the formation of ous volcanic origin is rejected by [15] because of (1) its surface. Another factor modifying the Martian sur- the large distance to known volcanic vents, (2) a lack face is water, both in liquid and frozen state, and at and of obvious structural control of dike-related eruptions, beneath the surface [e.g., 5]. Interactions of magma (3) the confinement to a specific latitude and elevation with water and/or ice should be common on Mars, range, (4) the setting in a compressional tectonic re- therefore. On Earth, such interactions are known to gime, and (5) the pitted cones being part of a broader trigger hydrovolcanism [6], the natural phenomenon of assemblage of landforms. magma or magmatic heat interacting with an external water source [6] producing tuff rings, tuff cones and maars as typical landforms. The existence of explosive volcanism on Mars was predicted on theoretical grounds [7], but only few direct observations are avail- able [8-13].
    [Show full text]