Structure and Evolution of Upheaval Dome: a Pinched-Off Salt Diapir
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Fault Formation at Impact Craters in Porous Sedimentary Rock Targets W.R
40th Lunar and Planetary Science Conference (2009) 1073.pdf FAULT FORMATION AT IMPACT CRATERS IN POROUS SEDIMENTARY ROCK TARGETS W.R. Orr Key1 and R.A. Schultz, Geomechanics-Rock Fracture Group, Department of Geological Sciences and Engineer- ing/172, Mackay School of Earth Sciences and Engineering, University of Nevada, Reno, NV 89557-0138, [email protected]. Summary: We present results of a study in which provides a unique opportunity to compare the mechan- the mechanics of faulting at high strain rates in porous ics of faulting at high and low strain rates. sedimentary rocks were evaluated at the Upheaval Results and Implications: It was decided that Dome impact crater in southeast Utah. We find that at faults would be evaluated within the Navajo Sandstone high strain rates, deformation band damage zones are and the rim syncline of the crater because mechanical absent and instead a cracking-dominated behavior gen- observations relating to fault formation are best ob- erating pulverized rock occurs. Using the measured served where offsets on the faults are minimal. Two of grain sizes of the pulverized rock, strain rates under these faults were identified for field investigation which this material formed are ~ 103 s-1. within the rim syncline of Upheaval Dome and are Introduction: Faulting in porous sedimentary shown in Figure 1. By contrast, offsets within the cen- rocks subjected to typical tectonic strain rates has been tral uplift at Upheaval Dome [10] are too great to allow extensively studied [1-3]. These studies have shown for the mechanical observations required for this study. that the strain is first accommodated by a localized reduction of porosity resulting in the formation of in- dividual deformation bands and as the strain continues to accumulate, deformation band damage zones (DBDZs) develop [2]. -
Terrestrial Impact Structures Provide the Only Ground Truth Against Which Computational and Experimental Results Can Be Com Pared
Ann. Rev. Earth Planet. Sci. 1987. 15:245-70 Copyright([;; /987 by Annual Reviews Inc. All rights reserved TERRESTRIAL IMI!ACT STRUCTURES ··- Richard A. F. Grieve Geophysics Division, Geological Survey of Canada, Ottawa, Ontario KIA OY3, Canada INTRODUCTION Impact structures are the dominant landform on planets that have retained portions of their earliest crust. The present surface of the Earth, however, has comparatively few recognized impact structures. This is due to its relative youthfulness and the dynamic nature of the terrestrial geosphere, both of which serve to obscure and remove the impact record. Although not generally viewed as an important terrestrial (as opposed to planetary) geologic process, the role of impact in Earth evolution is now receiving mounting consideration. For example, large-scale impact events may hav~~ been responsible for such phenomena as the formation of the Earth's moon and certain mass extinctions in the biologic record. The importance of the terrestrial impact record is greater than the relatively small number of known structures would indicate. Impact is a highly transient, high-energy event. It is inherently difficult to study through experimentation because of the problem of scale. In addition, sophisticated finite-element code calculations of impact cratering are gen erally limited to relatively early-time phenomena as a result of high com putational costs. Terrestrial impact structures provide the only ground truth against which computational and experimental results can be com pared. These structures provide information on aspects of the third dimen sion, the pre- and postimpact distribution of target lithologies, and the nature of the lithologic and mineralogic changes produced by the passage of a shock wave. -
Deformation Styles at Upheaval Dome, Utah Imply Both Meteorite Impact and Subsequent Salt Diapirism
41st Lunar and Planetary Science Conference (2010) 1969.pdf DEFORMATION STYLES AT UPHEAVAL DOME, UTAH IMPLY BOTH METEORITE IMPACT AND SUBSEQUENT SALT DIAPIRISM. R. G. Daly and S. A. Kattenhorn, University of Idaho Department of Geo- logical Sciences ([email protected]; [email protected]). Introduction: Upheaval Dome is a ~5.5 km wide that diapirism may have had an influence on the de- circular topographic depression in Canyonlands Na- formation present at the dome. tional Park, Utah (Fig. 1). Upturned beds around the Observations: Field work has focused on observ- feature indicate a structural dome located above salt ing brittle deformation in and around the ring syncline. layers in the Pennsylvanian aged Paradox Formation. This area is pervasively deformed and as such affords Its ambiguous origin, either as a salt diapir or a mete- many varied examples of brittle failure. This work orite impact, has been debated for the last 75 years. complements the extensive research done in the central Recently, planar deformation features (PDFs) were uplift of the dome [6]. Many different morphologies discovered at the dome. Based on current field work are present, such as joints, deformation bands, and we propose two methods of deformation present at the shear fractures. There is also variation within each dome: meteorite impact and subsequent salt diapirism. morphology. Many shear fractures are planar and regu- Based on field and aerial photograph analysis, we larly spaced; however, there are also many sets with a have identified and characterized both dynamic and distinct curvilinear shape, the orientation of which slowly-formed deformation features around the dome. -
A Novel Geomatics Method for Assessing the Haughton Impact Structure
Meteoritics & Planetary Science 1–13 (2020) doi: 10.1111/maps.13573-3267 Electronic-Only Article A novel geomatics method for assessing the Haughton impact structure Calder W. PATTERSON * and Richard E. ERNST Department of Earth Sciences, Ottawa Carleton Geoscience Center, Carleton University, 1125 Colonel By Drive, Ottawa, Ontario K1S 5B6, Canada *Corresponding author. E-mail: [email protected] (Received 22 July 2019; revision accepted 22 August 2020) Abstract–Terrestrial impact structures are typically modified by erosion, burial, and tectonic deformation. Their systematic morphologies are typically reconstructed through a combination of geological and topographic mapping, satellite imagery, and geophysical surveys. This study applies a novel geomatics approach to assessment of the morphology of the extensively studied Haughton impact structure (HIS), Devon Island, Nunavut, in order to test its potential to improve the accuracy and quality of future impact structure reconstruction. This new methodology integrates HIS lithological data, in the form of digitized geologic mapping, with a digital elevation model, within diametrically opposed, wedge-shaped couplets, and plots these data as pseudo cross sections that capitalize on the radial symmetry of the impact structure. The pseudo cross sections provide an accurate reconstruction of the near- surface stratigraphic sequences and terraces in the faulted annulus of the modified crater rim. The resultant pseudo cross sections support current interpretations regarding the 10–12 km diameter of the transient cavity, and successfully reproduce the visible outer ring and intermediate uplifted zone within the central basin. Observed positions of vertical offsets suggest that the extent of impact deformation extends beyond the current estimates of the apparent crater rim to radial distances of between 14 and 15 km. -
Terrestrial Impact Structures and Their Confirmation: Example from Dhala Structure, Central India
e-Journal Earth Science India, Vol.2 (IV), October, 2009, pp. 289 - 298 http://www.earthscienceindia.info/; ISSN: 0974 - 8350 Terrestrial Impact Structures and their Confirmation: Example from Dhala Structure, central India J. K. Pati1, K. Prakash2 and R. Kundu1 1Department of Earth & Planetary Sciences, Nehru Science Centre, University of Allahabad, Allahabad, India 2Department of Geology, Banaras Hindu University, Varanasi, India Email: [email protected]; [email protected] Abstract Although seventy percent of the Moon surface area is covered by meteoritic impact structures only 176 confirmed impact structures known on Earth hitherto. In India, the recently discovered Dhala impact structure, M.P. and the Lonar crater, Maharastra are the only two confirmed impact structures. The simple, complex and multi-ring impact structures are confirmed on the basis of mesoscopic and microscopic shock metamorphic features besides the physical and/or chemical signature(s) of the impactor (meteorite). The role of bolide impacts in the formation of mineral deposits and playing a crucial role in some of the major mass extinction events is also well known. The impact cratering process is considered responsible for the planetary evolution, landscape modification, and the presence of water and life on Earth. Introduction Bolide impact structures broadly cover the surfaces of planetary bodies in the solar system (Taylor, 1992) but predominantly occur in the planets of the inner solar system, their moons and asteroids. Nearly 70% of the Lunar surface is covered by impact structures. However, these are rare features on the surface of the planet Earth and only 176 structures are currently known (http://www.unb.ca/passc/ImpactDatabase/Age; October 10, 2009) as confirmed impact structures. -
The Ries-Steinheim Crater Pair and Two Major Earthquakes – New Discoveries Challenging the Double-Impact Theory
The Ries-Steinheim crater pair and two major earthquakes – New discoveries challenging the double-impact theory Elmar Buchner ( [email protected] ) University of Applied Sciences Neu-Ulm Volker Sach Meteorkratermuseum Steinheim Martin Schmieder USRA, Houston, Texas Article Keywords: impact-earthquakes, Nördlinger Ries, Steinheim Basin Posted Date: July 27th, 2020 DOI: https://doi.org/10.21203/rs.3.rs-43745/v1 License: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License Page 1/24 Abstract The Nördlinger Ries and the Steinheim Basin are widely perceived as a Middle Miocene impact crater doublet. We discovered two independent earthquake-produced seismite horizons in North Alpine Foreland Basin deposits. The older seismite horizon,associated with the Ries impact is overlain by in situ-preserved distal impact ejecta, forming a unique continental seismite-ejecta couplet within a distance up to 180 km from the crater. The younger seismite unit, also triggered by a major palaeo-earthquake, comprises clastic dikes that cut through the Ries seismite-ejecta couplet. The clastic dikes were likely formed in response to the Steinheim impact, some kyr after the Ries impact, in line with paleontologic results. With the Ries and Steinheim impacts as two separate events, Southern Germany witnessed a double disaster in the Middle Miocene. The magnitude–distance relationship of seismite formation during large earthquakes suggests the seismic and destructive potential of impact-earthquakes may be signicantly underestimated. Introduction The ~24 km-diameter Nördlinger Ries1,2,3,4 and the ~4 km-diameter Steinheim Basin1,5,6,7,8 impact structures in southern Germany (Fig. -
GEOLOGY of the MOAB REGION Introduction
GEOLOGY OF THE MOAB REGION (Arches, Dead Horse Point and Canyonlands) Annabelle Foos Geology Department, University of Akron Introduction The geology of Arches National Park, porphyry laccolith that was intruded during the Dead Horse Point State Park and the “Island in Oligocene, 30 million years ago and the Sky” section of Canyonlands National Park experienced glaciation during the Pleistocene. is very similar. They occur in the Canyonlands Melting snow which accumulates in the section of the Colorado Plateau, in the vicinity mountains during winter months, replenishes of the confluence between the Green and streams and recharges bedrock aquifers Colorado Rivers. The same stratigraphic units providing a valuable source of fresh water to outcrop in all three parks (figure 1) plus salt this region. (Doelling and others, 1987) tectonic features can be found in both Arches and Canyonlands. While in the Moab region you will become familiar with some of the stratigraphic units we will see throughout the Colorado Plateau, observe salt tectonic features, arch formation and in the distance you can view the La Sal Mountains. Cryptogamic Soils While in these three parks (and throughout this trip) you will be required to STAY ON THE DESIGNATED TRAILS. This rule is especially important at these parks in order to preserve the fragile cryptogamic soils (figure 2). Cryptogamic soils are a complex of lichens, algae, moss and fungus that occurs as a black coating on the ground surface and as small mounds where it is well developed. It plays an extremely important role in the desert ecology. It binds the soil together and inhibits wind erosion and erosion by sheet wash. -
Four Hundred Years of Hits and Misses in Scientific Impact Crater Research
NIR Workshop, Gardnos − Gol, June 9th 2009 Four Hundred Years of Hits and Misses in Scientific Impact Crater Research Teemu Öhman Division of Geology, Department of Geosciences and Division of Astronomy, Department of Physical Sciences University of Oulu Finland Galileo Galilei Galileo Galilei (1564−1642) • First observer of lunar craters, late November 1609, Padua, Italy • Surface previously supposed smooth can be divided to dark lowlands (“large spots”) and bright highlands, which are covered with pits that have uplifted rims • A clear description of a central uplift Galilaei, D=15.5 km (LO) Johannes Kepler (1571−1630) • Supposed, like e.g. Plutarch in 1st century A.D., that the lunar lowlands are filled with water • Coined the terms “mare” and “terra” • Believed meteor(ite)s to have a cosmic origin(?) Kepler, D=32 km (LO) Robert Hooke (1635−1703) • Crater observer: Hipparchus, D=150 km Halley Micrographia, 1665 Lunar Orbiter Robert Hooke • First crater experimentalist: 1. Dropping bullets to a mixture of tobacco pipe clay and water: Æcraters “not unlike these of the Moon; but considering the state and condition of the Moon, there seems not any probability to imagine, that it should proceed from any cause analogus to this; for it would be difficult to imagine whence those bodies should come; and next, how the substance of the Moon should be so soft;” Robert Hooke 2. A pot of boiling alabaster: • When the boiling ceased, the surface was covered with craters • Compared these to terrestrial volcanoes Æ “…these pits in the Moon seem to -
Impact Cratering: Bridging the Gap Between Modeling and Observations
IMPA_ CRATERING: BRIDGING THE GAP B_EEN MODELING AND OBSERVATIONS IIllll ..................... ,, ,, ,,, ,,,,,,,, ,r, II I I II I Houston, T<xas -- F_bruary 7-9, 2003 Abstract Volume LPI LPI Contribution No. 1155 Impact Cratering: Bridging the Gap Between Modeling and Observations February 7-9, 2003 Houston, Texas Sponsor Lunar and Planetary Institute National Aeronautics and Space Administration Conveners Robert Herrick, Lunar and Planetary Institute Elisabetta Pierrazzo, Planetary Science Institute Scientific Organizing Committee Bevan French, Natural History Museum Kevin Housen, Boeing Corporation William McKinnon, Washington University Jay Melosh, University of Arizona Michael Zolensky, NASA Johnson Space Center Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Contribution No. 1155 Compiled in 2003 by LUNAR AND PLANETARY INSTITUTE The Institute is operated by the Universities Space Research Association under Agreement No. NCC5-679 issued through the Solar System Exploration Division of the National Aeronautics and Space Administration. Any opinions, findings, and conclusions or recommendations expressed in this volume are those of the author(s) and do not necessarily reflect the views of the National Aeronautics and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. Abstracts in this volume may be cited as Author A. B. (2003) Title of abstract. In Impact Cratering: Bridging the Gap Between Modeling and Observations, p. XX. LPI Contribution No. 1155, Lunar and Planetary Institute, Houston. This volume is distributed by ORDER DEPARTMENT Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113, USA Phone: 281-486-2172 Fax: 281-486-2186 E-mail: [email protected] Mail order requestors will be invoiced for the cost of shipping and handling. -
New Structural Constraints on the Upheaval Dome Impact Crater: T
Lunar and Planetary Science XXXIII (2002) 1037.pdf NEW STRUCTURAL CONSTRAINTS ON THE UPHEAVAL DOME IMPACT CRATER: T. Kenkmann1 and D. Scherler1, 1Institut für Mineralogie, Museum für Naturkunde, Humboldt-Universität Berlin, Invalidenstrasse 43, D-10115 Berlin, Germany, [email protected]. Introduction: The Upheaval Dome structure, power law function in the limits of the slab extent and Utah, is a deeply eroded complex impact crater of 6-9 comparing the area with an undeformed strata where hf km final diameter, which allows a detailed structural = hi. Changes in layer thickness during the collapse of analysis of the crater floor due to a superb exposure. the transient cavity were accommodated by bedding Based on a geological map of the impact structure [1] parallel detachment faulting. The magnitude of inward and own data, we constructed new cross sections motion for the marker beds displayed in Figure 3 and 4 through the crater floor. The technique, which is known is about 460 m for Kayenta F., 290 m for the Wingate as balanced section construction [2], was applied Sandstone, and 130 m for the Church Rock Member of semiquantitatively using methods of thin-skinned the Chinle Formation. tectonics to unravel the kinematic history of crater Figure 1 modification. The basic premise behind this method is the requirement of compatibility which implies a variety of geometric constraints. The constructed section must be restorable to an undeformed stratigraphic template, that was present before the impact. Deformation during crater collapse occurs on more or less radial rather than plane-strain trajectories. Therefore gains and losses of material during inward and outward flow are typical on a 2-D section. -
Extrusions of Hormuz Salt in Iran
Downloaded from http://sp.lyellcollection.org/ by guest on September 26, 2021 Extrusions of Hormuz salt in Iran CHRISTOPHER J. TALBOT Hans Ramberg Tectonic I_xtborator~; blstitute of Earth Sciences, Uppsala Universit3, S-752 36 Uppsala, Sweden Abstract: This work illustrates that Lyell's approach to inferring geological processes from field observations can be improved by using field measurements of their rates to scale dynamic models. A controversy in the 1970s about whether crystalline rock salt can flow over the surface echoed an earlier controversy resolved with Lyell's help about whether ice could flow and carry exotic blocks. This work argues that the external shapes, internal fabrics and structures and rates of flow of current salt extrusions in the Zagros Mountains are keys not only to understanding past and future extrusion of salt. but also to the extrusion of metamorphic cores of orogens. Salt is shown to extrude first in hemispherical domes, which later spread to the shapes of viscous fountains until they are isolated from their source, They then rapidly assume the shapes of viscous droplets, which they maintain until they degrade to heaps of residual soils. Salt emerges as a linear viscous Bingham fluid, and strain rate hardens downslope to a power-law fluid (n = 3) beneath a thickening carapace of brittle dilated salt. The velocities of salt constrained in emergent diapirs by measurements of extruding salt sheets in Iran are remarkably rapid compared with rates estimated for buried equivalents elsewhere in or under which it is planned to store nuclear waste or to extract hydrocarbons. Because halite (NaC1) is the product of evaporation porating more upright box folds with shorter exceeding the supply of sea water, beds of rock salt hinges- compared to adjoining thrust wedges not often occur near the base of sedimentary sequences underlain by salt, which are narrower and have a that accumulate in new basins. -
Shatter Cone and Microscopic Shock-Alteration Evidence for a Post-Paleoproterozoic Terrestrial Impact Structure Near Santa Fe, New Mexico, USA
Earth and Planetary Science Letters 270 (2008) 290–299 Contents lists available at ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl Shatter cone and microscopic shock-alteration evidence for a post-Paleoproterozoic terrestrial impact structure near Santa Fe, New Mexico, USA Siobhan P. Fackelman a, Jared R. Morrow b,⁎, Christian Koeberl c, Thornton H. McElvain d a Earth Sciences Department, University of Northern Colorado, Greeley, CO 80639, USA b Department of Geological Sciences, San Diego State University, San Diego, CA 92182, USA c Department of Lithospheric Studies, University of Vienna, Althanstrasse 14, A-1090 Vienna, Austria d 111 Lovato Lane, Santa Fe, NM 87505, USA ARTICLE INFO ABSTRACT Article history: Field mapping, morphologic description, and petrographic analysis of recently discovered shatter cones Received 7 January 2008 within Paleoproterozoic crystalline rocks exposed over an area N5km2, located ∼8 km northeast of Santa Fe, Received in revised form 19 March 2008 New Mexico, USA, give robust evidence of a previously unrecognized terrestrial impact structure. Herein, we Accepted 20 March 2008 provisionally name this the “Santa Fe impact structure”. The shatter cones are composed of nested sub- Available online 7 April 2008 conical, curviplanar, and flat joint surfaces bearing abundant curved and bifurcating striations that strongly Editor: R.W. Carlson resemble the multiply striated joint surfaces (MSJS) documented from shatter cones at Vredefort dome. The cones occur as a penetrative feature in intrusive igneous and supracrustal metamorphic rocks, are unusually Keywords: large (up to 2 m long and 0.5 m wide at the base), display upward-pointing apices, and have subvertical, shatter cones northeastward-plunging axes that crosscut regional host-rock fabrics.