Regional Geophysical Investigations of the Moab-Needles Area, Utah

Total Page:16

File Type:pdf, Size:1020Kb

Regional Geophysical Investigations of the Moab-Needles Area, Utah Regional Geophysical Investigations of the Moab-Needles Area, Utah GEOLOGICAL SURVEY PROFESSIONAL PAPER 516-C Prepared partly on behalf of the U.S. Atomic Energy Commission REGIONAL GEOPHYSICAL INVESTIGATIONS MOAB-NEEDLES AREA, UTAH Aerial view of Upheaval Dome, San Juan County, Utah. Regional Geophysical Investigations of the Moab-Needles Area, Utah By H. R. JOESTING, ]. E. CASE, and DONALD PLOUFF GEOPHYSICAL FIELD INVESTIGATIONS GEOLOGICAL SURVEY PROFESSIONAL PAPER 516-C Prepared partly on behalf of the U.S. Atomic Energy Commission Gravity and magnetic surveys of parts of Canyonlands National Park UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON : 1966 GEOPHYSICAL FIELD INVESTIGATIONS REGIONAL GEOPHYSICAL INVESTIGATIONS OF THE MOAB-NEEDLES AREA, UTAH By H. R. JoESTING,1 J. E. CAsE, and DoNALD PLOUFF ABSTRACT southern part of the area is interpreted to be the result of com­ paratively dense basement and thinning of eva.porites at the Aeromagnetic and gravity surveys were made of about 1,450 north nose of the Monument uplift. Regional lo\vs near Mean­ square miles in the Moab-Needles area of Utah, in the north­ der anticline along the Colorado River may be associated with central parot of ·the Colorado Plateau. The area is within the less dense or deeper basement and thicker evaporites. Paradox evaporite basin, a subsurface feature of Pennsylvanian Another major buried trough and its flanking structural highs, age. These surveys were made to gain broad-scale information in the Mississippian and older rocks, trends northeast along the on the depth, composition, and configura,tion af the Precambrian Colorado River. These structures are indicated by gravity and basement, and on major salt ran'ticlines that may have influenced magnetic data and are partly corroborated by data from deep the occurrence of uranium, oil, and potassium-bearing evaporites. drilling. Minor rejuvenation of these features during Cenozoic Exposed sedimentary rocks range in age from Pennsylvani,an time may have affected the course of the Colorado River. to Recent. Oam'brian, Devonian, and Mississippian rocks have been found in deep wells. No igneous rocks have been reported, INTRODUCTION and no Precambrian ·rock•s have been penetrated by the drill. According to geophysical evidence, the P·recambrian rocks This report describes the results of aeromagnetic and differ in magnetization and density, reflecting differences in regional gravity surveys in southeastern Utah in the composition. The sedimentary rocks are almost nonmagnetic, area between Moab and The Needles, near the junction but their densities vary widely. In the northern third of the area, which lies within the of the Green and Colorado Rivers (fig. 1). It is one of deeper pavt of the Paradox evaporite basin, magnetie gradients a series of regional geophysical studies of the Colorado are lO'W, thus indicating almost uniform magnetization of the Plateau, made to gain additional broad-seale informa­ basement. This magnetization does, however, increase grad­ tion on the depth and configuration of the buried Pre­ ually tOIWard the northeast. In the southern third of the area, cambrian basement, and on regional structures that may which includes the north end of the Monument uplift, the mag­ netic field is diverse, an indication of compositional diversity have influenced the occurrence of uranium, potassium­ of the basement. In the central part, evidently a transition zone bearing salts, and oil ( J oesting and Byerly, 1958 ; between basin and uplift, are three prominent magnetic highs, Byerly and Joesting, 1959; Case and others, 1963). associated with large stocklike masses in the basement that are The area discussed here includes The Knoll, Moab, Up­ surrounded by rocks having about the same magnetization as heaval Dome, Hatch Point, The Needles, and Harts those in the northern part. Cpheaval Dome, a remarkable structural dome probably formed by an intrusive salt plug, is Point 15-minute quadrangles in parts of Grand, San near the crest of one of the magnetic highs, but the high is at J nan, V\r ayne, Garfield, and Emery Counties (fig. 1). least four times as wide as the dome. No surface structural The Canyonlands National Park lies partly within the features are associated with the other magnetic highs. area. The gravity anomalies are associated with density contrasts The Moab-Needles area is a land of broad high mesas within both the Precambrian and the sedimentary rocks, par­ ticularly between the evaporites and the sandstone, shale, ·and and of deep precipitous canyons cut into multicolored limestone. Prominent lows occur over the large salt anticlines sandstone and shale by the Colorado and Green Rivers of Moab and Salt Valleys in the northern pavt of the area. p.art and their tributaries. lTpheaval Dome, a symmetrieal of the anomaly along Moa'b Valley is evidently related to a struetural dome into whieh a remarkably deep circular basement fault that may have controlled the position of the salt anticline. A prominent gravity gradient in the central erater has been eroded (see frontispiece), is in the west­ part of the rarea evidently marks a major lithologic and struc­ ern part of the area. The Needles fault zone, with to­ tural change in the basement: from lower density in the deeper pography characterized by tall slender sandstone spires basin to the north to higher density in the buried uplift to the south. Part of the gradient is also related to thinning of evap­ and valleys ·with interior drainage, lies in the south­ orites to the south. The deep~seated basement structural fea­ "·estern part of the area just east of Cataract Canyon ture is also indicated by magnetic data. A gravity high in the of the Colorado River and south of Meander salt anti­ 1 Deceased, May 1965. cline. Broad and elongate valleys have formed along 01 C2 GEOPHYSICAL FIELD INVE1STIGATIONS 38°30' WAYNE Monticello 0 SAN JUAN DOLORES Blanding i 0 I 37°30'~----~~--------4-~~--------------~--------------~~----------------~--~I I, '~V1l' ::J J/ I \%.~ <, Cortez /,../' 0 I ~~ I 0 Bluff } / ~ ~ ~,, I ~/ I ~b. MONTEZU A ( ~/ . / Mexican Hat e.,. I /I //~ 1 ,_ 0 10 201 30 40 MILES / J J ! ~~-#Pu~ I L ~I I / 3ro0,_l _______ i_L _____ _:_~~-L---- UTA_!!__ --~OLOR~DO -~----- ARIZONA ------OF pp.RP.D~-----,.. NEW MEXICO --------------- EXPLANATION Jllllllllll ...__\ll La Sal Mountains Lisbon Valley area Uravan area Sa.lt Valley-Cisco Axis of salt anticline Igneous intrusions in area (Byerly and Joesting, 1959) (Joesting and Byerly, 1958) area or monoclinal uplift the La Sal Mountains (Case and others, 1963) (Joesting and Case, 1962) FIGURE 1.-Location of the Moab-Needles area (stippled) relative to major structures in the Paradox basin, Utah and Colorado. REGIONAL G'EIOPHYIS!lCA:L INVEISTIGATIONS, MOAB-NEED-LES AR'EA, UTAH C3 the breached crests of Moab Valley and Salt Valley the Geological Survey in the salt anticline region were salt anticlines in the northeastern part of the area. summarized by J oesting and Case ( 1960). More de­ Airborne magnetic surveys were made over the area tailed reports ·were prepared on areas adjoining the during 1954, and additional surveys were flown over Moab-Needles area: the Lisbon Valley area (Byerly Upheaval Dome in 1955. The airborne surveys were and J oesting, 1959) ; the La Sal Mountains area (Case directed by J. L. Meuschke and R. W. Bromery; com­ and others, 1963) to the east; and the Salt Valley­ pilation of aeromagnetic data was directed initially Cisco area ( ,J oesting and Case, 1962) to the north (fig. by James Aubrey and later by Paul Yeager. 1). A brief preliminary report on geophysical investi­ The gravity field party was initially under the direc­ gations in the vicinity of lTpheaval Dome was prepared tion of Richard Warrick; most of the fieldwork, how­ by J oesting and Plouff ( 1958). A gravity map and ever, was directed by Donald Plouff, assisted at various brief discussion of the Moab-Needles area also was re­ times by Winthrop Means, Jerome Marks, Marvin Bo­ leased ( J oesting and others, 1962). hannon, and Huntley Ingalls. A line of gravity sta­ This investigation has been supported jointly by the tions was later established down the Green River by U.S. Atomic Energy Commission and the U.S. Geologi­ P. E. Byerly, and a line down the Colorado River to cal Survey. Cataract Canyon by J. E. Case. Ground magnetometer GEOLOGIC SETTING and gravity meter traverses and transit traverses for The ~{oab-Needles area is in the north-central part vertical control were run in Upheaval Canyon and from of the Colorado Plateau, in the Canyon Lands section the rim to the bottom of Upheaval Dome by Joesting of Fenneman (1931). The area is within the Paradox and Plouff and later by J oesting and Case. basin, which is characterized by thick Pennsylvanian Geologic information to aid in the interpretation of evapori,tes that locally form the cores of salt anticlines the geophysical data was obtained mainly from publica­ (fig. 1). Structure of sedimentary rocks at the surface, tions of Baker ( 1933, 1946), Dane ( 1935), and Mc­ hmvever, gives no hint of the buried Pennsylvanian Knight (1940), from oil-company drill logs and from basin; the exposed rocks dip gently northward and oil scout reports. Information was also obtained from northeastward from the Monument uplift, in the south­ photogeologic maps of parts of the area by Bates (1955a, ern part of the area, toward the Uinta Basin, which lies b, c), Bergquist ( 1955), Hemphill ( 1955), and Sable farther north. A deep-seated fault or other vertical (1955a, b, c, and1956); and from unpublished maps of displacement within the Paradox basin, trending west­ parts of the Upheaval Dome and The Needles quad­ northwest across the area, divides the basin into a shal­ rangles by F. A.
Recommended publications
  • 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].
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • An Inventory of Non-Avian Dinosaurs from National Park Service Areas
    Lucas, S.G. and Sullivan, R.M., eds., 2018, Fossil Record 6. New Mexico Museum of Natural History and Science Bulletin 79. 703 AN INVENTORY OF NON-AVIAN DINOSAURS FROM NATIONAL PARK SERVICE AREAS JUSTIN S. TWEET1 and VINCENT L. SANTUCCI2 1National Park Service, 9149 79th Street S., Cottage Grove, MN 55016 -email: [email protected]; 2National Park Service, Geologic Resources Division, 1849 “C” Street, NW, Washington, D.C. 20240 -email: [email protected] Abstract—Dinosaurs have captured the interest and imagination of the general public, particularly children, around the world. Paleontological resource inventories within units of the National Park Service have revealed that body and trace fossils of non-avian dinosaurs have been documented in at least 21 National Park Service areas. In addition there are two historically associated occurrences, one equivocal occurrence, two NPS areas with dinosaur tracks in building stone, and one case where fossils have been found immediately outside of a monument’s boundaries. To date, body fossils of non- avian dinosaurs are documented at 14 NPS areas, may also be present at another, and are historically associated with two other parks. Dinosaur trace fossils have been documented at 17 NPS areas and are visible in building stone at two parks. Most records of NPS dinosaur fossils come from park units on the Colorado Plateau, where body fossils have been found in Upper Jurassic and Lower Cretaceous rocks at many locations, and trace fossils are widely distributed in Upper Triassic and Jurassic rocks. Two NPS units are particularly noted for their dinosaur fossils: Dinosaur National Monument (Upper Triassic through Lower Cretaceous) and Big Bend National Park (Upper Cretaceous).
    [Show full text]