GEOLOGY of the MOAB REGION Introduction
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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. -
Quaternary Tectonics of Utah with Emphasis on Earthquake-Hazard Characterization
QUATERNARY TECTONICS OF UTAH WITH EMPHASIS ON EARTHQUAKE-HAZARD CHARACTERIZATION by Suzanne Hecker Utah Geologiral Survey BULLETIN 127 1993 UTAH GEOLOGICAL SURVEY a division of UTAH DEPARTMENT OF NATURAL RESOURCES 0 STATE OF UTAH Michael 0. Leavitt, Governor DEPARTMENT OF NATURAL RESOURCES Ted Stewart, Executive Director UTAH GEOLOGICAL SURVEY M. Lee Allison, Director UGSBoard Member Representing Lynnelle G. Eckels ................................................................................................... Mineral Industry Richard R. Kennedy ................................................................................................. Civil Engineering Jo Brandt .................................................................................................................. Public-at-Large C. Williatn Berge ...................................................................................................... Mineral Industry Russell C. Babcock, Jr.............................................................................................. Mineral Industry Jerry Golden ............................................................................................................. Mineral Industry Milton E. Wadsworth ............................................................................................... Economics-Business/Scientific Scott Hirschi, Director, Division of State Lands and Forestry .................................... Ex officio member UGS Editorial Staff J. Stringfellow ......................................................................................................... -
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. -
The White Rim — East to West 4 Days/3 Nights
The White Rim — East to West 4 days/3 nights DAY 1 Needles districts of Canyonlands and beyond. We will shuttle from our shop in Moab to the TOTAL MILEAGE: 27 miles Island in the Sky District of Canyonlands National Park where we begin our ride with a DAY 3 dramatic descent of the Shafer Trail switchbacks. This 1,200 foot downhill lasts for three miles and We begin the day with a fun but technical brings us down to the White Rim sandstone layer. descent off the Hogback down to the White Points of interest include: the Colorado River Rim layer. Points of interest include Overlook, Musselman Arch, Little Bridge Canyon Candlestick Tower and Holeman Canyon, where we (prime Bighorn Sheep habitat) and Lathrop Canyon. may take a short hike. Hiking into this canyon is very The route continues with a downhill trend and then tricky and requires some interesting moves. The rolls gently to camp. After Lathrop Canyon, we will hanging gardens, pools of water and narrow canyon ride to our camp at Airport Tower and enjoy views of walls make this hike one of our favorites on the White the La Sal and Abajo mountains. Rim. We will then continue along in a downhill mode along the rim of the sheer canyon to Potato Bottom TOTAL MILEAGE: 18 miles where the White Rim sandstone layer disappears into the Green River. We’ll camp here under the DAY 2 cottonwoods on the bank of the Green River. Today, as we approach Monument Basin, we TOTAL MILEAGE: 21 miles will continue riding around the beautifully eroded canyons of the Colorado Plateau. -
Analysis of a Sponge Bioherm from the Hermosa Group, Molas Lake Area, Colorado
Bowling Green State University ScholarWorks@BGSU Honors Projects Honors College Spring 2014 Analysis of a Sponge Bioherm from the Hermosa Group, Molas Lake Area, Colorado Joanna Hamilton [email protected] Follow this and additional works at: https://scholarworks.bgsu.edu/honorsprojects Part of the Paleobiology Commons Repository Citation Hamilton, Joanna, "Analysis of a Sponge Bioherm from the Hermosa Group, Molas Lake Area, Colorado" (2014). Honors Projects. 116. https://scholarworks.bgsu.edu/honorsprojects/116 This work is brought to you for free and open access by the Honors College at ScholarWorks@BGSU. It has been accepted for inclusion in Honors Projects by an authorized administrator of ScholarWorks@BGSU. Analysis of a Sponge Bioherm from the Hermosa Group, Molas Lake Area, Colorado Joanna Hamilton Bowling Green State University Department of Geology April 2013 Introduction: The Hermosa Group The Hermosa Group is a Pennsylvanian (~310 Ma) rock unit found in the southwestern San Juan Mountains and the Paradox Basin. The Paradox Basin is a northwest-southeast trending basin related to the Uncompahgre Uplift in the north, salt deposition and movement throughout, and a Precambrian fault system in the underlying basement rocks (Brown 2002, Trudgill and Arbuckle 2009). The Uncompahgre Uplift occurred in response to the Ouachita – Marathon Orogeny (related to the Ancestral Rocky Mountains Orogeny) caused by the collision of North America and South America-Africa during the Late Mississippian (~ 320 Ma) (Trudgill and Arbuckle 2009, Pazzaglia et al. 1999). The Paradox Basin formed as a complimentary subsidence basin alongside the uplifted area (Brown 2002). When the basin subsided, smaller structural features formed within it, including step-down grabens close to the uplift and folded areas further away (Baars and Stevenson 1981, Brown 2002). -
Geologic Story of Canyonlands National Park
«u GEOLOGICAL SURVEY BULLETIN 1327 JUL 1 7 1990 Dacus Library Wmthrop College Documents Department -T7 LOOKING NORTH FROM EAST WALL OF DEVILS LANE, just south of the Silver Stairs. Needles are Cedar Mesa Sandstone. Junction Butte and Grand View Point lie across Colorado River in background. GEOLOGICAL SURVEY BULLETIN 1327 UNITED STATES DEPARTMENT OF THE INTERIOR ROGERS C. B. MORTON, Secretary GEOLOGICAL SURVEY V. E. McKelvey, Director Library of Congress catalog-card No. 74-600043 Reprinted 1977 and 1990 U.S. GOVERNMENT PRINTING OFFICE : 1974 For sale by the Books and Open-File Reports Section, U.S. Geological Survey, Federal Center, Box 25425, Denver, CO 80225 . Contents Page A new park is born 1 Major Powell's river expeditions 4 Early history 9 Prehistoric people 9 Late arrivals 14 Geographic setting 17 Rocks and landforms 20 How to see the park 26 The high mesas 27 Island in the Sky 27 Dead Horse Point State Park 30 North entrance 34 Shafer and White Rim Trails 34 Grand View Point 36 Green River Overlook 43 Upheaval Dome 43 Hatch Point 46 Needles Overlook 47 Canyonlands Overlook 48 U-3 Loop 49 Anticline Overlook 50 Orange Cliffs 54 The benchlands 5g The Maze and Land of Standing Rocks 58 The Needles district 60 Salt, Davis, and Lavender Canyons _ 64 The Needles and The Grabens 73 Canyons of the Green and Colorado Rivers 85 Entrenched and cutoff meanders 86 Green River 87 Colorado River _ 96 Summary of geologic history H2 Additional reading H7 Acknowledgments H8 Selected references n% Index 123 VII Illustrations Page Frontispiece . -
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. -
Front Cover.Pub
PENNSYLVANIAN-PERMIAN VEGETATIONAL CHANGES IN TROPICAL EURAMERICA William A. DiMichele, C. Blaine Cecil, Dan S. Chaney, Scott D. Elrick, Spencer G. Lucas, Richard Lupia, W. John Nelson, and Neil J. Tabor INTRODUCTION Vegetational changes across the Pennsylvanian-Permian boundary are recorded in several largely terrestrial basins across the Euramerican portions of equatorial Pangea. For the purposes of this paper, these include the Bursum-Abo Formation transition and its equivalents in several small basins in New Mexico, the Halgaito Formation of southeastern Utah, Markley Formation of the eastern shelf of the Midland Basin in north-central Texas, Council Grove Group of northern Oklahoma and southern Kansas, and Dunkard Group of the central Appalachian Basin. This transition also is recorded in numerous basins in Europe, reviewed by Roscher and Schneider (2006), based on paleoclimate indicators preserved in those regions. Collectively, these deposits form a west-to-east transect across the Pangean paleotropics and thus provide a paleogeographic setting for examination of both temporal and spatial changes in vegetation across the Pennsylvanian-Permian boundary (Figures 1 and 2). The Pennsylvanian-Permian transition records the change from wetland vegetation as the predominant assemblages found in the plant fossil record, to seasonally dry vegetation. This has often been called the “Paleophytic-Mesophytic” transition, a concept that is flawed Figure 1. Continental configuration at the Pennsylvanian-Permian boundary. Yellow ovals indicate the principal areas discussed herein: Left – New Mexico and Utah, Center – Texas and Oklahoma, Right – Central Appalachians/Dunkard. Map courtesy of Ron Blakey, Northern Arizona University. DiMichele, W. A., Cecil, C. B., Chaney, D. S., Elrich, S. -
Geology of the Northern Portion of the Fish Lake Plateau, Utah
GEOLOGY OF THE NORTHERN PORTION OF THE FISH LAKE PLATEAU, UTAH DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State - University By DONALD PAUL MCGOOKEY, B.S., M.A* The Ohio State University 1958 Approved by Edmund M." Spieker Adviser Department of Geology CONTENTS Page INTRODUCTION. ................................ 1 Locations and accessibility ........ 2 Physical features ......... _ ................... 5 Previous w o r k ......... 10 Field work and the geologic map ........ 12 Acknowledgements.................... 13 STRATIGRAPHY........................................ 15 General features................................ 15 Jurassic system......................... 16 Arapien shale .............................. 16 Twist Gulch formation...................... 13 Morrison (?) formation...................... 19 Cretaceous system .............................. 20 General character and distribution.......... 20 Indianola group ............................ 21 Mancos shale. ................... 24 Star Point sandstone................ 25 Blackhawk formation ........................ 26 Definition, lithology, and extent .... 26 Stratigraphic relations . ............ 23 Age . .............................. 23 Price River formation...................... 31 Definition, lithology, and extent .... 31 Stratigraphic relations ................ 34 A g e .................................... 37 Cretaceous and Tertiary systems . ............ 37 North Horn formation. .......... -
An Inventory of Trilobites from National Park Service Areas
Sullivan, R.M. and Lucas, S.G., eds., 2016, Fossil Record 5. New Mexico Museum of Natural History and Science Bulletin 74. 179 AN INVENTORY OF TRILOBITES FROM NATIONAL PARK SERVICE AREAS MEGAN R. NORR¹, VINCENT L. SANTUCCI1 and JUSTIN S. TWEET2 1National Park Service. 1201 Eye Street NW, Washington, D.C. 20005; -email: [email protected]; 2Tweet Paleo-Consulting. 9149 79th St. S. Cottage Grove. MN 55016; Abstract—Trilobites represent an extinct group of Paleozoic marine invertebrate fossils that have great scientific interest and public appeal. Trilobites exhibit wide taxonomic diversity and are contained within nine orders of the Class Trilobita. A wealth of scientific literature exists regarding trilobites, their morphology, biostratigraphy, indicators of paleoenvironments, behavior, and other research themes. An inventory of National Park Service areas reveals that fossilized remains of trilobites are documented from within at least 33 NPS units, including Death Valley National Park, Grand Canyon National Park, Yellowstone National Park, and Yukon-Charley Rivers National Preserve. More than 120 trilobite hototype specimens are known from National Park Service areas. INTRODUCTION Of the 262 National Park Service areas identified with paleontological resources, 33 of those units have documented trilobite fossils (Fig. 1). More than 120 holotype specimens of trilobites have been found within National Park Service (NPS) units. Once thriving during the Paleozoic Era (between ~520 and 250 million years ago) and becoming extinct at the end of the Permian Period, trilobites were prone to fossilization due to their hard exoskeletons and the sedimentary marine environments they inhabited. While parks such as Death Valley National Park and Yukon-Charley Rivers National Preserve have reported a great abundance of fossilized trilobites, many other national parks also contain a diverse trilobite fauna.