IMPACTITES at the UPHEAVAL DOME STRUCTURE, UTAH? Christian Koeberl1, J
Total Page:16
File Type:pdf, Size:1020Kb
Load more
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]. -
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. -
The Summerville Formation: Evidence for a Sub-Horizontal Stratigraphic Sequence Below the Post-Rift Nu Conformity in the Middleton Place Summerville Seismic Zone
University of South Carolina Scholar Commons Theses and Dissertations 2017 The ummeS rville Formation: Evidence for a Sub- Horizontal Stratigraphic Sequence below the Post- Rift nconforU mity in the Middleton Place Summerville Seismic Zone Joseph Edward Getz University of South Carolina Follow this and additional works at: https://scholarcommons.sc.edu/etd Part of the Geology Commons Recommended Citation Getz, J. E.(2017). The Summerville Formation: Evidence for a Sub-Horizontal Stratigraphic Sequence below the Post-Rift nU conformity in the Middleton Place Summerville Seismic Zone. (Master's thesis). Retrieved from https://scholarcommons.sc.edu/etd/4177 This Open Access Thesis is brought to you by Scholar Commons. It has been accepted for inclusion in Theses and Dissertations by an authorized administrator of Scholar Commons. For more information, please contact [email protected]. THE SUMMERVILLE FORMATION: EVIDENCE FOR A SUB- HORIZONTAL STRATIGRAPHIC SEQUENCE BELOW THE POST-RIFT UNCONFORMITY IN THE MIDDLETON PLACE SUMMERVILLE SEISMIC ZONE By Joseph Edward Getz Bachelor of Arts University of South Carolina, 2013 Submitted in Partial Fulfillment of the Requirements For the Degree of Master of Science in Geological Sciences College of Arts and Sciences University of South Carolina 2017 Accepted by: James H. Knapp, Director of Thesis Camelia C. Knapp, Reader Andrew Leier, Reader Cheryl L. Addy, Vice Provost and Dean of the Graduate School © Copyright by Joseph Edward Getz, 2017 All Rights Reserved. ii DEDICATION I would like to dedicate this to my grandparents and my mother, for without their support none of this would have been possible. iii ACKNOWLEDGEMENTS I would like to give a special thanks my major advisor, Dr. -
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. -
Stromatolites in the Todilto Formation? Dana S
New Mexico Geological Society Downloaded from: http://nmgs.nmt.edu/publications/guidebooks/56 Stromatolites in the Todilto Formation? Dana S. Ulmer-Scholle, 2005, pp. 380-388 in: Geology of the Chama Basin, Lucas, Spencer G.; Zeigler, Kate E.; Lueth, Virgil W.; Owen, Donald E.; [eds.], New Mexico Geological Society 56th Annual Fall Field Conference Guidebook, 456 p. This is one of many related papers that were included in the 2005 NMGS Fall Field Conference Guidebook. Annual NMGS Fall Field Conference Guidebooks Every fall since 1950, the New Mexico Geological Society (NMGS) has held an annual Fall Field Conference that explores some region of New Mexico (or surrounding states). Always well attended, these conferences provide a guidebook to participants. Besides detailed road logs, the guidebooks contain many well written, edited, and peer-reviewed geoscience papers. These books have set the national standard for geologic guidebooks and are an essential geologic reference for anyone working in or around New Mexico. Free Downloads NMGS has decided to make peer-reviewed papers from our Fall Field Conference guidebooks available for free download. Non-members will have access to guidebook papers two years after publication. Members have access to all papers. This is in keeping with our mission of promoting interest, research, and cooperation regarding geology in New Mexico. However, guidebook sales represent a significant proportion of our operating budget. Therefore, only research papers are available for download. Road logs, mini-papers, maps, stratigraphic charts, and other selected content are available only in the printed guidebooks. Copyright Information Publications of the New Mexico Geological Society, printed and electronic, are protected by the copyright laws of the United States. -
Geology and Stratigraphy Column
Capitol Reef National Park National Park Service U.S. Department of the Interior Geology “Geology knows no such word as forever.” —Wallace Stegner Capitol Reef National Park’s geologic story reveals a nearly complete set of Mesozoic-era sedimentary layers. For 200 million years, rock layers formed at or near sea level. About 75-35 million years ago tectonic forces uplifted them, forming the Waterpocket Fold. Forces of erosion have been sculpting this spectacular landscape ever since. Deposition If you could travel in time and visit Capitol Visiting Capitol Reef 180 million years ago, Reef 245 million years ago, you would not when the Navajo Sandstone was deposited, recognize the landscape. Imagine a coastal you would have been surrounded by a giant park, with beaches and tidal flats; the water sand sea, the largest in Earth’s history. In this moves in and out gently, shaping ripple marks hot, dry climate, wind blew over sand dunes, in the wet sand. This is the environment creating large, sweeping crossbeds now in which the sediments of the Moenkopi preserved in the sandstone of Capitol Dome Formation were deposited. and Fern’s Nipple. Now jump ahead 20 million years, to 225 All the sedimentary rock layers were laid million years ago. The tidal flats are gone and down at or near sea level. Younger layers were the climate supports a tropical jungle, filled deposited on top of older layers. The Moenkopi with swamps, primitive trees, and giant ferns. is the oldest layer visible from the visitor center, The water is stagnant and a humid breeze with the younger Chinle Formation above it. -
Stratigraphic Correlation Chart for Western Colorado and Northwestern New Mexico
New Mexico Geological Society Guidebook, 32nd Field Conference, Western Slope Colorado, 1981 75 STRATIGRAPHIC CORRELATION CHART FOR WESTERN COLORADO AND NORTHWESTERN NEW MEXICO M. E. MacLACHLAN U.S. Geological Survey Denver, Colorado 80225 INTRODUCTION De Chelly Sandstone (or De Chelly Sandstone Member of the The stratigraphic nomenclature applied in various parts of west- Cutler Formation) of the west side of the basin is thought to ern Colorado, northwestern New Mexico, and a small part of east- correlate with the Glorieta Sandstone of the south side of the central Utah is summarized in the accompanying chart (fig. 1). The basin. locations of the areas, indicated by letters, are shown on the index map (fig. 2). Sources of information used in compiling the chart are Cols. B.-C. shown by numbers in brackets beneath the headings for the col- Age determinations on the Hinsdale Formation in parts of the umns. The numbers are keyed to references in an accompanying volcanic field range from 4.7 to 23.4 m.y. on basalts and 4.8 to list. Ages where known are shown by numbers in parentheses in 22.4 m.y. on rhyolites (Lipman, 1975, p. 6, p. 90-100). millions of years after the rock name or in parentheses on the line The early intermediate-composition volcanics and related rocks separating two chronostratigraphic units. include several named units of limited areal extent, but of simi- No Quaternary rocks nor small igneous bodies, such as dikes, lar age and petrology—the West Elk Breccia at Powderhorn; the have been included on this chart. -
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. -
Mesozoic Stratigraphy at Durango, Colorado
160 New Mexico Geological Society, 56th Field Conference Guidebook, Geology of the Chama Basin, 2005, p. 160-169. LUCAS AND HECKERT MESOZOIC STRATIGRAPHY AT DURANGO, COLORADO SPENCER G. LUCAS AND ANDREW B. HECKERT New Mexico Museum of Natural History and Science, 1801 Mountain Rd. NW, Albuquerque, NM 87104 ABSTRACT.—A nearly 3-km-thick section of Mesozoic sedimentary rocks is exposed at Durango, Colorado. This section con- sists of Upper Triassic, Middle-Upper Jurassic and Cretaceous strata that well record the geological history of southwestern Colorado during much of the Mesozoic. At Durango, Upper Triassic strata of the Chinle Group are ~ 300 m of red beds deposited in mostly fluvial paleoenvironments. Overlying Middle-Upper Jurassic strata of the San Rafael Group are ~ 300 m thick and consist of eolian sandstone, salina limestone and siltstone/sandstone deposited on an arid coastal plain. The Upper Jurassic Morrison Formation is ~ 187 m thick and consists of sandstone and mudstone deposited in fluvial environments. The only Lower Cretaceous strata at Durango are fluvial sandstone and conglomerate of the Burro Canyon Formation. Most of the overlying Upper Cretaceous section (Dakota, Mancos, Mesaverde, Lewis, Fruitland and Kirtland units) represents deposition in and along the western margin of the Western Interior seaway during Cenomanian-Campanian time. Volcaniclastic strata of the overlying McDermott Formation are the youngest Mesozoic strata at Durango. INTRODUCTION Durango, Colorado, sits in the Animas River Valley on the northern flank of the San Juan Basin and in the southern foothills of the San Juan and La Plata Mountains. Beginning at the northern end of the city, and extending to the southern end of town (from north of Animas City Mountain to just south of Smelter Moun- tain), the Animas River cuts in an essentially downdip direction through a homoclinal Mesozoic section of sedimentary rocks about 3 km thick (Figs. -
Sequence Stratigraphy, Diagenesis, and Depositional Facies of an Exposed Megaflap: Pennsylvanian Hermosa Group, Gypsum Valley Salt Wall, Paradox Basin, Colorado
SEQUENCE STRATIGRAPHY, DIAGENESIS, AND DEPOSITIONAL FACIES OF AN EXPOSED MEGAFLAP: PENNSYLVANIAN HERMOSA GROUP, GYPSUM VALLEY SALT WALL, PARADOX BASIN, COLORADO KYLE THOMAS DEATRICK Master’s Program in Geological Sciences APPROVED: Katherine A. Giles, Ph.D., Chair Richard P. Langford, Ph.D. Gary L. Gianniny, Ph.D. Stephen Crites, Ph. D. Dean of the Graduate School Copyright © by Kyle Thomas Deatrick 2019 Dedication I wish to dedicate this work to my family and friends, especially my parents Julie and Dennis Deatrick for their unwavering support and encouragement. SEQUENCE STRATIGRAPHY, DIAGENESIS, AND DEPOSITIONAL FACIES OF AN EXPOSED MEGAFLAP: PENNSYLVANIAN HERMOSA GROUP, GYPSUM VALLEY SALT WALL, PARADOX BASIN, COLORADO by KYLE THOMAS DEATRICK, B.S. Geology THESIS Presented to the Faculty of the Graduate School of The University of Texas at El Paso in Partial Fulfillment of the Requirements for the Degree of MASTER OF SCIENCE Department of Geological Sciences THE UNIVERSITY OF TEXAS AT EL PASO December 2019 ProQuest Number:27671333 All rights reserved INFORMATION TO ALL USERS The quality of this reproduction is dependent on the quality of the copy submitted. In the unlikely event that the author did not send a complete manuscript and there are missing pages, these will be noted. Also, if material had to be removed, a note will indicate the deletion. ProQuest 27671333 Published by ProQuest LLC (2020). Copyright of the Dissertation is held by the Author. All Rights Reserved. This work is protected against unauthorized copying under Title 17, United States Code Microform Edition © ProQuest LLC. ProQuest LLC 789 East Eisenhower Parkway P.O. Box 1346 Ann Arbor, MI 48106 - 1346 Acknowledgements I wish to thank my committee members whose time and support provided tremendous input into my research. -
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. -
Oil and Gas Plays Ute Moutnain Ute Reservation, Colorado and New Mexico
Ute Mountain Ute Indian Reservation Cortez R18W Karle Key Xu R17W T General Setting Mine Xu Xcu 36 Can y on N Xcu McElmo WIND RIVER 32 INDIAN MABEL The Ute Mountain Ute Reservation is located in the northwest RESERVATION MOUNTAIN FT HALL IND RES Little Moude Mine Xcu T N ern portion of New Mexico and the southwestern corner of Colorado UTE PEAK 35 N R16W (Fig. UM-1). The reservation consists of 553,008 acres in Montezu BLACK 666 T W Y O M I N G MOUNTAIN 35 R20W SLEEPING UTE MOUNTAIN N ma and La Plata Counties, Colorado, and San Juan County, New R19W Coche T Mexico. All of these lands belong to the tribe but are held in trust by NORTHWESTERN 34 SHOSHONI HERMANO the U.S. Government. Individually owned lands, or allotments, are IND RES Desert Canyon PEAK N MESA VERDE R14W NATIONAL GREAT SALT LAKE W Marble SENTINEL located at Allen Canyon and White Mesa, San Juan County, Utah, Wash Towaoc PARK PEAK T and cover 8,499 acres. Tribal lands held in trust within this area cov Towaoc River M E S A 33 1/2 N er 3,597 acres. An additional forty acres are defined as U.S. Govern THE MOUND R15W SKULL VALLEY ment lands in San Juan County, Utah, and are utilized for school pur TEXAS PACIFIC 6-INCH OIL PIPELINE IND RES UNITAH AND OURAY INDIAN RESERVATION Navajo poses. W Ramona GOSHUTE 789 The Allen Canyon allotments are located twelve miles west of IND RES T UTAH 33 Blanding, Utah, and adjacent to the Manti-La Sal National Forest.