Potential for Potable Groundwater on State Land Near Canyonlands
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Geological Processes and Evolution
GEOLOGICAL PROCESSES AND EVOLUTION J.W. HEAD1, R. GREELEY2, M.P. GOLOMBEK3, W.K. HARTMANN4, E. HAUBER5, R. JAUMANN5, P. MASSON6, G. NEUKUM5, L.E. NYQUIST7 and M.H. CARR8 1Department of Geological Sciences, Brown University, Providence, RI 02912 USA 2Department of Geology, Arizona State University, Tempe, AZ 85287 USA 3Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109 USA 4Planetary Science Institute, Tucson, AZ 85705 USA 5DLR Institute of Space Sensor Technology and Planetary Exploration, Rutherfordstrasse 2, 12484 Berlin-Aldershof, Germany 6University of Paris-Sud, 91405, Orsay Cedex France 7Johnson Space Center, Houston TX 77058 USA 8US Geological Survey, Branch of Astrogeological Studies, 345 Middlefield Road, Menlo Park, CA 94025 USA Received:14 February 2001; accepted:12 March 2001 Abstract. Geological mapping and establishment of stratigraphic relationships provides an overview of geological processes operating on Mars and how they have varied in time and space. Impact craters and basins shaped the crust in earliest history and as their importance declined, evidence of extensive regional volcanism emerged during the Late Noachian. Regional volcanism characterized the Early Hesperian and subsequent to that time, volcanism was largely centered at Tharsis and Elysium, con- tinuing until the recent geological past. The Tharsis region appears to have been largely constructed by the Late Noachian, and represents a series of tectonic and volcanic centers. Globally distributed structural features representing contraction characterize the middle Hesperian. Water-related pro- cesses involve the formation of valley networks in the Late Noachian and into the Hesperian, an ice sheet at the south pole in the middle Hesperian, and outflow channels and possible standing bodies of water in the northern lowlands in the Late Hesperian and into the Amazonian. -
What Is the Zuni Sandstone Today
What is the ZuniSandstone Today -- 100 Years AfterDutton? A Discussion andReview of JurassicStratigraphy in West-Central New Mexico NEW MEXICO BUREAU OF MINES AND MINERAL RESOURCES OPEN-FILE REPORT 174 by Orin J. Anderson New MexicoBureau of Minesand Mineral Resources 1983 Contents Introduction P. 1 Discussion P. 3 Todilto Limestone - Navajo Sandstone P- 5 San Rafael Group Defined P. 8 Glen CanyonGroup Defined P. 9 MorrisonFormation Subdivided p. 14 Cow SpringsSandstone p. 17 1956 Memorandum from C. H. Dane p. 22 Zuni Sandstone Redefined p. 26 Summary p. 28 ReferencesCited p. 30 Figures Fig. 1 Index map of study area Fig. 2 Stratigraphic nomenclature and correlationchart- 1885 to present Fig. 3 Measured section at type locality of Zuni Sandstone (inside back cover) Fig. 4 Stratigraphiccross-section-Dakota and Zuni sandstones, showing southward thinning of Zuni Sandstone (inside back cover) WHAT IS THE ZUNISANDSTONE TODAY -- 100 YEARS AFTER DUTTON? A DISCUSSION AND REVIEW OF JURASSICSTRATIGRAPHY IN WEST-CENTRAL NEW MEXICO Introduction The massivesequence(s) of light colored, cross bedded sandstonesthat underliethe Dakota Sandstone (Upper Cretaceous) in west-central New Mexico and northeasternArizona were first described and namedby CaptainClarence E. Dutton ofthe U. S. Army Ordinance Corps. His reportentitled "Mount Taylor and the Zuni Plateau"(Dutton, 1885) contains an account of the stratigraphy and structure of those two areas and theimmediately surrounding region(the Zuni Plateau is thepresent day Zuni uplift). In thereport he described a "massive bright redsandstone" that overlies the "basal Triassediments" (the present day ChinleFormation) in theFort Wingate area; this unit henamed "provisionally"the Wingate Sandstone. Overlyingthe Wingate Dutton recognized "a series ofsandstones and sandy shales ..... -
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 . -
Stratigraphy and Sedimentology of a Dry to Wet Eolian Depositional System, Burns Formation, Meridiani Planum, Mars
Earth and Planetary Science Letters 240 (2005) 11–72 www.elsevier.com/locate/epsl Stratigraphy and sedimentology of a dry to wet eolian depositional system, Burns formation, Meridiani Planum, Mars J.P. Grotzinger a,*, R.E. Arvidson b, J.F. Bell III c, W. Calvin d, B.C. Clark e, D.A. Fike a, M. Golombek f, R. Greeley g, A. Haldemann f, K.E. Herkenhoff h, B.L. Jolliff b, A.H. Knoll i, M. Malin j, S.M. McLennan k, T. Parker e, L. Soderblom g, J.N. Sohl-Dickstein b, S.W. Squyres b, N.J. Tosca k, W.A. Watters a a Massachusetts Inst. of Technology, Earth, Atmos. and Planetary Sci., Cambridge, MA 02139, USA b Department Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA c Department of Astronomy, Space Sciences Bldg. Cornell University, Ithaca, NY 14853, USA d University of Nevada, Reno, NV 89501, USA e Lockheed Martin Corporation, Littleton, CO 80127, USA f Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA g Department Geological Sciences, Arizona State University, Box 871404, Tempe, AZ 85287-1404, USA h U.S. Geological Survey, Flagstaff, AZ 86001, USA i Botanical Museum, Harvard University, Cambridge MA 02138, USA j Malin Space Science Systems, Inc., San Diego, CA 92191, USA k Department of Geosciences, State University of New York, Stony Brook, NY 11794-2100, USA Accepted 22 September 2005 Editor: A.N. Halliday Abstract Outcrop exposures of sedimentary rocks at the Opportunity landing site (Meridiani Planum) form a set of genetically related strata defined here informally as the Burns formation. -
A Stratigraphic Section That Traverses the Noachian-Hesperian Capturing Diverse Habitable Environments
42nd Lunar and Planetary Science Conference (2011) 2355.pdf A STRATIGRAPHIC SECTION THAT TRAVERSES THE NOACHIAN-HESPERIAN CAPTURING DIVERSE HABITABLE ENVIRONMENTS. J. F. Mustard1 and B. L. Ehlmann1, 1Department of Geological Sciences, Box 1846, Brown University, Providence, RI 02912 [email protected]. Introduction: The evolution of distinct eras on enigmatic unit. It generally lies in local topographic Mars defined by specific hydrous mineral phases as lows, though it is observed to drape underlying topog- proposed by [1] provides a broad framework for as- raphy defined by the basement. In some places the sessing the nature of habitable environments and the spectroscopic signature is definitively olivine-bearing interaction of water with the crust and surface through [5, 6], while others the olivine signatures are supple- time. If processes on early Mars that resulted in altera- mented by absorptions diagnostic of magnesite [7]. In tion mineralogies dominated by phyllosilicate were a few regions serpentine is also detected in association followed by processes resulting in sulfate and other with olivine [8]. In the study region this unit is almost evaporite minerals during the middle period of Mars’ exclusively magnesite-bearing. Where well exposed it then it will be critical to identify and understand re- typically shows an irregular polygonal fracturing on gions of the crust that record these transitions. These the scale of meters. The olivine-magnesite unit is localities will capture a fundamental reorganization of commonly capped by a medium-toned spectrally bland aqueous processes on a planetary scale. The region of unit that preserves impact craters. The thickness of the the western Isidis Basin that transitions to the volcanic two units is on the order of several 10s of meters. -
North American Stratigraphic Code1
NORTH AMERICAN STRATIGRAPHIC CODE1 North American Commission on Stratigraphic Nomenclature FOREWORD TO THE REVISED EDITION FOREWORD TO THE 1983 CODE By design, the North American Stratigraphic Code is The 1983 Code of recommended procedures for clas- meant to be an evolving document, one that requires change sifying and naming stratigraphic and related units was pre- as the field of earth science evolves. The revisions to the pared during a four-year period, by and for North American Code that are included in this 2005 edition encompass a earth scientists, under the auspices of the North American broad spectrum of changes, ranging from a complete revision Commission on Stratigraphic Nomenclature. It represents of the section on Biostratigraphic Units (Articles 48 to 54), the thought and work of scores of persons, and thousands of several wording changes to Article 58 and its remarks con- hours of writing and editing. Opportunities to participate in cerning Allostratigraphic Units, updating of Article 4 to in- and review the work have been provided throughout its corporate changes in publishing methods over the last two development, as cited in the Preamble, to a degree unprece- decades, and a variety of minor wording changes to improve dented during preparation of earlier codes. clarity and self-consistency between different sections of the Publication of the International Stratigraphic Guide in Code. In addition, Figures 1, 4, 5, and 6, as well as Tables 1 1976 made evident some insufficiencies of the American and Tables 2 have been modified. Most of the changes Stratigraphic Codes of 1961 and 1970. The Commission adopted in this revision arose from Notes 60, 63, and 64 of considered whether to discard our codes, patch them over, the Commission, all of which were published in the AAPG or rewrite them fully, and chose the last. -
Lithostratigraphic Units
INTEGRATED STRATIGRAPHY Amalia Spina Amalia Spina, PhD. Office: Palazzina di Geologia, Second floor Tel. 0755852696 E-mail: [email protected] - Principles of stratigraphy - The time in stratigraphy; geological chronology (relative and absolute) the temporal sequence of events; standard global chronostratigraphical scale. Comparison between the stratigraphic scales in marine and continental successions. - Stratigraphic units standard (definition and principle): law of superimposition, principle of original horizontality, of lateral continuity and of biotic succession, the Stratigraphic Code. - The sedimentary cyclicity - Lithostratigraphy - Magnetostratigraphy - Biostratigraphy - Chemostratigraphy - Cronostratigraphy and geochronology - Astronomic cyclostratigraphy - Sequence stratigraphy - Palaeogeographic reconstructions. Prerequisites: In order to better comprehend the main topics of integrated stratigraphy, the students that follow this course must have: - knowledge of the fundamentals of geology; - knowledge of the sedimentary rocks (classification); - knowledge of the principle of stratigraphy; - knowledge of the principle of palaeontology; - knowledge of the principle of sedimentology; These preconditions are important for attending and not attending students. Written test: it consist of the solution of multiple choice test and graphic /practical exercises. The number of questions ranges between 15 and 30 on the basis of the difficulty.The test has a duration of no more than 80 minutes. The goal of the test is to verify the knowledge acquired on the course contents in order to ensure that the student learned the principles of integrated stratigraphy and its main applications. To complete the evaluation the test also consists on the discussion of a case study proposed by the Professor carried out individually or in small groups (max three students).It consists to discuss the stratigraphic features of a certain geological area and the implications for the subsurface hydrocarbon exploitation. -
Flood Surfaces and Deflation Surfaces Within the Cutler Formation and Cedar Mesa Sandstone (Permian), Southeastern Utah
Flood surfaces and deflation surfaces within the Cutler Formation and Cedar Mesa Sandstone (Permian), southeastern Utah RICHARD LANGFORD 1 „ „ . tr, , . „ , . „ . , rr . r , , , . 0,,,, MARJORIE A CHAN J Department of Geology and Geophysics, University of Utah, Salt Lake City, Utah 84112 ABSTRACT of dune masses and intervening interdune deposits results in the formation of first-order bounding surfaces (Mckee and Moiola,1975; Brookfield, Areally extensive erosion surfaces in eolian deposits have been 1977; Rubin and Hunter, 1982). First-order surfaces are limited in areal interpreted as long hiatuses in eolian deposition. Such erosion surfaces extent (several square kilometers) and form during relatively continuous form during deflationary episodes or during periods of erg stabiliza- eolian deposition. tion or contraction). They are called "super surfaces" and can be useful for stratigraphic correlation because of their regional extent. TOie Permian Cedar Mesa Sandstone and Cutler Formation con- tain a type of super surface (herein termed "flood surfaces"), -10-400+ tan2. Flood surfaces form as a result of fluvial floods into active dune seas. The surfaces may expand through nonclimbing mi- gration of eolian dunes but do not imply long hiatuses in eolian deposi- tion as do other types of super surfaces. Cutler and Cedar Mesa flood surfaces are overlain by shales and sandstones which thicken laterally and merge with fluvial channel-fill deposits. Flooding of active dune fields in the Cedar Mesa Sandstone is suggested by intertonguing of eolian dune and fluvial deposits. Flood surfaces can easily be mistaken for deflationary super surfaces but are distinguished by evidence of dune migration coincident with flood events and by an increase in the number of surfaces adjacent to associated aqueous deposits. -
Canyon Country
CANYONLANDS TRAVEL REGION ANYONANYON OUNTRYOUNTRY CCA Land Of EnchantmentCC his vast rock desert in southeastern Utah showcases deep, colorful T canyons, majestic natural monuments pictured in western movies, a fantasy land of towering pinnacles and slot canyons, rock arches and ANYONANYON OUNTRYOUNTRY bridges, and breathtaking vistas atop mesas. Much can be seen by car, and more of this endlessly intriguing country is accessible by foot, mountain Explanation CC CC bike, four-wheel-drive vehicle, or watercraft. Collapsed salt anticline You do not have to be a geologist to enjoy or interpret the scenery, for the Arches rocks easily divulge their stories of forming in seas or on land, in deserts or in deltas, in rivers or along beaches. What a fascinating heritage: dinosaurs Bridges once sauntered through lush lowlands leaving huge footprints in mud that Petroglyphs has now turned to rock, vast sand dunes that drifted across the area are Dinosaur tracks preserved as large sweeping lines in sandstone walls, and oceans that once Indian ruins covered this region left fossilized corals and seashells embedded in lime- Paradox basin salt boundary stone. Parks, monuments, recreation areas This guide introduces you to the rocks’ stories, to enhance your travels and Indian reservations your appreciation of the region. Along designated scenic byways, which are portrayed at the end of this pamphlet, look for the specific features Scenic byways described here and learn what their journey has been as you make yours. During your visit, tread lightly on this delicate land so that the pristine and 0 10 20 miles unique landscape remains unchanged. -
Late Quaternary Eolian and Alluvial Response to Paleoclimate, Canyonlands, Southeastern Utah
Late Quaternary eolian and alluvial response to paleoclimate, Canyonlands, southeastern Utah Marith C. Reheis† Richard L. Reynolds Harland Goldstein U.S. Geological Survey, MS-980, Federal Center, Box 25046, Denver, Colorado 80225, USA Helen M. Roberts Institute of Geography and Earth Sciences, University of Wales, Aberystwyth SY23 3DB, Wales, UK James C. Yount U.S. Geological Survey, MS-980, Federal Center, Box 25046, Denver, Colorado 80225, USA Yarrow Axford Institute of Arctic and Alpine Research, University of Colorado, Boulder, Colorado 80309, USA Linda Scott Cummings Paleo Research Institute, 2675 Youngfi eld Street, Golden, Colorado 80401, USA Nancy Shearin Bureau of Land Management, Monticello Field Offi ce, Monticello, Utah 84535, USA ABSTRACT began at ca. 6 ka and ended by ca. 3–2 ka, fol- sheets and dunes are common features of semi- lowed by a shift to drier modern conditions; arid regions, and their deposits and intercalated In upland areas of Canyonlands National localized mobilization of dune sand has per- paleosols potentially contain a long-term record Park, Utah, thin deposits and paleosols show sisted to the present. These interpretations of landscape response to climate fl uctuations. late Quaternary episodes of eolian sedimen- are similar to those of studies at the Chaco Mineral dust may strongly infl uence land- tation, pedogenesis, and climate change. dune fi eld, New Mexico, and the Tusayan scapes and ecosystems by adding materials to Interpretation of the stratigraphy and opti- dune fi eld, Arizona, and are consistent with soils that change their properties (e.g., Reheis cally stimulated luminescence ages of eolian paleoclimate interpretations of pollen and et al., 1995; Simonson, 1995; Herrmann et al., and nearby alluvial deposits, their pollen, packrat middens in the region. -
Geologic Resource Evaluation Report, Capitol Reef National Park
National Park Service U.S. Department of the Interior Natural Resource Program Center Capitol Reef National Park Geologic Resource Evaluation Report Natural Resource Report NPS/NRPC/GRD/NRR—2006/005 Capitol Reef National Park Geologic Resource Evaluation Report Natural Resource Report NPS/NRPC/GRD/NRR—2006/005 Geologic Resources Division Natural Resource Program Center P.O. Box 25287 Denver, Colorado 80225 September 2006 U.S. Department of the Interior Washington, D.C. The Natural Resource Publication series addresses natural resource topics that are of interest and applicability to a broad readership in the National Park Service and to others in the management of natural resources, including the scientific community, the public, and the NPS conservation and environmental constituencies. Manuscripts are peer-reviewed to ensure that the information is scientifically credible, technically accurate, appropriately written for the intended audience, and is designed and published in a professional manner. Natural Resource Reports are the designated medium for disseminating high priority, current natural resource management information with managerial application. The series targets a general, diverse audience, and may contain NPS policy considerations or address sensitive issues of management applicability. Examples of the diverse array of reports published in this series include vital signs monitoring plans; "how to" resource management papers; proceedings of resource management workshops or conferences; annual reports of resource programs or divisions of the Natural Resource Program Center; resource action plans; fact sheets; and regularly-published newsletters. Views and conclusions in this report are those of the authors and do not necessarily reflect policies of the National Park Service. Mention of trade names or commercial products does not constitute endorsement or recommendation for use by the National Park Service. -
Paleontology of the Bears Ears National Monument
Paleontology of Bears Ears National Monument (Utah, USA): history of exploration, study, and designation 1,2 3 4 5 Jessica Uglesich , Robert J. Gay *, M. Allison Stegner , Adam K. Huttenlocker , Randall B. Irmis6 1 Friends of Cedar Mesa, Bluff, Utah 84512 U.S.A. 2 University of Texas at San Antonio, Department of Geosciences, San Antonio, Texas 78249 U.S.A. 3 Colorado Canyons Association, Grand Junction, Colorado 81501 U.S.A. 4 Department of Integrative Biology, University of Wisconsin-Madison, Madison, Wisconsin, 53706 U.S.A. 5 University of Southern California, Los Angeles, California 90007 U.S.A. 6 Natural History Museum of Utah and Department of Geology & Geophysics, University of Utah, 301 Wakara Way, Salt Lake City, Utah 84108-1214 U.S.A. *Corresponding author: [email protected] or [email protected] Submitted September 2018 PeerJ Preprints | https://doi.org/10.7287/peerj.preprints.3442v2 | CC BY 4.0 Open Access | rec: 23 Sep 2018, publ: 23 Sep 2018 ABSTRACT Bears Ears National Monument (BENM) is a new, landscape-scale national monument jointly administered by the Bureau of Land Management and the Forest Service in southeastern Utah as part of the National Conservation Lands system. As initially designated in 2016, BENM encompassed 1.3 million acres of land with exceptionally fossiliferous rock units. Subsequently, in December 2017, presidential action reduced BENM to two smaller management units (Indian Creek and Shash Jáá). Although the paleontological resources of BENM are extensive and abundant, they have historically been under-studied. Here, we summarize prior paleontological work within the original BENM boundaries in order to provide a complete picture of the paleontological resources, and synthesize the data which were used to support paleontological resource protection.