Studies of the Chesapeake Bay Impact Structure— Introduction and Discussion
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Cross-References ASTEROID IMPACT Definition and Introduction History of Impact Cratering Studies
18 ASTEROID IMPACT Tedesco, E. F., Noah, P. V., Noah, M., and Price, S. D., 2002. The identification and confirmation of impact structures on supplemental IRAS minor planet survey. The Astronomical Earth were developed: (a) crater morphology, (b) geo- 123 – Journal, , 1056 1085. physical anomalies, (c) evidence for shock metamor- Tholen, D. J., and Barucci, M. A., 1989. Asteroid taxonomy. In Binzel, R. P., Gehrels, T., and Matthews, M. S. (eds.), phism, and (d) the presence of meteorites or geochemical Asteroids II. Tucson: University of Arizona Press, pp. 298–315. evidence for traces of the meteoritic projectile – of which Yeomans, D., and Baalke, R., 2009. Near Earth Object Program. only (c) and (d) can provide confirming evidence. Remote Available from World Wide Web: http://neo.jpl.nasa.gov/ sensing, including morphological observations, as well programs. as geophysical studies, cannot provide confirming evi- dence – which requires the study of actual rock samples. Cross-references Impacts influenced the geological and biological evolu- tion of our own planet; the best known example is the link Albedo between the 200-km-diameter Chicxulub impact structure Asteroid Impact Asteroid Impact Mitigation in Mexico and the Cretaceous-Tertiary boundary. Under- Asteroid Impact Prediction standing impact structures, their formation processes, Torino Scale and their consequences should be of interest not only to Earth and planetary scientists, but also to society in general. ASTEROID IMPACT History of impact cratering studies In the geological sciences, it has only recently been recog- Christian Koeberl nized how important the process of impact cratering is on Natural History Museum, Vienna, Austria a planetary scale. -
RI37 Stratigraphic Nomenclature Of
,--' ( UNIVERSITY OF DELAWARE DELAWARE GEOLOGICAL SURVEY REPORT OF INVESTIGATIONS NO.37 STRATIGRAPHIC NOMENCLATURE OF NONMARINE CRETACEOUS ROCKS OF INNER MARGIN OF COASTAL PLAIN IN DELAWARE AND ADJACENT STATES BY ROBERT R. JORDAN STATE OF DELAWARE.. NEWARK, DELAWARE JUNE 1983 STRATIGRAPHIC NOMENCLATURE OF NONMARINE CRETACEOUS ROCKS OF INNER MARGIN OF COASTAL PLAIN IN DELAWARE AND ADJACENT STATES By Robert R. Jordan Delaware Geological Survey June 1983 TABLE OF CONTENTS Page ABSTRACT. ....... 1 INTRODUCTION ..... 2 Purpose and Scope. 2 Acknowledgments.. 4 REGIONAL SETTING. 4 Regional Relationships . 4 Structural Features. 5 DESCRIPTIONS OF UNITS .. 8 Historical Summary 8 Potomac Formation. 13 Nomenclature. 13 Extent. 13 Lithology . 14 Patuxent Formation . 18 Nomenclature. 18 Extent.. 18 Lithology .... 18 Arundel Formation. 19 Nomenclature.. 19 Extent. .• 19 Lithology • 20 Page Patapsco Formation. .. 20 Nomenclature . 20 Extent .. 20 Lithology.. 20 Raritan Formation . 21 Nomenclature .. 21 Extent .. 22 Lithology.. 23 Magothy Formation .. 24 Nomenclature . 24 Extent .. 24 Lithology.. 25 ENVIRONMENTS OF DEPOSITION 28 AGES .... 29 SUBDIVISIONS AND CORRELATIONS .. 32 REFERENCES . 34 ILLUSTRATIONS Figure 1. Geologic map of nonmarine Cretaceous deposits .. ..•.• •.. 3 2. Structural features of the Coastal Plain. ............ 6 3. Schematic diagram of lateral and vertical relationships of nonmarine Cretaceous deposits•....•... 34 TABLES Page Table 1. Usage of group and formation names. 9 STRATIGRAPHIC NOMENCLATURE OF NONMARINE CRETACEOUS ROCKS OF INNER MARGIN OF COASTAL PLAIN IN DELAWARE AND ADJACENT STATES ABSTRACT Rocks of Cretaceous age deposited in continental and marginal environments, and now found along the inner edge of the northern Atlantic Coastal Plain, have historically been classified as the Potomac Group and the Potomac, Patuxent, Arundel, Patapsco, Raritan, and Magothy forma tions. -
AASG Geothermal Data Metadata Template
Geothermal References Allen, E.P., Wilson, W.F., 1968, Geology and Mineral Resources of Orange County, North Carolina, North Carolina Geologic Survey, Bulletin 81, pp58 Allingham, J.W., 1970, Principal Facts for Gravity Stations in Howard County, MD, U.S. Geological Survey Open File Report 70-4, 19 pp. Amsden, T.W., Overbeck, R.M., and Martin, R.O.R., 1954, The Water Resources of Garrett County: Maryland Geological Survey, Bulletin 13, 3 plates, 349 p. Anderson, Campbell, 1976, Soil Characteristics of the Litholigic Units of Wake County, North Carolina, Open-File Report 73-1, North Carolina Geological Survey Anderson, D.N., and J.W. Lund (eds.), 1979, Direct Utilization of Geothermal Energy: A Layman's Guide, Geothermal Resources Council, Special Report No. 8, Davis, California, under U.S. DOE Contract ET-78-G-06- Anderson, J., 1948, Cretaceous and Tertiary Subsurface Geology: The Stratigraphy, Paleontology, and Sedimentology of Three Deep Test Wells on the Eastern Shore of Maryland: Maryland Geological Survey, Bulletin Andres, A.S., 2004, The Cat Hill Formation and Bethany Formation of Delaware: Delaware Geological Survey, Report of Investigation 67, 12 p. Andres, A.S., and C.S. Howard, 2000, RI62 The Cypress Swamp Formation, Delaware: Delaware Geological Survey, Report of Investigation 62, 18 p. Andres, A.S., Martin, M.J., 2005, Estimation of the Water Table for the Inland Bays Watershed, Delaware, Delaware Geological Survey Report of Investigations 68, 21 pp Andres, A.S., R.N. Benson, K.W. Ramsey, and J.H. Talley, 1990, Geologic and Hydrologic Studies of the Oligocene- Pleistocene Section Near Lewes, Delaware: Delaware Geological Survey, Report of Investigations 48, 39p. -
Extraordinary Rocks from the Peak Ring of the Chicxulub Impact Crater: P-Wave Velocity, Density, and Porosity Measurements from IODP/ICDP Expedition 364 ∗ G.L
Earth and Planetary Science Letters 495 (2018) 1–11 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Extraordinary rocks from the peak ring of the Chicxulub impact crater: P-wave velocity, density, and porosity measurements from IODP/ICDP Expedition 364 ∗ G.L. Christeson a, , S.P.S. Gulick a,b, J.V. Morgan c, C. Gebhardt d, D.A. Kring e, E. Le Ber f, J. Lofi g, C. Nixon h, M. Poelchau i, A.S.P. Rae c, M. Rebolledo-Vieyra j, U. Riller k, D.R. Schmitt h,1, A. Wittmann l, T.J. Bralower m, E. Chenot n, P. Claeys o, C.S. Cockell p, M.J.L. Coolen q, L. Ferrière r, S. Green s, K. Goto t, H. Jones m, C.M. Lowery a, C. Mellett u, R. Ocampo-Torres v, L. Perez-Cruz w, A.E. Pickersgill x,y, C. Rasmussen z,2, H. Sato aa,3, J. Smit ab, S.M. Tikoo ac, N. Tomioka ad, J. Urrutia-Fucugauchi w, M.T. Whalen ae, L. Xiao af, K.E. Yamaguchi ag,ah a University of Texas Institute for Geophysics, Jackson School of Geosciences, Austin, USA b Department of Geological Sciences, Jackson School of Geosciences, Austin, USA c Department of Earth Science and Engineering, Imperial College, London, UK d Alfred Wegener Institute Helmholtz Centre of Polar and Marine Research, Bremerhaven, Germany e Lunar and Planetary Institute, Houston, USA f Department of Geology, University of Leicester, UK g Géosciences Montpellier, Université de Montpellier, France h Department of Physics, University of Alberta, Canada i Department of Geology, University of Freiburg, Germany j SM 312, Mza 7, Chipre 5, Resid. -
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. -
Bills Paid by Payee Second Quarter Fiscal Year 20/21
BILLS PAID BY PAYEE SECOND QUARTER FISCAL YEAR 20/21 A complete detailed record is available at the Elko County Comptroller's Office. Office Hours: Monday-Friday 8:00A.M. until 5:00P.M. 540 Court St. Suite 101 Elko, NV 89801 Office Phone (775)753-7073*Disclaimer-The original and any duplicate or copy of each receipt, bill,check,warrant,voucher or other similar document that supports a transaction, the amount of which is shown in the total of this report, along with the name of the person whom such allowance is made and the purpose of the allowance, is a public record that is available for inspection and copying by any person pursuant to the provisions of chapter 239 of NRS. VENDOR CHECK ARGO COMPANY, INC 821.98 A ARNOLD BECK CONSTRUCTION 1,599.40 AT&T 3,697.06 5TH GEAR POWER SPORTS 41.74 AT&T MOBILITY 42.24 A PLUS URGENT CARE 766 AUTO GRAPHICS 400 A PLUS URGENT CARE ELKO 846.33 B A-1 RADIATOR REPAIR INC. 1,079.00 BARBARA J HOFHEINS 121.9 ACKERMAN MATTHEW 1388.93 BARBARA JO MAPLE 762.5 ADVANCE AUTO CARE 629.89 BARRY RENTAL 86.03 ADVANCED RADIOLOGY 1195.5 BEI CAPELI 5,000.00 AIRGAS 541.3 BERTOLINI VALVES INC 1,859.12 AIRPORT SHELL 9 BETTY HICKS 177.56 ALCOHOL MONITORING SYSTEMS INC 791 BLAINE ROBINSON & NIKIERA CAST 1,132.00 ALERTUS TECHNOLOGIES LLC 4,950.00 BLOHM JEWELERS INC 5,000.00 ALICIA GUAMAN 58 BLUE 360 MEDIA LLC 70.75 ALLIED UNIVERAL SECURITY SERVI 37,229.50 BOARD OF REGENTS 14300.04 ALLUSIVE IMAGES 5,000.00 BOB BARKER COMPANY 4418.55 ALYSSA K DANN 120 BONANZA PRODUCE 320.23 AMANDA JEAN GIRMAUDO 160 BOSS TANKS 5,024.00 AMBER DAWN -
A Possible Albian Impact Crater at Murshid, Southern Oman
GeoArabia, Vol. 7, No. 4, 2002 Gulf PetroLink, Bahrain A possible Albian impact crater at Murshid, southern Oman Bruce Levell1, Pascal Richard2 and Folco Hoogendijk2, Petroleum Development Oman ABSTRACT During interpretation of a 3-D seismic survey in southern Oman a solitary, 2.5-km-wide circular basin with a central peak and raised rim was identified in the subsurface 35 km west of the Marmul oil field. The feature is the only one of its kind in the area. The basinal structure is probably of Late Cretaceous (Albian) age and the regional geology strongly suggests that it is neither a volcanic crater nor related to salt-dome tectonics or salt dissolution. It possibly represents a crater formed by a terrestrial impact event and has been named the Murshid crater. This report does not constitute a detailed investigation of the possible impact crater but rather records the 3-D seismic observations and the drilling that has taken place near the structure so far. INTRODUCTION During interpretation of a newly acquired 3-D seismic survey for oil exploration in southern Oman, a solitary 2.5-km-diameter circular basinal feature was identified as a possible impact structure and was named the Murshid crater. It lies 35 km west of the Marmul oil field in the South Oman Salt Basin (Figure 1). The center of the structure is at latitude 18º10’59"N, longitude 54º55’08”E, and it is buried at a depth of approximately 380 m below mean sea level (680 m below the ground surface). The authors are petroleum geologists who felt that the Murshid basinal structure needed reporting to the wider scientific community. -
COMMONWEALTH of VIRGINIA DEPARTMENT of CONSERVATION and ECONOMIC DEVELOPMENT DIVISION of MINERAL RESOURCES Robert C
VIRGINIA DIVISION OF MINERAL RESOURCES PUBLICATION 20 GEOLOGY OF THE OAK GROVE CORE . e- 1lg**** - rlrl""*"-*-lq j4;i; s" r "e .-e l;"* l* - :-* l,i.l-1" -*"4{ ' *-q-S''q-"_ l -a,T-,! - !:: ts"--l ::9: : ::5 :e 'l I ." t::::,:1,a::-:d:; r--" 4 f-d;:s ,:,S r,! ,:a:16:":, 9:-4:-:r:: -':"-lii;3? -F - d,* COMMONWEALTH OF VIRGINIA DEPARTMENT OF CONSERVATION AND ECONOMIC DEVELOPMENT DIVISION OF MINERAL RESOURCES Robert C. Milici, Commissioner of Mineral Resources and State Geologist CHARLOTTESVILLE, VIRGINIA 1980 VIRGINIA DIVISION OF MINERAL RESOURCES PUBLICATION 20 GEOLOGY OF THE OAK GROVE CORE COMMONWEALTH OF VI RGINIA DEPARTMENT OF CONSERVATION AND ECONOMIC DEVELOPMENT DIVISION OF MINERAL RESOURCES Robert C. Milici, Commissioner of Mineral Resources and State Geologist CHAR LOTTESVI LLE, VI RGI N IA 1980 VIRGINIA DIVISION OF MINERAL RESOURCES PUBLICATION 20 GEOLOGY OF THE OAK GROVE CORE COMMONWEALTH OF VI RGIN IA DEPARTMENT OF CONSERVATION AND ECONOMIC DEVELOPMENT DIVISION OF MINERAL RESOURCES Robert C. Milici, Commissioner of Mineral Resources and State Geologist CHARLOTTESVILLE, VIRGINIA 1980 COMMONWEALTH OT VIRGINIA DEPARTMENT OF PURCHASES AND SUPPLY . RICHMOND 1980 DEPARTMENT OF CONSERVATION AND ECONOMIC DEVELOPMENT Richmond, Virginia FRED W. WALKER, Director JERALDF. MOORE, Deputy Director BOARD J. H. JOHNSON, West Point, Chairman A. R. DUNNING, Millwood, Vice Chairman MYRON P. ERKILETIAN, Alexandria ARTHUR P. FLIPPO. Doswell HENRY T. N. GRAVES, Luray MILDRED LAYNE, Williamsburg FREDERIC S. REED, Manakin-Sabot GEORGE P. SHAFRAN, Arlington SHELDON H. SHORT,III, Chase City NICHOLAS D. STREET, Grundy SHERMAN WALLACE, Cleveland E. FLOYD YATES, Powhatan CONTENTS' Page Part 1. -
Impact Cratering
6 Impact cratering The dominant surface features of the Moon are approximately circular depressions, which may be designated by the general term craters … Solution of the origin of the lunar craters is fundamental to the unravel- ing of the history of the Moon and may shed much light on the history of the terrestrial planets as well. E. M. Shoemaker (1962) Impact craters are the dominant landform on the surface of the Moon, Mercury, and many satellites of the giant planets in the outer Solar System. The southern hemisphere of Mars is heavily affected by impact cratering. From a planetary perspective, the rarity or absence of impact craters on a planet’s surface is the exceptional state, one that needs further explanation, such as on the Earth, Io, or Europa. The process of impact cratering has touched every aspect of planetary evolution, from planetary accretion out of dust or planetesimals, to the course of biological evolution. The importance of impact cratering has been recognized only recently. E. M. Shoemaker (1928–1997), a geologist, was one of the irst to recognize the importance of this process and a major contributor to its elucidation. A few older geologists still resist the notion that important changes in the Earth’s structure and history are the consequences of extraterres- trial impact events. The decades of lunar and planetary exploration since 1970 have, how- ever, brought a new perspective into view, one in which it is clear that high-velocity impacts have, at one time or another, affected nearly every atom that is part of our planetary system. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
Relative Ages
CONTENTS Page Introduction ...................................................... 123 Stratigraphic nomenclature ........................................ 123 Superpositions ................................................... 125 Mare-crater relations .......................................... 125 Crater-crater relations .......................................... 127 Basin-crater relations .......................................... 127 Mapping conventions .......................................... 127 Crater dating .................................................... 129 General principles ............................................. 129 Size-frequency relations ........................................ 129 Morphology of large craters .................................... 129 Morphology of small craters, by Newell J. Fask .................. 131 D, method .................................................... 133 Summary ........................................................ 133 table 7.1). The first three of these sequences, which are older than INTRODUCTION the visible mare materials, are also dominated internally by the The goals of both terrestrial and lunar stratigraphy are to inte- deposits of basins. The fourth (youngest) sequence consists of mare grate geologic units into a stratigraphic column applicable over the and crater materials. This chapter explains the general methods of whole planet and to calibrate this column with absolute ages. The stratigraphic analysis that are employed in the next six chapters first step in reconstructing -
A Study About the Temporal Constraints on the Martian Yardangs’ Development in Medusae Fossae Formation
remote sensing Article A Study about the Temporal Constraints on the Martian Yardangs’ Development in Medusae Fossae Formation Jia Liu 1,2 , Zongyu Yue 1,3,*, Kaichang Di 1,3 , Sheng Gou 1,4 and Shengli Niu 4 1 State Key Laboratory of Remote Sensing Science, Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing 100101, China; [email protected] (J.L.); [email protected] (K.D.); [email protected] (S.G.) 2 University of Chinese Academy of Sciences, Beijing 100049, China 3 CAS Center for Excellence in Comparative Planetology, Hefei 230026, China 4 State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau 999078, China; [email protected] * Correspondence: [email protected]; Tel.: +86-10-64889553 Abstract: The age of Mars yardangs is significant in studying their development and the evolution of paleoclimate conditions. For planetary surface or landforms, a common method for dating is based on the frequency and size distribution of all the superposed craters after they are formed. However, there is usually a long duration for the yardangs’ formation, and they will alter the superposed craters, making it impossible to give a reliable dating result with the method. An indirect method by analyzing the ages of the superposed layered ejecta was devised in the research. First, the layered ejecta that are superposed on and not altered by the yardangs are identified and mapped. Then, the ages of the layered ejecta are derived according to the crater frequency and size distribution on them. These ages indicate that the yardangs ceased development by these times, and the ages are valuable for studying the evolution of the yardangs.