Largemeteoriteimpactsand Planetaryevolution

Total Page:16

File Type:pdf, Size:1020Kb

Largemeteoriteimpactsand Planetaryevolution qF URY 1997 LARGEMETEORITEIMPACTSAND PLANETARYEVOLUTION September1-3,1997 Sudbury,Ontario ! F CONFERENCE ON LARGE METEORITE IMPACTS AND PLANETARY EVOLUTION (SUDBURY 1997) Hosted by Ontario Geological Survey Sponsored by Inco Limited Falconbridge Limited The Barringer Crater Company Geological Survey of Canada Ontario Ministry of Northern Development and Mines Quebec Minist_re des Ressources naturelles Lunar and Planetary Institute Scientific Organizing Committee A. Deutsch University of Miinster, Germany B. O. Dressier, Chair Lunar and Planetary Institute, Houston, Texas B. M. French Smithsonian Institution, Washington, DC R. A. F. Grieve Geological Survey of Canada, Ottawa, Ontario G. W. Johns Ontario Geological Survey, Sudbury, Ontario V. L. Sharpton Lunar and Planetary Institute, Houston, Texas LPI Contribution No. 922 Compiled in 1997 by LUNAR AND PLANETARY INSTITUTE The Institute is operated by the Universities Space Research Association under Contract No. NASW-4574 with 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. (1997) Title of abstract. In Conference on Large Meteorite Impacts and Planetary Evolution (Sudbury 1997), p. XX, LPI Contribution No. 922, Lunar and Planetary Institute, Houston. This volume is distributed by ORDER DEPARTMENT Lunar and Planetary Iustitute 3600 Bay Area Boulevard Houston TX 77058-1113, USA Mail order requestors will be invoiced for the cost of shipping and handling. LP! Contribution No. 922 iii Contents BP and Oasis Impact Structures, Libya, and Their Relation to Libyan Desert Glass: Petrography, Geochemistry, and Geochronology B. Abate, C. Koeberl, J. R. Underwood Jr., E. P. Fisk, and R. F. Giegengack ................................... 1 - ( Overview of Bosumtwi Crater, Ghana S. T. Ahulu ........................................................................................................................................... 1 ._a..- Crater-fill Sequence, Onaping Formation: Petrographic and Geochemical Signature of Regional Hydrothermal Alteration D. E. Ames and H. L. Gibson .............................................................................................................. 1 - Impact-induced Hydrothermal Base Metal Mineralization, Whitewater Group, Sudbury Structure D. E. Ames, H. L. Gibson, and I. R. Jonasson .................................................................................... 2 - y Nickel- and Platinum-Group-Element-Enriched Quartz Norite in the Latest Jurassic Morokweng Impact Structure, South Africa M. A. G. Andreoli, R. J. Hart, L. D. Ashwal, and M. Tredoux ............................................................ 3 -5f Simulating Phase Equilibria and In Situ Differentiation for the Proposed Parental Sudbury Magmas A. A. Ariskin ........................................................................................................................................ 3 _'b, Investigations on the Green Member of the Onaping Formation, Sudbury Structure, Ontario, Canada M. E. Avermann .................................................................................................................................. 4 _ 7 Extraterrestrial Helium (He@C_ Trapped in Fullerenes in the Sudbury Impact Structure L. Becket, J. L. Bada, R. J. Poreda, and T. E. Bunch ......................................................................... 5 - Summary of Work in Manicouagan Impact Structure L. Boivin ............................................................................................................................................. 5 " Composition and Structure of the Chicxulub Crater Using Wide-Angle Seismic Velocities J.. Brittan, H Macintyre, and the Chicxulub Working Group ............................................................. 6 - / _ Synthetic Aperture Radar Characteristics of a Glacially Modified Meltsheet, Manicouagan, Quebec P. Budkewitsch and R. Grieve ............................................................................................................. 6- s/ New Potential Sources for Black Onaping Carbon T. E. Bunch, L. Becker, P H. Schultz, and W. S. Wolbach .................................................................. 7 -/L- Ecosystem-Structure Analysis Applied to Indication and Study of Earth Astroblemes G. G. Burba Jr 7 "-/_ Sedimentary Interbeds of the Rooiberg Group at the Loskop Dam Section, Bushveld Complex, South Africa M. E. Caress and W. E. Elston ............................................................................................................ 8 -/.4- iv 1997 Sudbury Conference The Chicxulub Seismic Experiment Chicxulub Working Group: d. Morgan, M. Warner, J. Brittan, H. Macintyre, D. Snyder, R. Hobbs, G. Suarez, L. Marin, A. Trejo, R. Buffler, G. Christeson, Y. Nakamura, A. Hildebrand, M. Pilkington, V..Sharpton, P Maguire, P Denton, G. Mackenzie, andA. Camargo .......................... .............................................................. 9 "/_" Structure of the Chicxulub Impact Crater from Wide-Angle Ocean-Bottom Seismograph Data G. L. Christeson, Y. Nakamura, R. T. Buffler, and the Chicxulub Working Group ............................................................................................................ 9 " /& The Chicxulub Impact Structure and Its Proximal Ejecta P. Claeys, A. Deutsch, F. Langenhorst, S. Heuschkel, B. Dissman, and D. Strffler ......................................................................................... 9 Chemical Compositions of Chicxulub Impact Breccias C. M. Corrigan, V. L. Sharpton, T. A. Vogel and L. E. Marin ................................................................................................................................ 10 Funnel-shaped Emplacement Geometry of the Sudbury Igneous Complex: A Structural Perspective E. J. Cowan and W. M. Schwerdtner ................................................................................................ 11 "/_ Sudbury: Geochemical Evidence for a Single-Impact Melting Event A. P. Dickin and d. H. Crocket .......................................................................................................... 11 --_,_ The Separation of Platinum and Palladium During High-Temperature Vaporization of Sulfide-rich Picrite Yu. P Dikov, V. V. Distler, M. V. Gerasimov, and O. L Yakovlev ....................................................... 12 -_ l The Sudbury Structure, Ontario, Canada: A Persistent Enigma B. O. Dressier and V. L. Sharpton .................................................................................................... 12" 2 ;i- Review of the Geophysical Signature of the Vredefort Structure and Its Interpretations R. J. Durrheim and W. U. Reimold ................................................................................................... 13 -,p._x Base of the Rooiberg Group: Evidence for an Initial Bushveld Catastrophe lE. E. Elston and M. E. Caress .......................................................................................................... 14 -D_ Classification and Distribution of Sudbury Breccia J S. Fedorowich, D. H. Rousell, and W. V. Peredery ....................................................................... 14 .,2_" Impact Materials with Mixed Compositions of Iron-Silicon-Nickel-Sulfur System S. Fukuyama, Y. Miura, and H. Kobayashi ...................................................................................... 15--76, Experimental Investigation of the Chemistry of Vaporization of Targets in Relation to the Chicxulub Impact M. V. Gerasimov, Yu. P Dikov, O. I. Yakovlev, and E grr/otzka.i ....... ,i............................................. 15=-2. 7 The Onaping Formation: Stratigraphy, Fragmentation, and Mechanisms of Emplacement S. F.. M. Gibbins, H. L. Gibson, D. E. Ames, and L R. Jonasson .................................................. 16 _ D _/ LPI ContributionNo. 922 v Diagnostic Criteria for the Recognition of Shatter Cones H. M. Gibson and J. G. Spray 16 - ,_ Multiple Origins for Impact-produced Diamonds I. Gilrnour, R. M. Hough, and C. T. Pillinger ................................................................................ 17 -30 Asteroid/Comet Mega-Impacts and Mantle Melting Episodes: Consequences for Precambrian Crustal Evolution A. Y. Glikson .................................................................................................................................. 17 t/ Large-Scale Impact of Cratering and Early Earth Evolution R. A. E Grieve and M. J. Cintala .................................................................................................. 18 -,,_,- Geophysical Modeling of the Mj_lnir Impact Structure, Barents Sea S. T. Gudlaugsson, F. Tsikalas, O. Eldholm, and J. I. Faleide ...................................................... 19 -:_-_ Magnetic Anomalies of the Vredefort Central Rise Structure H. Henkel ...................................................................................................................................... 19 "fl NBCS: The Baltic-Nordic Network for Impact Crater Studies H. Henkel ...................................................................................................................................... 20 _D Combined
Recommended publications
  • Ices on Mercury: Chemistry of Volatiles in Permanently Cold Areas of Mercury’S North Polar Region
    Icarus 281 (2017) 19–31 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Ices on Mercury: Chemistry of volatiles in permanently cold areas of Mercury’s north polar region ∗ M.L. Delitsky a, , D.A. Paige b, M.A. Siegler c, E.R. Harju b,f, D. Schriver b, R.E. Johnson d, P. Travnicek e a California Specialty Engineering, Pasadena, CA b Dept of Earth, Planetary and Space Sciences, University of California, Los Angeles, CA c Planetary Science Institute, Tucson, AZ d Dept of Engineering Physics, University of Virginia, Charlottesville, VA e Space Sciences Laboratory, University of California, Berkeley, CA f Pasadena City College, Pasadena, CA a r t i c l e i n f o a b s t r a c t Article history: Observations by the MESSENGER spacecraft during its flyby and orbital observations of Mercury in 2008– Received 3 January 2016 2015 indicated the presence of cold icy materials hiding in permanently-shadowed craters in Mercury’s Revised 29 July 2016 north polar region. These icy condensed volatiles are thought to be composed of water ice and frozen Accepted 2 August 2016 organics that can persist over long geologic timescales and evolve under the influence of the Mercury Available online 4 August 2016 space environment. Polar ices never see solar photons because at such high latitudes, sunlight cannot Keywords: reach over the crater rims. The craters maintain a permanently cold environment for the ices to persist. Mercury surface ices magnetospheres However, the magnetosphere will supply a beam of ions and electrons that can reach the frozen volatiles radiolysis and induce ice chemistry.
    [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]
  • Geologic Gems of California's State Parks
    STATE OF CALIFORNIA – EDMUND G. BROWN JR., GOVERNOR NATURAL RESOURCES AGENCY – JOHN LAIRD, SECRETARY CALIFORNIA GEOLOGICAL SURVEY DEPARTMENT OF PARKS AND RECREATION – LISA MANGAT, DIRECTOR JOHN D. PARRISH, Ph.D., STATE GEOLOGIST DEPARTMENT OF CONSERVATION – DAVID BUNN, DIRECTOR PLATE 1 The rugged cliffs of Del Norte Coast Redwoods State Park are composed of some of California’s Bio-regions the most tortured, twisted, and mobile rocks of the North American continent. The California’s Geomorphic Provinces rocks are mostly buried beneath soils and covered by vigorous redwood forests, which thrive in a climate famous for summer fog and powerful winter storms. The rocks only reveal themselves in steep stream banks, along road and trail cut banks, along the precipitous coastal cliffs and offshore in the form of towering rock monuments or sea stacks. (Photograph by CalTrans staff.) Few of California’s State parks display impressive monoliths adorned like a Patrick’s Point State Park displays a snapshot of geologic processes that have castle with towering spires and few permit rock climbing. Castle Crags State shaped the face of western North America, and that continue today. The rocks Park is an exception. The scenic beauty is best enjoyed from a distant exposed in the seacliffs and offshore represent dynamic interplay between the vantage point where one can see the range of surrounding landforms. The The Klamath Mountains consist of several rugged ranges and deep canyons. Klamath/North Coast Bioregion San Joaquin Valley Colorado Desert subducting oceanic tectonic plate (Gorda Plate) and the continental North American monolith and its surroundings are a microcosm of the Klamath Mountains The mountains reach elevations of 6,000 to 8,000 feet.
    [Show full text]
  • Study of Acoustic Cavitation Near Metal Surfaces Contaminated by Uranium Ran Ji
    Study of acoustic cavitation near metal surfaces contaminated by uranium Ran Ji To cite this version: Ran Ji. Study of acoustic cavitation near metal surfaces contaminated by uranium. Other. Université Montpellier, 2018. English. NNT : 2018MONTS131. tel-02282007 HAL Id: tel-02282007 https://tel.archives-ouvertes.fr/tel-02282007 Submitted on 9 Sep 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. THÈ SE POUR OBTENIR LE GRADE DE DOCTEUR DE L’UNIVERSITÉ DE MONTPELLIER En Chimie Sé parative - Maté riaux et Procé dé s É cole doctorale Sciences Chimiques Balard (ED 459) Unité de recherche Institut de Chimie Sé parative de Marcoule (UMR 5257) Study of Acoustic Cavitation near Metal Surfaces Contaminated by Uranium Pré senté e par Ran JI Le 13 novembre 2018 Sous la direction de Sergueï NIKITENKO Rapport de gestion Devant le jury composé de [Jean-Franç ois DUFÊ CHE, Prof, Université Montpellier] [Pré sident] [Jean-Yves HIHN, Prof, Université de Franche-Comté ] [Rapporteur] 2015 [Laurie BARTHE, MCF, INP Toulouse] [Rapporteur] [Sergueï NIKITENKO, DR, CNRS Montpellier] [Directeur de Thè se] [Claire LE NAOUR, CR, Université Paris Saclay] [Examinateur] [Micheline DRAYE, Prof, Université Savoie Mont Blanc] [Examinateur] [Rachel PFLIEGER, CR, CEA Marcoule] [Encadrant] [Matthieu VIROT, CR, CEA Marcoule] [Encadrant] [Pascal PILUSO, CR, CEA Cadarache] [Invité ] “The unity of inner knowledge and action” [Wang Yangming] Acknowledgements Acknowledgements The doctoral study of the past three years has greatly enriched my experience in academic and personal life.
    [Show full text]
  • Impact Melt Emplacement on Mercury
    Western University Scholarship@Western Electronic Thesis and Dissertation Repository 7-24-2018 2:00 PM Impact Melt Emplacement on Mercury Jeffrey Daniels The University of Western Ontario Supervisor Neish, Catherine D. The University of Western Ontario Graduate Program in Geology A thesis submitted in partial fulfillment of the equirr ements for the degree in Master of Science © Jeffrey Daniels 2018 Follow this and additional works at: https://ir.lib.uwo.ca/etd Part of the Geology Commons, Physical Processes Commons, and the The Sun and the Solar System Commons Recommended Citation Daniels, Jeffrey, "Impact Melt Emplacement on Mercury" (2018). Electronic Thesis and Dissertation Repository. 5657. https://ir.lib.uwo.ca/etd/5657 This Dissertation/Thesis is brought to you for free and open access by Scholarship@Western. It has been accepted for inclusion in Electronic Thesis and Dissertation Repository by an authorized administrator of Scholarship@Western. For more information, please contact [email protected]. Abstract Impact cratering is an abrupt, spectacular process that occurs on any world with a solid surface. On Earth, these craters are easily eroded or destroyed through endogenic processes. The Moon and Mercury, however, lack a significant atmosphere, meaning craters on these worlds remain intact longer, geologically. In this thesis, remote-sensing techniques were used to investigate impact melt emplacement about Mercury’s fresh, complex craters. For complex lunar craters, impact melt is preferentially ejected from the lowest rim elevation, implying topographic control. On Venus, impact melt is preferentially ejected downrange from the impact site, implying impactor-direction control. Mercury, despite its heavily-cratered surface, trends more like Venus than like the Moon.
    [Show full text]
  • Sedimentological Analysis of Resurge Deposits at the Lockne and Tvären Craters: Clues to Flow Dynamics
    Meteoritics & Planetary Science 42, Nr 11, 1929–1943 (2007) Abstract available online at http://meteoritics.org Sedimentological analysis of resurge deposits at the Lockne and Tvären craters: Clues to flow dynamics Jens ORMÖ1*, Erik STURKELL2, and Maurits LINDSTRÖM3 1Centro de Astrobiología (CAB), Instituto Nacional de Técnica Aeroespacial, Ctra de Torrejón a Ajalvir, km 4, 28850 Torrejón de Ardoz, Madrid, Spain 2Nordic Volcanological Center, Institute of Earth Sciences, University of Iceland, Sturlugata 7, 101 Reykjavík, Iceland 3Department of Geology and Geochemistry, Stockholm University, 10691 Stockholm, Sweden *Corresponding author. E-mail: [email protected] (Submitted 08 November 2006; revision accepted 14 May 2007) Abstract–The Lockne and Tvären craters formed about 455 million years ago in an epicontinental sea where seawater and mainly limestones covered a crystalline basement. The target water depth for Tvären (apparent basement crater diameter D = 2 km) was probably not over 150 m, and for Lockne (D = 7.5 km) recent best-fit numerical simulations suggest the target water depth of 500–700 m. Lockne has crystalline ejecta that partly cover an outer crater (14 km diameter) apparent in the target sediments. Tvären is eroded with only the crater infill preserved. We have line-logged cores through the resurge deposits within the craters in order to analyze the resurge flow. The focus was clast lithology, frequencies, and size sorting. We divide the resurge into “resurge proper,” with water and debris shooting into the crater and ultimately rising into a central water plume, “anti-resurge,” with flow outward from the collapsing plume, and “oscillating resurge” (not covered by the line-logging due to methodological reasons), with decreasing flow in diverse directions.
    [Show full text]
  • Pre-Mission Insights on the Interior of Mars Suzanne E
    Pre-mission InSights on the Interior of Mars Suzanne E. Smrekar, Philippe Lognonné, Tilman Spohn, W. Bruce Banerdt, Doris Breuer, Ulrich Christensen, Véronique Dehant, Mélanie Drilleau, William Folkner, Nobuaki Fuji, et al. To cite this version: Suzanne E. Smrekar, Philippe Lognonné, Tilman Spohn, W. Bruce Banerdt, Doris Breuer, et al.. Pre-mission InSights on the Interior of Mars. Space Science Reviews, Springer Verlag, 2019, 215 (1), pp.1-72. 10.1007/s11214-018-0563-9. hal-01990798 HAL Id: hal-01990798 https://hal.archives-ouvertes.fr/hal-01990798 Submitted on 23 Jan 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Open Archive Toulouse Archive Ouverte (OATAO ) OATAO is an open access repository that collects the wor of some Toulouse researchers and ma es it freely available over the web where possible. This is an author's version published in: https://oatao.univ-toulouse.fr/21690 Official URL : https://doi.org/10.1007/s11214-018-0563-9 To cite this version : Smrekar, Suzanne E. and Lognonné, Philippe and Spohn, Tilman ,... [et al.]. Pre-mission InSights on the Interior of Mars. (2019) Space Science Reviews, 215 (1).
    [Show full text]
  • Aquatic Ecosystems Bibliography Compiled by Robert C. Worrest
    Aquatic Ecosystems Bibliography Compiled by Robert C. Worrest Abboudi, M., Jeffrey, W. H., Ghiglione, J. F., Pujo-Pay, M., Oriol, L., Sempéré, R., . Joux, F. (2008). Effects of photochemical transformations of dissolved organic matter on bacterial metabolism and diversity in three contrasting coastal sites in the northwestern Mediterranean Sea during summer. Microbial Ecology, 55(2), 344-357. Abboudi, M., Surget, S. M., Rontani, J. F., Sempéré, R., & Joux, F. (2008). Physiological alteration of the marine bacterium Vibrio angustum S14 exposed to simulated sunlight during growth. Current Microbiology, 57(5), 412-417. doi: 10.1007/s00284-008-9214-9 Abernathy, J. W., Xu, P., Xu, D. H., Kucuktas, H., Klesius, P., Arias, C., & Liu, Z. (2007). Generation and analysis of expressed sequence tags from the ciliate protozoan parasite Ichthyophthirius multifiliis BMC Genomics, 8, 176. Abseck, S., Andrady, A. L., Arnold, F., Björn, L. O., Bomman, J. F., Calamari, D., . Zepp, R. G. (1998). Environmental effects of ozone depletion: 1998 assessment. Journal of Photochemistry and Photobiology B: Biology, 46(1-3), 1-108. doi: Doi: 10.1016/s1011-1344(98)00195-x Adachi, K., Kato, K., Wakamatsu, K., Ito, S., Ishimaru, K., Hirata, T., . Kumai, H. (2005). The histological analysis, colorimetric evaluation, and chemical quantification of melanin content in 'suntanned' fish. Pigment Cell Research, 18, 465-468. Adams, M. J., Hossaek, B. R., Knapp, R. A., Corn, P. S., Diamond, S. A., Trenham, P. C., & Fagre, D. B. (2005). Distribution Patterns of Lentic-Breeding Amphibians in Relation to Ultraviolet Radiation Exposure in Western North America. Ecosystems, 8(5), 488-500. Adams, N.
    [Show full text]
  • Impact Structures and Events – a Nordic Perspective
    107 by Henning Dypvik1, Jüri Plado2, Claus Heinberg3, Eckart Håkansson4, Lauri J. Pesonen5, Birger Schmitz6, and Selen Raiskila5 Impact structures and events – a Nordic perspective 1 Department of Geosciences, University of Oslo, P.O. Box 1047, Blindern, NO 0316 Oslo, Norway. E-mail: [email protected] 2 Department of Geology, University of Tartu, Vanemuise 46, 51014 Tartu, Estonia. 3 Department of Environmental, Social and Spatial Change, Roskilde University, P.O. Box 260, DK-4000 Roskilde, Denmark. 4 Department of Geography and Geology, University of Copenhagen, Øster Voldgade 10, DK-1350 Copenhagen, Denmark. 5 Division of Geophysics, University of Helsinki, P.O. Box 64, FIN-00014 Helsinki, Finland. 6 Department of Geology, University of Lund, Sölvegatan 12, SE-22362 Lund, Sweden. Impact cratering is one of the fundamental processes in are the main reason that the Nordic countries are generally well- the formation of the Earth and our planetary system, as mapped. reflected, for example in the surfaces of Mars and the Impact craters came into the focus about 20 years ago and the interest among the Nordic communities has increased during recent Moon. The Earth has been covered by a comparable years. The small Kaalijärv structure of Estonia was the first impact number of impact scars, but due to active geological structure to be confirmed in northern Europe (Table 1; Figures 1 and processes, weathering, sea floor spreading etc, the num- 7). First described in 1794 (Rauch), the meteorite origin of the crater ber of preserved and recognized impact craters on the field (presently 9 craters) was proposed much later in 1919 (Kalju- Earth are limited.
    [Show full text]
  • IMPACTS II: CRATERS and EJECTA 8:30 A.M
    40th Lunar and Planetary Science Conference (2009) sess505.pdf Thursday, March 26, 2009 IMPACTS II: CRATERS AND EJECTA 8:30 a.m. Waterway Ballroom 6 Chairs: Peter Schulte Tamara Goldin 8:30 a.m. van Soest M. C. * Wartho J.-A. Monteleone B. D. Hodges K. V. Koeberl C. Schmieder M. Buchner E. Spray J. G. Bezys R. K. Reimold W. U. (U-Th)/He Dating of Single Zircon and Apatite Crystals — A New Tool for Dating Terrestrial Impact Structures [#2041] The low temperature (U-Th)/He technique has been utilized to date individual crystals from the Manicouagan, Lake Saint Martin, and Bosumtwi impact structures. New (U-Th)/He zircon ages are in agreement with ages obtained via other dating methods. 8:45 a.m. Sapers H. M. * Osinski G. R. Banerjee N. Re-Evaluating the Rochechouart Impactites: Petrographic Classification, Hydrothermal Alteration and Evidence for Carbonate Bearing Target Rocks [#1284] A systematic classification of the Rochechouart impacts is proposed. Evidence for post-impact hydrothermal alteration was observed. A carbonate clast within the lithic impact breccia suggests the existence of carbonate in the pre-impact target rocks. 9:00 a.m. Mohr-Westheide T. * Reimold W. U. Chemical Analysis of Small-Scale Pseudotachylitic Breccia in Archean Gneiss of the Vredefort Dome, South Africa [#1528] Results of a new microchemical investigation of small-scale pseudotachylitic breccias from the Archean gneiss of the Vredefort dome are reported. Limited mixing and for small veinlets local melt formation are observed. 9:15 a.m. McDonald I. Koeberl C. * Gurov E. A Meteoritic Component in Melt Rocks from the Boltysh Impact Structure, Ukraine: First Assessment [#1252] A chondritic component has been detected in impact melt rocks from the Boltysh impact structure, Ukraine.
    [Show full text]
  • The Tennessee Meteorite Impact Sites and Changing Perspectives on Impact Cratering
    UNIVERSITY OF SOUTHERN QUEENSLAND THE TENNESSEE METEORITE IMPACT SITES AND CHANGING PERSPECTIVES ON IMPACT CRATERING A dissertation submitted by Janaruth Harling Ford B.A. Cum Laude (Vanderbilt University), M. Astron. (University of Western Sydney) For the award of Doctor of Philosophy 2015 ABSTRACT Terrestrial impact structures offer astronomers and geologists opportunities to study the impact cratering process. Tennessee has four structures of interest. Information gained over the last century and a half concerning these sites is scattered throughout astronomical, geological and other specialized scientific journals, books, and literature, some of which are elusive. Gathering and compiling this widely- spread information into one historical document benefits the scientific community in general. The Wells Creek Structure is a proven impact site, and has been referred to as the ‘syntype’ cryptoexplosion structure for the United State. It was the first impact structure in the United States in which shatter cones were identified and was probably the subject of the first detailed geological report on a cryptoexplosive structure in the United States. The Wells Creek Structure displays bilateral symmetry, and three smaller ‘craters’ lie to the north of the main Wells Creek structure along its axis of symmetry. The question remains as to whether or not these structures have a common origin with the Wells Creek structure. The Flynn Creek Structure, another proven impact site, was first mentioned as a site of disturbance in Safford’s 1869 report on the geology of Tennessee. It has been noted as the terrestrial feature that bears the closest resemblance to a typical lunar crater, even though it is the probable result of a shallow marine impact.
    [Show full text]
  • Select Bibliography
    Select Bibliography by the late F. Seymour-Smith Reference books and other standard sources of literary information; with a selection of national historical and critical surveys, excluding monographs on individual authors (other than series) and anthologies. Imprint: the place of publication other than London is stated, followed by the date of the last edition traced up to 1984. OUP- Oxford University Press, and includes depart­ mental Oxford imprints such as Clarendon Press and the London OUP. But Oxford books originating outside Britain, e.g. Australia, New York, are so indicated. CUP - Cambridge University Press. General and European (An enlarged and updated edition of Lexicon tkr WeltliU!-atur im 20 ]ahrhuntkrt. Infra.), rev. 1981. Baker, Ernest A: A Guilk to the B6st Fiction. Ford, Ford Madox: The March of LiU!-ature. Routledge, 1932, rev. 1940. Allen and Unwin, 1939. Beer, Johannes: Dn Romanfohrn. 14 vols. Frauwallner, E. and others (eds): Die Welt Stuttgart, Anton Hiersemann, 1950-69. LiU!-alur. 3 vols. Vienna, 1951-4. Supplement Benet, William Rose: The R6athr's Encyc/opludia. (A· F), 1968. Harrap, 1955. Freedman, Ralph: The Lyrical Novel: studies in Bompiani, Valentino: Di.cionario letU!-ario Hnmann Hesse, Andrl Gilk and Virginia Woolf Bompiani dille opn-e 6 tUi personaggi di tutti i Princeton; OUP, 1963. tnnpi 6 di tutu le let16ratur6. 9 vols (including Grigson, Geoffrey (ed.): The Concise Encyclopadia index vol.). Milan, Bompiani, 1947-50. Ap­ of Motkm World LiU!-ature. Hutchinson, 1970. pendic6. 2 vols. 1964-6. Hargreaves-Mawdsley, W .N .: Everyman's Dic­ Chambn's Biographical Dictionary. Chambers, tionary of European WriU!-s.
    [Show full text]