Laser Argon Dating of Melt Breccias from the Siljan Impact Structure, Sweden: Implications for a Possible Relationship to Late Devonian Extinction Events
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Laser Argon Dating of Melt Breccias from the Siljan Impact Structure, Sweden: Implications for a Possible Relationship to Late Devonian Extinction Events
Meteoritics & Planetary Science 40, Nr 4, 591–607 (2005) Abstract available online at http://meteoritics.org Laser argon dating of melt breccias from the Siljan impact structure, Sweden: Implications for a possible relationship to Late Devonian extinction events Wolf U. REIMOLD1*, Simon P. KELLEY2, Sarah C. SHERLOCK2, Herbert HENKEL3, and Christian KOEBERL4 1Impact Cratering Research Group, School of Geosciences, University of the Witwatersrand, Private Bag 3, P. O. Wits 2050, Johannesburg, South Africa 2Department of Earth Sciences, Open University, Walton Hall, Milton Keynes MK7 6AA, UK 3Department of Land and Water Resources Engineering, Division of Engineering Geology and Geophysics, Royal Institute of Technology, Teknikringen 72, SE 100-44 Stockholm, Sweden 4Department of Geological Sciences, University of Vienna, Althanstrasse 14, A-1090 Vienna, Austria *Corresponding author. E-mail: [email protected] (Received 12 July 2004; revision accepted 08 February 2005) Abstract–In earlier studies, the 65–75 km diameter Siljan impact structure in Sweden has been linked to the Late Devonian mass extinction event. The Siljan impact event has previously been dated by K- Ar and Ar-Ar chronology at 342–368 Ma, with the commonly quoted age being 362.7 ± 2.2 Ma (2 σ, recalculated using currently accepted decay constants). Until recently, the accepted age for the Frasnian/Famennian boundary and associated extinction event was 364 Ma, which is within error limits of this earlier Siljan age. Here we report new Ar-Ar ages extracted by laser spot and laser step heating techniques for several melt breccia samples from Siljan (interpreted to be impact melt breccia). The analytical results show some scatter, which is greater in samples with more extensive alteration; these samples generally yield younger ages. -
Evidence for Impact-Generated Deposition
EVIDENCE FOR IMPACT-GENERATED DEPOSITION ON THE LATE EOCENE SHORES OF GEORGIA by ROBERT SCOTT HARRIS (Under the direction of Michael F. Roden) ABSTRACT Modeling demonstrates that the Late Eocene Chesapeake Bay impact would have been capable of depositing ejecta in east-central Georgia with thicknesses exceeding thirty centimeters. A coarse sand layer at the base of the Upper Eocene Dry Branch Formation was examined for shocked minerals. Universal stage measurements demonstrate that planar fabrics in some fine to medium sand-size quartz grains are parallel to planes commonly exploited by planar deformation features (PDF’s) in shocked quartz. Possible PDF’s are observed parallel to {10-13}, {10-11}, {10-12}, {11-22} and {51-61}. Petrographic identification of shocked quartz is supported by line broadening in X-ray diffraction experiments. Other impact ejecta recognized include possible ballen quartz, maskelynite, and reidite-bearing zircon grains. The layer is correlative with an unusual diamictite that contains goethite spherules similar to altered microkrystites. It may represent an impact-generated debris flow. These discoveries suggest that the Chesapeake Bay impact horizon is preserved in Georgia. The horizon also should be the source stratum for Georgia tektites. INDEX WORDS: Chesapeake Bay impact, Upper Eocene, Shocked quartz, Impact shock, Shocked zircon, Impact, Impact ejecta, North American tektites, Tektites, Georgiaites, Georgia Tektites, Planar deformation features, PDF’s, Georgia, Geology, Coastal Plain, Stratigraphy, Impact stratigraphy, Impact spherules, Goethite spherules, Diamictite, Twiggs Clay, Dry Branch Formation, Clinchfield Sand, Irwinton Sand, Reidite, Microkrystite, Cpx Spherules, Impact debris flow EVIDENCE FOR IMPACT-GENERATED DEPOSITION ON THE LATE EOCENE SHORES OF GEORGIA by ROBERT SCOTT HARRIS B. -
EMD Shale Gas and Liquids Committee Annual Report, FY 2014
EMD Shale Gas and Liquids Committee Annual Report, FY 2014 Neil S. Fishman, Chair March 30, 2014 Vice Chairs: Brian Cardott, (Vice Chair, Government), Oklahoma Geological Survey, Norman, OK Harris Cander (Vice Chair, Industry), BP, Houston, TX Sven Egenhoff, (Vice Chair, University), Colorado State University, Fort Collins, CO Advisory Committee (in alphabetical order): Kent Bowker, Bowker Petroleum, The Woodlands, TX Ken Chew, IHS (retired), Perthsire, Scotland Thomas Chidsey, Utah Geological Survey, Salt Lake City, UT Russell Dubiel, U.S. Geological Survey, Denver, CO Catherine Enomoto, U.S. Geological Survey, Reston, VA William Harrison, Western Michigan University, Kalamazoo, MI Ursula Hammes, Bureau of Economic Geology, Austin, TX Shu Jiang, University of Utah, Salt Lake City, UT Margaret Keller, U.S. Geological Survey, Menlo Park, CA Julie LeFever, North Dakota Geological Survey, Grand Forks, ND Peng Li, Arkansas Geological Survey, Little Rock, AR Jock McCracken, Egret Consulting, Calgary, AB Stephen Nordeng, North Dakota Geological Survey, Grand Forks, ND Rich Nyahay, New York Museum, Albany, NY Stephen Sonnenberg, Colorado School of Mines, Golden, CO Michael D. Vanden Berg, Utah Geological Survey, Salt Lake City, UT Rachel Walker, Countrymark Energy Resources, LLC, Indianapolis, IN INTRODUCTION It is a pleasure to present this Annual Report from the EMD Shale Gas and Liquids Committee. This report contains information about specific shales across the U.S., Canada, Europe, China, as well as SE Asia from which hydrocarbons are currently being produced or shales that are of interest for hydrocarbon exploitation. The inclusion in this report of shales from which any hydrocarbon is produced reflects the expanded mission of the EMD Shale Gas and Liquids Committee to serve as a single point of access to technical information on shales regardless of the hydrocarbons produced from them (e.g., gas, oil, condensate). -
Flynn Creek Crater, Tennessee: Final Report, by David J
1967010060 ASTROGEOLOGIC STUDIES / ANNUAL PROGRESS REPORT " July 1, 1965 to July 1, 1966 ° 'i t PART B - h . CRATERINVESTIGATIONS N 67_1_389 N 57-" .]9400 (ACCEC_ION [4U _" EiER! (THRU} .2_ / PP (PAGLS) (CO_ w ) _5 (NASA GR OR I"MX OR AD NUMBER) (_ATEGORY) DEPARTMENT OF THE INTERIOR UNITED STATES GEOLOQICAL SURVEY • iri i i i i iiii i i 1967010060-002 ASTROGEOLOGIC STUDIES ANNUAL PROGRESS REPORT July i, 1965 to July I, 1966 PART B: CRATER INVESTIGATIONS November 1966 This preliminary report is distributed without editorial and technical review for conformity with official standards and nomenclature. It should not be quoted without permission. This report concerns work done on behalf of the National Aeronautics and Space Administration. DEPARTMENT OF THE INTERIOR UNITED STATES GEOLOGICAL SURVEY 1967010060-003 • #' C OING PAGE ,BLANK NO/" FILMED. CONTENTS PART B--CRATER INVESTIGATIONS Page Introduction ........................ vii History and origin of the Flynn Creek crater, Tennessee: final report, by David J. Roddy .............. 1 Introductien ..................... 1 Geologic history of the Flynn Creek crater ....... 5 Origin of the Flynn Creek crater ............ ii Conc lusions ...................... 32 References cited .................... 35 Geology of the Sierra Madera structure, Texas: progress report, by H. G. Wilshire ............ 41_ Introduction ...................... 41 Stratigraphy ...................... 41 Petrography and chemical composition .......... 49 S truc ture ....................... 62 References cited ............. ...... 69 Some aspects of the Manicouagan Lake structure in Quebec, Canada, by Stephen H. Wolfe ................ 71 f Craters produced by missile impacts, by H. J. Moore ..... 79 Introduction ...................... 79 Experimental procedure ................. 80 Experimental results .................. 81 Summary ........................ 103 References cited .................... 103 Hypervelocity impact craters in pumice, by H. J. Moore and / F. -
Lunar and Planetary Science XXIX 1379.Pdf
Lunar and Planetary Science XXIX 1379.pdf TEAGUE RING IMPACT STRUCTURE, WESTERN AUSTRALIA: GRAVITY SURVEY. J. B. Plescia, California Institute of Technology, Jet Propulsion Laboratory, Pasadena, CA 91109 ([email protected]) As part of an effort to better define the nature and the A reconnaissance gravity survey conducted in crustal structure of Teague Ring, a GPS controlled grav- 1986 (2) defined a significant negative anomaly over ity survey was undertaken in the austral winter of 1996. Teague Ring. To better define the structure a more de- The objective was to define the gravity field, identify any tailed survey was conducted in August 1996.. Gravity anomalies, and interpret that anomaly in terms of crustal station positions were established by a GPS survey; structure. positional information was collected for 10 minutes (600 Teague Ring is an impact structure in Western readings) and differentially corrected. The typical stan- Australia (25° 50’ S; 120° 55’ E). It has a diameter of 31 dard deviation of the station locations were 0.2 m hori- km and an age of ~1630 Ma. Teague Ring was first rec- zontal N, 0.2 m horizontal E, 0.6 m vertical with a vertical ognized by Butler (1) and various models of origin have PDOP mean of 3.3. The datum for reduction of the GPS been proposed. The most recent detailed work was un- data was AGD 1966. Gravity values were measured using dertaken by Eugene and Carolyn Shoemaker, but it has a Lacoste Romberg gravity meter (#G-1035). Approxi- been published only in limited form (2). -
Appendix a Recovery of Ejecta Material from Confirmed, Probable
Appendix A Recovery of Ejecta Material from Confirmed, Probable, or Possible Distal Ejecta Layers A.1 Introduction In this appendix we discuss the methods that we have used to recover and study ejecta found in various types of sediment and rock. The processes used to recover ejecta material vary with the degree of lithification. We thus discuss sample processing for unconsolidated, semiconsolidated, and consolidated material separately. The type of sediment or rock is also important as, for example, carbonate sediment or rock is processed differently from siliciclastic sediment or rock. The methods used to take and process samples will also vary according to the objectives of the study and the background of the investigator. We summarize below the methods that we have found useful in our studies of distal impact ejecta layers for those who are just beginning such studies. One of the authors (BPG) was trained as a marine geologist and the other (BMS) as a hard rock geologist. Our approaches to processing and studying impact ejecta differ accordingly. The methods used to recover ejecta from unconsolidated sediments have been successfully employed by BPG for more than 40 years. A.2 Taking and Handling Samples A.2.1 Introduction The size, number, and type of samples will depend on the objective of the study and nature of the sediment/rock, but there a few guidelines that should be followed regardless of the objective or rock type. All outcrops, especially those near industrialized areas or transportation routes (e.g., highways, train tracks) need to be cleaned off (i.e., the surface layer removed) prior to sampling. -
ANIC IMPACTS: MS and IRONMENTAL P ONS Abstracts Edited by Rainer Gersonde and Alexander Deutsch
ANIC IMPACTS: MS AND IRONMENTAL P ONS APRIL 15 - APRIL 17, 1999 Alfred Wegener Institute for Polar and Marine Research Bremerhaven, Germany Abstracts Edited by Rainer Gersonde and Alexander Deutsch Ber. Polarforsch. 343 (1999) ISSN 01 76 - 5027 Preface .......3 Acknowledgements .......6 Program ....... 7 Abstracts P. Agrinier, A. Deutsch, U. Schäre and I. Martinez: On the kinetics of reaction of CO, with hot Ca0 during impact events: An experimental study. .11 L. Ainsaar and M. Semidor: Long-term effect of the Kärdl impact crater (Hiiumaa, Estonia) On the middle Ordovician carbonate sedimentation. ......13 N. Artemieva and V.Shuvalov: Shock zones on the ocean floor - Numerical simulations. ......16 H. Bahlburg and P. Claeys: Tsunami deposit or not: The problem of interpreting the siliciclastic K/T sections in northeastern Mexico. ......19 R. Coccioni, D. Basso, H. Brinkhuis, S. Galeotti, S. Gardin, S. Monechi, E. Morettini, M. Renard, S. Spezzaferri, and M. van der Hoeven: Environmental perturbation following a late Eocene impact event: Evidence from the Massignano Section, Italy. ......21 I von Dalwigk and J. Ormö Formation of resurge gullies at impacts at sea: the Lockne crater, Sweden. ......24 J. Ebbing, P. Janle, J, Koulouris and B. Milkereit: Palaeotopography of the Chicxulub impact crater and implications for oceanic craters. .25 V. Feldman and S.Kotelnikov: The methods of shock pressure estimation in impacted rocks. ......28 J.-A. Flores, F. J. Sierro and R. Gersonde: Calcareous plankton stratigraphies from the "Eltanin" asteroid impact area: Strategies for geological and paleoceanographic reconstruction. ......29 M.V.Gerasimov, Y. P. Dikov, 0 . I. Yakovlev and F.Wlotzka: Experimental investigation of the role of water in the impact vaporization chemistry. -
Post-Impact Depositional Environments As a Proxy for Crater Morphology, Late Devonian Alamo Impact, Nevada
Crater morphology of the Late Devonian Alamo impact, Nevada Post-impact depositional environments as a proxy for crater morphology, Late Devonian Alamo impact, Nevada Andrew J. Retzler1,†,*, Leif Tapanila1,2,*, Julia R. Steenberg3,*, Carrie J. Johnson4,*, and Reed A. Myers5,* 1Department of Geosciences, Idaho State University, 921 South 8th Avenue, Pocatello, Idaho 83209-8072, USA 2Division of Earth Science, Idaho Museum of Natural History, 921 South 8th Avenue, Pocatello, Idaho 83209-8096, USA 3Minnesota Geological Survey, 2642 University Avenue W., St. Paul, Minnesota 55114-1032, USA 4Chesapeake Energy Corporation, Building 05, Offi ce 249, 6001 North Classen Boulevard, Oklahoma City, Oklahoma 73118, USA 5Department of Earth and Atmospheric Sciences, 1-26 Earth Sciences Building, University of Alberta, Edmonton, Alberta T6G2E3, Canada ABSTRACT INTRODUCTION as expected for marine bolide impacts (Dypvik and Jansa, 2003; Dypvik and Kalleson, 2010). Marine facies of carbonate and siliciclas- Marine bolide impact events are under- Estimates of the fi nal crater diameter have relied tic sediments deposited on top of the upper represented in the rock record due to their low exclusively on the extent and composition of the Devonian Alamo Breccia Member identify preservation potential. Consequently, few stud- Alamo Breccia Member and not on geomorphic the shape and size of the Alamo impact cra- ies exist documenting marine impact crater size, features specifi c to marine impact craters. ter in south-central Nevada (western USA). morphology, and effects on sedimentation pat- The aim of this paper is to interpret crater There are 13 measured sections that record terns; of the 27 known marine impact craters on morphology based on post-impact deposi- peritidal to deep-subtidal deposition across Earth, 20 of them are currently located on land tional environments in the context of a regional the impacted platform, and these are corre- (Dypvik and Jansa, 2003). -
Shatter Cone and Microscopic Shock-Alteration Evidence for a Post-Paleoproterozoic Terrestrial Impact Structure Near Santa Fe, New Mexico, USA
Earth and Planetary Science Letters 270 (2008) 290–299 Contents lists available at ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl Shatter cone and microscopic shock-alteration evidence for a post-Paleoproterozoic terrestrial impact structure near Santa Fe, New Mexico, USA Siobhan P. Fackelman a, Jared R. Morrow b,⁎, Christian Koeberl c, Thornton H. McElvain d a Earth Sciences Department, University of Northern Colorado, Greeley, CO 80639, USA b Department of Geological Sciences, San Diego State University, San Diego, CA 92182, USA c Department of Lithospheric Studies, University of Vienna, Althanstrasse 14, A-1090 Vienna, Austria d 111 Lovato Lane, Santa Fe, NM 87505, USA ARTICLE INFO ABSTRACT Article history: Field mapping, morphologic description, and petrographic analysis of recently discovered shatter cones Received 7 January 2008 within Paleoproterozoic crystalline rocks exposed over an area N5km2, located ∼8 km northeast of Santa Fe, Received in revised form 19 March 2008 New Mexico, USA, give robust evidence of a previously unrecognized terrestrial impact structure. Herein, we Accepted 20 March 2008 provisionally name this the “Santa Fe impact structure”. The shatter cones are composed of nested sub- Available online 7 April 2008 conical, curviplanar, and flat joint surfaces bearing abundant curved and bifurcating striations that strongly Editor: R.W. Carlson resemble the multiply striated joint surfaces (MSJS) documented from shatter cones at Vredefort dome. The cones occur as a penetrative feature in intrusive igneous and supracrustal metamorphic rocks, are unusually Keywords: large (up to 2 m long and 0.5 m wide at the base), display upward-pointing apices, and have subvertical, shatter cones northeastward-plunging axes that crosscut regional host-rock fabrics. -
Meteorite Impacts, Earth, and the Solar System
Traces of Catastrophe A Handbook of Shock-Metamorphic Effects in Terrestrial Meteorite Impact Structures Bevan M. French Research Collaborator Department of Mineral Sciences, MRC-119 Smithsonian Institution Washington DC 20560 LPI Contribution No. 954 i Copyright © 1998 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 portion thereof requires the written permission of the Insti- tute as well as the appropriate acknowledgment of this publication. Figures 3.1, 3.2, and 3.5 used by permission of the publisher, Oxford University Press, Inc. Figures 3.13, 4.16, 4.28, 4.32, and 4.33 used by permission of the publisher, Springer-Verlag. Figure 4.25 used by permission of the publisher, Yale University. Figure 5.1 used by permission of the publisher, Geological Society of America. See individual captions for reference citations. This volume may be cited as French B. M. (1998) Traces of Catastrophe:A Handbook of Shock-Metamorphic Effects in Terrestrial Meteorite Impact Structures. LPI Contribution No. 954, Lunar and Planetary Institute, Houston. 120 pp. This volume is distributed by ORDER DEPARTMENT Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113, USA Phone:281-486-2172 Fax:281-486-2186 E-mail:[email protected] Mail order requestors will be invoiced for the cost of shipping and handling. Cover Art.“One Minute After the End of the Cretaceous.” This artist’s view shows the ancestral Gulf of Mexico near the present Yucatán peninsula as it was 65 m.y. -
The Siljan Ring in Central Sweden - a Window Into the Palaeozoic History of Baltoscandia
Geophysical Research Abstracts Vol. 14, EGU2012-11247-1, 2012 EGU General Assembly 2012 © Author(s) 2012 The Siljan Ring in central Sweden - a window into the Palaeozoic history of Baltoscandia O. Lehnert (1), G. Meinhold (2), S.M. Bergström (3), M. Calner (4), J.O.R. Ebbestad (5), S. Egenhoff (6), Å.M. Frisk (7), A.E.S. Högström (8), and J. Maletz (9) (1) GeoZentrum Nordbayern, Lithosphere Dynamics, University of Erlangen-Nürnberg, Schloßgarten 5, D-91054, Erlangen, Germany ([email protected]), (2) Sedimentology & Environmental Geology, Geoscience Centre, University of Göttingen, Goldschmidtstrasse 3, D-37077 Göttingen, Germany ([email protected]), (3) School of Earth Sciences, Division of Earth History, The Ohio State University, 125 S. Oval Mall, Columbus, Ohio 443210, USA ([email protected]), (4) Department of Geology, Lund University, Sölvegatan 12, SE-223 62 Lund, Sweden ([email protected]), (5) Museum of Evolution, Uppsala University, Norbyvägen 16, SE - 752 36 Uppsala, Sweden ([email protected]), (6) Department of Geosciences, Colorado State University, 322 Natural Resources Building, Fort Collins, CO 80523-1482, USA ([email protected]), (7) Paläontologisches Institut und Museum, Karl Schmid-Strasse 4, 8006 Zürich, Switzerland ([email protected]), (8) Tromsö University Museum, Natural Sciences, N-9037 Tromsö, Norway ([email protected]), (9) Institut für Geologische Wissenschaften, Freie Universität Berlin, Malteser Str. 74-100, Haus B, Raum 322, D-12249 Berlin, Germany ([email protected]) The Siljan meteorite crater, the largest known impact crater in Europe, is a main target of the research project ‘Concentric Impact Structures in the Palaeozoic (CISP)’, an integral of the Swedish Deep Drilling Program (SDDP). -
Geological Survey Research 1962
Geological Survey Research 1962 Synopsis of Geologic, Hydrologic, and Topographic Results GEOLOGICAL SURVEY PROFESSIONAL PAPER 450-A Geological Survey Research 1962 THOMAS B. NOLAN, Director GEOLOGICAL SURVEY PROFESSIONAL PAPER 450 Asynopsis of results ofgeologic, hydro logic, and topo graphic investigations for fiscalyear 1962, accom panied by short papers in the fields of geology, hydrology, topography, and allied sciences. Pub lished separately as Chapters A, B, C, D, and E UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON : 1962 FOREWORD The reception accorded the 1960 and 1961 Annual Reviews of Geological Survey research has encouraged us to prepare this volume, "Geological Survey Research, 1962," in a con tinuing effort to publish more quickly the significant results of our current investigations. We continue to consider these reports as experimental and have again this year modified the content, format, and frequency of release of chapters in an attempt to serve better the interests of the users of the reports. The comments and suggestions of these users are here solicited and will be considered carefully as future volumes are planned. The current Annual Review consists of five chapters (Chapters A through E) of Pro fessional Paper 450. As in the preceding two Annual Reviews, Chapter A is a synopsis of recent findings in the many and varied lines of study pursued by Survey personnel. Chap ters, B, C, D, and E of this volume are collections of short articles in geology, hydrology, topography, and allied fields. These articles are numbered as follows: Prof. Paper 450-B Articles 1-59 Prof. Paper 450-C Articles 60-119 Prof.