Alamo Megabreccia: Record of a Late Devonian Impact in Southern Nevada John E
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
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. -
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. -
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. -
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. -
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. -
A New Way to Confirm Meteorite Impact Produced Planar Features in Quartz: Combining Universal Stage and Electron Backscatter Diffraction Techniques
A new way to confirm meteorite impact produced planar features in quartz: combining Universal Stage and Electron Backscatter Diffraction techniques M.H. Voorn MSc Thesis August 2010 Utrecht University - Earth Sciences department Structural Geology and Tectonic research group Abstract As recognised from the geological record, meteorite impact events can have a severe influence on (local) geology, climate and life. Solid evidence for these events is therefore important to obtain. The most convincing evidence comes from microstructures in quartz. Upon impact, Planar Fractures (PFs) and Planar Deformation Features (PDFs) form parallel to specific crystallographic planes in quartz. Non-impact formed (tectonic) Deformation Lamellae (DL) may be hard to distinguish qualitatively from PFs or PDFs with the optical microscope, but do not form parallel to crystallographic planes. Quantitative methods using the Universal Stage (U-Stage) on the optical microscope have therefore been applied widely to (dis)confirm this parallelism. With the method, the quartz c-axis and poles to planar features are measured and plotted. An improved technique requires so-called indexing of the measured orientations using a stereographic projection template. Even when these techniques are applied, some proposed impact structures remain debated. An important reason for this is the U-stage can not provide the full crystal orientation of quartz. The goal of this thesis was to check the classical U-stage techniques for quantitatively confirming impact planar features in quartz, and to see whether the addition of Electron Backscatter Diffraction (EBSD, on the Scanning Electron Microscope: SEM) and Cathodoluminescence (CL, on the SEM) can provide more solid evidence. Six previously confirmed impact and three non-impact samples were studied. -
A Paleozoic Age for the Tunnunik Impact Structure Camille Lepaulard, Jerome Gattacceca, Nicholas Swanson-Hysell, Yoann Quesnel, François Demory, Gordon Osinski
A Paleozoic age for the Tunnunik impact structure Camille Lepaulard, Jerome Gattacceca, Nicholas Swanson-Hysell, Yoann Quesnel, François Demory, Gordon Osinski To cite this version: Camille Lepaulard, Jerome Gattacceca, Nicholas Swanson-Hysell, Yoann Quesnel, François Demory, et al.. A Paleozoic age for the Tunnunik impact structure. Meteoritics and Planetary Science, Wiley, 2019, 54 (4), pp.740-751. 10.1111/maps.13239. hal-02048190 HAL Id: hal-02048190 https://hal.archives-ouvertes.fr/hal-02048190 Submitted on 26 Apr 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. 1 2 A Paleozoic age for the Tunnunik impact structure 3 4 Camille Lepaulard1, Jérôme Gattacceca1, Nicholas Swanson-Hysell2, Yoann Quesnel1, 5 François Demory1 , Gordon R. Osinski3,4, 6 7 1Aix Marseille Univ, CNRS, IRD, Coll France, INRA, CEREGE, Aix-en-Provence, France 8 2 Department of Earth and Planetary Science, University of California, Berkeley, California 9 94720-4767, USA 10 3 Dept. of Earth Sciences, Centre for Planetary Science and Exploration, University of Western 11 Ontario, -
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. -
Evidence for Subsolidus Quartz-Coesite Transformation in Impact Ejecta from the Australasian Tektite Strewn field
Available online at www.sciencedirect.com ScienceDirect Geochimica et Cosmochimica Acta 264 (2019) 105–117 www.elsevier.com/locate/gca Evidence for subsolidus quartz-coesite transformation in impact ejecta from the Australasian tektite strewn field Fabrizio Campanale a,b,⇑, Enrico Mugnaioli b, Luigi Folco a, Mauro Gemmi b Martin R. Lee c, Luke Daly c,e,f, Billy P. Glass d a Dipartimento di Scienze della Terra, Universita` di Pisa, V. S. Maria 53, 56126 Pisa, Italy b Center for Nanotechnology Innovation@NEST, Istituto Italiano di Tecnologia (IIT), Piazza San Silvestro 12, 56127 Pisa, Italy c Department of Geographical and Earth Sciences, University of Glasgow, Glasgow G12 8QQ, UK d Department of Geosciences, University of Delaware, Newark, DE, USA e Australian Centre for Microscopy and Microanalysis, University of Sydney, Sydney 2006, NSW, Australia f Space Science and Technology Centre, School of Earth and Planetary Science, Curtin University, Bentley, 6102 WA, Australia Received 1 April 2019; accepted in revised form 11 August 2019; Available online 21 August 2019 Abstract Coesite, a high-pressure silica polymorph, is a diagnostic indicator of impact cratering in quartz-bearing target rocks. The formation mechanism of coesite during hypervelocity impacts has been debated since its discovery in impact rocks in the 1960s. Electron diffraction analysis coupled with scanning electron microscopy and Raman spectroscopy of shocked silica grains from the Australasian tektite/microtektite strewn field reveals fine-grained intergrowths of coesite plus quartz bearing planar deformation features (PDFs).À Quartz and euhedral microcrystalline coesite are in direct contact, showing a recurrent pseudo iso-orientation, with the ½111* vector of quartz near parallel to the [0 1 0]* vector of coesite. -
Studies of the Chesapeake Bay Impact Structure— Introduction and Discussion
Studies of the Chesapeake Bay Impact Structure— Introduction and Discussion By J. Wright Horton, Jr., David S. Powars, and Gregory S. Gohn Chapter A of Studies of the Chesapeake Bay Impact Structure— The USGS-NASA Langley Corehole, Hampton, Virginia, and Related Coreholes and Geophysical Surveys Edited by J. Wright Horton, Jr., David S. Powars, and Gregory S. Gohn Prepared in cooperation with the Hampton Roads Planning District Commission, Virginia Department of Environmental Quality, and National Aeronautics and Space Administration Langley Research Center Professional Paper 1688 U.S. Department of the Interior U.S. Geological Survey iii Contents Abstract . .A1 Introduction . 1 Previous Work . 3 The Chesapeake Bay Impact Structure . 5 Form and Structure . 5 Character of the Target . 7 Land Surface Features . 7 The USGS-NASA Langley Core . 9 Significant Results . 11 Crystalline Basement Rocks . 11 Impact-Modified and Impact-Generated Sediments . 11 Postimpact Sediments . 13 Water Depths—Impact and Postimpact . 14 Dating the Impact Event . 14 Structural Interpretation of Seismic Data . 15 Interpretation of Audio-Magnetotelluric (AMT) Soundings . 15 Hydrologic Effects and Water-Resources Implications . 16 Conceptual Model . 16 Acknowledgments . 18 References Cited . 18 Appendix A1. Abstracts of Research on the Chesapeake Bay Impact Structure, 2001–2003 . 24 Figures A1. Regional map showing the location of the Chesapeake Bay impact structure, the USGS-NASA Langley corehole at Hampton, Va., and some other coreholes in southeastern Virginia . A2 A2. Map of southeastern Virginia showing locations of recently completed coreholes and geophysical surveys in relation to the Chesapeake Bay impact structure . .4 A3. Satellite image of Chesapeake Bay showing location of the buried impact structure and nearby Mesozoic to Cenozoic tectonic features. -
Sedimentary Record of Impact Events in Spain
Geological Society of America Special Paper 356 2002 Sedimentary record of impact events in Spain Enrique Dı´az-Martı´nez* Enrique Sanz-Rubio Jesu´s Martı´nez-Frı´as Centro de Astrobiologı´a Consejo Superior de Investigaciones Cientı´ficas—Instituto Nacional de Te´cnica Aeroespacial, Carretera, Torrejo´n-Ajalvir kilo´metro 4, 28850 Torrejo´n de Ardoz, Madrid, Spain ABSTRACT A review of the evidence of meteorite-impact events in the sedimentary record of Spain reveals that the only proven impact-related bed is the clay layer at the Cretaceous-Tertiary boundary (at Zumaya and Sopelana in the Bay of Biscay region, and at Caravaca, Agost, and Alamedilla in the Betic Cordilleras). Other deposits previously proposed as impact related can now be rejected, or are dubious and still debated. These include the Pelarda Formation, alleged to represent proximal ejecta from the Azuara structure; the Paleocene-Eocene boundary near Zumaya (western Pyrenees) and Alamedilla (Betic Cordillera); and the Arroyofrı´o Oolite Bed, which has been alleged as distal ejecta of an unknown Callovian-Oxfordian impact event. The scarcity of evidence for meteorite-impact events in the sedimentary record is possibly due to a lack of detailed studies. We propose several sedimentary units that could potentially be related to impact events, and where future research should focus. INTRODUCTION DISTAL RECORD OF IMPACT EVENTS The sedimentary record of Spain presents evidence for at The evidence from sedimentary units to be considered as least one impact event, as well as a number of units of potential distal impact ejecta may consist of geochemical anomalies of impact clastic origin (some of which are currently under inves- elements and isotopes (e.g., Ir, 187Os/188Os), the presence of tigation). -
Astroblemes, Scientific America~?-, Vol
Waste Isolation Pilot Plant Compliance Certification Application Reference 176 Dietz, R.S., August 1961. Astroblemes, Scientific America~?-, Vol. 205, #2, p 50-58. Submitted in accordance with 40 CFR § 194.13, Submission of Reference Materials. .. ~H ..\TTER COXE rour inrhes hi~h is one or many in igneous rork XEST OF COXES in dolomite. a tn~ or lime~tone. is rrom Wrlls or the \·rederort Ring in South ..\rrira. a strurture that i& prob Creek Ba~in ~trurture in Tenllt"'-"ft'. Thi& ~roup i~ II iMhet hi~h. ably the remains or tl1e large>l meteorite crater known on earth. Shork pre~~ur~ generated by meteorite imparl rreate ourh ron~. (;J..\.XT SH.-\TTER COXF., over rour reea long. i& !ihown in 1•lare amons jumbled rorks in a Rat. geolor:iralJy underormrd terrain at the Kentland Jime~tone quarry in Indiana. These c·ones round indirate that the quarry i~ an anrienl meteorite-im:-t ,ite. UMI Article Clearinghouse has reproduced this material with SO perLmLi'~-s~on of the copyright owner. Further reproduction IS Thi~ newly. ('Oined w·ord refers to anctent scars left in the earth·~ cru~t by huge tneteoriteH. The evidence for such itnpacts is largely the h igh-pre~~ure tnineral coesite and ~~shatter cones~' in the rocks b,· Hobert S. Dietz t is ;m awesome experience to stand authorih· was such that it took more than fall every 10,000 years, some 50,000 on the rim of B;minger Crater in :30 years' to re\·erse his judgment. But the giant meteorites must have struck the I Arizona and reflect on the cosmic scienc.-es progress not so much by the dis earth during the past 500 million ~·ears.