TERRESTRIAL IMPACTS: FEATURES at ALL SCALES 6:00 P.M
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Distribution of Chicxulub Ejecta at the Cretaceous-Tertiary Boundary
Geological Society of America Special Paper 356 2002 Distribution of Chicxulub ejecta at the Cretaceous-Tertiary boundary Philippe Claeys* Department of Geology, Vrije Universiteit Brussel, Pleinlann 2, B-1050, Brussels, Belgium Wolfgang Kiessling* Natural History Museum, Invalidenstr. 43 D-10099, Berlin, Germany Walter Alvarez* Department of Earth and Planetary Science, University of California, Berkeley, California 94720-4767, USA ABSTRACT The mineralogical, sedimentological, and geochemical information in a large database on the Cretaceous-Tertiary (K-T) boundary is used to document the distri- bution of impact debris derived from the Chicxulub crater. The database is coupled with a geographic information system (GIS) allowing the plotting of the information on a latest Cretaceous paleogeographic map. The database will be available in part on the internet in the near future, and contains data from 345 K-T boundary sites worldwide. However, relatively few sites are known in South America, Australia, Af- rica, and in the high latitudes. Major disturbances of sedimentation, such as massive debris flows, failure of platform margins, or significant erosion of Upper Cretaceous layers, occur throughout the Gulf of Mexico. Mass wasting of material also took place in the western and eastern parts of the Atlantic Ocean. Almost 100 K-T boundary sites analyzed for Ir recorded the positive anomaly; Ir is spread homogeneously throughout the world, but is diluted at proximal sites because of the high volume of sediment that was in suspension in the Gulf of Mexico after the impact. Shocked quartz is more common, and maybe larger in size west of the crater. The main ad- vantage of the database is to provide a convenient method to manage the huge amount of data available in the literature, and to reveal patterns or characteristics of the data. -
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. -
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. -
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. -
PDF Orientations in Shocked Quartz Grains Around the Chicxulub Crater
Meteoritics & Planetary Science 43, Nr 4, 745–760 (2008) AUTHOR’S PROOF Abstract available online at http://meteoritics.org PDF orientations in shocked quartz grains around the Chicxulub crater Yoichiro NAKANO1, Kazuhisa GOTO2*, Takafumi MATSUI3, Ryuji TADA1, and Eiichi TAJIKA1 1Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo, Build. #5, 7-3-1 Hongo, Tokyo 113-0033, Japan 2Tsunami Engineering Laboratory, Disaster Control Research Center, Graduate School of Engineering, Tohoku University, Aoba 06-6-11, Aramaki, Sendai 980-8579, Japan 3Department of Complexity Science and Engineering, Graduate School of Frontier Science, The University of Tokyo, 7-3-1 Hongo, Tokyo 113-0033, Japan *Corresponding author. E-mail: [email protected] (Received 07 August 2006; revision accepted 04 September 2007) Abstract–We measured 852 sets of planar deformation features (PDFs) in shocked quartz grains in impactite samples of the Yaxcopoil (YAX-1) core and from 4 Cretaceous/Tertiary (K/T) boundary deposits: the Monaca, the Cacarajícara, and the Peñalver formations in Cuba, and DSDP site 536, within 800 km of the Chicxulub crater, in order to investigate variations of PDF orientations in_ the ω proximity_ of the crater._ Orientations of_ PDFs show a broad distribution with peaks_ at _{1013}, π ξ {10_12}, and {1112},_ plus r, z {101_ 1} orientations with minor c(0001), s{1121}, t{2241} plus x{5161}, and m{1010} plus a{1120} orientations. Planar deformation features with c(0001) orientation are relatively more abundant in the proximity of the Chicxulub crater than in distal sites such as North America, the Pacific Ocean, and Europe. -
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. -
The Chicxulub Impact Is Synchronous with the Planktonic Foraminifera
Geologica Acta: an international earth science journal ISSN: 1695-6133 [email protected] Universitat de Barcelona España ARENILLAS, I.; ARZ, J.A.; GRAJALES-NISHIMURA, J.M.; MELÉNDEZ, A.; ROJAS- CONSUEGRA, R. The Chicxulub impact is synchronous with the planktonic foraminifera mass extinction at the Cretaceous/Paleogene boundary: new evidence from the Moncada section, Cuba Geologica Acta: an international earth science journal, vol. 14, núm. 1, marzo, 2016, pp. 35-51 Universitat de Barcelona Barcelona, España Available in: http://www.redalyc.org/articulo.oa?id=50544801004 How to cite Complete issue Scientific Information System More information about this article Network of Scientific Journals from Latin America, the Caribbean, Spain and Portugal Journal's homepage in redalyc.org Non-profit academic project, developed under the open access initiative Geologica Acta, Vol.14, Nº 1, March 2016, 35-51 DOI: 10.1344/GeologicaActa2016.14.1.4 The Chicxulub impact is synchronous with the planktonic foraminifera mass extinction at the Cretaceous/Paleogene boundary: new evidence from the Moncada section, Cuba I. ARENILLAS1 J.A. ARZ1 J.M. GRAJALES-NISHIMURA2 A. MELÉNDEZ1 R. ROJAS-CONSUEGRA3 1Departamento de Ciencias de la Tierra e Instituto de Investigación en Ciencias Ambientales (IUCA), Universidad de Zaragoza Pedro Cerbuna 12, 50009 Zaragoza, Spain. Arenillas E-mail: [email protected] Arz E-mail: [email protected] Meléndez E-mail: [email protected] 2Instituto de Geología, Universidad Nacional Autónoma de México Ciudad Universitaria, Coyoacán, México D.F., 04510, México. E-mail: [email protected] 3Museo Nacional de Historia Natural Obispo 61, Plaza de Armas Habana Vieja, 10100 La Habana, Cuba. -
Meteor Crater, Arizona
Petrographic, X-ray diffraction, and electron spin resonance analysis of deformed calcite: Meteor Crater, Arizona Item Type Article; text Authors Burt, J. B.; Pope, M. C.; Watkinson, A. J. Citation Burt, J. B., Pope, M. C., & Watkinson, A. J. (2005). Petrographic, Xray diffraction, and electron spin resonance analysis of deformed calcite: Meteor Crater, Arizona. Meteoritics & Planetary Science, 40(2), 297-306. DOI 10.1111/j.1945-5100.2005.tb00381.x Publisher The Meteoritical Society Journal Meteoritics & Planetary Science Rights Copyright © The Meteoritical Society Download date 05/10/2021 06:22:06 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/655967 Meteoritics & Planetary Science 40, Nr 2, 297–306 (2005) Abstract available online at http://meteoritics.org Petrographic, X-ray diffraction, and electron spin resonance analysis of deformed calcite: Meteor Crater, Arizona Jason B. BURT,1†* Mike C. POPE,1 and A. John WATKINSON1 1Department of Geological Sciences, Washington State University, Pullman, Washington 99164, USA †Present address: Department of Geosciences, Virginia Polytechnic and State University, Blacksburg, Virginia 24061, USA *Corresponding author. E-mail: [email protected] (Received 9 June 2003; revision accepted 16 December 2004) Abstract–Calcite crystals within the Kaibab limestone in Meteor Crater, Arizona, are examined to understand how calcite is deformed during a meteorite impact. The Kaibab limestone is a silty fine- grained and fossiliferous dolomudstone and the calcite crystals occur as replaced evaporite nodules with impact-induced twinning. Twinning in the calcite is variable with deformational regimes based on abundances of crystals with twins and twin densities within crystals. -
The Encyclopedia of Quantavolution And
A Written lower case as 'a, 'A' is first letter of English alphabet, also Greek (Alpha) and Hebrew (Aleph); originally in English as in Latin and Romanic tongues it is the sign for making the lowbackwide sound with jaws, pharynx, and lips open. Its prime position indicates importance of the sound, which has several meanings as an exclamation of wonder, approval, and worship. Ancient name of the Moon in several Near East cultures was "A" or kindred sounds and syllables, "Aa", "Ah", "Ai". "A" to Babylonians signified the Great Mother of the wise and "Akshara." Greek myth regarded "A" as the beginning of birth and creation, the entrance to the river Styx that wound about in the womb of the world, finally returning to Alpha. Aku, the Sumerian Moon, was also "the Measurer." The name "Abram" or "Abraham" might have originated as a combining of the Moon (Ab), Sun (ra) and Mercury (ram or raham). The letter has other uses as a word, as an indefinite article ("a bird"), in Latin languages, as an article and also as a preposition ("to" and "by")and feminine ending ("femina"); pragmatic uses as a vowel and word and exclamation in communication are thus known; ultimate significance is unknown, as, e.g., whether all languages must utter the full Asound in a certain range of frequencies or whether the sound preponderates in sacred utterance, etc. aa Form of lava which solidifies as a mass of blocklike fragments with a rough surface. Also called block lava. Aar Gorge A 1.6 kmlong cut through a limestone ridge near Meiringen, Switzerland, carrying the torrent of the Aar River that arises from the Aar Glacier. -
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. -
Polygonal Impact Craters in Argyre Region, Mars: Implications for Geology and Cratering Mechanics
Meteoritics & Planetary Science 43, Nr 10, 1605–1628 (2008) Abstract available online at http://meteoritics.org Polygonal impact craters in Argyre region, Mars: Implications for geology and cratering mechanics T. ÖHMAN1, 2*, M. AITTOLA2, V.-P. KOSTAMA2, J. RAITALA2, and J. KORTENIEMI2, 3 1Department of Geosciences, Division of Geology, University of Oulu, P.O. Box 3000, FI-90014, Finland 2Department of Physical Sciences, Division of Astronomy, University of Oulu, P.O. Box 3000, FI-90014, Finland 3Institut für Planetologie, Westfälische Wilhelms-Universität, Wilhelm-Klemm-Strasse 10, D-48149 Münster, Germany *Corresponding author. E-mail: [email protected] (Received 20 November 2007; revision accepted 15 April 2008) Abstract–Impact craters are not always circular; sometimes their rims are composed of several straight segments. Such polygonal impact craters (PICs) are controlled by pre-existing target structures, mainly faults or other similar planes of weakness. In the Argyre region, Mars, PICs comprise ∼17% of the total impact crater population (>7 km in diameter), and PICs are relatively more common in older geologic units. Their formation is mainly controlled by radial fractures induced by the Argyre and Ladon impact basins, and to a lesser extent by the basin-concentric fractures. Also basin-induced conjugate shear fractures may play a role. Unlike the PICs, ridges and graben in the Argyre region are mostly controlled by Tharsis-induced tectonism, with the ridges being concentric and graben radial to Tharsis. Therefore, the PICs primarily reflect an old impact basin-centered tectonic pattern, whereas Tharsis-centered tectonism responsible for the graben and the ridges has only minor influence on the PIC rim orientations. -
References 111 References
References 111 References Ahrens T. J. (1993) Impact erosion of terrestrial planetary atmos- Bischoff A. and Stöffler D. (1984) Chemical and structural changes pheres. Annu. Rev. Earth Planet. Sci., 21, 525–555. induced by thermal annealing of shocked feldspar inclusions Ahrens T. J. and O’Keefe J. D. (1977) Equations of state and in impact melt rocks from Lappajärvi Crater, Finland. Proc. impact-induced shock-wave attenuation on the Moon. In Lunar Planet. Sci. Conf. 14th, in J. Geophys. Res., 89, B645– Impact and Explosion Cratering: Planetary and Terrestrial B656. Implications (D. J. Roddy, R. O. Pepin, and R. B. Merrill, Bischoff L. and Oskierski W. (1987) Fractures, pseudotachylite eds.), pp. 639–656. Pergamon, New York. veins, and breccia dikes in the crater floor of the Rochechouart Aldersey-Williams H. (1995) The Most Beautiful Molecule: The impact structure, SW-France, as indicators of crater-forming Discovery of the Buckyball. John Wiley and Sons, New York. processes. In Research in Terrestrial Impact Structures ( J. Pohl, 340 pp. ed.), pp. 5–29. Earth Evolution Sciences, Intl. Mono. Ser., Alexopoulos J. S., Grieve R. A. F., and Robertson P. B. (1988) Friedr. Vieweg and Son, Wiesbaden, Germany. Microscopic lamellar deformation features in quartz: Dis- Bloss F. D. (1981) The Spindle Stage — Principles and Practice. criminative characteristics of shock-generated varieties. Cambridge Univ., New York. 340 pp. Geology, 16, 796–799. Bohor B. F. and Glass B. P. (1995) Origin and diagenesis of K/T Alvarez L. W., Alvarez W., Asaro F., and Michel H. V. (1980) impact spherules — From Haiti to Wyoming and beyond.