Non-Impact Origin of the Crater-Like Structures in the Gilf Kebir Area (Egypt): Implications for the Geology of Eastern Sahara
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Low-Altitude Airbursts and the Impact Threat
M.B.E. Boslough and D.A. Crawford / International Journal of Impact Engineering Low-altitude airbursts and the impact threat M.B.E. Boslough* and D.A. Crawford Sandia National Laboratories, PO Box 5800, Albuquerque NM 87185, USA International Journal of Impact Engineering 35 (2008) 1441–1448 Received 7 May 2007; Accepted 6 June 2008; Available online 5 August 2008 journal homepage: www.elsevier.com/locate/ijimpeng Abstract We present CTH simulations of airbursts in the Earth’s lower atmosphere from hypervelocity asteroid impacts. The intent of these simulations was to explore the phenomenology associated with low-altitude airbursts, with the particular goal of determining whether the altitude of maximum energy deposition can be used as a reasonable estimate of the equivalent height of a point source explosion. Our simulations suggest that this is not a good approximation. The center of mass of an exploding projectile is transported downward in the form of a high-temperature jet of expanding gas. The jet descends by a significant fraction of the burst altitude before its velocity becomes subsonic. The time scale of this descent is similar to the time scale of the explosion itself, so the jet simultaneously couples its kinetic energy and its internal energy to the atmosphere. Because of this downward flow, larger blast waves and stronger thermal radiation pulses are felt at the surface than would be predicted by a point source explosion at the height where the burst was initiated. For impacts with a kinetic energy above some threshold, the hot jet of vaporized projectile (the descending ―fireball‖) makes contact with the Earth’s surface, where it expands radially. -
Translitterering Och Alternativa Geografiska Namnformer
TRANSLITTERERING OCH ALTERNATIVA GEOGRAFISKA NAMNFORMER Version XX, 27 juli 2015, Stefan Nordblom 1 FÖRORD För många utländska egennamn, i första hand personnamn och geografiska namn, finns det på svenska väl etablerade namnformer. Om det inte finns någon sådan kan utländska egennamn dock vålla bekymmer vid översättning till svenska. Föreliggande material är tänkt att vara till hjälp i sådana situationer och tar upp fall av translitterering1 och transkribering2 samt exonymer3 . Problemen uppstår främst på grund av att olika språk har olika system för translitterering och transkribering från ett visst språk och på grund av att orter kan ha olika namn på olika utländska språk. Eftersom vi oftast översätter från engelska och franska innehåller sammanställningen även translittereringar och exonymer på engelska och franska (samt tyska). Man kan alltså i detta material göra en sökning på sådana namnformer och komma fram till den svenska namnformen. Om man t.ex. i en engelsk text träffar på det geografiska namnet Constance kan man söka på det namnet här och då få reda på att staden (i detta fall på tyska och) på svenska kallas Konstanz. Den efterföljande sammanställningen bygger i huvudsak på följande källor: Institutet för de inhemska språken (FI): bl.a. skriften Svenska ortnamn i Finland - http://kaino.kotus.fi/svenskaortnamn/ Iate (EU-institutionernas termbank) Nationalencyklopedin Nationalencyklopedins kartor Interinstitutionella publikationshandboken - http://publications.europa.eu/code/sv/sv-000100.htm Språkbruk (Tidskrift utgiven av Svenska språkbyrån i Helsingfors) Språkrådet© (1996). Publikation med rekommendationer i term- och språkfrågor som utarbetas av rådets svenska översättningsenhet i samråd med övriga EU-institutioner. TT-språket - info.tt.se/tt-spraket/ I de fall uppgifterna i dessa källor inte överensstämmer med varandra har det i enskilda fall varit nödvändigt att väga, välja och sammanjämka namnförslagen, varvid rimlig symmetri har eftersträvats. -
Earth and Planetary Science Letters Surface Vitrification Caused By
Earth and Planetary Science Letters 469 (2017) 15–26 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Surface vitrification caused by natural fires in Late Pleistocene wetlands of the Atacama Desert ∗ Pierrick Roperch a, , Jérôme Gattacceca b, Millarca Valenzuela c, Bertrand Devouard b, Jean-Pierre Lorand d, Cesar Arriagada e, Pierre Rochette b, Claudio Latorre f,g, Pierre Beck h a Géosciences Rennes, CNRS–INSU, Université de Rennes 1, Rennes, France b CNRS, Aix Marseille Univ., IRD, Coll France, CEREGE, Aix-en-Provence, France c Instituto de Astrofísica, P. Universidad Católica de Chile, Av. Vicuña Mackenna 4860, Santiago, Chile d Laboratoire de Planétologie et Géodynamique, CNRS UMR 6112, Université de Nantes, 2 Rue la Houssinière, 44322, Nantes, France e Departamento de Geología, Facultad de Ciencas Físicas y Matemáticas, Universidad de Chile, Plaza Ercilla 803, Santiago, Chile f Centro UC del Desierto de Atacama and Departamento de Ecología, Pontificia Universidad Católica de Chile, Alameda 340, Santiago, Chile g Institute of Ecology & Biodiversity (IEB), Santiago, Chile h Institut de Planétologie et d’Astrophysique de Grenoble (IPAG), 414, Rue de la Piscine, Domaine Universitaire, 38400 St-Martin d’Hères, France a r t i c l e i n f o a b s t r a c t Article history: We describe extended occurrences of unusual silicate glass surface layers from the Atacama Desert Received 16 November 2016 (Chile). These glasses, found near the town of Pica at four localities separated by up to 70 km, are neither Received in revised form 29 March 2017 fulgurites, nor volcanic glasses, nor metallurgical slags related to anthropic activity, but show close Accepted 3 April 2017 similarities to other glasses that have been previously attributed to large airbursts created by meteoroids Available online 21 April 2017 entering the Earth’s atmosphere. -
Impact and Non-Impact Craters in Eastern Sahara
Impact and non-impact craters in eastern Sahara M. Di Martino1 ; C. Cigolini2 1 INAF – Osservatorio Astronomico di Torino, Pino Torinese, Italy ; 2 Dipartimento di Scienze Mineralogiche e Petrologiche, Università di Torino, Torino, Italy ABSTRACT Recognizing true impact structures on the Earth is usually a very difficult task. Several circular crater-like structures are present in the eastern Sahara (SW Egypt, SE Libya). It has been previously suggested that some of them could be originated by cosmic body impacts, but the results of our geological and geophysical surveys in the area exclude this hypothesis. The first target of our investigations has been the Gilf Kebir region (SW Egypt), where a lot of small crater-like structures are present. On 2004 Paillou et al. [1] concluded that some of them are of meteoritic origin. This hypothesis is not supported by our observations and analyses, and we suggest an alternative interpretation [2]. The crater-like structures in Gilf Kebir area are likely related to endogenic processes typical of hydrothermal vent complexes in volcanic areas which may reflect the emplacement of subvolcanic intrusives. Moreover, a double circular structure, located in SE Libya, about 250 km south of Kufra oasis, was recognized as a double impact crater (the Arkenu craters) by [3], first in satellite imagery and then in the fieldwork, and was thus included in the terrestrial impact crater list. The Arkenu craters consist of a NE (Arkenu 1) and a SW structure (Arkenu 2), 10.3 km and 6.8 km in diameter, respectively, whose centers are located about 10 km apart. -
Very High-Temperature Impact Melt Products As Evidence For
Very high-temperature impact melt products PNAS PLUS as evidence for cosmic airbursts and impacts 12,900 years ago Ted E. Buncha,1, Robert E. Hermesb, Andrew M.T. Moorec, Douglas J. Kennettd, James C. Weavere, James H. Wittkea, Paul S. DeCarlif, James L. Bischoffg, Gordon C. Hillmanh, George A. Howardi, David R. Kimbelj, Gunther Kletetschkak,l, Carl P. Lipom, Sachiko Sakaim, Zsolt Revayn, Allen Westo, Richard B. Firestonep, and James P. Kennettq aGeology Program, School of Earth Science and Environmental Sustainability, Northern Arizona University, Flagstaff, AZ 86011; bLos Alamos National Laboratory (retired), Los Alamos, NM 87545; cCollege of Liberal Arts, Rochester Institute of Technology, Rochester, NY 14623; dDepartment of Anthropology, Pennsylvania State University, University Park, PA 16802; eWyss Institute for Biologically Inspired Engineering, Harvard University, Cambridge, MA 02138; fSRI International, Menlo Park, CA 94025; gUS Geological Survey, Menlo Park, CA 94025; hInstitute of Archaeology, University College London, London, United Kingdom; iRestoration Systems, LLC, Raleigh, NC 27604; jKimstar Research, Fayetteville, NC 28312; kFaculty of Science, Charles University in Prague, and lInstitute of Geology, Czech Academy of Science of the Czech Republic, v.v.i., Prague, Czech Republic; mInstitute for Integrated Research in Materials, Environments, and Society (IIRMES), California State University, Long Beach, CA 90840; nForschungsneutronenquelle Heinz Maier-Leibnitz (FRM II), Technische Universität München, Munich, Germany; oGeoScience Consulting, Dewey, AZ 86327; pLawrence Berkeley National Laboratory, Berkeley, CA 94720; and qDepartment of Earth Science and Marine Science Instititute, University of California, Santa Barbara, CA 93106 Edited by* Steven M. Stanley, University of Hawaii, Honolulu, HI, and approved April 30, 2012 (received for review March 19, 2012) It has been proposed that fragments of an asteroid or comet (2). -
The Kufrah Paleodrainage System in Libya: a Past Connection to the Mediterranean Sea? Philippe Paillou, Stephen Tooth, S
The Kufrah paleodrainage system in Libya: A past connection to the Mediterranean Sea? Philippe Paillou, Stephen Tooth, S. Lopez To cite this version: Philippe Paillou, Stephen Tooth, S. Lopez. The Kufrah paleodrainage system in Libya: A past connection to the Mediterranean Sea?. Comptes Rendus Géoscience, Elsevier Masson, 2012, 344 (8), pp.406-414. 10.1016/j.crte.2012.07.002. hal-00833333 HAL Id: hal-00833333 https://hal.archives-ouvertes.fr/hal-00833333 Submitted on 12 Jun 2013 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. *Manuscript / Manuscrit The Kufrah Paleodrainage System in Libya: 1 2 3 A Past Connection to the Mediterranean Sea ? 4 5 6 7 8 9 Le système paléo-hydrographique de Kufrah en Libye : 10 11 12 Une ancienne connexion avec la mer Méditerranée ? 13 14 15 16 17 18 19 20 Philippe PAILLOU 21 22 Univ. Bordeaux, LAB,UMR 5804, F-33270, Floirac, France 23 24 Tel: +33 557 776 126 Fax: +33 557 776 110 25 26 27 E-mail: [email protected] 28 29 30 31 32 Stephen TOOTH 33 34 Institute of Geography and Earth Sciences, Aberystwyth University, Ceredigion, UK 35 36 37 38 39 Sylvia LOPEZ 40 41 42 Univ. -
The Uweinat Area Contains Three Different
Chapter 8 CRATER FORMS IN THE UWEINAT REGION FAROUK EL-BAZ National Air and Space Museum Smithsonian Institution Washington, D.C. 29560 BAHAY ISSAWI Geological Survey of Egypt Abbasia, Cairo Egypt ABSTRACT The Uweinat area contains three different varieties of avater forms^ rtamely: 1} two, mutti-ringed impact structures in southeast Libya, including the Oasis astrobleme and the BP structure, and two other aimters of possible impact origin; 2} simple, breached, and complex volcanic craters northeast .of Gebel Uweinat^ some of which nay he maars and other aryptoexptosion structures; and 3) a complex of large ciraular, shallow depressions east of Gebel Kissu in north- west Sudan, Because the number and variety of crater forms in the Uweinat area is unique, additional photogeot ogic interpretations are required based on computer-enhanced Landeat images or high resolution photographs from the Shuttle. These interpretations will allow detailed correla- tions of crater forms in this region with similar features on planetary bodies such as the Moon, Mars and Mercury. INTRODUCTION The eastern part of the Sahara where the borders of Egypt, Libya and Sudan meet is underlain by a Précambrien complex of metamorphlc and intrusive rocks (Sandford, 1935c; Said, 1962 ; and Pesce, 1968). This complex is one of many that cropout in the middle of the Sahara, separating it into northern and southern parts. This "Oweinat series" (Hume, 1934, p. 55) of metamorphics is intruded by granites with subordinate rhyolites, which are believed to be of post- Carboniferous age (Pesce, 1968, p, 62). Four major intrusions average approximately 20 km in diameter including the mountains known as Gebel Babein, El-Bahri, Arkenu, and Uweinat (Fig, 8.1), The Precambrian rocks are surrounded by hard quartzitic sand- stones with highly consolidated conglomerate and syenite porphyry sheets, which are Interbedded with sandstones, phonolites and trachyte sills, all of Paleozoic age (Issawi, 1980). -
The Dakhleh Glass: Product of an Impact Airburst Or Cratering Event in the Western Desert of Egypt?
The Dakhleh Glass: Product of an impact airburst or cratering event in the Western Desert of Egypt? Item Type Article; text Authors Osinski, G. R.; Kieniewicz, J.; Smith, J. R.; Boslough, M. B. E.; Eccleston, M.; Schwarcz, H. P.; Kleindienst, M. R.; Haldemann, A. F. C.; Churcher, C. S. Citation Osinski, G. R., Kieniewicz, J., Smith, J. R., Boslough, M. B. E., Eccleston, M., Schwarcz, H. P., ... & Churcher, C. S. (2008). The Dakhleh Glass: Product of an impact airburst or cratering event in the Western Desert of Egypt?. Meteoritics & Planetary Science, 43(12), 2089-2107. DOI 10.1111/j.1945-5100.2008.tb00663.x Publisher The Meteoritical Society Journal Meteoritics & Planetary Science Rights Copyright © The Meteoritical Society Download date 07/10/2021 14:51:55 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/656510 Meteoritics & Planetary Science 43, Nr 12, 2089–2107 (2008) Abstract available online at http://meteoritics.org The Dakhleh Glass: Product of an impact airburst or cratering event in the Western Desert of Egypt? Gordon R. OSINSKI1*, Johanna KIENIEWICZ2, Jennifer R. SMITH3, Mark B. E. BOSLOUGH4, Mark ECCLESTON5, Henry P. SCHWARCZ6, Maxine R. KLEINDIENST7, Albert F. C. HALDEMANN8, and Charles S. CHURCHER9 1Departments of Earth Sciences/Physics and Astronomy, University of Western Ontario, London, ON N6A 5B7, Canada 2Department of Geosciences, Denison University, Granville, Ohio 43023, USA 3Earth and Planetary Sciences, Washington University, Campus Box 1169, One Brookings Drive, Saint Louis, Missouri 63130, USA 4Sandia National Laboratories, P.O. Box 5800, Albuquerque, New Mexico 87185, USA 5Archaeology Program, La Trobe University, Bundoora 3086, Australia 6School of Geography and Earth Sciences, McMaster University, Hamilton, ON L8S 4K1, Canada 7Department of Anthropology, University of Toronto at Mississauga, 3359 Mississauga Road North, Mississauga, ON L5L 1C6, Canada 8European Space Agency, ESTEC HME-ME, P.O. -
Meteorite-Times 2014 7.Pdf
Meteorite Times Magazine Contents by Editor Featured Articles Accretion Desk by Martin Horejsi Jim’s Fragments by Jim Tobin Meteorite Market Trends by Michael Blood Bob’s Findings by Robert Verish Micro Visions by John Kashuba Norm’s Tektite Teasers by Norm Lehrman Mr. Monning’s Collection by Anne Black IMCA Insights by The IMCA Team Meteorite of the Month by Editor Tektite of the Month by Editor Terms Of Use Materials contained in and linked to from this website do not necessarily reflect the views or opinions of The Meteorite Exchange, Inc., nor those of any person connected therewith. In no event shall The Meteorite Exchange, Inc. be responsible for, nor liable for, exposure to any such material in any form by any person or persons, whether written, graphic, audio or otherwise, presented on this or by any other website, web page or other cyber location linked to from this website. The Meteorite Exchange, Inc. does not endorse, edit nor hold any copyright interest in any material found on any website, web page or other cyber location linked to from this website. The Meteorite Exchange, Inc. shall not be held liable for any misinformation by any author, dealer and or seller. In no event will The Meteorite Exchange, Inc. be liable for any damages, including any loss of profits, lost savings, or any other commercial damage, including but not limited to special, consequential, or other damages arising out of this service. © Copyright 2002–2014 The Meteorite Exchange, Inc. All rights reserved. No reproduction of copyrighted material is allowed by any means without prior written permission of the copyright owner. -
GOTTHILF HAGEN (1797 – 1884) Todestag in Angemessener Form Ehren Würde!
DWhG-Mitteilungen Nr. 14/April 2009 ►ANHANG vorbildlichen Zustand versetzt worden. Es würde der heutigen Wasser- und Schifffahrtsverwaltung gut zu HANS-JOACHIM UHLEMANN: Gesicht stehen, wenn sie ihren „Altmeister“ an seinem GOTTHILF HAGEN (1797 – 1884) Todestag in angemessener Form ehren würde! Einführung Gotthilf Hagen - Leben und Wirken Am 3. Februar 2009 jährte sich zum 125. Mal der Todes- tag von Gotthilf Heinrich Hagen, dem wohl verdienst- I. Einleitung vollsten deutschen Wasserbauer der Vergangenheit. Mit Drei Männer der Vergangenheit sind es, denen seinem „Handbuch der Wasserbaukunst“ hat er Gene- vornehmlich die deutsche Wasserbaukunst ihr Entstehen rationen von Wasserbauern im 19. Jahrhundert geprägt und ihre Entwicklung verdankt: Tulla, Hagen und und auch später noch ist dieses letzte umfassende Stan- Franzius. dardwerk des gesamten Wasserbaues von vielen Johann Gottfried Tulla, 20. März 1770 bis 27. März 1828, Berufskollegen mit Gewinn gelesen worden. Teile der war bahnbrechend für den Ausbau des oberen Rheins, voluminösen Enzyklopädie standen, wie der Unter- also für die Regulierung eines binnenländischen Stroms. zeichner aus eigener Anschauung weiß, noch bis weit Ludwig Franzius, 1. März 1832 bis 23. Juni 1903, führte nach dem Zweiten Weltkrieg in den Handbibliotheken den ersten planmäßig gestalteten und erfolgreichen von Dienststellen der ostdeutschen Wasserstraßen- Ausbau der im Flutwechsel belegenen Mündungsstrecke verwaltung. Leider ist im Lauf der letzten Jahrzehnte die eines Stromes aus, der Unterweser nebst dem Erinnerung an diesen großen deutschen Wasserbauer Freihafen I in Bremen und der Außenweser. immer mehr verschwunden und sein Name bei den Fachkollegen der jüngeren Generation fast unbekannt. Gotthilf Hagen, 3. März 1797 bis 3. Februar 1884, Zu Unrecht, wie ich hier betonen möchte! Auch heute schließlich war nicht nur im Strombau und im Seebau noch kann man, insbesondere in historischer Sicht, aus erfolgreich tätig, sondern er war auch der erste dem gewaltigen Werk von Hagen schöpfen. -
The "Uweinat Desert" of Egypt, Libya and Sudan: a Fertile Field for Planetary Comparisons of Crater Forms
THE "UWEINAT DESERT" OF EGYPT, LIBYA AND SUDAN: A FERTILE FIELD FOR PLANETARY COMPARISONS OF CRATER FORMS. Farouk El-Baz, National Air and Space Museum, Smithsonian Institution, Washington, D.C. 20560. The Western Desert of Egypt and adjacent parts of Libya and Sudan constitute the driest expanses of land on Earth (1). The southeastern part of the Western Desert has been named the Arba'in Desert (2). The southwestern part of the Western Desert and adjacent areas of Libya and Sudan are here named the Uweinat Desert after the prominent, 60 x 40 km-large, 1900 m-high mountain at the intersection of the borders of the three countries (Fig. 1, left) . This region of the eastern Sahara displays numerous features that have been correlated with surface features of Mars (3,4,5). Of particular signifi- cance are the wind streaks caused by lag deposits and sand dunes (4,5), the pitted and fluted rocks strewn on the surface (5,7), and the dry valleys of fluvial origin that resemble tributaries of martian canyons (4,5). In addition there are both impact and volcanic crater forms (8) that can be correlated with craters on the surfaces of terrestrial planetary bodies. This paper deals with these crater forms, including the first report on an impact crater in the Great Sand Sea. Landsat images revealed a group of peculiarly circular features about 130 km E-SE of Gebel Uweinat (A in Fig. 1, left). The rims of these structures are marked by discontinuous arcs and knobs in a terrain that is heavily modified by eolian action. -
A 2003 Expedition Into the Libyan Desert Glass Strewn Field, Great Sand Sea, Western Egypt
Large Meteorite Impacts (2003) 4079.pdf A 2003 EXPEDITION INTO THE LIBYAN DESERT GLASS STREWN FIELD, GREAT SAND SEA, WESTERN EGYPT. Christian Koeberl1, Michael R. Rampino2, Dona A. Jalufka1, and Deborah H. Winiarski2. 1Department of Geological Sciences, University of Vienna, Althanstrasse 14, Vienna, A-1090, Austria, (chris- [email protected]), 2Earth & Environmental Science Program, New York University, 100 Washington Square East, New York, NY 10003, USA ([email protected]). Introduction: Libyan Desert Glass (LDG) is an partly digested mineral phases, lechatelierite (a high- enigmatic type of natural glass that is found in an area temperature mineral melt of quartz), and baddeleyite, a with an extension of several thousand square kilometers. high-temperature breakdown product of zircon. Literature values on the extent vary between about 2000 The rare earth element abundance patterns are and 6500 km². This area, or strewn field, is located indicative of a sedimentary precursor rock, and the trace between sand dunes of the southwestern corner of the element abundances and ratios are in agreement with an Great Sand Sea in western Egypt, near the border to upper crustal source. There is a similarity between LDG Libya. Therefore, the name "Libyan" Desert Glass is not major and trace element abundances and Sr and Nd entirely correct, given today’s geographical boundaries, isotopic compositions and the respective values for rocks but refers to the traditional name of the desert. P.A. from the B.P. and Oasis impact structures in eastern Clayton was the first to travel the region in the early Libya, but lack of age information for the two Libyan 1930s and to collect glass samples that were used to structures precludes a definitive conclusion.