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Ron Hartman and the Lucerne Valley Meteorites by Robert Verish Ron Hartman and the Lucerne Valley Meteorites
Meteorite Times Magazine Contents by Editor Featured Monthly Articles Accretion Desk by Martin Horejsi Jim's Fragments by Jim Tobin Meteorite Market Trends by Michael Blood Bob's Findings by Robert Verish IMCA Insights by The IMCA Team Micro Visions by John Kashuba Meteorite Calendar by Anne Black 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 2002–2011 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. -
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. -
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. -
Workshop on the Issue of Martian Meteorites 7027.Pdf
Workshop on the Issue of Martian Meteorites 7027.pdf RECOVERING MORE ANTARCTIC MARTIAN METEORITES: ANSWERS TO COMMON QUESTIONS. R. P. Harvey1 and W. A. Cassidy2, 1Case Western Reserve University, Cleveland OH 44106-7216, USA ([email protected]), 2Department of Geology and Planetary Science, University of Pittsburgh, Pittsburgh PA 15260, USA ([email protected]). Introduction: Of the 13 Martian meteorites reported, they could, tell them from Earth rocks), they can help us almost half were collected in Antarctica. With the increased find exposed blue ice, and help us discern the shape and interest in Martian meteorite studies accompanying the re- topography of an icefield. These images speed up our re- port of possible biogenic activity in ALH84001, many have connaissance and greatly facilitate systematic searching wondered whether recoveries of Antarctic Martian meteor- efforts. They also serve as the only available basemap for ites could be enhanced or accelerated. Given that the recov- precisely locating our finds, given that many Antarctic ice- ery of Antarctic meteorites is a planned activity, (unlike the fields lie off existing topographical maps. recovery of non-Antarctic Martian meteorites via random finds and falls), such questions are worth considering. 3. If we sent an army of professional meteorite Listed below are several topical questions, followed by an- hunters, could we gather Martian meteorites more swers based on experience gathered during the 21 com- quickly? pleted field seasons of ANSMET (the Antarctic Search for The answer to this one is “maybe”. Success in Meteorites program). finding Antarctic meteorites depends on a lot of factors, of which manpower is only one. -
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). -
Machine Learning for Semi-Automated Meteorite Recovery
Machine Learning for Semi-Automated Meteorite Recovery Seamus Anderson1*, Martin Towner1, Phil Bland1, Christopher Haikings2,3, William Volante4, Eleanor Sansom1, Hadrien Devillepoix1, Patrick Shober1, Benjamin Hartig1, Martin Cupak1, Trent Jansen- Sturgeon1, Robert Howie1, Gretchen Benedix1, Geoff Deacon5 1Space Science and Technology Center, Curtin University, GPO Box U1987, Perth, WA 6845, Australia 2Spectre UAV Concepts, 191 St Georges Terrace, Perth, WA 6000, Australia 3Amotus Pty Ltd, Level 25/71 Eagle St, Brisbane City, QLD 4000, Australia 4Department of Psychology, Clemson University, 418 Brackett Hall, Clemson, SC, 29634 5Western Australian Museum, 49 Kew St, Welshpool, WA 6106, Australia *Corresponding author: E-mail: [email protected]. Abstract We present a novel methodology for recovering meteorite falls observed and constrained by fireball networks, using drones and machine learning algorithms. This approach uses images of the local terrain for a given fall site to train an artificial neural network, designed to detect meteorite candidates. We have field tested our methodology to show a meteorite detection rate between 75-97%, while also providing an efficient mechanism to eliminate false-positives. Our tests at a number of locations within Western Australia also showcase the ability for this training scheme to generalize a model to learn localized terrain features. Our model-training approach was also able to correctly identify 3 meteorites in their native fall sites, that were found using traditional searching techniques. Our methodology will be used to recover meteorite falls in a wide range of locations within globe- spanning fireball networks. Introduction Fireballs and meteors have been observed since antiquity by Chinese, Korean, Babylonian and Roman astronomers (Bjorkman 1973), while meteorites and their unique metallurgical properties have also been known and used by various cultures around the world from Inuit tools (Rickard 1941) to an Egyptian ceremonial dagger (Comelli et al. -
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. -
Takysie Lake – the Classic “Pseudometeorite” – Found by Harvey H
Meteorite Times Magazine Contents Paul Harris Featured Articles Accretion Desk by Martin Horejsi Jim’s Fragments by Jim Tobin Bob’s Findings by Robert Verish Micro Visions by John Kashuba Norm’s Tektite Teasers by Norm Lehrman 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 2002–2016 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. Meteorite Times Magazine Oriented Canyon Diablo Meteorite? I hope so. -
The Aquarius Project: the First Student-Driven Underwater Meteorite Hunt
The Aquarius Project: The First Student-Driven Underwater Meteorite Hunt Chris Bresky1, Marc Fries2, 1Adler Planetarium, Chicago IL, 2NASA JSC Astromaterials Research and Exploration Science (ARES), Houston TX Introduction Project Overview Ongoing Work Opportunities for Researchers On February 6, 2017, a sonic boom woke residents of the Midwest as a bright green fireball streaked across the sky. The American Meteor Society (AMS) calculated a ground track that terminated over Lake Michigan (Figure 1). Weather radar imagery showed a large meteorite fall, with all meteorites falling into the lake, off the coast of Wisconsin. The strewn field is in deep water (~100m) and no detailed maps of the lake bed exist in this region, so the subsurface environment is unknown and difficult to explore. We know of no previous systematic attempt at underwater recovery of meteorites. It is this combination of knowns and unknowns that has inspired high school students and science professionals from across Chicago to mount, “The Aquarius Project.” This multidisciplinary endeavor is the first student driven attempt at underwater meteorite retrieval. In an unprecedented collaboration, scientists and educators from The Field Museum, The Shedd Aquarium, and the Adler Planetarium’s Far Horizons Program are joining forces to support this expedition. Background Senior Research Biologist Dr. Philip Willink from the Shedd Aquarium works with the Aquarius Project Currently: Nearly 50 teens from these institutes are currently collaborating students to learn the techniques of lake bottom mapping through sonar. Once the lake bottom terrain is digitally to improve on the initial designs. They are engineering environmental understood, these teens will have a better idea of where to implement their meteorite hunting tools. -
Mars Lifer’ ALH84001, the Diogenite NWA 5484
Meteorite Times Magazine Contents Paul Harris Featured Articles Accretion Desk by Martin Horejsi Jim’s Fragments by Jim Tobin Bob’s Findings by Robert Verish Micro Visions by John Kashuba Norm’s Tektite Teasers by Norm Lehrman Meteorites in the News 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 2002–2020 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. -
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. -
Paléomagnétisme De La Matière Extraterrestre: Implications Pour La
0 1 « Absorbé par les recherches sur l’infiniment grand, puis l’infiniment petit, le scientifique a négligé, de façon coupable, le fantastique potentiel de l’infiniment moyen. » Grégoire Lacroix 2 3 « Alors, tu en es où de tes études ? » « Et bien, j’ai rendu mon manuscrit de thèse au mois d’octobre et je soutiens le 4 décembre 2013 »…. Déjà. Ces trois année s de thèse sont passées à toute allure, entre expériences, rencontres, voyages, rigolades… (moment de nosta lgie… :-/ mais positive hein !! L’heure est donc aux remerciements ;-)). En premier lieu, je tiens à remercier mes directeurs de thèse, Mr Pierre Rochette et tout particulièrement Mr Jérôme Gattacceca, sans qui toute cette « histoire » n’aurait pas pu être écrite, pour la confiance qu’ils m’ont accordée en me confiant ce trav ail de recherche ainsi que pour leur aide, leurs encouragements et leurs précieux conseils au cours de ces années. Je les remercie aussi pour toutes les opportunités qu’ils m’ont offert es à travers de multiples voyages. Je remercie également Mr Nicolas Thouveny, directeur du laboratoire du CEREGE pour m’avoir accueillie au sein de cette institution et pour les conseils et les encouragements que j’ai eu l’honneur de recevoir de sa part. J’ai pu travailler dans un cadre particulièrement agréable, grâce à l’ensemble des membres de l’équipe « géophysique/planétologie » du CEREGE que j’ai intégrée pour ces 3 ans de thèse (et encore pour un an ;)), je vous en remercie. Ces trois années n’auraient pas été ce qu’elles ont été sans Mr François Demory, ingénieur de recherche, « mon mentor »… fidèle collègue et ami à qui j’aimerais adresser un remerciement particulier pour tout (il y en a tellement à dire mais bon, disons…) ses conseils, sa disponib ilité, son soutien indéfectible et ses tranches de rigolades J autour d’un café.