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Australian Aborigines and Meteorites
Records of the Western Australian Museum 18: 93-101 (1996). Australian Aborigines and meteorites A.W.R. Bevan! and P. Bindon2 1Department of Earth and Planetary Sciences, 2 Department of Anthropology, Western Australian Museum, Francis Street, Perth, Western Australia 6000 Abstract - Numerous mythological references to meteoritic events by Aboriginal people in Australia contrast with the scant physical evidence of their interaction with meteoritic materials. Possible reasons for this are the unsuitability of some meteorites for tool making and the apparent inability of early Aborigines to work metallic materials. However, there is a strong possibility that Aborigines witnessed one or more of the several recent « 5000 yrs BP) meteorite impact events in Australia. Evidence for Aboriginal use of meteorites and the recognition of meteoritic events is critically evaluated. INTRODUCTION Australia, although for climatic and physiographic The ceremonial and practical significance of reasons they are rarely found in tropical Australia. Australian tektites (australites) in Aboriginal life is The history of the recovery of meteorites in extensively documented (Baker 1957 and Australia has been reviewed by Bevan (1992). references therein; Edwards 1966). However, Within the continent there are two significant areas despite abundant evidence throughout the world for the recovery of meteorites: the Nullarbor that many other ancient civilizations recognised, Region, and the area around the Menindee Lakes utilized and even revered meteorites (particularly of western New South Wales. These accumulations meteoritic iron) (e.g., see Buchwald 1975 and have resulted from prolonged aridity that has references therein), there is very little physical or allowed the preservation of meteorites for documentary evidence of Aboriginal acknowledge thousands of years after their fall, and the large ment or use of meteoritic materials. -
Lost Lake by Robert Verish
Meteorite-Times Magazine Contents by Editor Like Sign Up to see what your friends like. 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 Galactic Lore by Mike Gilmer Meteorite Calendar by Anne Black Meteorite of the Month by Michael Johnson 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 2002–2010 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. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
Did a Comet Deliver the Chelyabinsk Meteorite?
EPSC Abstracts Vol. 11, EPSC2017-2, 2017 European Planetary Science Congress 2017 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2017 Did a Comet Deliver the Chelyabinsk Meteorite? O.G. Gladysheva Ioffe Physical-Technical Institute of RAS, St.Petersburg, Russa, ([email protected] / Fax: +7(812)2971017) Abstract source of the appearance of such a gradient can be only the direct bombardment of the crystal by SCR An explosion of a celestial body occurred on the iron nuclei with energy of 1-100 MeV [6]. fifteenth of February, 2013, near Chelyabinsk Interacting with the surface of the meteorite, protons (Russia). The explosive energy was determined as and helium GCR nuclei form isotopes, some ~500 kt of TNT, on the basis of which the mass of radioactive, which are allocated to a specific location the bolide was estimated at ~107 kg, and its diameter by depth in the body of the meteorite. A measurement of the composition of radionuclides at ~19 m [1]. Fragments of the meteorite, such as 22 26 54 60 LL5/S4-WO type ordinary chondrite [2] with a total Na, Al, Mn and Co in 12 fragments of the mass only of ~2·103 kg, fell to the earth’s surface [3]. Chelyabinsk meteorite, and a comparison of the Here, we will demonstrate that the deficit of the results with model calculations of the formation of celestial body’s mass can be explained by the arrival these isotopes in meteorites according to depth, of the Chelyabinsk chondrite on Earth by a showed that 4 fragments of the meteorite were significantly more massive but fragile ice-bearing located in a layer 30 cm deep, 3 fragments at a depth celestial body. -
Research Outputs 1
Research outputs 1. Annealing of the seymchan meteorite at the temperature of 700 °C Brusnitsyna, E. V., Muftakhetdinova, R. F., Yakovlev, G. A., Tyutrina, T. V. & Grokhovsky, V. I., 9 Dec 2020, VII International Young Researchers'' Conference - Physics, Technology, Innovations, PTI 2020. Volkovich, V. A., Kashin, I. V., Smirnov, A. A. & Narkhov, E. D. (eds.). American Institute of Physics Inc., 5 p. 060002. (AIP Conference Proceedings; vol. 2313). 2. Structural features of the seymchan meteorite substance after compressing by spherically converging shock waves Muftakhetdinova, R. F., Grokhovsky, V. I., Kuchko, D. P. & Vorobiev, A. V., 9 Dec 2020, VII International Young Researchers'' Conference - Physics, Technology, Innovations, PTI 2020. Volkovich, V. A., Kashin, I. V., Smirnov, A. A. & Narkhov, E. D. (eds.). American Institute of Physics Inc., 6 p. 060012. (AIP Conference Proceedings; vol. 2313). 3. Synthesis of nanostructures on the Chinga meteorite Begunova, A. S., Yakovlev, G. A., Kamalov, R. V., Pankrushina, E. A. & Grokhovsky, V. I., 9 Dec 2020, VII International Young Researchers'' Conference - Physics, Technology, Innovations, PTI 2020. Volkovich, V. A., Kashin, I. V., Smirnov, A. A. & Narkhov, E. D. (eds.). American Institute of Physics Inc., 6 p. 030039. (AIP Conference Proceedings; vol. 2313). 4. Post-impact metamorphism of the Chelyabinsk meteorite in shock experiment Grokhovsky, V. I., Muftakhetdinova, R. F., Yakovlev, G. A., Brusnitsyna, E. V. & Petrova, E. V., 1 Nov 2020, In: Planetary and Space Science. 192, 8 p., 105050. 5. Experimental constraints on the ordinary chondrite shock darkening caused by asteroid collisions Kohout, T., Petrova, E. V., Yakovlev, G. A., Grokhovsky, V. I., Penttila, A., Maturilli, A., Moreau, J. -
Chelyabinsk Airburst, Damage Assessment, Meteorite Recovery and Characterization
O. P. Popova, et al., Chelyabinsk Airburst, Damage Assessment, Meteorite Recovery and Characterization. Science 342 (2013). Chelyabinsk Airburst, Damage Assessment, Meteorite Recovery, and Characterization Olga P. Popova1, Peter Jenniskens2,3,*, Vacheslav Emel'yanenko4, Anna Kartashova4, Eugeny Biryukov5, Sergey Khaibrakhmanov6, Valery Shuvalov1, Yurij Rybnov1, Alexandr Dudorov6, Victor I. Grokhovsky7, Dmitry D. Badyukov8, Qing-Zhu Yin9, Peter S. Gural2, Jim Albers2, Mikael Granvik10, Läslo G. Evers11,12, Jacob Kuiper11, Vladimir Kharlamov1, Andrey Solovyov13, Yuri S. Rusakov14, Stanislav Korotkiy15, Ilya Serdyuk16, Alexander V. Korochantsev8, Michail Yu. Larionov7, Dmitry Glazachev1, Alexander E. Mayer6, Galen Gisler17, Sergei V. Gladkovsky18, Josh Wimpenny9, Matthew E. Sanborn9, Akane Yamakawa9, Kenneth L. Verosub9, Douglas J. Rowland19, Sarah Roeske9, Nicholas W. Botto9, Jon M. Friedrich20,21, Michael E. Zolensky22, Loan Le23,22, Daniel Ross23,22, Karen Ziegler24, Tomoki Nakamura25, Insu Ahn25, Jong Ik Lee26, Qin Zhou27, 28, Xian-Hua Li28, Qiu-Li Li28, Yu Liu28, Guo-Qiang Tang28, Takahiro Hiroi29, Derek Sears3, Ilya A. Weinstein7, Alexander S. Vokhmintsev7, Alexei V. Ishchenko7, Phillipe Schmitt-Kopplin30,31, Norbert Hertkorn30, Keisuke Nagao32, Makiko K. Haba32, Mutsumi Komatsu33, and Takashi Mikouchi34 (The Chelyabinsk Airburst Consortium). 1Institute for Dynamics of Geospheres of the Russian Academy of Sciences, Leninsky Prospect 38, Building 1, Moscow, 119334, Russia. 2SETI Institute, 189 Bernardo Avenue, Mountain View, CA 94043, USA. 3NASA Ames Research Center, Moffett Field, Mail Stop 245-1, CA 94035, USA. 4Institute of Astronomy of the Russian Academy of Sciences, Pyatnitskaya 48, Moscow, 119017, Russia. 5Department of Theoretical Mechanics, South Ural State University, Lenin Avenue 76, Chelyabinsk, 454080, Russia. 6Chelyabinsk State University, Bratyev Kashirinyh Street 129, Chelyabinsk, 454001, Russia. -
Handbook of Iron Meteorites, Volume 3 (Pima County – Ponca Creek)
974 Piedade do Bagre - Pima County Schreibersite is almost absent, but may be found as short, 5-l 0 J.1 wide grain boundary folia. Rhabdites are not observed. The bulk phosphorus content is estimated to be A between 0.05 and 0.10%. Troilite is scattered as small nodules and lenticular bodies, ranging from I to 5 mm in size. They occur with a frequency of about one per 20 cm2 , and contain 10-20% daubreelite in the form of parallel bars, 0.1-0.5 mm wide. Spencer & Hey (1930) reported cohenite, but this could not be confirmed. Piedade do Bagre is a somewhat annealed, medium octahedrite with an anomalously small bandwidth if com pared to Hen bury, Costilla Peak, Wabar and other irons of similar composition. The trace-element determination indi cates that it is in some degree related to these irons; Wasson (personal communication) feels, however, that it should be earmarked anomalous, since its combination of Ni, Ga, Ge and Ir places it outside the normal IliA range. This conclusion is supported by the bandwidth-Ni combination which is anomalous, too. Figure 1367. Pima County (U.S.N.M. no. 1447). The meteorite, originally a hexahedrite, is recrystallized due to shock and the Specimen in the U.S, National Museum in Washington: associated reheating. A heat-affected rim zone is present along the 398 g (no. 1559, 12 x 8.5 x 0.5 em) edge A-A. Imperfectly polished, black patches are due to corrosion. Deep-etched. Scale bar 10 mm. (Perry 1950: volume 7.) HISTORY Pierceville (iron), Kansas, U.S.A. -
ELEMENTAL ABUNDANCES in the SILICATE PHASE of PALLASITIC METEORITES Redacted for Privacy Abstract Approved: Roman A
AN ABSTRACT OF THE THESIS OF THURMAN DALE COOPER for theMASTER OF SCIENCE (Name) (Degree) in CHEMISTRY presented on June 1, 1973 (Major) (Date) Title: ELEMENTAL ABUNDANCES IN THE SILICATE PHASE OF PALLASITIC METEORITES Redacted for privacy Abstract approved: Roman A. Schmitt The silicate phases of 11 pallasites were analyzed instrumen- tally to determine the concentrations of some major, minor, and trace elements.The silicate phases were found to contain about 98% olivine with 1 to 2% accessory minerals such as lawrencite, schreibersite, troilite, chromite, and farringtonite present.The trace element concentrations, except Sc and Mn, were found to be extremely low and were found primarily in the accessory phases rather than in the pure olivine.An unusual bimodal Mn distribution was noted in the pallasites, and Eagle Station had a chondritic nor- malized REE pattern enrichedin the heavy REE. The silicate phases of pallasites and mesosiderites were shown to be sufficiently diverse in origin such that separate classifications are entirely justified. APPROVED: Redacted for privacy Professor of Chemistry in charge of major Redacted for privacy Chairman of Department of Chemistry Redacted for privacy Dean of Graduate School Date thesis is presented June 1,1973 Typed by Opal Grossnicklaus for Thurman Dale Cooper Elemental Abundances in the Silicate Phase of Pallasitic Meteorites by Thurman Dale Cooper A THESIS submitted to Oregon State University in partial fulfillment of the requirements for the degree of Master of Science June 1974 ACKNOWLEDGMENTS The author wishes to express his gratitude to Prof. Roman A. Schmitt for his guidance, suggestions, discussions, and thoughtful- ness which have served as an inspiration. -
Meteorites: Rocks from Space
Learning more... Meteorites: rocks from space Meteorites: Rocks from space It has been estimated that 100,000 rocks from space tonnes of extraterrestrial material Every year the Earth is showered by reach the Earth’s surface every year. It extraterrestrial material falling from can be anything from fine dust to space. The Museum’s mineralogy and metallic masses weighing many tonnes. petrology collections include a small Extraterrestrial material that falls towards the holding of meteorites, and a display of Earth is classified by size. The majority of this some of this material is on show in the material is in the form of tiny particles called rocks and minerals aisle of the main micrometeorites. They fall continuously, and court, along with a large touchable arrive unnoticed. specimen that fell in Nantan in China. Meteors or ‘shooting stars’ are often seen in a clear night sky. They are larger dust particles and small rocky fragments, many no more than a gram in weight, which are burnt up by friction as they fall through the Earth’s atmosphere. Meteorites are larger pieces of rock that reach the Earth’s surface without getting burnt up in the atmosphere. A meteorite whose arrival has been witnessed is called a fall. Meteorites discovered without a known time of fall are The Nantan meteorite called finds. All meteorites, falls and finds, are This meteorite comes from either Lihu or Yaozhai town in named after the place where they were picked Nantan County, Guangxi, China, where it fell in 1516. It is an iron meteorite weighing over 155 pounds (71kg), and is up. -
W Numerze: – Wywiad Z Kustoszem Watykańskiej Kolekcji C.D. – Cz¹stki
KWARTALNIK MI£OŒNIKÓW METEORYTÓW METEORYTMETEORYT Nr 3 (63) Wrzesieñ 2007 ISSN 1642-588X W numerze: – wywiad z kustoszem watykañskiej kolekcji c.d. – cz¹stki ze Stardusta a meteorytry – trawienie meteorytów – utwory sp³ywania na Sikhote-Alinach – pseudometeoryty – konferencja w Tucson METEORYT Od redaktora: kwartalnik dla mi³oœników OpóŸnieniami w wydawaniu kolejnych numerów zaczynamy meteorytów dorównywaæ „Meteorite”, którego sierpniowy numer otrzyma³em Wydawca: w paŸdzierniku. Tym razem g³ówn¹ przyczyn¹ by³y k³opoty z moim Olsztyñskie Planetarium komputerem, ale w koñcowej fazie redagowania okaza³o siê tak¿e, i Obserwatorium Astronomiczne ¿e brak materia³u. Musia³em wiêc poczekaæ na mocno opóŸniony Al. Pi³sudskiego 38 „Meteorite”, z którego dorzuci³em dwa teksty. 10-450 Olsztyn tel. (0-89) 533 4951 Przeskok o jeden numer niezupe³nie siê uda³, a zapowiedzi¹ [email protected] dalszych k³opotów jest mi³y sk¹din¹d fakt, ¿e przep³yw materia³ów zacz¹³ byæ dwukierunkowy. W najnowszym numerze „Meteorite” konto: ukaza³ siê artyku³ Marcina Cima³y o Moss z „Meteorytu” 3/2006, 88 1540 1072 2001 5000 3724 0002 a w kolejnym numerze zapowiedziany jest artyku³ o Morasku BOŒ SA O/Olsztyn z „Meteorytu” 4/2006. W rezultacie jednak bêdzie mniej materia³u do Kwartalnik jest dostêpny g³ównie t³umaczenia i trzeba postaraæ siê o dalsze w³asne teksty. Czy mo¿e ktoœ w prenumeracie. Roczna prenu- merata wynosi w 2007 roku 44 z³. chcia³by coœ napisaæ? Zainteresowanych prosimy o wp³a- Z przyjemnoœci¹ odnotowujê, ¿e nabieraj¹ tempa przygotowania cenie tej kwoty na konto wydawcy do kolejnej konferencji meteorytowej, która planowana jest na 18—20 nie zapominaj¹c o podaniu czytel- nego imienia, nazwiska i adresu do kwietnia 2008 r. -
Zac Langdon-Pole Art Basel Hong Kong
Zac Langdon-Pole Art Basel Hong Kong Michael Lett 312 Karangahape Road Cnr K Rd & East St PO Box 68287 Newton Auckland 1145 New Zealand P+ 64 9 309 7848 [email protected] www.michaellett.com Zac Langdon-Pole Passport (Argonauta) (i) 2018 paper nautilus shell, Seymchan meteorite (iron pallasite, landsite: Serbia, Russia) 79 x 25 x 45mm ZL5205 Zac Langdon-Pole Passport (Argonauta) (i) (side view) 2018 paper nautilus shell, Seymchan meteorite (iron pallasite, landsite: Serbia, Russia) 79 x 25 x 45mm ZL5205 Zac Langdon-Pole Passport (Argonauta) (ii) 2018 paper nautilus shell, Sikhote Alin meteorite (iron; coarse octahedrite, landsite: Sikhote Alin mountains, Russia) 103 x 30 x 55mm ZL5209 Zac Langdon-Pole Passport (Argonauta) (ii) (side view) 2018 paper nautilus shell, Sikhote Alin meteorite (iron; coarse octahedrite, landsite: Sikhote Alin mountains, Russia) 103 x 30 x 55mm ZL5209 Zac Langdon-Pole Passport (Argonauta) (iii) (front view and side view) 2018 paper nautilus shell, Nantan meteorite (iron; coarse octahedrite, landsite: Nantan, Peoples Republic of China) 135 x 45 x 95mm ZL5213 Zac Langdon-Pole Passport (Argonauta) (iv) (front view and side view) 2018 paper nautilus shell, Muonionalusta meteorite (iron; fine octahedrite, landsite: Norrbotten, Sweden) 95 x 33 x 65mm ZL5208 Zac Langdon-Pole Passport (Argonauta) (v) 2018 paper nautilus shell, Sericho meteorite (iron pallasite, landsite: Sericho, Kenya) 107 x 33 x 56mm ZL5210 Zac Langdon-Pole Passport (Argonauta) (v) (side view) 2018 paper nautilus shell, Sericho meteorite (iron -
Numerical Modeling of the 2013 Meteorite Entry in Lake Chebarkul, Russia
Nat. Hazards Earth Syst. Sci., 17, 671–683, 2017 www.nat-hazards-earth-syst-sci.net/17/671/2017/ doi:10.5194/nhess-17-671-2017 © Author(s) 2017. CC Attribution 3.0 License. Numerical modeling of the 2013 meteorite entry in Lake Chebarkul, Russia Andrey Kozelkov1,2, Andrey Kurkin2, Efim Pelinovsky2,3, Vadim Kurulin1, and Elena Tyatyushkina1 1Russian Federal Nuclear Center, All-Russian Research Institute of Experimental Physics, Sarov, 607189, Russia 2Nizhny Novgorod State Technical University n. a. R. E. Alekseev, Nizhny Novgorod, 603950, Russia 3Institute of Applied Physics, Nizhny Novgorod, 603950, Russia Correspondence to: Andrey Kurkin ([email protected]) Received: 4 November 2016 – Discussion started: 4 January 2017 Revised: 1 April 2017 – Accepted: 13 April 2017 – Published: 11 May 2017 Abstract. The results of the numerical simulation of possi- Emel’yanenko et al., 2013; Popova et al., 2013; Berngardt et ble hydrodynamic perturbations in Lake Chebarkul (Russia) al., 2013; Gokhberg et al., 2013; Krasnov et al., 2014; Se- as a consequence of the meteorite fall of 2013 (15 Febru- leznev et al., 2013; De Groot-Hedlin and Hedlin, 2014): ary) are presented. The numerical modeling is based on the – the meteorite with a diameter of 16–19 m flew into the Navier–Stokes equations for a two-phase fluid. The results of ◦ the simulation of a meteorite entering the water at an angle earth’s atmosphere at about 20 to the horizon at a ve- ∼ −1 of 20◦ are given. Numerical experiments are carried out both locity of 17–22 km s . when the lake is covered with ice and when it is not.