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Astronomy 150: Killer Skies Lecture 5, January 27
Astronomy 150: Killer Skies Lecture 5, January 27 Last time: began Astro Threat I: Impacts Today: Meteors and Asteroids Homework: ‣ HW 1 due today, but allowing submission up until next Monday. ‣ HW 2 posted today, due next Friday at the start of class http://epod.usra.edu/blog/2011/01/fireball-breakup.html http://epod.usra.edu/blog/2011/05/willamette-meteorite.html Friday, January 27, 2012 Register your i>clicker Go to link on class web page to register your i>clicker ‣ Register with first part of your @illinois.edu email (NetID) If you can’t read your i>clicker ID ‣ Go the Illini bookstore bag-check counter ‣ Vote with your i>clicker ‣ Clicker ID will be displayed on the base unit https://online-s.physics.uiuc.edu/cgi/courses/shell/iclicker.pl Friday, January 27, 2012 Register your i>clicker Go to link on class web page to register your i>clicker ‣ Register with first part of your @illinois.edu email (NetID) If you can’t read your i>clicker ID ‣ Go the Illini bookstore bag-check counter ‣ Vote with your i>clicker ‣ Clicker ID will be displayed on the base unit https://online-s.physics.uiuc.edu/cgi/courses/shell/iclicker.pl Friday, January 27, 2012 Planetarium Session Purpose: ‣ To help you understand the motions of the sky Dates: 1/30, 1/31, 2/2, 2/6, 2/7, 2/8 @ Staerkel Planetarium, Parkland College ‣ Show starts at 7pm, runs ~80 minutes ‣ $3 door charge, please bring exact change Report due Feb 24th in class ‣ Details on class website ‣ Attach ticket from the show to your report Reserve a seat online ‣ Link to reservation site on class website Friday, January 27, 2012 Fireballs Since most meteors are from small objects, they burn up before they hit the ground. -
Disequilibrium Melting and Melt Migration Driven by Impacts: Implications for Rapid Planetesimal Core Formation
Available online at www.sciencedirect.com Geochimica et Cosmochimica Acta 100 (2013) 41–59 www.elsevier.com/locate/gca Disequilibrium melting and melt migration driven by impacts: Implications for rapid planetesimal core formation Andrew G. Tomkins ⇑, Roberto F. Weinberg, Bruce F. Schaefer 1, Andrew Langendam School of Geosciences, P.O. Box 28E, Monash University, Melbourne, Victoria 3800, Australia Received 20 January 2012; accepted in revised form 24 September 2012; available online 12 October 2012 Abstract The e182W ages of magmatic iron meteorites are largely within error of the oldest solar system particles, apparently requir- ing a mechanism for segregation of metals to the cores of planetesimals within 1.5 million years of initial condensation. Cur- rently favoured models involve equilibrium melting and gravitational segregation in a static, quiescent environment, which requires very high early heat production in small bodies via decay of short-lived radionuclides. However, the rapid accretion needed to do this implies a violent early accretionary history, raising the question of whether attainment of equilibrium is a valid assumption. Since our use of the Hf–W isotopic system is predicated on achievement of chemical equilibrium during core formation, our understanding of the timing of this key early solar system process is dependent on our knowledge of the seg- regation mechanism. Here, we investigate impact-related textures and microstructures in chondritic meteorites, and show that impact-generated deformation promoted separation of liquid FeNi into enlarged sulfide-depleted accumulations, and that this happened under conditions of thermochemical disequilibrium. These observations imply that similar enlarged metal accumu- lations developed as the earliest planetesimals grew by rapid collisional accretion. -
The History of the Hoba Meteorite III: Known and Loved by All
the hoba meteorite The History of the Hoba Meteorite III: Known and loved by all ... P E Spargo Department of Physics, University of Cape Town, Rondebosch 7701, South Africa [email protected] In spite of its remote location in the However, apart from Luyten’s very brief then little-visited and almost unknown note in the Harvard College Observatory territory of South-West Africa (Namibia Bulletin (Luyten, 1929a, reproduced in today), we saw previously (Spargo facsimile in Fig. 8 in the second of this 2008b) that the second decade of the series of articles) and his short, largely great meteorite’s life opened with its descriptive articles in the South African existence being relatively widely known Journal of Science (Luyten 1929b) and to the public in South Africa and the Popular Astronomy (Luyten, 1930), noth- United States. This was as a result of ing of serious scientific import had been articles in Die Volksblad (Bloemfon- published. tein), The Cape Times (Cape Town), The Star (Johannesburg) and The New York It will be recalled, however, that on 5 Times1. There were also brief notes in September 1929 the meteorite had been Die Sterne (R.H., 1930), the popular visited by a small party of geologists who German astronomical magazine, which were on an excursion to Southwest Africa at least alerted German astronomers following the International Geological to its existence, and the Zeitschrift für Congress, which had held its XV Session Praktische Geologie (Schneiderhöhn, in South Africa in July and August of that 1929) performing a similar function for year. -
Greenland Last Ice Area
kn Greenland Last Ice Area Potentials for hydrocarbon and mineral resources activities Mette Frost, WWF-DK Copenhagen, September 2014 Report Greenland Last Ice Area. Potentials for hydrocarbon and mineral resources activities. The report is written by Mette Frost, WWF Verdensnaturfonden. Published by WWF Verdensnaturfonden, Svanevej 12, 2400 København NV. Denmark. Phone +45 3536 3635 – E-mail: [email protected] WWF Global Arctic Programme, 275 Slater Street, Ottawa, Ontario, K1P 5L4. Canada. Phone: +1 613 232 2535 Project The report has been developed under the Last Ice Area project, a joint project between WWF Canada, WWF Denmark and WWF Global Arctic Programme. Other WWF reports on Greenland – Last Ice Area Greenland Last Ice Area. Scoping study: socioeconomic and socio-cultural use of the Greenland LIA. By Pelle Tejsner, consultant and PhD. and Mette Frost, WWF-DK. November 2012. Seals in Greenland – an important component of culture and economy. By Eva Garde, WWF-DK. November 2013. Front page photo: Yellow house in Kullorsuaq, Qaasuitsup Kommunia, Greenland. July 2012. Mette Frost, WWF Verdensnaturfonden. The report can be downloaded from www.wwf.dk [1] CONTENTS Last Ice Area Introduction 4 Last Ice Area / Sikuusarfiit Nunngutaat 5 Last Ice Area/ Den Sidste Is 6 Summary 7 Eqikkaaneq 12 Sammenfatning 18 1. Introduction – scenarios for resources development within the Greenland LIA 23 1.1 Last Ice Area 23 1.2 Geology of the Greenland LIA 25 1.3 Climate change 30 2. Mining in a historical setting 32 2.1 Experiences with mining in Greenland 32 2.2 Resources development to the benefit of society 48 3. -
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. -
Handbook of Iron Meteorites, Volume 3
1350 Yenberrie - York (Iron) Specimens in the U.S. National Museum in Washington: 3.54 kg on three slices (no. 607) 290 g part slice (no. 1626) York (Iron), Nebraska, U.S.A. Approximately 40°52'N, 97°35'W; 500 m Medium octahedrite, Om. Bandwidth 1.00±0.15 mm. E-structure. HV 305 ±15 . Probably group III A. About 7.7% Ni and 0.12% P. HISTORY A mass of 835 g was found in 1878 on the farm of ~ - . Robert M. Lytle, near York in York County. The mass was Figure 2007. Yenberric (U.S.N.M. no. 607). Taenite with cloudy plowed up from a edges and martensitic interior in which cloudy patches occasionally depth of 20 em in virgin, black loamy occur. Part of the explanation may be sought in the taenite lamella prairie soil. It was in the fmder's possession until 1895 being parallel to the plane of section. Etched. Scale bar 200 J.L. See when it was acquired by Barbour (1898) who described it also Figures 109 and 119. and gave figures of the exterior and of etched slices. COLLECfiONS \ New York (701 g), Washington (30 g). \ ANALYSES Kunz reported (in Barbour 1898) 7.38% Ni and 0 .74% Co. The sum appears correct, but the present author would expect that some of the nickel has been included with the cobalt. The meteorite is estimated to have the following composition: 7 .7±0.2% Ni, 0.50% Co, 0.12±0.02% P, with trace elements placing it in the chemical group IliA. -
Richardton and New Leipzig Meteorites Returning to North Dakota by Ed Murphy on the Evening of June 30, 1918 (About 10:00 P.M
Richardton and New Leipzig Meteorites Returning to North Dakota By Ed Murphy On the evening of June 30, 1918 (about 10:00 p.m. he received from Muggli, to George Merrill, Head Curator of mountain time), the Richardton meteorite fell to earth on either Geology at the Smithsonian. Merrill verified it was a stony side of ND Highway 8 about equidistance between the towns meteorite, but interestingly enough noted that it was quite of Richardton and Mott (fig. 1). The fireball of the meteoroid, weathered and that it probably belonged to an earlier fall, as it raced across the sky, was witnessed over an area of at that is, it was not the Richardton meteorite. least 18,000 square miles (fig. 2). A witness who was 130 miles to the southwest said, “As it came down, it illuminated Leonard was attempting to purchase specimens of the the landscape to almost the brilliancy of sunlight.” Witnesses Richardton meteorite when he received a letter dated closer to the fall area likened the sound of the meteoroid to an November 10, 1918 from T.T. Quirke. Quirke, a professor of “airship” or motorcycle. The 200-pound meteoroid broke geology at the University of Minnesota, had been sent out by into at least 200 pieces perhaps at a height of 60 miles above that department to investigate the fall. There is evidence that the earth. The sound of the breakup was said to have been a John Muggli contacted Quirke when he was unable to reach “fearful and terrifying noise,” “a deep tone thundering,” “a violent Leonard. -
Meteorite Collections: Sample List
Meteorite Collections: Sample List Institute of Meteoritics Department of Earth and Planetary Sciences University of New Mexico October 01, 2021 Institute of Meteoritics Meteorite Collection The IOM meteorite collection includes samples from approximately 600 different meteorites, representative of most meteorite types. The last printed copy of the collection's Catalog was published in 1990. We will no longer publish a printed catalog, but instead have produced this web-based Online Catalog, which presents the current catalog in searchable and downloadable forms. The database will be updated periodically. The date on the front page of this version of the catalog is the date that it was downloaded from the worldwide web. The catalog website is: Although we have made every effort to avoid inaccuracies, the database may still contain errors. Please contact the collection's Curator, Dr. Rhian Jones, ([email protected]) if you have any questions or comments. Cover photos: Top left: Thin section photomicrograph of the martian shergottite, Zagami (crossed nicols). Brightly colored crystals are pyroxene; black material is maskelynite (a form of plagioclase feldspar that has been rendered amorphous by high shock pressures). Photo is 1.5 mm across. (Photo by R. Jones.) Top right: The Pasamonte, New Mexico, eucrite (basalt). This individual stone is covered with shiny black fusion crust that formed as the stone fell through the earth's atmosphere. Photo is 8 cm across. (Photo by K. Nicols.) Bottom left: The Dora, New Mexico, pallasite. Orange crystals of olivine are set in a matrix of iron, nickel metal. Photo is 10 cm across. (Photo by K. -
W Numerze: – Wspominanie R. Nortona – Po¿Egnanie G
KWARTALNIK MI£OŒNIKÓW METEORYTÓW METEORYTMETEORYT Nr 4 (72) Grudzieñ 2009 ISSN 1642-588X Gujba W numerze: – wspominanie R. Nortona – po¿egnanie G. Kurata i Ch. Angera – intryguj¹ce ciemne inkluzje – jeszcze o meteorycie Lixna – skandal wokó³ ALH 84001 – 40 rocznica lotu Apollo 11 Od redaktora: METEORYT Zgodnie z zapowiedzi¹, w ostatnim numerze Meteorite z roku 2009 znalaz³y kwartalnik dla mi³oœników siê wspomnienia o Richardzie Nortonie, które w ca³oœci przenios³em do tego meteorytów numeru. Przez wiele lat mogliœmy czytaæ artyku³y Richarda w Meteorycie, a znaj¹cy jêzyk angielski mogli tak¿e czytaæ jego znakomite ksi¹¿ki. Pozna³em Wydawca: Richarda, gdy zwróci³em uwagê na zaskakuj¹c¹ zbie¿noœæ naszych losów Olsztyñskie Planetarium zawodowych: obaj zaczêliœmy od planetarium, a potem zajêliœmy siê i Obserwatorium Astronomiczne meteorytami; tylko moje osi¹gniêcia s¹ skromniejsze. Poniewa¿ znajomoœæ Al. Pi³sudskiego 38 nasza zaczê³a siê w erze przed-emailowej, pozosta³a kolekcja piêknych listów 10-450 Olsztyn od Richarda na charakterystycznym, firmowym papierze. tel. (0-89) 533 4951 OpóŸnienie tego numeru i z³y los sprawi³y, ¿e niespodziewanie ¿egnamy nie tylko Richarda. Odszed³ Gero Kurat, d³ugoletni kustosz wiedeñskiej kolekcji [email protected] meteorytów, od którego przed laty otrzyma³em cenne informacje i zdjêcia konto: meteorytu Bia³ystok, a którego zas³ugi dla meteorytyki przypominaj¹ 88 1540 1072 2001 5000 3724 0002 wspó³pracownicy. ¯egnamy te¿ Christiana Angera, ogromnie lubianego BOŒ SA O/Olsztyn w meteorytowym œwiatku, który zas³yn¹³ tym, ¿e pierwszy meteoryt, jaki uda³o mu siê znaleŸæ samodzielnie, by³ jedynym okazem meteorytu Moravka, który Kwartalnik jest dostêpny g³ównie sta³ siê dostêpny dla prywatnych kolekcjonerów. -
Elastic Properties of Iron Meteorites. Nikolay Dyaur1, Robert R. Stewart1, and Martin Cassidy1, 1University of Houston, Science
51st Lunar and Planetary Science Conference (2020) 3063.pdf Elastic properties of iron meteorites. Nikolay Dyaur1, Robert R. Stewart1, and Martin Cassidy1, 1University of Houston, Science and Research Building 1, 3507 Cullen Boulevard, room 312, Houston, TX 77204, [email protected] Introduction: We investigate the elastic properties of a ture, in the iron meteorites indicates directionality in variety of iron meteorites using ultrasonic (0.5 MHz to 5 physical properties. So, we explored the possibility of MHz) laboratory measurements. Our meteorite samples elastic anisotropy. First, we estimated Vp- and Vs- include Campo de Cielo, Canyon Diablo, Gibeon, and anisotropy from the measured maximum and minimum Nantan. The densities of the meteorites range from 7.15 velocity for each sample. g/cc to 7.85 g/cc. P-wave velocities are from 5.58 km/s to 7.85 km/s, and S-wave velocities are from 2.61 km/s to 3.37 km/s. There is a direct relationship between P-wave velocity and density (approximately quadratic). We find evidence of anisotropy and S-wave splitting in the Gibe- on sample. These measurements may help inform studies related to planetary core properties, asteroid mining, and Earth protection. Iron meteorites are composed of Fe-Ni mixes with Fe content around 90%. The principal minerals are kamacite and taenite with some inclusions mainly repre- sented by troilite, graphite, diamond, gold, quartz, and some others. Iron meteorites are divided into groups based on their structure linked to Ni content: Hexahe- drites (4-6% of Ni), Octahedrites (6-14% of Ni) and Nickel-rich ataxites (>12% of Ni) [1]. -
Greenland Pt Anomaly May Point to Noncataclysmic Cape York Meteorite Entry
LETTER LETTER Greenland Pt anomaly may point to noncataclysmic Cape York meteorite entry Petaev et al. (1) tested the suite of hypotheses velocity and entry angle yields a crater of simplest explanation is to associate the anom- (collectively known as the “impact hypothe- between 15 and 20 km in diameter, unlikely aly with a local noncataclysmic event that is sis”) that a swarm of impacts or airbursts to have eluded discovery. Petaev et al. (1) also independently known to have taken place, from comets, chondritic, or stony asteroids suggest that the anomaly could be explained and that would have produced Pt-rich fallout: caused an abrupt climate change, continen- by multiple impacts of smaller iron meteor- the Cape York meteorite fall. tal-scale wildfires, mass extinctions, and col- ites, like Sikhote-Alin, a crater-forming clus- lapse of the Clovis culture at or near the ter in 1947 with a total recovered mass of ACKNOWLEDGMENTS. This work was supported in ∼ part by Sandia National Laboratories. Sandia is a multi- Younger Dryas Boundary (YDB). The authors 23 tons (3). A global Pt anomaly would program laboratory operated by Sandia Corporation, a identify a large Pt anomaly in the Green- require on the order of 105 such impacts. Lockheed Martin Company, for the US Department of land Ice Sheet Project 2 (GISP2) core and Widely dispersed impact swarms of this scale Energy, under Contract DE-AC04-94AL85000. suggest that it hints at an extraterrestrial have never been observed and no physical 1 source. Because there is no corresponding model has been proposed for their formation. -
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adustroaliawn conin auctieiosns AUCTION 336 This auction has NO room participation. Live bidding online at: auctions.downies.com AUCTION DATES Monday 18th May 2020 Commencing 9am Tuesday 19th May 2020 Commencing 9am Wednesday 20th May 2020 Commencing 9am Thursday 21st May 2020 Commencing 9am Important Information... Mail bidders Mail Prices realised All absentee bids (mail, fax, email) bids must Downies ACA A provisional Prices Realised list be received in this office by1pm, Friday, PO Box 3131 for Auction 336 will be available at 15th May 2020. We cannot guarantee the Nunawading Vic 3131 www.downies.com/auctions from execution of bids received after this time. Australia noon Friday 22nd May. Invoices and/or goods will be shipped as soon Telephone +61 (0) 3 8677 8800 as practicable after the auction. Delivery of lots Fax +61 (0) 3 8677 8899 will be subject to the receipt of cleared funds. Email [email protected] Website www.downies.com/auctions Bid online: auctions.downies.com 1 WELCOME TO SALE 336 Welcome to Downies Australian Coin Auctions Sale 336! As with so many businesses, and the Australian community in general, the COVID-19 pandemic has presented Downies with many challenges – specifically, in preparing Sale 336. The health and safety of our employees and our clients is paramount, and we have worked very hard to both safeguard the welfare of all and create an auction of which we can be proud. As a consequence, we have had to make unprecedented modifications to the way Sale 336 will be run. For example, the sale will be held without room participation.