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The Villalbeto De La Peña Meteorite Fall: II. Determination of Atmospheric Trajectory and Orbit
Meteoritics & Planetary Science 41, Nr 4, 505–517 (2006) Abstract available online at http://meteoritics.org The Villalbeto de la Peña meteorite fall: II. Determination of atmospheric trajectory and orbit Josep M. TRIGO-RODRÍGUEZ1, 2*, JiÚí BOROVIª.$3, Pavel SPURNÝ3, José L. ORTIZ4, José A. DOCOBO5, Alberto J. CASTRO-TIRADO4, and Jordi LLORCA2, 6 1Institut de Ciències de l’Espai (ICE-CSIC), Campus UAB, Facultat de Ciències, Torre C-5, parells, 2a planta, 08193 Bellaterra (Barcelona), Spain 2Institut d’Estudis Espacials de Catalunya (IEEC), Ed. Nexus, Gran Capità 2-4, 08034 Barcelona, Spain 3Astronomical Institute of the Academy of Sciences, OndÚHMRY2EVHUYDWRU\&]HFK5HSXEOLF 4Instituto de Astrofísica de Andalucía (IAA-CSIC), P.O. Box 3004, 18080 Granada, Spain 5Observatorio Astronómico Ramón Maria Aller, Universidade de Santiago de Compostela, Spain 6Institut de Tècniques Energètiques, Universitat Politècnica de Catalunya, Diagonal 647, 08028 Barcelona, Spain *Corresponding author. E-mail: [email protected] (Received 23 April 2005; revision accepted 3 November 2005) Abstract–The L6 ordinary chondrite Villalbeto de la Peña fall occurred on January 4, 2004, at 16:46: 45 r 2 s UTC. The related daylight fireball was witnessed by thousands of people from Spain, Portugal, and southern France, and was also photographed and videotaped from different locations of León and Palencia provinces in Spain. From accurate astrometric calibrations of these records, we have determined the atmospheric trajectory of the meteoroid. The initial fireball velocity, calculated from measurements of 86 video frames, was 16.9 r 0.4 km/s. The slope of the trajectory was 29.0 r 0.6° to the horizontal, the recorded velocity during the main fragmentation at a height of 27.9 r 0.4 km was 14.2 r 0.2 km/s, and the fireball terminal height was 22.2 r 0.2 km. -
Directions from Las Vegas to Hollywood California
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Arizona Rural Transit Needs Study May 2008
Arizona Rural Transit Needs Study May 2008 Final Report prepared for Arizona Department of Transportation prepared by Cambridge Systematics, Inc. in association with TranSystems Corporation www.camsys.com Arizona Rural Transit Needs Study Table of Contents Executive Summary ..................................................................................................ES-1 Study Baseline Report ...................................................................................... ES-1 Future Trend Analysis ..................................................................................... ES-3 Transit Demand and Need .............................................................................. ES-4 Funding Issues and Solutions ......................................................................... ES-9 Vision, Goals, and Objectives........................................................................ ES-10 Service Alternatives and Solutions............................................................... ES-11 Supporting Policies and Practices ................................................................ ES-15 Summary.......................................................................................................... ES-16 1.0 Introduction .........................................................................................................1-1 2.0 Vision, Goals, and Objectives ..........................................................................2-1 2.1 Vision............................................................................................................2-1 -
Transportation and Arizona
APRIL 2015 - ARIZONA TOWN HALL TRANSPORTATION & ARIZONA 2014-2015 ARIZONA TOWN HALL OFFICERS, BOARD OF DIRECTORS, COMMITTEE CHAIRS, AND STAFF EXECUTIVE COMMITTEE OFFICERS The Officers and the following: J. Scott Rhodes Cathy Weiss Arlan Colton EX OFFICIO Board Chair Secretary Trinity Donovan Ron Walker Linda Elliott-Nelson Mark Nexsen James Jayne Board Chair Elect Treasurer Frances Mclane Merryman Steven Betts Richard Morrison Vice Chair Alberto Olivas BOARD OF DIRECTORS Steven A. Betts Linda J. Elliott-Nelson John C. Maynard Sandra L. Smith President, Chanen Development Dean of Instruction, Arizona Supervisor, Santa Cruz President and CEO, Pinal Company, Inc., Phoenix Western College, Yuma County, Nogales Partnership; Fmr. Member, Brian Bickel Julie Engel Patrick McWhortor Pinal County Board of Ret. CEO, Southeast Arizona President & CEO, Greater Yuma President & CEO, Alliance of Supervisors, Apache Junction Medical Center, Douglas Economic Development, Yuma Arizona Nonprofits, Phoenix Ken L. Strobeck Sandra Bierman Catherine M. Foley Frances McLane Merryman Executive Director, League of Director of Legal Services, Blue Cross Executive Director, Arizona Vice President & Senior Arizona Cities & Towns, Phoenix Blue Shield of Arizona, Phoenix Citizens for the Arts, Phoenix Wealth Strategist, Northern Michael Stull Kerry Blume Jennifer Frownfelter Trust Company, Tucson Manager, Public & Consultant, Flagstaff Vice President, URS Richard N. Morrison Government Relations, Cox Richard M. Bowen Corporation, Phoenix Attorney, Salmon, Lewis & Communications, Phoenix Associate Vice President, Economic Richard E. Gordon Weldon, PLC, Gilbert W. Vincent Thelander III Development and Sustainability, Pima County Superior Court Robyn Nebrich Vice President & Senior Client Northern Arizona University Juvenile Judge, Tucson Assistant Development Director, Manager, Bank of America, Phoenix Sheila R. -
Radar-Enabled Recovery of the Sutter's Mill Meteorite, A
RESEARCH ARTICLES the area (2). One meteorite fell at Sutter’sMill (SM), the gold discovery site that initiated the California Gold Rush. Two months after the fall, Radar-Enabled Recovery of the Sutter’s SM find numbers were assigned to the 77 me- teorites listed in table S3 (3), with a total mass of 943 g. The biggest meteorite is 205 g. Mill Meteorite, a Carbonaceous This is a tiny fraction of the pre-atmospheric mass, based on the kinetic energy derived from Chondrite Regolith Breccia infrasound records. Eyewitnesses reported hearing aloudboomfollowedbyadeeprumble.Infra- Peter Jenniskens,1,2* Marc D. Fries,3 Qing-Zhu Yin,4 Michael Zolensky,5 Alexander N. Krot,6 sound signals (table S2A) at stations I57US and 2 2 7 8 8,9 Scott A. Sandford, Derek Sears, Robert Beauford, Denton S. Ebel, Jon M. Friedrich, I56US of the International Monitoring System 6 4 4 10 Kazuhide Nagashima, Josh Wimpenny, Akane Yamakawa, Kunihiko Nishiizumi, (4), located ~770 and ~1080 km from the source, 11 12 10 13 Yasunori Hamajima, Marc W. Caffee, Kees C. Welten, Matthias Laubenstein, are consistent with stratospherically ducted ar- 14,15 14 14,15 16 Andrew M. Davis, Steven B. Simon, Philipp R. Heck, Edward D. Young, rivals (5). The combined average periods of all 17 18 18 19 20 Issaku E. Kohl, Mark H. Thiemens, Morgan H. Nunn, Takashi Mikouchi, Kenji Hagiya, phase-aligned stacked waveforms at each station 21 22 22 22 23 Kazumasa Ohsumi, Thomas A. Cahill, Jonathan A. Lawton, David Barnes, Andrew Steele, of 7.6 s correspond to a mean source energy of 24 4 24 2 25 Pierre Rochette, Kenneth L. -
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. -
Identification of Meteorite Source Regions in the Solar System
Icarus 311 (2018) 271–287 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Identification of meteorite source regions in the Solar System ∗ Mikael Granvik a,b, , Peter Brown c,d a Department of Physics, P.O. Box 64, 0 0 014 University of Helsinki, Finland b Department of Computer Science, Electrical and Space Engineering, Luleå University of Technology, Kiruna, Box 848, S-98128, Sweden c Department of Physics and Astronomy, University of Western Ontario, London N6A 3K7, Canada d Centre for Planetary Science and Exploration, University of Western Ontario, London N6A 5B7, Canada a r t i c l e i n f o a b s t r a c t Article history: Over the past decade there has been a large increase in the number of automated camera networks that Received 27 January 2018 monitor the sky for fireballs. One of the goals of these networks is to provide the necessary information Revised 6 April 2018 for linking meteorites to their pre-impact, heliocentric orbits and ultimately to their source regions in the Accepted 13 April 2018 solar system. We re-compute heliocentric orbits for the 25 meteorite falls published to date from original Available online 14 April 2018 data sources. Using these orbits, we constrain their most likely escape routes from the main asteroid belt Keywords: and the cometary region by utilizing a state-of-the-art orbit model of the near-Earth-object population, Meteorites which includes a size-dependence in delivery efficiency. While we find that our general results for escape Meteors routes are comparable to previous work, the role of trajectory measurement uncertainty in escape-route Asteroids identification is explored for the first time. -
Milley 2010.Pdf (10.17Mb)
University of Calgary PRISM: University of Calgary's Digital Repository Graduate Studies Legacy Theses 2010 Physical Properties of Fireball-Producing Earth-Impacting Meteoroids and Orbit Determination through Shadow Calibration of the Buzzard Coulee Meteorite Fall Milley, Ellen Palesa Milley, E. P. (2010). Physical Properties of Fireball-Producing Earth-Impacting Meteoroids and Orbit Determination through Shadow Calibration of the Buzzard Coulee Meteorite Fall (Unpublished master's thesis). University of Calgary, Calgary, AB. doi:10.11575/PRISM/17766 http://hdl.handle.net/1880/47937 master thesis University of Calgary graduate students retain copyright ownership and moral rights for their thesis. You may use this material in any way that is permitted by the Copyright Act or through licensing that has been assigned to the document. For uses that are not allowable under copyright legislation or licensing, you are required to seek permission. Downloaded from PRISM: https://prism.ucalgary.ca UNIVERSITY OF CALGARY Physical Properties of Fireball-Producing Earth-Impacting Meteoroids and Orbit Determination through Shadow Calibration of the Buzzard Coulee Meteorite Fall by Ellen Palesa Milley A THESIS SUBMITTED TO THE FACULTY OF GRADUATE STUDIES IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF SCIENCE DEPARTMENT OF GEOSCIENCE CALGARY, ALBERTA April, 2010 ©c Ellen Palesa Milley 2010 The author of this thesis has granted the University of Calgary a non-exclusive license to reproduce and distribute copies of this thesis to users of the University of Calgary Archives. Copyright remains with the author. Theses and dissertations available in the University of Calgary Institutional Repository are solely for the purpose of private study and research. -
Greyhound Tickets to Las Vegas
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Tufesa Bus Tickets Phoenix
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Lev A. Muravyev , Viktor I. Grokhovsky
The Chrono List of Bad Meteorites Harmful № Date Name Place Type Fall Description Source 1Ural Federal University, specimen 1,2 Lombardia, Doubtful 2 1 04.09.1511 Crema shwr several killed birds, sheep, and a man (dbt) [3, 7] Lev A. Muravyev , Institute of Geophysics Ural Branch of RAS, Italy meteorite Doubtful 2 04.09.1654 Milan Italy {?} - killed a monk (dbt) [3, 7] 1 Ekaterinburg, Russia; meteorite Aquitaine, crushed cottage, killed farmer and Viktor I. Grokhovsky 3 24.07.1790 Barbotan H5 shwr - [1, 10] [email protected], [email protected] France some cattle (dbt) Uttar Pradesh, [7, 9, Abstract. The problem of the asteroid-comet hazard is now being 4 19.12.1798 Benares (a) LL4 shwr 0,9 kg building India 10] actively discussed, because the consequences of the fall of large cosmic Bayern, 5 13.12.1803 Mässing Howardite U - building struck [1, 10] bodies on the earth can be catastrophic and affect the survival of Germany humanity and all living things. Fragments of smaller celestial bodies - Moscow, 6 05.09.1812 Borodino H5 U 0,5 kg observed by a soldier on guard [7] meteorites, fall to the earth much more often, and they can also emanate Russia a certain danger. In several papers that were published about 20 years Rajasthan, Doubtful killed a men and injured a women 7 16.01.1825 Oriang {?} - [3, 7] ago, attempts were made to compile a list of events related to the India meteorite (dbt) Uttar Pradesh, [3, 7, 9, damage caused by meteorites falling from the sky. -
The Fall of the Peekskill Meteorite: Video Observations, Atmospheric
The Fall of the Peekskill Meteorite: Video Observaüons, Atmospheric Path, Fragmentation Record and Orbit. M. Beech 1, P. Brown 2, R. L. Hawkes3, Z. Ceplecha4, K. Mossman3, and G. Wetherill5. 1 Astronomy Department, The University of Western Ontario, London, Ontario, Canada. 2 Physics Department, The University of Western Ontario, London, Ontario, Canada. 3 Department of Physics, Engineering and Geology, Mount Allison University, Sackville, New Brunswick, Canada. 40ndrejov Observatory, Astronomieal Institute of the Academy of Sciences of the Czech Republic, Ondrejov, Czech Republic. 5 Camegie lnsütute of Washington, Department of Terrestrial Magneüsm, 5241 Broad Branch Road, Washington, D. C., U.S.A. Abstract A general overview of the events surrounding the fall of the Peekskill meteorite is presented. Earth, Moon, and Planets 68: 189-197, 1995. © 1995 Kluwer Academic Publlshers. Printed in the Netherlands. 190 1. Introduetion: The events surrounding the fall of the Peekskill meteorite on October 9th, 1992 are quite remarkable. Not only did the meteorite announce its arrival by hitting a parked car in suburban Peekskill, N.Y., but the fireball that preceded the fall of the meteorite was videographed by at least 16 independent videographers. Eye-witness accounts indicate that the fireball associated with the Peekskill meteodte first appeared over West Virginia at 23:48 UT (±1 min.). The fireball, which traveled in an approximately northeasterly direction, had a pronounced greenish colour, and attained an estimated peak visual magnitude of -13 (comparable to the Full Moon). During a luminous flight time that exceeded 40 seconds the fireball covered a ground path of some 700 to 800 km (Brown et al., 1994).