Handbook of Iron Meteorites, Volume 2 (Braunau
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Tardi-Magmatic Precipitation of Martian Fe/Mg-Rich Clay Minerals Via Igneous Differentiation
©2020TheAuthors Published by the European Association of Geochemistry ▪ Tardi-magmatic precipitation of Martian Fe/Mg-rich clay minerals via igneous differentiation J.-C. Viennet1*, S. Bernard1, C. Le Guillou2, V. Sautter1, P. Schmitt-Kopplin3, O. Beyssac1, S. Pont1, B. Zanda1, R. Hewins1, L. Remusat1 Abstract doi: 10.7185/geochemlet.2023 Mars is seen as a basalt covered world that has been extensively altered through hydrothermal or near surface water-rock interactions. As a result, all the Fe/Mg-rich clay minerals detected from orbit so far have been interpreted as secondary, i.e. as products of aqueous alteration of pre-existing silicates by (sub)surface water. Based on the fine scale petrographic study of the evolved mesostasis of the Nakhla mete- orite, we report here the presence of primary Fe/Mg-rich clay minerals that directly precipitated from a water-rich fluid exsolved from the Cl-rich parental melt of nakhlites during igneous differentiation. Such a tardi-magmatic precipitation of clay minerals requires much lower amounts of water compared to production via aque- ous alteration. Although primary Fe/Mg-rich clay minerals are minor phases in Nakhla, the contribution of such a process to Martian clay formation may have been quite significant during the Noachian given that Noachian magmas were richer in H2O. In any case, the present discovery justifies a re-evaluation of the exact origin of the clay minerals detected on Mars so far, with potential consequences for our vision of the early magmatic and climatic histories of Mars. Received 26 January 2020 | Accepted 27 May 2020 | Published 8 July 2020 Letter mafic crustal materials (Smith and Bandfield, 2012; Ehlmann and Edwards, 2014). -
New Mars Meteorite Fall in Marocco: Final Strewn Field
Available online at www.ilcpa.pl International Letters of Chemistry, Physics and Astronomy 11 (2013) 20-25 ISSN 2299-3843 New Mars meteorite fall in Marocco: final strewn field Abderrahmane Ibhi Laboratory of Geo-heritage and Geo-materials Science, Ibn Zohr University, Agadir, Morocco E-mail address: [email protected] ABSTRACT The Tissint fireball is the only fireball to have been observed and reported by numerous witnesses across the south-east of Morocco. The event was extremely valuable to the scientific community; show an extraordinary and rare event and were also the brightest and most comprehensively observed fireball in Morocco’s known astronomical history. Since the abstract of A. Ibhi (2011) [1]. In 1012-2013 concerning a number of Martian meteorite fragments found in the region of Tata (Morocco), a number of expeditions have been made to the area. A. ibhi has done a great amount of field work. He discovered the strewn field and collected the fragments of this Martian meteorite and many information. Each expedition has had the effect of expanding the size of the strewn field which is now documented to cover more than 70 sq. kilometers. The size of the strewn field is now estimated to be about a 17 km long. Keywords: fireball; Martian meteorite; Shergottite; Strewn field; Tissint; Morocco. 1. INTRODUCTION A meteoritic body entered the earth’s atmosphere in the south-east skies of Tata, Morocco, On Sunday July, 18th, 2011 at 2 o’clock in the morning. Its interaction with the atmosphere led to brilliant light flashes accompanied with detonations. -
An Evaluation of the Palladium-Silver Isotope Systematics in the Oldest Differentiated Planetesimal: Beyond Shock
43rd Lunar and Planetary Science Conference (2012) 1116.pdf AN EVALUATION OF THE PALLADIUM-SILVER ISOTOPE SYSTEMATICS IN THE OLDEST DIFFERENTIATED PLANETESIMAL: BEYOND SHOCK. M.F. Horan1, R.W. Carlson1,and J. Blichert-Toft2 Department of Terrestrial Magnetism, Carnegie Institution of Washington (5241 Broad Branch Road NW, Washing- ton DC 20015. [email protected]), 2Ecole Normale Supérieure de Lyon, Université Claude Bernard Lyon 1 and CNRS (69007 Lyon, France). Introduction: Troilite from Muonionalusta (iron Troilite from slab 1 contained 5.612 ng/g Ag with meteorite group IVA) gives the oldest absolute age yet 107Ag/109Ag of 1.127±0.002, and 0.780±0.002 ng/g Pd, measured for a differentiated planetesimal corresponding to 108Pd/109Ag of 0.05946 ±0.00010. (4565.3±0.1 Ma) which suggests that the IVA parent HCl-insoluble inclusions (probably schreibersite) with- body accreted, differentiated, and cooled within 2-3 in this troilite yielded 1.758±0.006 ng/g Ag with Ma after CAI formation [1]. The aim of this study is to 107Ag/109Ag of 1.130±0.002, and 5168±10 ng/g Pd, use the quick evolution and volatile-depleted (high corresponding to 108Pd/109Ag of 1691±8. Troilite from Pd/Ag) composition of IVA irons to better constrain slab 2 contained 11.75±0.04 ng/g Ag and had a the initial Solar System abundance of 107Pd ( 107Pd 107Ag/109Ag ratio of 1.0833±0.0004 [6]. The Pd con- 107 Ag with t1/2 = 6.5 Ma). Most Pd/Ag ages have been centration was 0.291±0.1 ng/g corresponding to referenced to 107Pd/108Pd = (2.40±0.05) x 10-5 obtained 108Pd/109Ag of 13.9±0.1. -
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, -
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. -
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. -
Can Mars' Current Atmosphere Land Block Island Sized Meteorites?
41st Lunar and Planetary Science Conference (2010) 2351.pdf CAN MARS’ CURRENT ATMOSPHERE LAND BLOCK ISLAND SIZED METEORITES? J.E.Chappelow1 and M.P. Golombek2, 1SAGA Inc., 1148 Sundance Loop, Fairbanks, AK 99709 (john.chap- [email protected]), 2Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109. Introduction: In 2005-6 Chappelow and Sharpton mass and vf is the final velocity, were used to sort the showed that iron meteorites up to a few kg in mass BI meteorite outcomes out of the results. should be expected on Mars [1,2] and that even irons Results: We found that Mars’ current atmosphere the mass of Heat Shield Rock (hereafter HSR, also can decelerate iron meteoroids as large as Block Is- named Meridiani Planum) (50 – 60 kg) could be land below 2 km/s, but only if they start with very spe- landed, even under as low-density a martian atmo- cific masses, speeds, and (especially) entry angles. All sphere as the one that exists today, though only rarely. of the positive results for BI that were found followed They would have to encounter the planet within nar- the type 3 flight path shown on Fig. 1 (termed “fall- row limits of initial mass, entry velocity, and entry back” trajectories in the caption). On this type of tra- angle [3] to have their velocity reduced sufficiently be- jectory, the meteoroid enters the atmosphere, initially low hypervelocity impact speeds (< 2 km/s) to land a descends, but then ascends briefly as the planet curves meteorite as opposed to forming a primary crater and away beneath it, before finally slowing and redescend- being destroyed or severely deformed. -
N Arieuican%Mllsellm
n ARieuican%Mllsellm PUBLISHED BY THE AMERICAN MUSEUM OF NATURAL HISTORY CENTRAL PARK WEST AT 79TH STREET, NEW YORK 24, N.Y. NUMBER 2I63 DECEMBER I9, I963 The Pallasites BY BRIAN MASON' INTRODUCTION The pallasites are a comparatively rare type of meteorite, but are remarkable in several respects. Historically, it was a pallasite for which an extraterrestrial origin was first postulated because of its unique compositional and structural features. The Krasnoyarsk pallasite was discovered in 1749 about 150 miles south of Krasnoyarsk, and seen by P. S. Pallas in 1772, who recognized these unique features and arranged for its removal to the Academy of Sciences in St. Petersburg. Chladni (1794) examined it and concluded it must have come from beyond the earth, at a time when the scientific community did not accept the reality of stones falling from the sky. Compositionally, the combination of olivine and nickel-iron in subequal amounts clearly distinguishes the pallasites from all other groups of meteorites, and the remarkable juxtaposition of a comparatively light silicate mineral and heavy metal poses a nice problem of origin. Several theories of the internal structure of the earth have postulated the presence of a pallasitic layer to account for the geophysical data. No apology is therefore required for an attempt to provide a comprehensive account of this remarkable group of meteorites. Some 40 pallasites are known, of which only two, Marjalahti and Zaisho, were seen to fall (table 1). Of these, some may be portions of a single meteorite. It has been suggested that the pallasite found in Indian mounds at Anderson, Ohio, may be fragments of the Brenham meteorite, I Chairman, Department of Mineralogy, the American Museum of Natural History. -
The Tennessee Meteorite Impact Sites and Changing Perspectives on Impact Cratering
UNIVERSITY OF SOUTHERN QUEENSLAND THE TENNESSEE METEORITE IMPACT SITES AND CHANGING PERSPECTIVES ON IMPACT CRATERING A dissertation submitted by Janaruth Harling Ford B.A. Cum Laude (Vanderbilt University), M. Astron. (University of Western Sydney) For the award of Doctor of Philosophy 2015 ABSTRACT Terrestrial impact structures offer astronomers and geologists opportunities to study the impact cratering process. Tennessee has four structures of interest. Information gained over the last century and a half concerning these sites is scattered throughout astronomical, geological and other specialized scientific journals, books, and literature, some of which are elusive. Gathering and compiling this widely- spread information into one historical document benefits the scientific community in general. The Wells Creek Structure is a proven impact site, and has been referred to as the ‘syntype’ cryptoexplosion structure for the United State. It was the first impact structure in the United States in which shatter cones were identified and was probably the subject of the first detailed geological report on a cryptoexplosive structure in the United States. The Wells Creek Structure displays bilateral symmetry, and three smaller ‘craters’ lie to the north of the main Wells Creek structure along its axis of symmetry. The question remains as to whether or not these structures have a common origin with the Wells Creek structure. The Flynn Creek Structure, another proven impact site, was first mentioned as a site of disturbance in Safford’s 1869 report on the geology of Tennessee. It has been noted as the terrestrial feature that bears the closest resemblance to a typical lunar crater, even though it is the probable result of a shallow marine impact. -
Investigate the History of the Solar System
ARTHUR ROSS HALL OF METEORITES Grades 9-12 Investigate the History of the Solar System Overview Correlations to Standards Students will learn about meteorites and how scientists use these space rocks NY ES4 1.2C: Our solar system formed to investigate how the solar system formed and evolved. about five billion years ago from a giant cloud of gas and debris. Gravity caused • Before Your Visit: Students will complete a formative assessment probe, Earth and other planets to become and read and discuss a text about how and why scientists study meteorites. layered according to density differences in their materials. • During Your Visit: In the Arthur Ross Hall of Meteorites, students will observe meteorite samples to uncover the story of the formation and evolution of the solar system. Then, in the Gottesman Hall of Planet Earth, students will learn more about the formation of the Earth-Moon system, and search for impact craters on Earth and the Moon. • Back in the Classroom: Students will produce an illustrated text that describes the history of the solar system and explains how meteorites help scientists uncover this history. Background for Educators Meteorites are space debris that has fallen to Earth. They’re called meteoroids when still in deep space, meteors (or “shooting stars”) when falling through the atmosphere, and meteorites after they land on Earth. Meteorites range in size from microscopic to kilometers in diameter. They all originate inside our solar system. Most are fragments of small rocky and metallic bodies that broke apart long ago and orbit the Sun in the asteroid belt between Mars and Jupiter. -
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.