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Meteorites, Asteroids, and Comets
Space Sci Rev (2018) 214:36 https://doi.org/10.1007/s11214-018-0474-9 Water Reservoirs in Small Planetary Bodies: Meteorites, Asteroids, and Comets Conel M.O’D. Alexander1 · Kevin D. McKeegan2 · Kathrin Altwegg3 Received: 10 January 2018 / Accepted: 11 January 2018 / Published online: 23 January 2018 © Springer Science+Business Media B.V., part of Springer Nature 2018 Abstract Asteroids and comets are the remnants of the swarm of planetesimals from which the planets ultimately formed, and they retain records of processes that operated prior to and during planet formation. They are also likely the sources of most of the water and other volatiles accreted by Earth. In this review, we discuss the nature and probable origins of asteroids and comets based on data from remote observations, in situ measurements by spacecraft, and laboratory analyses of meteorites derived from asteroids. The asteroidal par- ent bodies of meteorites formed ≤ 4 Ma after Solar System formation while there was still a gas disk present. It seems increasingly likely that the parent bodies of meteorites spectro- scopically linked with the E-, S-, M- and V-type asteroids formed sunward of Jupiter’s orbit, while those associated with C- and, possibly, D-type asteroids formed further out, beyond Jupiter but probably not beyond Saturn’s orbit. Comets formed further from the Sun than any of the meteorite parent bodies, and retain much higher abundances of interstellar mate- rial. CI and CM group meteorites are probably related to the most common C-type asteroids, and based on isotopic evidence they, rather than comets, are the most likely sources of the H and N accreted by the terrestrial planets. -
I-Xe Analysis of Enstatite Meteorites and a Eucrite
Testing an integrated chronology: I-Xe analysis of enstatite meteorites and a eucrite Item Type Article; text Authors Busfield, A.; Turner, G.; Gilmour, J. D. Citation Busfield, A., Turner, G., & Gilmour, J. D. (2008). Testing an integrated chronology: IXe analysis of enstatite meteorites and a eucrite. Meteoritics & Planetary Science, 43(5), 883-897. DOI 10.1111/j.1945-5100.2008.tb01087.x Publisher The Meteoritical Society Journal Meteoritics & Planetary Science Rights Copyright © The Meteoritical Society Download date 26/09/2021 21:32:45 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/656429 Meteoritics & Planetary Science 43, Nr 5, 883–897 (2008) AUTHOR’S PROOF Abstract available online at http://meteoritics.org Testing an integrated chronology: I-Xe analysis of enstatite meteorites and a eucrite A. BUSFIELD, G. TURNER, and J. D. GILMOUR* School of Earth, Atmospheric and Environmental Science, University of Manchester, Oxford Road, Manchester M13 9PL, UK *Corresponding author. E-mail: [email protected] (Supplementary tables and figures are available online at http://meteoritics.org/online supplements.htm) (Received 06 October 2006; revision accepted 21 November 2007) Abstract–We have determined initial 129I/127I ratios for mineral concentrates of four enstatite meteorites and a eucrite. In the case of the enstatite meteorites the inferred ages are associated with the pyroxene-rich separates giving pyroxene closure ages relative to the Shallowater standard of Indarch (EH4, 0.04 ± 0.67 Ma), Khairpur (EL6, −4.22 ± 0.67 Ma), Khor Temiki (aubrite, −0.06 Ma), and Itqiy (enstatite achondrite, −2.6 ± 2.6 Ma), negative ages indicate closure after Shallowater. -
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. -
Bartoschewitz - Catalogue of Meteorites
BARTOSCHEWITZ - CATALOGUE OF METEORITES *FALL TOTAL BC- BC - NAME COUNTRY FIND WEIGHT TYPE No. SPECIMEN WEIGHT (kg) (gms) 1.1 CHONDRITES - ORDINARY OLIVINE BRONZITE CHONDRITES ACFER 005 Algeria March 1989 0,115 H 3.9/4 613.1 cut endpiece 32,70 ACFER 006 Algeria March 1989 0,561 H 3.9/4 614.1 slice 1,30 ACFER 011 Algeria 1989 3,8 H 5 399.1 cut fragm. 3,00 ACFER 020 Algeria 1989 0,708 H 5 401.1 cut fragm. 2,50 ACFER 028 Algeria 1989 3,13 H 3.8 844.1 part slice 1,70 ACFER 050 Algeria 1989 1,394 H 5-6 443.1 complete slice 105,00 ACFER 084 Algeria Apr. 16, 1990 6,3 H 5 618.1 cut corner piece 12,60 ACFER 089 Algeria 1990 0,682 H 5 437.1 complete slice 62,00 ACFER 098 Algeria 1990 5,5 H 5 615.1 cut fragment 29,20 ACFER 222 Algeria 1991 0,334 H 5-6 536.1 cut fragm. with crust 2,50 ACFER 284 Algeria 1991 0,12 H 5 474.1 slice 11,00 ACHILLES USA, Kansas 1924 recogn. 1950 16 H 5 314.1 slice 3,40 ACME USA, New Mexico 1947 75 H 5 303.1 slice 10,80 AGEN France *Sept. 5, 1815 30 H 5 208.1 fragm. with crust 54,40 ALAMOGORDO USA, New Mexico 1938 13,6 H 5 2.1 fragment 0,80 ALLEGAN USA *July 10, 1899 35 H 5 276.0 5 small fragments 1,52 ALLEGAN USA *July 10, 1899 35 H 5 276.1 5 small fragments 1,50 ALLEGAN USA *July 10, 1899 35 H 5 276.2 chondrules 0,02 ALLEN USA, Texas 1923 recogn. -
Meteorite Falls and the Fragmentation of Meteorites Daniel Momeni, Westmont High School, Campbell, CA 95008
Meteorite Falls and the Fragmentation of Meteorites Daniel Momeni Westmont High School, Campbell, CA 95008 In order to understand the fragmentation of objects entering the atmosphere and why some produce more fragments than others, I have searched the Meteoritical Society database for meteorites >20 kg that fell in the USA, China, and India. I also studied the video and film records of 21 fireballs that produced meteorites. A spreadsheet was prepared that noted smell, fireball, explosion, whistling, rumbling, the number of fragments, light, and impact sounds. Falls with large numbers of fragments were examined to look for common traits. These were: The Norton County aubrite, explosion and a flare >100 fragments The Forest City H5 chondrite explosion, a flare, a dust trail 505 specimens. The Richardton H5 chondrite explosion and light 71 specimens. The Juancheng H5 chondrite explosion, a rumbling, a flare, 1000 specimens. a dust trail The Tagish Lake C2 chondrite explosion, flare, dust trail 500 specimens. I conclude that fragmentation is governed by the following: (1) Bigger meteors undergo more stress which results in more specimens; (2) Harder meteorites also require more force to break them up which will cause greater fragmentation; (3) Force and pressure are directly proportional during falls. General observations made were; (1) Meteorites produce fireballs sooner due to high friction; (2) Meteors tend to explode as well because of high stress; (3) Softer meteorites tend to cause dust trails; (4) Some falls produce light as they fall at high velocity. I am grateful to NASA Ames for this opportunity and Derek Sears, Katie Bryson, and Dan Ostrowski for discussions. -
Silicate-Bearing Iron Meteorites and Their Implications for the Evolution Of
Chemie der Erde 74 (2014) 3–48 Contents lists available at ScienceDirect Chemie der Erde j ournal homepage: www.elsevier.de/chemer Invited Review Silicate-bearing iron meteorites and their implications for the evolution of asteroidal parent bodies ∗ Alex Ruzicka Cascadia Meteorite Laboratory, Portland State University, 17 Cramer Hall, 1721 SW Broadway, Portland, OR 97207-0751, United States a r t a b i c s t l r e i n f o a c t Article history: Silicate-bearing iron meteorites differ from other iron meteorites in containing variable amounts of sili- Received 17 July 2013 cates, ranging from minor to stony-iron proportions (∼50%). These irons provide important constraints Accepted 15 October 2013 on the evolution of planetesimals and asteroids, especially with regard to the nature of metal–silicate Editorial handling - Prof. Dr. K. Heide separation and mixing. I present a review and synthesis of available data, including a compilation and interpretation of host metal trace-element compositions, oxygen-isotope compositions, textures, miner- Keywords: alogy, phase chemistries, and bulk compositions of silicate portions, ages of silicate and metal portions, Asteroid differentiation and thermal histories. Case studies for the petrogeneses of igneous silicate lithologies from different Iron meteorites groups are provided. Silicate-bearing irons were formed on multiple parent bodies under different con- Silicate inclusions Collisions ditions. The IAB/IIICD irons have silicates that are mainly chondritic in composition, but include some igneous lithologies, and were derived from a volatile-rich asteroid that underwent small amounts of silicate partial melting but larger amounts of metallic melting. A large proportion of IIE irons contain fractionated alkali-silica-rich inclusions formed as partial melts of chondrite, although other IIE irons have silicates of chondritic composition. -
Meteorites in the Coe College Museum Cedar Rapids, Iowa
Proceedings of the Iowa Academy of Science Volume 35 Annual Issue Article 43 1928 Meteorites in the Coe College Museum Cedar Rapids, Iowa Glenn S. Dillé Let us know how access to this document benefits ouy Copyright ©1928 Iowa Academy of Science, Inc. Follow this and additional works at: https://scholarworks.uni.edu/pias Recommended Citation Dillé, Glenn S. (1928) "Meteorites in the Coe College Museum Cedar Rapids, Iowa," Proceedings of the Iowa Academy of Science, 35(1), 225-232. Available at: https://scholarworks.uni.edu/pias/vol35/iss1/43 This Research is brought to you for free and open access by the Iowa Academy of Science at UNI ScholarWorks. It has been accepted for inclusion in Proceedings of the Iowa Academy of Science by an authorized editor of UNI ScholarWorks. For more information, please contact [email protected]. Dillé: Meteorites in the Coe College Museum Cedar Rapids, Iowa METEORITES IN THE COE COLLEGE MUSEUM CEDAR RAPIDS, row A GLENN s. DILLE There are a number of meteorites in the Coe College }Vfuseum collections, most of which are fragments or individuals of falls recorded from the state of Iowa. A few are from other states. lVIuch of the material is fragmentary, some are entire, others are parts of stony meteorites. The College is indebted to the Iowa Masonic Library at Cedar Rapids for a number of the meteorites. They were in its posses sion when the entire geological collection was given to Coe College. Much credit is clue Mr. Newton R. Parvin, for many years curator of the Library, for his faithful preservation of the meteorites and the data concerning each. -
North American Geology
DEPARTMENT OF THE INTERIOR ALBERT B. FALL, Secretary UNITED STATES GEOLOGICAL SURVEY GEORGE OTIS SMITH, Director 0 Bulletin 731 BIBLIOGRAPHY OF NORTH AMERICAN GEOLOGY FOR 1919-1920 BY JOHN M. NICKLES WASHINGTON GOVERNMENT PRINTING OFFICE 1922 CONTENTS. Page. Introduction ________ ___ ___ 1 Serials examined ___ __ _____ _ _____ _____ __ ____ _ ___ 3 Bibliography _________ _______ _ _______ __ ___ 9 Index _ __ _ _ __i. __ 147 Lists _______ _ ______________ _________________ 241 Chemical analyses _ ____ __ ___ _____ ___ 241 Mineral analyses _ _ ___ _ ____ _ ________ 242 Minerals described __ ____ __ __ _ __________ ___ 242 Rocks described ___ _ ____ __ ___ ____ _ ___ 244 Geologic formations described. ___ __ _ ______ _____ _ __ _ 241 ' BIBLIOGRAPHY 0¥ NORTH AMERICAN GEOLOGY FOB 1919-1920. By JOHN M. NICKLES. INTRODUCTION. The bibliography of North American geology, including paleon tology. petrologj7, and mineralogy, for the years 1919 and 1920 con tains publications on the geology of the Continent of North America and adjacent islands and on Panama and the Hawaiian Islands. It includes textbooks and papers of general character by American au thors, .but not those by foreign authors, except papers that appear in American publications. The papers, with full title and medium of publication and explana tory note if the title is not fully self-explanatory, are listed under the names of their authors, which are arranged in alphabetic order. The author list is followed by an index to the literature listed. The bibliography of North American geology is comprised in the following bulletins of the United States Geological Survey: No. -
Abstracts 5002-5050.Fm
Meteoritics & Planetary Science 38, Nr 7, Supplement, A9–A153 (2003) http://meteoritics.org Abstracts POTENTIAL NEW IMPACT SITES IN PATAGONIA, ARGENTINA, SPIN DYNAMICS OF TERRESTRIAL PLANETS FROM EARTH- SOUTH AMERICA BASED RSDI M. C. L. Rocca. Mendoza 2779–16A, Ciudad de Buenos Aires, Argentina, I. V. Holin. Space Research Institute, Moscow, Russia. E-mail: (1428DKU). E-mail: [email protected] [email protected] Introduction: The southern part of Argentina has a total surface of Introduction: Despite wide Earth-based observations and many 786,112 km2. It is composed of five provinces: Neuquen, Rio Negro, Chubut, spacecraft missions, much remains unknown in spin dynamics of terrestrial Santa Cruz, and Tierra del Fuego. So far, no impact sites have been reported planets and related issues. Through accurate measurement of spin vectors and in this region. As part of an ongoing project to discover meteorite impact their variations with time, we may look deeply into planetary interiors. It has sites, this area was investigated through examination of 76 color LANDSAT not been possible to do so with known Earth-based techniques and spacecraft satellite images (1:250,000; resolution = 250 m) at the Instituto Geografico missions have been the only way to obtain such data. The upcoming Militar (IGM) (Military Geographic Institute) of Buenos Aires. When a Messenger (USA) and BepiColombo (Europe, Japan) orbiting and orbiting/ potential candidate was found, a more detailed study of images was done. landing missions should give obliquity and librations of Mercury closely LANDSAT color images at the scale of 1:100,000 and aerial photographs at related with its internal constitution [1]. -
Enstatite Chondrites EL3 As Building Blocks for the Earth: the Debate 1 Over the 146 Sm-142 Nd Systematics Maud Boyet, A
Enstatite chondrites EL3 as building blocks for the Earth: the debate 1 over the 146 Sm-142 Nd systematics Maud Boyet, A. Bouvier, P. Frossard, Tahar Hammouda, M. Garçon, Abdelmouhcine Gannoun To cite this version: Maud Boyet, A. Bouvier, P. Frossard, Tahar Hammouda, M. Garçon, et al.. Enstatite chondrites EL3 as building blocks for the Earth: the debate 1 over the 146 Sm-142 Nd systematics. Earth and Planetary Science Letters, Elsevier, 2018, 488, pp.68-78. 10.1016/j.epsl.2018.02.004. hal-01723716 HAL Id: hal-01723716 https://hal.uca.fr/hal-01723716 Submitted on 5 Mar 2018 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. 1 Enstatite chondrites EL3 as building blocks for the Earth: the debate 2 over the 146Sm-142Nd systematics 3 4 M. Boyet1, A. Bouvier2, P. Frossard1, T. Hammouda1, M. Garçon3, A. Gannoun1 5 1 Laboratoire Magmas et Volcans, Université Clermont Auvergne, France 6 2 Department of Earth Sciences, Centre for Planetary Science and Exploration, 7 University of Western Ontario, London, Canada 8 3 Department of Earth Sciences, ETH Zurich, Switzerland 9 10 Earth and Planetary Science Letters 488 (2018) 68–78 11 12 13 Keywords: 146Sm-142Nd systematics, enstatite chondrites, Earth’s evolution, Earth’s 14 building blocks 15 16 Abstract 17 The 146Sm-142Nd extinct decay scheme (146Sm half-life of 103 My) is a powerful tool 18 to trace early Earth silicate differentiation. -
Cosette Gilmour
Economic significance of platinum group elements and water in asteroids: Insights from chondritic meteorites by Cosette Gilmour A thesis submitted in partial fulfillment of the requirements for the degree of Master of Science Department of Earth and Atmospheric Sciences University of Alberta © Cosette Gilmour, 2017 Abstract Asteroids are considered to be rich sources of precious metals, water, and essential volatiles for life. Such a consideration has been derived from the study of meteorites and asteroid reflectance spectra which have both been vital to our understanding of asteroid compositions. The vast amount of valuable resources in asteroids that are in close proximity to Earth (Near-Earth Asteroids; NEAs) has designated such asteroids as prime targets for extra- terrestrial mining. Of the resources that can be extracted from asteroids, the platinum group elements (PGEs) and water are two of the most sought-after materials. The PGEs are highly valuable given their rarity on Earth, while having an available water source in space can help facilitate future space exploration (i.e., rocket fuel, radiation shielding, drinking water, etc.). Before mining of these resources can commence, asteroid miners must develop a detailed understanding of how the different compositions of asteroids can affect the distribution of such resources. Since it is an expensive endeavor to visit asteroids for such an assessment, meteorite studies take precedence in obtaining the necessary information for selecting an asteroid target to mine. The premise of this master’s thesis is to provide insight into the PGE and water resources that can be mined from asteroids through the study of chondritic meteorites.