THE GEOLOGIC CLASSIFICATIGK of the METEORITES By

Total Page:16

File Type:pdf, Size:1020Kb

THE GEOLOGIC CLASSIFICATIGK of the METEORITES By The geologic classification of the meteorites Item Type text; Dissertation-Reproduction (electronic) Authors Elston, Donald Parker, 1926- Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 10/10/2021 10:53:49 Link to Item http://hdl.handle.net/10150/565179 THE GEOLOGIC CLASSIFICATIGK OF THE METEORITES by.. : Donald Parker Elston ■ A Dissertation'' Submitted to the Faculty of th DEPARTMENT OF GEOLOGY In Partial Fulfillment of the Requirements For the Degree of . / .. ■ Doctor of Philosophy ; • - 'In the Graduate College ' : THE UNIVERSITY OF ARIZONA THE UNIVERSITY OF ARIZONA GRADUATE COLLEGE I hereby recommend that this dissertation prepared under my direction by Donald P. Elston______________________________ entitled The Geologic Classification of the Meteorites be accepted as fulfilling the dissertation requirement of the degree of _______Doctor of Philosophy______________________ C-'.Cc O-l sertation Director Date i- After inspection of the final copy of the dissertation, the following members of the Final Examination Committee concur in its approval and recommend its acceptance:* s,\x\ 1 V This approval and acceptance is contingent on the candidate's adequate performance and defense of this dissertation at the final oral examination. The inclusion of this sheet bound into the library copy of the dissertation is evidence of satisfactory performance at the final examination. statement by author This dissertation has been submitted in partial fulfillment of requirements for an advanced degree at The University of Arizona and is deposited in the University Library to be made available for bor­ rowers under rules of the Library. Brief quotations from this dissertation are allowable.without ' special permission, provided that accurate acknowledgment of source is made. Requests for permission for extended quotation from or re­ production of this manuscript in whole or in part may be granted by the head of the major department or the Dean of the Graduate College when in his.judgment the proposed use of the material is in the in- ■ terests of scholarship. In all other, instances, however, permission must be obtained from the author. Murray carbonaceous chondrite; Specimen Ho. 635.1? 32.7 g? Arizona State University Meteorite Collection, Tempe, Arizona. Murray carbonaceous chondrite ' : ACKNOWIEDGMSKTS The opportunity to study meteorites was made possible through support provided by the Training Act of the United. States Geological Survey, Besuits presented here summarize dissertation work at the University of Arizona, Tucson, undertaken in partial fulfillment of requirements for the PhD degree in. geology, . 1 wish to acknowledge the support of the faculty of the Geology Department of the University of Arizona, in particular Professor Spencer R. Titley,, faculty and disser­ tation advisor, and Professors Paul E,. Damon,. Robert L. DuEois, John M,' Guilbert, and Evans B, Mayo. The work was made possible by the existence of excellent meteor ite collections at Arizona;State University, Tempe, and at the University of Arizona.,. X wish to thank Professor CarletonB. Moore, Director of Research, Center for Meteorite Studies at Arizona State . University, for the extended loan of several meteorites, for numerous fruitful discussions and manuscript review, and for bringing to my attention unpublished data of his that led to correlations of the hypersthene and bronzite chondrites with the Ga-Ge II and III group irons, respectively. I also wish to acknowledge and thank Dr. Michael B. Duke, Uo S. Geological Survey, for making available thin sections of a number of pyroxene-plagioclase 'achondrites, and for his review of an : early version of this manuscript. Much of. the photographic work was done by Mr, B. D. Lindsay, Jr The.preparation of figures and tables was carried out at facilities at the Center of Astrogeology, U. S. Geological Survey, Flagstaff? Arizona. Thanks are extended to the staff of the Water Resources Division Office of the U. S. Geological-Survey, Tucson, for providing office space and administrative support. ' , ' The meticuluous work of Geoffrey P. Elston, who painstakingly measured amd catalogued map data that led to plots of the size-frequency distribution of materials in the Murray carbonaceous chondrite, is ; gratefully acknowledged. The wholehearted and unselfish support of my wife5 Shirley, is directly responsible for the existence of this manuscript. TABES OF COBTEETS ' . y : . ; . ; ; ; ' Page;: HST OF JLmSTRATIOHS = „ « . 0 0 . 0 . / . , =: o. ,o: ix III S3? OF TABLES, o o o o © o© © © © ©© © © © © ©, © © © © © © © © © xxx ABSxBAOT © © © 0 0 0 ©. © © © o 0 0 © © © o o 0 0 .© © © . 0 0 © © © © 5cx'V* I© Il^ITRODUCTION © © © © © ■ © © © © © © © © © © © © © © © © © © © © 3- : . 2o-. : THE METEOEITE. CLASSES', > . = . „ = . .. « „ . 4 Descriptive Classification ' „ * „ .• *• » . « , » » » 4 Proposed Genetic Classification .. »• . „ « . » „ - s , » . 5 . ' 3.. EVIDENCE FOR GEEETIC GROUPINGS . v . \ . „ . 0 0 0 0 . » . 9 Compositional and Mineralogical Characteristics . „ , . « 9 Chemical Compositions o o o p 0 0 0 0 o 0-0 © - o © © © © 9 . Distrihution of Elements '© ©: © » © ,© © © . © © © © © © - 10 Individuality of the Chondrite Classes © © © © © © © . 16 Correlations "between Chondrites and Achondrites © © © © 20 Petrologic Evidence for the Metamorphism.of Chondrites © © 23 Chemical-petrologic Classification of the Chondrites © ©•© © © © © © © © © © © © © © © © © 23 Mineralogic-petrologic Classification of the. •’ Calcium-poor Stony Meteorites © © © © .©'. „ © .’ © © 26 Correlation of Irons and Pallasites with Chondrites © © © ,. 30 "Ga-Ge Groups © © © © © .© © © © © © © © © © © © © © © © 30 Correlations with the Chondrites © © © © © © © © » Y .© 36 . Summary © © © © © © © © © © © © © © © © © © © © © © © © © © 4l 4© CHOEDEITES, THE FIRST ROCKS © © © © © © © © © © © © © © b .. © » 42 :: : Murray Carbonaceous Chondrite © © © © © © © © © © © © © © © 43 \ : Circumstances of Fall © © © © © © © © ©. © © © © © © © © 43 . General Characteristics © © © © © © © © ,©©©»«©» . 44 Paragenetic and Textural Studies © .©; © © © » © © . © © 48 Recognition of Components ls 29 and 3 in other . ChondripeS © © © © © © © © © © .© © © © © © © © © © © ^6 ■ Chondrule Formation and Chondrite Accretion © © © © © © © © 84 Aggregation of Solids © © © © © 84 Inferred Character of Early Solar System © © © ©. © - © © © © 86 vii TABLE OF COIfTEjNTS--Continued Page Possible Enrichment of Volatile Elements in Inner Part of Component 1 Dust Cloud . „ . » . 91 Evidence for a Common Parent Material . , . 92 Elemental Abundances in Carbonaceous Meteorites and the Solar Photosphere ............ 92 Uniformity of Fe and the Rare Earth Elements in Chondrites ............. ...... 9^ Evidence for a Genetic Relationship between Components 2 and 3 in the Chondrites ...... 96 Model for Accretion of Chondrites and Formation of Farenc Bodies .................... 9^ Character of Parent Bodies for the Chondritic Meoeontes . * . * . .. » 102 5. CALCIUM-RICH ACHOHDRITES ........ ... 106 Pyroxene-plagioclase Achondrites ............. 106 Diopside-olivine and Augite Achondrites .......... 107 Rare Earth Elements and Oxygen Isotopes in Stony Meteorites and Terrestrial Materials . 109 Uniformity of REE in Chondrites ............ 109 Calcium-poor and Calcium-rich Achondrites ....... 113 Meteorites and Terrestrial Mantle Materials ...... 115 Reflectance Characteristics of Stony Meteorites and the Zloon ......... ........ ... 11^ Remanent Magnetism in Meteorites ............. 118 Summary . © © . * . @ 12 ^ 6. METEORITE BRECCIAS 128 Monomict and Polymict Breccias .............. 128 General Descriptions and Definitions of Terms . .. 128 Dense Impactites ................... 157 Classification of the Meteorite Breccias ......... 169 Volatile-rich Breccias ................ 173 Volatile-poor Breccias ................ 17^ Interpretation of Record in Breccias ........... 17^ Comet-asteroid and Interasteroidal Collisions, Breakup of Asteroids, and Formation of Lunar Basins . 174 . Recent Cratering of the Moon ............. 184 Tektites, and Lunar and Terrestrial Craters ...... 189 APPENDIX I. Sources of Data for Table 4 - Elemental Abundances of Meteoritic Materials . « . 198 APPENDIX II. Notes and References for Table 20 .... ,. 208 ,'' \ -7:; .' -,'- ' : ■ , : ; '' " " -;y /' ;:: .^, viii • . v; : : y: . TABIE OF COMEIffS—Continued " ■ APPEMDIX IIIo List of Brecciated Meteorites Arranged in Genetic Groupings • » .. » e o • .•«>•.' 2lh APPEHDIX IVo Ages of Selected Stones and Irons used for Estimating the Ages of Collision Events Outlined in Table 21 „ , 9» o <. i » » «• •„ . ,. „ i . 220 EEFEREHCES CITED ». „ o « . , 0 ». , * , . =• , , , = ». , » « 9 » . 227 LIST OF ILLUSTRATIONS Figure • 1. Relationship between oxidized iron, and iron as metal and sulfide in analyses of observed falls in chondrites. 17 2„ Olivine composition, determined by X-ray diffraction, showing compositional hiatus in olivine-bronzite and olivine-hypersthene chondrites 19 3. Plot of CaO (weight percent) against FeO/FeO+MgO (mole percent) for the achondrites « . „ „ 0 . » e . » e . 6 . 22 4. Variation of Ga and Ge contents of iron meteorites . » . 32-33 5. Relation between Ga and Ge concentrations in iron
Recommended publications
  • Asteroids 2867 Steins and 21 Lutetia: Surface Composition from Far Infrared Observations with the Spitzer Space Telescope
    A&A 477, 665–670 (2008) Astronomy DOI: 10.1051/0004-6361:20078085 & c ESO 2007 Astrophysics Asteroids 2867 Steins and 21 Lutetia: surface composition from far infrared observations with the Spitzer space telescope M. A. Barucci1, S. Fornasier1,2,E.Dotto3,P.L.Lamy4, L. Jorda4, O. Groussin4,J.R.Brucato5, J. Carvano6, A. Alvarez-Candal1, D. Cruikshank7, and M. Fulchignoni1,2 1 LESIA, Observatoire de Paris, 92195 Meudon Principal Cedex, France e-mail: [email protected] 2 Université Paris Diderot, Paris VII, France 3 INAF, Osservatorio Astronomico di Roma, via Frascati 33, 00040 Monteporzio Catone, Roma, Italy 4 Laboratoire d’Astrophysique de Marseille, BP 8, 13376 Marseille Cedex 12, France 5 INAF, Osservatorio Astronomico di Capodimonte, via Moiariello 16, 80131 Napoli, Italy 6 Observatorio National (COAA), rua Gal. José Cristino 77, CEP20921–400 Rio de Janeiro, Brazil 7 NASA Ames Research Center, MS 245-6, Moffett Field, CA 94035-1000, USA Received 14 June 2007 / Accepted 3 October 2007 ABSTRACT Aims. The aim of this paper is to investigate the surface composition of the two asteroids 21 Lutetia and 2867 Steins, targets of the Rosetta space mission. Methods. We observed the two asteroids through their full rotational periods with the Infrared Spectrograph of the Spitzer Space Telescope to investigate the surface properties. The analysis of their thermal emission spectra was carried out to detect emissivity features that diagnose the surface composition. Results. For both asteroids, the Christiansen peak, the Reststrahlen, and the Transparency features were detected. The thermal emissiv- ity shows a clear analogy to carbonaceous chondrite meteorites, in particular to the CO–CV types for 21 Lutetia, while for 2867 Steins, already suggested as belonging to the E-type asteroids, the similarity to the enstatite achondrite meteorite is confirmed.
    [Show full text]
  • Geophysical Abstracts, 180-183 January-December 1960
    Geophysical Abstracts, 180-183 January-December 1960 GEOLOGICAL SURVEY BULLETIN 1116 Abstracts of current literature pertaining to the physics of the solid earth and to f!eophysical exploration • UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON : 1961 UNITED STATES DEPARTMENT OF THE INTERIOR STEWART L. UDALL, Secretary GEOLOGICAL SURVEY Thomas B. Nolan, Director 1 CONTENTS [The letters in parentheses are those used to designate the chapters for separate publication] Page (A) Geophysical Abstracts 180, January-March--------------------- 1 (B) Geophysical Abstracts 181, April-June------------------------- 129 (C) Geophysical Abstracts 182, July-September--------------------- 281 (D) Geophysical Abstracts 183, October-December------------------ 457 (E) Index to Geophysical Abstracts 180-183, 1960 ------------------- 637 Under department orders, Geophysical Abstracts has been published at different times by the Bureau of Mines orthe Geological Survey as noted below. 1-86, May 1929-June 1936, Bureau of Mines Information Circulars. [Mimeographed] 87, July-December 1936, Geological Survey Bulletin 887. 88-91, 'January-December 1937, Geological Survey Bulletin 895. 92-95, January-December 1938, Geological Survey Bulletin 909. 96-99, January-December 1939, Geological Survey Bulletin 915. 100-103, January-December 1940, Geological Survey Bulletin 925. 104-107, January-December 1941, Geological Survey Bulletin 932. 108-111, January-December 1942, Geological Survey Bulletin 939. 112-127, January 1943-December 1946, Bureau of Mines Information Circu- lars. [Mimeographed] 128-131, January-December 1947, Geological Survey Bulletin 957. 132-135, January-December 1948, Geological Survey Bulletin 959. 136-139, January-December 1949, Geological Survey Bulletin 966. 140-143, January-December 1950, Geological Survey Bulletin 976. 144-147, January-December 1951, Geological Survey Bulletin 981. 148-151, January-December 1952, Geological Survey Bulletin 991.
    [Show full text]
  • 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,
    [Show full text]
  • Curt Teich Postcard Archives Towns and Cities
    Curt Teich Postcard Archives Towns and Cities Alaska Aialik Bay Alaska Highway Alcan Highway Anchorage Arctic Auk Lake Cape Prince of Wales Castle Rock Chilkoot Pass Columbia Glacier Cook Inlet Copper River Cordova Curry Dawson Denali Denali National Park Eagle Fairbanks Five Finger Rapids Gastineau Channel Glacier Bay Glenn Highway Haines Harding Gateway Homer Hoonah Hurricane Gulch Inland Passage Inside Passage Isabel Pass Juneau Katmai National Monument Kenai Kenai Lake Kenai Peninsula Kenai River Kechikan Ketchikan Creek Kodiak Kodiak Island Kotzebue Lake Atlin Lake Bennett Latouche Lynn Canal Matanuska Valley McKinley Park Mendenhall Glacier Miles Canyon Montgomery Mount Blackburn Mount Dewey Mount McKinley Mount McKinley Park Mount O’Neal Mount Sanford Muir Glacier Nome North Slope Noyes Island Nushagak Opelika Palmer Petersburg Pribilof Island Resurrection Bay Richardson Highway Rocy Point St. Michael Sawtooth Mountain Sentinal Island Seward Sitka Sitka National Park Skagway Southeastern Alaska Stikine Rier Sulzer Summit Swift Current Taku Glacier Taku Inlet Taku Lodge Tanana Tanana River Tok Tunnel Mountain Valdez White Pass Whitehorse Wrangell Wrangell Narrow Yukon Yukon River General Views—no specific location Alabama Albany Albertville Alexander City Andalusia Anniston Ashford Athens Attalla Auburn Batesville Bessemer Birmingham Blue Lake Blue Springs Boaz Bobler’s Creek Boyles Brewton Bridgeport Camden Camp Hill Camp Rucker Carbon Hill Castleberry Centerville Centre Chapman Chattahoochee Valley Cheaha State Park Choctaw County
    [Show full text]
  • Calcium Isotopes in Natural and Experimental Carbonated Silicate Melts
    Western University Scholarship@Western Electronic Thesis and Dissertation Repository 2-27-2018 2:30 PM Calcium Isotopes in Natural and Experimental Carbonated Silicate Melts Matthew Maloney The University of Western Ontario Supervisor Bouvier, Audrey The University of Western Ontario Co-Supervisor Withers, Tony The University of Western Ontario Graduate Program in Geology A thesis submitted in partial fulfillment of the equirr ements for the degree in Master of Science © Matthew Maloney 2018 Follow this and additional works at: https://ir.lib.uwo.ca/etd Part of the Geochemistry Commons Recommended Citation Maloney, Matthew, "Calcium Isotopes in Natural and Experimental Carbonated Silicate Melts" (2018). Electronic Thesis and Dissertation Repository. 5256. https://ir.lib.uwo.ca/etd/5256 This Dissertation/Thesis is brought to you for free and open access by Scholarship@Western. It has been accepted for inclusion in Electronic Thesis and Dissertation Repository by an authorized administrator of Scholarship@Western. For more information, please contact [email protected]. Abstract The calcium stable isotopic compositions of mantle-sourced rocks and minerals were investigated to better understand the carbon cycle in the Earth’s mantle. Bulk carbonatites and kimberlites were analyzed to identify a geochemical signature of carbonatite magmatism, while inter-mineral fractionation was measured in co-existing Ca-bearing carbonate and silicate minerals. Bulk samples show a range of composition deviating from the bulk silicate Earth δ44/40Ca composition indicating signatures of magmatic processes or marine carbonate addition 44/40 to source materials. Δ Cacarbonate-silicate values range from -0.55‰ to +1.82‰ and positively correlate with Ca/Mg ratios in pyroxenes.
    [Show full text]
  • Geological Survey Canada
    70-66 GEOLOGICAL PAPER 70-66 ., SURVEY OF CANADA DEPARTMENT OF ENERGY, MINES AND RESOURCES REVISED CATALOGUE OF THE NATIONAL METEORITE COLLECTION OF CANADA LISTING ACQUISITIONS TO AUGUST 31, 1970 J. A. V. Douglas 1971 Price, 75 cents GEOLOGICAL SURVEY OF CANADA CANADA PAPER 70-66 REVISED CATALOGUE OF THE NATIONAL METEORITE COLLECTION OF CANADA LISTING ACQUISITIONS TO AUGUST 31, 1970 J. A. V. Douglas DEPARTMENT OF ENERGY, MINES AND RESOURCES @)Crown Copyrights reserved Available by mail from Information Canada, Ottawa from the Geological Survey of Canada 601 Booth St., Ottawa and Information Canada bookshops in HALIFAX - 1735 Barrington Street MONTREAL - 1182 St. Catherine Street West OTTAWA - 171 Slater Street TORONTO - 221 Yonge Street WINNIPEG - 499 Portage Avenue VANCOUVER - 657 Granville Street or through your bookseller Price: 75 cents Catalogue No. M44-70-66 Price subject to change without notice Information Canada Ottawa 1971 ABSTRACT A catalogue of the National Meteorite Collection of Canada, published in 1963 listed 242 different meteorite specimens. Since then specimens from 50 a dditional meteorites have been added to the collection and several more specimens have been added to the tektite collection. This report describes all specimens in the collection. REVISED CATALOGUE OF THE NATIONAL METEORITE COLLECTION OF CANADA LISTING ACQUISITIONS TO AUGUST 31, 1970 INTRODUCTION At the beginning of the nineteenth century meteorites were recog­ nized as unique objects worth preserving in collections. Increasingly they have become such valuable objects for investigation in many fields of scienti­ fic research that a strong international interest in their conservation and pre­ servation has developed (c. f.
    [Show full text]
  • Asteroid Regolith Weathering: a Large-Scale Observational Investigation
    University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Doctoral Dissertations Graduate School 5-2019 Asteroid Regolith Weathering: A Large-Scale Observational Investigation Eric Michael MacLennan University of Tennessee, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_graddiss Recommended Citation MacLennan, Eric Michael, "Asteroid Regolith Weathering: A Large-Scale Observational Investigation. " PhD diss., University of Tennessee, 2019. https://trace.tennessee.edu/utk_graddiss/5467 This Dissertation is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a dissertation written by Eric Michael MacLennan entitled "Asteroid Regolith Weathering: A Large-Scale Observational Investigation." I have examined the final electronic copy of this dissertation for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Doctor of Philosophy, with a major in Geology. Joshua P. Emery, Major Professor We have read this dissertation and recommend its acceptance: Jeffrey E. Moersch, Harry Y. McSween Jr., Liem T. Tran Accepted for the Council: Dixie L. Thompson Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) Asteroid Regolith Weathering: A Large-Scale Observational Investigation A Dissertation Presented for the Doctor of Philosophy Degree The University of Tennessee, Knoxville Eric Michael MacLennan May 2019 © by Eric Michael MacLennan, 2019 All Rights Reserved.
    [Show full text]
  • Report of the United States National Museum
    — THE METEORITE COLLECTION IN THE U. S. NATIONAL MUSEUM; A CATALOGUE OF METEORITES REPRESENTED NOVEMBER 1, 1886, By F. W. Clarke. The following catalogue has been prepared mainly to facilitate ex- changes and to aid in the upbuilding of the collection. In addition to the usual information as to title, date of fall, and weight of specimen, it has beeu thought well to give the source from which each example was obtained ; and it may be interesting to note that the meteorites ac- credited to Dr. J. Berrien. Lindsley were mainly received by him from the late Dr. J. Lawrence Smith. In the catalogue of the Shepard col- lection, now on deposit in the Museum, the arrangement of Professor Shepard himself has been followed without change. Including the Shepard meteorites, over 200 falls are now on exhibition, giving the entire collection a very respectable place among the larger collections of the world. The Tucson iron is unique, and therefore a cut of it is inserted. METEORIC IRONS. 1. Scriba, Oswego County, N. Y. Fouud about 1834. Fragment, 9.15 grammes. By exchange from S. C. H. Bailey. 2. Burlington, Otsego County, N. Y. Ploughed up previous to 1819. Weight of specimen, 76.87 grammes. By exchange from Prof. C. U. Shepard. 3. Lockport, Niagara County, N. Y. Ploughed up earlier thau 1845. Slice weigh- ing 155 grammes. By exchange from the cabinet of Yale College. 4. Jenny's Cheek, Wayne County, W. Va. Found in 1884. Several small frag- ments, 25.5 grammes in all; largest fragment, 15.3 grammes.
    [Show full text]
  • The Origin of S-Process Isotope Heterogeneity in the Solar Protoplanetary Disk
    The origin of s-process isotope heterogeneity in the solar protoplanetary disk Mattias Ek1,2*, Alison C. Hunt1, Maria Lugaro3,4, Maria Schönbächler1 Preprint version of manuscript published in Nature Astronomy on December 9th 2019 (https://doi.org/10.1038/s41550-019-0948-z). Online, free-for-all, access to the published pdf is available through the Springer Nature SharedIt initiative here. 1 Institute for Geochemistry and Petrology, ETH Zürich, Clausiusstrasse 25, 8092 Zürich, Switzerland. 2 Bristol Isotope Group, School of Earth Sciences, University of Bristol, Wills Memorial Building, Queen’s Road, Bristol BS8 1RJ, United Kingdom. 3 Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, MTA Centre for Excellence, H-1121 Budapest, Hungary. 4 Monash Centre for Astrophysics, School of Physics and Astronomy, Monash University, VIC 3800, Australia. *e-mail: [email protected] 1 Rocky asteroids and planets display nucleosynthetic isotope variations that are attributed to the heterogeneous distribution of stardust from different stellar sources in the solar protoplanetary disk. Here we report new high precision palladium isotope data for six iron meteorite groups, which display smaller nucleosynthetic isotope variations than the more refractory neighbouring elements. Based on this observation we present a new model in which thermal destruction of interstellar medium dust results in an enrichment of s-process dominated stardust in regions closer to the Sun. We propose that stardust is depleted in volatile elements due to incomplete condensation of these elements into dust around asymptotic giant branch (AGB) stars. This led to the smaller nucleosynthetic variations for Pd reported here and the lack of such variations for more volatile elements.
    [Show full text]
  • List of Meteorites in the Collections of the Central Siberian Geological Museum at the V.S.Sobolev Institute of Geology and Mineralogy SB RAS (SIGM)
    List of meteorites in the collections of the Central Siberian Geological Museum at the V.S.Sobolev Institute of Geology and Mineralogy SB RAS (SIGM). Year Mass in Pieces in Main mass in Indication Meteorite Country Type found SIGM SIGM SIGM in MB Novosibirsk Russia 1978 H5/6 9.628 kg 2 yes 59 Markovka Russia 1967 H4 7.9584 kg 5 yes 48 Ochansk Russia 1887 H4 407 g 1 Kunashak Russia 1949 L6 268 g 1 6 Saratov Russia 1918 L4 183.4 g 1 Elenovka Ukraine 1951 L5 148.7 g 2 6 Zhovtnevyi Ukraine 1938 H6 88.5 g 1 Nikolskoe Russia 1954 L4 39.5 g 1 6 Krymka Ukraine 1946 LL3.2 11.1 g 1 Yurtuk Ukraine 1936 Howardite 5.3 g 1 Pervomaisky Russia 1933 L6 595 g 1 Ivanovka Russia 1983 H5 904 g 1 63 Tsarev Russia 1968 H5 1.91972 kg 3 59 Norton County USA 1948 Aubrite 144 g 1 Stannern Cz. Republic 1808 18.1 g 1 Eucrite-mmict Poland 1868 H5 63.02 g 1 Pultusk Chelyabinsk Russia 2013 LL5 1.55083 kg 28 102 Yaratkulova Russia 2016 H5 25.71 g 1 105 Tobychan Russia 1971 Iron, IIE 41.4998 kg 2 yes 51 Elga Russia 1959 Iron, IIE 10.5 kg 1 16 Sikhote-Alin Russia 1947 Iron, IIAB 37.1626 kg 12 Chebankol Russia 1938 Iron, IAB-sHL 87.1 g 1 Chinga (Chinge) Russia 1912 Iron, ungrouped 5.902 kg 3 13 Kaalijarv (Kaali) Estonia 1937 2.88 g a lot of Iron, IAB-MG Boguslavka Russia 1916 Iron, IIAB 55.57 g 1 Bilibino Russia 1981 Iron, IIAB 570.94 g 1 60 Anyujskij Russia 1981 Iron, IIAB 435.4 g 1 60 Sychevka Russia 1988 Iron, IIIAB 1.581 kg 1 70 Darjinskoe Kazakhstan 1984 Iron, IIC 6 kg 1 yes 78 Maslyanino Russia 1992 Iron, IAB complex 58 kg 2 yes 78 Onello Russia 1998 Iron, ungrouped
    [Show full text]
  • 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.
    [Show full text]
  • Fiscal Year 1964 and 1965
    NOTE TO READERS: ALL PRINTED PAGES ARE INCLUDED, UNNUMBERED BLANK PAGES DURING SCANNING AND QUALITY CONTROL CHECK HAVE BEEN DELETED EXECUTIVE OFFICE OF THE PRESIDENT NATIONAL AERONAUTICS AND SPACE COUlNClL WASHINGTON. D. C. 20M2 THE WHITE HOUSE WASH I NGTON January 27, 1965 TO THE CONGRESS OF THE UNITED STATES: I am proud to transmit -- as I know the Congress will be proud to receive -- this review of the significant successes of our Nation's aeronautics and space efforts in the calendar year of 1964. The advances of 1964 were gratifying and heartening omens of the gains and good to come from our determined national undertaking in exploring the frontiers of space. While this great enterprise is still young, we began during the year past to realize its potential in our life on earth. As this report notes, practical uses of the benefits of space technology were almost commonplace around the globe -- warning us of gathering storms, guiding our ships at sea, assisting our map-makers and serving, most valuably of all, to bring the peoples of many nations closer together in joint peaceful endeavors. Substantial strides have been made in a very brief span of time -- and more are to come. We expect to explore the moon, not just visit it or photograph it. We plan to explore and chart planets as well. We shall expand our earth laboratories into space laboratories and extend our national strength into the space dimension. The purpose of the American people -- expressed in the earliest days of the Space Age -- remains unchanged and unwavering.
    [Show full text]