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RESALE Numberor Stating You Are a Retailor In
TucsonAuction08.html 9th Annual Tucson Meteorite Auction ----------------------------- Tucson Meteorite Auction 2008 Saturday, February 9th, 2008 Bidding starts 7:30PM Sharp Viewing & Socializing begins 5:30PM Food and Drink available http://www.michaelbloodmeteorites.com/TucsonAuction08.html (1 z 36) [2008-05-28 18:09:44] TucsonAuction08.html (Please drink only with a designated driver) ----------------------- While in Tucson I will have a cell phone: (619) 204-4138 (Feb2-Feb10) NEW LOCATION VFW Hall (Post # 549) 1884 So. Craycroft, Tucson, AZ 85711 (see directions below) NOTE: Click HERE for printer friendly copy of this catalog (Click on any photo to see a greatly enlarged image) 1 AH 1 Claxton L6, GeorgiaDecember 10 th , 1984 - Hit A Mailbox! .992g Rim Crusted Part Slice (21mm X 20mm X 2mm) No Minimum 2 AH 2 Dhofar 908 Lunar Meteorite - Rosetta - 1.242g Full Slice (24mm X 16mm X 2mm) No Minaimum - (est: $2.5K min) 3 AH 3 NWA 2999 Angrite Famous Paper "The Case For Samples From Mercury" 3.216g FC End Piece (18mm X 15mm X 7mm) No Minimum http://www.michaelbloodmeteorites.com/TucsonAuction08.html (2 z 36) [2008-05-28 18:09:44] TucsonAuction08.html 4 AH 4 NWA 4473 Polymict Diogenite 13g Full Slice(70mm X 13mm X ~2.5mm) No Minimum 5 AH 5 NWA 4880 (Shergottite) .540g 70% F Crusted Whole Stone (11mm X 9mm X 5mm) No Minimum 6 AH 6 NWA 4880 (Shergottite) 32.3g 92% FC Oriented Main Mass (35mm X 32mm X 32mm) Minimum Bid: $12,900.00 (Less Than $400/g) 7 AH 7 Oued el Hadjar (LL6) Fall March 1986 - "The Wedding Stone" 6.322 g (41mm X 30m X 3mm) The stone was broken into many pieces, then sacrificed on an alter during a wedding ceremony. -
Zinc and Copper Isotopic Fractionation During Planetary Differentiation Heng Chen Washington University in St
Washington University in St. Louis Washington University Open Scholarship Arts & Sciences Electronic Theses and Dissertations Arts & Sciences Winter 12-15-2014 Zinc and Copper Isotopic Fractionation during Planetary Differentiation Heng Chen Washington University in St. Louis Follow this and additional works at: https://openscholarship.wustl.edu/art_sci_etds Part of the Earth Sciences Commons Recommended Citation Chen, Heng, "Zinc and Copper Isotopic Fractionation during Planetary Differentiation" (2014). Arts & Sciences Electronic Theses and Dissertations. 360. https://openscholarship.wustl.edu/art_sci_etds/360 This Dissertation is brought to you for free and open access by the Arts & Sciences at Washington University Open Scholarship. It has been accepted for inclusion in Arts & Sciences Electronic Theses and Dissertations by an authorized administrator of Washington University Open Scholarship. For more information, please contact [email protected]. WASHINGTON UNIVERSITY IN ST. LOUIS Department of Earth and Planetary Sciences Dissertation Examination Committee: Bradley L. Jolliff, Chair Jeffrey G. Catalano Bruce Fegley, Jr. Michael J. Krawczynski Frédéric Moynier Zinc and Copper Isotopic Fractionation during Planetary Differentiation by Heng Chen A dissertation presented to the Graduate School of Arts & Sciences of Washington University in partial fulfillment of the requirements for the degree of Doctor of Philosophy December 2014 St. Louis, Missouri Copyright © 2014, Heng Chen All rights reserved. Table of Contents LIST OF FIGURES -
1962-11 Millman
MINUTES SPECIAL COUNCIL MEETING OF THE METEORITICAL SOCIETY held at Los Angeles, Calif., Sat., 17 Nov. 1962 PRESENT: President Peter M. Millman, Past-President John A. Russell, Editor Dorrit Hoffleit, Councilor C. H. Cleminshaw, and Secretary Gerald L. Rowland. Since Peter Millman and Dorrit Hoffleit were both in Los Angeles at the same time, and since it was possible to get a quorum of the Council together, President Millman called a Special meeting of the Council for Sat., 17 Nov. 1962. The last Council minutes (of 4 Sept., 1962) were read in order that those present might know the business that was transacted at Socorro, New Mexico. After some discussion, it was moved, seconded, and approved that arrangements be made for the transfer of a suitable number (approximately 40) of the 4 issues of Vol. I of Meteoritics from Springer Transfer Co. in Albuquerque, N. M., to John Russell at U.S.C. The Council approved the expenditure of whatever funds are necessary for this operation. John Russell reported that the Leonard Memorial Medal, which was displayed at the Socorro meeting, was unsatisfactory and that it is being re-done by the Southern California Trophy Co. The Council was reminded that the fund established for the Leonard Memorial Medal is still open for contributions. The cost of engraving and striking each individual medal to be presented will call for a nominal expenditure from time to time. The Council next suggested the following chairmen (subject to the individual's acceptance) for the standing committees of the Society: Eugene Shoemaker (Membership and Fellowship); Oscar Monnig (Finance and Endowment); Editor Dorrit Hoffleit (Publications). -
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. -
Breve Histórico Dos Meteoritos Brasileiros
Parte 1 Breve histórico dos meteoritos brasileiros Maria Elizabeth Zucolotto (MN/UFRJ) Os meteoritos se prestam ao estudo das condições e processos físicos da formação do sistema solar. São fragmentos de corpos em diversos estágios de diferenciação planetária, sendo encontrados desde meteoritos primitivos, de composição solar, até representantes da crosta, manto e núcleo de corpos planetários diferenciados. A história dos meteoritos brasileiros está diretamente ligada à história da meteorítica, pois o Bendegó foi descoberto em 1784 quando ainda se desconhecia a natureza extraterrestre dos meteoritos. O Bendegó foi durante muitos anos o maior meteorito em exposição em um museu. O Brasil possui hoje apenas 62 meteoritos certificados, alguns muito importantes como o Angra dos Reis, que deu origem a uma classe de meteoritos, os “angritos”. Pedras sagradas Embora os meteoritos só tenham sido aceitos pela ciência como objetos de origem extraterrestre no início do século 19, o fenômeno de queda de rochas e ferro sobre a Terra (meteoros e bólidos) era conhecido desde a antiguidade. Papiros egípcios, de 4 mil anos, registram objetos luminosos riscando os céus numa representação típica de queda de meteoritos, isto é, queda de objetos sólidos no chão. Escritos gregos, de 3,5 mil e 2,5 mil anos, mencionam a queda de pedras e ferro do céu. Provavelmente pela natureza extraterrestre e supostos poderes mágicos, al- guns meteoritos foram objetos de veneração em várias civilizações, dos quais só restaram algumas descrições históricas. A mais interessante é a de Tito Lívio rela- tando que, em 204 AEC, a pedra negra que simbolizava a Magna Mater (Grande Mãe, também chamada Cibele), foi levada para Roma em situação interessante: os exércitos de Aníbal tinham penetrado nos territórios romanos disseminan- do o pânico entre a população. -
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. -
The Oscar E. Monnig Meteorite Collection and Museum. Rg
41st Lunar and Planetary Science Conference (2010) 1162.pdf THE OSCAR E. MONNIG METEORITE COLLECTION AND MUSEUM. R. G. Mayne1 and T. Moss1 De- partment of Geology, TCU Box 298830, Texas Christian University, Fort Worth, TX 76109 ([email protected]) The Man Behind the Meteorites [1]: Oscar not knowing the full extent of what was to come. In Monnig was born in Fort Worth, Texas in 1902, and he the years that followed a number of meteorites were lived there till his death in 1999. He was a business- transferred to TCU, but it was not until his death in man and he started work for his family’s dry goods 1999 that the full generosity of Oscar’s offer came to company after earning his law degree from the Univer- light. TCU not only inherited all of Oscar’s meteorite sity of Texas in 1925 and was the CEO of the company collection, but also a large amount of his estate for when it was sold in 1982. However, Oscar’s passion “education, care, and maintenance of the meteorite was for meteorites, he was an avid collector. He even collection.” gave self-printed brochures to his traveling salesmen to The Monnig Meteorite Collection at TCU: The distribute that described how to identify meteorites and collection donated by Oscar Monnig was one of the offered to purchase any that were found. finest private collections of its day, and it is now one In 1960 Oscar Monnig introduced himself to a new of the finest University-based collections in the world, hire in the TCU Geology department, Dr. -
Meteorite Collections: Catalog
Meteorite Collections: Catalog Institute of Meteoritics Department of Earth and Planetary Sciences University of New Mexico July 25, 2011 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. -
O Lunar and Planetary Institute Provided by the NASA Astrophysics Data System the BELLS CARBONACEOUS CHONDRITE
BELLS-A CARBONACEOUS CHONDRITE RELATED TO C1 AND C2 CHONDRITES; Andrew M. ~avisland Edward 01sen2. l~amesFranck Institute, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637; 2~epartmentof Geology, Field Museum of Natural History, Chicago, IL 60605. The Bells, Texas meteorite fell on September 9, 1961. It was classified as a Type I1 carbonaceous chondrite by Mason [I]. Bulk samples of Bells have been found to contain 13 to 16 wt% magnetite by magnetic methods [2,3]. This is far more magnetite than is normally found in C2 chondrites and is slightly higher than the levels found in C1 chondrites [3]. McSween and Richardson [41 measured the bulk composition of "matrix" in many carbonaceous chondrites (including Bells) by broad beam electron microprobe analysis. They found a range of compositions among the phyllosilicate matrices of C1 and C2 chond- rites. Bells and the C1 chondrites are at the Fe-poor, Mg- and Si-rich end of this range. McSween [5] point-counted many C2 chondrites and found Bells to be among the most matrix-rich of them. He found a correlation between the composition of matrix and vol% matrix and suggested that increasing degree of alteration of chondrules and inclusions leads to increasing matrix fraction and decreasing Fe content of the matrix. According to his model, Bells should be among the most heavily altered of the C2 chondrites. Until recently, most of the recovered samples of Bells have been in the private collection of Mr. Oscar Monnig and the only sample available for pet- rographic study has been a tiny thin section. -
CONTENTS – W Through Z
67th Annual Meteoritical Society Meeting (2004) alpha_w-z.pdf CONTENTS – W through Z The Location of Martian Atmospheric Argon in Three Martian Basalts: Controls Exerted by Shock Effects E. L. Walton, S. P. Kelley, and J. G. Spray ............................................................................................ 5182 Core Formation in Planetesimals: Constraints from Siderophile Elements in Ureilites P. H. Warren .......................................................................................................................................... 5223 Lunar Meteorite Yamato-983885: A Relatively KREEPy Regolith Breccia Not Paired with Y-791197 P. H. Warren and J. C. Bridges.............................................................................................................. 5095 Extensive Melting of Amoeboid-Olivine Inclusions J. T. Wasson, A. E. Rubin, and J. M. Trigo-Rodriguez........................................................................... 5202 Fabric Analysis of Allende Matrix Using EBSD L. E. Watt, P. A. Bland, S. S. Russell, and D. J. Prior............................................................................ 5037 Unraveling the Exposure Histories of Aubrites K. C. Welten, K. Nishiizumi, D. J. Hillegonds, M. W. Caffee, and J. Masarik....................................... 5220 Nitrogen-Mapping and Nitrogen-XANES Spectroscopy of Interplanetary Dust Particles S. Wirick, G. J. Flynn, L. P. Keller, and C. Jacobsen ............................................................................ 5092 Further -
STUDIES of Brazillan METEORITES. II. the AVANHANDAVA CHONDRITE: MINERALOGY, PETROLOGY and CHEMISTRY
Revista Brasileira de Geocüncias Vclume B, 1976 201 STUDIES OF BRAZILlAN METEORITES. II. THE AVANHANDAVA CHONDRITE: MINERALOGY, PETROLOGY AND CHEMISTRY W. PAAR", K. KEIL, C.B. GOMES"", Department of Geology and Institute of Meteoritics, University of New Mexico,Albuquerque, New México 87131, USA and E. JAROSEWICH Department of Mineral Sciences, Smithsonian Institution, National Museum of Natural History, Washington, D.e. 20560, USA ABSTRACT A description of the Avanhandava, State of São Paulc. Braail; meteorite, which fell in 1952, is given using optical, microprobe, and bulk chemical data, Thia Hcgroup- or olivine -bronzite chondrite contains olivine (Fa I7.3), bronzite (Fs 16'5)' díopeide (Wo45.3En49'O Fs5.7), oli goclase (Or 5.4 Ab 84.1 An IO' 4)' whitlockite, chlorapatite, kamacite, taenite (plessite), -troilite, chromite, native copper, pentlandite, ilmenite, bravoite, mackinawite, and chalcopyrrhotite. On the basis of mineral and bulk compositions as well as its texture, the Avanhandava meteorite is classified as an H4 chondrite. RESU MO Dados ópticos e .. químicos são fornecidos para o meteorito de Avanhandáva, Estado de São Paulo, Brasil, cuja queda teve lugar em 1952. Este olivina-bronzita condrito, pertencente ,,=0 grupo H, consiste em, olivina (FaI7,3)' bronzita (Fs I6,5)' diopsídio (Wo45,3 En49,o FS5,7)' oligoclásio (Or 5,4 Ab 84, 1 An 10,4)' whitlockita, cloroapatita, kamacita, taenita [plesaita], troilita, crornitá, cobre nativo, pentlandita, ilmenita, bravoita, mackinawita e calcopirita. Com base em dados químicos (composição mineral e global] e' texturais, o meteorito de Avanhandava é classificado como um con drito H4. INTRODUCTION The Avanhandava, State of São Paulo, Brazil, stone meteorite fell . -
Catalogue of Meteorites from South America Springerbriefs in Earth System Sciences
SPRINGER BRIEFS IN EARTH SYSTEM SCIENCES SOUTH AMERICA AND THE SOUTHERN HEMISPHERE Rogelio Daniel Acevedo Maximiliano C. L. Rocca Víctor Manuel García Catalogue of Meteorites from South America SpringerBriefs in Earth System Sciences South America and the Southern Hemisphere Series editors Gerrit Lohmann Jorge Rabassa Justus Notholt Lawrence A. Mysak Vikram Unnithan For further volumes: http://www.springer.com/series/10032 Rogelio Daniel Acevedo Maximiliano C. L. Rocca Víctor Manuel García Catalogue of Meteorites from South America 123 Rogelio Daniel Acevedo Víctor Manuel García Centro Austral de Investigaciones Centro Austral de Investigaciones Científicas Científicas Tierra del Fuego Tierra del Fuego Argentina Argentina Maximiliano C. L. Rocca The Planetary Society Buenos Aires Argentina There may be instances where the authors have been unable to trace or contact the copyright holders. If notified the publisher will be pleased to rectify any errors or omissions at the earliest opportunity. ISSN 2191-589X ISSN 2191-5903 (electronic) ISBN 978-3-319-01924-6 ISBN 978-3-319-01925-3 (eBook) DOI 10.1007/978-3-319-01925-3 Springer Cham Heidelberg New York Dordrecht London Library of Congress Control Number: 2013949406 Ó The Author(s) 2014 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. Exempted from this legal reservation are brief excerpts in connection with reviews or scholarly analysis or material supplied specifically for the purpose of being entered and executed on a computer system, for exclusive use by the purchaser of the work.