The Monnig Meteorite Collection Numbers Revisited
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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. -
Petrography and Mineral Chemistry of Escalón Meteorite, an H4 Chondrite, México
148 Reyes-SalasRevista Mexicana et al. de Ciencias Geológicas, v. 27, núm. 1, 2010, p. 148-161 Petrography and mineral chemistry of Escalón meteorite, an H4 chondrite, México Adela M. Reyes-Salas1,*, Gerardo Sánchez-Rubio1, Patricia Altuzar-Coello2, Fernando Ortega-Gutiérrez1, Daniel Flores-Gutiérrez3, Karina Cervantes-de la Cruz1, Eugenio Reyes4, and Carlos Linares5 1 Universidad Nacional Autónoma de México, Instituto de Geología, Del. Coyoacán, 04510 México D.F., Mexico. 2 Universidad Nacional Autónoma de México, Centro de Investigación en Energía, Campus Temixco, Priv. Xochicalco s/n, 62580 Temixco Morelos, Mexico. 3 Universidad Nacional Autónoma de México, Instituto de Astronomía, Del. Coyoacán, 04510 México D.F., Mexico. 4 Universidad Nacional Autónoma de México, Facultad de Química, Del. Coyoacán, 04510 México D.F., Mexico. 5 Universidad Nacional Autónoma de México, Instituto de Geofísica, Del. Coyoacán, 04510 México D.F., Mexico. * [email protected] ABSTRACT The Escalón meteorite, a crusted mass weighing 54.3 g, was recovered near Zona del Silencio in Escalón, state of Chihuahua, México. The stone is an ordinary chondrite belonging to the high iron group H, type 4. Electron microprobe analyses of olivine (Fa18.1) and pyroxene (Fs16.5), phosphate, plagioclase, opaque phases, matrix and chondrule glasses are presented. The metal phases present are kamacite (6.08 % Ni), taenite (31.66 % Ni), high nickel taenite (50.01 % Ni) and traces of native Cu. The chondrules average apparent diameter measures 0.62 mm. X-ray diffraction pattern shows olivine, pyroxene and kamacite. Alkaline-type glass is found mainly in chondrules. This meteorite is a stage S3, shock-blackened chondrite with weathering grade W0. -
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 -
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. -
Noble Gas Study of the Saratov L4 Chondrite
Meteoritics & Planetary Science 45, Nr 3, 361–372 (2010) doi: 10.1111/j.1945-5100.2010.01026.x Noble gas study of the Saratov L4 chondrite Jun-ichi MATSUDA1*, Hidetomo TSUKAMOTO1, Chie MIYAKAWA1, and Sachiko AMARI2 1Department of Earth and Space Science, Graduate School of Science, Osaka University, Toyonaka, Osaka 560-0043, Japan 2Laboratory for Space Sciences and the Physics Department, Washington University, St. Louis, Missouri 63130, USA *Corresponding author. E-mail: [email protected] (Received 10 September 2008; revision accepted 28 December 2009) Abstract–We have determined the elemental abundances and the isotopic compositions of noble gases in a bulk sample and an HF ⁄ HCl residue of the Saratov (L4) chondrite using stepwise heating. The Ar, Kr, and Xe concentrations in the HF ⁄ HCl residue are two orders of magnitude higher than those in the bulk sample, while He and Ne concentrations from both are comparable. The residue contains only a portion of the trapped heavy noble gases in Saratov; 40 ± 9% for 36Ar, 58 ± 12% for 84Kr, and 48 ± 10% for 132Xe, respectively. The heavy noble gas elemental pattern in the dissolved fraction is similar to that in the residue but has high release temperatures. Xenon isotopic ratios of the HF ⁄ HCl residue indicate that there is no Xe-HL in Saratov, but Ne isotopic ratios in the HF ⁄ HCl residue lie on a straight line connecting the cosmogenic component and a composition between Ne-Q and Ne-HL. This implies that the Ne isotopic composition of Q has been changed by incorporating Ne-HL (Huss et al. -
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. -
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. -
Minerals in Meteorites
APPENDIX 1 Minerals in Meteorites Minerals make up the hard parts of our world and the Solar System. They are the building blocks of all rocks and all meteorites. Approximately 4,000 minerals have been identified so far, and of these, ~280 are found in meteorites. In 1802 only three minerals had been identified in meteorites. But beginning in the 1960s when only 40–50 minerals were known in meteorites, the discovery rate greatly increased due to impressive new analytic tools and techniques. In addition, an increasing number of different meteorites with new minerals were being discovered. What is a mineral? The International Mineralogical Association defines a mineral as a chemical element or chemical compound that is normally crystalline and that has been formed as a result of geological process. Earth has an enormously wide range of geologic processes that have allowed nearly all the naturally occurring chemical elements to participate in making minerals. A limited range of processes and some very unearthly processes formed the minerals of meteorites in the earliest history of our solar system. The abundance of chemical elements in the early solar system follows a general pattern: the lighter elements are most abundant, and the heavier elements are least abundant. The miner- als made from these elements follow roughly the same pattern; the most abundant minerals are composed of the lighter elements. Table A.1 shows the 18 most abundant elements in the solar system. It seems amazing that the abundant minerals of meteorites are composed of only eight or so of these elements: oxygen (O), silicon (Si), magnesium (Mg), iron (Fe), aluminum (Al), calcium (Ca), sodium (Na) and potas- sium (K). -
Intercom Debates Image, Tuition Hikes Students Voice Concerns
'TALL TALE' STAR MEASURES UP - PAGE 4 TCU DAILY SKIFF FRIDAY, MARCH 24,1995 TEXAS CHRISTIAN UNIVERSITY, FORT WORTH, TEXAS 92ND YEAR, NO. 90 Intercom debates image, tuition hikes Students voice concerns . - with Board of Trustees BY GINGER RICHARDSON "1 have a daughter here and would TCU DAILY SKIFF rather not see tuition increase to that extent," Scharbauer said. "1 think if Finding ways to improve the uni- we market ourselves as being as good versity's image while keeping tuition as Tulane, Vanderbilt or Wake Forest and fees at a reasonable level was the and then say, 'Oh, by the way, we're main issue of concern at Thursday's also $ 10,000 to $ 15,000 cheaper than f meeting between Intercom and mem- those schools,' that will be a draw to bers of the Board of Trustees. students." Student leaders and the Intercom members also asked the P» Trustee/Student Relations Commit- trustees to consider allocating funds ' j^J^jiiM^R*". tee also discussed what the financial for additional faculty, greater handi- ^^n . priorities of the university should be cap accessibility, residence hall ren- ^^^■^F # m. 'Mi,'. over the course of the next several ovations and increased scholarships years. — all of which would help improve Louis H. Barnett. a trustee from TCU's image, they said. Fort Worth, proposed increasing "The main thing we are concerned tuition to the level of schools such as about is image," said Scott Wheatley. ''*,'//'uM/t^^ i^k Tulane or Wake Forest to solve what a junior political science major and ™ %Jlmh some trustees and Intercom members student body president.