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Wedderburn – Wickenburg
Weaver Mountains - Wedderburn 1295 Figure 1908. Weaver Mountains (U.S.N.M. no. 1427). Kamacite Figure 1909. Weaver Mountains (U.S.N.M. no. 1427). Kamacite grains with schreibersite crystals (S). Duplex, almost unresolvable grains with numerous schreibersite particles, usually in contact with matrix. Etched. Scale bar 50 ll· (Perry 1950: volume 7.) taenite along at least one surface. Etched. Scale bar 40 ll· (Perry 1950: volume 7 .) forms together occur with a frequency of about 600 per mm 2 . The a-phase has subboundaries, but neither Specimens in the U.S. National Museum in Washington: Neumann bands nor hatched structures were observed. 546 g slice (no. 1427, 19 x 9 x 0.6 em) The plessitic matrix appears to be of a bainitic, duplex 167 g part slice (no. 1427, 12 x 8 x 0.3 em) type, but requires electron microscopy for any details to be 60 g part slice (no. 3145,5 x 3.5 x 0.5 em) seen. It appears striped at low magnification, apparently along the Widmanstiitten directions, as defmed by the scattered a-lamellae. The hardness is 300±15 and rather uniform right to the corroded edge of the specimens. Wedderburn , Victoria, Australia Schreibersite occurs as a few, "large" crystals, 40 x 60 Approximately 36°26'S, 143°38'E or 120 x 2011 in size, but most of the phosphides are present as evenly distributed blebs, 1-1011 across. They Nickel-rich ataxite, D. Numerous a-spindles 10±2~t wide. Neumann have nucleated narrow rims of swathing kamacite, but the bands. -
Meteorite Mineralogy Alan Rubin , Chi Ma Index More Information
Cambridge University Press 978-1-108-48452-7 — Meteorite Mineralogy Alan Rubin , Chi Ma Index More Information Index 2I/Borisov, 104, See interstellar interloper alabandite, 70, 96, 115, 142–143, 151, 170, 174, 177, 181, 187, 189, 306 Abbott. See meteorite Alais. See meteorite Abee. See meteorite Albareto. See meteorite Acapulco. See meteorite Albin. See meteorite acapulcoites, 107, 173, 179, 291, 303, Al-Biruni, 3 309, 314 albite, 68, 70, 72, 76, 78, 87, 92, 98, 136–137, 139, accretion, 238, 260, 292, 347, 365 144, 152, 155, 157–158, 162, 171, 175, 177–178, acetylene, 230 189–190, 200, 205–206, 226, 243, 255–257, 261, Acfer 059. See meteorite 272, 279, 295, 306, 309, 347 Acfer 094. See meteorite albite twinning, 68 Acfer 097. See meteorite Aldrin, Buzz, 330 achondrites, 101, 106–108, 150, 171, 175, 178–179, Aletai. See meteorite 182, 226, 253, 283, 291, 294, 303, 309–310, 318, ALH 77307. See meteorite 350, 368, 374 ALH 78091. See meteorite acute bisectrix, 90 ALH 78113. See meteorite adamite, 83 ALH 81005. See meteorite addibischoffite, 116, 167 ALH 82130. See meteorite Adelaide. See meteorite ALH 83009. See meteorite Adhi Kot. See meteorite ALH 83014. See meteorite Admire. See meteorite ALH 83015. See meteorite adrianite, 117, 134, 167, 268 ALH 83108. See meteorite aerogel, 234 ALH 84001. See meteorite Aeschylus, 6 ALH 84028. See meteorite agate, 2 ALH 85085. See meteorite AGB stars. See asymptotic giant branch stars ALH 85151. See meteorite agglutinate, 201, 212, 224, 279, 301–302, 308 ALHA76004. See meteorite Agpalilik. See Cape York ALHA77005. -
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THn AMERrclr.l M rNERALocrsr JOURNAL OF THE MINERALOGICAI SOCIETY OF AMERICA Vol. 52 MARCH_APRIL, 1961 Nos. 3 and 4 EXTRATERRESTRIAL MINERALOGY1 Bnrarq Masow, U. S. National Museum, Washington,D. C. In looking over the list of my illustrious predecessorsin the position of president of this society, I am intrigued to see that only two were museum curators (although some were university professorswho were also curators of extensive collections). The last curator to stand in my present shoeswas William F. Foshag in 1940, and his presidential ad- dress was entitled "Problems in the study of meteorites." Coming from the same institution, I feel it is not inappropriate to follow his good ex- ample, and to provide you with some account of the recent progress of meterorite mineralogy. Although the obvious minerals of meterorites were recognized quite early, the study of the most abundant (and mineralogically complex) meteorites, the chondrites, was not possibleuntil the introduction of the polarizing microscopeabout 100 years ago. The techniquesof microscopic petrology were applied to stony meteorites originally by Sorby, who published a paper on this subject in 1863. The fortunate conjunction of a first-rate microscopist, Gustav Tschermak, and the outstanding mete- orite collection of that day, the Vienna collection, resulted in a classic monograph on the mineralogy and petrology of meteorites, Tschermak,s "Die mikroskopischeBeschaffenheit der Meteoriten," publishedin 1885. This remarkable work, long unavailable except in a few libraries, was recently republished, in facsimile, with an English translation by Wood (1964).In it Tschermakrecognized sixteen minerals occurring in meteor- ites. Table 1 traces the development of meteorite mineralogy over the following seventy years. -
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Report of the Secretary and Financial Report of the Executive Committee of the Board of Regents Smithsonian Institution Report of the Secretary and Financial Report of the Executive Committee of the Board of Regents For the year ended June 30 1960 Smithsonian Publication 4429 U.S. GOVERNMENT PRINTING OFFICE WASHINGTON : 1960 CONTENTS Page List of officials v General statement 1 The Establishment 6 The Board of Regents q Finances 7 Visitors 7 Reports of branches of the Institution: United States National Museum 9 Bureau of American Ethnology 48 Astrophysical Observatory 83 National Collection of Fine Arts 97 Freer Gallery of Art 106 National Air Museum 119 National Zoological Park 131 Canal Zone Biological Area 172 International Exchange Service 177 National Gallery of Art 186 Report on the library 199 Report on publications 202 Other activities: Lectures 211 Bio-Sciences Information Exchange 211 Smithsonian Museum Service 212 Report of the executive committee of the Board of Regents 214 in THE SMITHSONIAN INSTITUTION June 30, 1960 Presiding Officer ex officio.—Dwight D. Eisenhower, President of the United States. Chancellor.—Eael Wabben, Chief Justice of the United States. Members of the Institution: Dwight D. Eisenhowee, President of the United States. RiCHAED M. Nixon, Vice President of the United States. Earl Wareen, Chief Justice of the United States. Christian A. Heeter, Secretary of State. RoBEET B. Andebson, Secretary of the Treasury. Thomas S. Gates, Je., Secretary of Defense. William P. Rogees, Attorney General. Abthtje E. Summebpield, Postmaster General. Feed A. Seaton, Secretary of the Interior. EzBA Taft Benson, Secretary of Agriculture. Feedeeick H. Mueller, Secretary of Commerqe. -
Editorial for Special Issue “Mineralogy of Meteorites”
minerals Editorial Editorial for Special Issue “Mineralogy of Meteorites” Victor V. Sharygin 1,2 1 V.S. Sobolev Institute of Geology and Mineralogy, Siberian Branch of the RAS, 3 Acad. Koptyuga pr., 630090 Novosibirsk, Russia; [email protected]; Tel.: +7-383-330-80-84 2 ExtraTerra Consortium, Institute of Physics and Technology, Ural Federal University, 19 Mira str., 620002 Ekaterinburg, Russia Over 435 mineral species have been found in different types of meteorites (updated list for 2016) [1]. Classification of meteorites is based on their mineralogy and petrography, bulk-rock chemical and O-isotopic compositions, as well as the chemical composition of the main minerals [2–8]. For example, compositions in endmembers for olivine and low-Ca pyroxene and microstructural features of minerals are the powerful instruments for classification of ordinary chondrites (determination of the chemical group and petrologic type) [4–8]. In general, the individual minerals and mineral associations may record the history of meteorites (and their parental bodies) before and after their landing on the Earth. Rubin and Ma [1] outlined the basic processes responsible for mineral formation in meteorites: condensation from gaseous media around evolved stars and in the solar nebula; crystallization in chondrule, CAI (calcium-aluminium-rich inclusions), and AOA (amoeboid olivine aggregates) melts; exsolution during the cooling of CAIs, chondrules, and opaque assemblages; rapid quenching of amorphous phases; thermal and shock meta- morphism; aqueous/hydrothermal alteration and metasomatism; condensation during impact events; crystallization of melts in parental bodies; condensation from residual fluid in differentiated bodies; post-solidus transformations within cooling igneous materials; heating and remelting near perihelion; melting during atmospheric entrance; and terrestrial replacements. -
Planetesimal Differentiation and Impact Mineralization
This is the peer-reviewed, final accepted version for American Mineralogist, published by the Mineralogical Society of America. The published version is subject to change. Cite as Authors (Year) Title. American Mineralogist, in press. DOI: https://doi.org/10.2138/am-2021-7632. http://www.minsocam.org/ 1 #7632—REVISION #2—03 August 2020—submitted to American Mineralogist 2 3 An evolutionary system of mineralogy, Part IV: Planetesimal 4 differentiation and impact mineralization (4566 to 4560 Ma) 1 1,* 5 SHAUNNA M. MORRISON AND ROBERT M. HAZEN 1 6 Earth and Planets Laboratory, Carnegie Institution for Science, 7 5251 Broad Branch Road NW, Washington D.C. 20015, U. S. A. 8 ABSTRACT 9 The fourth installment of the evolutionary system of mineralogy considers two stages of 10 planetesimal mineralogy that occurred early in the history of the solar nebula, commencing by 11 4.566 Ga and lasting for at least 5 million years: (1) primary igneous minerals derived from 12 planetesimal melting and differentiation into core, mantle, and basaltic components; and (2) 13 impact mineralization resulting in shock-induced deformation, brecciation, melting, and high- 14 pressure phase transformations. 15 We tabulate 90 igneous differentiated asteroidal minerals, including the earliest known 16 occurrences of minerals with Ba, Cl, Cu, F, and V as essential elements, as well as the first 17 appearances of numerous phosphates, quartz, zircon, and amphibole group minerals. We also 18 record 40 minerals formed through high-pressure impact alteration, commencing with the period 19 of asteroid accretion and differentiation. These stages of mineral evolution thus mark the first 20 time that high pressures, both static and dynamic, played a significant role in mineral 21 paragenesis. -
The Wedderburn Meteorite Revisited
CSIRO Publishing The Royal Society of Victoria, 131, 74–83, 2019 www.publish.csiro.au/journals/rs 10.1071/RS19010 THE WEDDERBURN METEORITE REVISITED WILLIAM D. BIRCH Geosciences, Museums Victoria, GPO Box 666, Melbourne, Victoria 3001, Australia Correspondence: Bill Birch, [email protected] ABSTRACT: The Wedderburn meteorite from Victoria is a small nickel-rich iron belonging to the rare sLH subgroup of the IAB complex. Donated to the Mines Department in 1950, it came to public attention in 1953 when the initial description was published by Dr Austin Edwards in the Proceedings of the Royal Society of Victoria. Since then, pieces of the meteorite have been distributed to major institutions in Europe and North America, where leading researchers have investigated the meteorite’s unusual chemistry, mineralogy and microtexture in great detail. The recent approval of a new iron carbide mineral named edscottite, with the formula Fe5C2, in Wedderburn has prompted this review of the meteorite’s history, from its discovery to its current classification status. Keywords: Wedderburn, meteorite, sLH subgroup, iron carbides, edscottite, history INTRODUCTION was Charles Frederick Bell, a well-known local miner and prospector, who spent his entire life from 1889 until 1965 The Wedderburn meteorite is one of 18 recorded meteorites in the Rushworth district. Wedderburn is some 140 km from Victoria (Henry 2003; Birch et al. 2019) and one west of Rushworth, so Mr Bell must have prospected over of five that are broadly categorised as irons (the others a wide area. Although the description of the find site is are Cranbourne, Lismore, Willow Grove and Ballarat). -
Australian Meteorites
R.O. Chaimers, Commemorative Papers (Mineralogy, Meteoritics, Geology) Edited by Lin Sutherland Australian meteorites ................................................................................. A. W.R. Bevan Composition ofpyromorphites from Broken Hill, New South Wales ............ Adedayo I. Inegbenebor, Peter A. Williams, Richard E. Bevins, Michael P. Lambert & Alan D. Hart Auriferous limonitic stalactites from the Bimbimbie gold mine, New South Wales ........ .. ........ ...... ............................ ..... .......... ..................... .............. .................... L.J. Lawrence Possible origins and ages for sapphire and diamond from the central Queensland gem fields ...................................................................... A.D.C. Robertson & F.L. Sutherland Zeolites from a new locality at Ben Lomond, New England region, New South Wales ........................................................................................................... Brian M. England 55 Laumontite and heulandite-clinoptilolite pseudomorphous after Jurassic gastropods from Ponganui, New Zealand ...................................................... K.A. Rodgers & N. Hudson 73 From Pleistocene to Present: obsidian sources in West New Britain, Papua New Guinea .............................................................. R. Torrence, J. Specht, R. Fullagar & R. Bird 83 Samuel Stutchbury and the Australian Museum ........................................... D. Branagan 9.) Minerals in the Australian Museum - 1901 to 1945 ................................ -
Notes on Australian Meteorites
AUSTRALIAN MUSEUM SCIENTIFIC PUBLICATIONS Mason, B., 1974. Notes on Australian meteorites. Records of the Australian Museum 29(5): 169–186, plates 6–7. [15 May 1974]. doi:10.3853/j.0067-1975.29.1974.228 ISSN 0067-1975 Published by the Australian Museum, Sydney naturenature cultureculture discover discover AustralianAustralian Museum Museum science science is is freely freely accessible accessible online online at at www.australianmuseum.net.au/publications/www.australianmuseum.net.au/publications/ 66 CollegeCollege Street,Street, SydneySydney NSWNSW 2010,2010, AustraliaAustralia NOTES ON AUSTRALIAN METEORITES By BRIAN MASON Smithsonian Institution, Washington, D.C., U.S.A. Plates 6 and 7. Figures 1 and 2. Manuscript received 3rd June, 1973. ABSTRACT A reVIew of Australian meteorites, eliminating paired falls, gives a total of 184, compnsmg 67 irons, 9 stony-irons, and 108 stones (6 anchondrites and 102 chondrites); 10 of these were observed falls. Olivine and pyroxene compositions have been determined by microprobe analysis for most of the chondrites, and they have been examined microscopically and classified according to the Van Schmus Wood classification. Additional data on mineral compositions are given for the enstatite achondrite Mt Egerton and the ureilites North Haig and Dingo Pup Donga; a bulk analysis of a small sample of the eucrite Emmaville has been made. Ringwoodite and majorite are recorded from the Coolamon meteorite, the third occurrence of these meteorite minerals. A list of Australian irons and stony-irons, giving Ni and Ge contents, structural type, and Ge-Ga class has been compiled, and the Ni-Ge data presented in a diagram. INTRODUCTION Research on Australian meteorites may perhaps be dated from 1861, the year in which Haidinger published the first account of the Cranbourne irons. -
Annual Report for the Year Ended June 30, 1959
Q 11 U52Z FISH United States 1960 ANNUAL REPORT The United States National Museum Annual Report for the Year Ended June 30, 1960 SMITHSONIAN INSTITUTION United States Xatioxal Museum. UxDER Direction of the Smithsoxiax Institution. Washincjton. D.C.. August 15. 1960. Sir; I have the honor to submit herewith a report upon the present condition of the United States Xational Museum and upon the work accomphshed in its various departments during; the fiscal year ended Jime 30. 1960. Very respectfully, Remington Kellogg. Director. U.S. Xational Museum. Dr. Leonard Carmichael, Secretary, Smithsonian Institution, n Contents Page Introduction 1 Exhibits 8 Accessions 30 Care of Collections 43 Investigation and Research 52 Anthropology 52 Zoology 57 Botany 70 Geology 74 Science and Technology 82 Arts and Manufactures 84 Civil History 90 Armed Forces History 93 Publications 96 Donors to the National Collections 108 III June 30, 1960 United States National Museum Director: Remington Kellogg Registrar: Helena M. Weiss Museum of Natural History Director: Albert C. Smith Department of Anthropology: Frank M. Setzler, head curator A. Joseph Andrews, exhibits specialist Archeology: Waldo R. Wedel, curator Eugene I. Knez, associate curator Clifford Evans, Jr., associate curator Robert A. Elder, Jr., assistant curator Gus W. Van Beek, associate curator Physical Anthropology: T. Dale Ethnology: Saul H. Riesenberg, cura- Stewart, curator tor Marshall T. Newman, associate cura- Gordon D. Gibson, associate curator tor Department of Zoology: Herbert Friedmann, head curator Mammals: David H. Johnson, curator Ralph E. Crabill, Jr., associate curator Henry W. Setzer, associate curator William D. Field, associate curator Charles O. Handley, Jr., associate Sophy Parfin, assistant curator curator Marine Invertebrates: Fenner A. -
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.