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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. -
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. -
From the Lingyan Temple, Changqing, Shandong, China
Technical Study of Polychrome Arhat Figures Dated From the Song Dynasty(960-1279 CE) From the Lingyan Temple, Changqing, Shandong, China Yongdong Tong University of Science and Technology Beijing Youzhen Cai Shandong Cultural Relic Conservation and Restoration Center Xuening Wang Shandong Cultural Relic Conservation and Restoration Center Zhimin Li Shandong University Austin Nevin Courtauld Institute of Art: The Courtauld Institute of Art Qinglin Ma ( [email protected] ) Shandong University https://orcid.org/0000-0002-5542-2388 Research Article Keywords: Lingyan Temple, Arhat statues, paint layers, scientic analysis Posted Date: June 30th, 2021 DOI: https://doi.org/10.21203/rs.3.rs-662279/v1 License: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License Page 1/29 Abstract Scientic analysis revealed the materials and techniques used in the process of making the polychrome sculptures providing a solid foundation for the protection and restoration of the painted statues. In addition analysis revealed changes in colour schemes applied to the sculptures can provide the basis for the virtual restoration of the painted statues. In order carry out scientically-informed protection and restoration of the Bodhidharma statue from the Lingyan Temple, Changqinq, Shandong, several analytical methods such as optical microscope (OM), Micro-Raman spectroscopy (μ-RS), scanning electron microscopy coupled with energy dispersive X-ray analysis (SEM-EDS) and Fourier transform infrared spectroscopy (FTIR) were employed. Analysis clearly reveal the information including the stratigraphic structure and the composition of pigment. The use of silver foils and golden yellow pyrophyllite mineral to replace gold foils were found in the gilding paint layer in the later repainting after the Song Dynasty. -
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 -
New Mineral Names*
American Mineralogist, Volume 95, pages 204–208, 2010 New Mineral Names* PAULA C. PIILONEN † AND GLENN POIRIER Mineral Sciences Division, Canadian Museum of Nature, P.O. Box 3443, Station D, Ottawa, Ontario K1P 6P4, Canada NEW MINERALS ing features: broad absorption maxima at 3586, 3555, 3414, 3223, and 3104 cm–1 are attributed to OH stretching and absorption at 1619 cm–1 is attributed to H-O-H bending. Overlapping bands BRAITH W AITEITE * attributed to As-O stretching are observed at 865, 843, and 812 –1 –1 W.H. Parr, M.A. Cooper, F.C. Hawthorne, E. Moffat, M.E. cm ; weak absorption bands at 2338 cm are assigned to ν(O-H) –1 Gunther, A.C. Roberts, and P.J. Dunn (2009) Braithwaiteite, stretching and bands at 1189 and 1156 cm are possibly O-H in-plane banding. NaCu5(TiSb)O2(AsO4)4[AsO3(OH)]2(H2O)8, a new mineral species from Laurani, Bolivia, Can. Mineral., 47, 947–953. A powder X-ray diffraction pattern was obtained using CuKα F.C. Hawthorne, M.A. Cooper, and W.H. Parr (2008) The crystal radiation and a Debye-Scherrer camera. The strongest seven structure of braithwaiteite. J. Coord. Chem., 61, 15–29. lines in the pattern are [dhkl in Å(Iobs%,hkl)] 9.825(100,001), 5.887(50,011), 4.635(30,102), 3.354(30,122), 3.232(30,2 11), Braithwaiteite was discovered as several small crystals in a 2.947(60,022), 2.736(30,2 22). The crystal structure was de- sample of silicified volcanic rock from Laurani in the Bolivian termined using direct methods with a R1 of 0.025 for 3584 Ag-Sn belt. -
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. -
Of Chemistry
,\1l.'Jl~N(,'() SOUTHERN BRAZILIAN JOURNAL OF CHEMISTRY ISSN 0104-5431 \N l'T~ R'.' \ rl0"'1AL FOf{l \1 FOi{ TllE RAPID Pl HL.I< \ 1'10~ <H 01{1<~1'\ \I SCIF~TIFI< \Rl'ICLES Df Al.l:\C \\ ITll CIU \-llS IR\ \'.'.I> Rl-J ..\ TTD 11' I .. ,ROIS( IPLl"i:\R\ -\R ... .\S \ <) L l ' '\ 1 E ~ I N E ,r E E N Of.('~,;\1BER 2011 EDITOR LA VINEL G. IONESCU, SCIENCO, Consultoria Cientifka, Viamao, RS, BRA.SIL ASSISTANT EDITOR LUIS ALCIDES BRANDINI DE BONI, Tchequimica LTDA, Porto Alegre, RS. Brasil. EDITORIAL BOARD FARUK NOME AGUILERA, Departamento de Quimica, Universidade FederaJ de Santa Catarina, Florian6polis, SC, Brasil D. BALASUBRAMANIAN, Centre for Cellular and Molecular Biology, Hyderabad, INDIA HECTOR E. BERTORELLO, Departamento de Quimica Organica, Facultad de Ciencias Quimicas, Universidad Nacional de Cordoba, Cordoba, ARGENTINA AECIO P. CHAGAS, Instituto de Quimica, UNICAMP, Campinas, SP, BRASIL JUAN JOSE COSA, Departamento de Quimica y Fisica, Facultad de Ciencias Exactas. Universidad Nacional de Rio Cuarto, Rio Cuarto, ARGENTINA GLENN A. CROSBY, Department of Chemistry, Washington State University, Pullman, WA, USA VITTORIO DEGIORGIO, Dipartimento di Elettronica, Sezione di Fisica Applicata, Universita di Pavia, Pavia IT ALIA JOSE C. TEIXEIRA DIAS, Departamento de Quimica, Universidade de Coimbra, Coimbra, PORTUGAL OMAR A. EL SEOUD, Instituto de Quimica, Universidade de Sao Paulo, Sao Paulo, SP, BRASIL FERNANDO GALEMBECK, Instituto de Quimica, UNICAMP, Campinas, SP, BRASIL NISSIM GARTI, Casali Institute of Applied Science, Hebrew University of Jerusalem, Jerusalem, ISRAEL GASPAR GONZALEZ, Centro de Pesquisa, CENPES-PETROBRAS, Ilha do Fundao, Rio de Janeiro, RJ , BRASIL YOSHITAKA GUSHIKEM, Instituto de Quimica, UNICAMP, Campinas, SP, BRASIL WILLIAM HASE, Department of Chemistry, Texas Tech University, Lubbock, Texas, USA I. -
Minerals Localities
MINERALS and their LOCALITIES This book is respectfully dedicated to the memory of Dr. John Sinkankas for his kind initiative and support to publish this book in English version. MINERALS and their LOCALITIES Jan H. Bernard and Jaroslav Hyršl Edited by Vandall T. King © 2004 by Granit, s.r.o. © 2004 Text by Jan H. Bernard and Jaroslav Hyršl © 2004 Photos by Jaroslav Hyršl (463), Studio Granit (534), Jaromír Tvrdý (34), Petr Zajíček (4) The photographed specimens are from the collections of both authors as well as from many other collections. The autors are grateful to all institutions and persons who allowed to photograph their specimens for this book. Front cover photos: Turquoise, polished, 55 mm, Zhilandy, Kazakhstan, G Galena, 45 mm, Madan, Bulgaria, G Sphalerite, xx 12 mm, Morococha, Peru, H Gypsum, xx 40 mm, Las Salinas, Peru, H Variscite, xx 5 mm, Itumbiara, Brazil, H Rhodochrosite, polished, 50 mm, Capillitas, Argentina, H Back cover photo: Wolframite, 45 mm, Yaogangxian, China, H Page 1: Muscovite, 45 mm, Linopolis, Brazil, H Page 2: Vivianite, 100 mm, Huanzala, Bolivia, H Page 3: Liddicoatite, polished, 70 mm, Anjanabonoina, Madagaskar, G Page 5: Opal - fire, polished, 50 mm, Mezezo, Ethiopia, G Page 12: Brazilianite, 35 mm, Linopolis, Brazil, H Page 13: Gold, 35 mm, Eagle's Nest Mine, California, G Published by Granit, s.r.o. Štefánikova 43, 150 00 Praha 5, Czech Republic e-mail: [email protected] www.granit-publishing.cz Composition and reproduction by Studio VVG, Prague Printed in Czech Republic by Finidr, s.r.o., Český Těšín 14/02/03/01 All rights reserved. -
LEMANSKIITE, Nacacu5(Aso4)4Cl•5H2O, a NEW MINERAL SPECIES from the ABUNDANCIA MINE, CHILE
523 The Canadian Mineralogist Vol. 44, pp. 523-531 (2006) LEMANSKIITE, NaCaCu5(AsO4)4Cl•5H2O, A NEW MINERAL SPECIES FROM THE ABUNDANCIA MINE, CHILE PETR ONDRUŠ AND FRANTIˇSEK VESELOVSKY´ Czech Geological Survey, Geologická 6, CZ-15200 Prague, Czech Republic ROMAN SKÁLA§ Institute of Geology, Academy of Sciences of the Czech Republic, Rozvojová 269, CZ-16500 Praha 6 – Lysolaje, Czech Republic JIˇRÍ SEJKORA National Museum, Václavské nám. 68, CZ-11579 Prague 1, Czech Republic RICHARD PAŽOUT U pruhonu˚ 42, CZ-17000 Prague 7, Czech Republic JIˇRÍ FRYDA´ AND ANANDA GABAŠOVÁ Czech Geological Survey, Geologická 6, CZ-15200 Prague, Czech Republic JOSEF VAJDAK Pequa Rare Minerals, 342 Forest Avenue, Massapequa, New York 11758-5707, USA ABSTRACT Lemanskiite, ideally NaCaCu5(AsO4)4Cl•5H2O, is a new mineral species from the Abundancia mine, El Guanaco mining district, Chile. It is dimorphous with lavendulan and represents the Ca-analogue of zdenekite. It occurs as rosette-shaped aggre- gates (up to 5 mm) of thin lamellar, subparallel, strongly bent intergrowths (0.3 mm 10 m) or needle-shaped aggregates of 0.8 mm length and 10 m in thickness. Individual thin tabular crystals (up to 4 mm in length) are invariably bent. It is associated with lammerite, olivenite, mansfi eldite, senarmontite, a mineral of the crandallite group, rutile, anatase, and talc. Lemanskiite is dark sky blue, translucent, nonfl uorescent with a light blue streak. It is brittle with an excellent cleavage parallel to (001); its luster is vitreous, and its Mohs hardness is ~2½. The mineral displays no parting, and its fracture is uneven. It is optically negative, uniaxial, with indices = 1.647(2) and = 1.749(2); its birefrigence is 0.102, and the pleochroism is very strong.