Sulfosalt Melts and Heavy Metal
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Interpretation of Exploration Geochemical Data for the Mount Katmai Quadrangle and Adjacent Parts of the Afognak and Naknek Quadrangles, Alaska
Interpretation of Exploration Geochemical Data for the Mount Katmai Quadrangle and Adjacent Parts of the Afognak and Naknek Quadrangles, Alaska By S.E. Church, J.R. Riehle, and R.J. Goldfarb U.S. GEOLOGICAL SURVEY BULLETIN 2020 Descriptive and interpretive supporting data for the mineral resource assessn~entof this Alaska Mineral Resource Assessnzent Program (AMRAP) study area UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON : 1994 U.S. DEPARTMENT OF THE INTERIOR BRUCE BABBITT, Secretary U.S. GEOLOGICAL SURVEY Gordon P. Eaton, Director For Sale by U.S. Geological Survey, Map Distribution Box 25286, MS 306, Federal Center Denver, CO 80225 Any use of trade, product, or firm names in this publication is for descriptive purposes only and does not imply endorsement by the U.S. Government. Library of Congress Cataloging-in-PublieatlonData Church, S.E. Interpretation of exploration geochemical data for the Mount Katmai quadrangle and adjacent parts of the Afognak and Nalrnek quadrangles, Alaska 1 by S.E. Church, J.R. Riehle, and R.J. Goldfarb. p. cm. - (U.S. Geological Survey bulletin ;2020) Includes bibliographical references. Supt. of Docs. no. : 119.3 :2020 1. Mines and mineral resources-Alaska. 2. Mining gedogy- Alaska 3. Geochemical prospecting-Alaska I. Riehle, J.R. 11. Goldfarb, R.J. UI. Title. IV. Series. QE75.B9 no. 2020 [TN24.A4] 557.3 5420 93-2012 [553'.09798] CIP CONTENTS Abstract ............................................................................................................................. Introduction...................................................................................................................... -
A Single-Crystal Epr Study of Radiation-Induced Defects
A SINGLE-CRYSTAL EPR STUDY OF RADIATION-INDUCED DEFECTS IN SELECTED SILICATES A Thesis Submitted to the College of Graduate Studies and Research In Partial Fulfillment of the Requirements For the Degree of Doctor of Philosophy In the Department of Geological Sciences University of Saskatchewan Saskatoon By Mao Mao Copyright Mao Mao, October, 2012. All rights reserved. Permission to Use In presenting this thesis in partial fulfilment of the requirements for a Doctor of Philosophy degree from the University of Saskatchewan, I agree that the Libraries of this University may make it freely available for inspection. I further agree that permission for copying of this thesis in any manner, in whole or in part, for scholarly purposes may be granted by the professor or professors who supervised my thesis work or, in their absence, by the Head of the Department or the Dean of the College in which my thesis work was done. It is understood that any copying or publication or use of this thesis or parts thereof for financial gain shall not be allowed without my written permission. It is also understood that due recognition shall be given to me and to the University of Saskatchewan in any scholarly use which may be made of any material in my thesis. Requests for permission to copy or to make other use of material in this thesis in whole or part should be addressed to: Head of the Department of Geological Sciences 114 Science Place University of Saskatchewan Saskatoon, Saskatchewan S7N5E2, Canada i Abstract This thesis presents a series of single-crystal electron paramagnetic resonance (EPR) studies on radiation-induced defects in selected silicate minerals, including apophyllites, prehnite, and hemimorphite, not only providing new insights to mechanisms of radiation-induced damage in minerals but also having direct relevance to remediation of heavy metalloid contamination and nuclear waste disposal. -
ABSTRACTS ACTAS IAGOD 2019 31Ene.Pmd
SALTA, ARGENTINA 28-31 AUGUST 2018 15th Quadrennial International Association on the Genesis of Ore Deposits Symposium SPONSORS PLATINUM SPONSORS GOLD SPONSORS SILVER SPONSORS BRONZE SPONSORS COPPER SPONSORS Co-sponsored by SALTA, ARGENTINA 28-31 AUGUST 2018 15th Quadrennial International Association on the Genesis of Ore Deposits Symposium SYMPOSIUM PROCEEDINGS SCIENTIFIC COMMITTEE CHAIR Lira Raúl – (University of Córdoba – CONICET, Argentina) MEMBERS Bineli-Betsi Thierry – (Botswana International University of Science and Technology) Chang Zhaoshan – (Colorado School of Mines, USA) Cherkasov Sergey – (Vernadsky State Geological Museum of Russian Academy of Sciences) Cook Nigel – (University of Adelaide, Australia) Gozalvez Martín – (Geological and Mining Survey of Argentina) Guido Diego – (CONICET/Austral Gold S.A, Argentina) Lentz David – (University of New Brunswick, Economic Geology Chair) López Luis – (National Atomic Energy Commission, Argentina) Mao Jingwen – (Chinese Academy of Geological Sciences/Hebei GEO University, China) Meinert Larry – (Consultant) Pons Josefina – (IIPG – University of Río Negro – University of Comahue – CONICET, Argentina) Rubinstein Nora – (IGEBa–University of Buenos Aires – CONICET) Sanematsu Kenzo – (Geological Survey of Japan, AIST) Schutesky Della Giustina Maria Emilia – (University of Brasília, Brasil) Tornos Fernando – (Spanish National Research Council – CSIC) Watanabe Yasushi – (Faculty of International Resource Sciences, Akita University, Japan) EDITED BY Daniel Rastelli, Dolores Álvarez, Noelia -
Solution Deposition of a Bournonite Cupbsbs3 Semiconductor Thin Film from the Dissolution of Bulk Materials with a Thiol-Amine Sol- Vent Mixture Kristopher M
Solution Deposition of a Bournonite CuPbSbS3 Semiconductor Thin Film from the Dissolution of Bulk Materials with a Thiol-Amine Sol- vent Mixture Kristopher M. Koskela, Brent C. Melot, and Richard L. Brutchey* Department of Chemistry, University of Southern California, Los Angeles, CA 90089, United States ABSTRACT: There is considerable interest in the exploration of new solar absorbers that are environmentally stable, absorb through the visible, and possess a polar crystal structure. Bournonite CuPbSbS3 is a naturally occurring sulfosalt mineral that crys- tallizes in the non-centrosymmetric Pmn21 space group and possesses an optimal band gap for single junction solar cells; however, the synthetic literature on this quaternary semiconductor is sparse and it has yet to be deposited and studied as a thin film. Here we describe the ability of a binary thiol-amine solvent mixture to dissolve the bulk bournonite mineral as well as inexpensive bulk CuO, PbO, and Sb2S3 precursors at room temperature and ambient pressure to generate an ink. The synthetic compound ink derived from the dissolution of the bulk binary precursors in the right stoichiometric ratios yields phase-pure thin films of CuPbSbS3 upon solution deposition and annealing. The resulting semiconductor thin films possess a direct optical band gap of 1.24 eV, an absorp- tion coefficient ~105 cm–1 through the visible, mobilities of 0.01-2.4 cm2 (V•s)–1, and carrier concentrations of 1018 – 1020 cm–3. These favorable optoelectronic properties suggest CuPbSbS3 thin films are excellent -
Ralphcannonite, Agzn2tlas2s6, a New Mineral of the Routhierite
1 1 Ralphcannonite, AgZn2TlAs2S6, a new mineral of the 2 routhierite isotypic series from Lengenbach, Binn 3 Valley, Switzerland 4 1* 2 3 5 LUCA BINDI , CRISTIAN BIAGIONI , THOMAS RABER , PHILIPPE 4 5 6 ROTH , FABRIZIO NESTOLA 7 8 9 10 1 Dipartimento di Scienze della Terra, Università degli Studi di Firenze, Via G. La Pira, 4, I- 11 50121 Firenze, Italy 12 2 Dipartimento di Scienze della Terra, Università di Pisa, Via Santa Maria, 53, I-56126 Pisa, 13 Italy 14 3 FGL (Forschungsgemeinschaft Lengenbach), Edith-Stein-Str. 9, D-79110 Freiburg, 15 Germany 16 4 FGL (Forschungsgemeinschaft Lengenbach), Ilanzhofweg 2, CH-8057 Zurich, Switzerland 17 5 Dipartimento di Geoscienze, Università di Padova, Via Gradenigo, 6, I-35131 Padova, Italy 18 19 20 21 22 *e-mail address: [email protected] 23 2 24 ABSTRACT 25 The new mineral species ralphcannonite, AgZn2TlAs2S6, was discovered in the Lengenbach 26 quarry, Binn Valley, Wallis, Switzerland. It occurs as metallic black equant, isometric to 27 prismatic crystals, up to 50 μm, associated with dufrénoysite, hatchite, realgar, and baryte. 28 Minimum and maximum reflectance data for COM wavelengths in air are [λ (nm): R (%)]: 29 471.1: 25.8/27.1; 548.3: 25.2/26.6; 586.6: 24.6/25.8; 652.3: 23.9/24.8. Electron microprobe 30 analyses give (wt%): Cu 2.01(6), Ag 8.50(16), Zn 10.94(20), Fe 3.25(8), Hg 7.92(12), Tl 31 24.58(26), As 18.36(19), Sb 0.17(4), S 24.03(21), total 99.76(71). -
Valid Unnamed Minerals, Update 2012-01
VALID UNNAMED MINERALS, UPDATE 2012-01 IMA Subcommittee on Unnamed Minerals: Jim Ferraiolo*, Jeffrey de Fourestier**, Dorian Smith*** (Chairman) *[email protected] **[email protected] ***[email protected] Users making reference to this compilation should refer to the primary source (Dorian G.W. Smith & Ernest H. Nickel (2007): A System of Codification for Unnamed Minerals: Report of the SubCommittee for Unnamed Minerals of the IMA Commission on New Minerals, Nomenclature and Classification. Canadian Mineralogist v. 45, p.983-1055), and to this website . Additions and changes to the original publication are shown in blue print; deletions are "greyed out and struck through". IMA Code Primary Reference Secondary Comments Reference UM1886-01-OC:HNNa *Bull. Soc. Minéral. 9 , 51 Dana (7th) 2 , 1104 Probably an oxalate but if not is otherwise similar to lecontite UM1892-01-F:CaY *Am. J. Sci. 44 , 386 Dana (7th) 2 , 37 Low analytical total because F not reported; unlike any other known fluoride 3+ UM1910-01-PO:CaFeMg US Geol. Surv. Bull. 419, 1 Am. Mineral. 34 , 513 (Ca,Fe,Mg)Fe 2(PO4)2(OH)2•2H2O; some similarities to mitridatite UM1913-01-AsO:CaCuV *Am. J. Sci. 35 , 441 Dana (7th) 2 , 818 Possibly As-bearing calciovolborthite UM1922-01-O:CuHUV *Izv. Ross. Akad. Nauk [6], 16 , 505 Dana (7th) 2 , 1048 Some similarities to sengierite 3+ UM1926-01-O:HNbTaTiU *Bol. Inst. Brasil Sc., 2 , 56 Dana (7th) 1 , 807 (Y,Er,U,Th,Fe )3(Ti,Nb,Ta)10O26; some similarities to samarskite-(Y) UM1927-01-O:CaTaTiW *Gornyi Zhurn. -
Mercury's Hollows: Chalcogenide Pyro
44th Lunar and Planetary Science Conference (2013) 2840.pdf MERCURY’S HOLLOWS: CHALCOGENIDE PYRO-THERMOKARST ANALOG OF THERMOKARST ON EARTH, MARS, AND TITAN. J.S. Kargel1 1Department of Hydrology and Water Resources, University of Arizona, Tucson, AZ 85721, USA ([email protected]). Introduction/Summary: MESSENGER has ac- quired stunning images of pitted, light-toned or varie- gated light/dark terrains located primarily on many of Mercury’s crater floors (Fig. 1) and on some ejecta blankets. Termed “hollows” by the imaging team, the pits have been described as unique in the Solar System. However, these terrains are geomorphologically simi- lar to some on Mars formed by sublimation of ice-rich permafrost (Fig. 2) and to lowland thermokarst on Earth formed by permafrost thaw; to “swiss cheese” terrain forming by sublimation of frozen CO2 at the Martian South Pole (Fig. 3); and to terrain at Titan’s poles thought to be hydrocarbon thermokarst (Fig. 4). Mercury lacks eolian processes that could erode the pits, and the pits do not possess volcanic characteris- tics. The most plausible explanation for Mercury’s hollows is terrain degradation involving melting or sublimation of heterogeneous chalcogenide and sul- fosalt mineral assemblages. Adapting the term ther- mokarst, I refer to these Mercurian features as pyro- thermokarst; the etymological redundancy distin- guishes the conditions and mineral agents from the ice- related features on Earth and Mars, though some of the physical processes may be similar. Working Hypothesis: Whereas ice has been long suspected and recently was discovered in permanently shadowed craters of Mercury’s polar regions, the hol- lows occur down to the equator, where neither ice nor sulfur is plausible. -
Memorial of Daniel E. Appleman 1931–1998
American Mineralogist, Volume 83, pages 1133±1135, 1998 Memorial of Daniel E. Appleman 1931±1998 MALCOLM ROSS1,* AND JEFFREY E. POST2 1Scientist Emeritus, U.S. Geological Survey, Reston, Virginia 20192, U.S.A. 2Smithsonian Institution, Department of Mineral Sciences, NHB 119, Washington, D.C. 20560, U.S.A. Daniel Appleman, a long-time member and fellow of the MSA, passed away on Friday, January 2, 1998, after a courageous year-long ®ght with cancer. Thus ended an extraordinary lifeÐa life devoted to the mineralogical sciences, museum directorship, public service, the arts, and most importantly to his beloved wife, Peggy, and his daughter, Rebecca. Dan became a fellow of the Miner- alogical Society of America in 1955 and has served our society in many capacities for over forty years. His re- search, management, and curatorial skills were very in- ¯uential in furthering the scienti®c and educational pro- grams of three major institutionsÐthe U.S. Geological Survey in Reston, Virginia, the National Museum of Nat- ural History (NMNH) in Washington, D.C., and the Cran- brook Institute of Science in Bloom®eld Hills, Michigan. For his contributions to public awareness of mineralogy and other physical and natural sciences through the de- sign and supervision of numerous museum exhibitions and educational programs, Dan was posthumously award- ed the Public Service Medal of the Mineralogical Society of America at the 1998 annual meeting in Toronto, Canada. Dan was born on April 11, 1931, in Berkeley, Califor- nia and he grew up in a stimulating environment; his father was a professor of botany at UCLA and his mother taught biology in a California high school for many years. -
The Rarer Metals
THE RARER METALS. By FRANK L. HESS. INTRODUCTION. Great gold placer fields, now mere wastes of overturned gravels; worked-out coal fields; exhausted gold, silver, and other mines, with their sterile dumps, gaunt head frames, and decaying shaft houses and mills, testify that, unlike manufactures and agricultural prod ucts, mineral deposits are diminishing assets, and the fact that a large production of some mineral has been made in one year does not necessarily imply that it can be repeated under the impetus of great need. In estimating the possible production of any mineral for any period, a proper weighing of the attending circumstances, the statistics of production of preceding years, and a knowledge of the deposits themselves are all necessary, and these statements probably apply more forcibly to the metals used in alloy steels than to others, for these metals occur in vastly less quantities than coal, iron, copper, or the other common metals, and the individual deposits are smaller' and much less widely distributed and, unlike those of copper or iron, are in very few places concentrated from lean into richer deposits. Comparatively restricted markets and lack of knowledge concern ing these metals themselves and of the minerals in which they occur have prevented prospecting for them until within the last few years, so that as a rule developments of such deposits are small. The subjects briefly discussed here with reference to their avail ability as war supplies are treated more fully in Mineral Resources and other publications of the.United States Geological Survey, espe cially those for recent years. -
VEIN and GREISEN SN and W DEPOSITS (MODELS 15A-C; Cox and Bagby, 1986; Reed, 1986A,B) by James E. Elliott, Robert J. Kamilli, Wi
VEIN AND GREISEN SN AND W DEPOSITS (MODELS 15a-c; Cox and Bagby, 1986; Reed, 1986a,b) by James E. Elliott, Robert J. Kamilli, William R. Miller, and K. Eric Livo SUMMARY OF RELEVANT GEOLOGIC, GEOENVIRONMENTAL, AND GEOPHYSICAL INFORMATION Deposit geology Vein deposits consist of simple to complex fissure filling or replacement quartz veins, including discrete single veins, swarms or systems of veins, or vein stockworks, that contain mainly wolframite series minerals (huebnerite-ferberite) and (or) cassiterite as ore minerals (fig. 1). Other common minerals are scheelite, molybdenite, bismuthinite, base- etal sulfide minerals, tetrahedrite, pyrite, arsenopyrite, stannite, native bismuth, bismuthinite, fluorite, muscovite, biotite, feldspar, beryl, tourmaline, topaz, and chlorite (fig. 2). Complex uranium, thorium, rare earth element oxide minerals and phosphate minerals may be present in minor amounts. Greisen deposits consist of disseminated cassiterite and cassiterite-bearing veinlets, stockworks, lenses, pipes, and breccia (fig. 3) in gangue composed of quartz, mica, fluorite, and topaz. Veins and greisen deposits are found within or near highly evolved, rare-metal enriched plutonic rocks, especially near contacts with surrounding country rock; settings in or adjacent to cupolas of granitic batholiths are particularly favorable. Figure 1. Generalized longitudinal section through the Xihuashan and Piaotang tungsten deposits in the Dayu district, China. Other vein systems are indicated by heavy lines. I, upper limits of ore zones; II, lower limits of ore zones. Patterned area is granite batholith. Unpatterned area is sedimentary and metamorphic rocks (from Elliott, 1992). Figure 2. Maps and sections of tungsten vein deposits illustrating mineral and alteration zoning. A, Chicote Grande deposit, Bolivia; B, Xihuashan, China (from Cox and Bagby, 1986). -
Allchar Mineral Assemblage 3
Geologica Macedonica, Vol. 15-16, p. 1-23 (2001-2002) Suppl. GEOME2 SSN 0352 - 1206 Manuscript received: December 15, 200 1 UDC: 553.08 (497 .7) Accepted: March 3, 2002 Original scientific paper ~• ALLCHAR l\1INERAL ASSEMBLAGE l 3 l 4 Blazo Boev , Vladimir Bermanec , Todor Serafimovski\ Sonja Lepitkova , Snezana Mikulcic , 5 5 5 Marin ~oufek\ Gligor Jovanovski , Trajce Stafilov , Metodija Najdoski IDepartment ofPetrology, Mineralogy and Geochemistry, Faculty ofMining and Geology, "Sv. Kiril i Metodij" University, Goce Delcev 89, MK-2000 Stip, Republic ofMacedonia 2Department ofMineral Deposits, Faculty ofMining and Geology, "Sv. Kiril i Metodij" University, Goce Delcev 89, MK-2000 Stip, Republic of Macedonia 3Institute ofMineralogy and Petrology, Department ofGeology, Faculty ofScience, University ofZagreb, Horvatovac bb, HR-JOOOO Zagreb, Croatia 4Department ofMineralogy and Petrology, Croatian Natural History Museum, Demetrova I, HR-JOOOO Zagreb, Croatia 5Institute of Chemistry, Faculty ofScience, "Sv. Kiril i Metodij" University, P.o. Box 162, MK-JOOI Skopje, Republic ofMacedonia Abstract. The paper is a summary of investigatioris carried out on minerals of the Allchar deposit. It discusses the TI-As-Sb-Au mineral ill emblage after detailed and intense research work. Four types of mineralization have been distinguished based on the mineral assemblage present: I. The first ly pe is characterised by high c ment of iron and sulphur, but lower arsenic and thalli um contenl. The pyrite-marcasite mineral assemblage is characterized by the presence of some quantities of arsenic-pyrite. 2. The second type is characterized by the high antimony and low iron and thallium content. Stibnite is the most common mineral in the group. -
Joint Meeting
Joint Meeting 19. Jahrestagung der Deutschen Gesellschaft für Kristallographie 89. Jahrestagung der Deutschen Mineralogischen Gesellschaft Jahrestagung der Österreichischen Mineralogischen Gesellschaft (MinPet 2011) 20.-24. September 2011 Salzburg Referate Oldenbourg Verlag – München Inhaltsverzeichnis Plenarvorträge ............................................................................................................................................................ 1 Goldschmidt Lecture .................................................................................................................................................. 3 Vorträge MS 1: Crystallography at High Pressure/Temperature ................................................................................................. 4 MS 2: Functional Materials I ........................................................................................................................................ 7 MS 3: Metamorphic and Magmatic Processes I ......................................................................................................... 11 MS 4: Computational Crystallography ....................................................................................................................... 14 MS 5: Synchrotron- and Neutron Diffraction ............................................................................................................. 17 MS 6: Functional Materials II and Ionic Conductors ................................................................................................