The Opaque Minerals of the Ultramafic Rocks of New Caledonia
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Paolovite Pd2sn C 2001-2005 Mineral Data Publishing, Version 1
Paolovite Pd2Sn c 2001-2005 Mineral Data Publishing, version 1 Crystal Data: Orthorhombic. Point Group: 2/m 2/m 2/m. As irregular grains embedded in other minerals. Twinning: Polysynthetic. Physical Properties: Hardness = n.d. VHN = 329–378 (10 g load). D(meas.) = n.d. D(calc.) = 11.08 Optical Properties: Opaque. Color: Lilac-rose. Luster: Metallic. Pleochroism: Dark lilac-rose to pale rose. R1–R2: (400) — , (420) 44.4–46.5, (440) 44.6–47.2, (460) 45.0–48.2, (480) 45.5–49.1, (500) 45.9–50.3, (520) 46.7–51.6, (540) 47.7–52.8, (560) 49.0–54.1, (580) 50.9–55.4, (600) 52.9–56.7, (620) 55.3–57.7, (640) 57.7–59.2, (660) 59.8–59.5, (680) 61.5–60.3, (700) 62.7–60.6 Cell Data: Space Group: P bnm. a = 8.11(1) b = 5.662(6) c = 4.324(2) Z = 4 X-ray Powder Pattern: Oktyabr deposit, Russia. 2.28 (100), 2.16 (70), 1.955 (50), 2.36 (40), 1.397 (40), 1.315 (40), 1.120 (40) Chemistry: (1) (2) (3) Pd 64.8 64.3 64.19 Pt 2.5 Sn 35.5 35.0 35.81 Sb 0.3 Bi 0.2 Total 103.3 99.3 100.00 (1) Oktyabr deposit, Russia; by electron microprobe, corresponding to (Pd1.98Pt0.04)Σ=2.02Sn0.98. (2) Western Platinum mine, South Africa; by electron microprobe, corresponding to Pd2.02Sn0.98. (3) Pd2Sn. Occurrence: In Cu–Ni sulfide ores; in cubanite–chalcopyrite, cubanite–talnakhite, and cubanite–mooihoekite assemblages (Oktyabr deposit, Russia). -
Accretion of Water in Carbonaceous Chondrites: Current Evidence and Implications for the Delivery of Water to Early Earth
ACCRETION OF WATER IN CARBONACEOUS CHONDRITES: CURRENT EVIDENCE AND IMPLICATIONS FOR THE DELIVERY OF WATER TO EARLY EARTH Josep M. Trigo-Rodríguez1,2, Albert Rimola3, Safoura Tanbakouei1,3, Victoria Cabedo Soto1,3, and Martin Lee4 1 Institute of Space Sciences (CSIC), Campus UAB, Facultat de Ciències, Torre C5-parell-2ª, 08193 Bellaterra, Barcelona, Catalonia, Spain. E-mail: [email protected] 2 Institut d’Estudis Espacials de Catalunya (IEEC), Edif.. Nexus, c/Gran Capità, 2-4, 08034 Barcelona, Catalonia, Spain 3 Departament de Química, Universitat Autònoma de Barcelona, 08193 Bellaterra, Catalonia, Spain. E-mail: [email protected] 4 School of Geographical and Earth Sciences, University of Glasgow, Gregory Building, Lilybank Gardens, Glasgow G12 8QQ, UK. Manuscript Pages: 37 Tables: 2 Figures: 10 Keywords: comet; asteroid; meteoroid; meteorite; minor bodies; primitive; tensile strength Accepted in Space Science Reviews (SPAC-D-18-00036R3, Vol. Ices in the Solar System) DOI: 10.1007/s11214-019-0583-0 Abstract: Protoplanetary disks are dust-rich structures around young stars. The crystalline and amorphous materials contained within these disks are variably thermally processed and accreted to make bodies of a wide range of sizes and compositions, depending on the heliocentric distance of formation. The chondritic meteorites are fragments of relatively small and undifferentiated bodies, and the minerals that they contain carry chemical signatures providing information about the early environment available for planetesimal formation. A current hot topic of debate is the delivery of volatiles to terrestrial planets, understanding that they were built from planetesimals formed under far more reducing conditions than the primordial carbonaceous chondritic bodies. -
A Sheffield Hallam University Thesis
An evaluation of river catchment quality in relation to restoration issues. AHMED, Badria S. Available from the Sheffield Hallam University Research Archive (SHURA) at: http://shura.shu.ac.uk/19204/ A Sheffield Hallam University thesis This thesis is protected by copyright which belongs to the author. The content must not be changed in any way or sold commercially in any format or medium without the formal permission of the author. When referring to this work, full bibliographic details including the author, title, awarding institution and date of the thesis must be given. Please visit http://shura.shu.ac.uk/19204/ and http://shura.shu.ac.uk/information.html for further details about copyright and re-use permissions. Return to Learning Centre of issue Fines are charged at 50p per hour 2 6 JUL J U X V U l 1 V /-L i REFERENCE ProQuest Number: 10694084 All rights reserved INFORMATION TO ALL USERS The quality of this reproduction is dependent upon the quality of the copy submitted. In the unlikely event that the author did not send a complete manuscript and there are missing pages, these will be noted. Also, if material had to be removed, a note will indicate the deletion. uest ProQuest 10694084 Published by ProQuest LLC(2017). Copyright of the Dissertation is held by the Author. All rights reserved. This work is protected against unauthorized copying under Title 17, United States Code Microform Edition © ProQuest LLC. ProQuest LLC. 789 East Eisenhower Parkway P.O. Box 1346 Ann Arbor, Ml 4 8 1 0 6 - 1346 An Evaluation of River Catchment Quality in Relation to Restoration Issues. -
Cu-Fe-S Phases in Lunar Rocks
American Mineralogist, Volume 58, pages 952-954, 1973 Cu-Fe-SPhases in LunarRocks LawnnNcn A. Tevronl Departmentol Geosciences,Purdue Uniuersity, Lalaye t te, I ndiana47 907 KBNNrrn L. Wnrrnus Departmentof Applied Earth Sciences,Stanlord Uniaersity, Stanford, Calilornia 943 0 5 Abstract The sulfide minerals reported to be present in lunar rocks include troilite, mackinawite, the discredited mineral "chalcopyrrhotite", sphalerite, chalcopyrite, and cubanite. Apollo 12 sam- ple l2D2l,l34 contains these last two minerals, and the first chemical analyses of the Cu-Fe-S phases are presented. These minerals occur along cracks and grain boundaries within troilite and are probably exsolution products formed at low temperatures (i.e, 100"-300'C) from a cupriferous troilite. Introduction Cu-Fe-S Minerals The opaqueminerals, although constituting only a "Chalcopyrrhotite", a discreditedmineral (Yund minor amount of a given sample,have proven useful and Kullerud, 1966; Cabri, 7967) , hasbeen reported as indicators of the genesisand cooling histories of from Apollo 12, 14, and 15 rocks (El Goresyet al, the lunar rocks (e.9., Reid, 1971; Taylor and Mc- l97la,b; 1972a,b). It wasdescribed as a yellowish, Callister, 19721,Taylor et al, I973b). The most chalcopyrite-coloredphase which appearsisotropic abundant opaque mineral is ilmenite, and many of and is alwaysfound within troilite. It is probablethat the oxide phasesin lunar rocks are unique (e.6'., this phase is either talnakhite, a mineral originally armalcolite as per Anderson et al, l97A). In addi- describedby Cabri (1967) andhaving a composition tion to native Fe metal, native Cu, and schreibersite, of CusFesSro(Cabri and Harris, 1971) near chal- the remaining opaqueminerals consistof sulfides. -
MACKINAWITE from SOUTH AFRICA W. C J. Van RDNSBU*.O, Geological Surtey Oj Soulh Africa, Preloria, Soulh A.[Ri Co, L. Lrbnunsbyc
TI.IE AMERICAN MINERALOGIST, VOL 52, JULY AUGUST, 1967 MACKINAWITE FROM SOUTH AFRICA W. C J. vAN RDNSBU*.o,Geological Surtey oJ Soulh Africa, Preloria,Soulh A.[rico, AND L. LrBnuNsByc, Deparlment of Geology,Llnit:ersity of Pretoria, Pre!oria,Soul h Africa. ABSTRAcT Mackinawite has been identified in mafic and ultramafic rocks of the Bushveld igneous complex and Insizwa and also in the carbonatite and pegmatoid of Loolekop, Phalaborrva complex in South Africa. The mineral occurs predominantly as somewhat irregular to oriented intergrowths in pentlandite in all these occurrences and less commonly as regular oriented lamellae in chalcopyrite and rarely in cubanite. The textural evidence suggests that mackinawite may represent an exsolution product of pentlandite, chalcopyrite and cubanite. INrnonucrroN The iron sulphide, mackinawite was recently named in a paper by Evans, et al, (1964). Natural occurrencesof this mineral f rom Finland were describedby- Kouvo et al (1963)and from the Muskox intrusion in Canada by Chamberlain and Delabio (1965). During the presentinvestigation mackinawite was distinguishedfrom valleriite in the carbonatite and pegmatoid of Loolekop, Phalaborwa complex, in the Bushveld igneous complex, and from Insizwa, Cape Province.The mode of occurrenceof the mackinawite in the carbonatite difiers somewhatfrom that in the mafic rocks of Insizwa and the Bush- veld complex. MrNnn.q.rocv The physicaland optical propertiesof mackinawitefrom the Bushveid complex,Insizwa and Loolekop are very similar and are in closeagree- ment with the propertiesgiven for the same mineral from the Muskox intrusion by Chamberlain and Delabio (1965). The mineral takes a fairly good polish,particularly after buffing with a chromic oxide slurry. -
Minerals and Mineral Products in Our Bedroom Bed Hematite
Minerals and Mineral Products in our Bedroom Make-Up Kit Muscovite Bed Talc Hematite: hinges, handles, Mica mattress springs Hematite: for color Chromite: chrome plating Bismuth Radio Barite Copper: wiring Plastic Pail Quartz: clock Mica Gold: connections Cassiterite: solder Toilet Bowl / Tub Closet Feldspar: porcelain Chromite: chrome plating Pyrolusite: coloring Hematite: hinges, handles (steel) Chromite: plumbing fixtures Quartz : mirror on door Copper: tubing Desk Toothpaste Hematite: hinges, handles (steel) Apatite: teeth Chromite: chrome plating Fluorite: toothpaste Mirror Rutile: to color false Hematite: handle, frame teeth yellow Chromite: plating Gold: fillings Gold: plating Cinnabar: fillings Quartz: mirror Towels Table Lamp Sphalerite: dyes Brass (an alloy of copper and Chromite: dyes zinc): base Quartz: bulb Water Pipe/Faucet/Shower bulb Wolframite: lamp filament Brass Copper: wiring Iron Nickel Minerals and Mineral Products in our Bedroom Chrome: stainless steel Bathroom Cleaner Department of Environment and Natural Resources Borax: abrasive, cleaner, and antiseptic MINES AND GEOSCIENCES BUREAU Deodorant Spray Can Cassiterite Chromite Copper Carpet Quartz Sphalerite: dyes Telephone Chromite: dyes Drinking Glasses Copper: wiring Sulfur: foam padding Quartz Chromite: plating Gold: red color Clock Silver: electronics Pentlandite: spring Graphite: batteries Refrigerator Quartz: glass, time keeper Hematite Television Chromite: stainless steel Chromite: plating Computer Galena Wolframite: monitor Wolframite: monitor Copper Copper: -
JNC Thermodynamic Database for Performance Assessment of High-Level Radioactive Waste Disposal System
JNC TN8400 99-070 JP0055253 JNC Thermodynamic Database for Performance Assessment of High-level Radioactive Waste Disposal System November, 1999 330030611® Tokai Works Japan Nuclear Cycle Development Institute JL- 1 / A s • mm T3i9-i 194 Inquiries about copyright and reproduction should be addressed to: Technical Information Section, Administration Division, Tokai Works, Japan Nuclear Cycle Development Institute 4-33 Muramatsu, Tokai-mura, Naka-gun, Ibaraki-ken, 319-1194 Japan © 1&W&-*)-1 9 ;u|i8§$8$f (Japan Nuclear Cycle Development Institute) 1999 Please be aware that all of the Missing Pages in this document were originally blank pages JNC TN8400 99-070 November, 1999 JNC Thermodynamic Database for Performance Assessment of High-level Radioactive Waste Disposal System Mikazu Yui*, Jiro Azuma*, and Masahiro Shibata* Abstract This report is a summary of status, frozen datasets, and future tasks of the JNC thermodynamic database (JNC-TDB) for assessing performance of high-level radioactive waste in geological environments. The JNC-TDB development was carried out after the first progress report on geological disposal research in Japan (H3). In the development, thermodynamic data (equilibrium constants at 25 °C, 1=0) for important radioactive elements were selected/determined based on original experimental data using different models (e.g., SIT, Pitzer). As a result, the reliability and traceability of the data for most of the important elements were improved over those of the PNC-TDB used in H-3 report. For detailed information of data analysis and selections for each element, see the JNC technical reports listed in this document. *: Waste Isolation Research Division, Tokai Works, Japan Nuclear Cycle Development Institute (JNC) JNC TN8400 99-070 -^-^ (JNC-TDB) (m % m. -
Pyrrhotite and Pentlandite in Ll3 to Ll6 Chondrites: Determining Compositional and Microstructural Indicators of Formation Conditions
49th Lunar and Planetary Science Conference 2018 (LPI Contrib. No. 2083) 2621.pdf PYRRHOTITE AND PENTLANDITE IN LL3 TO LL6 CHONDRITES: DETERMINING COMPOSITIONAL AND MICROSTRUCTURAL INDICATORS OF FORMATION CONDITIONS. D. L. Schrader1 and T. J. Zega2, 1Center for Meteorite Studies, School of Earth and Space Exploration, Arizona State Uni- versity, Tempe, AZ 85287-1404, USA ([email protected]), 2Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona 85721, USA ([email protected]). Introduction: The compositions, textures, and electron microscope (FIB-SEM) at UAz and the JEOL crystal structures of sulfides can be used to constrain JXA-8530F Hyperprobe EPMA at Arizona State Uni- oxygen fugacity, aqueous, thermal, and cooling history versity (ASU). The FIB-SEM was also used to extract [e.g., 1–5]. The most abundant sulfides in extraterres- ~10 × 5 µm sections transecting the pyrrhotite- trial samples are the pyrrhotite group [(Fe,Ni,Co,Cr)1– pentlandite interfaces within sulfide grains from each xS], which can occur with pentlandite [(Fe,Ni,Co,Cr)9– meteorite, which were thinned to electron transparency xS8]. The pyrrhotite group sulfides are largely non- (<100 nm) using methods of [14]. FIB sections were stoichiometric and have a range of compositions then analyzed using the 200 keV aberration-corrected (0<x<0.125) and distinct crystal structures (polytypes). Hitachi HF5000 scanning transmission electron micro- The stoichiometric end members are 2C (troilite; FeS, scope (TEM) at UAz. hexagonal) and 4C (Fe7S8, monoclinic) pyrrhotite. There are also non-integral NC-pyrrhotites with inter- mediate compositions with 0<x<0.125 (all hexagonal); which includes the integral 5C (Fe9S10), 6C (Fe11S12), and 11C (Fe10S11) pyrrhotites [e.g., 6–8]. -
Frontiers in Interfacial and Nano Catalysis
Frontiers in Interfacial and Nano Catalysis Meeting of the Catalysis and Chemical Transformations Program Chemical Sciences, Geosciences and Biosciences Division Office of Basic Energy Sciences U.S Department of Energy Wintergreen, VA May 23-26, 2007 Frontiers in Interfacial and Nano Catalysis Meeting of the Catalysis and Chemical Transformations Program Chemical Sciences, Geosciences and Biosciences Division Office of Basic Energy Sciences, U.S Department of Energy Wintergreen, VA — May 23-26, 2007 Cover figures (clockwise): 1. Nuzzo, R., et al.: HRTEM of oxygen-treated Au particles with various sizes and shapes 2. Liu, M.: Potential energy profiles for the interactions of O2 and LaSrMn electrolyte 3. Stair, P.: Oxidative dehydrogenation on VOx over nanostructured membranes This document was produced under contract number DE-AC05-06OR23100 between the U.S. Department of Energy and Oak Ridge Associated Universities. FOREWORD The 2007 Catalysis and Chemical Transformations Program Meeting is sponsored by the Division of Chemical Sciences, Geosciences and Biosciences, Office of Basic Energy Sciences (OBES), U.S. Department of Energy. It is being held on May 23-26, 2007, at the Wintergreen Resort, Wintergreen, VA. The main purpose of the meeting is to discuss the advances made by the program PIs over the past two years, to discuss the future directions for the program and catalysis, and to foster exchange of ideas and cooperation among participants. This year’s meeting will encompass projects in heterogeneous catalysis, surface science and electrochemistry, and some of the projects recently started in nanoscience, biocatalysis, hydrogen fuel initiative, and chemical imaging. Catalysis activities within OBES emphasize fundamental research aimed at understanding and controlling the chemical reactivity of fluid and condensed matter. -
Millerite and Other Nickel Sulfides from the Siderite Deposit „Steirischer Erzberg“, Styria, Austria
MITT. ÖSTERR. MINER. GES. 164 (2018) MILLERITE AND OTHER NICKEL SULFIDES FROM THE SIDERITE DEPOSIT „STEIRISCHER ERZBERG“, STYRIA, AUSTRIA Eugen Libowitzky*1, Anton Beran1 & Richard Göd2 1Institut für Mineralogie und Kristallographie 2 Department of Lithospheric Research Universität Wien, Althanstrasse 14, 1090 Wien / *[email protected] Abstract Millerite, NiS, has been identified for the first time in cinnabar- and pyrite-bearing siderite ore samples from „Steirischer Erzberg“, Styria, Austria. In addition, the occurrence of other nickel sulfides has been confirmed, such as siegenite-violarite solid-solutions (ss), CoNi2S4- FeNi2S4, and Gersdorffite, Ni[AsS]. Whereas milleri- te and gersdorffite are close to ideal chemistry with only minor Co and Fe contents, siegenite-violarite ss show a wide range of compositions. Almost pure siegenite with Fe below detection limit occurs in separated crystals within cinnabar or mil- lerite. In contrast, small grains (sometimes in equilibrium with millerite) within a pyrite host contain up to ~14.1 wt% Fe and thus plot in the compositional field of violarite. Zusammenfassung Millerit, NiS, wurde zum ersten mal in Zinnober- und Pyrit-führenden Sideriterz- proben vom Steirischen Erzberg, Steiermark, Österreich, nachgewiesen. Zusätzlich wurde auch das Vorkommen weitere Nickelsulfide wie Siegenit-Violarit-Mischkri- stalle (ss), CoNi2S4-FeNi2S4, und Gersdorffit, Ni[AsS], bestätigt. Während Millerit und Gersdorffit nahe der Idealchemie mit nur geringen Co- und Fe-Gehalten sind, zeigen Siegenit-Violarit ss einen weiten Zusammensetzungsbereich. Nahezu reiner Siegenit mit Fe unter der Nachweisgrenze kommt in separaten Kristallen innerhalb von Zinnober und Millerit vor. Im Gegensatz dazu enthalten kleine Einschlüsse (manchmal im Gleichgewicht mit Millerit) im Pyrit bis zu ~14.1 Gew.-% Fe und fallen damit in das Zusammensetzungsfeld von Violarit. -
High-Pressure Crystal Chemistry of Cubanite, Cufers
American Mineralogist, Volume 77, pages 937-944, 1992 High-pressure crystal chemistry of cubanite,CuFerS, CarnnnrNr McClvrmoNr* JrNvrrN ZruNG, RonBnr M. HlznNo Llnnv W. FrNcBn GeophysicalLaboratory and Centerfor High-PressureResearch, Carnegie Institution of Washington, 5251Broad Branch Road NW, Washington,DC 20015-1305,U.S.A. ABSTRACT We have studied cubanite, CuFerS, (orthorhombic, space gtoup Pcmn, a: 6.46, b : 11.10, c : 6.22 A), using single-crystalX-ray diffraction in a diamond-anvil cell at room temperature from 0 to 3.68 GPa. Refinementswere performed aI 0, 1.76, and 3.59 GPa, and cell parameterswere measuredat 20 pressuresup to 3.68 GPa. The linear compress- ibilities of the a, b, and c crystalaxes are 0.00513(5),0.00479(5),and 0.00575(4)GPa ', respectively.Compressibility data were fitted to a Birch-Murnaghan equation of statewith parametersKo : 55.3 + 1.7 GPa with Ko' constrained to be 4. High-pressurerefinement data indicate that the principal responseof the crystal structure to compression is a re- duction in Cu-S bond lengths, whereasFe-S bond lengths remain essentiallyunchanged. Results are compared to bulk moduli and polyhedral bulk moduli of other sulfides. INrnonucrroN lography provides an excellent means for examining the effect of pressure on individual atomic configurations. The crystal structure of cubanite, CuFerSr, is ortho- Cubanite is a worthy candidate becauseof the interest in rhombic with ordered tetrahedral cation sites and S at- the effect ofpressure on intervalence transitions (see,for oms in approximately hexagonal closest packing. The example,Burns, I 98 l) and becausevery few sulfideshave structure was first determined by Buerger (1945, 1947) beenexamined with this technique.We undertook a crys- and described as slices of wurtzite structure parallel to tallographic study of cubanite at high pressurewith the (010) with widthb/2,joined such that every other slab is following goals: (l) to determine the relative axial com- inverted, resulting in edge-sharedpairs oftetrahedra. -
Covellite) Probed by NQR
Phase transition and anomalous electronic behavior in layered dichalcogenide CuS (covellite) probed by NQR R.R. Gainov 1*, A.V. Dooglav 1, I.N. Pen’kov 2, I.R. Mukhamedshin 1,3, N.N. Mozgova 4, A.V. Evlampiev 1, and I.A. Bryzgalov 5 1 Department of Physics, Magnetic RadioSpectroscopy Laboratory, Kazan State University, Kazan, Kremlevskaya str. 18, 420008, Russian Federation 2 Department of Geology, Kazan State University, Kazan, Kremlevskaya str. 4/5, 420111, Russian Federation 3 Laboratoire de Physique des Solides, UMR 8502, Universite Paris-Sud, 91405 Orsay, France 4 Institute of geology of ore deposits, petrography, mineralogy and geochemistry (Russian Academy of Science), Staromonetny per. 35, Moscow 109017, Russian Federation 5 Department of Geology, Moscow State University, Moscow, Vorob’evy gory, 119991, Russian Federation * Corresponding author: tel.: 7-843-2315175; fax.: 7-843-2387201. Electronic address: [email protected] (R.R. Gainov). Nuclear quadrupole resonance (NQR) on copper nuclei has been applied for studies of the electronic properties of quasi-two-dimensional low-temperature superconductor CuS (covellite) in the temperature region between 1.47 and 290 K. Two NQR signals corresponding to two non- equivalent sites of copper in the structure, Cu(1) and Cu(2), has been found. The temperature dependences of copper quadrupole frequencies, line-widths and spin-lattice relaxation rates, which so far had never been investigated so precisely for this material, altogether demonstrate the structural phase transition near 55 K, which accompanies transformations of electronic spectrum not typical for simple metals. The analysis of NQR results and their comparison with literature data show that the valence of copper ions at both sites is intermediate in character between monovalent and divalent states with the dominant of the former.