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Sarkinite Mn (Aso4)(OH)
2+ Sarkinite Mn2 (AsO4)(OH) c 2001-2005 Mineral Data Publishing, version 1 Crystal Data: Monoclinic. Point Group: 2/m. Crystals typically thick tabular {100}, elongated, to 4 mm, short prismatic, or tabular along [010]. May be crudely spherical, granular massive. Physical Properties: Cleavage: On {100}, distinct. Fracture: Subconchoidal to uneven. Hardness = 4–5 D(meas.) = 4.08–4.18 D(calc.) = 4.20 Optical Properties: Semitransparent. Color: Flesh-red to dark blood-red, rose-red, orange, orange-brown, brown, reddish yellow to yellow; pale rose to yellow in transmitted light. Streak: Rose-red to yellow. Luster: Greasy. Optical Class: Biaxial (–). Pleochroism: Weak. Orientation: Y = b; X ∧ c = –54◦. Dispersion: r< v. Absorption: X > Z > Y. α = 1.790–1.793 β = 1.794–1.807 γ = 1.798–1.809 2V(meas.) = 83◦ Cell Data: Space Group: P 21/a. a = 12.779(2) b = 13.596(2) c = 10.208(2) β = 108◦530 Z=16 X-ray Powder Pattern: Pajsberg [Harstigen mine, near Persberg], Sweden. 3.18 (10), 3.04 (10), 3.29 (9), 3.48 (8), 2.90 (7), 2.65 (6), 6.0 (3) Chemistry: (1) (2) (3) (1) (2) (3) P2O5 0.21 ZnO 0.15 As2O5 41.60 44.09 43.23 PbO 0.25 CO2 0.76 MgO 0.98 0.19 FeO 0.13 0.02 CaO 1.40 0.29 MnO 51.60 51.77 53.38 H2O 3.06 [3.40] 3.39 CuO 0.01 insol. 0.38 Total 100.37 [99.92] 100.00 (1) Pajsberg [Harstigen mine, near Persberg], Sweden. -
U-Pb Age, Re-Os Isotopes, and Hse Geochemistry of Northwest Africa 6704
44th Lunar and Planetary Science Conference (2013) 1841.pdf U-PB AGE, RE-OS ISOTOPES, AND HSE GEOCHEMISTRY OF NORTHWEST AFRICA 6704. T. Iizuka1, Y. Amelin2, I. S. Puchtel3, R. J. Walker3, A. J. Irving4, A. Yamaguchi5, Y. Takagi6, T. Noguchi6 and M. Kimura5. 1Department of Earth and Planetary Science, University of Tokyo, Hongo 7-3-1, Bunkyo, Tokyo 113-0033, Japan ([email protected]), 2Research School of Earth Sciences, Australian National University, Canberra ACT, Australia, 3Department of Geology, University of Maryland, College Park, MD, USA, 4Department of Earth and Space Sciences, University of Washington, Seattle, WA, USA, 5National Institute of Polar Research, Tachikawa, Tokyo 190-8518, Japan, 6College of Science, Ibaraki University, Bunkyo 2-1-1, Mito, Ibaraki 310-8512, Japan. Introduction: Northwest Africa (NWA) 6704 is a of Maryland using standard high temperature acid diges- very unusual ungrouped fresh achondrite. It consists of tion, chemical purification and mass spectrometry tech- abundant coarse-grained (up to 1.5 mm) low-Ca py- niques [3]. The quantities of each of the HSE was at roxene, less abundant olivine, chromite, merrillite and least 1000 times greater than the blanks measured at the interstitial sodic plagioclase. Minor minerals are same time. Thus, blanks had no impact on the measure- awaruite, heazlewoodite, and pentlandite. Raman spec- ments. Accuracy and precision of Ir, Ru, Pt and Pd con- troscopy shows that a majority of the low-Ca pyroxene centrations are estimated to be <2%, of Re <0.4%, and is orthopyroxene. Bulk major element abundances are of Os <0.1%. -
Mineral Processing
Mineral Processing Foundations of theory and practice of minerallurgy 1st English edition JAN DRZYMALA, C. Eng., Ph.D., D.Sc. Member of the Polish Mineral Processing Society Wroclaw University of Technology 2007 Translation: J. Drzymala, A. Swatek Reviewer: A. Luszczkiewicz Published as supplied by the author ©Copyright by Jan Drzymala, Wroclaw 2007 Computer typesetting: Danuta Szyszka Cover design: Danuta Szyszka Cover photo: Sebastian Bożek Oficyna Wydawnicza Politechniki Wrocławskiej Wybrzeze Wyspianskiego 27 50-370 Wroclaw Any part of this publication can be used in any form by any means provided that the usage is acknowledged by the citation: Drzymala, J., Mineral Processing, Foundations of theory and practice of minerallurgy, Oficyna Wydawnicza PWr., 2007, www.ig.pwr.wroc.pl/minproc ISBN 978-83-7493-362-9 Contents Introduction ....................................................................................................................9 Part I Introduction to mineral processing .....................................................................13 1. From the Big Bang to mineral processing................................................................14 1.1. The formation of matter ...................................................................................14 1.2. Elementary particles.........................................................................................16 1.3. Molecules .........................................................................................................18 1.4. Solids................................................................................................................19 -
NEW MINERAL NAMES Mrcnnnr Fr-Brscnpn
THE AMERICAN MINERAI,OGIST, VOL. 55, JANUARY-FEBRUARY, 1970 NEW MINERAL NAMES Mrcnnnr Fr-Brscnpn Barringerite P. R. Busrcr (1969) Phosphide from meteorites.' Barringerite, a new iron-nickel mineral. Sci,ence165, 169-17 1,. The average of microprobe analyses was Fe 44.3*0.9, Ni 33.9+0.7, Co 0.25+0.03, P 21.8+0.4, stm 10O.25/6,corresponding to (Irer.roNio.srCoo.n)P,or (Fe, Ni)rP. X-ray study shows it to be hexagonal,space group P62 m, a 5.87 -t0.07, c 3.M+0.04 ft. The strongest X-ray lines (including many overlapping troilite or schreibersite; those starred do not overlap) are 2.98 (110),2.85* (101),2.53(200),2.23(lll),2.03*(201), 1.88* (r20), r.72(t00), 1.68(300, t2r), L.48(220), t.4t(3t0, 22r), r.29*(31r), 1.28(122), t.27 (400), 1.205(302),1.197(4oD.The structure is similar to those of synthetic FerP and NirP. p (calc) 6.92. Color white, very similar to that of kamacite, bluish compared to schreibersite. Harder than either kamacite or schreibersite. Reflectivity in air and oil slightly higher than that of schreibersite, lower than that of kamacite. Noticeably anisotropic (white to blue). Bireflectance not observed. The mineral occurs as bands 10-15 pm wide and several hundred microns long; they consist of individual grains less than 1 pm in diameter. They occur in the Ollague pallasite along the contacts between schreibersite and troilite. The name is for D. -
Third-Generation Synchrotron X-Ray Diffraction of 6- M Crystal of Raite, Na
Proc. Natl. Acad. Sci. USA Vol. 94, pp. 12263–12267, November 1997 Geology Third-generation synchrotron x-ray diffraction of 6-mm crystal of raite, 'Na3Mn3Ti0.25Si8O20(OH)2z10H2O, opens up new chemistry and physics of low-temperature minerals (crystal structureymicrocrystalyphyllosilicate) JOSEPH J. PLUTH*, JOSEPH V. SMITH*†,DMITRY Y. PUSHCHAROVSKY‡,EUGENII I. SEMENOV§,ANDREAS BRAM¶, CHRISTIAN RIEKEL¶,HANS-PETER WEBER¶, AND ROBERT W. BROACHi *Department of Geophysical Sciences, Center for Advanced Radiation Sources, GeologicalySoilyEnvironmental, and Materials Research Science and Engineering Center, 5734 South Ellis Avenue, University of Chicago, Chicago, IL 60637; ‡Department of Geology, Moscow State University, Moscow, 119899, Russia; §Fersman Mineralogical Museum, Russian Academy of Sciences, Moscow, 117071, Russia; ¶European Synchrotron Radiation Facility, BP 220, 38043, Grenoble, France; and UOP Research Center, Des Plaines, IL 60017 Contributed by Joseph V. Smith, September 3, 1997 ABSTRACT The crystal structure of raite was solved and the energy and metal industries, hydrology, and geobiology. refined from data collected at Beamline Insertion Device 13 at Raite lies in the chemical cooling sequence of exotic hyperal- the European Synchrotron Radiation Facility, using a 3 3 3 3 kaline rocks of the Kola Peninsula, Russia, and the 65 mm single crystal. The refined lattice constants of the Monteregian Hills, Canada (2). This hydrated sodium- monoclinic unit cell are a 5 15.1(1) Å; b 5 17.6(1) Å; c 5 manganese silicate extends the already wide range of manga- 5.290(4) Å; b 5 100.5(2)°; space group C2ym. The structure, nese crystal chemistry (3), which includes various complex including all reflections, refined to a final R 5 0.07. -
Moon Minerals a Visual Guide
Moon Minerals a visual guide A.G. Tindle and M. Anand Preliminaries Section 1 Preface Virtual microscope work at the Open University began in 1993 meteorites, Martian meteorites and most recently over 500 virtual and has culminated in the on-line collection of over 1000 microscopes of Apollo samples. samples available via the virtual microscope website (here). Early days were spent using LEGO robots to automate a rotating microscope stage thanks to the efforts of our colleague Peter Whalley (now deceased). This automation speeded up image capture and allowed us to take the thousands of photographs needed to make sizeable (Earth-based) virtual microscope collections. Virtual microscope methods are ideal for bringing rare and often unique samples to a wide audience so we were not surprised when 10 years ago we were approached by the UK Science and Technology Facilities Council who asked us to prepare a virtual collection of the 12 Moon rocks they loaned out to schools and universities. This would turn out to be one of many collections built using extra-terrestrial material. The major part of our extra-terrestrial work is web-based and we The authors - Mahesh Anand (left) and Andy Tindle (middle) with colleague have build collections of Europlanet meteorites, UK and Irish Peter Whalley (right). Thank you Peter for your pioneering contribution to the Virtual Microscope project. We could not have produced this book without your earlier efforts. 2 Moon Minerals is our latest output. We see it as a companion volume to Moon Rocks. Members of staff -
Sugilite in Manganese Silicate Rocks from the Hoskins Mine and Woods Mine, New South Wales, Australia
Sugilite in manganese silicate rocks from the Hoskins mine and Woods mine, New South Wales, Australia Y. KAWACHI Geology Department, University of Otago, P.O.Box 56, Dunedin, New Zealand P. M. ASHLEY Department of Geology and Geophysics, University of New England, Armidale, NSW 2351, Australia D. VINCE 1A Ramsay Street, Essendon, Victoria 3040, Australia AND M. GOODWIN P.O.Bo• 314, Lightning Ridge, NSW 2834, Australia Abstract Sugilite relatively rich in manganese has been found at two new localities, the Hoskins and Woods mines in New South Wales, Australia. The occurrences are in manganese-rich silicate rocks of middle to upper greenschist facies (Hoskins mine) and hornblende hornfels facies (Woods mine). Coexisting minerals are members of the namansilite-aegirine and pectolite-serandite series, Mn-rich alkali amphiboles, alkali feldspar, braunite, rhodonite, tephroite, albite, microcline, norrishite, witherite, manganoan calcite, quartz, and several unidentified minerals. Woods mine sugilite is colour-zoned with pale mauve cores and colourless rims, whereas Hoskins mine sugilite is only weakly colour-zoned and pink to mauve. Within single samples, the chemical compositions of sugilite from both localities show wide ranges in A1 contents and less variable ranges of Fe and Mn, similar to trends in sugilite from other localities. The refractive indices and cell dimensions tend to show systematic increases progressing from Al-rich to Fe- Mn-rich. The formation of the sugilite is controlled by the high alkali (especially Li) and manganese contents of the country rock, reflected in the occurrences of coexisting high alkali- and manganese- bearing minerals, and by high fo2 conditions. KEYWORDS: sugilite, manganese silicate rocks, milarite group, New South Wales, Australia Introduction Na2K(Fe 3 +,Mn 3 +,Al)2Li3Sit2030. -
Addibischoffite, Ca2al6al6o20, a New Calcium Aluminate Mineral from The
1 Revision 3 2 Addibischoffite, Ca2Al6Al6O20, a new calcium aluminate mineral from 3 the Acfer 214 CH carbonaceous chondrite: A new refractory phase from 4 the solar nebula 5 Chi Ma1,*, Alexander N. Krot2, Kazuhide Nagashima2 6 1Division of Geological and Planetary Sciences, California Institute of Technology, 7 Pasadena, California 91125, USA 8 2Hawai‘i Institute of Geophysics and Planetology, University of Hawai‘i at Mānoa, 9 Honolulu, Hawai‘i 96822, USA 10 11 ABSTRACT 12 Addibischoffite (IMA 2015-006), Ca2Al6Al6O20, is a new calcium aluminate mineral 13 that occurs with hibonite, perovskite, kushiroite, Ti-kushiroite, spinel, melilite, 14 anorthite and FeNi-metal in the core of a Ca-Al-rich inclusion (CAI) in the Acfer 15 214 CH3 carbonaceous chondrite. The mean chemical composition of type 16 addibischoffite by electron probe microanalysis is (wt%) Al2O3 44.63, CaO 15.36, 17 SiO2 14.62, V2O3 10.64, MgO 9.13, Ti2O3 4.70, FeO 0.46, total 99.55, giving rise to 18 an empirical formula of 3+ 3+ 2+ 19 (Ca2.00)(Al2.55Mg1.73V 1.08Ti 0.50Ca0.09Fe 0.05)Σ6.01(Al4.14Si1.86)O20. The general 20 formula is Ca2(Al,Mg,V,Ti)6(Al,Si)6O20. The end-member formula is Ca2Al6Al6O20. 21 Addibischoffite has the P1 aenigmatite structure with a = 10.367 Å, b = 10.756 Å, c 22 = 8.895 Å, α = 106.0°, β = 96.0°, γ = 124.7°, V = 739.7 Å3, and Z = 2, as revealed by 23 electron back-scatter diffraction. The calculated density using the measured 24 composition is 3.41 g/cm3. -
NI 43-101 Preliminary Economic Assessment Report
N.I. 43-101 TECHNICAL REPORT & PRELIMINARY ECONOMIC ASSESSMENT FOR THE TURNAGAIN PROJECT British Columbia, Canada Report date: November 18, 2020 Effective date: October 28, 2020 Prepared for: Suite 203 – 700 West Pender St., Vancouver, BC, V6C 1G8 www.gigametals.com Prepared by: 1066 W. Hastings St., Vancouver, BC, V6E 3X2 Qualified Persons Ian Thompson, P.Eng., Persio Rosario, P.Eng., Evan Jones, P.Eng., Gerald Schwab, P.Eng., & Stefan Hlouschko, P.Eng. – Hatch Ltd. • Garth Kirkham, P.Geo – Kirkham Geosystems • Daniel Friedman, P.Eng. – Knight Piésold • Ron Monk, P.Eng. – Kerr Wood Leidal • Chris Martin, C.Eng. MIMMM – Blue Coast Metallurgy • Andrew Mitchell, PhD, C.Eng – Wood Mackenzie Kirkham Geosystems Ltd. IMPORTANT NOTICE TO READER This report was prepared by the qualified persons (QPs) listed in Table 2.1. Each QP assumes responsibility for those sections or areas of this report that are referenced opposite their name in Table 2.1. None of the QPs, however, accepts any responsibility or liability for the sections or areas of this report that were prepared by other QPs. This report was prepared to allow Giga Metals Corporation (the “Owner”) to reach informed decisions respecting the development of the Turnagain Project. Except for the purposes legislated under provincial securities law, any use of this report by any third party is at that party's sole risk, and none of the contributors shall have any liability to any third party for any such use for any reason whatsoever, including negligence. This report is intended to be read as a whole, and sections should not be read or relied upon out of context. -
Thirty-Fourth List of New Mineral Names
MINERALOGICAL MAGAZINE, DECEMBER 1986, VOL. 50, PP. 741-61 Thirty-fourth list of new mineral names E. E. FEJER Department of Mineralogy, British Museum (Natural History), Cromwell Road, London SW7 5BD THE present list contains 181 entries. Of these 148 are Alacranite. V. I. Popova, V. A. Popov, A. Clark, valid species, most of which have been approved by the V. O. Polyakov, and S. E. Borisovskii, 1986. Zap. IMA Commission on New Minerals and Mineral Names, 115, 360. First found at Alacran, Pampa Larga, 17 are misspellings or erroneous transliterations, 9 are Chile by A. H. Clark in 1970 (rejected by IMA names published without IMA approval, 4 are variety because of insufficient data), then in 1980 at the names, 2 are spelling corrections, and one is a name applied to gem material. As in previous lists, contractions caldera of Uzon volcano, Kamchatka, USSR, as are used for the names of frequently cited journals and yellowish orange equant crystals up to 0.5 ram, other publications are abbreviated in italic. sometimes flattened on {100} with {100}, {111}, {ill}, and {110} faces, adamantine to greasy Abhurite. J. J. Matzko, H. T. Evans Jr., M. E. Mrose, lustre, poor {100} cleavage, brittle, H 1 Mono- and P. Aruscavage, 1985. C.M. 23, 233. At a clinic, P2/c, a 9.89(2), b 9.73(2), c 9.13(1) A, depth c.35 m, in an arm of the Red Sea, known as fl 101.84(5) ~ Z = 2; Dobs. 3.43(5), D~alr 3.43; Sharm Abhur, c.30 km north of Jiddah, Saudi reflectances and microhardness given. -
Carnegie/DOE Alliance Center (CDAC): a CENTER of EXCELLENCE for HIGH PRESSURE SCIENCE and TECHNOLOGY
CARNEGIE/DOE ALLIANCE CENTER A Center of Excellence for High Pressure Science and Technology Supported by the Stockpile Stewardship Academic Alliances Program of DOE/NNSA Year Three Annual Report September 2006 Russell J. Hemley, Director Ho-kwang Mao, Associate Director Stephen A. Gramsch, Coordinator Carnegie/DOE Alliance Center (CDAC): A CENTER OF EXCELLENCE FOR HIGH PRESSURE SCIENCE AND TECHNOLOGY YEAR THREE ANNUAL REPORT 1. Overview 1.1 Mission of CDAC 3 1.2 Highlights from Year 3 4 1.3 Year 3 Work Plan and Milestones 6 2. Scientific Progress 2.1 High P-T Phase Relations and Structures 10 2.2 P-V-T EOS Measurements 19 2.3 Phonons, Vibrational Thermodynamics and Elasticity 22 2.4 Plasticity, Yield Strength and Deformation 26 2.5 Electronic and Magnetic Structure and Dynamics 27 2.6 High P-T Chemistry 36 3. Education, Training, and Outreach 3.1 CDAC Graduate Students and Post-doctoral Associates 40 3.2 CDAC Collaborators 43 3.3 Undergraduate Student Participation 47 3.4 DC Area High School Outreach 49 3.5 Synergy of 21st Century High-Pressure Science and Technology Workshop 50 3.6 Visitors to CDAC 56 3.7 High Pressure Seminars 58 4. Technology Development 4.1 High P-T Experimental Techniques 60 4.2 Facilities at Brookhaven, LANSCE, and Carnegie 64 4.3 Commissioning and Activities at HPCAT 66 5. Interactions with NNSA/DP National Laboratories 5.1 Overview 67 5.2 Academic Alliance and Laboratory Collaborations 69 6. Management and Oversight 6.1 CDAC Organization and Staff 71 6.2 CDAC Oversight 73 6.3 Second Year Review 74 7. -
Previously Unknown Quasicrystal Periodic Approximant Found in Space Received: 13 August 2018 Luca Bindi 1, Joyce Pham 2 & Paul J
www.nature.com/scientificreports OPEN Previously unknown quasicrystal periodic approximant found in space Received: 13 August 2018 Luca Bindi 1, Joyce Pham 2 & Paul J. Steinhardt3,4 Accepted: 16 October 2018 We report the discovery of Al Ni Fe , the frst natural known periodic crystalline approximant Published: xx xx xxxx 34 9 2 to decagonite (Al71Ni24Fe5), a natural quasicrystal composed of a periodic stack of planes with quasiperiodic atomic order and ten-fold symmetry. The new mineral has been approved by the International Mineralogical Association (IMA 2018-038) and ofcially named proxidecagonite, which derives from its identity to periodic approximant of decagonite. Both decagonite and proxidecagonite were found in fragments from the Khatyrka meteorite. Proxidecagonite is the frst natural quasicrystal approximant to be found in the Al-Ni-Fe system. Within this system, the decagonal quasicrystal phase has been reported to transform at ~940 °C to Al13(Fe,Ni)4, Al3(Fe,Ni)2 and the liquid phase, and between 800 and 850 °C to Al13(Fe,Ni)4, Al3(Fe,Ni) and Al3(Fe,Ni)2. The fact that proxidecagonite has not been observed in the laboratory before and formed in a meteorite exposed to high pressures and temperatures during impact-induced shocks suggests that it might be a thermodynamically stable compound at high pressure. The most prominent structural motifs are pseudo-pentagonal symmetry subunits, such as pentagonal bipyramids, that share edges and corners with trigonal bipyramids and which maximize shortest Ni–Al over Ni–Ni contacts. 1,2 Te frst decagonal quasicrystalline (QC) phase found in nature, decagonite Al71Ni24Fe5 , was discovered in the Khatyrka meteorite, a CV3 carbonaceous chondrite3–8.