New Minerals and Nomenclature Modifications Approved in 2017
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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 -
Petrology of Nepheline Syenite Pegmatites in the Oslo Rift, Norway: Zr and Ti Mineral Assemblages in Miaskitic and Agpaitic Pegmatites in the Larvik Plutonic Complex
MINERALOGIA, 44, No 3-4: 61-98, (2013) DOI: 10.2478/mipo-2013-0007 www.Mineralogia.pl MINERALOGICAL SOCIETY OF POLAND POLSKIE TOWARZYSTWO MINERALOGICZNE __________________________________________________________________________________________________________________________ Original paper Petrology of nepheline syenite pegmatites in the Oslo Rift, Norway: Zr and Ti mineral assemblages in miaskitic and agpaitic pegmatites in the Larvik Plutonic Complex Tom ANDERSEN1*, Muriel ERAMBERT1, Alf Olav LARSEN2, Rune S. SELBEKK3 1 Department of Geosciences, University of Oslo, PO Box 1047 Blindern, N-0316 Oslo Norway; e-mail: [email protected] 2 Statoil ASA, Hydroveien 67, N-3908 Porsgrunn, Norway 3 Natural History Museum, University of Oslo, Sars gate 1, N-0562 Oslo, Norway * Corresponding author Received: December, 2010 Received in revised form: May 15, 2012 Accepted: June 1, 2012 Available online: November 5, 2012 Abstract. Agpaitic nepheline syenites have complex, Na-Ca-Zr-Ti minerals as the main hosts for zirconium and titanium, rather than zircon and titanite, which are characteristic for miaskitic rocks. The transition from a miaskitic to an agpaitic crystallization regime in silica-undersaturated magma has traditionally been related to increasing peralkalinity of the magma, but halogen and water contents are also important parameters. The Larvik Plutonic Complex (LPC) in the Permian Oslo Rift, Norway consists of intrusions of hypersolvus monzonite (larvikite), nepheline monzonite (lardalite) and nepheline syenite. Pegmatites ranging in composition from miaskitic syenite with or without nepheline to mildly agpaitic nepheline syenite are the latest products of magmatic differentiation in the complex. The pegmatites can be grouped in (at least) four distinct suites from their magmatic Ti and Zr silicate mineral assemblages. -
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. -
Astrophyllite–Alkali Amphibole Rhyolite, an Evidence of Early Permian A-Type Alkaline Volcanism in the Western Mongolian Altai
Journal of Geosciences, 61 (2016), 93–103 DOI: 10.3190/jgeosci.205 Original paper Astrophyllite–alkali amphibole rhyolite, an evidence of early Permian A-type alkaline volcanism in the western Mongolian Altai Vladimír Žáček1*, David BurIánek1, Zoltán Pécskay2, radek ŠkODa1 1 Czech Geological Survey, Klárov 3, 118 21 Prague 1, Czech Republic; [email protected] 2 Institute for Nuclear Research, Hungarian Academy of Sciences (ATOMKI), Bem tér 18/c, Debrecen, Hungary * Corresponding author A dyke of alkali rhyolite intrudes the Tsetseg and Zuun Nuruu volcanosedimentary sequence of Ordovician–Silurian age (Hovd Zone, Central Asian Orogenic Belt) at the Botgon bag, Mankhan Soum, Hovd District in Western Mongolia. The rock consists of quartz and K-feldspar phenocrysts set in fine-grained groundmass composed of quartz, K-feldspar, albite, blue alkali amphibole (riebeckite–arfvedsonite containing up to 1.94 wt. % ZrO2), tiny brown radial astrophyllite, annite and accessory zircon, ilmenite, fluorite, monazite, hematite, chevkinite and bastnäsite. Astrophyllite has unusual, highly ferroan composition and occurs as two sharply bound zones of astrophyllite I and II with the average empirical formulae: 2+ (K1.71 Na0.01Rb0.08Cs0.01) (Na0.93Ca0.07) (Fe 6.52Mn0.31Zn0.06) (Ti0.84Zr0.50Nb0.55) Si7.68Al0.32 O26 (OH)3.78 F0.66 (astrophyllite I, 2+ Zr–Nb-rich); (K1.52Rb0.07) (Na0.81Ca0.19) (Fe 6.31 Mn0.28Zn0.06) (Ti1.28Nb0.30Zr0.28) Si7.68Al0.32 O26 (OH)2.85 F0.67 (astrophyllite II). Geochemically, the rhyolite corresponds to strongly fractionated silicic alkaline A-type (ferroan) magmatic rock with t 75.5–75.9 wt. -
New Mineral Names*,†
American Mineralogist, Volume 106, pages 1186–1191, 2021 New Mineral Names*,† Dmitriy I. Belakovskiy1 and Yulia Uvarova2 1Fersman Mineralogical Museum, Russian Academy of Sciences, Leninskiy Prospekt 18 korp. 2, Moscow 119071, Russia 2CSIRO Mineral Resources, ARRC, 26 Dick Perry Avenue, Kensington, Western Australia 6151, Australia In this issue This New Mineral Names has entries for 10 new species, including huenite, laverovite, pandoraite-Ba, pandoraite- Ca, and six new species of pyrochlore supergroup: cesiokenomicrolite, hydrokenopyrochlore, hydroxyplumbo- pyrochlore, kenoplumbomicrolite, oxybismutomicrolite, and oxycalciomicrolite. Huenite* hkl)]: 6.786 (25; 100), 5.372 (25, 101), 3.810 (51; 110), 2.974 (100; 112), P. Vignola, N. Rotiroti, G.D. Gatta, A. Risplendente, F. Hatert, D. Bersani, 2.702 (41; 202), 2.497 (38; 210), 2.203 (24; 300), 1.712 (60; 312), 1.450 (37; 314). The crystal structure was solved by direct methods and refined and V. Mattioli (2019) Huenite, Cu4Mo3O12(OH)2, a new copper- molybdenum oxy-hydroxide mineral from the San Samuel Mine, to R1 = 3.4% using the synchrotron light source. Huenite is trigonal, 3 Carrera Pinto, Cachiyuyo de Llampos district, Copiapó Province, P31/c, a = 7.653(5), c = 9.411(6) Å, V = 477.4 Å , Z = 2. The structure Atacama Region, Chile. Canadian Mineralogist, 57(4), 467–474. is based on clusters of Mo3O12(OH) and Cu4O16(OH)2 units. Three edge- sharing Mo octahedra form the Mo3O12(OH) unit, and four edge-sharing Cu-octahedra form the Cu4O16(OH)2 units of a “U” shape, which are in Huenite (IMA 2015-122), ideally Cu4Mo3O12(OH)2, trigonal, is a new mineral discovered on lindgrenite specimens from the San Samuel turn share edges to form a sheet of Cu octahedra parallel to (001). -
Mineral Index
Mineral Index Abhurite T.73, T.355 Anandite-Zlvl, T.116, T.455 Actinolite T.115, T.475 Anandite-20r T.116, T.45S Adamite T.73,T.405, T.60S Ancylite-(Ce) T.74,T.35S Adelite T.115, T.40S Andalusite (VoU, T.52,T.22S), T.27S, T.60S Aegirine T.73, T.30S Andesine (VoU, T.58, T.22S), T.41S Aenigmatite T.115, T.46S Andorite T.74, T.31S Aerugite (VoU, T.64, T.22S), T.34S Andradite T.74, T.36S Agrellite T.115, T.47S Andremeyerite T.116, T.41S Aikinite T.73,T.27S, T.60S Andrewsite T.116, T.465 Akatoreite T.73, T.54S, T.615 Angelellite T.74,T.59S Akermanite T.73, T.33S Ankerite T.74,T.305 Aktashite T.73, T.36S Annite T.146, T.44S Albite T.73,T.30S, T.60S Anorthite T.74,T.415 Aleksite T.73, T.35S Anorthoclase T.74,T.30S, T.60S Alforsite T.73, T.325 Anthoinite T.74, T.31S Allactite T.73, T.38S Anthophyllite T.74, T.47S, T.61S Allanite-(Ce) T.146, T.51S Antigorite T.74,T.375, 60S Allanite-(La) T.115, T.44S Antlerite T.74, T.32S, T.60S Allanite-(Y) T.146, T.51S Apatite T.75, T.32S, T.60S Alleghanyite T.73, T.36S Aphthitalite T.75,T.42S, T.60 Allophane T.115, T.59S Apuanite T.75,T.34S Alluaudite T.115, T.45S Archerite T.75,T.31S Almandine T.73, T.36S Arctite T.146, T.53S Alstonite T.73,T.315 Arcubisite T.75, T.31S Althausite T.73,T.40S Ardaite T.75,T.39S Alumino-barroisite T.166, T.57S Ardennite T.166, T.55S Alumino-ferra-hornblende T.166, T.57S Arfvedsonite T.146, T.55S, T.61S Alumino-katophorite T.166, T.57S Argentojarosite T.116, T.45S Alumino-magnesio-hornblende T.159,T.555 Argentotennantite T.75,T.47S Alumino-taramite T.166, T.57S Argyrodite (VoU, -
IMA Master List
The New IMA List of Minerals – A Work in Progress – Update: February 2013 In the following pages of this document a comprehensive list of all valid mineral species is presented. The list is distributed (for terms and conditions see below) via the web site of the Commission on New Minerals, Nomenclature and Classification of the International Mineralogical Association, which is the organization in charge for approval of new minerals, and more in general for all issues related to the status of mineral species. The list, which will be updated on a regular basis, is intended as the primary and official source on minerals. Explanation of column headings: Name: it is the presently accepted mineral name (and in the table, minerals are sorted by name). Chemical formula: it is the CNMNC-approved formula. IMA status: A = approved (it applies to minerals approved after the establishment of the IMA in 1958); G = grandfathered (it applies to minerals discovered before the birth of IMA, and generally considered as valid species); Rd = redefined (it applies to existing minerals which were redefined during the IMA era); Rn = renamed (it applies to existing minerals which were renamed during the IMA era); Q = questionable (it applies to poorly characterized minerals, whose validity could be doubtful). IMA No. / Year: for approved minerals the IMA No. is given: it has the form XXXX-YYY, where XXXX is the year and YYY a sequential number; for grandfathered minerals the year of the original description is given. In some cases, typically for Rd and Rn minerals, the year may be followed by s.p. -
Robert T Downs
Curriculum Vitae – Robert T. Downs 1 Field of Specialization: The crystallography and spectroscopy of minerals, with emphasis on crystal chemistry, bonding, temperature and pressure effects, characterization and identification. Contact Information: Dr Robert T Downs Department of Geosciences Voice: 520-626-8092 Gould-Simpson Building Lab: 520-626-3845 University of Arizona Fax: 520-621-2672 Tucson Arizona 85721-0077 [email protected] Education: University of British Columbia 1986 B.S. Mathematics Virginia Tech 1989 M.S. Geological Sciences Virginia Tech 1992 Ph.D. Geological Sciences Graduate Advisors: G.V. Gibbs (Mineralogy) and M.B. Boisen, Jr. (Mathematics) Carnegie Institution of Washington, Geophysical Laboratory, 1993 – 1996 Post-doc Advisors: R.M. Hazen and L.W. Finger Academic and Professional Appointments: Assistant Professor, Department of Geosciences, University of Arizona, August 1996 – 2002 Associate Professor, Department of Geosciences, University of Arizona, 2002 – 2008 Professor, Department of Geosciences, University of Arizona, 2008 – present Assistant to curator Joe Nagel: University of British Columbia, 1985 Assistant to curator Gary Ansell: National Mineral Collections of Canada, 1986 Assistant to curator Susan Eriksson: Virginia Tech Museum of Geological Sciences, 1990 Graduate teaching assistant: Virginia Tech, 1988 – 1992 Pre-doctoral Fellowship: Carnegie Institution of Washington, Geophysical Laboratory, 1991 Post-doctoral Fellowship: CIW, Geophysical Laboratory, February 1993 – July 1996 Visiting Professor, -
Sell-0567 , AGS Field Guide to Superior Area, Oct 1995
CONTACT INFORMATION Mining Records Curator Arizona Geological Survey 416 W. Congress St., Suite 100 Tucson, Arizona 85701 520-770-3500 http://www.azgs.az.gov [email protected] The following file is part of the James Doyle Sell Mining Collection ACCESS STATEMENT These digitized collections are accessible for purposes of education and research. We have indicated what we know about copyright and rights of privacy, publicity, or trademark. Due to the nature of archival collections, we are not always able to identify this information. We are eager to hear from any rights owners, so that we may obtain accurate information. Upon request, we will remove material from public view while we address a rights issue. CONSTRAINTS STATEMENT The Arizona Geological Survey does not claim to control all rights for all materials in its collection. These rights include, but are not limited to: copyright, privacy rights, and cultural protection rights. The User hereby assumes all responsibility for obtaining any rights to use the material in excess of “fair use.” The Survey makes no intellectual property claims to the products created by individual authors in the manuscript collections, except when the author deeded those rights to the Survey or when those authors were employed by the State of Arizona and created intellectual products as a function of their official duties. The Survey does maintain property rights to the physical and digital representations of the works. QUALITY STATEMENT The Arizona Geological Survey is not responsible for the accuracy of the records, information, or opinions that may be contained in the files. The Survey collects, catalogs, and archives data on mineral properties regardless of its views of the veracity or accuracy of those data. -
High-Temperature Behaviour of Astrophyllite, K2nafe7 2+Ti2
Phys Chem Minerals DOI 10.1007/s00269-017-0886-1 ORIGINAL PAPER High-temperature behaviour of astrophyllite, 2+ K2NaFe7 Ti2(Si4O12)2O2(OH)4F: a combined X-ray diffraction and Mössbauer spectroscopic study Elena S. Zhitova1,2 · Sergey V. Krivovichev1,3 · Frank C. Hawthorne4 · Maria G. Krzhizhanovskaya1 · Andrey A. Zolotarev1 · Yassir A. Abdu4,5 · Viktor N. Yakovenchuk3 · Yakov A. Pakhomovsky3 · Alexey G. Goncharov1 Received: 27 May 2016 / Accepted: 14 March 2017 © Springer-Verlag Berlin Heidelberg 2017 Abstract High-temperature X-ray powder-diffraction c = 11.4332(9) Å, α = 112.530(8), β = 94.539(6), 2+ 3 study of astrophyllite, K2NaFe7 Ti2(Si4O12)2O2(OH)4F, γ = 103.683(7)º, V = 633.01(9) Å for the HT (annealed) and investigation of the samples annealed at 600 and modification of astrophyllite. The oxidation of iron is 700 °C, reveal the occurrence of a phase transformation due confirmed: (1) by the presence of an exothermic effect to the thermal iron oxidation coupled with (1) deprotonation at 584 °C in the DTA/TG curves in an Ar–O atmosphere 2+ − 3+ 2− according to the scheme Fe + OH → Fe + O + ½H2 ↑, and its absence in an Ar–Ar atmosphere and (2) by ex situ and (2) defluorination according to the scheme Mössbauer spectroscopy that showed the oxidation of Fe2+ Fe2+ + F− → Fe3+ + O2−. The phase transformation occurs to Fe3+ in the samples heated to 700 °C. Deprotonation at 500 °C, it is irreversible and without symmetry changes. was detected by the evolution of IR spectra in the region The mineral decomposes at 775 °C. -
4F, a New Astrophyllite-Super- Group Mineral from Mont Saint-Hilaire, Quebec,´ Canada
201 The Canadian Mineralogist Vol. 57, pp. 201-213 (2019) DOI: 10.3749/canmin.1800071 LAVEROVITE, K2NaMn7Zr2(Si4O12)2O2(OH)4F, A NEW ASTROPHYLLITE-SUPER- GROUP MINERAL FROM MONT SAINT-HILAIRE, QUEBEC,´ CANADA § ELENA SOKOLOVA ,MAXWELL C. DAY, AND FRANK C. HAWTHORNE Department of Geological Sciences, University of Manitoba, Winnipeg, Manitoba R3T 2N2 Canada ANATOLY V. KASATKIN Fersman Mineralogical Museum, Russian Academy of Sciences, Leninskii Prospekt, 18-2, 119071 Moscow, Russia ROBERT T. DOWNS Department of Geosciences, University of Arizona, 1040 E 4th Street, Tucson, Arizona 85721-0077, USA LA´ SZLO´ HORVATH´ AND ELSA PFENNINGER-HORVATH´ 594 Main Road, Hudson Heights, Quebec´ J0P 1J0, Canada ABSTRACT Laverovite (IMA 2017-009b), ideally K2NaMn7Zr2(Si4O12)2O2(OH)4F, is a kupletskite-group (astrophyllite-supergroup) mineral from Mont Saint-Hilaire, Quebec,´ Canada. Associated minerals are zircophyllite, kupletskite, astrophyllite, aegirine, analcime, orthoclase, and albite. Laverovite is brown, transparent in thin grains, and has a vitreous luster. Mohs hardness is 3, 3 Dcalc. ¼ 3.367 g/cm . Laverovite is biaxial (–) with refractive indices (k ¼ 589 nm) a ¼ 1.670(2), b ¼ 1.710(5), c ¼ 1.740(5); 2Vmeas. ¼ 82(2)8,2Vcalc. ¼ 808, strong dispersion: r . v. Cleavage is perfect parallel to {001}. Chemical analysis by electron microprobe gave Nb2O5 0.56, ZrO2 9.78, TiO2 4.69, SiO2 33.52, Al2O3 0.94, SrO 0.13, ZnO 0.07, FeO 13.94, MnO 20.51, CaO 0.48, MgO 0.76, Cs2O 0.05, K2O 6.00, Na2O 2.28, F 1.80, H2Ocalc. 2.57, sum 97.32 wt.%; H2O was calculated from crystal-structure analysis. -
Sursassite: Hydrogen Bonding, Cation Order, and Pumpellyite Intergrowth
American Mineralogist, Volume 94, pages 1440–1449, 2009 Sursassite: Hydrogen bonding, cation order, and pumpellyite intergrowth MARIKO NAGASHIMA ,1,* MASAHIDE AKASAKA ,2 TETSUO MINAKAWA ,3 EUGEN LIBOWITZKY,4 AND THOMAS ARMBRUSTER 1 1Mineralogical Crystallography, Institute of Geological Sciences, University of Bern, Freiestrasse 3, CH-3012 Bern, Switzerland 2Department of Geoscience, Faculty of Science and Engineering, Shimane University, Matsue 690-8504, Japan 3Department of Earth Science, Faculty of Science, Ehime University, Matsuyama 790-5877, Japan 4Institute of Mineralogy and Crystallography, University of Vienna—Geocenter, Althanstrasse 14, A-1090 Vienna, Austria ABSTRACT 2+ The crystal chemistry of sursassite, simplified formula Mn2 Al3Si3O11(OH)3, from six different localities [(1) Falotta, Switzerland, (2) Woodstock, New Brunswick, Canada, (3) Kamisugai, Japan, (4) Kamogawa, Japan, (5) Molinello, Italy, and (6) Gambatesa, Italy] was studied using electron mi- croprobe analysis (EMPA), Fourier transform infrared spectroscopy (FTIR), and single-crystal X-ray diffraction methods. The structure has two symmetry independent Mn sites. The Mn1 site is seven coordinated by O and hosts, in addition to Mn2+, up to 20% Ca, whereas Mn2 has octahedral coordina- tion and is strongly selective for Mn2+. In the simplified formula, three smaller octahedral M sites are occupied by Al. However, M1 also accepts significant amounts of divalent cations, such as Cu, Mg, Fe, and Mn, whereas M2 is occupied exclusively by Al. The unit-cell parameters of sursassite are a = 8.698–8.728, b = 5.789–5.807, c = 9.778–9.812 Å, β = 108.879–109.060°, V = 465.7–470.0 Å3, the space group is P21/m.