High Temperature Sulfate Minerals Forming on the Burning Coal Dumps from Upper Silesia, Poland
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IMA Commission on New Minerals, Nomenclature and Classification (CNMNC)
Mineralogical Magazine, August 2015, Vol. 79(4), pp. 941À947 CNMNC Newsletter IMA Commission on New Minerals, Nomenclature and Classification (CNMNC) NEWSLETTER 26 New minerals and nomenclature modifications approved in 2015 1 2 3 U. HA˚ LENIUS (Chairman, CNMNC), F. HATERT (Vice-Chairman, CNMNC), M. PASERO (Vice-Chairman, 4 CNMNC) AND S. J. MILLS (Secretary, CNMNC) 1 Department of Mineralogy, Naturhistoriska Riksmuseet, Box 50007, SE-104 05 Stockholm, Sweden – [email protected] 2 Laboratoire de Mine´ralogie, Universite´ de Lie`ge, B-4000 Lie`ge, Belgium À [email protected] 3 Dipartimento di Scienze della Terra, Universita` degli Studi di Pisa, Via Santa Maria 53, I-56126 Pisa, Italy À [email protected] 4 Geosciences, Museum Victoria, PO Box 666, Melbourne, Victoria 3001, Australia À [email protected] The information given here is provided by the IMA Commission on New Minerals, Nomenclature and Classification for comparative purposes and as a service to mineralogists working on new species. Each mineral is described in the following format: Mineral name, if the authors agree on its release prior to the full description appearing in press Chemical formula Type locality Full authorship of proposal E-mail address of corresponding author Relationship to other minerals Crystal system, Space group; Structure determined, yes or no Unit-cell parameters Strongest lines in the X-ray powder diffraction pattern Type specimen repository and specimen number Citation details for the mineral prior to publication of full description Citation details concern the fact that this information will be published in the Mineralogical Magazine on a routine basis, as well as being added month by month to the Commission’s web site. -
New Mineral Names*,†
American Mineralogist, Volume 104, pages 625–629, 2019 New Mineral Names*,† DMITRIY I. BELAKOVSKIY1 AND FERNANDO CÁMARA2 1Fersman Mineralogical Museum, Russian Academy of Sciences, Leninskiy Prospekt 18 korp. 2, Moscow 119071, Russia 2Dipartimento di Scienze della Terra “Ardito Desio”, Universitá di degli Studi di Milano, Via Mangiagalli, 34, 20133 Milano, Italy IN THIS ISSUE This New Mineral Names has entries for 8 new minerals, including fengchengite, ferriperbøeite-(Ce), genplesite, heyerdahlite, millsite, saranchinaite, siudaite, vymazalováite and new data on lavinskyite-1M. FENGCHENGITE* X-ray diffraction pattern [d Å (I%; hkl)] are: 7.186 (55; 110), 5.761 (44; 113), 4.187 (53; 123), 3.201 (47; 028), 2.978 (61; 135). 2.857 (100; 044), G. Shen, J. Xu, P. Yao, and G. Li (2017) Fengchengite: A new species with 2.146 (30; 336), 1.771 (36; 24.11). Single-crystal X-ray diffraction data the Na-poor but vacancy-dominante N(5) site in the eudialyte group. shows the mineral is trigonal, space group R3m, a = 14.2467 (6), c = Acta Mineralogica Sinica, 37 (1/2), 140–151. 30.033(2) Å, V = 5279.08 Å3, Z = 3. The structure was solved by direct methods and refined to R = 0.043 for all unique I > 2σ(I) reflections. Fengchengite (IMA 2007-018a), Na Ca (Fe3+,) Zr Si (Si O ) 12 3 6 3 3 25 73 Fenchengite is the Fe3+ analog of eudialyte with a structural difference (H O) (OH) , trigonal, is a new eudialyte-group mineral discovered in 2 3 2 in vacancy dominant N5 site and splitting its Na site N1 into N1a and the agpaitic nepheline syenites and its pegmatite facies near the Saima N1b sites. -
Mirabilite Na2so4 • 10H2O C 2001-2005 Mineral Data Publishing, Version 1
Mirabilite Na2SO4 • 10H2O c 2001-2005 Mineral Data Publishing, version 1 Crystal Data: Monoclinic. Point Group: 2/m. Crystals short to long prismatic, with complex form development, also crude, to 10 cm, in interlocking masses; crystalline, granular to compact massive, commonly as efflorescences. Twinning: Rare on {001} or {100}. Physical Properties: Cleavage: On {100}, perfect; on {010} and {001}, good to fair. Fracture: Conchoidal. Hardness = 1.5–2.5 D(meas.) = 1.464 D(calc.) = 1.467 Quickly dehydrates to th´enarditein dry air; very soluble in H2O, taste cool, then saline and bitter. Optical Properties: Transparent to opaque. Color: Colorless to white; colorless in transmitted light. Streak: White. Luster: Vitreous. Optical Class: Biaxial (–). Orientation: X = b; Z ∧ c =31◦. Dispersion: r< v,strong, crossed. α = 1.391–1.394 β = 1.394–1.396 γ = 1.396–1.398 2V(meas.) = 75◦560 Cell Data: Space Group: P 21/c (synthetic). a = 11.512(3) b = 10.370(3) c = 12.847(2) β = 107.789(10)◦ Z=4 X-ray Powder Pattern: Synthetic. (ICDD 11-647). 5.49 (100), 3.21 (75), 3.26 (60), 3.11 (60), 4.77 (45), 3.83 (40), 2.516 (35) Chemistry: (1) (2) SO3 25.16 24.85 Na2O 18.67 19.24 H2O 55.28 55.91 Total 99.11 100.00 • (1) Kirkby Thore, Westmoreland, England. (2) Na2SO4 10H2O. Occurrence: Typically in salt pans, playas, and saline lakes, where deposition may be seasonal, and bedded deposits formed therefrom; rarely in caves and lava tubes; in volcanic fumaroles; a product of hydrothermal sericitic alteration; a post-mining precipitate. -
Euchlorine Knacu3o(SO4)3 C 2001-2005 Mineral Data Publishing, Version 1
Euchlorine KNaCu3O(SO4)3 c 2001-2005 Mineral Data Publishing, version 1 Crystal Data: Monoclinic. Point Group: 2/m. As crystals, tabular on {001}, with rectangular outline, to 2 mm; typically as an incrustation. Physical Properties: Cleavage: In two directions. Hardness = n.d. D(meas.) = 3.27 D(calc.) = 3.28 Soluble in H2O. Optical Properties: Semitransparent. Color: Emerald-green; emerald-green in transmitted light. Optical Class: Biaxial (+). Pleochroism: X = pale grass-green; Y = grass-green; Z = bright yellow-green. α = 1.580 β = 1.605 γ = 1.644 2V(meas.) = Moderately large. Cell Data: Space Group: C2/a. a = 18.41(5) b = 9.43(3) c = 14.21(5) β = 113.7(3)◦ Z=8 X-ray Powder Pattern: Vesuvius, Italy. 8.44 (100), 2.816 (47), 2.544 (45), 2.843 (40), 2.852 (37), 3.475 (30), 3.237 (25) Chemistry: (1) (2) SO3 41.41 43.13 Al2O3 0.06 CuO 43.69 42.85 MgO 0.17 CaO 0.07 Na2O 6.35 5.56 K2O 8.25 8.46 Total [100.00] 100.00 (1) Vesuvius, Italy; by electron microprobe, average of seven analyses, recalculated to 100% 2− from an original total of 101.86%, (SO4) shown present by IR; corresponds to K1.01Na1.18 Mg0.02Ca0.01Cu3.15O1.27(SO4)3. (2) KNaCu3O(SO4)3. Occurrence: A rare sublimate around volcanic fumaroles. Association: Dolerophanite, eriochalcite, chalcocyanite, melanothallite (Vesuvius, Italy); stoiberite, fingerite, ziesite, th´enardite,mcbirneyite (Izalco volcano, El Salvador); eriochalcite, melanothallite, fedotovite, vergasovaite, chalcocyanite, dolerophanite, tenorite, cuprian anglesite, gold (Tolbachik volcano, Russia). -
A Mineralogy of Anthropocene E
1 A Minerology for the Anthropocene Pierre FLUCK Institut Universitaire de France / Docteur-ès-Sciences / geologist and archeologist / Emeritus Professor at Université de Haute-Alsace This essay is a follow-up on « La signature stratigraphique de l’Anthropocène », which is also available on HAL- Archives ouvertes. Table of contents 1. Introduction: neoformation minerals in ancient mining galleries 2. Minerals from burning coal mines 3. Minerals from the mineral processing industry 4 ...and metallurgy 5. Neoformations in slags 6. Speciation of heavy metals in soils 7. Metal objects in their archaeological environment, or affected by fire 8. Neoformations in or on the surface of building stones 9. A mineralogy of materials. The “miracle of the potter”. The minerals in cement 10. A mineralogy of the biosphere? Conclusions Warning. This paper is written to be read by both specialists and a wider audience. However, it contains many mineral names. While these may resonate in the minds of mineralogists or collectors, they may not be as meaningful to less discerning readers. Such readers should not be scared, for they may find excellent encyclopaedic records on the web, including chemical composition, crystallographic properties and description of each of these species. This is why we have decided not to include further information in this paper. Acknowledgements. I would like to thank the mineralogists with whom I have had the opportunity to maintain fruitful exchanges for a long time: my pupil Hubert Bari, Éric Asselborn, Cédric Lheur, François Farges. And I would like to honour the memories of René Weil (1901-1983), my master in descriptive mineralogy, and of Jacques Geffroy (1918-1993), pupil of Alfred Lacroix, my master in metallogeny. -
Salt Crystallization in Porous Construction Materials I Estimation of Crystallization Pressure
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by EPrints Complutense Salt crystallization in porous construction materials I Estimation of crystallization pressure A. La Iglesiaa,*, V. Gonzalezb, V. L6pez-Acevedoc, C. Viedmac , Inslituto de Geologia Economica del CSIC, Facultad de Ciencias Ge% gicas, UCM, E·280411 Madrid. Spain b Deparlamento de Quimica, ETSI, Agronomos, UPM, E·28IJ40 Madrid, Spain , Deparlamenlo de Cristalografia y Mineralogia, Facultad de Ciencias Ge% gicas, UCM. E·28040 Madrid, Spain Abstract The crystallization process of soluble salts inside the natural and artificial porous materials partially immersed in different saline solutions has been studied, This procedure is used to simulate the conditions of exposure to salt weathering in which foundations and lower walls of building structures are within the zone of capillary rise of saline ground water. Crystallization pressures that can develop in the samples, which are a function of the pore size and salt-solution interfacial tension, have been calculated and are compared with experimental values of the materials tensile strength. since both these parameters allow the prediction of porous materials behaviour against salt weathering. Keywords: Salt weathering; Porous media; Salt crystallization; Crystallization pressure 1. Introduction The problem of crystallization pressure of salt was first studied by Correns [6J, who presented The crystallization process of soluble salts in a workable equation based on the Riecke principle porous materials can generate pressures inside the from which the pressure generated P versus salt pores sufficient to exceed the elastic limit of the supersaturation may be calculated: material, causing its breakage. -
Copper Oxosulphates from Fumaroles of Tolbachik Volcano
Eur. J. Mineral. 2017, 29, 499–510 Published online 10 January 2017 Copper oxosulphates from fumaroles of Tolbachik volcano: puninite, Na2Cu3O(SO4)3 – a new mineral species and structure refinements of kamchatkite and alumoklyuchevskite 1,* 1 2 1 OLEG I. SIIDRA ,EVGENII V. NAZARCHUK ,ANATOLY N. ZAITSEV ,EVGENIYA A. LUKINA , 1 3 4 1 EVGENIYA Y. AVDONTSEVA ,LIDIYA P. VERGASOVA ,NATALIA S. VLASENKO ,STANISLAV K. FILATOV , 5 3 RICK TURNER and GENNADY A. KARPOV 1 Department of Crystallography, St. Petersburg State University, University emb. 7/9, 199034 St. Petersburg, Russia *Corresponding author, e-mail: [email protected] 2 Department of Mineralogy, St. Petersburg State University, University emb. 7/9, 199034 St. Petersburg, Russia 3 Institute of Volcanology and Seismology, Russian Academy of Sciences, Bulvar Piypa 9, 683006 Petropavlovsk-Kamchatskiy, Russia 4 Research Park, Resource Centre Geomodel, St. Petersburg State University, University emb. 7/9, 199034 St. Petersburg, Russia 5 The Drey, Allington Track, Allington, Salisbury SP4 0DD, Wiltshire, UK Abstract: Typical characteristics of many anhydrous sulphates of exhalative origin at fumaroles at the Second scoria cone of the Northern Breakthrough of the Great Tolbachik Fissure Eruption, Tolbachik volcano, Kamchatka, Russia, are the presence of additional oxygen atoms (Oa) in the composition. Recent field works on the fumaroles of the Second scoria cone in 2014 and 2015 resulted in discovery of a new mineral species, puninite, and collection of fresh alumoklyuchevskite and kamchatkite samples which allowed the re-refinement of crystal structures. The crystal structure of kamchatkite, KCu3O(SO4)2Cl, was solved and refined in Pnma 3 space group (a = 9.755(2), b = 7.0152(15), c = 12.886(3) Å, V = 881.8(3) Å , R1 = 0.021), whereas alumoklyuchevskite, K3Cu3 AlO2(SO4)4, is triclinic, P1(a = 4.952(3), b = 11.978(6), c = 14.626(12) Å, a = 87.119(9), b = 80.251(9), g = 78.070(9)°, V = 836.3 3 (9) Å , R1 = 0.049) in contrast to previously reported data. -
Barite (Barium)
Barite (Barium) Chapter D of Critical Mineral Resources of the United States—Economic and Environmental Geology and Prospects for Future Supply Professional Paper 1802–D U.S. Department of the Interior U.S. Geological Survey Periodic Table of Elements 1A 8A 1 2 hydrogen helium 1.008 2A 3A 4A 5A 6A 7A 4.003 3 4 5 6 7 8 9 10 lithium beryllium boron carbon nitrogen oxygen fluorine neon 6.94 9.012 10.81 12.01 14.01 16.00 19.00 20.18 11 12 13 14 15 16 17 18 sodium magnesium aluminum silicon phosphorus sulfur chlorine argon 22.99 24.31 3B 4B 5B 6B 7B 8B 11B 12B 26.98 28.09 30.97 32.06 35.45 39.95 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 potassium calcium scandium titanium vanadium chromium manganese iron cobalt nickel copper zinc gallium germanium arsenic selenium bromine krypton 39.10 40.08 44.96 47.88 50.94 52.00 54.94 55.85 58.93 58.69 63.55 65.39 69.72 72.64 74.92 78.96 79.90 83.79 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 rubidium strontium yttrium zirconium niobium molybdenum technetium ruthenium rhodium palladium silver cadmium indium tin antimony tellurium iodine xenon 85.47 87.62 88.91 91.22 92.91 95.96 (98) 101.1 102.9 106.4 107.9 112.4 114.8 118.7 121.8 127.6 126.9 131.3 55 56 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 cesium barium hafnium tantalum tungsten rhenium osmium iridium platinum gold mercury thallium lead bismuth polonium astatine radon 132.9 137.3 178.5 180.9 183.9 186.2 190.2 192.2 195.1 197.0 200.5 204.4 207.2 209.0 (209) (210)(222) 87 88 104 105 106 107 108 109 110 111 112 113 114 115 116 -
Mineralogy of the Martian Surface
EA42CH14-Ehlmann ARI 30 April 2014 7:21 Mineralogy of the Martian Surface Bethany L. Ehlmann1,2 and Christopher S. Edwards1 1Division of Geological & Planetary Sciences, California Institute of Technology, Pasadena, California 91125; email: [email protected], [email protected] 2Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109 Annu. Rev. Earth Planet. Sci. 2014. 42:291–315 Keywords First published online as a Review in Advance on Mars, composition, mineralogy, infrared spectroscopy, igneous processes, February 21, 2014 aqueous alteration The Annual Review of Earth and Planetary Sciences is online at earth.annualreviews.org Abstract This article’s doi: The past fifteen years of orbital infrared spectroscopy and in situ exploration 10.1146/annurev-earth-060313-055024 have led to a new understanding of the composition and history of Mars. Copyright c 2014 by Annual Reviews. Globally, Mars has a basaltic upper crust with regionally variable quanti- by California Institute of Technology on 06/09/14. For personal use only. All rights reserved ties of plagioclase, pyroxene, and olivine associated with distinctive terrains. Enrichments in olivine (>20%) are found around the largest basins and Annu. Rev. Earth Planet. Sci. 2014.42:291-315. Downloaded from www.annualreviews.org within late Noachian–early Hesperian lavas. Alkali volcanics are also locally present, pointing to regional differences in igneous processes. Many ma- terials from ancient Mars bear the mineralogic fingerprints of interaction with water. Clay minerals, found in exposures of Noachian crust across the globe, preserve widespread evidence for early weathering, hydrothermal, and diagenetic aqueous environments. Noachian and Hesperian sediments include paleolake deposits with clays, carbonates, sulfates, and chlorides that are more localized in extent. -
The Partnership of Smithson Tennant and William Hyde Wollaston
“A History of Platinum and its Allied Metals”, by Donald McDonald and Leslie B. Hunt 9 The Partnership of Smithson Tennant and William Hyde Wollaston “A quantity of platina was purchased by me a few years since with the design of rendering it malleable for the different purposes to which it is adapted. That object has now been attained. ” WILLIAM HYDE W O L L A S T O N Up to the end of the eighteenth century the attempts to produce malleable platinum had advanced mainly in the hands of practical men aiming at its pre paration and fabrication rather than at the solution of scientific problems. These were now to be attacked with a marked degree of success by two remarkable but very different men who first became friends during their student days at Cam bridge and who formed a working partnership in 1800 designed not only for scientific purposes but also for financial reasons. They were of the same genera tion and much the same background as the professional scientists of London whose work was described in Chapter 8, and to whom they were well known, but with the exception of Humphry Davy they were of greater stature and made a greater advance in the development of platinum metallurgy than their predecessors. Their combined achievements over a relatively short span of years included the successful production for the first time of malleable platinum on a truly com mercial scale as well as the discovery of no less than four new elements contained in native platinum, a factor that was of material help in the purification and treatment of platinum itself. -
I Identification and Characterization of Martian Acid-Sulfate Hydrothermal
Identification and Characterization of Martian Acid-Sulfate Hydrothermal Alteration: An Investigation of Instrumentation Techniques and Geochemical Processes Through Laboratory Experiments and Terrestrial Analog Studies by Sarah Rose Black B.A., State University of New York at Buffalo, 2004 M.S., State University of New York at Buffalo, 2006 A thesis submitted to the Faculty of the Graduate School of the University of Colorado in partial fulfillment of the requirement for the degree of Doctor of Philosophy Department of Geological Sciences 2018 i This thesis entitled: Identification and Characterization of Martian Acid-Sulfate Hydrothermal Alteration: An Investigation of Instrumentation Techniques and Geochemical Processes Through Laboratory Experiments and Terrestrial Analog Studies written by Sarah Rose Black has been approved for the Department of Geological Sciences ______________________________________ Dr. Brian M. Hynek ______________________________________ Dr. Alexis Templeton ______________________________________ Dr. Stephen Mojzsis ______________________________________ Dr. Thomas McCollom ______________________________________ Dr. Raina Gough Date: _________________________ The final copy of this thesis has been examined by the signatories, and we find that both the content and the form meet acceptable presentation standards of scholarly work in the above mentioned discipline. ii Black, Sarah Rose (Ph.D., Geological Sciences) Identification and Characterization of Martian Acid-Sulfate Hydrothermal Alteration: An Investigation -
Cement Render and Mortar and Their Damages Due to Salt Crystallization in the Holy Trinity Church, Dominicans Monastery in Cracow, Poland
minerals Article Cement Render and Mortar and Their Damages Due to Salt Crystallization in the Holy Trinity Church, Dominicans Monastery in Cracow, Poland Mariola Marszałek * , Krzysztof Dudek and Adam Gaweł Department of Mineralogy, Petrography and Geochemistry, AGH University of Science and Technology, al. Mickiewicza 30, 30-059 Kraków, Poland; [email protected] (K.D.); [email protected] (A.G.) * Correspondence: [email protected] Received: 22 June 2020; Accepted: 17 July 2020; Published: 20 July 2020 Abstract: The investigations focused on the façade of the 17th-century Myszkowskis chapel at the 13th-century Church of the Holy Trinity in Cracow, Poland. Most of the chapel’s façade is made of rusticated limestone blocks, but its lower part is covered with cement render, and the basement consists of irregular pieces of limestone and sandstone, bound and partly replaced with cement mortar. The façade exhibited clearly visible damages: gray soiling of the surface, cracks, scaling, and efflorescence. The study presents characteristics of the cement render and mortar used for stone repair and/or substitution, as well as efflorescence from the lower part of the Myszkowskis chapel façade. The materials were analyzed with optical microscopy, scanning electron microscopy (SEM-EDS), Raman microspectroscopy, X-ray diffractometry (XRPD), and mercury intrusion porosimetry. The analyses demonstrated that the render covering some of the decayed limestone blocks was prepared using Portland cement (residual clinker grains represent alite and belite) as a binding agent, mixed with crushed stone as an aggregate. The cement mortar consisted of rounded quartz grains, rock fragments, and feldspars in very fine-grained masses of calcite and gypsum, also containing relics of cement clinker (alite, belite, ferrite, and aluminate).