CO2 Seq, Yeager Senior Thesis
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Washington State Minerals Checklist
Division of Geology and Earth Resources MS 47007; Olympia, WA 98504-7007 Washington State 360-902-1450; 360-902-1785 fax E-mail: [email protected] Website: http://www.dnr.wa.gov/geology Minerals Checklist Note: Mineral names in parentheses are the preferred species names. Compiled by Raymond Lasmanis o Acanthite o Arsenopalladinite o Bustamite o Clinohumite o Enstatite o Harmotome o Actinolite o Arsenopyrite o Bytownite o Clinoptilolite o Epidesmine (Stilbite) o Hastingsite o Adularia o Arsenosulvanite (Plagioclase) o Clinozoisite o Epidote o Hausmannite (Orthoclase) o Arsenpolybasite o Cairngorm (Quartz) o Cobaltite o Epistilbite o Hedenbergite o Aegirine o Astrophyllite o Calamine o Cochromite o Epsomite o Hedleyite o Aenigmatite o Atacamite (Hemimorphite) o Coffinite o Erionite o Hematite o Aeschynite o Atokite o Calaverite o Columbite o Erythrite o Hemimorphite o Agardite-Y o Augite o Calciohilairite (Ferrocolumbite) o Euchroite o Hercynite o Agate (Quartz) o Aurostibite o Calcite, see also o Conichalcite o Euxenite o Hessite o Aguilarite o Austinite Manganocalcite o Connellite o Euxenite-Y o Heulandite o Aktashite o Onyx o Copiapite o o Autunite o Fairchildite Hexahydrite o Alabandite o Caledonite o Copper o o Awaruite o Famatinite Hibschite o Albite o Cancrinite o Copper-zinc o o Axinite group o Fayalite Hillebrandite o Algodonite o Carnelian (Quartz) o Coquandite o o Azurite o Feldspar group Hisingerite o Allanite o Cassiterite o Cordierite o o Barite o Ferberite Hongshiite o Allanite-Ce o Catapleiite o Corrensite o o Bastnäsite -
Adamsite-(Y), a New Sodium–Yttrium Carbonate Mineral
1457 The Canadian Mineralogist Vol. 38, pp. 1457-1466 (2000) ADAMSITE-(Y), A NEW SODIUM–YTTRIUM CARBONATE MINERAL SPECIES FROM MONT SAINT-HILAIRE, QUEBEC JOEL D. GRICE§ and ROBERT A. GAULT Research Division, Canadian Museum of Nature, P.O. Box 3443, Station D, Ottawa, Ontario K1P 6P4, Canada ANDREW C. ROBERTS Geological Survey of Canada, 601 Booth Street, Ottawa, Ontario K1A 0E8, Canada MARK A. COOPER Department of Geological Sciences, University of Manitoba, Winnipeg, Manitoba R3T 2N2, Canada ABSTRACT Adamsite-(Y), ideally NaY(CO3)2•6H2O, is a newly identified mineral from the Poudrette quarry, Mont Saint-Hilaire, Quebec. It occurs as groups of colorless to white and pale pink, rarely pale purple, flat, acicular to fibrous crystals. These crystals are up to 2.5 cm in length and form spherical radiating aggregates. Associated minerals include aegirine, albite, analcime, ancylite-(Ce), calcite, catapleiite, dawsonite, donnayite-(Y), elpidite, epididymite, eudialyte, eudidymite, fluorite, franconite, gaidonnayite, galena, genthelvite, gmelinite, gonnardite, horváthite-(Y), kupletskite, leifite, microcline, molybdenite, narsarsukite, natrolite, nenadkevichite, petersenite-(Ce), polylithionite, pyrochlore, quartz, rhodochrosite, rutile, sabinaite, sérandite, siderite, sphalerite, thomasclarkite-(Y), zircon and an unidentified Na–REE carbonate (UK 91). The transparent to translucent mineral has a vitreous to pearly luster and a white streak. It is soft (Mohs hardness 3) and brittle with perfect {001} and good {100} and {010} cleav- ␣  ␥ ° ° ages. Adamsite-(Y) is biaxial positive, = V 1.480(4), = 1.498(2), = 1.571(4), 2Vmeas. = 53(3) , 2Vcalc. = 55 and is nonpleochroic. Optical orientation: X = [001], Y = b, Z a = 14° (in  obtuse). It is triclinic, space group P1,¯ with unit-cell parameters refined from powder data: a 6.262(2), b 13.047(6), c 13.220(5) Å, ␣ 91.17(4),  103.70(4), ␥ 89.99(4)°, V 1049.1(5) Å3 and Z = 4. -
Infrare D Transmission Spectra of Carbonate Minerals
Infrare d Transmission Spectra of Carbonate Mineral s THE NATURAL HISTORY MUSEUM Infrare d Transmission Spectra of Carbonate Mineral s G. C. Jones Department of Mineralogy The Natural History Museum London, UK and B. Jackson Department of Geology Royal Museum of Scotland Edinburgh, UK A collaborative project of The Natural History Museum and National Museums of Scotland E3 SPRINGER-SCIENCE+BUSINESS MEDIA, B.V. Firs t editio n 1 993 © 1993 Springer Science+Business Media Dordrecht Originally published by Chapman & Hall in 1993 Softcover reprint of the hardcover 1st edition 1993 Typese t at the Natura l Histor y Museu m ISBN 978-94-010-4940-5 ISBN 978-94-011-2120-0 (eBook) DOI 10.1007/978-94-011-2120-0 Apar t fro m any fair dealin g for the purpose s of researc h or privat e study , or criticis m or review , as permitte d unde r the UK Copyrigh t Design s and Patent s Act , 1988, thi s publicatio n may not be reproduced , stored , or transmitted , in any for m or by any means , withou t the prio r permissio n in writin g of the publishers , or in the case of reprographi c reproductio n onl y in accordanc e wit h the term s of the licence s issue d by the Copyrigh t Licensin g Agenc y in the UK, or in accordanc e wit h the term s of licence s issue d by the appropriat e Reproductio n Right s Organizatio n outsid e the UK. Enquirie s concernin g reproductio n outsid e the term s state d here shoul d be sent to the publisher s at the Londo n addres s printe d on thi s page. -
Adsorption of RNA on Mineral Surfaces and Mineral Precipitates
Adsorption of RNA on mineral surfaces and mineral precipitates Elisa Biondi1,2, Yoshihiro Furukawa3, Jun Kawai4 and Steven A. Benner*1,2,5 Full Research Paper Open Access Address: Beilstein J. Org. Chem. 2017, 13, 393–404. 1Foundation for Applied Molecular Evolution, 13709 Progress doi:10.3762/bjoc.13.42 Boulevard, Alachua, FL, 32615, USA, 2Firebird Biomolecular Sciences LLC, 13709 Progress Boulevard, Alachua, FL, 32615, USA, Received: 23 November 2016 3Department of Earth Science, Tohoku University, 2 Chome-1-1 Accepted: 15 February 2017 Katahira, Aoba Ward, Sendai, Miyagi Prefecture 980-8577, Japan, Published: 01 March 2017 4Department of Material Science and Engineering, Yokohama National University, 79-5 Tokiwadai, Hodogaya-ku, Yokohama This article is part of the Thematic Series "From prebiotic chemistry to 240-8501, Japan and 5The Westheimer Institute for Science and molecular evolution". Technology, 13709 Progress Boulevard, Alachua, FL, 32615, USA Guest Editor: L. Cronin Email: Steven A. Benner* - [email protected] © 2017 Biondi et al.; licensee Beilstein-Institut. License and terms: see end of document. * Corresponding author Keywords: carbonates; natural minerals; origins of life; RNA adsorption; synthetic minerals Abstract The prebiotic significance of laboratory experiments that study the interactions between oligomeric RNA and mineral species is difficult to know. Natural exemplars of specific minerals can differ widely depending on their provenance. While laboratory-gener- ated samples of synthetic minerals can have controlled compositions, they are often viewed as "unnatural". Here, we show how trends in the interaction of RNA with natural mineral specimens, synthetic mineral specimens, and co-precipitated pairs of synthe- tic minerals, can make a persuasive case that the observed interactions reflect the composition of the minerals themselves, rather than their being simply examples of large molecules associating nonspecifically with large surfaces. -
Alkalic Rocks of Iron Hill Gunnison County, Colorado
If yon do not need this publication after it has served your purpose, please return it to the Geological Survey, using the official mailing label at the end UNITED STATES DEPARTMENT OF THE INTERIOR ALKALIC ROCKS OF IRON HILL GUNNISON COUNTY, COLORADO GEOLOGICAL SURVEY PROFESSIONAL PAPER 197-A UNITED STATES DEPARTMENT OF THE INTERIOR Harold L. Ickes, Secretary GEOLOGICAL SURVEY W. C. Mendenhall, Director Professional Paper 197-A ALKALIC ROCKS OF IRON HILL GUNNISON COUNTY, COLORADO BY ESPER S. LARSEN Shorter contributions to general geology, 1941 (Pages 1-64) UNITED STATES GOVERNMENT PRINTING OFFICE WASHINGTON : 1942 For sale by the Superintendent of Documents, Washington, D. C. ......... Price 40 cents CONTENTS Page Preface, by G. F. Loughlin_________________________ v Other dike rocks_______________-____________________ 29 Abstract____"_--__-___--__________________________ 1 Augite syenite and shonkinite ____.__--___--__--__ 29 Introduction. ______________________________________ 1 Olivine gabbro. ________________________________ 30 Location and topography. _______________________ 1 Carbonate veins_________----__---------__--_---___- 31 Field work and acknowledgments.________________ 2 Character __ __________________________________ 31 Geology of the surrounding area__________________ 2 Origin _______ _ ____ _ __ _.. __ __. ___ .__. 31 Age of the Iron Hill stock_____________________ 2 Hydrothermal processes- ______--_-___-_---_--__-___- 31 General geology of the Iron Hill stock _____________ 3 The hydrothermal products. _____________________ -
Synthesis Methods and Favorable Conditions for Spherical Vaterite Precipitation: a Review
crystals Review Synthesis Methods and Favorable Conditions for Spherical Vaterite Precipitation: A Review Donata Konopacka-Łyskawa Department of Process Engineering and Chemical Technology, Faculty of Chemistry, Gda´nskUniversity of Technology, Narutowicza 11/12, 80-233 Gda´nsk,Poland; [email protected]; Tel.: +48-58-347-2910 Received: 15 March 2019; Accepted: 18 April 2019; Published: 25 April 2019 Abstract: Vaterite is the least thermodynamically stable anhydrous calcium carbonate polymorph. Its existence is very rare in nature, e.g., in some rock formations or as a component of biominerals produced by some fishes, crustaceans, or birds. Synthetic vaterite particles are proposed as carriers of active substances in medicines, additives in cosmetic preparations as well as adsorbents. Also, their utilization as a pump for microfluidic flow is also tested. In particular, vaterite particles produced as polycrystalline spheres have large potential for application. Various methods are proposed to precipitate vaterite particles, including the conventional solution-solution synthesis, gas-liquid method as well as special routes. Precipitation conditions should be carefully selected to obtain a high concentration of vaterite in all these methods. In this review, classical and new methods used for vaterite precipitation are presented. Furthermore, the key parameters affecting the formation of spherical vaterite are discussed. Keywords: vaterite; calcium carbonate; polymorph; precipitation; synthesis; carbonation 1. Introduction Vaterite is the least thermodynamically stable anhydrous calcium carbonate polymorph and it easily transforms into more stable calcite or aragonite in the presence of water. This form of calcium carbonate mineral was named to honor the German chemist and mineralogist, Heinrich Vater, in 1903. -
Carbon Mineral Ecology: Predicting the Undiscovered Minerals of Carbon
American Mineralogist, Volume 101, pages 889–906, 2016 Carbon mineral ecology: Predicting the undiscovered minerals of carbon ROBERT M. HAZEN1,*, DANIEL R. HUMMER1, GRETHE HYSTAD2, ROBERT T. DOWNS3, AND JOSHUA J. GOLDEN3 1Geophysical Laboratory, Carnegie Institution, 5251 Broad Branch Road NW, Washington, D.C. 20015, U.S.A. 2Department of Mathematics, Computer Science, and Statistics, Purdue University Calumet, Hammond, Indiana 46323, U.S.A. 3Department of Geosciences, University of Arizona, 1040 East 4th Street, Tucson, Arizona 85721-0077, U.S.A. ABSTRACT Studies in mineral ecology exploit mineralogical databases to document diversity-distribution rela- tionships of minerals—relationships that are integral to characterizing “Earth-like” planets. As carbon is the most crucial element to life on Earth, as well as one of the defining constituents of a planet’s near-surface mineralogy, we focus here on the diversity and distribution of carbon-bearing minerals. We applied a Large Number of Rare Events (LNRE) model to the 403 known minerals of carbon, using 82 922 mineral species/locality data tabulated in http://mindat.org (as of 1 January 2015). We find that all carbon-bearing minerals, as well as subsets containing C with O, H, Ca, or Na, conform to LNRE distributions. Our model predicts that at least 548 C minerals exist on Earth today, indicating that at least 145 carbon-bearing mineral species have yet to be discovered. Furthermore, by analyzing subsets of the most common additional elements in carbon-bearing minerals (i.e., 378 C + O species; 282 C + H species; 133 C + Ca species; and 100 C + Na species), we predict that approximately 129 of these missing carbon minerals contain oxygen, 118 contain hydrogen, 52 contain calcium, and more than 60 contain sodium. -
Nördlingen 2010: the Ries Crater, the Moon, and the Future of Human Space Exploration, P
Program and Abstract Volume LPI Contribution No. 1559 The Ries Crater, the Moon, and the Future of Human Space Exploration June 25–27, 2010 Nördlingen, Germany Sponsors Museum für Naturkunde – Leibniz-Institute for Research on Evolution and Biodiversity at the Humboldt University Berlin, Germany Institut für Planetologie, University of Münster, Germany Deutsches Zentrum für Luft- und Raumfahrt DLR (German Aerospace Center) at Berlin, Germany Institute of Geoscience, University of Freiburg, Germany Lunar and Planetary Institute (LPI), Houston, USA Deutsche Forschungsgemeinschaft (German Science Foundation), Bonn, Germany Barringer Crater Company, Decatur, USA Meteoritical Society, USA City of Nördlingen, Germany Ries Crater Museum, Nördlingen, Germany Community of Otting, Ries, Germany Märker Cement Factory, Harburg, Germany Local Organization City of Nördlingen Museum für Naturkunde – Leibniz- Institute for Research on Evolution and Biodiversity at the Humboldt University Berlin Ries Crater Museum, Nördlingen Center of Ries Crater and Impact Research (ZERIN), Nördlingen Society Friends of the Ries Crater Museum, Nördlingen Community of Otting, Ries Märker Cement Factory, Harburg Organizing and Program Committee Prof. Dieter Stöffler, Museum für Naturkunde, Berlin Prof. Wolf Uwe Reimold, Museum für Naturkunde, Berlin Dr. Kai Wünnemann, Museum für Naturkunde, Berlin Hermann Faul, First Major of Nördlingen Prof. Thomas Kenkmann, Freiburg Prof. Harald Hiesinger, Münster Prof. Tilman Spohn, DLR, Berlin Dr. Ulrich Köhler, DLR, Berlin Dr. David Kring, LPI, Houston Dr. Axel Wittmann, LPI, Houston Gisela Pösges, Ries Crater Museum, Nördlingen Ralf Barfeld, Chair, Society Friends of the Ries Crater Museum Lunar and Planetary Institute LPI Contribution No. 1559 Compiled in 2010 by LUNAR AND PLANETARY INSTITUTE The Lunar and Planetary Institute is operated by the Universities Space Research Association under a cooperative agreement with the Science Mission Directorate of the National Aeronautics and Space Administration. -
Carbonatites of the World, Explored Deposits of Nb and REE—Database and Grade and Tonnage Models
Carbonatites of the World, Explored Deposits of Nb and REE—Database and Grade and Tonnage Models By Vladimir I. Berger, Donald A. Singer, and Greta J. Orris Open-File Report 2009-1139 U.S. Department of the Interior U.S. Geological Survey U.S. Department of the Interior KEN SALAZAR, Secretary U.S. Geological Survey Suzette M. Kimball, Acting Director U.S. Geological Survey, Reston, Virginia: 2009 For product and ordering information: World Wide Web: http://www.usgs.gov/pubprod/ Telephone: 1-888-ASK-USGS For more information on the USGS—the Federal source for science about the Earth, its natural and living resources, natural hazards, and the environment: World Wide Web: http://www.usgs.gov/ Telephone: 1-888-ASK-USGS Suggested citation: Berger, V.I., Singer, D.A., and Orris, G.J., 2009, Carbonatites of the world, explored deposits of Nb and REE— database and grade and tonnage models: U.S. Geological Survey Open-File Report 2009-1139, 17 p. and database [http://pubs.usgs.gov/of/2009/1139/]. Any use of trade, product, or firm names is for descriptive purposes only and does not imply endorsement by the U.S. Government. ii Contents Introduction 1 Rules Used 2 Data Fields 2 Preliminary analysis: —Grade and Tonnage Models 13 Acknowledgments 16 References 16 Figures Figure 1. Location of explored Nb– and REE–carbonatite deposits included in the database and grade and tonnage models 4 Figure 2. Cumulative frequency of ore tonnages of Nb– and REE–carbonatite deposits 14 Figure 3 Cumulative frequency of Nb2O5 grades of Nb– and REE–carbonatite deposits 15 Figure 4 Cumulative frequency of RE2O3 grades of Nb– and REE–carbonatite deposits 15 Figure 4 Cumulative frequency of P2O5 grades of Nb– and REE–carbonatite deposits 16 Tables Table 1. -
Vigrishinite
Vigrishinite Zn2Ti4-xSi4O14(OH,H2O, 8 (x < 1) - Crystal Data: Triclinic. Point Group: 1 . As split and blocky rectangular or irregular plates flattened on (001), to 3 cm. Physical Properties: Cleavage: Perfect on {001}. Tenacity: Brittle. Fracture: Stepped. Hardness = 2.5-3 D(meas.) = 3.03(2) D(calc.) = 2.97 Optical Properties: Transparent to translucent. Color: Pale pink, yellowish pink, colorless. Streak: White. Luster: Vitreous. Optical Class: Biaxial (-). α = 1.755(5) β = 1.820(10) γ = 1.835(8) 2V(meas.) = 45(10)° 2V(calc.) = 50° Dispersion: r < v, strong. Pleochroism: None. - Cell Data: Space Group: P1 . a = 8.743(9) b = 8.698(9) c = 11.581(11) α = 91.54(8)° β = 98.29(8)° γ = 105.65(8)° Z = 2 X-ray Powder Pattern: Lovozero alkaline massif, Kola Peninsula, Russia. (similar to murmanite) 2.861 (100), 11.7 (67), 4.17 (65), 5.73 (54), 8.27 (50), 6.94 (43), 2.609 (30) Chemistry: (1) (1) Na2O 0.98 Al2O3 0.36 K2O 0.30 SiO2 32.29 CaO 0.56 TiO2 29.14 SrO 0.05 ZrO2 2.08 BaO 0.44 Nb2O5 7.34 MgO 0.36 F 0.46 MnO 2.09 H2O 9.1 ZnO 14.39 –O=F2 0.19 Fe2O3 2.00 Total 101.75 (1) Lovozero alkaline massif, Kola Peninsula, Russia; average of 9 electron microprobe analyses, H2O by modified Penfield method, corresponds to H7.42(Zn1.30Na0.23Mn0.22Ca0.07Mg0.07K0.05 3+ Ba0.02)Σ=1.96(Ti2.68Nb0.41Fe 0.18Zr0.12)Σ=3.39(Si3.95Al0.05)Σ=4O20.31F0.18. -
Properties of Minerals for Processing
2 C h a p t e r Properties of Minerals for Processing 2.1 SAMPLING Sampling is a process of obtaining a small portion from a large quantity of a similar material such that, it truly represents the composition of the whole lot. It is an important step before testing of any material in the laboratory. Sampling of homogeneous materials is easy as compared to heterogeneous materials and hence, has to be conducted carefully. It is so because unlike heterogeneous materials, homogeneous materials have a uniform composition. However, almost all metallurgical materials are heterogeneous in nature. 2.1.1 Sampling of Ores/Minerals The process of sampling is complicated because of the following reasons: (1) A large variety of constituents are present in ores and minerals. (2) There is a large variation in the distribution of these constituents throughout the material. (3) In many cases, weight of the sample may vary from, 0.5 to 5 gm or 10 gm. Small fraction from large quantity like 50 to 250 tonnes are not true representative of the entire lot. The size of the sample required for testing depends on the method of testing and the testing machine which is used. However, sampling may involve three operations, namely, crushing and/or grinding, mixing and finally cutting. These operations may be executed repeatedly wherein the quantity of sample can be reduced to a desired weight. Sampling should be based on the relation between maximum particle size and the amount of sample. The size of ore/mineral particles taken for sampling depends on uniformity of composition, i.e., if the composition is more uniform, smaller particle size of the sample is taken and vice versa. -
Zeolites in Tasmania
Mineral Resources Tasmania Tasmanian Geological Survey Record 1997/07 Tasmania Zeolites in Tasmania by R. S. Bottrill and J. L. Everard CONTENTS INTRODUCTION ……………………………………………………………………… 2 USES …………………………………………………………………………………… 2 ECONOMIC SIGNIFICANCE …………………………………………………………… 2 GEOLOGICAL OCCURRENCES ………………………………………………………… 2 TASMANIAN OCCURRENCES ………………………………………………………… 4 Devonian ………………………………………………………………………… 4 Permo-Triassic …………………………………………………………………… 4 Jurassic …………………………………………………………………………… 4 Cretaceous ………………………………………………………………………… 5 Tertiary …………………………………………………………………………… 5 EXPLORATION FOR ZEOLITES IN TASMANIA ………………………………………… 6 RESOURCE POTENTIAL ……………………………………………………………… 6 MINERAL OCCURRENCES …………………………………………………………… 7 Analcime (Analcite) NaAlSi2O6.H2O ……………………………………………… 7 Chabazite (Ca,Na2,K2)Al2Si4O12.6H2O …………………………………………… 7 Clinoptilolite (Ca,Na2,K2)2-3Al5Si13O36.12H2O ……………………………………… 7 Gismondine Ca2Al4Si4O16.9H2O …………………………………………………… 7 Gmelinite (Na2Ca)Al2Si4O12.6H2O7 ……………………………………………… 7 Gonnardite Na2CaAl5Si5O20.6H2O ………………………………………………… 10 Herschelite (Na,Ca,K)Al2Si4O12.6H2O……………………………………………… 10 Heulandite (Ca,Na2,K2)2-3Al5Si13O36.12H2O ……………………………………… 10 Laumontite CaAl2Si4O12.4H2O …………………………………………………… 10 Levyne (Ca2.5,Na)Al6Si12O36.6H2O ………………………………………………… 10 Mesolite Na2Ca2(Al6Si9O30).8H2O ………………………………………………… 10 Mordenite K2.8Na1.5Ca2(Al9Si39O96).29H2O ………………………………………… 10 Natrolite Na2(Al2Si3O10).2H2O …………………………………………………… 10 Phillipsite (Ca,Na,K)3Al3Si5O16.6H2O ……………………………………………… 11 Scolecite CaAl2Si3O10.3H20 ………………………………………………………