Nak5cl2(S2O6)2 Revisited
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Mineral Classifications-No Links
CLASSIFYING MINERALS Minerals are divided into nine (9) broad classifications. They are typically classified based on the negatively charged (anionic) portion of their chemical composition. For example, copper oxide (CuO) consists of copper (Cu ++ ) and oxygen (O -- ) ions, and the negatively charged oxygen ion puts it in the “Oxide” classification (which also includes iron oxide, titanium dioxide, etc). The classifications are: Silicate class The largest group of minerals by far, the silicates are mostly composed of silicon and oxygen, combined with ions like aluminum, magnesium, iron, and calcium. Some important rock-forming silicates include the feldspars, quartz, olivines, pyroxenes, garnets, and micas. Carbonate class 2− The carbonate minerals contain the anion (CO 3) . They are deposited in marine settings from accumulated shells of marine life and also in evaporitic areas like the Great Salt Lake and karst regions where they form caves, stalactites and stalagmites. Typical carbonates include calcite and aragonite (both calcium carbonate), dolomite (magnesium/calcium carbonate) and siderite (iron carbonate). The carbonate class also includes the nitrate and borate minerals. Sulfate class 2− Sulfate minerals all contain the sulfate anion, SO 4 . Sulfates commonly form in evaporitic settings where highly saline waters slowly evaporate, in hydrothermal vein systems as gangue minerals and as secondary oxidation products of original sulfide minerals. Common sulfates include anhydrite (calcium sulfate), celestine (strontium sulfate), barite (barium sulfate), and gypsum (hydrated calcium sulfate). The sulfate class also includes the chromate, molybdate, selenate, sulfite, tellurate, and tungstate minerals. Halide class The halide minerals form the natural salts and include fluorite (calcium fluoride), halite (sodium chloride) and sylvite (potassium chloride). -
Access to Aryl Mellitic Acid Esters Through a Surprising Oxidative Esterification Reaction Margarita R
CORE Metadata, citation and similar papers at core.ac.uk Provided by Digital Repository @ Iowa State University Chemistry Publications Chemistry 2014 Access to Aryl Mellitic Acid Esters through a Surprising Oxidative Esterification Reaction Margarita R. Geraskina Iowa State University, [email protected] Mark James Juetten Iowa State University, [email protected] Arthur Winter Iowa State University, [email protected] Follow this and additional works at: http://lib.dr.iastate.edu/chem_pubs Part of the Materials Chemistry Commons, Other Chemistry Commons, and the Physical Chemistry Commons The ompc lete bibliographic information for this item can be found at http://lib.dr.iastate.edu/ chem_pubs/146. For information on how to cite this item, please visit http://lib.dr.iastate.edu/ howtocite.html. This Article is brought to you for free and open access by the Chemistry at Iowa State University Digital Repository. It has been accepted for inclusion in Chemistry Publications by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. Access to Aryl Mellitic Acid Esters through a Surprising Oxidative Esterification Reaction Abstract A serendipitously discovered oxidative esterification reaction of cyclohexane hexacarboxylic acid with phosphorus pentachloride and phenols provides one-pot access to previously unknown aryl mellitic acid esters. The er action features a solvent-free digestion and chromatography-free purifications and demonstrates the possibility of cyclohexane-to-benzene conversions under relatively mild, metal-free conditions. Disciplines Materials Chemistry | Other Chemistry | Physical Chemistry Comments Reprinted (adapted) with permission from J. Org. Chem., 2014, 79 (11), pp 5334–5337. Copyright 2014 American Chemical Society. -
(12) United States Patent (10) Patent No.: US 8.475,747 B1 Johnson Et Al
USOO8475747B1 (12) United States Patent (10) Patent No.: US 8.475,747 B1 Johnson et al. (45) Date of Patent: Jul. 2, 2013 (54) PROCESSING FISSILE MATERAL (56) References Cited MIXTURES CONTAINING ZIRCONUM AND/OR CARBON U.S. PATENT DOCUMENTS 3,012,849 A 12, 1961 Horn ................................. 423.4 Inventors: Michael Ernest Johnson, Richland, WA 3,965,237 A * 6/1976 Paige .......... ... 423f4 (75) 2003. O156675 A1* 8, 2003 Venneri et al. ... 376/189 (US); Martin David Maloney, 2003/0234223 A1* 12/2003 Kuraoka et al. .... ... 210,660 Evergreen, CO (US) 2007,0290.178 A1* 12/2007 Baron et al. ....... ... 252/643 2008/022410.6 A1* 9, 2008 Johnson et al. ... 252/625 (73) Assignee: U.S. Department of Energy, 2010/0314592 A1* 12/2010 Bourg et al. .................. 252,636 Washington, DC (US) OTHER PUBLICATIONS General Atomics & US DOE, “Development Plan for Advanced High (*) Notice: Subject to any disclaimer, the term of this Temperature Coated-Particle Fuels'. http://nuclearinl.gov/ patent is extended or adjusted under 35 deliverables/docs/pc-000513 0 relpdf, 2003.* U.S.C. 154(b) by 784 days. Pereira, Candido. “UREX-- Process Overview” www.ne.doe.gov/ pdfFiles/DOENRCUREXSeminar.pdfSimilar, Mar. 26, 2008.* Del Cul et al. “TRISO Coated Fuel Processing to Support High (21) Appl. No.: 12/484,561 Temperature Gas-Cooled Reactors.” http://nuclear.gov/peis/refer ences/RM923 DelCuletal 2002.pdf, p. 1-62, Mar. 2002.* (22) Filed: Jun. 15, 2009 Minato et al. “Retention of fission product caesium in ZrC-coated fuel particles for high-temperature gas-cooled reactors.” J. Nuclear Materials, 279, pp. -
Step Polymerization
Chapter 6 Step Polymerization The step polymerization builds up the molecular weight of polymer by stepwise function. Sometimes, the polymerization involves the release of small molecule by-product, so it is also called condensation polymerization. It is the earliest polymerization technique in the synthetic polymers. In 1907, Leo Baekeland of Germany created the first completely synthetic polymer, Bakelite, by reacting phenol and formaldehyde. It is also called phenolic resin. The molecular weight of the phenolic resin builds up stepwise by removing water. The product was com- mercialized in 1909 by forming a company bearing his name as Bakelite until present day. Table 6.1 lists some of the commercially important polymers prepared by step- reaction polymerization. The reaction mechanisms, kinetics of polyesters and polyamides have been thoroughly studied. Thus, we are discussing the degree of polymerization DP and the polymerization rate of step polymerization using these two polymers as examples. 6.1 Chemical Reactions and Reaction Mechanisms of Step Polymerization The type of products formed in step polymerization is determined by the func- tionality of the monomers, i.e., by the average number of reactive functional groups per monomer molecule. Monofunctional monomers give only low molecular weight products. Bifunctional monomers give linear polymers. Poly- functional monomers, with more than two functional groups per molecule, give branched or crosslinked polymers. The properties of the linear and the crosslinked polymers differ widely. -
Combustion of Organic Molecules by the Thermal Decomposition of Perchlorate Salts: Implications for Organics at the Mars Phoenix Scout Landing Site
COMBUSTION OF ORGANIC MOLECULES BY THE THERMAL DECOMPOSITION OF PERCHLORATE SALTS: IMPLICATIONS FOR ORGANICS AT THE MARS PHOENIX SCOUT LANDING SITE. D. W. Ming1, H. V. Lauer, Jr.2, P. D. Archer, Jr.3, B. Sutter4, D. C. Golden5, R. V. Morris1, P. B. Niles1, and W. V. Boynton4; 1NASA Johnson Space Center, Houston, TX 77058 ([email protected]), 2ESCG/Barrios Tech., Houston, TX, 3Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, 4Jacobs/ESCG, Houston, TX, 5ESCG/Hamilton Sundstrand, Houston, TX. Introduction: The Mars 2007 Phoenix Scout Mis- testbed to understand the effects of the thermal de- sion successfully landed on May 25, 2008 and oper- composition of perchlorate salts on organic molecules. ated on the northern plains of Mars for 150 sols. The Materials and Methods: A three component mix- primary mission objective was to study the history of ture was designed to simulate the thermal decomposi- water and evaluate the potential for past and present tion of perchlorate salt in the presence of organic mate- habitability in Martian arctic ice-rich soil [1]. Phoenix rial. The mixture consisted of 2.3 wt. % Mg- landed near 68° N latitude on polygonal terrain created perchlorate (Mg(ClO4)2.6H2O, 8.4 wt. % mellitic acid, by ice layers that are a few centimeters under loose and 87.3 wt. % SiO2. Mg-perchlorate was chosen be- soil materials. The Phoenix Mission is assessing the cause it is a leading candidate for the perchlorate salt potential for habitability by searching for organic in the Phoenix soils [3]. Mellitic acid (benzenehex- molecules in the ice or icy soils at the landing site. -
Mineralogy and Origin of Coarse-Grained Segregations in the Pyrometallurgical Zn-Pb Slags from Katowice-Wełnowiec (Poland)
Miner Petrol DOI 10.1007/s00710-016-0439-1 ORIGINAL PAPER Mineralogy and origin of coarse-grained segregations in the pyrometallurgical Zn-Pb slags from Katowice-Wełnowiec (Poland) R. Warchulski1 & A. Gawęda 1 & J. Janeczek1 & M. Kądziołka-Gaweł2 Received: 20 December 2015 /Accepted: 9 March 2016 # The Author(s) 2016. This article is published with open access at Springerlink.com Abstract The unique among pyrometallurgical slags, coarse- Introduction grained (up to 2.5 cm) segregations (up to 40 cm long) rimmed by Baplitic^ border zones occur within holocrystalline histor- Pyrometallurgical slags from base-metal smelting have recent- ical Zn-smelting slag in Katowice, S Poland. Slag surrounding ly been studied extensively mainly with the purpose of the segregations consists of olivine, spinel series, melilite, assessing their environmental impact for many of them con- clinopyroxene, leucite, nepheline and sulphides. Ca-oliv- tain elevated concentrations of potentially toxic metals, in- ines, kalsilite and mica compositionally similar to cluding As, Cd, Cu, Pb and Zn (e.g. Ettler et al. 2001; oxykinoshitalite occur in border zones in addition to Puziewicz et al. 2007; Álvarez-Valero et al. 2009,Piatakand olivine, spinel series and melilite. Miarolitic and mas- Seal 2010; Vítková et al. 2010;Kierczaketal.2010;Ettlerand sive pegmatite-like segregations are built of subhedral Johan 2014). Those metals may be partitioned among phases crystals of melilite, leucite, spinel series, clinopyroxene with different leaching potential during weathering. and hematite. Melilite, clinopyroxenes and spinels in the Therefore, the detailed knowledge of phase composition of segregationsareenrichedinZnrelativelytooriginal slags is prerequisite for understanding their leaching behav- slag and to fine-grained border zones. -
Deep UV Raman Spectroscopy for Planetary Exploration: the Search for in Situ Organics
Icarus 290 (2017) 201–214 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Deep UV Raman spectroscopy for planetary exploration: The search for in situ organics ∗ William J. Abbey a, Rohit Bhartia a, , Luther W. Beegle a, Lauren DeFlores a, Veronica Paez b, Kripa Sijapati c, Shakher Sijapati d, Kenneth Williford a, Michael Tuite a, William Hug c, Ray Reid c a Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive Ave, Pasadena, CA 91109, United States b Georgia Institute of Technology, North Ave NW, Atlanta, GA, 30332, United States c Photon Systems Inc.,1512 W Industrial Park St, Covina, CA 91722, United States d University of Wisconsin-Madison, Madison, WI 53706, United States a r t i c l e i n f o a b s t r a c t Article history: Raman spectroscopy has emerged as a powerful, non-contact, non-destructive technique for detection and Received 26 September 2016 characterization of in situ organic compounds. Excitation using deep UV wavelengths ( < 250 nm), in par- Revised 24 January 2017 ticular, offers the benefits of spectra obtained in a largely fluorescence-free region while taking advantage Accepted 26 January 2017 of signal enhancing resonance Raman effects for key classes of organic compounds, such as the aromatics. Available online 1 March 2017 In order to demonstrate the utility of this technique for planetary exploration and astrobiological appli- Keywords: cations, we interrogated three sets of samples using a custom built Raman instrument equipped with a Astrobiology deep UV (248.6 nm) excitation source. -
Options for Treatment of Legacy and Advanced
OPTIONS FOR TREATMENT OF LEGACY AND ADVANCED NUCLEAR FUELS A thesis submitted to the University of Manchester for the degree of in the Faculty of Engineering and Physical Sciences. 2014 CHRIS MAHER SCHOOL OF CHEMICAL ENGINEERING AND ANALYTICAL SCIENCE TABLE OF CONTENTS 1. INTRODUCTION ............................................................................ 22 2. OVERALL OBJECTIVES .................................................................. 26 3. TECHNOLOGY FOR THE HEAD-END TREATMENT OF LEGACY, CURRENT AND FUEL ADVANCED NUCLEAR FUELS ......................... 27 3.1. Aims and objectives .................................................................. 27 3.2. Science and technology of Head-End and influence of potential future challenges ............................................................................... 27 3.2.1. Introduction ..................................................................... 28 3.2.2. Current practice ................................................................ 31 3.2.2.1. Fuel conditioning ....................................................... 32 3.2.2.2. Dissolution ............................................................... 33 3.2.2.3. Dissolver liquor conditioning ....................................... 40 3.2.2.4. Accountancy and buffer storage .................................. 42 3.2.3. Potential developments to meet future challenges ................. 43 3.2.3.1. Dissolution chemistry of alternative fuel types .............. 44 3.2.3.2. Fuel conditioning - potential benefits -
The Missing Organic Molecules on Mars
The missing organic molecules on Mars Steven A. Benner*, Kevin G. Devine, Lidia N. Matveeva, and David H. Powell Departments of Chemistry, Anatomy, and Cell Biology, University of Florida, Gainesville, FL 32611 Communicated by Leslie Orgel, The Salk Institute for Biological Studies, San Diego, CA, December 13, 1999 (received for review November 4, 1998) GC-MS on the Viking 1976 Mars missions did not detect organic and with the irradiation of the surface by ultraviolet light, the molecules on the Martian surface, even those expected from failure to detect organic substances led many to conclude that meteorite bombardment. This result suggested that the Martian one must dig deeply (and perhaps very deeply) below the regolith might hold a potent oxidant that converts all organic Martian surface to have a chance of encountering any organic molecules to carbon dioxide rapidly relative to the rate at which molecules that may have arisen from life on Mars (perhaps they arrive. This conclusion is influencing the design of Mars present several billion years ago, when the surface of Mars was missions. We reexamine this conclusion in light of what is known more like the surface of Earth at that time and when life almost about the oxidation of organic compounds generally and the certainly had emerged on Earth) or of encountering organic nature of organics likely to come to Mars via meteorite. We molecules that may have been delivered to Mars via meteorite conclude that nonvolatile salts of benzenecarboxylic acids, and (9, 10). perhaps oxalic and acetic acid, should be metastable intermediates Because this interpretation is influencing the design of mis- of meteoritic organics under oxidizing conditions. -
Summer 1989 Gems & Gemology
VOLUME XXV SUMMER 1989 I The quarterly journal of the Gemological Institute of America SUMMER 1989 Volume 25 No. 2 TABLE OF CONTENTS EDITORIAL 67 New Challenges for the Diamond Industry Richard T Liddicoat FEATURE 68 The Characteristics and Identification ARTICLES of Filled Diamonds John I. Koivula, Robert C. Kam~nerling, Emmanuel Fritsch, C. W Fryer, David Hargett, and Robert E. Kane NOTES , , , 84 A Preliminary Gemological Study of AND NEW Synthetic Diamond Thin Films TECHNIQUES Emmanuel Fritsch, Laurie Conner, and John I. Koivula Grading the Hope Diamond Robert Crowningshield Contribution to the Identification of Treated Colored Diamonds: Diamonds with Peculiar Color-Zoned Pavilions Emmanuel Fritsch and lames E. Shigley REGULAR 102 Gem Trade Lab Notes FEATURES 109 Editorial Forum 110 Gem News 119 Book Reviews 120 Gemological Abstracts ABOUT THE COVER: Fine diamonds in fine jewelry -like this superb necklace and matching earclips -represent the heart of the jewelry industry. Because of the premier importance of diamonds, however, the rewards of making a diamond "better" are potentially very great. Although historically there have been numerous diamond substitutes, modern technology has led to new industries devoted to the treatment of natural diamonds. Three of the articles in this issue deal with some of the most important-or potentially important-diamond treatments. The fourth deals with one of the world's most notorious untreated diamonds: the Hope. The necklace (97.75 ct total weight) and earclips (24.63 ct total weight) are courtesy of Van Cleef ed Arpels. Photo @ Harold e'J Erica Van Pelt - Photographers, Los Angeles, CA. Typesetting for Gems & Gemology is by Scientific Composition, Los Angeles, CA. -
Degradable Chelants Having Sulfonate Groups, Uses and Compositions Thereof
Europa,schesP_ MM II M M MM I MM MM M M I M J European Patent Office «• o - B4 © Publication number: 0 516 102 B1 Office_„. europeen des brevets © EUROPEAN PATENT SPECIFICATION © Date of publication of patent specification: 10.05.95 © Int. CI.6: C07C 309/14, C1 1 D 3/34 © Application number: 92108980.1 @ Date of filing: 27.05.92 Degradable chelants having sulfonate groups, uses and compositions thereof. © Priority: 31.05.91 US 708534 © Proprietor: THE DOW CHEMICAL COMPANY 2030 Dow Center, @ Date of publication of application: Abbott Road 02.12.92 Bulletin 92/49 Midland, Michigan 48640 (US) © Publication of the grant of the patent: 10.05.95 Bulletin 95/19 @ Inventor: Crump, Druce K. 142 Oyster Creek Drive, Number 48 © Designated Contracting States: Lake Jackson, AT BE CH DE DK ES FR GB GR IT LI LU MC Texas 77566 (US) NL PT SE Inventor: Wilson, David A. 229 San Saba © References cited: Richwood, DE-A- 3 337 026 Texas 77531 (US) US-A- 3 091 522 US-A- 3 703 545 US-A- 3 726 912 © Representative: Huber, Bernhard, Dlpl.-Chem. et al Patentanwalte H. Weickmann, Dr. K. Fincke F.A. Weickmann, B. Huber Dr. H. Liska, Dr. J. Prechtel, Dr. B. Bohm Postfach 86 08 20 CD D-81635 Munchen (DE) CM O CO lo Note: Within nine months from the publication of the mention of the grant of the European patent, any person ® may give notice to the European Patent Office of opposition to the European patent granted. Notice of opposition Q,. -
List of Spectra /Compound Names
IS NIR Spectra Complete collection (6049 spectra) This collection includes all NIR spectra collected within this project. Those are organic and inorganic chemicals, pharmaceutical excipients, drugs, polymers, additives, coatings, dyes, pigments, toxic substances, hazardous substances like explosives, agrochemicals and other types of materials. This collection should be chosen by customers with broad range of analytical applications. The near infrared spectral library „IS NIR Spectra“ is a unique collection of 6049 NIR (near infrared) digital spectra. The spectra have been collected in range 4200-10000 cm-1 (=2.4 – 1 micrometers). „IS NIR Spectra“ is the biggest and newest NIR library available on the market. This spectral library has been designed for users who use their NIR spectrometer not only for quantitative and chemometric analysis, but also want to identify unknown samples or just want to use the library as reference spectra database. ra t IS means “Intergrating Sphere” and at the same time “Identify Samplec”. e Technical parameters: p The „IS NIR Spectra“ were collected using the FT-NIR Spectrometer equipped with Integrating Sphere Accessory. Resolution: standard 4cm-1 IR Customized resolution: upon special request the speNctra can be delivered in customized resolution to reach better correspondence with spectr a collected by customer NIR instrument Spectral range in wavenumbers units: 4200-1000I0S cm-1 Spectral range in wavelength units: 2.4 – 1 micr ometers Only one spectrum/compound covering the mentioned spectral range Typical text information about the sample inmcludes (when available): Compound name including synonyms o CAS number .c Chemical formula a Molecular weight tr Additional information about thec sample like manufacturer and comments.