The Rare Earth and Actinoid Elements
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Rainbow 18C PT 0318 Ad Ge訂正
1 18 1 H 2 He 1.008 4.003 hydrogen Rainbow Periodic Table helium 2.20 +1 guide☆ 1 with Quad electron data atomic number 82 Pb symbol 1 atomic weight 207.2 categories(Wikipedia): 2 -1 2 name 13 14 15 16 17 lead known oxidation state Alkali metals Post-transition metals 3 Li 4 Be electronegativity 2.33 +4 highest Alkaline earth metals Metalloids 5 B 6 C 7 N 8 O 9 F 10 Ne 14 [ ]:common Transition metals Reactive nonmetals 6.941 9.012 Quad electron data 10.81 12.01 14.01 16.00 19.00 20.18 lithium beryllium 2 10 [ ]:uncommon Lanthanides Noble gases boron carbon nitrogen oxygen fluorine neon 14 10 2 2 2 2 0.98 +1 1.57 +2 [Xe] 4f 5d 6s 6p [Xe] -4 lowest Actinides Unknown chemical properties 2.04 +3 2.55 +4 3.04 +5 3.44 +2 3.98 -1 shells 1 2 3 4 5 6 1 2 l=3 2 2 2 2 2 2 [He] +1 [He] +1 n=1 n=2 n=3 n=4 n=5 n=6 n=7 n=8 [He] -5 [He] -4 [He] -3 [He] -2 [He] -1 [He] f 11 Na 12 Mg orbitals l=1 p d l=2 13 Al 14 Si 15 P 16 S 17 Cl 18 Ar 22.99 24.31 s 26.98 28.09 30.97 32.07 35.45 39.95 sodium magnesium K L M N O P Q R aluminium silicon phosphorus sulfur chlorine argon 0.93 +1 1.31 +2 l=0 nickname*: 'Ketchup' 'MustardYellow' 'Ocean Blue' 'Quin Violet' 1.61 +3 1.90 +4 2.19 +5 2.58 +6 3.16 +7 3 'Ladyfinger' 'NatureGreen' 'Pansy Blue' 'Ricecake' * suggested by Valery Tsimmerman 1 2 3 4 5 6 1 2 2 2 2 2 2 2 [Ne] -1 [Ne] +1 3 4 5 6 7 8 9 10 11 12 [Ne] -2 [Ne] -4 [Ne] -3 [Ne] -2 [Ne] -1 [Ne] 19 K 20 Ca 21 Sc 22 Ti 23 V 24 Cr 25 Mn 26 Fe 27 Co 28 Ni 29 Cu 30 Zn 31 Ga 32 Ge 33 As 34 Se 35 Br 36 Kr 39.10 40.08 44.96 47.87 50.94 52.00 54.94 55.85 58.93 58.69 63.55 -
Classification of Elements and Periodicity in Properties
74 CHEMISTRY UNIT 3 CLASSIFICATION OF ELEMENTS AND PERIODICITY IN PROPERTIES The Periodic Table is arguably the most important concept in chemistry, both in principle and in practice. It is the everyday support for students, it suggests new avenues of research to After studying this Unit, you will be professionals, and it provides a succinct organization of the able to whole of chemistry. It is a remarkable demonstration of the fact that the chemical elements are not a random cluster of • appreciate how the concept of entities but instead display trends and lie together in families. grouping elements in accordance to An awareness of the Periodic Table is essential to anyone who their properties led to the wishes to disentangle the world and see how it is built up development of Periodic Table. from the fundamental building blocks of the chemistry, the understand the Periodic Law; • chemical elements. • understand the significance of atomic number and electronic Glenn T. Seaborg configuration as the basis for periodic classification; • name the elements with In this Unit, we will study the historical development of the Z >100 according to IUPAC Periodic Table as it stands today and the Modern Periodic nomenclature; Law. We will also learn how the periodic classification • classify elements into s, p, d, f follows as a logical consequence of the electronic blocks and learn their main configuration of atoms. Finally, we shall examine some of characteristics; the periodic trends in the physical and chemical properties • recognise the periodic trends in of the elements. physical and chemical properties of elements; 3.1 WHY DO WE NEED TO CLASSIFY ELEMENTS ? compare the reactivity of elements • We know by now that the elements are the basic units of all and correlate it with their occurrence in nature; types of matter. -
How Earth Got Its Moon Article
FEATURE How Earth Got its MOON Standard formation tale may need a rewrite By Thomas Sumner he moon’s origin story does not add up. Most “Multiple impacts just make more sense,” says planetary scientists think that the moon formed in the earli- scientist Raluca Rufu of the Weizmann Institute of Science in est days of the solar system, around 4.5 billion years Rehovot, Israel. “You don’t need this one special impactor to Tago, when a Mars-sized protoplanet called Theia form the moon.” whacked into the young Earth. The collision sent But Theia shouldn’t be left on the cutting room floor just debris from both worlds hurling into orbit, where the rubble yet. Earth and Theia were built largely from the same kind of eventually mingled and combined to form the moon. material, new research suggests, and so had similar composi- If that happened, scientists expect that Theia’s contribution tions. There is no sign of “other” material on the moon, this would give the moon a different composition from Earth’s. perspective holds, because nothing about Theia was different. Yet studies of lunar rocks show that Earth and its moon are “I’m absolutely on the fence between these two opposing compositionally identical. That fact throws a wrench into the ideas,” says UCLA cosmochemist Edward Young. Determining planet-on-planet impact narrative. which story is correct is going to take more research. But the Researchers have been exploring other scenarios. Maybe answer will offer profound insights into the evolution of the the Theia impact never happened (there’s no direct evidence early solar system, Young says. -
Selective Radiation from Various Substances, Iii
. SELECTIVE RADIATION FROM VARIOUS SUBSTANCES, III By W. W. Coblentz CONTENTS Page. I. Introduction 243 II. Apparatus and Methods 244 1 The Spectrometer 244 2. Comparison of Dispersion of Prisms 246 3. The Radiometers 247 4. The Rotating Sectored Disk 249 5. Accuracy Attainable 252 III. The Acetylene Flame.' 253 1 Historical 253 2. The Visible Spectrum 257 3. The Emissivity a Function of the Thickness of the Radiating Layer. 261 4. Comparison of Acetylene Flame and a Solid Radiator 264 5. Absorptivity of an Acetylene Flame 266 6. Summary 273 IV. The Selective Emission oif the Welsbach Mantle 274 1 Historical 274 2. The Visible Spectrum 277 3. Comparison of a Gas Mantle with a Solid Glower 278 V. Miscellaneous Substances 287 1 Emission of Arc of Nemst Glower Materials 287 2. Color Match Versus Spectral Intensity Match 288 I. INTRODUCTION The present investigation is the beginning of an attempt to supply a long-felt need of an accurate knov/ledge of the spectral energy distribution, of some standard sources of Hght, in the visible and in the ultra-violet parts of the spectrum. The problem is a difficult one and heretofore has never been given thorough attention. Once the spectral energy distribution of a standard source of illumination is accurately known, it is possible to obtain the spectral energy distribution of other weaker sources of radia- tion by indirect methods, such as by spectrophotography or spectrophotometry. The standard sources which are the most easily reproduced are probably well seasoned incandescent lamps 243 244 Bulletin of the Bureau of Standards [Voi. -
!History of Lightingv2.Qxd
CONTENTS Introduction 3 The role of lighting in modern society 3 1. The oldest light sources 4 Before the advent of the lamp 4 The oldest lamps 4 Candles and torches 5 Further development of the oil lamp 6 2. Gaslight 9 Introduction 9 Early history 9 Gas production 10 Gaslight burners 10 The gas mantle 11 3. Electric lighting before the incandescent lamp 14 Introduction 14 Principle of the arc lamp 15 Further development of the arc lamp 16 Applications of the arc lamp 17 4. The incandescent lamp 20 The forerunners 20 The birth of the carbon-filament lamp 22 Further development of the carbon-filament lamp 25 Early metal-filament lamps 27 The Nernst lamp 28 The birth of the tungsten-filament lamp 29 Drawn tungsten filaments 30 Coiled filaments 30 The halogen incandescent lamp 31 5. Discharge lamps 32 Introduction 32 The beginning 32 High-voltage lamps 33 Early low-pressure mercury lamps 34 The fluorescent lamp 35 High-pressure mercury lamps 36 Sodium lamps 37 The xenon lamp 38 6. Electricity production and distribution 39 Introduction 39 Influence machines and batteries 39 Magneto-electric generators 40 Self-exciting generators 41 The oldest public electricity supply systems 41 The battle of systems 42 The advent of modern a.c. networks 43 The History of Light and Lighting While the lighting industry is generally recognized as being born in 1879 with the introduction of Thomas Alva Edison’s incandescent light bulb, the real story of light begins thousands of years earlier. This brochure was developed to provide an extensive look at one of the most important inventions in mankind’s history: artificial lighting. -
Optimization Studies of the CERN-ISOLDE Neutron Converter and Fission Target System
Optimization Studies of the CERN-ISOLDE neutron converter and fission target system Raul Luís1, José G. Marques, Thierry Stora, Pedro Vaz, Luca Zanini 1ITN – Estrada Nacional 10, 2686-953, Sacavém, Portugal 2CERN – CH-1211, Genève 23, Switzerland 3PSI – 5232 Villigen, Switzerland E-mail: [email protected] Abstract. The ISOLDE facility at CERN has been one of the leading isotope separator on-line (ISOL) facilities worldwide since it became operative in 1967. More than 1000 isotopes are available at ISOLDE, produced after the bombardment of various primary targets with a pulsed proton beam of energy 1.4 GeV and an average intensity of 2 μA. A tungsten solid neutron converter has been used for ten years to produce neutron-rich fission fragments in UCx targets. In this work, the Monte Carlo code FLUKA and the cross section codes TALYS and ABRABLA were used to study the current layout of the neutron converter and fission target system of the ISOLDE facility. An optimized target system layout is proposed, which maximizes the production of neutron-rich isotopes and reduces the contamination by undesired proton-rich isobars. The studies here reported can already be applied to ISOLDE and will be of special relevance for the future facilities HIE-ISOLDE and EURISOL. 1. Introduction One of the most efficient ways to study nuclei far from stability is the Isotope Separation On-Line (ISOL) method, in which a beam of high-energy hadrons hits a thick target, producing a great variety of radioactive products through different processes like fission, spallation and fragmentation [1]. The resulting nuclides can be studied after they are extracted from the target, ionized and mass separated. -
Dirac-Exact Relativistic Methods: the Normalized Elimination of the Small Component Method† Dieter Cremer,∗ Wenli Zou and Michael Filatov
Advanced Review Dirac-exact relativistic methods: the normalized elimination of the small component method† Dieter Cremer,∗ Wenli Zou and Michael Filatov Dirac-exact relativistic methods, i.e., 2- or 1-component methods which exactly reproduce the one-electron energies of the original 4-component Dirac method, have established a standard for reliable relativistic quantum chemical calculations targeting medium- and large-sized molecules. Their development was initiated and facilitated in the late 1990s by Dyall’s development of the normalized elimination of the small component (NESC). Dyall’s work has fostered the conversion of NESC and related (later developed) methods into routinely used, multipurpose Dirac- exact methods by which energies, first-order, and second-order properties can be calculated at computational costs, which are only slightly higher than those of nonrelativistic methods. This review summarizes the development of a generally applicable 1-component NESC algorithm leading to the calculation of reliable energies, geometries, electron density distributions, electric moments, electric field gradients, hyperfine structure constants, contact densities and Mossbauer¨ isomer shifts, nuclear quadrupole coupling constants, vibrational frequencies, infrared intensities, and static electric dipole polarizabilities. In addition, the derivation and computational possibilities of 2-component NESC methods are discussed and their use for the calculation of spin-orbit coupling (SOC) effects in connection with spin-orbit splittings and SOC-corrected -
History of Electric Light
SMITHSONIAN MISCELLANEOUS COLLECTIONS VOLUME 76. NUMBER 2 HISTORY OF ELECTRIC LIGHT BY HENRY SGHROEDER Harrison, New Jersey PER\ ^"^^3^ /ORB (Publication 2717) CITY OF WASHINGTON PUBLISHED BY THE SMITHSONIAN INSTITUTION AUGUST 15, 1923 Zrtie Boxb QSaftitnore (prcee BALTIMORE, MD., U. S. A. CONTENTS PAGE List of Illustrations v Foreword ix Chronology of Electric Light xi Early Records of Electricity and Magnetism i Machines Generating Electricity by Friction 2 The Leyden Jar 3 Electricity Generated by Chemical Means 3 Improvement of Volta's Battery 5 Davy's Discoveries 5 Researches of Oersted, Ampere, Schweigger and Sturgeon 6 Ohm's Law 7 Invention of the Dynamo 7 Daniell's Battery 10 Grove's Battery 11 Grove's Demonstration of Incandescent Lighting 12 Grenet Battery 13 De Moleyns' Incandescent Lamp 13 Early Developments of the Arc Lamp 14 Joule's Law 16 Starr's Incandescent Lamp 17 Other Early Incandescent Lamps 19 Further Arc Lamp Developments 20 Development of the Dynamo, 1840-1860 24 The First Commercial Installation of an Electric Light 25 Further Dynamo Developments 27 Russian Incandescent Lamp Inventors 30 The Jablochkofif " Candle " 31 Commercial Introduction of the Differentially Controlled Arc Lamp ^3 Arc Lighting in the United States 3;^ Other American Arc Light Systems 40 " Sub-Dividing the Electric Light " 42 Edison's Invention of a Practical Incandescent Lamp 43 Edison's Three-Wire System 53 Development of the Alternating Current Constant Potential System 54 Incandescent Lamp Developments, 1884-1894 56 The Edison " Municipal -
Concurrent Reduction and Distillation; an Improved Technique for the Recovery and Chemical Refinement of the Isotopes of Cadmium and Zinc*
If I CONCURRENT REDUCTION AND DISTILLATION; AN IMPROVED TECHNIQUE FOR THE RECOVERY AND CHEMICAL REFINEMENT OF THE ISOTOPES OF CADMIUM AND ZINC* H. H. Cardill L. E. McBride LOHF-821046—2 E. W. McDaniel DE83 001931 Operations Division Oak Ridge National Laboratory Oak Ridge, Tennessee 3 7830 .DISCLAIMER • s prepared es an accouni oi WOTk sconsQ'ed by an agency of itie United Slates Cover r "iiit?3 Stilt 65 Gov(?fnft»gn ^ ri(jt ^nv aQcncy Tllf GO* ^or rlny O^ tt^^ir ^rnployut^. TigV MASTER lostifl. ion, apod'aiuj pioiJut;. <y vned nghtv Reference hcein xc any v>t^-'T*t. ^ Dv ^.r^de narno, tf^Oernafk^ mir'ij'iJClureT. or otrierw «d <Jo*^ •nenaalion. or liivONng bv 'Vhe United _^_ . vs and opinions of authors enp'«i«] herein do noi IOM t' irip UnitK* Stales Govefnrneni c a^v agency For presentation at the 11th World Conference of the International Nuclear Target Development Society, October 6-8, 1982, Seattle, Washington. By acceptance of this article, the publisher or recipient acknowledge* the U.S. Govarnment's right to retain a nonaxclusiva, royalty-frtta license in and to any copyright covering tha article. NOTICE P0T09_0£-Jfns,J^SPQRT_JfgE_Il,LESIBLE. I has been reproauce.1 from the best available aopy to pensit the broadest possible avail- ability* *Research sponsored by the Office of Basic Energy Science, U.S. Department of Energy under contract W-7405-eng-26 with the Union Carbide Co rpcration,, DISTRIBUTION OF THIS DOCUMEHT 18 UNLIMITED ' CONCURRENT REDUCTION AND DISTILLATION - AY. IMPROVED TECHNIQUE FOR THE RECOVERY AND CHEMICAL REFINEMENT OF THE ISOTOPES OF CADMIUM AND ZINC H. -
Scientific Literacy Theme : Periodic Classification of Elements Unit 1
SCIENTIFIC LITERACY THEME : PERIODIC CLASSIFICATION OF ELEMENTS UNIT 1 : IUPAC NOMENCLATURE OF ELEMENTS While studying the arrangement of elements Aditya found that there are some elements with atomic number greater than 100 have not named till now as per the periodic table. He tried to find the system to know their names and he found that IUPAC recommended a system of naming new elements till they have given a proper name. the table for naming the elements is given below. With every name a suffix ‘ium’ is added. Digit 0 1 2 3 4 5 6 7 8 9 Root nil un bi tri quad pent hep sept oct Enn abbreviation n u b t q p h s o e Question 1 The IUPAC name for the element with atomic number 120 is (a) Ununquadrdium (b) Unununium (c) Unbinilium (d) unmilennium Question 2 The symbol for IUPAC element unnilquadium is (a) unt (b) unq (c) uno (d) uub Question 3 what is the name and symbol of element with atomic number 118? ------------------------------------------------------------------------------------------------------------------------------- ------------------------------------------------------------------------------------------------------------------------------- Question 4 Write the name and atomic number of element with symbol uuu ------------------------------------------------------------------------------------------------------------------------------- ------------------------------------------------------------------------------------------------------------------------------- UNIT 2 : ELEMENT POSITION IN PERIODIC TABLE Three elements X, -
Periodic Table of the Elements
PERIODIC TABLE OF THE ELEMENTS GROUP 1 18 IA VIIIA 1 1,00794 2 4,002602 Legend Categories Common Constants H He 1 Hydrogen 2,1 Atomic Number 1 1,00794 †Atomic Weight Non Metals Poor Metals Absolute Zero -273.15 °C Fine-structure constant α 0.0072973525 Helium - -27 -11 3 -1 -2 Atomic Mass Unit mu 1.660539x10 kg Gravitation Constant G 6,67408x10 m kg s 23 -1 -1 -1 Symbol Avogadro Constant N 6,022137x10 mol Molar Gas Constant R 8,31451J mol K 2 1s1 2 probable Poor A 13 14 15 16 17 1s H Alkali Metals 3 1,-1 Metals Base of Natural Logarithms e 2.718281828 Molar Volume (Ideal Gas) 0.02241410 m /mol 0 IIA Name Hydrogen 2,2 *Electronegativity Boltzmann constant k 1,380658x10-23 J/K π π 3.14159265358979 IIIA IVA VA VIA VIIA (Pauling) probable Alkali Electron Mass m 9,1093897x10-31 kg Planck Constant h 6,626076x10-34 Js 3 6,941 4 9,012182 e 5 10,811 6 12,011 7 14,00674 8 15,9994 9 18,9984032 10 20,1797 1 Metalloids 2 1s †Electron Configuration Metals 0.510998 MeV/c Proton-Electron Mass Ratio me/mp 1836,15267389 [NOTE] Electron Radius (Classical) r0- 2.8179403x10-15 m Rydberg Constant R 10 973 732 m-1 +1,-1 Possible Oxid. States Alkaline Hearth ∞ Li Be probable Metalloids Electron Volt eV 1.602176x10-19 J Speed of Light in a Vacuum c 299 792 458 m/s B C N O F Ne Metals -19 Lithium 0,98 Beryllium 1,57 Elementry Charge e 1,6021773x10 C Speed of sound in air at STP 343.8 m/s Boron 2,04 Carbon 2,55 Nitrogen 3,04 Oxygen 3,44 Fluorine 3,98 Neon - 2 probable Alkaline Faraday Constant F 9,648531x104 C/mol-1 Standard Pressure 101 325 Pa Phase at STP Halogens -
The Invention of the Electric Light
The Invention of the Electric Light B. J. G. van der Kooij This case study is part of the research work in preparation for a doctorate-dissertation to be obtained from the University of Technology, Delft, The Netherlands (www.tudelft.nl). It is one of a series of case studies about “Innovation” under the title “The Invention Series”. About the text—This is a scholarly case study describing the historic developments that resulted in the steam engine. It is based on a large number of historic and contemporary sources. As we did not conduct any research into primary sources, we made use of the efforts of numerous others by citing them quite extensively to preserve the original character of their contributions. Where possible we identified the individual authors of the citations. As some are not identifiable, we identified the source of the text. Facts that are considered to be of a general character in the public domain are not cited. About the pictures—Many of the pictures used in this case study were found at websites accessed through the Internet. Where possible they were traced to their origins, which, when found, were indicated as the source. As most are out of copyright, we feel that the fair use we make of the pictures to illustrate the scholarly case is not an infringement of copyright. Copyright © 2015 B. J. G. van der Kooij Cover art is a line drawing of Edison’s incandescent lamp (US Patent № 223.898) and Jablochkoff’s arc lamp (US Patent № 190.864) (courtesy USPTO). Version 1.1 (April 2015) All rights reserved.