Almost Forgotten Anniversaries in 2019 Introduction
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Historical Development of the Periodic Classification of the Chemical Elements
THE HISTORICAL DEVELOPMENT OF THE PERIODIC CLASSIFICATION OF THE CHEMICAL ELEMENTS by RONALD LEE FFISTER B. S., Kansas State University, 1962 A MASTER'S REPORT submitted in partial fulfillment of the requirements for the degree FASTER OF SCIENCE Department of Physical Science KANSAS STATE UNIVERSITY Manhattan, Kansas 196A Approved by: Major PrafeLoor ii |c/ TABLE OF CONTENTS t<y THE PROBLEM AND DEFINITION 0? TEH-IS USED 1 The Problem 1 Statement of the Problem 1 Importance of the Study 1 Definition of Terms Used 2 Atomic Number 2 Atomic Weight 2 Element 2 Periodic Classification 2 Periodic Lav • • 3 BRIEF RtiVJiM OF THE LITERATURE 3 Books .3 Other References. .A BACKGROUND HISTORY A Purpose A Early Attempts at Classification A Early "Elements" A Attempts by Aristotle 6 Other Attempts 7 DOBEREBIER'S TRIADS AND SUBSEQUENT INVESTIGATIONS. 8 The Triad Theory of Dobereiner 10 Investigations by Others. ... .10 Dumas 10 Pettehkofer 10 Odling 11 iii TEE TELLURIC EELIX OF DE CHANCOURTOIS H Development of the Telluric Helix 11 Acceptance of the Helix 12 NEWLANDS' LAW OF THE OCTAVES 12 Newlands' Chemical Background 12 The Law of the Octaves. .........' 13 Acceptance and Significance of Newlands' Work 15 THE CONTRIBUTIONS OF LOTHAR MEYER ' 16 Chemical Background of Meyer 16 Lothar Meyer's Arrangement of the Elements. 17 THE WORK OF MENDELEEV AND ITS CONSEQUENCES 19 Mendeleev's Scientific Background .19 Development of the Periodic Law . .19 Significance of Mendeleev's Table 21 Atomic Weight Corrections. 21 Prediction of Hew Elements . .22 Influence -
A Brief History of Nuclear Astrophysics
A BRIEF HISTORY OF NUCLEAR ASTROPHYSICS PART I THE ENERGY OF THE SUN AND STARS Nikos Prantzos Institut d’Astrophysique de Paris Stellar Origin of Energy the Elements Nuclear Astrophysics Astronomy Nuclear Physics Thermodynamics: the energy of the Sun and the age of the Earth 1847 : Robert Julius von Mayer Sun heated by fall of meteors 1854 : Hermann von Helmholtz Gravitational energy of Kant’s contracting protosolar nebula of gas and dust turns into kinetic energy Timescale ~ EGrav/LSun ~ 30 My 1850s : William Thompson (Lord Kelvin) Sun heated at formation from meteorite fall, now « an incadescent liquid mass » cooling Age 10 – 100 My 1859: Charles Darwin Origin of species : Rate of erosion of the Weald valley is 1 inch/century or 22 miles wild (X 1100 feet high) in 300 My Such large Earth ages also required by geologists, like Charles Lyell A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. -
The Rare Earths II
Redis co very of the Elements The Ra re Earth s–The Con fusing Years I A gallery of rare earth scientists and a timeline of their research I I James L. Marshall, Beta Eta 1971 , and Virginia R. Marshall, Beta Eta 2003 , Department of Chemistry, University of North Texas, Denton, TX 76203-5070, [email protected] The rare earths after Mosander. In the pre - vi ou s HEXAGON “Rediscovery” article, 1p we were introduced to the 17 rare earths, found in the f-block and the Group III chemical family of Figure 1. Important scientists dealing with rare earths through the nineteenth century. Johan Gadolin the Periodic Table. Because of a common (1760 –1852) 1g —discovered yttrium (1794). Jöns Jacob Berzelius (1779 –1848) and Martin Heinrich valence electron configuration, the rare earths Klaproth (1743 –1817) 1d —discovered cerium (1803). Carl Gustaf Mosander (1787 –1858) 1p —discovered have similar chemical properties, and their lanthanum (1839), didymium (1840), terbium, and erbium (1843). Jean-Charles deGalissard Marignac chemical separation from one another can be (1817 –1894) 1o —discovered ytterbium (1878) and gadolinium (1880). Per Teodor Cleve (1840 –1905) 1n — difficult. From preparations of the first two rare discovered holmium and thulium (1879). Lars Fredrik Nilson (1840 –1899) 1n —discovered scandium earth element s—yttrium and ceriu m—the (1879). Paul-Émile Lecoq de Boisbaudran (1838 –1912) —discovered samarium (1879) and dysprosium Swedish chemist Carl Gustaf Mosander (Figure (1886). 1b Carl Auer von Welsbach (1858 –1929) 1c —discovered praseodymium and neodymium (1885); 1, 2) was able to separate four additional ele - co-discovered lutetium (1907). -
Project Note Weston Solutions, Inc
PROJECT NOTE WESTON SOLUTIONS, INC. To: Canadian Radium & Uranium Corp. Site File Date: June 5, 2014 W.O. No.: 20405.012.013.2222.00 From: Denise Breen, Weston Solutions, Inc. Subject: Determination of Significant Lead Concentrations in Sediment Samples References 1. New York State Department of Environmental Conservation. Technical Guidance for Screening Contaminated Sediments. March 1998. [45 pages] 2. U.S. Environmental Protection Agency (EPA) Office of Emergency Response. Establishing an Observed Release – Quick Reference Fact Sheet. Federal Register, Volume 55, No. 241. September 1995. [7 pages] 3. International Union of Pure and Applied Chemistry, Inorganic Chemistry Division Commission on Atomic Weights and Isotopic Abundances. Atomic Weights of Elements: Review 2000. 2003. [120 pages] WESTON personnel collected six sediment samples (including one environmental duplicate sample) from five locations along the surface water pathway of the Canadian Radium & Uranium Corp. (CRU) site in May 2014. The sediment samples were analyzed for Target Analyte List (TAL) Metals and Stable Lead Isotopes. 1. TAL Lead Interpretation: In order to quantify the significance for Lead, Thallium and Mercury the following was performed: 1. WESTON personnel tabulated all available TAL Metal data from the May 2014 Sediment Sampling event. 2. For each analyte of concern (Lead, Thallium, and Mercury), the highest background concentration was selected and then multiplied by three. This is the criteria to find the significance of site attributable release as per Hazard Ranking System guidelines. 3. One analytical lead result (2222-SD04) of 520 mg/kg (J) was qualified with an unknown bias. In accordance with US EPA document “Using Data to Document an Observed Release and Observed Contamination”, 2222-SD03 lead concentration was adjusted by dividing by the factor value for lead of 1.44 to equal 361 mg/kg. -
RBRC-32 BNL-6835.4 PARITY ODD BUBBLES in HOT QCD D. KHARZEEV in This ~A~Er We Give a Pedawwicalintroduction~0 Recent Work Of
RBRC-32 BNL-6835.4 PARITY ODD BUBBLES IN HOT QCD D. KHARZEEV RIKEN BNL Research Center, Br$ookhauenNational Laboratory, . Upton, New York 11973-5000, USA R.D. PISARSKI Department of Physics, Brookhaven National Laboratoy, Upton, New York 11973-5000, USA M.H.G. TYTGAT Seruice de Physique Th&orique, (7P 225, Uniuersitc4Libre de Bruzelles, B[ud. du !t%iomphe, 1050 Bruxelles, Belgium We consider the topological susceptibility for an SU(N) gauge theory in the limit of a large number of colors, N + m. At nonzero temperature, the behavior of the topological susceptibility depends upon the order of the reconfining phrrse transition. The meet interesting possibility is if the reconfining transition, at T = Td, is of second order. Then we argue that Witten’s relation implies that the topological suscepti~lfity vanishes in a calculable fdion at Td. Ae noted by Witten, this implies that for sufficiently light quark messes, metaetable etates which act like regions of nonzero O — parity odd bubbles — can arise at temperatures just below Td. Experimentally, parity odd bubbles have dramatic signature% the rI’ meson, and especially the q meson, become light, and are copiously produced. Further, in parity odd bubbles, processes which are normally forbidden, such as q + rr”ro, are allowed. The most direct way to detect parity violation is by measuring a parity odd global seymmetry for charged pions, which we define. 1 Introduction In this .-~a~er we give a Pedawwicalintroduction~0 recent work of ours? We I consider an SU(IV) gau”ge t~e~ry in the limit of a large number of colors, N + co, This is, of course, a familiar limit? We use the large N expansion I to investigate the behavior of the theory at nonzero temperature, especially for the topological susceptibility. -
Scandium Fathi Habashi
Laval University From the SelectedWorks of Fathi Habashi 2008 Scandium Fathi Habashi Available at: https://works.bepress.com/fathi_habashi/743/ Metall-Magazin Scandium Habashi, F. (1) When the Russian chemist Dmitri Ivanovich num. Although scan- that he called thortveitite, contained Mendeleev (1834-1907) proposed the Periodic dium has two elec- 30 to 40% of Sc2O3. This mineral was Table in 1869 he predicted the existence of trons in the outermost also found later, in Madagascar. It has eka-boron, which would have an atomic weight shell and one would the composition (Sc,Y)2Si2O7. between 40 of calcium and 48 of titanium. The expect that it would Bazzite: Be3(Sc,Al)2Si6O18 is another element was discovered by Swedish chemist Lars form divalent com- silicate mineral containing scandium Fredrik Nilson (1840-1899) in 1878 by spec- pounds, yet its most discovered in 1915. troscopic analysis of the minerals euxenite and common valency state Euxenite: (Y,Ca,Ce,U,Th)(Nb,Ta,Ti)2O6 gadolinite, which had not yet been found any- is three resembling occurs in granite pegmatites and detri- where except in Scandinavia. By processing 10 aluminum. tal black sands. It is commonly par- kg of euxenite and other residues of rare-earth Scandium is usually tially amorphous due to radiation associated with the damage.It was first described in 1870 minerals, Nilson was able to prepare about 2 lanthanides and the and named from the Greek word g of the oxide of the new metal in high purity metal has hexago- meaning hospitable or friendly to and called the metal scandium in honour of his nal structure like the strangers, in allusion to the many rare fatherland. -
High Strength Aluminum Alloys with Emphasis on Scandium Addition K
CAFP - 2008 Special Metal Casting and Forming Processes HIGH STRENGTH ALUMINUM ALLOYS WITH EMPHASIS ON SCANDIUM ADDITION K. Venkateswarlu, V. Rajinikanth, Ajoy Kumar Ray National Metallurgical Laboratory, Jamshedpur 831007 e-mail: [email protected] INTRODUCTION Aluminium is perhaps the youngest among the large group of metallic elements. It was first commercially produced in the year 1886 and rose in prominence meteorically to occupy today the second position in the total weight produced, next only to steel. Aluminium is a silvery white ductile metal with a FCC structure. It has excellent electrical and thermal conductivity (next only to copper and silver). It has low density (2.7 g/cc) which gives it a very high specific modulus and strength. Pure aluminium is the soft metal with the modulus value of 70 GPa and the yield strength of about 40 MPa. One of the most important properties of aluminium is to form a thin protective oxide layer on the surface. This layer is tenacious, adherent, deformable and impervious to most corroding elements. Aluminium is the common structural material because of the following properties. Light weight : Aluminium weighs roughly one third of iron and steel, but is one and a half times as heavy as magnesium. It finds application in reducing the weight of the component and structures particularly connected with transport, especially with aerospace application. High strength to weight ratio can be achieved in certain alloys, which show marked response to age hardening. High strength to weight ratio saves a lot commercially when dead weight is decreased and pay load of transport vehicle is increased. -
THE MAJOR RARE-EARTH-ELEMENT DEPOSITS of AUSTRALIA: GEOLOGICAL SETTING, EXPLORATION, and RESOURCES Figure 1.1
CHAPTER ONE WHAT ARE RARE- EARTH ELEMENTS? 1.1. INTRODUCTION latter two elements are classified as REE because of their similar physical and chemical properties to the The rare-earth elements (REE) are a group of seventeen lanthanides, and they are commonly associated with speciality metals that form the largest chemically these elements in many ore deposits. Chemically, coherent group in the Periodic Table of the Elements1 yttrium resembles the lanthanide metals more closely (Haxel et al., 2005). The lanthanide series of inner- than its neighbor in the periodic table, scandium, and transition metals with atomic numbers ranging from if its physical properties were plotted against atomic 57 to 71 is located on the second bottom row of the number then it would have an apparent number periodic table (Fig. 1.1). The lanthanide series of of 64.5 to 67.5, placing it between the lanthanides elements are often displayed in an expanded field at gadolinium and erbium. Some investigators who want the base of the table directly above the actinide series to emphasise the lanthanide connection of the REE of elements. In order of increasing atomic number the group, use the prefix ‘lanthanide’ (e.g., lanthanide REE: REE are: lanthanum (La), cerium (Ce), praseodymium see Chapter 2). In some classifications, the second element of the actinide series, thorium (Th: Mernagh (Pr), neodymium (Nd), promethium (Pm), samarium 1 (Sm), europium (Eu), gadolinium (Gd), terbium (Tb), and Miezitis, 2008), is also included in the REE dysprosium (Dy), holmium (Ho), erbium (Er), thulium group, while promethium (Pm), which is a radioactive (Tm), ytterbium (Yb), and lutetium (Lu). -
The Coordination Chemistry of Solvated Metal Ions in DMPU
The Coordination Chemistry of Solvated Metal Ions in DMPU A Study of a Space-Demanding Solvent Daniel Lundberg Faculty of Natural Resources and Agricultural Sciences Department of Chemistry Uppsala Doctoral thesis Swedish University of Agricultural Sciences Uppsala 2006 Acta Universitatis Agriculturae Sueciae 2006: 23 ISSN 1652-6880 ISBN 91-576-7072-2 © 2006 Daniel Lundberg, Uppsala Tryck: SLU Service/Repro, Uppsala 2006 Abstract Lundberg, D., 2006, The Coordination Chemistry of Solvated Metal Ions in DMPU – A Study of a Space-Demanding Solvent. Doctor’s dissertation. ISSN 1652-6880, ISBN 91-576-7072-2 This thesis summarizes and discusses the results of several individual studies on the solvation of metal ions in the solvent N,N’-dimethylpropyleneurea, DMPU, including the iron(II), iron(III), zinc(II), cadmium(II), and lanthanoid(III) ions. These studies have shown that the solvation process in DMPU is sometimes very different to those in corresponding aqueous systems. This is due to the the space-demanding properties the DMPU molecule has when coordinating to metal ions, with its two methyl groups close to the coordinating oxygen atom. The methyl groups effectively hinder/hamper the metal ion from reaching the coordination numbers present in hydrate and solvate complexes with solvent molecules with much lower spatial demands. The investigations were performed with different X-ray techniques, including extended X-ray absorption fine structure (EXAFS), large angle X-ray scattering (LAXS), and single crystal X-ray diffraction (XRD) and included both studies in solution (EXAFS and LAXS) and solid state (EXAFS and XRD). A coordination number reduction, compared to the corresponding hydrates, was found in all of the studied systems, except cadmium(II). -
24 August 2013 Seminar Held
PROCEEDINGS OF THE NOBEL PRIZE SEMINAR 2012 (NPS 2012) 0 Organized by School of Chemistry Editor: Dr. Nabakrushna Behera Lecturer, School of Chemistry, S.U. (E-mail: [email protected]) 24 August 2013 Seminar Held Sambalpur University Jyoti Vihar-768 019 Odisha Organizing Secretary: Dr. N. K. Behera, School of Chemistry, S.U., Jyoti Vihar, 768 019, Odisha. Dr. S. C. Jamir Governor, Odisha Raj Bhawan Bhubaneswar-751 008 August 13, 2013 EMSSSEM I am glad to know that the School of Chemistry, Sambalpur University, like previous years is organizing a Seminar on "Nobel Prize" on August 24, 2013. The Nobel Prize instituted on the lines of its mentor and founder Alfred Nobel's last will to establish a series of prizes for those who confer the “greatest benefit on mankind’ is widely regarded as the most coveted international award given in recognition to excellent work done in the fields of Physics, Chemistry, Physiology or Medicine, Literature, and Peace. The Prize since its introduction in 1901 has a very impressive list of winners and each of them has their own story of success. It is heartening that a seminar is being organized annually focusing on the Nobel Prize winning work of the Nobel laureates of that particular year. The initiative is indeed laudable as it will help teachers as well as students a lot in knowing more about the works of illustrious recipients and drawing inspiration to excel and work for the betterment of mankind. I am sure the proceeding to be brought out on the occasion will be highly enlightening. -
A Brief History of Nuclear Astrophysics
A BRIEF HISTORY OF NUCLEAR ASTROPHYSICS Stellar Origin of Energy the Elements Nuclear Astrophysics Astrophysics Nuclear Physics A BRIEF HISTORY OF NUCLEAR ASTROPHYSICS PART I THE ENERGY OF STARS Thermodynamics: the age of the Earth and the energy of the Sun 1847 : Robert Julius von Mayer Sun heated by fall of meteors 1854 : Hermann von Helmholtz Gravitational energy of protosolar nebula turns into kinetic energy of meteors Time ~ EGrav/LSun ~ 30 My 1850s : William Thompson (Lord Kelvin) Sun heated at formation from meteorite fall, now « an incadescent liquid mass » cooling age 10 – 100 My 1859: Charles Darwin Origin of species : Rate of erosion of the Weald valley is 1 inch/century or 22 miles wild (X 1100 feet high) in 300 My A gaseous, contracting and heating Sun Mean solar density : ~1.35 g/cc Sun liquid Incompressible 1860s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Lane -Ritter A gaseous, contracting and heating Sun Mean solar density : ~1.35 g/cc Sun liquid Incompressible 1860s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Lane -Ritter A gaseous, contracting and heating Sun Mean solar density : ~1.35 g/cc Sun liquid Incompressible 1860s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Lane -Ritter A gaseous, contracting and heating Sun Mean solar density : ~1.35 g/cc Sun liquid Incompressible 1860s: J. -
Dynamis-7 29.Indd
Making isotopes matter: Francis Aston and the mass-spectrograph Jeff Hughes Centre for the History of Science, Technology and Medicine. University of Manchester. [email protected] Dynamis Fecha de recepción: 22 de febrero de 2008 [0211-9536] 2009; 29: 131-165 Fecha de aceptación: 23 de julio de 2008 SUMMARY: 1.―Introduction. 2.―From bottlewasher to gentleman-researcher: Francis Aston at the Cavendish laboratory. 3.―Negotiating the nuclear atom: Rutherford, Bohr and Soddy. 4.―From positive rays to mass-spectrograph: Aston and the element of surprise. 5.―Ruther- ford, Aston and the constitutive role of the mass-spectrograph. 6.―The Nobel Prizes and the history of isotopes. 7.―Conclusion. ABSTRACT: Francis Aston «discovered» the isotopes of the light elements at the Cavendish Laboratory in 1919 using his newly devised mass-spectrograph. With this device, a modi- fication of the apparatus he had used as J.J. Thomson’s lab assistant before the war, Aston was surprised to find that he could elicit isotopes for many of the elements. This work was contested, but Rutherford, recently appointed to head the Cavendish, was a strong supporter of Aston’s work, not least because it supported his emergent programme of re- search into nuclear structure. This paper will explore Aston’s work in the context of skilled practice at the Cavendish and in the wider disciplinary contexts of physics and chemistry. Arguing that Aston’s work was made significant by Rutherford ―and other constituencies, including chemists and astrophysicists― it will explore the initial construction of isotopes as scientific objects through their embodiment in material practices.