IUPAC Periodic Table of the Isotopes
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Evolution and Understanding of the D-Block Elements in the Periodic Table Cite This: Dalton Trans., 2019, 48, 9408 Edwin C
Dalton Transactions View Article Online PERSPECTIVE View Journal | View Issue Evolution and understanding of the d-block elements in the periodic table Cite this: Dalton Trans., 2019, 48, 9408 Edwin C. Constable Received 20th February 2019, The d-block elements have played an essential role in the development of our present understanding of Accepted 6th March 2019 chemistry and in the evolution of the periodic table. On the occasion of the sesquicentenniel of the dis- DOI: 10.1039/c9dt00765b covery of the periodic table by Mendeleev, it is appropriate to look at how these metals have influenced rsc.li/dalton our understanding of periodicity and the relationships between elements. Introduction and periodic tables concerning objects as diverse as fruit, veg- etables, beer, cartoon characters, and superheroes abound in In the year 2019 we celebrate the sesquicentennial of the publi- our connected world.7 Creative Commons Attribution-NonCommercial 3.0 Unported Licence. cation of the first modern form of the periodic table by In the commonly encountered medium or long forms of Mendeleev (alternatively transliterated as Mendelejew, the periodic table, the central portion is occupied by the Mendelejeff, Mendeléeff, and Mendeléyev from the Cyrillic d-block elements, commonly known as the transition elements ).1 The periodic table lies at the core of our under- or transition metals. These elements have played a critical rôle standing of the properties of, and the relationships between, in our understanding of modern chemistry and have proved to the 118 elements currently known (Fig. 1).2 A chemist can look be the touchstones for many theories of valence and bonding. -
NOBELIUM Element Symbol: No Atomic Number: 102
NOBELIUM Element Symbol: No Atomic Number: 102 An initiative of IYC 2011 brought to you by the RACI KERRY LAMB www.raci.org.au NOBELIUM Element symbol: No Atomic number: 102 The credit for discovering Nobelium was disputed with 3 different research teams claiming the discovery. While the first claim dates back to 1957, it was not until 1992 that the International Union of Pure and Applied Chemistry credited the discovery to a research team from Dubna in Russia for work they did in 1966. The element was named Nobelium in 1957 by the first of its claimed discoverers (the Nobel Institute in Sweden). It was named after Alfred Nobel, a Swedish chemist who invented dynamite, held more than 350 patents and bequeathed his fortune to the establishment of the Nobel Prizes. Nobelium is a synthetic element and does not occur in nature and has no known uses other than in scientific research as only tiny amounts of the element have ever been produced. Nobelium is radioactive and most likely metallic. The appearance and properties of Nobelium are unknown as insufficient amounts of the element have been produced. Nobelium is made by the bombardment of curium (Cm) with carbon nuclei. Its most stable isotope, 259No, has a half-life of 58 minutes and decays to Fermium (255Fm) through alpha decay or to Mendelevium (259Md) through electron capture. Provided by the element sponsor Freehills Patent and Trade Mark Attorneys ARTISTS DESCRIPTION I wanted to depict Alfred Nobel, the namesake of Nobelium, as a resolute young man, wearing the Laurel wreath which is the symbol of victory. -
The Periodic Table of Elements
The Periodic Table of Elements 1 2 Atomic Number = Number of Protons = Number of Electrons H 6 He HYDROGEN HELIUM 1 Chemical Symbol NON-METALS 4 3 4 C 5 6 7 8 9 10 Li Be CARBON Chemical Name B C N O F Ne LITHIUM BERYLLIUM Atomic Weight = Number of Protons + Number of Neutrons* BORON CARBON NITROGEN OXYGEN FLUORINE NEON 7 9 12 11 12 14 16 19 20 11 12 13 14 15 16 17 18 Na Mg Al Si P S Cl Ar SODIUM MAGNESIUM ALUMINUM SILICON PHOSPHORUS SULFUR CHLORINE ARGON 23 24 METALS 27 28 31 32 35 40 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 K Ca Sc Ti V Cr Mn Fe Co Ni Cu Zn Ga Ge As Se Br Kr POTASSIUM CALCIUM SCANDIUM TITANIUM VANADIUM CHROMIUM MANGANESE IRON COBALT NICKEL COPPER ZINC GALLIUM GERMANIUM ARSENIC SELENIUM BROMINE KRYPTON 39 40 45 48 51 52 55 56 59 59 64 65 70 73 75 79 80 84 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 Rb Sr Y Zr Nb Mo Tc Ru Rh Pd Ag Cd In Sn Sb Te I Xe RUBIDIUM STRONTIUM YTTRIUM ZIRCONIUM NIOBIUM MOLYBDENUM TECHNETIUM RUTHENIUM RHODIUM PALLADIUM SILVER CADMIUM INDIUM TIN ANTIMONY TELLURIUM IODINE XENON 85 88 89 91 93 96 98 101 103 106 108 112 115 119 122 128 127 131 55 56 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 Cs Ba Hf Ta W Re Os Ir Pt Au Hg Tl Pb Bi Po At Rn CESIUM BARIUM HAFNIUM TANTALUM TUNGSTEN RHENIUM OSMIUM IRIDIUM PLATINUM GOLD MERCURY THALLIUM LEAD BISMUTH POLONIUM ASTATINE RADON 133 137 178 181 184 186 190 192 195 197 201 204 207 209 209 210 222 87 88 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 Fr Ra Rf Db Sg Bh Hs Mt Ds Rg Uub Uut Uuq Uup Uuh Uus Uuo FRANCIUM RADIUM -
The Development of the Periodic Table and Its Consequences Citation: J
Firenze University Press www.fupress.com/substantia The Development of the Periodic Table and its Consequences Citation: J. Emsley (2019) The Devel- opment of the Periodic Table and its Consequences. Substantia 3(2) Suppl. 5: 15-27. doi: 10.13128/Substantia-297 John Emsley Copyright: © 2019 J. Emsley. This is Alameda Lodge, 23a Alameda Road, Ampthill, MK45 2LA, UK an open access, peer-reviewed article E-mail: [email protected] published by Firenze University Press (http://www.fupress.com/substantia) and distributed under the terms of the Abstract. Chemistry is fortunate among the sciences in having an icon that is instant- Creative Commons Attribution License, ly recognisable around the world: the periodic table. The United Nations has deemed which permits unrestricted use, distri- 2019 to be the International Year of the Periodic Table, in commemoration of the 150th bution, and reproduction in any medi- anniversary of the first paper in which it appeared. That had been written by a Russian um, provided the original author and chemist, Dmitri Mendeleev, and was published in May 1869. Since then, there have source are credited. been many versions of the table, but one format has come to be the most widely used Data Availability Statement: All rel- and is to be seen everywhere. The route to this preferred form of the table makes an evant data are within the paper and its interesting story. Supporting Information files. Keywords. Periodic table, Mendeleev, Newlands, Deming, Seaborg. Competing Interests: The Author(s) declare(s) no conflict of interest. INTRODUCTION There are hundreds of periodic tables but the one that is widely repro- duced has the approval of the International Union of Pure and Applied Chemistry (IUPAC) and is shown in Fig.1. -
The Periodic Table of Elements
The Periodic Table of Elements 1 2 6 Atomic Number = Number of Protons = Number of Electrons HYDROGENH HELIUMHe 1 Chemical Symbol NON-METALS 4 3 4 C 5 6 7 8 9 10 Li Be CARBON Chemical Name B C N O F Ne LITHIUM BERYLLIUM = Number of Protons + Number of Neutrons* BORON CARBON NITROGEN OXYGEN FLUORINE NEON 7 9 12 Atomic Weight 11 12 14 16 19 20 11 12 13 14 15 16 17 18 SODIUMNa MAGNESIUMMg ALUMINUMAl SILICONSi PHOSPHORUSP SULFURS CHLORINECl ARGONAr 23 24 METALS 27 28 31 32 35 40 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 POTASSIUMK CALCIUMCa SCANDIUMSc TITANIUMTi VANADIUMV CHROMIUMCr MANGANESEMn FeIRON COBALTCo NICKELNi CuCOPPER ZnZINC GALLIUMGa GERMANIUMGe ARSENICAs SELENIUMSe BROMINEBr KRYPTONKr 39 40 45 48 51 52 55 56 59 59 64 65 70 73 75 79 80 84 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 RUBIDIUMRb STRONTIUMSr YTTRIUMY ZIRCONIUMZr NIOBIUMNb MOLYBDENUMMo TECHNETIUMTc RUTHENIUMRu RHODIUMRh PALLADIUMPd AgSILVER CADMIUMCd INDIUMIn SnTIN ANTIMONYSb TELLURIUMTe IODINEI XeXENON 85 88 89 91 93 96 98 101 103 106 108 112 115 119 122 128 127 131 55 56 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 CESIUMCs BARIUMBa HAFNIUMHf TANTALUMTa TUNGSTENW RHENIUMRe OSMIUMOs IRIDIUMIr PLATINUMPt AuGOLD MERCURYHg THALLIUMTl PbLEAD BISMUTHBi POLONIUMPo ASTATINEAt RnRADON 133 137 178 181 184 186 190 192 195 197 201 204 207 209 209 210 222 87 88 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 FRANCIUMFr RADIUMRa RUTHERFORDIUMRf DUBNIUMDb SEABORGIUMSg BOHRIUMBh HASSIUMHs MEITNERIUMMt DARMSTADTIUMDs ROENTGENIUMRg COPERNICIUMCn NIHONIUMNh -
An Octad for Darmstadtium and Excitement for Copernicium
SYNOPSIS An Octad for Darmstadtium and Excitement for Copernicium The discovery that copernicium can decay into a new isotope of darmstadtium and the observation of a previously unseen excited state of copernicium provide clues to the location of the “island of stability.” By Katherine Wright holy grail of nuclear physics is to understand the stability uncover its position. of the periodic table’s heaviest elements. The problem Ais, these elements only exist in the lab and are hard to The team made their discoveries while studying the decay of make. In an experiment at the GSI Helmholtz Center for Heavy isotopes of flerovium, which they created by hitting a plutonium Ion Research in Germany, researchers have now observed a target with calcium ions. In their experiments, flerovium-288 previously unseen isotope of the heavy element darmstadtium (Z = 114, N = 174) decayed first into copernicium-284 and measured the decay of an excited state of an isotope of (Z = 112, N = 172) and then into darmstadtium-280 (Z = 110, another heavy element, copernicium [1]. The results could N = 170), a previously unseen isotope. They also measured an provide “anchor points” for theories that predict the stability of excited state of copernicium-282, another isotope of these heavy elements, says Anton Såmark-Roth, of Lund copernicium. Copernicium-282 is interesting because it University in Sweden, who helped conduct the experiments. contains an even number of protons and neutrons, and researchers had not previously measured an excited state of a A nuclide’s stability depends on how many protons (Z) and superheavy even-even nucleus, Såmark-Roth says. -
The Oganesson Odyssey Kit Chapman Explores the Voyage to the Discovery of Element 118, the Pioneer Chemist It Is Named After, and False Claims Made Along the Way
in your element The oganesson odyssey Kit Chapman explores the voyage to the discovery of element 118, the pioneer chemist it is named after, and false claims made along the way. aving an element named after you Ninov had been dismissed from Berkeley for is incredibly rare. In fact, to be scientific misconduct in May5, and had filed Hhonoured in this manner during a grievance procedure6. your lifetime has only happened to Today, the discovery of the last element two scientists — Glenn Seaborg and of the periodic table as we know it is Yuri Oganessian. Yet, on meeting Oganessian undisputed, but its structure and properties it seems fitting. A colleague of his once remain a mystery. No chemistry has been told me that when he first arrived in the performed on this radioactive giant: 294Og halls of Oganessian’s programme at the has a half-life of less than a millisecond Joint Institute for Nuclear Research (JINR) before it succumbs to α -decay. in Dubna, Russia, it was unlike anything Theoretical models however suggest it he’d ever experienced. Forget the 2,000 ton may not conform to the periodic trends. As magnets, the beam lines and the brand new a noble gas, you would expect oganesson cyclotron being installed designed to hunt to have closed valence shells, ending with for elements 119 and 120, the difference a filled 7s27p6 configuration. But in 2017, a was Oganessian: “When you come to work US–New Zealand collaboration predicted for Yuri, it’s not like a lab,” he explained. that isn’t the case7. -
IUPAC Wire See Also
News and information on IUPAC, its fellows, and member organizations. IUPAC Wire See also www.iupac.org Flerovium and Livermorium Join the Future Earth: Research for Global Periodic Table Sustainability n 30 May 2012, IUPAC officially approved he International Council for Science (ICSU), of the name flerovium, with symbol Fl, for the which IUPAC is a member, announced a new Oelement of atomic number 114 and the name T10-year initiative named Future Earth to unify livermorium, with symbol Lv, for the element of atomic and scale up ICSU-sponsored global environmental- number 116. The names and symbols were proposed change research. by the collaborating team of the Joint Institute for Nuclear Research (Dubna, Russia) and the Lawrence Operational in 2013, this new ICSU initiative will Livermore National Laboratory (Livermore, California, provide a cutting-edge platform to coordinate scien- USA) to whom the priority for the discovery of these tific research to respond to the most critical social and elements was assigned last year. The IUPAC recom- environmental challenges of the 21st century at global mendations presenting these names is to appear in and regional levels. “This initiative will link global envi- the July 2012 issue of Pure and Applied Chemistry. ronmental change and fundamental human develop- ment questions,” said Diana Liverman, co-director of The name flerovium, with symbol Fl, lies within the Institute of the Environment at the University of tradition and honors the Flerov Laboratory of Nuclear Arizona and co-chair of the team Reactions in Dubna, Russia, where the element of that is designing Future Earth. -
Darmstadtium, Roentgenium and Copernicium Form Strong Bonds with Cyanide
Darmstadtium, Roentgenium and Copernicium Form Strong Bonds With Cyanide Taye B. Demissie∗and Kenneth Ruudy March 23, 2017 Abstract We report the structures and properties of the cyanide complexes of three super- heavy elements (darmstadtium, roentgenium and copernicium) studied using two- and four-component relativistic methodologies. The electronic and structural properties of these complexes are compared to the corresponding complexes of platinum, gold and mercury. The results indicate that these superheavy elements form strong bonds with cyanide. Moreover, the calculated absorption spectra of these superheavy-element cyanides show similar trends to those of the corresponding heavy-atom cyanides. The calculated vibrational frequencies of the heavy-metal cyanides are in good agreement with available experimental results lending support to the quality of our calculated vibrational frequencies for the superheavy-atom cyanides. ∗Centre for Theoretical and Computational Chemistry, Department of Chemistry, UiT The Arctic Uni- versity of Norway, N-9037 Tromsø, Norway yCentre for Theoretical and Computational Chemistry, Department of Chemistry, UiT The Arctic Uni- versity of Norway, N-9037 Tromsø, Norway 1 Relativistic two- and four-component density-functional theory is used to demonstrate that the superheavy elements darmstadtium, roentgenium and copernicium form stable complexes with cyanide, providing new insight into the chemistry of these superheavy elements. 2 INTRODUCTION The term heavy atom refers roughly to elements in the 4th - -
Gas-Phase Chemistry of Element 114, Flerovium
EPJ Web of Conferences 131, 07003 (2016) DOI: 10.1051/epjconf/201613107003 Nobel Symposium NS160 – Chemistry and Physics of Heavy and Superheavy Elements Gas-phase chemistry of element 114, flerovium Alexander Yakushev1,2,a and Robert Eichler3,4 1 GSI Helmholtzzentrum für Schwerionenforschung GmbH, 64291 Darmstadt, Germany 2 Helmholtz-Institut Mainz, 55099 Mainz, Germany 3 Paul Scherrer Institut, 5232 Villigen PSI, Switzerland 4 University of Bern, Department of Chemistry and Biochemistry, 3012 Bern, Switzerland Abstract. Element 114 was discovered in 2000 by the Dubna-Livermore collaboration, and in 2012 it was named flerovium. It belongs to the group 14 of the periodic table of elements. A strong relativistic stabilisation of 2 2 the valence shell 7s 7p1/2 is expected due to the orbital splitting and the 2 2 contraction not only of the 7s but also of the spherical 7p1/2 closed subshell, resulting in the enhanced volatility and inertness. Flerovium was studied chemically by gas-solid chromatography upon its adsorption on a gold surface. Two experimental results on Fl chemistry have been published so far. Based on observation of three atoms, a weak interaction of flerovium with gold was suggested in the first study. Authors of the second study concluded on the metallic character after the observation of two Fl atoms deposited on gold at room temperature. 1. Introduction Man-made superheavy elements (SHE, atomic number Z ≥ 104) are unique in two aspects. Their nuclei exist only due to nuclear shell effects, and their electron structure is influenced by increasingly important relativistic effects [1–3]. Recently the synthesis of elements 113, 115, 117 and 118 has been approved, thus, the discovery of all elements of the 7th row in the periodic table of elements with proton number Z up to 118 has been acknowledged [4]. -
Atomic Properties of the Elements
P E R I O D I C T A B L E Group 1 18 IA Atomic Properties of the Elements VIIIA 2 1 S FREQUENTLY USED FUNDAMENTAL PHYSICAL CONSTANTS§ S 1 1/2 Physical Measurement Laboratory www.nist.gov/pml 2 0 1 second = 9 192 631 770 periods of radiation corresponding to the H transition between the two hyperfine levels of the ground state of 133Cs Standard Reference Data www.nist.gov/srd He 1 Hydrogen −1 § For the most accurate Helium speed of light in vacuum c 299 792 458 m s (exact) values of these and 1.008* −34 4.002602 2 1s 2 Planck constant h 6.626 070 x 10 J s ( ħ /2 ) other constants, visit 13 14 15 16 17 1s −19 13.5984 IIA elementary charge e 1.602 177 x 10 C physics.nist.gov/constants IIIA IVA VA VIA VIIA 24.5874 −31 2 1 electron mass me 9.109 384 x 10 kg 2 3 4 3 2 1 3 S1/2 4 S0 2 5 P°1/2 6 P0 7 S3/2° 8 P2 9 P3/2° 10 S0 mec 0.510 999 MeV −27 Solids Li Be proton mass mp 1.672 622 x 10 kg B C N O F Ne 2 Lithium Beryllium fine-structure constant 1/137.035 999 Liquids Boron Carbon Nitrogen Oxygen Fluorine Neon 6.94* 9.0121831 −1 10.81* 12.011* 14.007* 15.999* 18.99840316* 20.1797 Rydberg constant R 10 973 731.569 m 2 2 2 Gases 2 2 2 2 2 2 2 3 2 2 4 2 2 5 2 2 6 15 1s 2s 2p 1s 2s 1s 2s 1s 2s 1s 2s 1s 2s 1s 2s R c 3.289 841 960 x 10 Hz 2p 2p 1s 2s 2p 2p 2p 5.3917 9.3227 Artificially 8.2980 11.2603 14.5341 13.6181 17.4228 21.5645 R hc 13.605 693 eV 2 1 -19 Prepared 2 3 4 3 2 1 11 S1/2 12 S0 electron volt eV 1.602 176 6 x 10 J 13 P1/2° 14 P0 15 S3/2° 16 P2 17 P3/2° 18 S0 −23 −1 Boltzmann constant k 1.380 65 x 10 J K −1 −1 Na Mg molar gas constant -
Quest for Superheavy Nuclei Began in the 1940S with the Syn Time It Takes for Half of the Sample to Decay
FEATURES Quest for superheavy nuclei 2 P.H. Heenen l and W Nazarewicz -4 IService de Physique Nucleaire Theorique, U.L.B.-C.P.229, B-1050 Brussels, Belgium 2Department ofPhysics, University ofTennessee, Knoxville, Tennessee 37996 3Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831 4Institute ofTheoretical Physics, University ofWarsaw, ul. Ho\.za 69, PL-OO-681 Warsaw, Poland he discovery of new superheavy nuclei has brought much The superheavy elements mark the limit of nuclear mass and T excitement to the atomic and nuclear physics communities. charge; they inhabit the upper right corner of the nuclear land Hopes of finding regions of long-lived superheavy nuclei, pre scape, but the borderlines of their territory are unknown. The dicted in the early 1960s, have reemerged. Why is this search so stability ofthe superheavy elements has been a longstanding fun important and what newknowledge can it bring? damental question in nuclear science. How can they survive the Not every combination ofneutrons and protons makes a sta huge electrostatic repulsion? What are their properties? How ble nucleus. Our Earth is home to 81 stable elements, including large is the region of superheavy elements? We do not know yet slightly fewer than 300 stable nuclei. Other nuclei found in all the answers to these questions. This short article presents the nature, although bound to the emission ofprotons and neutrons, current status ofresearch in this field. are radioactive. That is, they eventually capture or emit electrons and positrons, alpha particles, or undergo spontaneous fission. Historical Background Each unstable isotope is characterized by its half-life (T1/2) - the The quest for superheavy nuclei began in the 1940s with the syn time it takes for half of the sample to decay.