The Darmstadtium Cornerstone Dieter Ackermann Explains Why Element 110 Occupies a Significant Place in the Superheavy Corner of the Periodic Table

Total Page:16

File Type:pdf, Size:1020Kb

The Darmstadtium Cornerstone Dieter Ackermann Explains Why Element 110 Occupies a Significant Place in the Superheavy Corner of the Periodic Table in your element The darmstadtium cornerstone Dieter Ackermann explains why element 110 occupies a significant place in the superheavy corner of the periodic table. he first isotope of darmstadtium to be region is characterized by enhanced nuclear synthesized was 269Ds, in November stability at atomic number 108 (hassium), 1994, through a cold fusion reaction and at neutron numbers 152 and 162, T 62 208 between Ni and Pb (ref. 1). The concept which are often called deformed sub-shell of cold fusion, where a nucleus is formed closures5. Towards higher atomic numbers in a fusion process at low excitation energy, and higher mass, theory predicts that had already been exploited successfully in nuclear deformation vanishes and the area of the hunt for superheavy nuclei by the team spherical nuclei, which should be stabilized working at the accelerator laboratory GSI in by quantum mechanical effects — referred to Darmstadt, Germany — the city that gave its as the ‘island of stability’ — will be reached6. name to this element. PHOTO PETER SCHICKERT/ALAMY STOCK Its nuclear deformation is also the cause The team at GSI had already successfully of a striking feature of one of its isotopes, synthesized elements 107 (bohrium), The Darmstadtium conference centre in 270Ds, which represents the heaviest case of a 108 (hassium) and 109 (meitnerium) in Darmstadt holds a copy of the publication metastable state — referred to as a K isomer. 1981, 1984 and 1982, respectively. Ten years reporting the discovery of its eponymous element This state resembles a wobble stone with had elapsed, during which the group had in its cornerstone. an axis of total spin, which is inclined with improved the efficiency of their experimental respect to its symmetry axis, and whose set-up to cope with ever-lower probabilities decay is ‘forbidden’ by quantum mechanics. for the synthesis of ever-heavier elements. the fusing system across a complex potential It is more stable than the ground state — an To attempt the synthesis of element 110, it energy landscape. This concept — which had uncommon feature for nuclei. This is possibly was crucial to first measure the ‘excitation also constituted part of a controversial debate a first hint of some interesting physics, yet to function’ — a production probability as a within the GSI group during measurement be discovered, at the onset of the development function of energy — of the hassium isotope of the 266Hs excitation function3 — had failed towards the nuclear sphericity predicted 266Hs (Z = 108). An extrapolation then here, however. to occur in this area. In addition, these allowed the team to successfully predict the Experimental superheavy-element metastable states, depending on deformation, correct energy needed for the synthesis of chemistry is an extremely challenging have the potential to be tracers guiding us darmstadtium. undertaking and other, even heavier elements towards the ‘island of stability’7. The targeted isotope 269Ds was indeed seem to promise more exciting features than These interesting features make 270Ds one produced by fusion between 62Ni and 208Pb, darmstadtium. Therefore, this chemistry has of the cornerstones in the arc leading to the followed by ‘cooling down’ of the fused not been attempted yet and only theoretical superheavy elements. ❐ system through a one-neutron emission. predictions of the chemical properties But there was more: the team had enough of darmstadtium exist. They point to a DIETER ACKERMANN is at the Alternative time to change the projectile to 64Ni and different ground-state configuration than Energies and Atomic Energy Commission, synthesize a second isotope, 271Ds, and to that of its lighter homologues in group 10, at the Large Heavy Ion National Accelerator then go one step further. They exchanged but nevertheless a rather similar chemical Centre (GANIL), CEA-CNRS, Bd. Becquerel, the 208Pb foil that had served as the target behaviour. As for all the superheavy elements, 55027, F-14076 Caen, France. He is at for the previous two reactions to a 209Bi one, relativistic effects are of major importance present also supported by the European featuring one more proton, thus producing here. These effects arise from the acceleration Commission in the framework of the element 111 (roentgenium) in the same of the inner electrons to the highest velocities CEA-EUROTALENT programme. exciting run. in the strong Coulomb field created by the e-mail: [email protected] An earlier attempt to synthesize 271Ds many protons (here 110) in the heavy nucleus4. at higher beam energy had failed in 1985, In contrast to its chemistry, the physical References despite having applied a beam dose that was properties of darmstadtium — or rather of 1. Hofmann, S. et al. Z. Phys. A 350, 277–280 (1995). three times higher2. One of the reasons for its isotopes — have been experimentally 2. Münzenberg, G. et al. in GSI Scientific Report 1985, GSI Report the choice of the higher energy had been a studied, revealing some exciting nuclear 1986-1 (ed. Grundinger, U.) 29 (GSI, 1986). 3. Hofmann, S. On Beyond Uranium: Journey to the End of the concept called ‘extra push’, according to which structure features. The known darmstadtium Periodic Table (Taylor & Francis, 2002). an additional amount of energy may push isotopes sit on the edge of a region of 4. Türler, A. & Pershina, V. Chem. Rev. 113, 1237–1312 (2013). deformed nuclei in the Segrè chart — the 5. Ackermann, D. & Theisen, Ch. Phys. Scr. 92, 083002 (2017). 6. Cwiok, S., Heenen, P.-H. & Nazarewicz, W. Nature representation of nuclides as a function of 433, 705–709 (2005). their proton and neutron numbers. This 7. Ackermann, D. Nucl. Phys. A 944, 376–387 (2015). Bh Hs Mt Ds Rg Cn Nh Fl Mc Lv Ts Og 119 120 121 122 123 124 125 126 127 1034 NATURE CHEMISTRY | VOL 9 | OCTOBER 2017 | www.nature.com/naturechemistry ©2017 Mac millan Publishers Li mited, part of Spri nger Nature. All ri ghts reserved. .
Recommended publications
  • 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.
    [Show full text]
  • 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
    [Show full text]
  • 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
    [Show full text]
  • 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.
    [Show full text]
  • 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 -
    [Show full text]
  • ROENTGENIUM Element Symbol: Rg Atomic Number: 111
    ROENTGENIUM Element Symbol: Rg Atomic Number: 111 An initiative of IYC 2011 brought to you by the RACI PATRICIA ZUBER www.raci.org.au ROENTGENIUM Element symbol: Rg Atomic number: 111 Roentgenium has the symbol Rg and atomic number 111. However, it is not a stable element and can only be produced by cold fusion between other elements (for example by bombarding bismuth with nickel). Once formed, it is a synthetic radioactive element that falls apart in less than 20 sec. Therefore, there is currently no direct use for it. This element was first discovered by the Gesellschaft für Schwerionenforschung (GSI) in Darmstadt, Germany in 1994. GSI also proposed a name for this new element: Roentgenium. They honoured the achievements of Wilhelm Conrad Röntgen, a physicist, who discovered X-rays in 1895 while being professor at the University of Wuerzburg in Germany. Röntgen is considered the father of diagnostic radiology, the medical specialty which uses imaging to diagnose disease. Roentgen never patented anything because he believed that knowledge should be available for everybody. He received the very first Nobel Prize in Physics in 1901. Provided by the element sponsor Martina Stenzel ARTISTS DESCRIPTION Lino cut, silk screen Roentgenium is a synthetic radioactive element produced by cold fusion. It has a half life of 20 seconds and decays by spontaneous fission. Not an easy element to create an image from! I decided to use a diagram of its atomic structure and fission lines as a basis for a relief image. I cut a paper stencil of Rg 111 and silk screened it in silver across the centre of this printed image.
    [Show full text]
  • 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.
    [Show full text]
  • Physics of Superheavy Elements Kouichi Hagino
    Frontiers in Science II 2013.11.6 Physics of superheavy elements Kouichi Hagino Nuclear Theory Group, Department of Physics, Tohoku University What is nuclear physics? What are superheavy elements? How to create superheavy elements? What are chemical properties of superheavy elements? Introduction: atoms and atomic nuclei What would you see if you magnified the dog? ~ 50 cm Introduction: atoms and atomic nuclei cells ~ 50 cm ~ m = 10-6 m Introduction: atoms and atomic nuclei DNA cells -8 ~ 50 cm ~ m = 10-6 m ~ 10 m atom All things are made of atoms. ~ 10-10 m All things are made of atoms. • Thales, Democritus (ancient Greek) • Dalton (chemist, 19th century) • Boltzmann(19th century) • Einstein (1905) ~ 10-10 m STM image (surface physics group, Tohoku university) Introduction: atoms and atomic nuclei DNA cells -8 ~ 50 cm ~ 10 m atom atomic nucleus ~ 10-15 m ~ 10-10 m proton (+e) neutron (no charge) electron cloud (-e) Neutral atoms: # of protons = # of electrons Chemical properties of atoms # of electrons Mp ~ Mn ~ 2000 Me the mass of atom ~ the mass of nucleus Periodic table of chemical elements tabular arrangement of chemical elements based on the atomic numbers (= # of electrons = # of protons) What are we made of ? oxygen 43 kg cerium 40 mg gallium 0.7 mg carbon 16 kg barium 22 mg tellurium 0.7 mg hydrogen 7 kg iodine 20 mg yttrium 0.6 mg nitrogen 1.8 kg tin 20 mg bismuth 0.5 mg calcium 1.0 kg titanium 20 mg thallium 0.5 mg phosphorus 780 g boron 18 mg indium 0.4 mg potassium 140 g nickel 15 mg gold 0.2 mg sulphur 140 g selenium
    [Show full text]
  • Roentgenium Periodic Table of Elements
    Periodic Table of Elements https://periodic-table.pro/Element/Rg/enView online at https://periodic-table.pro Roentgenium Roentgenium is named for Wilhelm Conrad Roentgen, who discovered x-rays. His element is highly radioactive, but disappointingly it does not, despite its name, emit x-rays when it decays. 01. OVERVIEW Symbol Rg Atomic number 111 Atomic weight 272 Density N/A Melting point N/A Boiling point N/A 02. THERMAL PROPERTIES Phase N/A Melting point N/A Boiling point N/A Absolute melting point N/A Absolute boiling point N/A Critical pressure N/A Critical temperature N/A Heat of fusion N/A Heat of vaporization N/A Heat of combustion N/A Specific heat N/A Adiabatic index N/A Neel point N/A Thermal conductivity N/A Thermal expansion N/A 03. PHYSICAL PROPERTIES Density N/A Density (liquid) N/A Molar volume N/A Molar mass 282.169u Brinell hardness N/A Mohs hardness N/A Vickers hardness N/A Bulk modulus N/A Shear modulus N/A Young modulus N/A Poisson ratio N/A Refractive index N/A Speed of sound N/A Thermal conductivity N/A Thermal expansion N/A 04. REACTIVITY Valence N/A Electronegativity N/A Electron affinity N/A Ionization energies N/A 05. SAFETY Autoignition point N/A Flashpoint N/A Heat of combustion N/A 06. CLASSIFICATIONS Alternate names N/A Names of allotropes N/A Block, Group, Period d, 11, 7 Electron configuration [Rn]5f¹⁴6d⁹7s² Color N/A Discovery 1994 in Germany Gas phase N/A 07.
    [Show full text]
  • Periodic Table 1 Periodic Table
    Periodic table 1 Periodic table This article is about the table used in chemistry. For other uses, see Periodic table (disambiguation). The periodic table is a tabular arrangement of the chemical elements, organized on the basis of their atomic numbers (numbers of protons in the nucleus), electron configurations , and recurring chemical properties. Elements are presented in order of increasing atomic number, which is typically listed with the chemical symbol in each box. The standard form of the table consists of a grid of elements laid out in 18 columns and 7 Standard 18-column form of the periodic table. For the color legend, see section Layout, rows, with a double row of elements under the larger table. below that. The table can also be deconstructed into four rectangular blocks: the s-block to the left, the p-block to the right, the d-block in the middle, and the f-block below that. The rows of the table are called periods; the columns are called groups, with some of these having names such as halogens or noble gases. Since, by definition, a periodic table incorporates recurring trends, any such table can be used to derive relationships between the properties of the elements and predict the properties of new, yet to be discovered or synthesized, elements. As a result, a periodic table—whether in the standard form or some other variant—provides a useful framework for analyzing chemical behavior, and such tables are widely used in chemistry and other sciences. Although precursors exist, Dmitri Mendeleev is generally credited with the publication, in 1869, of the first widely recognized periodic table.
    [Show full text]
  • IUPAC/IUPAP Provisional Report)
    Pure Appl. Chem. 2018; 90(11): 1773–1832 Provisional Report Sigurd Hofmanna,*, Sergey N. Dmitrieva, Claes Fahlanderb, Jacklyn M. Gatesb, James B. Robertoa and Hideyuki Sakaib On the discovery of new elements (IUPAC/IUPAP Provisional Report) Provisional Report of the 2017 Joint Working Group of IUPAC and IUPAP https://doi.org/10.1515/pac-2018-0918 Received August 24, 2018; accepted September 24, 2018 Abstract: Almost thirty years ago the criteria that are currently used to verify claims for the discovery of a new element were set down by the comprehensive work of a Transfermium Working Group, TWG, jointly established by IUPAC and IUPAP. The recent completion of the naming of the 118 elements in the first seven periods of the Periodic Table of the Elements was considered as an opportunity for a review of these criteria in the light of the experimental and theoretical advances in the field. In late 2016 the Unions decided to estab- lish a new Joint Working Group, JWG, consisting of six members determined by the Unions. A first meeting of the JWG was in May 2017. One year later this report was finished. In a first part the works and conclusions of the TWG and the Joint Working Parties, JWP, deciding on the discovery of the now named elements are summarized. Possible experimental developments for production and identification of new elements beyond the presently known ones are estimated. Criteria and guidelines for establishing priority of discovery of these potential new elements are presented. Special emphasis is given to a description for the application of the criteria and the limits for their applicability.
    [Show full text]
  • Critical Mineral Resources of the United States— Economic and Environmental Geology and Prospects for Future Supply
    Critical Mineral Resources of the United States— Economic and Environmental Geology and Prospects for Future Supply Professional Paper 1802 U.S. Department of the Interior U.S. Geological Survey Periodic Table of Elements 1A 8A 1 2 hydrogen helium 1.008 2A 3A 4A 5A 6A 7A 4.003 3 4 5 6 7 8 9 10 lithium beryllium boron carbon nitrogen oxygen fluorine neon 6.94 9.012 10.81 12.01 14.01 16.00 19.00 20.18 11 12 13 14 15 16 17 18 sodium magnesium aluminum silicon phosphorus sulfur chlorine argon 22.99 24.31 3B 4B 5B 6B 7B 8B 11B 12B 26.98 28.09 30.97 32.06 35.45 39.95 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 potassium calcium scandium titanium vanadium chromium manganese iron cobalt nickel copper zinc gallium germanium arsenic selenium bromine krypton 39.10 40.08 44.96 47.88 50.94 52.00 54.94 55.85 58.93 58.69 63.55 65.39 69.72 72.64 74.92 78.96 79.90 83.79 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 rubidium strontium yttrium zirconium niobium molybdenum technetium ruthenium rhodium palladium silver cadmium indium tin antimony tellurium iodine xenon 85.47 87.62 88.91 91.22 92.91 95.96 (98) 101.1 102.9 106.4 107.9 112.4 114.8 118.7 121.8 127.6 126.9 131.3 55 56 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 cesium barium hafnium tantalum tungsten rhenium osmium iridium platinum gold mercury thallium lead bismuth polonium astatine radon 132.9 137.3 178.5 180.9 183.9 186.2 190.2 192.2 195.1 197.0 200.5 204.4 207.2 209.0 (209) (210)(222) 87 88 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 francium radium rutherfordium
    [Show full text]