Chemical Properties of Rutherfordium \(Rf\) and Dubnium
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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. -
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. -
Tables of Parameters Tables of Parameters for Extended Hückel Calculations Calculations
TABLES OF PARAMETERS FOR EXTENDED HÜCKEL CALCULATIONS Santiago Alvarez Universitat de Barcelona 1999 - 1 - PART 1. STANDARD Hii's and SLATER EXPONENTS AND COEFFICIENTS. H He Li Be B C N O F Ne Na Mg Al Si P S Cl Ar K Ca Sc Ti V Cr Mn Fe Co Ni Cu Zn Ga Ge As Se Br Kr Rb Sr Y Zr Nb Mo Tc Ru Rh Pd Ag Cd In Sn Sb Te I Xe Cs Ba Hf Ta W Re Os Ir Pt Au Hg Tl Pb Bi Po At Rn Fr Ra Rf Db Sg Bh Hs Mt La Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu Ac Th Pa U Np Pu Am Cm Bk Cf Es Fm Md No Lr Parameters for all elements except the shaded ones are included in these Tables. - 2 - General Observations References are to the original paper which first reported EH calculations with the given Hii for a related set of molecules or solids. For some elements, when no EH calculations have been reported, the experimental ionization potentials are given and the references correspond to those experimental values. Although these tables are intended to be of some use in locating atomic parameters, reference to the original work is encouraged. Ionization potentials ( Hii) a) All energies are in eV. Hii's for most transition metals are charge-iterated for model compounds like metal carbonyls or typical organometallic molecules with Cp, CH3, CO, etc. Exceptions, including bulk metals are conveniently indicated. For cases in which charge-iterated Hii's are not available, the standard sources are the Hinze and Jaffé's tables of ionization potentials.1 b) When alternative sets of Hii's were available for the same element, the one which fits better with the trend along a group or a period of the periodic table has been chosen. -
LN–2 IDLE MIND SOLUTIONS 1. We Recognize That, According To
LN–2 LN–2 IDLE MIND SOLUTIONS 1. We recognize that, according to Pauling’s electronegativity scale, compounds with Δx > 1.7 are strongly ionic and exhibit properties which reflect the electrostatic interactions under conditions of energy minimization: (1) Non–directionality of the electrostatic forces will thus lead to an ordered solid (crystalline). (2) Octet stabilization makes the solid non–conducting (electrical insulator). (3) Stability will also most likely make the material transparent in the visible. (4) The magnitude of the attractive forces may make the solid melt at elevated temperature only. (5) Etc. 2. (a) C2Cl3H in Lewis notation: Cl H C = C Cl Cl Note that the H may be located on any one of the 4 (sp2) hybrid orbitals without changing the properties of the compound. (b) On each carbon there are: three equivalent sp2 bonding orbitals in sp2 a plane and one p orbital normal to the sp2 sp2 plane. sp2 p On each chlorine there is: one singly occupied p orbital. Cl p On the hydrogen we have: one singly occupied 1s orbital. H LN–2 σ 2. (c) 2 sp2–sp2 orbitals → 1σ C–C π 2 p–p orbitals → 1π C–C 6 bonds 3 sp2–p orbitals → 3σ C–Cl 1 sp2–s orbital → 1σ C–H 3. Silicon (Si) is a group 4 element like C (carbon) and wil also exhibit sp3 hybridization: 4 sp3 orbitals at B.A. = 109o. Unlike carbon, silicon cannot form double or triple bonds (by lateral p orbital overlap) because the atom is too large to permit lateral overlap! (a) Si + 2Cl2 → SiCl4 Si is in the center of a tetrahedron with the chlorine atoms as the four corners. -
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. -
Interactive Chemistry Exhibition
United Nations International Year All-Russian United Nations International Year All-Russian Educational, Scientific and of the Periodic Table Science Educational, Scientific and of the Periodic Table Science Cultural Organization of Chemical Elements Festival Cultural Organization of Chemical Elements Festival Science for All: Interactive Chemistry Exhibition The Management Committee of the International Year of the Periodic Table of Chemical Elements (IYPT2019) in partnership with All - Russian Science Festival invites you to visit an Interactive Exhibition on Chemistry at UNESCO Headquarters from 28 to 30 January 2019. Launched as part of the Opening Ceremony of the International Year of the Periodic Table of Chemical Elements (IYPT2019) on January 29th, this exhibition will travel around the world during the year 2019. Science for All: Interactive Chemistry Exhibition - an exciting journey into the world of «living» Chemistry where you will have the opportunity to feel like a real scientist, to carry out a series of chemical experiments, discover the history, immerse yourself into virtual reality and explore outer space. 1. Historical zone. Take a selfie in Mendeleev’s Cabinet This year, it is a century and a half since the creation of the Periodic Table. In 1869 there were no Internet, computers, smartphones and many other modern devices. We reconstructed the study of a chemist who worked in the nineteenth century. In the exhibition, visitors can see the basic scientific tools of that time, look at the first publication of the Table, and even take a selfie with its creator, Dmitrii Ivanovich Mendeleev. 2. Zone of space. Find out where it all came from How did hydrogen appear? And Iron? And what about Gold? Answers to these seemingly simple questions lie in the depths of the Universe. -
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. -
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. -
Product Profiles Chemical Element Index
Product Profiles Chemical Element Index Chemical Element Index – By Name (Alphabetical) Atomic Atomic Atomic Name Symbol Number Name Symbol Number Name Symbol Number Actinium Ac 89 Hassium Hs 108 Promethium Pm 61 Aluminum Al 13 Helium He 2 Protactinium Pa 91 Americium Am 95 Holmium Ho 67 Radium Ra 88 Antimony Sb 51 Hydrogen H 1 Radon Rn 86 Argon Ar 18 Indium In 49 Rhenium Re 75 Arsenic As 33 Iodine I 53 Rhodium Rh 45 Astatine At 85 Iridium Ir 77 Rubidium Rb 37 Barium Ba 56 Iron Fe 26 Ruthenium Ru 44 Berkelium Bk 97 Krypton Kr 36 Rutherfordium Rf 104 Beryllium Be 4 Lanthanum La 57 Samarium Sm 62 Bismuth Bi 83 Lawrencium Lr 103 Scandium Sc 21 Boron B 5 Lead Pb 82 Seaborgium Sg 106 Bromine Br 35 Lithium Li 3 Selenium Se 34 Cadmium Cd 48 Lutetium Lu 71 Silicon Si 14 Calcium Ca 20 Magnesium Mg 12 Silver Ag 47 Californium Cf 98 Manganese Mn 25 Sodium Na 11 Carbon C 6 Meitnerium Mt 109 Strontium Sr 38 Cerium Ce 58 Mendelevium Md 101 Sulfur S 16 Cesium Cs 55 Mercury Hg 80 Tantalum Ta 73 Chlorine Cl 17 Molybdenum Mo 42 Technetium Tc 43 Chromium Cr 24 Neilsborium Ns 107 Tellurium Te 52 Cobalt Co 27 Neodymium Nd 60 Terbium Tb 65 Copper Cu 29 Neon Ne 10 Thallium Tl 81 Curium Cm 96 Neptunium Np 93 Thorium Th 90 Dubnium Db 105 Nickel Ni 28 Thulium Tm 69 Dysprosium Dy 66 Niobium Nb 41 Tin Sn 50 Einsteinium Es 99 Nitrogen N 7 Titanium Ti 22 Erbium Er 68 Nobelium No 102 Tungsten W 74 Europium Eu 63 Osmian Os 76 Uranium U 92 Fermium Fm 100 Oxygen O 8 Vanadium V 23 Fluorine F 9 Palladium Pd 46 Xenon Xi 54 Francium Fr 87 Phosphorus P 15 Ytterbium Yb 70 Gadolinium -
WO 2017/161171 A2 21 September 2017 (21.09.2017) P O P C T
(12) INTERNATIONAL APPLICATION PUBLISHED UNDER THE PATENT COOPERATION TREATY (PCT) (19) World Intellectual Property Organization International Bureau (10) International Publication Number (43) International Publication Date WO 2017/161171 A2 21 September 2017 (21.09.2017) P O P C T (51) International Patent Classification: (81) Designated States (unless otherwise indicated, for every B01J 23/10 (2006.01) B82Y 30/00 (201 1.01) kind of national protection available): AE, AG, AL, AM, B01J 35/02 (2006.01) C07C 2/84 (2006.01) AO, AT, AU, AZ, BA, BB, BG, BH, BN, BR, BW, BY, BZ, CA, CH, CL, CN, CO, CR, CU, CZ, DE, DJ, DK, DM, (21) Number: International Application DO, DZ, EC, EE, EG, ES, FI, GB, GD, GE, GH, GM, GT, PCT/US20 17/022787 HN, HR, HU, ID, IL, IN, IR, IS, JP, KE, KG, KH, KN, (22) International Filing Date: KP, KR, KW, KZ, LA, LC, LK, LR, LS, LU, LY, MA, 16 March 2017 (16.03.2017) MD, ME, MG, MK, MN, MW, MX, MY, MZ, NA, NG, NI, NO, NZ, OM, PA, PE, PG, PH, PL, PT, QA, RO, RS, (25) Filing Language: English RU, RW, SA, SC, SD, SE, SG, SK, SL, SM, ST, SV, SY, (26) Publication Language: English TH, TJ, TM, TN, TR, TT, TZ, UA, UG, US, UZ, VC, VN, ZA, ZM, ZW. (30) Priority Data: 62/309,284 16 March 2016 (16.03.2016) US (84) Designated States (unless otherwise indicated, for every kind of regional protection available): ARIPO (BW, GH, (71) Applicant: SILURIA TECHNOLOGIES, INC. GM, KE, LR, LS, MW, MZ, NA, RW, SD, SL, ST, SZ, [US/US]; 409 Illinois Street, Suite 5032, San Francisco, TZ, UG, ZM, ZW), Eurasian (AM, AZ, BY, KG, KZ, RU, California 94158 (US). -
The Quest to Explore the Heaviest Elements Raises Questions About How Far Researchers Can Extend Mendeleev’S Creation
ON THE EDGE OF THE PERIODIC TABLE The quest to explore the heaviest elements raises questions about how far researchers can extend Mendeleev’s creation. BY PHILIP BALL 552 | NATURE | VOL 565 | 31 JANUARY 2019 ©2019 Spri nger Nature Li mited. All ri ghts reserved. ©2019 Spri nger Nature Li mited. All ri ghts reserved. FEATURE NEWS f you wanted to create the world’s next undiscovered element, num- Berkeley or at the Joint Institute for Nuclear Research (JINR) in Dubna, ber 119 in the periodic table, here’s a possible recipe. Take a few Russia — the group that Oganessian leads — it took place in an atmos- milligrams of berkelium, a rare radioactive metal that can be made phere of cold-war competition. In the 1980s, Germany joined the race; I only in specialized nuclear reactors. Bombard the sample with a beam an institute in Darmstadt now named the Helmholtz Center for Heavy of titanium ions, accelerated to around one-tenth the speed of light. Ion Research (GSI) made all the elements between 107 and 112. Keep this up for about a year, and be patient. Very patient. For every The competitive edge of earlier years has waned, says Christoph 10 quintillion (1018) titanium ions that slam into the berkelium target Düllmann, who heads the GSI’s superheavy-elements department: — roughly a year’s worth of beam time — the experiment will probably now, researchers frequently talk to each other and carry out some produce only one atom of element 119. experiments collaboratively. The credit for creating later elements On that rare occasion, a titanium and a berkelium nucleus will collide up to 118 has gone variously, and sometimes jointly, to teams from and merge, the speed of their impact overcoming their electrical repul- sion to create something never before seen on Earth, maybe even in the Universe. -
Syntheses, Structures, Optical Properties, and Theoretical Calculations of Cs2bi2zns5,Cs2bi2cds5, and Cs2bi2mns5 Fu Qiang Huang, Rebecca C
ARTICLE IN PRESS Journal of Solid State Chemistry 174 (2003) 334–341 Syntheses, structures, optical properties, and theoretical calculations of Cs2Bi2ZnS5,Cs2Bi2CdS5, and Cs2Bi2MnS5 Fu Qiang Huang, Rebecca C. Somers, Adam D. McFarland, Richard P. Van Duyne, and James A Ibersà Department of Chemistry, Northwestern University, 2145 Sheridan Road, Evanston, IL 60208-3113, USA Received 24 December 2002; received in revised form 14 April 2003; accepted 25 April 2003 Abstract Three new compounds, Cs2Bi2ZnS5,Cs2Bi2CdS5, and Cs2Bi2MnS5, have been synthesized from the respective elements and a reactive flux Cs2S3 at 973 K. The compounds are isostructural and crystallize in a new structure type in space group Pnma of the orthorhombic system with four formula units in cells of dimensions at 153 K of a=15.763(3), b=4.0965(9), c=18.197(4) A˚ , ˚ 3 ˚ ˚ 3 V=1175.0(4) A for Cs2Bi2ZnS5; a=15.817(2), b=4.1782(6), c=18.473(3) A, V=1220.8(3) A for Cs2Bi2CdS5; and a=15.830(2), ˚ ˚ 3 2 2À b=4.1515(5), c=18.372(2) A, V=1207.4(2) A for Cs2Bi2MnS5. The structure is composed of two-dimensional N[Bi2MS5 ] (M=Zn, Cd, Mn) layers that stack perpendicular to the [100] axis and are separated by Cs+ cations. The layers consist of edge- 1 6À 1 4À sharing N[Bi2S6 ] and N[MS3 ] chains built from BiS6 octahedral and MS4 tetrahedral units. Two crystallographically unique Cs atoms are coordinated to S atoms in octahedral and monocapped trigonal prismatic environments. The structure of Cs2Bi2MS5,is 0 0 related to that of Na2ZrCu2S4 and those of the AMM Q3 materials (A=alkali metal, M=rare-earth or Group 4 element, M = Group 11 or 12 element, Q=chalcogen).