Monday, March 31, 2014

Flevorium (114)

Flerovium [FLEA-ROH-VEE-UM] is the superheavy artificial chemical element with the symbol Fl and atomic number 114. It is an extremely radioactive element that can only be created in the laboratory and does not occur in nature. The element is named after the Flerov Laboratory of Nuclear Reactions of the Joint Institute for Nuclear Research in Dubna, Russia, where the element was discovered in 1998. The name of the laboratory, in turn, honors the Russian physicist Georgy Flyorov. The name was adopted by IUPAC on May 30, 2012 (Right after my birthday!).
In the periodic table of the elements, it is a transactinide element in the p-block. It is a member of the 7th period and is currently placed as the heaviest known member of the carbon group. Initial chemical studies performed in 2007–2008 indicated that flerovium was unexpectedly volatile for a group 14 element; in preliminary results it even seemed to exhibit properties similar to those of the noble gases.  More recent results show that flerovium's reaction with gold is similar to that of copernicium, showing that it is a very volatile element that may even be gaseous at standard temperature and pressure, and that while it would show metallic properties, consistent with it being the heavier homologue of lead, it would also be the least reactive metal in group 14.
About 80 atoms of flerovium have been observed to date: 50 were synthesized directly, while the rest were made from the radioactive decay of even heavier elements. All of these flerovium atoms have been shown to have mass numbers from 285 to 289. The most stable known flerovium isotope, flerovium-289, has a half-life of around 2.6 seconds, but it is possible that this flerovium isotope may have a nuclear isomer with a longer half-life of 66 seconds; this would be one of the longest half-lives of any isotope of a superheavy element. Flerovium is predicted to be near the center of the theorized island of stability, and it is expected that heavier flerovium isotopes, especially the possibly doubly magic flerovium-298, may have even longer half-lives.

  • Name: Flerovium
  • Symbol: Fl
  • Atomic number: 114
  • Atomic weight: [ 289 ]
  • Standard state: presumably a solid at 298 K
  • CAS Registry ID: 54085-16-4
  • Group in periodic table: 14
  • Period in periodic table: 7
  • Block in periodic table: p-block
  • Color: unknown, but probably metallic and silvery white or grey in appearance
  • Classification: Metallic

Historical information
Only one atom of flerovium (289114Fl)has ever been made (through a nuclear reaction involving fusing a calcium atom with a plutonium atom) isolation of an observable quantity has never been achieved, and may well never be. The discovery was reported informally in January 1999 following experiments towards the end of December 1998 involving scientists at Dubna (Joint Institute for Nuclear Research) in Russia and the Lawrence Livermore National Laboratory, USA.
From the late 1940s to the early 1960s, the early days of the synthesis of heavier and heavier transuranium elements, it was predicted that since such heavy elements did not occur in nature, they would have shorter and shorter half-lives to spontaneous fission, until they stopped being able to exist altogether at around element 108. Initial work in the synthesis of the actinides appeared to confirm this. However, the nuclear shell model was introduced in the late 1960s, which stated that the protons and neutrons formed shells within a nucleus, just like electrons forming electron shells within an atom. The noble gases are unreactive due to their having full electron shells; thus it was theorized that elements with full nuclear shells – having so-called "magic" numbers of protons or neutrons – would be stabilized against radioactive decay. A doubly-magic isotope, having magic numbers of both protons and neutrons, would be especially stabilized, and it was calculated that the next doubly-magic isotope after lead-208 would be flerovium-298 with 114 protons and 184 neutrons, which would form the center of a so-called "island of stability". This island of stability, supposedly centering around elements 112 to element 118, would come just after a long "sea of instability" from elements 101 to 111, and the flerovium isotopes in it were speculated in 1966 to have half-lives in excess of a hundred million years.  It was not until thirty years later, however, that the first isotopes of flerovium would be synthesized. More recent work, however, suspects that the local islands of stability around hassium and flerovium are due to these nuclei being respectively deformed and oblate, which make them resistant towards spontaneous fission, and that the true island of stability for spherical nuclei occurs at around unbibium-306 (with 122 protons and 184 neutrons.
Flerovium was first synthesized in December 1998 by a team of scientists at the Joint Institute for Nuclear Research (JINR) in Dubna, Russia led by Yuri Oganessian, who bombarded a target of plutonium-244 with accelerated nuclei of calcium-48:
A single atom of flerovium, decaying by alpha emission with a half-life of 30 seconds, was detected. This observation was assigned to the isotope flerovium-289 and was subsequently published in January 1999. However, the decay chain observed has not been repeated and the exact identity of this activity is unknown, although it is possible that it is due to a metastable isomer, namely 289mFl.
Glenn T. Seaborg, a scientist at the Lawrence Berkeley National Laboratory who had been involved in work to synthesize such superheavy elements, stated in December 1997 that "one of his longest-lasting and most cherished dreams was to see one of these magic elements." He had, by this time, suffered a massive stroke which affected his memory. He received notice of the synthesis of flerovium from his colleague Albert Ghiorso soon after its publication 1999. Ghiorso later recalled:
“I wanted Glenn to know, so I went to his bedside and told him. I thought I saw a gleam in his eye, but the next day when I went to visit him he didn't remember seeing me. As a scientist, he had died when he had that stroke.”  — Albert Ghiorso

Physical properties
  • Melting point: 340 K; 67 C; 160 F (predicted)
  • Boiling point: 420 K; 147 C; 297 F (predicted)
  • Density of solid: 14 (predicted) g cm-3
  • Heat of vaporization: 38 (predicted) kJ mol-1
Orbital properties
  • Ground state electron configuration:  [Rn].5f14.6d10.7s2.7p2 (a guess based upon that of lead)
  • Shell structure:  2.8.18.32.32.18.4
  • Term symbol:   3P0 (a guess based upon guessed electronic structure)
  • Pauling electronegativity: no data (Pauling units)
  •  First ionization energy: no data kJ mol-1
  •  Second ionization energy: no data kJ mol-1
Isolation
Isolation: as only about three atoms of flerovium has ever been made (through nuclear reaction involving fusing a calcium atom with a plutonium atom) isolation of an observable quantity has never been achieved, and may well never be.
24494Pu + 4820Ca → 288114Fl + 4 1n
24494Pu + 4820Ca → 289114Fl + 3 1n
The element decomposes through the emission of an α-particle to form element 112, copernicium, with a half-life of about 30 seconds for 289114Fl and 2 seconds for 288114Fl.
A different isotope of element 114, 285114Fl, is observed as a decomposition product of the recently observed element 118. Elements 118 and 116 were identified by accelerating a beam of krypton-86 (8636Kr) ions to an energy of 449 million electron volts and directing the beam onto targets of lead-208 (20882Pb). After 11 days work, just three atoms of the new element were identified. The production rates for element 118 are approximately one in every 1012 interactions.
20882Pb + 8636Kr → 293118Uuo + 1n
Element 118 nucleus decays less than a millisecond after its formation by emitting an α-particle. This results in an isotope of flerovium (mass number 289, containing 116 protons and 173 neutrons). This isotope of element 116 is also radioactive and undergoes further α-decay processes to an isotope of flerovium, element 114, and so on down to at least element 106.
293118Uuo → 289116Lv + 42He (0.12 milliseconds)
289116Lv → 285114Fl + 42He (0.60 milliseconds)
285114Fl → 281112Cn + 42He (0.58 milliseconds)
281112Cn → 277110Ds + 42He (0.89 milliseconds)
277110Rg → 273108Hs + 42He (3 milliseconds)
273108Hs → 269106Sg + 42He (1200 milliseconds)

Thursday, March 27, 2014

Nihonium (113) *UPDATED!*

Nihonium: the essentials
Nihonium is the name of a chemical element with the symbol of Nh and was formerly known as Ununtrium, with the temporary symbol Uut and atomic number 113. The element was named for Japan, as it was first discovered at RIKEN in Japan in 2004.
It was known as eka-thallium or simply element 113, is an extremely radioactive synthetic element (an element that can be created in a laboratory but is not found in nature); the most stable known isotope, ununtrium-286, has a half-life of 20 seconds. Ununtrium was first created in 2003 by the Joint Institute for Nuclear Research in Dubna, Russia, with collaboration with scientists at the Lawrence Livermore National Laboratory in Livermore, California.
The claim for discovery has not yet been ratified, but the results are now published in a reputable peer-reviewed journal. Once the discovery is confirmed, then naming will commence.
  • Name: Nihonium
  • Symbol: Nh
  • Atomic number: 113
  • Atomic weight: [ 284 ]
  • Standard state: presumably a solid at 298 K
  • CAS Registry ID: 54084-70-7
  • Group in periodic table: 13 (boron group)
  • Group name: (none)
  • Period in periodic table: 7
  • Block in periodic table: p-block
  • Color: unknown, but probably metallic and silvery white or grey in appearance
  • Classification: Metallic

Historical information
Experimental results reported in 2004 involving the bombardment of americium-243 with calcium-48 ions are consistent with the formation in the laboratory of a few atoms of elements 113 and 115. In experiments conducted at the JINR U400 cyclotron with the Dubna gas-filled separator between July 14 and Aug. 10, 2003, atomic decay patterns were observed said to confirm the existence of element 115 and element 113. In these decay chains, element 113 is produced via the α-decay of element 115.
If you want to read more about the discovery of this element, the results are published in the 1 February 2004 issue of Physical Review C: "Experiments on the synthesis of element 115 in the reaction 243Am(48Ca,xn)21–x115", Yu. Ts. Oganessian, V. K. Utyonkoy, Yu. V. Lobanov, F. Sh. Abdullin, A. N. Polyakov, I. V. Shirokovsky, Yu. S. Tsyganov, G. G. Gulbekian, S. L. Bogomolov, A. N. Mezentsev, S. Iliev, V. G. Subbotin, A. M. Sukhov, A. A. Voinov, G. V. Buklanov, K. Subotic, V. I. Zagrebaev, M. G. Itkis, J. B. Patin, K. J. Moody, J. F. Wild, M. A. Stoyer, N. J. Stoyer, D. A. Shaughnessy, J. M. Kenneally, and R. W. Lougheed, Phys. Rev. C, 2004, 69, 021601(R).
Physical properties
  • Melting point: 700 K, 430 C, 810 F
  • Boiling point: 1430 K, 1130 C, 2070 F
  • Density of solid: 16000 (predicted) kg m-3
  • Heat of Fusion:  7.61kJ mol-1
Orbital properties
  • Ground state electron configuration:  [Rn].5f14.6d10.7s2.7p1
  • Shell structure:  2.8.18.32.32.18.3
  • Term symbol:   2P1/2 (a guess based upon guessed electronic structure)
  • Pauling electronegativity: no data (Pauling units)
  •  First ionization energy: 704.9 kJ mol-1
  •  Second ionization energy: 2240 kJ mol-1
  • Third ionization energy: 3020 kJ mol-1
Isolation
Currently, the identification of element 113 is yet to be confirmed by IUPAC, but the experiments leading to element 113 are now published in a prestigious peer reviewed journal. As only about four atoms of element 113 has ever been made (through decomposition of element 115 nuclei made in nuclear reactions involving fusing calcium nuclei with americium nuclei) isolation of an observable quantity has never been achieved, and may well never be. In the experiments leading to element 115 the following reactions occurred
24395Am + 4820Ca → 287115Uup + 4 1n
24395Am + 4820Ca → 288115Uup + 3 1n
In these first experiments, three nuclei of the 288Nh isotope were made and one of the 287Nh isotope. All the nuclei formed decayed in less than a second by emitting α-particles. These decays resulted in isotopes of ununtrium, element 113, (mass number 283 or 284, containing 113 protons and either 170 or 171 neutrons). These isotopes of element 113 are also radioactive and underwent further α-decay processes to isotopes of element 111 and so on down to at least element 105 (dubnium). One of the nuclei took over a second to decay to element 111.
287115Uup → 283113Uut + 42He (46.6 milliseconds) → 279111Uuu + 42He (147 milliseconds)
288115Uup → 284113Uut + 42He (80.3 milliseconds) → 280111Uuu + 42He (376 milliseconds)
288115Uup → 284113Uut + 42He (18.6 milliseconds) → 279111Uuu + 42He (1196 milliseconds)
288115Uup → 284113Uut + 42He (280 milliseconds) → 279111Uuu + 42He (517 milliseconds)

Wednesday, March 26, 2014

Copernicium (112)

Copernicium (originally called ununbium) is a chemical element with symbol Cn and atomic number 112. It is an extremely radioactive synthetic element that can only be created in a laboratory. The most stable known isotope, copernicium-285, has a half-life of approximately 29 seconds, but it is possible that this copernicium isotope may have a nuclear isomer with a longer half-life, 8.9 min. Copernicium was first created on 9 February, 1996 by the GSI Helmholtz Centre for Heavy Ion Research near Darmstadt, Germany. It is named after the astronomer Nicolaus Copernicus.
In honor of scientist and astronomer Nicolaus Copernicus (1473-1543), the discovering team around Professor Sigurd Hofmann suggested the name copernicium with the element symbol Cn (the original proposal was Cp) for the new element 112, discovered at the GSI Helmholtzzentrum für Schwerionenforschung (Center for Heavy Ion Research) in Darmstadt. It was Copernicus who discovered that the Earth orbits the Sun, thus paving the way for our modern view of the world. Thirteen years ago, element 112 was discovered by an international team of scientists at the GSI accelerator facility. A few weeks ago, the International Union of Pure and Applied Chemistry, IUPAC, officially confirmed their discovery. In around six months, IUPAC will officially endorse the new element's name. This period is set to allow the scientific community to discuss the suggested name copernicium before the IUPAC naming.
  • Name: Copernicium
  • Symbol: Cn
  • Atomic number: 112
  • Atomic weight: [ 285 ]
  • Standard state: presumably a liquid at 298 K
  • CAS Registry ID: 54084-26-3
  • Group in periodic table: 12
  • Group name: (none)
  • Period in periodic table: 7
  • Block in periodic table: d-block
  • Color: unknown, but probably metallic and silvery white or grey in appearance
  • Classification: Metallic

Copernicium: historical information
Copernicium was first created on February 9, 1996, at the Gesellschaft für Schwerionenforschung (GSI) in Darmstadt, Germany, by Sigurd Hofmann, Victor Ninov et al. This element was created by firing accelerated zinc-70 nuclei at a target made of lead-208 nuclei in a heavy ion accelerator. A single atom (the second was subsequently dismissed) of copernicium was produced with a mass number of 277.
In May 2000, the GSI successfully repeated the experiment to synthesize a further atom of copernicium-277. This reaction was repeated at RIKEN using the Search for a Super-Heavy Element Using a Gas-Filled Recoil Separator set-up in 2004 to synthesize two further atoms and confirm the decay data reported by the GSI team.
The IUPAC/IUPAP Joint Working Party (JWP) assessed the claim of discovery by the GSI team in 2001 and 2003. In both cases, they found that there was insufficient evidence to support their claim. This was primarily related to the contradicting decay data for the known nuclide rutherfordium-261. However, between 2001 and 2005, the GSI team studied the reaction 248Cm(26Mg,5n)269Hs, and were able to confirm the decay data for hassium-269 and rutherfordium-261. It was found that the existing data on rutherfordium-261 was for an isomer, now designated rutherfordium-261m.
In May 2009, the JWP reported on the claims of discovery of element 112 again and officially recognized the GSI team as the discoverers of element 112. This decision was based on the confirmation of the decay properties of daughter nuclei as well as the confirmatory experiments at RIKEN.

Copernicium: physical properties
Copernicium: orbital properties
  • Ground state electron configuration:  [Rn].5f14.6d10.7s2 (a guess based upon that of mercury)
  • Shell structure:  2.8.18.32.32.18.2
  • Term symbol:   1S0 (a guess based upon guessed electronic structure)
Isolation
As only a few atoms of element 112 (provisionally named copernicium, Cn) have ever been made (through a nuclear reaction involving fusing a zinc atom with a lead atom) isolation of an observable quantity has never been achieved, and may well never be.
208Pb + 70Zn → 277Cn + 1n
This is because atoms of the element decompose through the emission of α-particles with a half life of only about 240 microseconds.