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Ununoctium,  118Uuo
General properties
Name, symbol ununoctium, Uuo
Alternative names element 118, eka-radon
Ununoctium in the periodic table


Atomic number 118
Standard atomic weight [294]
Element category unknown, but probably a noble gas
Group, block group 18, p-block
Period period 7
Electron configuration [Rn] 5f14 6d10 7s2 7p6 (predicted)[1][2]
per shell 2, 8, 18, 32, 32, 18, 8 (predicted)
Physical properties
Phase solid (predicted)[1]
Boiling point 350±30 K ​(80±30 °C, ​170±50 °F) (extrapolated)[1]
Density liquid, at m.p. 4.9–5.1 g·cm−3 (predicted)[3]
Critical point 439 K, 6.8 MPa (extrapolated)[4]
Heat of fusion 23.5 kJ·mol−1 (extrapolated)[4]
Heat of vaporization 19.4 kJ·mol−1 (extrapolated)[4]
Atomic properties
Oxidation states −1,[2] 0, +1,[5] +2,[6] +4,[6] +6[2](predicted)
Ionization energies 1st: 839.4 kJ·mol−1 (predicted)[2]
2nd: 1563.1 kJ·mol−1 (predicted)[7]
Covalent radius 157 pm (predicted)[8]
CAS number 54144-19-3[9]
Naming IUPAC systematic element name
Discovery Joint Institute for Nuclear Research and Lawrence Livermore National Laboratory (2002)
Most stable isotopes
iso NA half-life DM DE (MeV) DP
294Uuo[10] syn ~0.89 ms α 11.65±0.06 290Lv

Ununoctium is the temporary IUPAC name[11] for the transactinide element with the atomic number 118 and temporary element symbol Uuo. It is also known as eka-radon or element 118, and on the periodic table of the elements it is a p-block element and the last one of the 7th period. Ununoctium is currently the only synthetic member of group 18. It has the highest atomic number and highest atomic mass of all the elements discovered so far.

The radioactive ununoctium atom is very unstable, due to its high mass, and since 2005, only three or possibly four atoms of the isotope 294Uuo have been detected.[12] Although this allowed very little experimental characterization of its properties and possible compounds, theoretical calculations have resulted in many predictions, including some unexpected ones. For example, although ununoctium is a member of group 18, it may possibly not be a noble gas, unlike all the other group 18 elements.[1] It was formerly thought to be a gas under normal conditions but is now predicted to be a solid due to relativistic effects.[1]


  • History 1
    • Unsuccessful synthesis attempts 1.1
    • Discovery reports 1.2
  • Naming 2
  • Characteristics 3
    • Nuclear stability and isotopes 3.1
    • Calculated atomic and physical properties 3.2
    • Predicted compounds 3.3
  • See also 4
  • Notes 5
  • References 6
  • Further reading 7
  • External links 8


Unsuccessful synthesis attempts

In late 1998, Polish physicist Robert Smolańczuk published calculations on the fusion of atomic nuclei towards the synthesis of superheavy atoms, including ununoctium.[13] His calculations suggested that it might be possible to make ununoctium by fusing lead with krypton under carefully controlled conditions.[13]

In 1999, researchers at Lawrence Berkeley National Laboratory made use of these predictions and announced the discovery of livermorium and ununoctium, in a paper published in Physical Review Letters,[14] and very soon after the results were reported in Science.[15] The researchers reported to have performed the reaction

+ 208
+ n.

The following year, they published a retraction after researchers at other laboratories were unable to duplicate the results and the Berkeley lab itself was unable to duplicate them as well.[16] In June 2002, the director of the lab announced that the original claim of the discovery of these two elements had been based on data fabricated by principal author Victor Ninov.[17][18]

Discovery reports

The first decay of atoms of ununoctium was observed at the Joint Institute for Nuclear Research (JINR) by Yuri Oganessian and his group in Dubna, Russia, in 2002.[19] On October 9, 2006, researchers from JINR and Lawrence Livermore National Laboratory of California, US, working at the JINR in Dubna, announced[10] that they had indirectly detected a total of three (possibly four) nuclei of ununoctium-294 (one or two in 2002[20] and two more in 2005) produced via collisions of californium-249 atoms and calcium-48 ions.[21][22][23][24][25]

+ 48
+ 3 n.
Schematic diagram of ununoctium-294 alpha decay, with a half-life of 0.89 ms and a decay energy of 11.65 MeV. The resulting livermorium-290 decays by alpha decay, with a half-life of 10.0 ms and a decay energy of 10.80 MeV, to flerovium-286. Flerovium-286 has a half-life of 0.16 s and a decay energy of 10.16 MeV, and undergoes alpha decay to copernicium-282 with a 0.7 rate of spontaneous fission. Copernicium itself has a half-life of only 1.9 ms and has a 1.0 rate of spontaneous fission.
Radioactive decay pathway of the isotope ununoctium-294.[10] The decay energy and average half-life is given for the parent isotope and each daughter isotope. The fraction of atoms undergoing spontaneous fission (SF) is given in green.

In 2011, IUPAC evaluated the 2006 results of the Dubna-Livermore collaboration and concluded: "The three events reported for the Z = 118 isotope have very good internal redundancy but with no anchor to known nuclei do not satisfy the criteria for discovery".[26]

Because of the very small fusion reaction probability (the fusion cross section is ~0.3–0.6 pb or (3–6)×10−41 m2) the experiment took four months and involved a beam dose of 4×1019 calcium ions that had to be shot at the californium target to produce the first recorded event believed to be the synthesis of ununoctium.[9] Nevertheless, researchers are highly confident that the results are not a false positive, since the chance that the detections were random events was estimated to be less than one part in 100000.[27]

In the experiments, the alpha-decay of three atoms of ununoctium was observed. A fourth decay by direct spontaneous fission was also proposed. A half-life of 0.89 ms was calculated: 294
decays into 290
by alpha decay. Since there were only three nuclei, the half-life derived from observed lifetimes has a large uncertainty: 0.89+1.07

+ 4

The identification of the 294
nuclei was verified by separately creating the putative daughter nucleus 290
directly by means of a bombardment of 245
with 48

+ 48
+ 3 n,

and checking that the 290
decay matched the decay chain of the 294
nuclei.[10] The daughter nucleus 290
is very unstable, decaying with a lifetime of 14 milliseconds into 286
, which may experience either spontaneous fission or alpha decay into 282
, which will undergo spontaneous fission.[10]

In a quantum-tunneling model, the alpha decay half-life of 294
was predicted to be 0.66+0.23
[28] with the experimental Q-value published in 2004.[29] Calculation with theoretical Q-values from the macroscopic-microscopic model of Muntian–Hofman–Patyk–Sobiczewski gives somewhat low but comparable results.[30]


Until the 1960s ununoctium was known as eka-emanation (emanation is the old name for radon).[31] In 1979 the IUPAC published recommendations according to which the element was to be called ununoctium,[32] a systematic element name, as a placeholder until the discovery of the element is confirmed and the IUPAC decides on a name.

Before the retraction in 2002, the researchers from Berkeley had intended to name the element ghiorsium (Gh), after Albert Ghiorso (a leading member of the research team).[33]

The Russian discoverers reported their synthesis in 2006. In 2007, the head of the Russian institute stated the team were considering two names for the new element: flyorium, in honor of Moscow Oblast where Dubna is located.[34] He also stated that although the element was discovered as an American collaboration, who provided the californium target, the element should rightly be named in honor of Russia since the Flerov Laboratory of Nuclear Reactions at JINR was the only facility in the world which could achieve this result.[35] These names were later proposed for element 114 (flerovium) and element 116 (moscovium).[36] However, the final name proposed for element 116 was instead livermorium.[37]

No name has yet been officially suggested for the element as no claims for discovery have yet been accepted by the IUPAC. According to current guidelines from IUPAC, the ultimate name for all new elements should end in "-ium", which means the name for ununoctium will almost certainly end in "-ium", not "-on", even if ununoctium turns out to be a noble gas, which traditionally have names ending in "-on" (with the exception of helium, which was not known to be a noble gas when it was discovered).[38]


Nuclear stability and isotopes

Ununoctium (row 118) is slightly above the "island of stability" (white circle) and thus its nuclei are slightly more stable than otherwise predicted.

The stability of nuclei decreases greatly with the increase in atomic number after superheavy elements last longer than predicted.[40] Ununoctium is radioactive and has a half-life that appears to be less than a millisecond. Nonetheless, this is still longer than some predicted values,[28][41] thus giving further support to the idea of this "island of stability".[42]

Calculations using a quantum-tunneling model predict the existence of several neutron-rich isotopes of ununoctium with alpha-decay half-lives close to 1 ms.[43][44]

Theoretical calculations done on the synthetic pathways for, and the half-life of, other isotopes have shown that some could be slightly more stable than the synthesized isotope 294Uuo, most likely 293Uuo, 295Uuo, 296Uuo, 297Uuo, 298Uuo, 300Uuo and 302Uuo.[28][45] Of these, 297Uuo might provide the best chances for obtaining longer-lived nuclei,[28][45] and thus might become the focus of future work with this element. Some isotopes with many more neutrons, such as some located around 313Uuo could also provide longer-lived nuclei.[46]

Calculated atomic and physical properties

Ununoctium is a member of group 18, the zero-valence elements. The members of this group are usually inert to most common chemical reactions (for example, combustion) because the outer valence shell is completely filled with eight electrons. This produces a stable, minimum energy configuration in which the outer electrons are tightly bound.[47] It is thought that similarly, ununoctium has a closed outer valence shell in which its valence electrons are arranged in a 7s27p6 configuration.[1]

Consequently, some expect ununoctium to have similar physical and chemical properties to other members of its group, most closely resembling the noble gas above it in the periodic table, radon.[48] Following the periodic trend, ununoctium would be expected to be slightly more reactive than radon. However, theoretical calculations have shown that it could be quite reactive, so that it probably cannot be considered a noble gas.[6] In addition to being far more reactive than radon, ununoctium may be even more reactive than elements flerovium and copernicium.[1] The reason for the apparent enhancement of the chemical activity of ununoctium relative to radon is an energetic destabilization and a radial expansion of the last occupied 7p-subshell.[1][1] More precisely, considerable spin–orbit interactions between the 7p electrons with the inert 7s2 electrons, effectively lead to a second valence shell closing at flerovium, and a significant decrease in stabilization of the closed shell of element 118.[1] It has also been calculated that ununoctium, unlike other noble gases, binds an electron with release of energy—or in other words, it exhibits positive electron affinity.[49][50][2]

Ununoctium is expected to have by far the broadest [51] or 247 K.[52] Even given the large uncertainties of the calculations, it seems highly unlikely that ununoctium would be a gas under standard conditions,[1][3] and as the liquid range of the other gases is very narrow, between 2 and 9 kelvins, this element should be solid at standard conditions. If ununoctium forms a gas under standard conditions nevertheless, it would be one of the densest gaseous substances at standard conditions (even if it is monatomic like the other noble gases).

Because of its tremendous polarizability, ununoctium is expected to have an anomalously low ionization energy (similar to that of lead which is 70% of that of radon[5] and significantly smaller than that of flerovium[53]) and a standard state condensed phase.[1]

Predicted compounds

Skeletal model of a planar molecule with a central atom symmetrically bonded to four peripheral (fluorine) atoms.
has a square planar configuration.

Skeletal model of a terahedral molecule with a central atom (Uuo) symmetrically bonded to four peripheral (fluorine) atoms.
is predicted to have a tetrahedral configuration.

No compounds of ununoctium have been synthesized yet, but calculations on theoretical compounds have been performed since 1964.[31] It is expected that if the ionization energy of the element is high enough, it will be difficult to oxidize and therefore, the most common oxidation state will be 0 (as for other noble gases);[54] nevertheless, this appears not to be the case.[7]

Calculations on the diatomic molecule Uuo
showed a bonding interaction roughly equivalent to that calculated for Hg
, and a dissociation energy of 6 kJ/mol, roughly 4 times of that of Rn
.[1] But most strikingly, it was calculated to have a bond length shorter than in Rn
by 0.16 Å, which would be indicative of a significant bonding interaction.[1] On the other hand, the compound UuoH+ exhibits a dissociation energy (in other words proton affinity of Uuo) that is smaller than that of RnH+.[1]

The bonding between ununoctium and hydrogen in UuoH is predicted to be very limp and can be regarded as a pure van der Waals interaction rather than a true chemical bond.[5] On the other hand, with highly electronegative elements, ununoctium seems to form more stable compounds than for example copernicium or flerovium.[5] The stable oxidation states +2 and +4 have been predicted to exist in the fluorides UuoF
and UuoF
.[55] The +6 state would be less stable due to the strong binding of the 7p1/2 subshell.[7] This is a result of the same spin-orbit interactions that make ununoctium unusually reactive. For example, it was shown that the reaction of ununoctium with F
to form the compound UuoF
would release an energy of 106 kcal/mol of which about 46 kcal/mol come from these interactions.[5] For comparison, the spin-orbit interaction for the similar molecule RnF
is about 10 kcal/mol out of a formation energy of 49 kcal/mol.[5] The same interaction stabilizes the tetrahedral Td configuration for UuoF
, as distinct from the square planar D4h one of XeF
, which RnF
is also expected to have.[55] The Uuo–F bond will most probably be ionic rather than covalent, rendering the UuoFn compounds non-volatile.[6][56] UuoF2 is predicted to be partially ionic due to ununoctium's high electropositivity.[57] Unlike the other noble gases (except possibly xenon),[58][59] ununoctium was predicted to be sufficiently electropositive[57] to form a Uuo–Cl bond with chlorine.[6]

See also


  1. ^ The actual quote is "The reason for the apparent enhancement of chemical activity of element 118 relative to radon is the energetic destabilization and radial expansion of its occupied 7p3/2 spinor shell."
  2. ^ Nevertheless, quantum electrodynamic corrections have been shown to be quite significant in reducing this affinity by decreasing the binding in the anion Uuo by 9%, thus confirming the importance of these corrections in superheavy elements. See Pyykkö.
  3. ^ It is debatable if the name of the group "noble gases" will be changed if ununoctium is shown to be non-volatile.


  1. ^ a b c d e f g h i j k l m n o p Nash, Clinton S. (2005). "Atomic and Molecular Properties of Elements 112, 114, and 118". Journal of Physical Chemistry A 109 (15): 3493–3500.  
  2. ^ a b c d Haire, Richard G. (2006). "Transactinides and the future elements". In Morss; Edelstein, Norman M.; Fuger, Jean. The Chemistry of the Actinide and Transactinide Elements (3rd ed.). Dordrecht, The Netherlands:  
  3. ^ Bonchev, Danail; Kamenska, Verginia (1981). "Predicting the Properties of the 113–120 Transactinide Elements". J. Phys. Chem. 85: 1177–1186.  
  4. ^ a b c Eichler, R.; Eichler, B., Thermochemical Properties of the Elements Rn, 112, 114, and 118, Paul Scherrer Institut, retrieved 2010-10-23 
  5. ^ a b c d e f Han, Young-Kyu; Bae, Cheolbeom; Son, Sang-Kil; Lee, Yoon Sup (2000). "Spin–orbit effects on the transactinide p-block element monohydrides MH (M=element 113–118)". Journal of Chemical Physics 112 (6): 2684.  
  6. ^ a b c d e Kaldor, Uzi; Wilson, Stephen (2003). Theoretical Chemistry and Physics of Heavy and Superheavy Elements. Springer. p. 105.  
  7. ^ a b c Fricke, Burkhard (1975). "Superheavy elements: a prediction of their chemical and physical properties". Recent Impact of Physics on Inorganic Chemistry 21: 89–144.  
  8. ^ Chemical Data. Ununoctium - Uuo, Royal Chemical Society
  9. ^ a b "Ununoctium". WebElements Periodic Table. Retrieved 2007-12-09. 
  10. ^ a b c d e f Oganessian, Y. T.; Utyonkov, V. K.; Lobanov, Y. V.; Abdullin, F. S.; Polyakov, A. N.; Sagaidak, R. N.; Shirokovsky, I. V.; Tsyganov, Y. S.; Voinov, A. A.; Gulbekian, G. G.; Bogomolov, S. L.; Gikal, B. N.; Mezentsev, A. N.; Iliev, S.; Subbotin, V. G.; Sukhov, A. M.; Subotic, K.; Zagrebaev, V. I.; Vostokin, G. K.; Itkis, M. G.; Moody, K. J.; Patin, J. B.; Shaughnessy, D. A.; Stoyer, M. A.; Stoyer, N. J.; Wilk, P. A.; Kenneally, J. M.; Landrum, J. H.; Wild, J. F.; Lougheed, R. W. (2006-10-09). Ca fusion reactions"48Cm+245Cf and 249"Synthesis of the isotopes of elements 118 and 116 in the .  
  11. ^ Wieser, M.E. (2006). "Atomic weights of the elements 2005 (IUPAC Technical Report)". Pure Appl. Chem. 78 (11): 2051–2066.  
  12. ^ "The Top 6 Physics Stories of 2006". Discover Magazine. 2007-01-07. Retrieved 2008-01-18. 
  13. ^ a b Smolanczuk, R. (1999). "Production mechanism of superheavy nuclei in cold fusion reactions".  
  14. ^ Ninov, Viktor (1999). "Observation of Superheavy Nuclei Produced in the Reaction of  
  15. ^ Service, R. F. (1999). "Berkeley Crew Bags Element 118". Science 284 (5421): 1751.  
  16. ^ Public Affairs Department (2001-07-21). "Results of element 118 experiment retracted". Berkeley Lab. Retrieved 2008-01-18. 
  17. ^ Dalton, R. (2002). "Misconduct: The stars who fell to Earth".  
  18. ^ Element 118 disappears two years after it was discovered. Retrieved on 2012-04-02.
  19. ^ Oganessian, Yu. T. et al. (2002). experiment"48
    "Results from the first . JINR Communication (JINR, Dubna).
  20. ^ Oganessian, Yu. T. et al. (2002). experiment"48Ca + 249Cf"Element 118: results from the first . Communication of the Joint Institute for Nuclear Research. 
  21. ^ "Livermore scientists team with Russia to discover element 118". Livermore press release. 2006-12-03. Retrieved 2008-01-18. 
  22. ^ Oganessian, Yu. T. (2006). "Synthesis and decay properties of superheavy elements". Pure Appl. Chem. 78 (5): 889–904.  
  23. ^ Sanderson, K. (2006). "Heaviest element made – again". Nature News ( 
  24. ^ Schewe, P. and Stein, B. (2006-10-17). "Elements 116 and 118 Are Discovered". Physics News Update.  
  25. ^ Weiss, R. (2006-10-17). "Scientists Announce Creation of Atomic Element, the Heaviest Yet". Washington Post. Retrieved 2008-01-18. 
  26. ^ Barber, Robert C.; Karol, Paul J.; Nakahara, Hiromichi; Vardaci, Emanuele; Vogt, Erich W. (2011). "Discovery of the elements with atomic numbers greater than or equal to 113 (IUPAC Technical Report)". Pure and Applied Chemistry 83 (7): 1.  
  27. ^ "Element 118 Detected, With Confidence". Chemical and Engineering news. 2006-10-17. Retrieved 2008-01-18. I would say we're very confident. 
  28. ^ a b c d Chowdhury, Roy P.; Samanta, C.; Basu, D. N. (2006). "α decay half-lives of new superheavy elements". Phys. Rev. C 73: 014612.  
  29. ^ Oganessian, Yu. Ts.; Utyonkov, V.; Lobanov, Yu.; Abdullin, F.; Polyakov, A.; Shirokovsky, I.; Tsyganov, Yu.; Gulbekian, G.; Bogomolov, S.; Gikal, B. N. et al. (2004). "Measurements of cross sections and decay properties of the isotopes of elements 112, 114, and 116 produced in the fusion reactions 233,238U, 242Pu, and 248Cm+48Ca". Physical Review C 70 (6): 064609.  
  30. ^ Samanta, C.; Chowdhury, R. P.; Basu, D.N. (2007). "Predictions of alpha decay half-lives of heavy and superheavy elements". Nucl. Phys. A 789: 142–154.  
  31. ^ a b Grosse, A. V. (1965). "Some physical and chemical properties of element 118 (Eka-Em) and element 86 (Em)". Journal of Inorganic and Nuclear Chemistry (Elsevier Science Ltd.) 27 (3): 509–19.  
  32. ^ Chatt, J. (1979). "Recommendations for the Naming of Elements of Atomic Numbers Greater than 100". Pure Appl. Chem. 51 (2): 381–384.  
  33. ^ "Discovery of New Elements Makes Front Page News". Berkeley Lab Research Review Summer 1999. 1999. Retrieved 2008-01-18. 
  34. ^ "New chemical elements discovered in Russia`s Science City". 2007-02-12. Retrieved 2008-02-09. 
  35. ^ Yemel'yanova, Asya (2006-12-17). "118-й элемент назовут по-русски (118th element will be named in Russian)" (in Russian). Retrieved 2008-01-18. 
  36. ^ "Российские физики предложат назвать 116 химический элемент московием (Russian Physicians Will Suggest to Name Element 116 Moscovium)" (in Russian). 2011. Retrieved 2011-05-08. 
  37. ^ "News: Start of the Name Approval Process for the Elements of Atomic Number 114 and 116". International Union of Pure and Applied Chemistry. Retrieved 2011-12-02. 
  38. ^ Koppenol, W. H. (2002). "Naming of new elements (IUPAC Recommendations 2002)". Pure and Applied Chemistry 74 (5): 787.  
  39. ^ de Marcillac, Pierre; Coron, Noël; Dambier, Gérard; Leblanc, Jacques; Moalic, Jean-Pierre (April 2003). "Experimental detection of α-particles from the radioactive decay of natural bismuth". Nature 422 (6934): 876–878.  
  40. ^ Considine, Glenn D.; Kulik, Peter H. (2002). Van Nostrand's scientific encyclopedia (9 ed.). Wiley-Interscience.  
  41. ^ Oganessian, Yu. T. (2007). "Heaviest nuclei from 48Ca-induced reactions". Journal of Physics G: Nuclear and Particle Physics 34 (4): R165–R242.  
  42. ^ "New Element Isolated Only Briefly".  
  43. ^ Chowdhury, Roy P.; Samanta, C.; Basu, D. N. (2008). "Search for long lived heaviest nuclei beyond the valley of stability". Physical Reviews C 77 (4): 044603.  
  44. ^ Chowdhury, R. P.; Samanta, C.; Basu, D.N. (2008). "Nuclear half-lives for α -radioactivity of elements with 100 ≤ Z ≤ 130". At. Data & Nucl. Data Tables 94 (6): 781–806.  
  45. ^ a b Royer, G.; Zbiri, K.; Bonilla, C. (2004). "Entrance channels and alpha decay half-lives of the heaviest elements". Nuclear Physics A 730 (3–4): 355–376.  
  46. ^ Duarte, S. B.; Tavares, O. A. P.; Gonçalves, M.; Rodríguez, O.; Guzmán, F.; Barbosa, T. N.; García, F.; Dimarco, A. (2004). "Half-life predictions for decay modes of superheavy nuclei". Journal of Physics G: Nuclear and Particle Physics 30 (10): 1487–1494.  
  47. ^ Bader, Richard F.W. "An Introduction to the Electronic Structure of Atoms and Molecules". McMaster University. Retrieved 2008-01-18. 
  48. ^ "Ununoctium (Uuo) – Chemical properties, Health and Environmental effects". Lenntech. Archived from the original on January 16, 2008. Retrieved 2008-01-18. 
  49. ^ Goidenko, Igor; Labzowsky, Leonti; Eliav, Ephraim; Kaldor, Uzi; Pyykko¨, Pekka (2003). "QED corrections to the binding energy of the eka-radon (Z=118) negative ion". Physical Review A 67 (2): 020102(R).  
  50. ^ Eliav, Ephraim; Kaldor, Uzi; Ishikawa, Y; Pyykkö, P (1996). "Element 118: The First Rare Gas with an Electron Affinity". Physical Review Letters 77 (27): 5350–5352.  
  51. ^  
  52. ^ Takahashi, N. (2002). "Boiling points of the superheavy elements 117 and 118". Journal of Radioanalytical and Nuclear Chemistry 251 (2): 299–301.  
  53. ^ Nash, Clinton S.; Bursten, Bruce E. (1999). "Spin-Orbit Effects, VSEPR Theory, and the Electronic Structures of Heavy and Superheavy Group IVA Hydrides and Group VIIIA Tetrafluorides. A Partial Role Reversal for Elements 114 and 118". Journal of Physical Chemistry A 1999 (3): 402–410.  
  54. ^ "Ununoctium: Binary Compounds". WebElements Periodic Table. Retrieved 2008-01-18. 
  55. ^ a b Han, Young-Kyu; Lee, Yoon Sup (1999). "Structures of RgFn (Rg = Xe, Rn, and Element 118. n = 2, 4.) Calculated by Two-component Spin-Orbit Methods. A Spin-Orbit Induced Isomer of (118)F4". Journal of Physical Chemistry A 103 (8): 1104–1108.  
  56. ^ Pitzer, Kenneth S. (1975). "Fluorides of radon and element 118". Journal of the Chemical Society, ChemicalCommunications (18): 760–761.  
  57. ^ a b Seaborg (c. 2006). "transuranium element (chemical element)". Encyclopædia Britannica. Retrieved 2010-03-16. 
  58. ^ 张青莲 (November 1991). 《无机化学丛书》第一卷:稀有气体、氢、碱金属. Beijing: Science Press. pp. P72.  
  59. ^ Proserpio, Davide M.; Hoffmann, Roald; Janda, Kenneth C. (1991). "The xenon-chlorine conundrum: van der Waals complex or linear molecule?". Journal of the American Chemical Society 113 (19): 7184.  

Further reading

  • Eric Scerri, The Periodic Table, Its Story and Its Significance, Oxford University Press, New York, 2007.

External links

  • Element 118: experiments on discovery, archive of discoverers' official web page
  • Chemistry Blog: Independent analysis of 118 claim
  • It's Elemental: Ununoctium
  • Ununoctium at The Periodic Table of Videos (University of Nottingham)
  • On the Claims for Discovery of Elements 110, 111, 112, 114, 116, and 118 (IUPAC Technical Report)
  • "Element 118, Heaviest Ever, Reported for 1,000th of a Second",
  • WebElements: Ununoctium
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