Ununennium
properties | |
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Properties (if known) | |
Name , symbol , atomic number | Ununennium, Uue, 119 |
Element category | Unknown |
Group , period , block | 1 , 8 , p |
CAS number | 54143-88-3 |
Atomic | |
Atomic mass | estimated 295 u |
Electron configuration | [ Og ] 8 s 1 (?) |
Electrons per energy level | 2, 8, 18, 32, 32, 18, 8, 1 |
As far as possible and customary, SI units are used. Unless otherwise noted, the data given apply to standard conditions . Values that are particularly questionable are marked with (?) |
Ununennium is a currently hypothetical chemical element with atomic number 119, it is also known as Eka - Francium .
In the periodic table, it is between 118 Oganesson (first synthesized in 2006) and 120 Unbinilium . The element does not occur in nature, it could only be produced in the future by nuclear reaction .
In the extended periodic table (it is outside the “normal” periodic table ) it belongs to the alkali metals and the transactinoids . The name is the temporary systematic IUPAC name and stands for the three digits (Un-un-enn-ium) of the ordinal number. Furthermore, the 8th period, which has not yet been explored, begins with him . In the periodic table of the elements, it is expected to be an s-block element, an alkali metal, and the first element of the eighth period.
Synthetic routes
Ununennium is the element with the smallest atomic number that has not yet been synthesized. Several attempts were made by American, German, and Russian teams to synthesize this element. They have all been unsuccessful. Experiments suggest that the synthesis of Ununennium (and following elements) is likely to be much more difficult than that of the previous elements. Perhaps it is already the penultimate element that can be synthesized with current technology. Further trials by Japanese and Russian teams are planned for 2019-2020. Its position as the seventh alkali metal suggests that it could have properties similar to the lighter elements of main group 1. However, relativistic effects can lead to some properties differing from the expected trends. For example, it is expected that Ununennium is less reactive than cesium and francium and behaves more like potassium or rubidium and, in addition to the characteristic +1 oxidation number of alkali metals, could also have a +3 oxidation number.
Failed synthesis attempts
As early as 1985 an attempt was unsuccessful at the superHILAC linear accelerator in Berkeley to generate Ununennium by bombarding Einsteinium -254 with calcium -48 ions.
This reaction is unlikely to be successful because it is very difficult to make a sufficient amount of the Einsteinium target .
Target-projectile combinations for cores with Z = 119
The following table shows all the combinations for targets and projectiles that could be used to generate cores with a charge number of 119 whose half-life does not stand in the way (T 1/2 > 0.2 a):
Target | projectile | product | ||||
---|---|---|---|---|---|---|
core | HWZ (a) | core | HWZ (a) | core | core | comment |
208 Pb | stable | 87 Rb | 48 billion | 295 uue | 292 uue | too neutron poor °) |
232 Th | 14 billion | 65 Cu | stable | 297 Uue | 294 uue | |
238 U | 4.5 billion | 59 Co | stable | 297 Uue | 294 uue | |
238 U | 4.5 billion | 60 Co | 5.3 | 298 uue | 295 uue | |
237 Np | 2.1 million | 58 feet | stable | 295 uue | 292 uue | too neutron poor °) |
237 Np | 2.1 million | 60 feet | 2.6 million | 297 Uue | 294 uue | |
244 Pu | 80 million | 55 mn | stable | 299 uue | 296 uue | |
243 On | 7370 | 54 Cr | stable | 297 Uue | 294 uue | |
248 cm | 340000 | 51 V | stable | 299 uue | 296 uue | |
250 cm | 9000 | 51 V | stable | 301 Uue | 298 uue | |
247 Bk | 1380 | 50 Ti | stable | 297 Uue | 294 uue | |
248 Bk | 9 | 50 Ti | stable | 298 uue | 295 uue | |
249 Bk | 0.88 | 50 Ti | stable | 299 uue | 296 uue | |
249 Cf | 351 | 45 Sc | stable | 294 uue | 291 uue | too neutron poor °) |
250 cf | 13 | 45 Sc | stable | 295 uue | 292 uue | too neutron poor °) |
251 Cf | 900 | 45 Sc | stable | 296 uue | 293 uue | too neutron poor °) |
252 Cf | 2.6 | 45 Sc | stable | 297 Uue | 294 uue | |
252 it | 1.3 | 48 approx | ~ stable | 300 uue | 297 Uue | |
254 it | 0.75 | 48 approx | ~ stable | 302 Uue | 299 uue |
°) If one follows the trend of the last generated isotopes of 115 Moscovium and 117 Tenness, these nuclei contain far too few neutrons to have longer half-lives.
Prediction of the decay characteristics
The alpha decay half-lives of 1700 isotopes with a charge number between 100 and 130 were predicted on the basis of model calculations. The half-lives found for 291–307 Uue amount to a few microseconds. The isotope 294 Uue should have the longest half-life of almost half a millisecond .
Individual evidence
- ↑ RW Lougheed, JH Landrum, EK Hulet, JF Wild, RJ Dougan, AD Dougan, H. Gäggeler, M. Skull, KJ Moody, KE Gregorich, GT Seaborg: Search for superheavy elements using the 48 Ca + 254 Es g reaction . In: Physical Review C . tape 32 , no. 5 , 1985, pp. 1760-1763 , doi : 10.1103 / PhysRevC.32.1760 .
- ↑ C. Samanta, P. R Chowdhury, DN Basu: Predictions of alpha decay half lives of heavy and superheavy elements . In: Nuclear Physics, Section A . tape 789 , no. 1–4 , 2007, pp. 142-154 , doi : 10.1016 / j.nuclphysa.2007.04.001 , arxiv : nucl-th / 0703086v2 .
- ^ P. Roy Chowdhury, C. Samanta, DN Basu: Search for long lived heaviest nuclei beyond the valley of stability . In: Physical Review C (Nuclear Physics) . tape 77 , no. 4 , 2008, p. 044603-10 , doi : 10.1103 / PhysRevC.77.044603 , arxiv : 0802.3837v1 .
- ↑ P. R Chowdhury, C. Samanta, DN Basu: Nuclear half-lives for α-radioactivity of elements with 100 ≤ Z ≤ 130 . In: Atomic Data and Nuclear Data Tables . tape 94 , no. 6 , 2008, p. 781-806 , doi : 10.1016 / j.adt.2008.01.003 , arxiv : 0802.4161v2 .