Ununennium, also known as eka-francium or element 119, is a hypothetical chemical element; it has symbol Uue and atomic number 119. Ununennium and Uue are the temporary systematic IUPAC name and symbol respectively, which are used until the element has been discovered, confirmed, and a permanent name is decided upon. In the periodic table of the elements, it is expected to be an s-block element, an alkali metal, and the first element in the eighth period. It is the lightest element that has not yet been synthesized. Attempts to synthesize the element have been ongoing since 2018 in RIKEN in Japan, and since 2026 at the Joint Institute for Nuclear Research in Dubna, Russia. The Heavy Ion Research Facility in Lanzhou, China (HIRFL) also plans to make an attempt. Theoretical and experimental evidence has shown that the synthesis of ununennium will likely be far more difficult than that of the previous elements. Ununennium's position as the seventh alkali metal suggests that it would have similar properties to its lighter congeners. However, relativistic effects may cause some of its properties to differ from those expected from a straight application of periodic trends. For example, ununennium is expected to be less reactive than caesium and francium and closer in behavior to potassium or rubidium, and while it should show the characteristic +1 oxidation state of the alkali metals, it is also predicted to show the +3 and +5 oxidation states, which are unknown in any other alkali metal.
Introduction
History
Synthesis attempts
Past Elements 114 to 118 (flerovium through oganesson) were discovered in "hot fusion" reactions at the Joint Institute for Nuclear Research (JINR) in Dubna, Russia. This involved bombarding the actinides plutonium through californium with calcium-48, a quasi-stable neutron-rich isotope which could be used as a projectile to produce more neutron-rich isotopes of superheavy elements. (The term "hot" refers to the high excitation energy of the resulting compound nucleus.) This cannot easily be continued to element 119, because it would require a target of the next actinide einsteinium. Tens of milligrams of einsteinium would be needed for a reasonable chance of success, but only micrograms have so far been produced. An attempt to make element 119 from calcium-48 and less than a microgram of einsteinium was made in 1985 at the superHILAC accelerator at Berkeley, California, but did not succeed.
25499Es + 4820Ca → 302119Uue* → no atoms More practical production of further superheavy elements requires projectiles heavier than 48Ca, but this makes the reaction more symmetric and gives it a smaller chance of success. Attempts to synthesize element 119 push the limits of current technology, due to the decreasing cross sections of the production reactions and the probably short half-lives of produced isotopes, expected to be on the order of microseconds. From April to September 2012, an attempt to synthesize 295Uue and 296Uue was made by bombarding a target of berkelium-249 with titanium-50 at the GSI Helmholtz Centre for Heavy Ion Research in Darmstadt, Germany. This reaction between 249Bk and 50Ti was predicted to be the most favorable practical reaction for formation of ununennium, as it is the most asymmetric reaction available. Moreover, as berkelium-249 decays to californium-249 (the next element) with a short half-life of 327 days, this allowed elements 119 and 120 to be searched for simultaneously. Due to the predicted short half-lives, the GSI team used new "fast" electronics capable of registering decay events within microseconds.
24997Bk + 5022Ti → 299119Uue* → no atoms 24998Cf + 5022Ti → 299120Ubn* → no atoms Neither element 119 nor element 120 was observed. This implied a limiting cross-section of 65 femtobarn for producing element 119 in these reactions, and 200 fb for element 120. The experiment was originally planned to continue to November 2012, but was stopped early to make use of the 249Bk target to confirm the synthesis of tennessine (thus changing the projectile to 48Ca).
Present
The team at RIKEN in Wakō, Japan began bombarding curium-248 targets with a vanadium-51 beam in January 2018 to search for element 119. Curium was chosen as a target, rather than heavier berkelium or californium, as these heavier targets are difficult to prepare. The 248Cm targets were provided by Oak Ridge National Laboratory. RIKEN developed a high-intensity vanadium beam. The experiment began at a cyclotron while RIKEN upgraded its linear accelerators; the upgrade was completed in 2020. Bombardment may be continued with both machines until the first event is observed. The RIKEN team's efforts are being financed by the Emperor of Japan.
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![Ununennium: A graphic depiction of a nuclear fusion reaction. Two nuclei fuse into one, emitting a neutron. Reactions that created new elements to this moment were similar, though varying numbers of neutrons – or alternatively charged particles – may be emitted instead.[9]](https://upload.wikimedia.org/wikipedia/commons/thumb/3/3b/Deuterium-tritium_fusion.svg/330px-Deuterium-tritium_fusion.svg.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
![Ununennium: Scheme of an apparatus for creation of superheavy elements, based on the Dubna Gas-Filled Recoil Separator set up in the Flerov Laboratory of Nuclear Reactions in JINR. The trajectory within the detector and the beam focusing apparatus changes because of a dipole magnet in the former and quadrupole magnets in the latter.[36]](https://upload.wikimedia.org/wikipedia/commons/thumb/3/34/Apparatus_for_creation_of_superheavy_elements_en.svg/500px-Apparatus_for_creation_of_superheavy_elements_en.svg.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
![Ununennium: The curium oxide targets used by RIKEN for the search for element 119[63]](https://upload.wikimedia.org/wikipedia/commons/thumb/7/78/Curium_oxide_targets.jpg/500px-Curium_oxide_targets.jpg?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
![Ununennium: A chart of nuclide stability as used by the Dubna team in 2010. Characterized isotopes are shown with borders. Beyond element 118 (oganesson, the last known element), the line of known nuclides is expected to rapidly enter a region of instability. The white ring encloses the predicted location of the island of stability.[57]](https://upload.wikimedia.org/wikipedia/commons/thumb/8/89/Island_of_Stability_derived_from_Zagrebaev.svg/500px-Island_of_Stability_derived_from_Zagrebaev.svg.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
![Ununennium: Orbitals with high azimuthal quantum number are raised in energy, eliminating what would otherwise be a gap in orbital energy corresponding to a closed proton shell at element 114, as shown in the left diagram which does not take this effect into account. This raises the next proton shell to the region around element 120, as shown in the right diagram, potentially increasing the half-lives of element 119 and 120 isotopes.[80]](https://upload.wikimedia.org/wikipedia/commons/thumb/7/70/Next_proton_shell.svg/500px-Next_proton_shell.svg.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
