room temperature [36]. It has also been proposed that cooled to its solid phase, oganesson would be a semiconductor [37].

And Beyond . . .

With the synthesis of element 117, the 7th Period has been completed. In Chapter 1, the issue of the future was addressed from the nucleosynthesis aspect. From the chemistry perspective, it is not about synthesizing a few fleeting atoms, but about finding long-lived isotopes — if they exist. Is there an “island of stability” yet to be found? If so, can super-neutron-rich projectiles be synthesized to bombard superheavy nuclei and reach the “island” [38]? Though such claims have been made before, it really does seem that the limit of actual chemistry of any new element has been reached. Yet there is the tantalization that such elements would open new possibilities in electron structure. Beyond the 8s orbitals loom the possibility of the 5g set. What are the properties of elements with g electrons? Will the orbitals fill in sequence or will things become “messy” as Pyykkö has suggested, in what is now called the Pyykkö Model [39].

Gilead has commented upon the “eka-elements” — those which are not actually known [40]:

There is no guarantee that they [eka-elements] will eventually be discovered, synthesized, or isolated as actual.

Perhaps this is indeed the completion of elemental chemistry as chemists know it.

Commentary

The actinoids exhibit a wider variety of chemical behavior than do the lanthanoids. Even though the first members of the actinoid series are no longer placed with the transition metals, nevertheless, in the highest oxidation states, there are strong chemical similarities to them. In addition, toward the end of the series, the preference for a 5f14 electron configuration marks results in two surprisingly low stable oxidation states. Unfortunately, the short half-lives of these later actinoids decrease the ability to fully explore their chemistry. Despite the strong influence of relativistic effects, even for the post-actinoid elements, the element properties so far seem to be mostly those expected for the appropriate group membership.

Will this continue into the 8th Period? As Haba has commented [41]:

Owing to the predicted strong influence of relativistic effect, any experimental investigation of their properties is fascinating.

Is attaining stable enough atoms of elements of the 8th Period a feasible goal or simply fantasy? Only time will tell.

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