The chemical nature and aggregate state of superheavy copernicium (Cn) have been subject of speculation for many years.W hile strong relativistic effects render Cn chemically inert, which led Pitzer to suggest an oble-gas-like behavior in 1975, Eichler and co-workers in 2008 reported substantial interactions with ag old surface in atom-at-a-time experiments,s uggesting am etallic character and as olid aggregate state.H erein, we explore the physicochemical properties of Cn by means of first-principles free-energy calculations,w hichc onfirm Pitzerso riginal hypothesis:W ith predicted melting and boiling points of 283 AE 11 Ka nd 340 AE 10 K, Cn is indeed avolatile liquid and exhibits adensity very similar to that of mercury.H owever,i ns tark contrast to mercury and the lighter Group 12 metals,wefind bulk Cn to be bound by dispersion and to exhibit alarge band gap of 6.4 eV, which is consistent with an oble-gas-like character.T his nongroup-conforming behavior is eventually traced backtostrong scalar-relativistic effects,a nd in the non-relativistic limit, Cn appears as ac ommon Group 12 metal.Supportinginformation and the ORCID identification number(s) for the author(s) of this article can be found under: https://doi.org/10.