The Hg-Ra phase diagram is not known. The melting points of Hg and Ra are −38.8290 and 700 °C, respectively. Information about the crystallographic features of both metals is given in Table 1. [1910Cur] prepared ∼0.8 at.% Ra amalgam by electrolysis. It looked completely fluid at room temperature. When heated, it became solid at 400 °C and emanated the rest of the Hg at 700 °C. [1962Koz] calculated the solubility of Ra in liquid Hg of 1.1 at.% Ra at 25 °C using a semiempirical equation relating metal solubility to its entropy of melting. Calculations by the same author [1992Koz], using a regular solution approximation and the cellular model of Miedema et al. [1983Nie], resulted in solubility values both equal to 0.5 at.% Ra. In the opinion of this evaluator, these estimations give the proper order of magnitude for Ra solubility. One may predict a probable Hg-Ra phase relationships by an extrapolation of the systematic changes in the behavior of Mg, Ca, Sr, and Ba in their binary alloys with Hg [2004Gum]. A distinct tendency to formation of the Hgricher compounds is observed with an increase in the atomic number of the alkaline earth metal series. Therefore, it is not clear whether HgRa2 exists, but most probably the congruently melting HgRa and Hg2Ra compounds should be the most stable phases of the Hg-Ra system. Moreover, a formation of Hg31Ra7, Hg11Ra, and Hg∼6Ra, by analogy to the Ba-Hg compounds, is expected. [1992Koz] reported the formation of HgRa, Hg2Ra, and Hg4Ra, but the experimental evidence underlying this report is unknown. Strong affinity between Hg and Ra is manifested in the partial excess Gibbs energy of Ra in its very diluted amalgam. This energy was found to be −255 ± 10 kJ/mol Ra near room temperature, and −243.8 kJ/mol Ra at 25 °C, respectively, according to [1975Nug] and [1990Kor]. These values point to stronger Hg-Ra interactions in the Hg-rich RaHg alloys than was observed in the Ba-Hg system [2000Gum]. The partial excess Gibbs energy was calculated from the difference between the standard potential of Ra/ Ra(II) and the polarographic half-wave potential of Ra, which was experimentally determined by a radiopolarographic method [1975Nug]. [1977Koz] reported the partial excess Gibbs energy (−250 kJ/mol) and enthalpy (−313 kJ/ mol) of Ra in its diluted amalgam by an extrapolation of the corresponding values for Ca, Sr, and Ba compared with the electronegativity or atom radii of these elements to the position of Ra. Because neither the electronegativity nor the atomic radius of Ra is precisely known, the strongly negative partial enthalpy value should be treated very tentatively. The activity coefficient of Ra in a dilute amalgam was estimated by [1989Gum] to be on the order of 10. This also points to a very strong interaction between Hg and Ra.
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