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The physicochemical properties of the three heaviest alkaline-earth cations, Sr 2+ , Ba 2+ , and Ra 2+  in water have been studied by means of classical molecular dynamics (MD) simulations. A specific set of cation–water intermolecular potentials based on ab initio potential energy surfaces has been built on the basis of the hydrated ion concept. The polarizable and flexible model of water MCDHO2 was adopted. The theoretical–experimental comparison of structural, dynamical, energetic, and spectroscopical properties of Sr 2+  and Ba 2+  aqueous solutions is satisfactory, which supports the methodology developed. This good behavior allows a reasonable reliability for the predicted Ra 2+  physicochemical data not experimentally determined yet. Simulated extended X-ray absorption fine-structure (EXAFS) and X-ray absorption near-edge spectroscopy spectra have been computed from the snapshots of the MD simulations and compared with the experimental information available for Sr 2+  and Ba 2+ . For the Ra 2+  case, the Ra L 3 -edge EXAFS spectrum is proposed. Structural and dynamical properties of the aqua ions for the three cations have been obtained and analyzed. Along the [M(H 2 O)  n  ]  m +  series, the M–O distance for the first-hydration shell is 2.57, 2.81, and 2.93 Å for Sr 2+ , Ba 2+ , and Ra 2+ , respectively. The hydration number also increases when one is going down along the group: 8.1, 9.4, and 9.8 for Sr 2+ , Ba 2+ , and Ra 2+ , respectively. Whereas [Sr(H 2 O) 8 ] 2+  is a typical aqua ion with a well-defined structure, the Ba 2+  and Ra 2+  hydration provides a picture exhibiting an average between the ennea- and the deca-hydration. These results show a similar chemical behavior of Ba 2+  and Ra 2+  aqueous solutions and support experimental studies on the removal of Ra-226 of aquifers by different techniques, where Ra 2+  is replaced by Ba 2+ . A comparison of the heavy alkaline ions, Rb +  and Cs + , with the heavy alkaline-earth ions is made.

Hydration of Heavy Alkaline-Earth Cations Studied by Molecular Dynamics Simulations and X-ray Absorption Spectroscopy