Complex mixtures of sulfates, silicates, and ice have been observed in a variety of planetary environments on Earth, Mars and the icy satellites of the solar system. Characterizing the properties of the corresponding compositional endmembers is important for understanding the interiors of a range of planetary bodies in which these phases are observed. To measure the electronic and vibrational properties of the iron endmember, szomolnokite, (FeSO 4 ⋅H 2 O), we have performed synchrotron 57 Fe nuclear resonant inelastic and forward scattering experiments in the diamond anvil cell up to 14.5 GPa. This pressure range covers depths within Earth's interior relevant to sulfur cycling in subduction zones and the range of pressures expected within icy satellites interiors. We nd evidence of crystal lattice softening, changes in elastic properties, and changes in the electric eld gradients of iron atoms associated with two structural transitions occurring within the experimental pressure range. We apply these ndings to icy satellite interiors, including discussion of elastic properties and implications for tidal observations.