We have performed an extensive computational investigation of the potential energy surfaces for the reactions of SO x (x = 2 or 3) with H 2 S and H 2 O in the gas phase and in aqueous solution at the CCSD(T)/CBS level of theory plus a self-consistent reaction field approach. Formation of a gas-phase H 2 SO 4 from the hydrolysis of SO 3 at lower temperatures requires the presence of additional water molecules. When additional waters are introduced, the barrier for H 2 SO 4 formation is significantly reduced, and a barrierless transition occurs with only three excess waters as well as in aqueous solution. In a mixture of H 2 O, H 2 S, and SO 3 , formation of H 2 S 2 O 3 has a lower barrier in the gas phase than does the formation of H 2 SO 4 . In aqueous solution, no barrier is predicted, and both are likely to be formed. Introduction of an additional water to the SO 3 + H 2 S reaction results in a decrease in barrier height, nearly identical to the ∼18 kcal/mol catalytic effect of the first additional water in SO 3 hydrolysis, with the barrier for H 2 S 2 O 3 formation disappearing altogether in aqueous solution. Formation of H 2 SO 3 by the way of SO 2 hydrolysis is unlikely. Excess waters reduce the barrier for SO 2 hydrolysis; however, the overall endothermicity is increased as waters are added. The formation of H 2 S 2 O 2 from SO 2 and H 2 S via an isostructural pathway to SO 2 hydrolysis is unlikely, with additional water molecules resulting in a small increase in the overall endothermicity and a catalytic effect smaller than that observed for the SO 3 reactions. The results of this work have implications pertaining to the formation of H 2 SO 4 , H 2 S 2 O 3 , H 2 SO 3 , and H 2 S 2 O 2 in the atmospheres of Earth and Venus. These results also question the existence of H 2 S 2 O 2 as an intermediate in the Claus process.