Aqueous S[IV] species (HSO3−, SO32−) derived from volcanogenic atmospheric SO2 are  important to planetary habitability through their roles in proposed origins-of-life chemistry and influence on atmospheric sulfur haze formation, but the early cycling of S[IV] is poorly understood. Here, we combine new laboratory constraints on S[IV] disproportionation kinetics with a novel aqueous photochemistry model to estimate the concentrations of S[IV] in natural waters on prebiotic Earth. We show that S[IV] disproportionation is slow in pH≥ 7 waters, with timescale T≥ 1 year at room temperature, meaning that S[IV] was present in prebiotic natural waters. However, we also show that photolysis of S[IV] by UV light on prebiotic Earth limited [S[IV]]< 100μM in global-mean steady-state. Because of photolysis, [S[IV]] was much lower in natural waters compared to the concentrations generally invoked in laboratory simulations of origins-of-life chemistry (≥ 10 mM), meaning further work is needed to confirm whether laboratory S[IV]- dependent prebiotic chemistries could have functioned in nature. [S[IV]]≥ 1μM in terrestrial waters for: (1) SO2 outgassing ≥ 20× modern, (2) pond depths < 10 cm, or UV-attenuating agents present in early waters or the prebiotic atmosphere. Marine S[IV] was sub-saturated with respect to atmospheric SO2, meaning that atmospheric SO2  deposition was efficient and that, within the constraints of present knowledge, UV-attenuating sulfur hazes could only have persisted on prebiotic Earth if sulfur emission rates were very high (≳ 100× modern). Our work illustrates the synergy between planetary science, geochemistry and synthetic organic chemistry towards understanding the emergence and maintenance of life on early Earth.