Sulfur is important to planetary habitability, but the early sulfur
cycle is poorly understood. In particular, S[IV] species
(HSO,
SO), derived from volcanogenic
SO, are critically invoked in recent proposals for
origins-of-life chemistry and also influence atmospheric sulfur haze
formation, but their abundance in early natural waters is unclear. Here,
we combine new laboratory constraints on the kinetics of S[IV]
disproportionation 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] limits [S[IV]]< 100 μM in
global-mean steady state. Marine S[IV] was sub-saturation with
respect to atmospheric SO, meaning that
climate-altering, UV-attenuating sulfur hazes did not persist on
prebiotic Earth. [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 S[IV]-dependent prebiotic chemistries
discovered in the lab could have realistically functioned in nature.
[S[IV]]≥1 μM in terrestrial waters for: (1) SO
outgassing ≥20× modern, (2) pond depths <10 cm, or (3)
UV-attenuating agents present in early waters or the prebiotic
atmosphere. Our work illustrates the synergy between planetary science,
geochemistry and synthetic organic chemistry experiments in
understanding the emergence and maintenance of life on early Earth.