Sulfur isotopic anomalies (Δ 33 S and Δ 36 S) have been used to trace the redox evolution of the Precambrian atmosphere and to document the photochemistry and transport properties of the modern atmosphere. Recently, it was shown that modern sulfate aerosols formed in an oxidizing atmosphere can display important isotopic anomalies, thus questioning the significance of Archean sulfate deposits. Here, we performed in situ 4S-isotope measurements of 3.2-and 3.5-billion-year (Ga)-old sulfates. This in situ approach allows us to investigate the diversity of Archean sulfate texture and mineralogy with unprecedented resolution and from then on to deconvolute the ocean and atmosphere Archean sulfur cycle. A striking feature of our data is a bimodal distribution of δ 34 S values at ∼+5‰ and +9‰, which is matched by modern sulfate aerosols. The peak at +5‰ represents barite of different ages and host-rock lithology showing a wide range of Δ 33 S between −1.77‰ and +0.24‰. These barites are interpreted as primary volcanic emissions formed by SO 2 photochemical processes with variable contribution of carbonyl sulfide (OCS) shielding in an evolving volcanic plume. The δ 34 S peak at +9‰ is associated with non-33 S-anomalous barites displaying negative Δ 36 S values, which are best interpreted as volcanic sulfate aerosols formed from OCS photolysis. Our findings confirm the occurrence of a volcanic photochemical pathway specific to the early reduced atmosphere but identify variability within the Archean sulfate isotope record that suggests persistence throughout Earth history of photochemical reactions characteristic of the present-day stratosphere.Archean | sulfate | sulfur isotopes | atmosphere photochemistry T he amount of sulfate and its sulfur isotopic composition in the ocean through time is a function of the dynamic changes of sulfate sources (oxidative weathering on land, magmatic and hydrothermal input, and atmospheric photochemical reactions) and sulfate sinks (microbial and hydrothermal sulfate reduction and sulfate mineral precipitation). Although the Earth's sulfate budget can be reasonably well constrained after ∼2.3 billion years (Ga) ago, when free oxygen became a permanent component of the atmosphere, our understanding of the ocean sulfate budget before 2.3 Ga ago is subject to uncertainties. The occurrence of mass-independent sulfur-isotope anomalies (MIF-S, noted Δ 33 S and Δ 36 S) in sedimentary sulfur (sulfide and sulfate) of Archean age (1) and the photochemical models (2) for the production and preservation of these anomalies support the view that the Archean atmospheric O 2 concentration was lower than 10 −5 times the present atmospheric level. In this model, photochemical reactions involving volcanic SO 2 in the anoxic atmosphere yields both a reduced sulfur reservoir that can carry a highly positive Δ 33 S and an oxidized sulfur reservoir with modestly negative Δ 33 S, the Δ 36 S values being of opposite sign. The corollary to this model is that sulfate influx from oxidative weathering on land should...