Mass-independent fractionation of sulfur isotopes (S MIF) in Archean and Paleoproterozoic rocks provides strong evidence for an anoxic atmosphere before ∼2,400 Ma. However, the origin of this isotopic anomaly remains unclear, as does the identity of the molecules that carried it from the atmosphere to Earth's surface. Irrespective of the origin of S MIF, processes in the biogeochemical sulfur cycle modify the primary signal and strongly influence the S MIF preserved and observed in the geological record. Here, a detailed model of the marine sulfur cycle is used to propagate and distribute atmospherically derived S MIF from its delivery to the ocean to its preservation in the sediment. Bulk pyrite in most sediments carries weak S MIF because of microbial reduction of most sulfur compounds to form isotopically homogeneous sulfide. Locally, differential incorporation of sulfur compounds into pyrite leads to preservation of S MIF, which is predicted to be most highly variable in nonmarine and shallow-water settings. The Archean ocean is efficient in diluting primary atmospheric S MIF in the marine pools of sulfate and elemental sulfur with inputs from SO 2 and H 2 S, respectively. Preservation of S MIF with the observed range of magnitudes requires the S MIF production mechanism to be moderately fractionating ( ± 20-40‰). Constraints from the marine sulfur cycle allow that either elemental sulfur or organosulfur compounds (or both) carried S MIF to the surface, with opposite sign to S MIF in SO 2 and H 2 SO 4 . Optimal progress requires observations from nonmarine and shallow-water environments and experimental constraints on the reaction of photoexcited SO 2 with atmospheric hydrocarbons.W ith few exceptions, the enrichment or depletion of the rare, stable isotopes of sulfur ( 33 S, 34 S, and 36 S) relative to the abundant isotope ( 32 S) scale as the mass difference between the isotopes (1). Sulfur isotope mass-independent fractionation (S MIF) is defined as a departure from these theoretically derived and empirically observed mass laws, and denoted Δ 33 S and Δ 36 S. S MIF is observed in modern atmospheric sulfate aerosols, as well as in sulfate-bearing layers hosted in glacial ice (2, 3), but is conspicuously absent from the sedimentary record of the last 2,400 My. In contrast, older rocks of the Archean and early Paleoproterozoic eons preserve large and variable S MIF (4, 5). On the basis of experimental SO 2 photolysis and atmospheric chemistry models, the prevailing hypothesis to explain this observation is that the absence of atmospheric oxygen before ∼2,400 Ma allowed both the photochemical production of S MIF and its delivery to the surface in the reduced and oxidized products of sulfur photochemistry (4-7). Thus, S MIF is considered strong geochemical evidence for an anoxic atmosphere before ∼2,400 Ma.Although research converges on atmospheric processes as the source of S MIF, its production mechanism and the identity of its vectors to the surface remain unclear. A focus on photolysis experiments and meas...