The Mesoarchaean Murchison Greenstone Belt is composed of a strongly deformed volcano-sedimentary succession metamorphosed up to amphibolite facies and surrounded by metaluminous and peraluminous granitoids in the north of the Kaapvaal Craton of southern Africa.A circa 40 km-long shear-zone of strongly carbonatised rocks (the Antimony Line, or Sb-Line) oriented along the main trend of the greenstone belt (WSW-ENE) hosts important Sb deposits with accessory Au.These commodities mostly occur as stibnite and native gold hosted by quartz-carbonate rocks at the center of the Sb-Line, underlining the importance of CO2-rich fluid flow for mineralization during deformation and metamorphism.In this study, we compare the elemental and stable isotope (C-O-Mg) composition of carbonates from the Sb-Line with regionally distributed carbonates hosted by the volcano-sedimentary succession distal to mineralization.The carbonates of the Sb-Line and regional rocks have overlapping major element compositionsBoth magnesite and dolomite in most Sb-Line samples have marked light-REE-depleted patterns with variable pos. Eu anomalies.Carbon isotope ratios define two clusters, with marked δ13C peaks at ca. -5 ‰ for Sb-Line rocks and ca. -2 ‰ for regional rocks, implying sep. C-sources.The peak at ca. -2 ‰ likely represents early carbonatisation through sea-floor alteration, whereas the first peak at ca. -5 ‰ is indicative of deep CO2 (mantle, or magma-derived) introduced during tectonic activity of the Sb-Line.Magnesium isotope ratios of regional rocks reveal limited fractionation (bulk δ26Mg = -0.27 ± 0.10 ‰) that overlap with mantle values, but some carbonate-bearing veins present 26Mg-depleted compositions (bulk δ26Mg = -1.91 to -0.40 ‰).Sb-Line carbonated rocks have more fractionated Mg isotope compositions (bulk δ26Mg = -0.8 to 0.0 ‰) and carbonates display marked neg. 26Mg values (δ26Mg from -1.46 to -0.31 ‰).We interpret these results in terms of preferential remobilisation of isotopically light Mg during fluid-rock interaction and dissolution of carbonate in the host-rocks.The lack of correlation between δ13C and δ26Mg indicates decoupling of these isotopic systems, implying contribution from isotopically distinct sources of C and Mg to the mineralized zone.Similar to other structurally controlled Au-Sb mineralization in Archaean greenstone belts, metal transport and ore deposition in the Murchison Greenstone Belt was closely related to the deep cycle of carbon, linking C-draw-down during sea-floor alteration, carbonate re-mobilisation during metamorphism and CO2 degassing from deep sources along major crustal discontinuities.In contrast to models for orogenic Au-Sb deposits invoking a purely intra-crustal, metamorphic origin of mineralizing fluids, our results underline the importance of deep-sourced fluids originating from an external source from the volcano-sedimentary succession.