“…Although these positive fractionation factors are opposite to the kinetic isotope fractionation during FeS precipitation, either from Fe(II) aq solutions at room temperature (Butler et al, 2005) or from silicate melt at magmatic temperatures (Schuessler et al, 2007), it may explain the occurrence of positive A different interpretation involves sulphidisation of Fe-oxide minerals for the origin of these grains, as positive δ 56 Fe values have so far been described mainly from BIFs in the Archaean rock record Dauphas et al, 2004;Rouxel et al, 2005;Whitehouse and Fedo, 2007). Evidence for sulphidisation of Fe and Fe-Ti oxides, such as magnetite and ilmenite, collectively referred as "black sands", as well as BIF clasts has been observed in previous studies (Ramdohr, 1958) and resulted in a long-standing debate on the timing of sulphidisation, with the "placerists" arguing for pre-depositional sulphidisation (Ramdohr, 1958;Reimer and Mossman, 1990) and the "hydrothermalists" arguing for postdepositional sulphidisation of "black sands" (Barnicoat et al, 1997;Law and Phillips, 2006). (Yamaguchi et al, 2005).…”