Variations in the structural setting and mineralogy of Proterozoic iro
n oxide Cu-U-Au-REE (rare earth element) deposits, particularly regard
ing apparent depth of formation, have resulted in models ranging from
direct injection of an Fe-oxide melt to formation via hydrothermal rep
lacement. The Emmie Bluff Fe-oxide deposit, South Australia, is unequi
vocally of hydrothermal origin and exhibits overprinting relations, vi
sible at both the meso- and microscopic scale, that strongly support a
model involving two temporally distinct fluids, as previously propose
d for the enormous Olympic Dam deposit. The evidence indicates that th
e first stage of magnetite-rich ore formation was associated with high
-temperature fluids from a major mid-Proterozoic felsic intrusive even
t. This was followed by infiltration of lower temperature fluids that
produced the hematite-rich mineralization. Whole-rock stable isotope a
nalyses are consistent with this model and suggest that the initial fl
uids were magmatic, with a deltaO-18 value of 8 parts per thousand-9 p
arts per thousand, whereas the later mineralizing fluids, had lower va
lues, 0 parts per thousand-2 parts per thousand, perhaps indicative of
a meteoric fluid component.