The
mean annual surface temperatures on present and early Mars
likely remain well below 0 °C with episodic warming to temperatures
as high as 20 °C. Temperature exerts a strong control on geochemical
processes but fundamental phenomena like iron oxidation and the formation
of iron oxides have not been widely studied below 20 to 25 °C.
Earlier studies have demonstrated the effectiveness of chlorate in
oxidizing dissolved Fe(II) to form Fe(III)-bearing minerals commonly
found on Mars. Here, we determined the rate of oxidation of dissolved
ferrous iron by chlorate and the resulting formation of mineral precipitates
as a function of temperature in Mars-relevant fluids. The results
demonstrate that chlorate oxidizes dissolved Fe(II) at temperatures
as low as 0 °C on the time scale of weeks to months. Mixtures
of different Fe(III) phases, including goethite, lepidocrocite, schwertmannite,
and akaganeite, were produced and the minerals formed were found to
be primarily dependent on the fluid type, pH, concentration, and temperature.
Chloride-rich solutions favored the formation of akaganeite at 4 °C
while 24 °C solutions favored lepidocrocite. In both chloride-
and sulfate-rich solutions, lepidocrocite formation was favored at
4 °C whereas 24 °C fluids preferably produced goethite.
Schwertmannite formed in sulfate-rich solutions that started at low
pH. An established kinetic rate law model parametrized at higher temperatures
was found to be accurate in determining the rate of Fe(II) oxidation
at temperatures as low as 0 °C. Rate comparisons of Fe(II) oxidation
showed that in an ∼1 mmol L–1 chlorate solution
at 0 °C the rate is about three times faster than under 1 bar
oxygen at 25 °C, demonstrating the effectiveness of chlorate
as an important Fe(II) oxidant on Mars. The impact of temperature
in determining the Fe(III) oxidation products suggests that iron mineralogy
in cryogenic systems on Mars may be distinct from the phases forming
in more clement terrestrial analog environments.