XAS investigations of Fe(VI)

Recent attention has been given to a reexamination of results from the early Viking missions to Mars that suggested the presence of one or more strong oxidants in Martian soil. Since Fe is one of the main constituents of the Martian surface and Fe( VI) is known to be a highly reactive, strong oxidant, we have made XANES and EXAFS measurements of Fe( II), Fe( III), Fe( IV), and Fe( VI) in solid and solution forms. Results from these studies indicate a preedge XANES feature from Fe( VI) samples similar to that commonly seen from Cr( VI) samples. Results of first shell analysis indicate a linear relationship between the Fe-O bondlength and Fe valence state.