In recent years, innovative studies have shown that sorption of metals onto
natural materials results in the formation of new mineral-like precipitate
phases that increase in stability with aging time. While these findings ha
ve demonstrated the usefulness of current state-of-the-art molecular-scale
methods for confirming macroscopic data and elucidating mechanisms, basic k
inetic and thermodynamic parameters for the formation of the metal precipit
ates have not been examined. This study examined Ni-sorption kinetics on py
rophyllite, talc, gibbsite, amorphous silica, and a mixture of gibbsite and
amorphous silica over a temperature range of 9 to 35 degreesC. Using the A
rrhenius and Eyring equations, we calculated the energy of activation (E-a)
and enthalpy (DeltaH(double dagger)), entropy (DeltaS(double dagger)), and
free energy of activation (DeltaG(double dagger)), related to the formatio
n of the Ni precipitates. Based on values of E-a (93.05 to 123.71 kJ mol(-1
)) and DeltaS(double dagger) (-27.51 to -38.70 J mol(-1)), Ni sorption on t
hese sorbents was surface-controlled and an associative mechanism, The Delt
aH(double dagger) values (90.60 to 121.26 kJ mol(-1)) suggest, as indicated
by E-a values, that an energy barrier was present for the system to overco
me in order for the reaction to occur, Additionally, the large, positive De
ltaG(double dagger) values suggest there is an energy barrier for product f
ormation. Although metal precipitation reactions often occur in the natural
environment, this study shows that the rate of these reactions depends str
ongly on temperature.