We present the results from a recent study of the structure and energi
es of the low-index surfaces of spinel (MgAl2O4) using atomistic simul
ation techniques. These illustrate the complexity of modelling the sur
faces of ternary oxides, particularly since cation ordering, resulting
in the formation of inverse spinel, plays a crucial role in determini
ng the relative surface stability. The simulations show some agreement
with the very limited experimental data available for the spinel clas
s of compounds. However, agreement with the most common experimental m
orphologies requires the consideration of kinetic factors.