Atomistic simulation techniques were used to investigate the surface e
nergies and stabilities of the sphalerite form of ZnS. The results sho
w that for pure ZnS the lowest energy surfaces are type I and all of t
he form {110} with a calculated surface energy of 0.65 J/m(2). In addi
tion, we illustrate how type III surfaces, such as {(111) over bar}, c
an be stabilized with respect to {110} by the introduction of point de
fects to the surface layer. Such defects lead to changes in stoichiome
try an to the valence state of surface species. In general, the result
s suggest that for Zn-poor surface stoichiometries, the (111) surface
becomes the most stable, whereas for Zn-rich compositions the ((111) o
ver bar) is stabilized to the greatest extent.