It is shown that after a sufficiently long propagation time, the nonli
near dust-acoustic waves appear as a stationary shock wave structure.
The latter arises as a result of a balance between the nonlinear wave
breaking and the dissipation of the wave energy due to the variation o
f the dust particle charges. The presented analytical theory shows tha
t a necessary condition for the shock formation demands that the dust
acoustic wave frequency omega is considerably smaller than the dust ch
arging frequency omega(q0). In this frequency regime, the shock wave p
ropagation is described by the well-known Burgers equation. Furthermor
e, the breakdown of the analytical theory has been studied by solving
the basic set of fluid equations numerically. The numerical solutions
exhibit that shock waves may also occur for omega of the order of omeg
a(q0), viz. in a wave frequency regime that is not covered by our anal
ytical theory.