  Modified Newtonian dynamics, a successful alternative to the cosmic dark
matter model, proposes that gravitational field deviates from the Newtonian law
when the field strength $g$ is weaker than a critical value $g_0$. We will show
that the dynamics of MOND can be derived from an induced gravity model. New
dynamics is shown to be compatible with the spatial deformation of scalar
fields coupled to the system. Approximate solutions are shown explicitly for a
simple toy model.
