  Using canonical (Schrodinger) quantization of spherically symetric
gravitational dust systems, we find the quasi-classical (coherent) state,
|\alpha^{(s)}>, that corresponds to the classical Schwarzschild solution. We
calculate the ``quasi-classical Schwarzschild mertic", which is the expectation
value of the quantized metric in thhis quasi-classical state. Depending on the
quantization scheme that we use, we study three different quasi- classical
geometries, all of which turn out to be singularity free. Their maximal
extensions are complete manifolds with no singularities, describing a tower of
asymptotically flat universes connected through Planck size wormholes.
