  We summarize the use of Noether symmetries in Minisuperspace Quantum
Cosmology. In particular, we consider minisuperspace models, showing that the
existence of conserved quantities gives selection rules that allow to recover
classical behaviors in cosmic evolution according to the so called Hartle
criterion. Such a criterion selects correlated regions in the configuration
space of dynamical variables whose meaning is related to the emergence of
classical observable universes. Some minisuperspace models are worked out
starting from Extended Gravity, in particular coming from scalar tensor, f(R)
and f(T) theories. Exact cosmological solutions are derived.
