  We derive the cosmological Big Bounce scenario from the dipole approximation
of Loop Quantum Gravity. We show that a non-singular evolution takes place for
any matter field and that, by considering a massless scalar field as a
relational clock for the dynamics, the semi-classical proprieties of an initial
state are preserved on the other side of the bounce. This model thus enhances
the relation between Loop Quantum Cosmology and the full theory.
