  The theory of macroscopic gravity provides a formalism to average the
Einstein field equations from small scales to largest scales in space-time. It
is well known that averaging is an operation that does not commute with
calculating the Einstein tensor and this leads to a correction term in the
field equations known as back-reaction. In this work, we derive exact solutions
to the macroscopic gravity field equations assuming that the averaged geometry
is plane or spherically symmetric, and the source is taken as vacuum, dust, or
perfect fluid. We then focus on the specific cases of spherical symmetry and
derive solutions that are analogous to the Schwarzschild, Tolman VII, and
Lema\^{\i}tre-Tolman-Bondi solutions. The geodesic equations and curvature
structure are contrasted with the general relativistic counterparts for the
Schwarzschild and Lema\^{\i}tre-Tolman-Bondi solutions.
