  In the context of the braneworld, a method to find consistent solutions to
Einstein's field equations in the interior of a spherically symmetric, static
and non uniform stellar distribution with Weyl stresses is developed. This
method, based in the fact that any braneworld stellar solution must have the
general relativity solution as a limit, produces a constraint which reduces the
degrees of freedom on the brane. Hence the non locality and non closure of the
braneworld equations can be overcome. The constraint found is physically
interpreted as a necessary condition to regain general relativity, and a
particular solution for it is used to find an exact and physically acceptable
analytical internal solution to no-uniform stellar distributions on the brane.
It is shown that such an exact solution is possible due to the fact that bulk
corrections to pressure, density and a metric component are a null source of
anisotropic effects on the brane. A conjecture is proposed about the
possibility of finding physically relevant exact solutions to non-uniform
stellar distributions on the brane.
