  Using a perturbative approach we solve stellar structure equations for
low-density (solar-type) stars whose interior is described with a polytropic
equation of state in scenarios involving a subset of modified gravity theories.
Rather than focusing on particular theories, we consider a model-independent
approach in which deviations from General Relativity are effectively described
by a single parameter $\xi$. We find that for length scales below those set by
stellar General Relativistic radii the modifications introduced by modified
gravity can affect the computed values of masses and radii. As a consequence,
the stellar luminosity is also affected. We discuss possible further
implications for higher density stars and observability of the effects before
described.
