  We present the non-relativistic limit of the stellar structure equations of
Ricci-based gravities, a family of metric-affine theories whose Lagrangian is
built via contractions of the metric with the Ricci tensor of an a priori
independent connection. We find that this limit is characterized by four
parameters that arise in the expansion of several geometric quantities in
powers of the stress-energy tensor of the matter fields. We discuss the
relevance of this result for the phenomenology of non-relativistic stars, such
as main-sequence stars as well as several substellar objects.
