Empirical and theoretical evidence show that the astrophysical problem
of dark matter might be solved by a theory of Einstein-Mayer type. In
this theory, up to global Lorentz rotations, the reference system is
determined by the motion of cosmic matter. Thus, one is led to a ''Rie
mannian space with teleparallelism'' realizing a geometric version of
the Mach-Einstein doctrine. The field equations of this gravitational
theory contain hidden matter terms, where the existence of hidden matt
er is inferred solely from its gravitational effects. It is argued tha
t, in the nonrelativistic mechanical approximation, they provide an in
ertia-fee mechanics, where the inertial mass of a body is induced by t
he gravitational action of the comic masses. Interpreted from the Newt
onian point of view, this mechanics shows that the effective gravitati
onal mass of astrophysical objects depends on r such that one expects
the existence of dark matter.