  We examine the relative orientations of radio jets, central dust and stars in
low-power (i.e., FR I and FR I/II) radio galaxies. We use the position angles
of jet and dust to constrain the three-dimensional angle $\theta_{\rm DJ}$
between jet and dust. For galaxies with filamentary dust 'lanes' (which tend to
be misaligned with the galaxy major axis) the jet is approximately
perpendicular to the dust structure, while for galaxies with elliptical dust
distributions (typically aligned with the galaxy major axis) there is a much
wider distribution of $\theta_{\rm DJ}$. nThe dust ellipses are consistent with
being nearly circular thin disks viewed at random viewing angles. The lanes are
likely warped, unsettled dust structures. We consider two scenarios to explain
the dust/jet orientation dichotomy.
