  We calculate the shear viscosity $\eta$ and thermal conductivity $\kappa$ of
a nuclear pasta phase in neutron star crusts. This involves complex
non-spherical shapes. We use semiclassical molecular dynamics simulations
involving 40,000 to 100,000 nucleons. The viscosity $\eta$ can be simply
expressed in terms of the height $Z^*$ and width $\Delta q$ of the peak in the
static structure factor $S_p(q)$. We find that $\eta$ increases somewhat,
compared to a lower density phase involving spherical nuclei, because $Z^*$
decreases from form factor and ion screening effects. However, we do not find a
dramatic increase in $\eta$ from non-spherical shapes, as may occur in
conventional complex fluids.
