The method of a previous paper is generalized to yield all solutions to Einstein's equations for planar-symmetric walls composed of surface energy density $\ensuremath{\sigma}$ and tension $\ensuremath{\tau}$, with constant ratios in the physical range $\frac{\ensuremath{\tau}}{\ensuremath{\sigma}}\ensuremath{\le}1$. Special cases include domain walls, walls of cosmic strings, dust walls, and (when $\ensuremath{\tau}<0$) pressure walls. Attention is focused on the sense in which a wall is gravitationally repulsive when the tension is strong, the sense in which repulsion gives way to attraction as $\frac{\ensuremath{\tau}}{\ensuremath{\sigma}}$ is reduced below the value \textonehalf{}, and the way in which these features are reflected in the motion of the wall. Also studied is the way in which the unique static planar-symmetric solution fits within the classes of solutions.
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