The mean gaseous motion in solid and, less commonly, hybrid rocket motors has been traditionally described assuming inviscid flow in a porous cylinder of fixed radius and constant mass addition at the sidewall. This model, usually referred to as the Taylor-Culick profile, is a simple inviscid rotational solution that captures the bulk gaseous motion in a rocket chamber with sidewall injection. In practice, however, the radius of the rocket motor increases as the propellant burns, thus leading to time-dependent effects on the mean flow that are not embraced by the Taylor-Culick model. In this work, we revisit the problem of the viscous flow in a porous cylinder and allow the radius to be time dependent. By implementing Uchida's well established similarity transformation in space and time, the incompressible Navier-Stokes equations are first reduced to a nonlinear fourth-order ordinary differential equation with four boundary conditions that contain, in the case of an axisymmetric chamber, an irregular limit. This equation is then solved both numerically and asymptotically, using the injection Reynolds number, Re, and the dimensionless wall regression ratio, α, as primary and secondary perturbation parameters. At the outset, closed-form analytical solutions are obtained for both large and small Re with small-to-moderate α. The resulting approximations are then compared to the numerical solution obtained for an equivalent third-order ODE in which both shooting and the irregular limit are circumvented. We find our code capable of producing the stable solutions for this problem over a wide range of Reynolds numbers and wall regression ratios. The code also enables us to confirm the accuracy of the asymptotic approximations, both of which being presented either for the first time in the case of small suction and injection or reconstructed with additional detail in the case of large injection.