 Marginal escape geodesic in Schwarzschild spacetime

The outgoing radial timelike geodesic with zero speed at infinity has $k=1$ and $dr/d\tau =\sqrt{2GM/r}$. Thus $r(\tau )=[r_0^{3/2}+(3/2)\sqrt{2GM}\tau {]}^{2/3}$ and the local static-observer speed is $\sqrt{2GM/r}$.