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We study solutions of the decoupled Maxwell equations in the exterior regionof a Schwarzschild black hole. In stationary regions, where the Schwarzschildcoordinate $r$ ranges over $2M < r_1 < r < r_2$, we obtain a decay rate of$t^{-1}$ for all components of the Maxwell field. We use vector field methodsand do not require a spherical harmonic decomposition.  In outgoing regions, where the Regge-Wheeler tortoise coordinate is large,$r_*>\epsilon t$, we obtain decay for the null components with rates of$|\phi_+| \sim |\alpha| < C r^{-5/2}$, $|\phi_0| \sim |\rho| + |\sigma| < Cr^{-2} |t-r_*|^{-1/2}$, and $|\phi_{-1}| \sim |\underline{\alpha}| < C r^{-1}|t-r_*|^{-1}$. Along the event horizon and in ingoing regions, where $r_*<0$,and when $t+r_*1$, all components (normalized with respect to an ingoing nullbasis) decay at a rate of $C \uout^{-1}$ with $\uout=t+r_*$ in the exteriorregion.

Decay of the Maxwell field on the Schwarzschild manifold