We show that the statistical error, $σ_τ$, in estimating the optical depth, $τ$, due to microlensing is substantially higher than the naive Poisson estimate: $σ_τ = \sqrt{η/ N} τ$, where $N$ is the number of detections and $1.65 \leq η\lsim 3$. We construct a ``microlensing map'' using an observationally well-constrained barred bulge model and compare this with a map based on a spherical bulge model. The result indicates a significant differences in the distribution of optical depths. If the optical depths are determined over a wide range of positions around the Galactic center, one could make a rudimentary determination of the geometry of the mass distribution of the Galactic bulge by observing $\sim 200$ events. About 800 events are required to determine the relative contributions to the event rate by bulge and disk Machos.

13 pages, 2 figures, 1 tables, request hard copy of preprint to cheongho@payne.mps.ohio-state.edu, OSU-TA-23/94