VLBI observations remain the only direct evidence for relativistic outflows from supermassive black holes in active galactic nuclei (AGN).  The MOJAVE program realizes one of the envisioned goals of the VLBA, which is to provide long-term, systematic monitoring of relativistic motion in AGN jets on parsec-scales. The major aims of our program are to a) provide a significant improvement over previous surveys in terms of image resolution, size, and statistical completeness, and b) to characterize the kinematics and polarization evolution of AGN jets and to determine how these relate to other source properties. We are currently providing up-to-date parsec-scale structural information on nearly 300 AGN jets in support of the Fermi Gamma-Ray Observatory.