The MMT Adaptive optics exoPlanet characterization System (MAPS) is an exoplanet characterization program that encompasses instrument development, observational science, and education. MAPS will characterize the composition and physical characteristics of substellar companions including systems with close-in orbits identified by transit and radial velocity techniques, and wide-orbit companions identified by direct imaging. The MAPS spectral coverage will provide a single snapshot observation covering 1 to 5 micron (with gaps) at a high spectral resolution R~45,000. An upgrade is being proposed for an ultra-high resolution mode at R~100,000. The adaptive optics (AO) system has a versatile optical/infrared wavefront sensor based on two pyramid wavefront sensors (one optical, one infrared) to lock on obscured or faint guide stars, incorporating two state-of-the-art detectors than can be used to optimize the AO correction for a broad range of targets, with the control loop operating at up to a1 kHz rate. The 6.5m MMT telescope will have an upgraded adaptive secondary mirror with 336 actuators to improve the performance while
preserving the desired low backgrounds for long wavelength observations. With the completed MAPS instrument, we will execute a 60-night science program to characterize the atmospheric composition and dynamics of ~50-75 planets around other stars. The AO system had first light observations and the system commissioning is in progress. The science and education programs are in planning and preparation.