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This paper is devoted to exploring how we can discover and study nearby (<1-2 kpc) planetary and binary systems by observing their action asgravitational lenses. Lensing can extend the realm of nearby binaries andplanets that can be systematically studied to include dark and dim binaries,and face-on systems. As with more traditional studies, which use light from thesystem, orbital parameters (including the total mass, mass ratio, and orbitalseparation) can be extracted from lensing data, Also in common with thesetraditional methods, individual systems can be targeted for study. We discussthe specific observing strategies needed in order to optimize the discovery andstudy of nearby planetary and binary systems by observing their actions aslenses.

Discovery and Study of Nearby Planetary and Binary Systems Via Mesolensing