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Orbital resonances are believed to be responsible for the delivery of mainbelt asteroids to the inner Solar System. Several possibilities have beensuggested to transport asteroids and their fragments into mean motion andsecular resonances including non-gravitational forces and gravitationalscattering. We investigate future resonance crossings of known asteroids thatoccur in the main belt over the next century. Our goal is to identifypotentially observable injections of asteroids into source regions for NearEarth Objects (NEOs) as well as to determine the role of close encounters amongmain belt asteroids in this process.

On future opportunities to observe gravitational scattering of main belt asteroids into NEO source regions