The Younger Dryas (YD) cosmic impact hypothesis is gaining support due to the increasing amount of proxy evidence from 26 Younger Dryas Boundary sites that includes depositions of magnetic, silicate, and carbon spherules; high‐temperature meltglass and melt accretions; nanodiamonds, and Ir and Pt deposits, as well as evidence of major biomass burning and widespread extinctions in stratigraphic layers dated ∼12.8 kyr ago. Among the possible causes, an encounter with a swarm of fragments on an orbit similar to that of 2P/Encke is proposed. This work suggests another potential source of impacting material that requires no special events in the Solar System: Main Belt asteroids excited into highly eccentric Earth‐crossing orbits via mean‐motion resonance with Jupiter and the ν6 secular resonance with Saturn—the established mechanisms of Main Asteroid Belt depletion and Earth‐bound meteorite delivery. It is shown that the probability of and the time between collisions of ejected material with Earth (Δt ∼ 32 kyr), as well as the energy of impacts, are broadly compatible with the YD impact proxy evidence. Such events may reoccur via bombardments of fragment swarms, potentially challenging existing asteroid deflection concepts.