1. UV radiation from massive stars in Orion may promote the growth of planetesimals by removing dust-depleted gas from protoplanetary disks via photoevaporation. 2. As grains grow and sediment to the disk midplane, the gas-to-dust ratio at the surface increases. UV ablation then leaves behind a metal-enriched midplane. 3. The higher metallicity allows gravitational instability to rapidly form kilometer-scale planetesimals on shorter timescales than radial drift of solids. Some evidence supports this process occurring in Orion's proplyds.