Inferred disk mass distribution in OMC-2 (red) compared to the disk mass distribution in low-mass star-forming regions (left) and to disks in the inner 1.5′ × 1.5′ of the ONC (blue, right). Data for the low-mass regions comes from Ansdell et al. (2016) for Lupus, Pascucci et al. (2016) for Cham I, and Barenfeld et al. (2016) for Upper Sco; only Class II objects with known stellar masses are included. For the ONC, disk masses come from Eisner et al. (2018). The three low-mass regions are reproduced as gray silhouettes in the right panel to facilitate the comparison.