Image Details
Caption: Figure 3.
The estimated parent-body diameters and formation ages of families reported in this catalog. See Sections 2.5 and 2.6 for the method used to determine these parameters. The color indicates ﹩f={({D}_{{\rm{LM}}}/{D}_{{\rm{PB}}})}^{3}﹩ where DLM and DPB are the estimated largest-member and parent-body diameters, respectively. The families produced by the cratering collisions appear as dark blue dots; the catastrophic breakups with f < 0.5 are shown in red.
© 2026. The Author(s). Published by the American Astronomical Society.