Image Details
Caption: Figure 3.
The fraction of total carbon reservoir left at 10 Myr, relative to a planetesimal’s initial C abundance, for planetesimals with varying radii. Blue, green, red, and orange lines are bodies of EH, OC, CV, and CI compositions. Dashed lines are the fraction of bulk carbon in completely sintered layers.
© 2026. The Author(s). Published by the American Astronomical Society.