Image Details
Caption: Figure 7.
Comparison of (top) mass-loss rates, dM/dt [kg s−1], (middle) nucleus radii, rn [km], and (bottom) specific mass-loss rates, ﹩{ \mathcal L }﹩ [kg km−2 s−1], for Bennu (B) and cometary bodies 133P/Elst–Pizarro, 2P/Encke, 67P/Churyumov–Gerasimenko and C/1995 O1 (Hale–Bopp). The Bennu data refer to HST measurements from the present work.
© 2026. The Author(s). Published by the American Astronomical Society.