The Bulk Densities of Small Solar System Bodies as a Probe of
Planetesimal Formation
The Bulk Densities of Small Solar System Bodies as a Probe of
Planetesimal Formation
Constraining the formation processes of small solar system bodies is crucial for gaining insights into planetesimal formation. Their bulk densities, determined by their compressive strengths, offer valuable information about their formation history. In this paper, we utilize a formulation of the compressive strength of dust aggregates obtained from dust $N$-body …