Equilibrium rubble pile ellipsoids. The models are obtained through numerical N-body simulations, using the GRAINS software. Simulations are performed using non-spherical particles, mutually interacting under contact/collisions and self-gravity. See Ferrari & Tanga 2020 (doi: 10.1016/j.icarus.2020.113871) for analysis and discussion of results. See Ferrari et al 2020 (doi: 10.1093/mnras/stz3458), Ferrari et al 2016 (doi: 10.1007/s11044-016-9547-2) for further details on the numerical model.

{"references": ["Ferrari & Tanga (2020). Doi: 10.1016/j.icarus.2020.113871)", "Ferrari et al (2016). Doi: 10.1007/s11044-016-9547-2", "Ferrari et al (2020). Doi: 10.1093/mnras/stz3458"]}