Parent aggregates

Description

Rubble pile models of parent aggregates. 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), 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.

Resources

Name Format Description Link
0 http://data.europa.eu/88u/dataset/oai-zenodo-org-3952097
0 http://data.europa.eu/88u/dataset/oai-zenodo-org-3952097
0 http://data.europa.eu/88u/dataset/oai-zenodo-org-3952097
0 http://data.europa.eu/88u/dataset/oai-zenodo-org-3952097
0 http://data.europa.eu/88u/dataset/oai-zenodo-org-3952097
0 http://data.europa.eu/88u/dataset/oai-zenodo-org-3952097
0 http://data.europa.eu/88u/dataset/oai-zenodo-org-3952097
0 http://data.europa.eu/88u/dataset/oai-zenodo-org-3952097

Tags

  • rubble-pile
  • small-body
  • n-body-simulation
  • asteroid

Topics

Categories