Published July 14, 2020 | Version 1.0

Rubble pile models

Authors/Creators

  • 1. Politecnico di Milano

Description

Rubble pile models of small-body objects. 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.

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Additional details

Related works

Cites
Journal article: 10.1016/j.icarus.2020.113871 (DOI)
Journal article: 10.1093/mnras/stz3458 (DOI)
Journal article: 10.1007/s11044-016-9547-2 (DOI)

Funding

European Commission
GRAINS - Gravitation of Rubble-pile Asteroid with Internal N-body Structure 800060

References

  • 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