Asteroid Evolution: Role of Geotechnical Properties
arXiv:1511.08293 · doi:10.1017/S1743921315008583
Abstract
This paper presents a brief review and latest results of the work that has been carried out by the Planetary Science community in order to understand that role of the geotechnical properties of granular asteroids (commonly known as "rubble-pile" asteroids) in their formation, evolution and possible disruption. As such, we will touch in aspects of the theoretical and numerical tools that have been used with this objective and how the obtained results compare to the observed asteroids.
Invited review paper presented at the XXIX IAU General Assembly, August, 2015
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Cited by in corpus (4)
- Small Solar System Bodies as granular media
- The fast spin of near-Earth asteroid (455213) 2001 OE84, revisited after 14 years: constraints on internal structure
- Exploring the recycling model of Phobos formation: rubble-pile satellites
- Sub-surface granular dynamics in the context of oblique, low-velocity impacts into angular granular media