Critical spin periods of sub-km-sized cohesive rubble-pile asteroids: dependencies on material parameters
Shoucun Hu, Derek C. Richardson, Yun Zhang, Jianghui Ji

TL;DR
This study investigates how material properties influence the critical spin periods of sub-km-sized cohesive rubble-pile asteroids using numerical simulations and analytical comparisons.
Contribution
It introduces a detailed numerical model exploring the dependencies of critical spin periods on multiple material parameters and compares results with continuum theory.
Findings
Both cohesion and particle shape strengthen rubble piles.
Critical diameter D_{cri,ρ} marks a reversal in T_c dependence on density.
The ratio of interparticle to bulk cohesion is approximately 88.3.
Abstract
In this work, we employ a soft-sphere discrete element method with a cohesion implementation to model the dynamical process of sub-km-sized cohesive rubble piles under continuous spinup. The dependencies of critical spin periods on several material parameters for oblate rubble piles with different bulk diameters are explored. Our numerical simulations show that both the increase of interparticle cohesion and particle shape parameter in our model can strengthen the bodies, especially for the smaller ones. In addition, we find there exists some critical diameter at which the variation trend of with the bulk density reverses. Though a greater static friction coefficient can strengthen the body, this effect attains a minimum at a critical diameter close to . The continuum theory (analytical method) is used for…
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