Stick-slip dynamics in penetration experiments on simulated regolith

TL;DR

This study investigates the stick-slip dynamics of probe insertion into simulated planetary regolith across different gravity levels, revealing that microgravity suppresses stick-slip behavior and that probe speed influences these dynamics.

Contribution

It provides new insights into regolith behavior under varying gravity conditions, highlighting the limitations of scaling terrestrial experiments to microgravity environments.

Findings

Stick-slip events increase with gravity level.

Microgravity environments show negligible stick-slip behavior.

Faster probe insertion suppresses stick-slip in low gravity.

Abstract

The surfaces of many planetary bodies, including asteroids and small moons, are covered with dust to pebble-sized regolith held weakly to the surface by gravity and contact forces. Understanding the reaction of regolith to an external perturbation will allow for instruments, including sensors and anchoring mechanisms for use on such surfaces, to implement optimized design principles. We analyze the behavior of a flexible probe inserted into loose regolith simulant as a function of probe speed and ambient gravitational acceleration to explore the relevant dynamics. The EMPANADA experiment (Ejecta-Minimizing Protocols for Applications Needing Anchoring or Digging on Asteroids) flew on several parabolic flights. It employs a classic granular physics technique, photoelasticity, to quantify the dynamics of a flexible probe during its insertion into a system of bi-disperse, cm-sized model grains. We identify the force-chain structure throughout the system during probe insertion at a variety of speeds and for four different levels of gravity: terrestrial, martian, lunar, and microgravity. We identify discrete, stick-slip failure events that increase in frequency as a function of the gravitational acceleration. In microgravity environments, stick-slip behaviors are negligible, and we find that faster probe insertion can suppress stick-slip behaviors where they are present. We conclude that the mechanical response of regolith on rubble pile asteroids is likely quite distinct from that found on larger planetary objects, and scaling terrestrial experiments to microgravity conditions may not capture the full physical dynamics.