Regolith behavior under asteroid-level gravity conditions: Low-velocity impacts into mm- and cm-sized grain targets

TL;DR

This study experimentally investigates how coarse regolith grains respond to very-low-speed impacts under microgravity, revealing impact dynamics, ejecta behavior, and scaling laws relevant for asteroid surface processes and spacecraft interactions.

Contribution

It provides new experimental data on low-velocity impacts into mm- and cm-sized grains under microgravity, enhancing understanding of asteroid surface mechanics and impact outcomes.

Findings

Ejecta produced at impact speeds above 12 cm/s

Ejecta speed scales with impact speed and grain size ratio

Coefficient of restitution is independent of grain size

Abstract

In situ observations of small asteroids show that surfaces covered by boulders and coarse terrain are frequent on such bodies. Regolith grain sizes have distributions on approximately mm and cm scales, and the behavior of such large grains in the very low-gravity environments of small body surfaces dictates their morphology and evolution. In order to support the understanding of natural processes (e.g., the recapturing of impact ejecta) or spacecraft-induced interactions (e.g., the fate of a small lander), we aim to experimentally investigate the response of coarse-grained target surfaces to very-low-speed impacts (below 2 m/s). We present the outcome of 86 low-speed impacts of a cm-sized spherical projectile into a bed of simulated regolith, composed of irregular mm- and cm-sized grains. These impacts were performed under vacuum and microgravity conditions. Our results include measurements for the projectile coefficient of restitution and penetration depth, as well as ejecta production, speed, and mass estimation. We find that impact outcomes include the frequent occurrence of projectile bouncing and tangential rolling on the target surface upon impact. Ejecta is produced for impact speeds higher than about 12 cm/s, and ejecta speeds scale with the projectile to target the grain size ratio and the impact speed. Ejected mass estimations indicate that ejecta is increasingly difficult to produce for increasing grain sizes. Coefficients of restitution of rebounding projectiles do not display a dependency on the target grain size, unlike their maximum penetration depth, which can be scaled with the projectile to target grain size ratio. Finally, we compare our experimental measurements to spacecraft data and numerical work on Hayabusa 2's MASCOT landing on the surface of the asteroid Ryugu.