Modeling Early Clustering of Impact-induced Ejecta Particles Based on Laboratory and Numerical Experiments
Kanon Nakazawa, Satoshi Okuzumi, Kosuke Kurosawa, Sunao Hasegawa

TL;DR
This study combines laboratory experiments, numerical simulations, and analytical modeling to understand the early formation of impact ejecta patterns, revealing a rapid, two-stage process driven by inelastic collisions and geometric expansion.
Contribution
It provides new experimental, simulation, and analytical insights into the rapid formation of impact ejecta patterns, emphasizing the role of initial collisions and expansion in pattern development.
Findings
Pattern formation completes within ~10 microseconds.
Pattern growth driven by initial inelastic collisions and geometric expansion.
Analytical model reproduces cluster sizes and confirms rapid pattern development.
Abstract
A projectile impact onto a granular target produces an ejecta curtain with the heterogeneous material distribution. Understanding how the heterogeneous pattern forms is potentially important for understanding how crater rays form. Previous studies predicted that the pattern formation is induced by inelastic collisions of ejecta particles in the early stages of crater formation and is terminated by the ejecta's expanding motion. In this study, we test this prediction based on a hyper-velocity impact experiment together with N-body simulations where the trajectories of inelastically colliding granular particles are calculated. Our laboratory experiment suggests that pattern formation is already completed on a timescale comparable to the geometrical expansion of the ejecta curtain, which is ~ 10 microseconds in our experiment. Our simulations confirm the previous prediction that the…
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Taxonomy
TopicsPlanetary Science and Exploration · Astro and Planetary Science · Particle Dynamics in Fluid Flows
