Crater-ray formation through mutual collisions of hypervelocity-impact induced ejecta particles
Toshihiko Kadono, Ayako I. Suzuki, Rintaro Matsumura, Junta Naka, Ryo, Suetsugu, Kosuke Kurosawa, Sunao Hasegawa

TL;DR
This study examines crater-ray patterns formed by hypervelocity impacts, revealing that the pattern angle is independent of impact velocity, particle size, and shape, and is governed by particle collision dynamics.
Contribution
It introduces a new analysis linking pattern angles to particle collision velocities and confirms this relation through experiments and simulations, extending understanding of crater-ray formation.
Findings
Pattern angle is consistent across impact velocities.
Pattern structure is unaffected by particle size and shape.
Pattern formation is governed by collision dynamics, not elastic properties.
Abstract
We investigate the patterns observed in ejecta curtain induced by hypervelocity impact (2-6 km/s) with a variety of the size and shape of target particles. We characterize the patterns by an angle, defined as the ratio of the characteristic length of the pattern obtained by Fourier transformation to the distance from the impact point. This angle is found to be almost the same as that obtained by the reanalysis of the patterns in the previous study at lower impact velocities (Kadono et al., 2015, Icarus 250, 215-221), which are consistent with lunar crater-ray systems. Assuming that the pattern is formed by mutual collision of particles with fluctuation velocity in excavation flow, we evaluate an angle at which the pattern growth stops and show that this angle is the same in the order of magnitude as the ratio of the fluctuation velocity and the radial velocity. This relation is…
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