Centroid migration on an impacted granular slope due to asymmetric ejecta deposition and landsliding

preprint2020arXivOpen access

Abstract

For a fundamental understanding of terrain relaxation occurring on sloped surfaces of terrestrial bodies, we analyze the crater shape produced by an impact on an inclined granular (dry-sand) layer. Owing to asymmetric ejecta deposition followed by landsliding, the slope of the impacted inclined surface can be relaxed. Using the experimental results of a solid projectile impact on an inclined dry-sand layer, we measure the distance of centroid migration induced by asymmetric cratering. We find that the centroid migration distance xmigx_\mathrm{mig} normalized to the crater minor-axis diameter DcyD_\mathrm{cy} can be expressed as a function of the initial inclination of the target tan⁡θ\tanθ, the effective friction coefficient μμ, and two parameters KK and cc that characterize the asymmetric ejecta deposition and oblique impact effect: xmig/Dcy=Ktan⁡θ/(1−(tan⁡θ/μ)2)+cx_\mathrm{mig}/D_\mathrm{cy}=K \tanθ/(1-(\tanθ/μ)^2)+c, where K=0.6K=0.6, μ=0.8μ=0.8, and c=−0.1c=-0.1 to 0.30.3. This result is consistent with a previous study that considered the effect of asymmetric ejecta deposition. The obtained results provide fundamental information for analyzing the degradation of sloped terrain on planetary surfaces, such as crater-shape degradation due to the accumulation of micro-impacts.

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