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      Sand Creep Motion in Slow Spin-up Experiment: An Analogue of Regolith Migration on Asteroids

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          Abstract

          We studied the creep motion of granular materials in a gradient potential field that is created using a slow spin-up experiment device. Natural sand confined in the acrylic box is spun up by a controlled turntable and the surface flows are captured using video-based measurements. Various spin-up accelerations were considered to understand the responses of creep motion on different accelerating paths. Convergent behaviors in the morphological change of sand surface were observed in the final steady state. To quantify the quasi-static spin-up process, we examined the net flux and the surface slope as a function of the spin rate and offset from the rotation axis. Evolution of sand creep motion demonstrated behaviors similar to regolith migration in numeric simulations, showing intermittency like general sheared granular systems. We noticed the sand surface approaches criticality as the spin-up proceeding, consistent with the observation that top-shaped asteroids near limiting spin rate take on critical shape. Comparisons to large-scale numeric simulations and analytical solutions reveal underlying similarities between our experiments and the million-year evolution of asteroid regolith under YORP acceleration, which raises the possibility of studying asteroid surface processes in laboratory analogue experiments.

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          Author and article information

          Journal
          19 May 2021
          Article
          2105.09498
          fc8d3bd6-97d1-49ed-bd4e-ff53039b6537

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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          astro-ph.EP

          Planetary astrophysics
          Planetary astrophysics

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