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 quasistatic 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. The creep motion of sand demonstrated behaviors similar to the regolith migration in numeric simulations. We have 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 shapes. Comparisons to large-scale numeric simulations and analytical solutions reveal underlying similarities between the experiments and the million-year evolution of asteroid regolith under Yarkovsky-O'Keefe-Radzievskii-Paddack acceleration, which raises the possibility of studying asteroid surface processes in laboratory analog experiments.

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• Granular flows
• Self-organized criticality
• Asteroids, meteors, & meteorites