A systematic investigation of the gravity dependence of static and dynamic angles of repose from 0.01g to 1g
This study utilizes controlled avalanche experiments on the China Space Station to demonstrate that while the static angle of repose remains constant across gravity levels from 0.01g to 1g, the dynamic angle of repose increases with gravity up to approximately 0.16g before saturating, a behavior attributed to a gravity-dependent rolling friction coefficient that significantly improves models of regolith on small Solar System bodies.