I. Introduction
Climbing robots can advance scientific exploration of our solar system by enabling access to exposed strata found on steep terrain that conventional wheeled rovers cannot reach, such as the cliff faces observed in Jezero and Victoria Craters on Mars, or lava tubes with vent openings on the Martian and lunar surfaces [1]–[4]. Robust, reliable adhesion to vertical or even overhanging surfaces can be achieved through the use of microspines, which use small, sharp hooks to take advantage of millimeter to sub-millimeter scale surface features. Unlike other adhesion mechanisms such as suction, magnetism, or dry adhesion, microspines are well-suited to the rough rock and cliff surfaces commonly encountered during planetary exploration [5]–[7].