  Craters formed by the impact of agglomerated materials are commonly observed
in nature, such as asteroids colliding with planets and moons. In this paper,
we investigate how the projectile spin and cohesion lead to different crater
shapes. For that, we carried out DEM (discrete element method) computations of
spinning granular projectiles impacting onto cohesionless grains, for different
bonding stresses, initial spins and initial heights. We found that, as the
bonding stresses decrease and the initial spin increases, the projectile's
grains spread farther from the collision point, and, in consequence, the crater
shape becomes flatter, with peaks around the rim and in the center of craters.
Our results shed light on the dispersion of the projectile's material and the
different shapes of craters found on Earth and other planetary environments.
