Wark-Lovering rims refer to a type of geological feature commonly found in impact craters on the surface of planets and moons. These rims are characterized by a distinct pattern of ridges and troughs that extend outward from the crater rim. They are thought to be formed as a result of the intense heat and pressure generated by the impact event, which causes the rocks at the rim of the crater to deform and flow outward, creating the distinctive pattern seen in wark-lovering rims. Studying these features can provide valuable insights into the processes and conditions present during impact events, as well as the geological history of the planetary bodies where they are found.