In rotational motion, when a mass attached to a rope falls a distance x meters, the string must also move through x meters around the rim or disk. This relationship can be expressed mathematically as s = rθ, where s is the linear displacement, r is the radius, and θ is the angular displacement in radians. The discussion emphasizes that the linear distance fallen by the mass directly correlates to the angular distance traveled by the rim or disk. This connection highlights the conservation of distance in the system. Understanding this relationship is crucial for analyzing rotational dynamics effectively.