Relative angular velocity is defined as the rate of change of angle (dθ/dt) of one object in relation to another, typically measured in a polar coordinate system. To understand this concept better, one can convert angular speed to linear speed, where the relative speed between two objects can be expressed as the difference in their velocities. The discussion uses the example of Earth and a Kuiper Belt Object (KBO) to illustrate how relative speeds can be calculated. An analogy with clock hands is provided to clarify how relative motion works, emphasizing that the apparent motion of one object can differ from its actual motion due to the influence of another object's movement. Understanding these principles is crucial for solving problems related to relative angular velocity.