The motion of an ideal pendulum can be explained using torque, specifically through the equation for gravitational torque, which is mgL sin θ. By applying the moment of inertia (I) and the angular acceleration (α), the relationship I α = mgL sin θ can be established, leading to the differential equation for angular motion. For small angles, sin θ approximates θ, simplifying the equation to a linear form that describes simple harmonic motion. Even for larger angles, the conservation of energy principle holds, as the only force acting on the pendulum is gravity, allowing for the conversion between gravitational potential energy and kinetic energy. Thus, torque effectively describes the dynamics of an ideal pendulum.