Particles in spacetime follow paths of longest proper time due to the action principle, which dictates that the extremal action corresponds to these trajectories. In flat spacetime, the proper time is maximized when a particle is not subject to external forces, leading to straight-line geodesics. Light, which travels along paths with zero proper time, represents a unique case as it is the only path available, making it both the longest and shortest in a trivial sense. The discussion highlights that while massive and massless particles can follow geodesics, they do not meet in future events, indicating different paths. Understanding this relationship between proper time and geodesics is crucial for grasping the principles of special and general relativity.