Naked singularities present a theoretical challenge in general relativity (GR), as they defy conventional understanding of event horizons and gravity. Unlike Newtonian gravity, GR's complexity means that gravitational effects cannot be simply defined by mass and distance. Event horizons are nonlocal constructs that require knowledge of the universe's entire future, complicating their measurement. While explicit solutions for naked singularities exist, they are not expected to occur in reality, and their study suggests a need for a unified theory incorporating quantum mechanics. Ultimately, naked singularities highlight the limitations of GR and the necessity for further theoretical development.