In general relativity, a naked singularity is a gravitational singularity without an event horizon. In a black hole, the singularity is completely enclosed by a boundary known as the event horizon, inside which the gravitational force of the singularity is so strong that light cannot escape. Hence, objects inside the event horizon including the singularity itself cannot be directly observed. A naked singularity, by contrast, is observable from the outside.

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AERT - Infinitely Dense Point Mass

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