Black holes: formation, theory, and evidence

Gravity trapping light: black hole definition

A black hole is an extremely compact astronomical object whose gravity is so strong that it prevents anything—including light—from escaping. In general relativity, this happens for any sufficiently compact mass, and the boundary beyond which escape is impossible is called the event horizon. Once an object crosses the event horizon, it becomes trapped inside; locally there may be no detectable change at the crossing, though the object’s future is constrained by the spacetime geometry. General relativity also predicts that black holes contain a central singularity, where spacetime curvature becomes infinite (ignoring quantum effects). The event horizon is defined as a one-way causal boundary: events inside cannot affect outside observers, so the horizon cannot be located using local measurements alone. While black holes are often described as regions of spacetime from which no information-carrying signals can escape, practical identification relies on observational signatures such as gravitational effects on nearby matter and radiation, including accretion disks, gravitational lensing, and—when mergers occur—gravitational waves.

0/2 modes complete

Event horizon as the no-escape boundary

0/2 modes complete