Black holes are dense spacetime entities formed from the remnants of collapsed stars, accumulation of matter, or possibly from the Big Bang. They interact gravitationally and quantum mechanically, revealing their presence by affecting nearby objects. The singularity at the core of a black hole is a point where matter is compressed to an infinite density, while the event horizon represents the boundary beyond which nothing can escape. The size of a black hole is typically described by the extent of its event horizon, which can vary significantly from a few kilometers for collapsed stars to the size of solar systems for supermassive black holes. Evidence suggests that black holes exist in every galaxy, with notable examples like Cygnus X-1.