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A black hole is a region in space where the gravitational force is so strong that nothing, not even light, can escape its pull. It is formed when a massive star collapses in on itself, creating a singularity with infinite density and zero volume. Because of its strong gravitational field, a black hole can distort the fabric of space and time, creating a phenomenon known as "spacetime curvature." Black holes are typically classified based on their mass: stellar black holes, intermediate black holes, and supermassive black holes. Stellar black holes are the most common, with a mass ranging from a few to tens of times that of the sun. Intermediate black holes are thought to exist, but their existence is not yet confirmed. Supermassive black holes, on the other hand, have a mass billions of times that of the sun and are thought to exist at the centers of most galaxies, including our Milky Way.
