Science & Physics
A black hole is a region in space where gravity is so intense that nothing, not even light, can escape its pull once it crosses a boundary called the event horizon.
Imagine you're throwing a ball upward. On Earth, you throw it hard enough and it escapes Earth's gravity. But if Earth were compressed into a tiny space, its gravity would become so strong that even light—the fastest thing in the universe—couldn't escape. That's essentially what a black hole is: a point in space where matter has been compressed so densely that the escape velocity exceeds the speed of light.
Black holes typically form when massive stars (at least 20-25 times the mass of our Sun) exhaust their nuclear fuel. Without the outward pressure from nuclear fusion to balance the inward pull of gravity, the star collapses under its own weight. This collapse creates a singularity—a point of infinite density—surrounded by an event horizon.
Black holes are laboratories for testing the limits of physics. They help us understand gravity, spacetime, and how matter behaves under extreme conditions. The first image of a black hole's event horizon was captured in 2019 by the Event Horizon Telescope, confirming Einstein's theory of general relativity.
They also play crucial roles in galaxy formation and evolution, and studying them helps us understand the universe's structure and history.