Black holes form when very massive stars—typically those more than 20–25 times the mass of our Sun—reach the end of their life cycle. After burning all their nuclear fuel, the star can no longer support its own weight. Its core collapses under its own gravity, triggering a massive explosion called a supernova. What remains is an extremely dense point called a singularity, surrounded by the event horizon, beyond which nothing can escape.
The gravity of a black hole is so strong because a huge amount of mass is compressed into a tiny space. This extreme density bends space-time, creating a gravitational pull powerful enough to trap even light. The closer matter gets to the singularity, the stronger the gravitational effects become.