When two black holes collide, they typically enter a tight hyperbolic orbit before potentially merging, especially if influenced by a third body. If they pass closely, significant gravitational energy can be radiated, leading to eventual fusion into a larger rotating black hole. In some cases, if they move directly towards each other without angular momentum, they may collide and merge instantly. The primary radiation observed during these events is gravitational energy, with Hawking radiation also present. The detection of gravitational waves from such collisions, particularly the rising frequency chirp before merging, is a key focus in current astrophysical research.