A black hole is an area of spacetime where gravity is so powerful that nothing can escape it, including particles and electromagnetic waves like light. A sufficiently compact mass may bend spacetime to generate a black hole, according to general relativity theory. The event horizon is the point at which there is no way out. Although it has a huge impact on the fate and circumstances of an item passing through it, it has no locally discernible properties, according to general relativity. A black hole is similar to an ideal black body in that it does not reflect light. Furthermore, in curved spacetime, quantum field theory predicts that event horizons emit Hawking radiation, which has the same spectrum as a black body with a temperature that is inversely proportional to its mass. For black holes of stellar mass, this temperature is on the order of billionths of a kelvin, making direct observation very impossible. A galaxy passes behind a Schwarzschild black hole on a plane pe...