The phenomenon of light bending around black holes, also known as gravitational lensing, is a result of the intense gravitational pull of a black hole. This pull causes light rays to bend as they pass near the black hole, creating distorted and magnified images of objects behind it.
Light bending around black holes allows us to see objects that would otherwise be hidden behind the black hole. It also allows us to study the effects of gravity on light, providing valuable insights into the nature of space and time.
Light bending around black holes is a real phenomenon that has been observed and studied by scientists. The first evidence of this phenomenon was observed in 1919 during a solar eclipse, when the position of stars near the sun appeared to shift due to its gravitational pull.
Light bends around black holes because of the immense gravitational pull they exert. According to Einstein's theory of general relativity, massive objects like black holes cause a distortion in the fabric of space-time, which in turn affects the path of light.
The amount of light bending around a black hole is directly proportional to its mass. The larger the black hole, the stronger its gravitational pull and therefore the greater the amount of light bending. This is why supermassive black holes in the centers of galaxies have a significant effect on the light passing through them.