A stream of light from a source, which can be bent by gravitational lensing.A light beam is a directed stream of photons traveling through space. In everyday contexts, it's what comes out of a flashlight or laser. In astrophysics, light beams are crucial because they carry information about distant objects and can be manipulated by gravity. When a light beam passes near a massive object like a galaxy or black hole, its path bends—a phenomenon called gravitational lensing.
The bending of light by gravity was predicted by Albert Einstein's general relativity in 1915 and first confirmed by Arthur Eddington during the 1919 solar eclipse. The concept of gravitational lensing was further developed by Einstein and others in the 1930s.
Light travels in straight lines through flat spacetime, but massive objects curve spacetime around them. A light beam follows the curved geometry, so its path appears bent to an outside observer. This bending can focus or distort the beam, creating multiple images, arcs, or Einstein rings of background sources. The effect is stronger with more massive objects and closer passage.
Gravitational lensing is used to map dark matter distributions, measure galaxy masses, and detect distant exoplanets through microlensing surveys.
The Sun itself acts as a gravitational lens, focusing light from distant stars at a focal point about 550 astronomical units away—a region proposed for a future space telescope.



