An effect in which light rays are bent by the gravitational field of a massive object, such as a galaxy or black hole. The Sun produces a slight gravitational lens effect (see gravitational deflection), but on cosmological scales the effect is seen as the formation of double or multiple images of a distant galaxy or quasar by a foreground object (as in, for example, the Einstein Cross). More complicated lensing effects also occur, including the formation of Einstein rings, luminous arcs, and microlensing. Gravitational lensing is divided into strong lensing, which creates obvious arcs and rings, and weak lensing, which only subtly distorts the shapes of background objects.
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