Gravitational Lensing Images
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This effect is known as gravitational microlensing.
A gravitational lens is a distribution of matter such as a cluster of galaxies between a distant light source and an observer that is capable of bending the light from the source as the light travels towards the observerthis effect is known as gravitational lensing and the amount of bending is one of the predictions of albert einsteins general theory of relativity.
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Gravitational lensing images. In general relativity the presence of matter energy density can curve spacetime and the path of a light ray will be deflected as a result. The simplest type of gravitational lensing occurs when there is a single concentration of matter at the center such as the dense core of a galaxy. This bending can produce multiple images of the same source. Glass lenses in optics.
Gravitational lensing x rays and other forms of light from distant objects such as this galaxy can be bent by the gravitational field of an intervening galaxy. The light of a distant galaxy is redirected around this core often producing multiple images of the background galaxy. Gravitational lensing is the natural phenomenon by which we see the magnified and multiple images of the distant objects galaxies stars quasar etc when the light emitted by these objects passes through the gravity of massive objects these massive objects distort the spacetime eg. The multiple image effect is produced by a process called gravitational lensing in which the gravitational field of a massive object bends and amplifies light from an object farther behind it.
Nasas hubble space telescope captured the first ever picture of a group of five star like images of a single distant quasar. Astronomers use those shapes to determine the distribution of mass in the galaxy clusters doing the lensing or to figure out their distribution of dark matter. In many of its views distant galaxies are smeared into arcs.