Decades passed before astronomical technology verified that idea: It wasn't until 1979 that astronomers detected a real - life
example of a gravitational lens in the double image of a quasar — side - by - side glimpses of a galaxy's blazing heart, resembling a pair of oncoming headlights.
Jackson and colleagues used the Karl G. Jansky Very Large Array, in New Mexico, US, to study four
examples of gravitational lens systems where the background quasar appears in a ring of four, distorted images.
Not exact matches
Since the discovery
of the first
gravitational lens in 1979, astronomers have in fact seen innumerable
examples.
For
example, the powerful
gravitational field
of a massive cluster
of galaxies can bend the light rays from more distant galaxies, just as a camera
lens bends light to form a picture.
The basic steps
of a visual search for
gravitational lenses are: (1) prepare the images, (2) display them to an inspector, (3) record the inspector's classification
of each image (as, for
example, containing a
lens candidate or not) and (4) analyse that classification along with all others to produce a final candidate list.