Gravitational Lensing: Light Bent by Massive Objects

  1. Gravitational lensing occurs when massive objects like galaxies bend the path of light.
  2. Einstein’s theory of general relativity predicted this cosmic light-bending.
  3. Massive objects warp spacetime, curving the routes that light must follow.
  4. Lensing can magnify distant galaxies, acting like a natural cosmic telescope.
  5. Strong lensing creates multiple images, arcs, or even “Einstein rings” of background objects.
  6. Weak lensing subtly distorts galaxy shapes, helping map invisible dark matter.
  7. Microlensing happens when stars or planets briefly brighten as they pass in front of another star.
  8. The first gravitational lens was confirmed in 1979 with twin images of a distant quasar.
  9. Astronomers use lensing to study galaxies too faint or far to see directly.
  10. Gravitational lensing provides one of the best tools for probing dark energy and the structure of the universe.