Gravitational Lensing: Learn More about Einstein Rings

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SUMMARY

Gravitational lensing is a phenomenon where light from a distant quasar is bent by the gravitational field of an intervening galaxy, resulting in the formation of an Einstein ring. This effect occurs because light travels slower near massive objects, similar to how light behaves when passing through a convex glass lens. The first observation of gravitational lensing was made during a solar eclipse, allowing astronomers to see distorted constellations behind the sun. For further understanding, refer to the Wikipedia article on gravitational lensing and explore related concepts such as gravitational microlensing.

PREREQUISITES
  • Understanding of basic astrophysics concepts
  • Familiarity with the principles of light propagation
  • Knowledge of gravitational effects on light
  • Awareness of astronomical observation techniques
NEXT STEPS
  • Read the Wikipedia article on gravitational lensing
  • Explore gravitational microlensing and its applications in extrasolar planet detection
  • Investigate the historical observations of gravitational lensing during solar eclipses
  • Examine simulations of gravitational lensing effects
USEFUL FOR

Astronomy enthusiasts, astrophysicists, and students interested in the effects of gravity on light and the study of distant celestial objects.

Sourabh N
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I read that when a galaxy comes in the path of light coming from a quasar, its path bends slightly resulting in the formation of a giant luminous arc (called einstein ring). The phenomenon is called gravitational lensing. Can someone tell me something more about gravitational lensing ? Please use as simple language as possible.
 
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How 'bout an analogy? You've seen normal glass lenses, that are thicker in the middle ("convex"), and make the object behind them appear bigger. This focusing or light waves occurs because the light travels slower through glass than air. It turns out that light also travels slower near large masses (actually, because time itself flows slower), compared to far away in emptier space, so the focussing of light gravitationally (say, by a galaxy) works very similarly to a glass lens. The first observation of gravitational lensing was during a solar eclipse, since by blocking out the sunlight you can observe that whatever constellation is almost-behind the sun looks distorted (stretched).
 
You might also want to read about gravitational microlensing, which is currently being explored as a method of extrasolar planet detection.
 

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