Gravitational Lensing: Learn More about Einstein Rings

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Discussion Overview

The discussion centers around gravitational lensing, specifically the phenomenon of Einstein rings formed when a galaxy obstructs light from a quasar. Participants explore the concept, its implications, and related topics such as gravitational microlensing.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • One participant describes gravitational lensing as the bending of light due to the gravitational influence of a galaxy, resulting in luminous arcs known as Einstein rings.
  • Another participant provides an analogy comparing gravitational lensing to the focusing effect of convex glass lenses, noting that light behaves similarly near massive objects.
  • A suggestion is made to read an article on gravitational lensing from Wikipedia, which includes a simulation of the effect.
  • Another participant mentions gravitational microlensing and its potential use in detecting extrasolar planets.

Areas of Agreement / Disagreement

The discussion includes various perspectives on gravitational lensing and related concepts, but no consensus is reached on specific details or implications.

Contextual Notes

Some participants express a desire for simpler explanations, indicating a potential gap in understanding complex aspects of gravitational lensing.

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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