Testing whether gravity bends light

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    Gravity Light Testing
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SUMMARY

The discussion centers on Einstein's theory of gravity bending light, specifically the method of observing this phenomenon during a solar eclipse. By comparing the apparent positions of stars near the Sun to their normal positions, astronomers can determine the bending of light caused by the Sun's gravitational field. This method relies on the fact that light from stars appears shifted when it passes close to the Sun, allowing for a visual confirmation of Einstein's predictions. The experiment effectively demonstrates the relationship between gravity and light, validating key aspects of general relativity.

PREREQUISITES
  • Understanding of Einstein's General Relativity
  • Familiarity with solar eclipses and their observational significance
  • Knowledge of light propagation and its interaction with gravitational fields
  • Basic principles of astronomical observation techniques
NEXT STEPS
  • Research the historical context of the 1919 solar eclipse experiment
  • Study the mathematical framework of General Relativity
  • Explore modern techniques for measuring gravitational lensing
  • Investigate the implications of light bending on astrophysics and cosmology
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Astronomers, physicists, students of general relativity, and anyone interested in the intersection of gravity and light in astrophysical phenomena.

Drops of Fire
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The experiment Einstein proposed that supposedly proved successful kind of confuses me. If you can prove a beam of light bends when near the sun, how can we prove that from Earth with a picture because by the time we're able to see it to take a picture, the light has already gone passed the sun and reached Earth and any effect it would've had on it would be gone by then. At that point, all the light would appear to be bent everywhere about the about the same despite whether or not some of it passed the sun to get here, right?
 
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The trick is that as the light passes the Sun and bends it leaves the Sun's vicinity along a different line than what it came from. when that light reaches us, we see the object that produced the light in a different position than we would have if the Sun had not bent it's path. By comparing the apparent positions of stars next to the Sun during an eclipse as compared to their normal relative positions, we can tell if they seem to shift position when their light skims the Sun on the way to us.

Here's an image that illustrates this:

http://astrobob.areavoices.com/astrobob/images/1919_light_bending_Jose_Wudka_1.jpg
 
In a nutshell, the idea was to observe the (apparent) distance between two stars when the light from each passed close to the sun and when it didn't.
 

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