The light from Mercury, the Sun's corona and gravity

In summary, The position of Mercury during a solar eclipse in 1919 confirmed the ideas of General Relativity, as measured by Eddington. The effect of the Sun's corona was considered, but it was found to be negligible. Later, improved measurements using radio interferometry and VLBI have further confirmed the deflection of light by gravity predicted by General Relativity.
  • #1
Wondermine
The question is:
The General Relativity Ideas were confirmed by the position of Mercury by Eddington. How could they be certain that the light deviation was due to gravity rather than the lens effect the Sun's corona may have had?
What process was used,if any,to remove the effect of the corona on the light from Mercury?
The corona is an high energy particle "fog" which would lens light like a crystal. How to remove this in order to be certain gravity bent the light?
 
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  • #2
You're conflating two different tests of General Relativity. What Eddington measured was the deviation of the position of stars due to the deflection of the starlight by the sun's gravity. He measured the positions of these stars during a total solar eclipse and again after the sun had moved away. The precession of the perihelion of Mercury was known since the 1800's to be more than Newton's theory predicted. Eddington was not part of this.

Your question still holds, however. I think the deflection due to the lensing effect of the corona is negligible, but I have no references to back this up. The density of the corona is known, so this deflection could be calculated.
 
  • #3
This paper by Will reviews the history of measurements of light bending by the Sun:

https://arxiv.org/pdf/1409.7812.pdf

He notes on p. 10 that recent measurements have taken readings in multiple frequency bands, to correct for the effects of the Sun's corona (which is expected to deflect radiation of different frequencies by different amounts, whereas the GR effect is the same for all frequencies).
 
  • #4
Wondermine said:
How could they be certain that the light deviation was due to gravity rather than the lens effect the Sun's corona may have had?

That 1919 eclipse observation is certainly of historical significance. But it may interest you to know that since that time we have observations that are a lot more definitive.
See, for example, this article by Clifford M. Will: http://link.springer.com/article/10.12942/lrr-2014-4#Sec4. Here is a relevant passage:

[...]the development of radio interferometery, and later of very-long-baseline radio interferometry (VLBI), produced greatly improved determinations of the deflection of light.
 

1. How does the light from Mercury differ from the light from the Sun's corona?

The light from Mercury is primarily reflected sunlight, while the light from the Sun's corona is a result of the Sun's extreme heat and magnetic field causing ionized particles to emit light.

2. Why does the Sun's corona appear brighter during a solar eclipse?

The Sun's corona is actually much brighter than the photosphere (visible surface) of the Sun, but it is usually overpowered by the brightness of the Sun's surface. During a solar eclipse, the Moon blocks out the photosphere, allowing the corona to be seen more clearly.

3. How does gravity play a role in the movement of Mercury?

Gravity is the force that keeps the planets in orbit around the Sun. The strong gravitational pull of the Sun causes Mercury to orbit around it, while the gravitational pull of other planets and objects in the solar system can slightly alter its orbit.

4. Can the light from Mercury and the Sun's corona be harmful to humans?

The light from Mercury and the Sun's corona is not harmful to humans in small amounts. However, prolonged exposure to the intense light and radiation from the Sun's corona can be dangerous and cause damage to the eyes and skin.

5. How does studying the light from Mercury and the Sun's corona help us understand the universe?

Studying the light from Mercury and the Sun's corona can provide valuable information about the composition and behavior of these celestial bodies. It can also help us understand the effects of gravity and magnetic fields on the movement of objects in space, and expand our knowledge of the universe as a whole.

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