Gravity vs Diffraction in Troposphere of a Star

In summary, the dominant effect causing light to bend near the surface of a star can be determined by comparing the calculated gravitational deflection with the actual measured deflection at a known distance from the star. If the measured deflection is considerably larger, then refraction is the dominant effect. However, calculating the refractive part would require detailed knowledge of the atmosphere's density and composition.
  • #1
Buckeye
165
2
How can we decide which process is causing light to bend near the surface of a star? Gravity is said to cause light to bend or deflect as it passes near the huge mass of a star. But matter in the troposphere of a star should also cause light to bend or deflect as it passes through the troposphere of the star because there should be a lot of matter (electrons, protons, H and He) in the troposphere of a star. How do I decide which is the dominant effect?
 
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  • #2
I am new to relativity and you should consider some expert opinion than mine, but as this question is more of optics, let me take a chance. I will only say about the refraction point of view.

As refraction depends upon the refractive index of the material (which depends upon wavelength), light with different wavelengths (all from same distant star) should refract to different extents. Thus, If considerable refraction is taking place at all, the distant star should be seen as images of the star in many different colors. Just like prism separates visible light. Plus, the refractive index back calculated comes out to be near 2, which is not plausible for any gaseous mixture. (There is a paper on arxive regarding this and some refraction point of view for black holes).

Again, don't depend upon my point of view.
 
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  • #3
Correct, refraction depends on the wavelength of the light (this is called dispersion), whereas gravitational bending doesn't. Also, gravitational bending of radio waves by the sun, from pulsars or some such thing, has been studied at large angles from the sun (as seen from the earth) where the sun's atmosphere would not be involved at all.
 
  • #4
Buckeye said:
How can we decide which process is causing light to bend near the surface of a star? Gravity is said to cause light to bend or deflect as it passes near the huge mass of a star. But matter in the troposphere of a star should also cause light to bend or deflect as it passes through the troposphere of the star because there should be a lot of matter (electrons, protons, H and He) in the troposphere of a star. How do I decide which is the dominant effect?

It can be done if you have the mass of the star, and a measurement of the deflection at some known distance from the star.

Calculate the gravitational deflection for the known mass and distance, and compare it to the actual measured deflection. If they're nearly equal, then gravity is the dominant effect. If the measurement is considerably larger than the calculation, then refraction dominates.

p.s. While a calculation of the refractive part is possible in principle, it would require detailed knowledge of the atmosphere's density and composition as a function of altitude above the surface.
 
  • #5
jtbell said:
...(as seen from the earth) where the sun's atmosphere would not be involved at all.
Sun's atmosphere extends to Earth and even beyond (Encyclopedia Britannica: "Corona"), not that it makes any difference though, as It won't achieve the necessary refractive index!
 

1. What is the difference between gravity and diffraction in the troposphere of a star?

Gravity and diffraction are two different phenomena that can occur in the troposphere of a star. Gravity is a force that pulls objects towards each other, while diffraction is the bending of light as it passes through different mediums. In the case of a star, gravity is the dominant force that holds the star together, while diffraction can occur when light passes through the star's atmosphere.

2. How does gravity affect the troposphere of a star?

Gravity plays a crucial role in the troposphere of a star. It is responsible for the star's formation, as well as maintaining its structure and stability. Gravity also determines the temperature and pressure within the star's atmosphere, which can have a significant impact on the star's overall behavior.

3. Can diffraction occur in the troposphere of a star?

Yes, diffraction can occur in the troposphere of a star. As light passes through the star's atmosphere, it can be bent or scattered due to differences in temperature, pressure, and composition. This can result in various phenomena such as twinkling, mirages, and color changes in the star's appearance.

4. How do scientists study the effects of gravity and diffraction in the troposphere of a star?

Scientists use a variety of techniques to study the troposphere of a star, including telescopes, spectroscopy, and computer simulations. By observing the star's behavior and analyzing the spectral lines of light emitted by the star, scientists can gather valuable information about the role of gravity and diffraction in the star's atmosphere.

5. Can gravity and diffraction be used to determine the properties of a star?

Yes, gravity and diffraction can provide valuable insights into the properties of a star. By studying the star's behavior and analyzing the effects of gravity and diffraction, scientists can determine the star's mass, temperature, composition, and other important characteristics. This information is crucial for understanding the life cycle of stars and their role in the universe.

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