Angular Velocity of a source of light

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SUMMARY

The discussion centers on the hypothetical scenario of light having a non-constant speed, particularly in the context of a binary star system. Participants analyze the angular velocity (ω) of a smaller star orbiting a larger star, specifically how it affects the timing of light reaching Earth. The key equation derived is ω=v/r, where the values of ω are expressed in terms of the speed of light (c), radius (r), and distance (L) from Earth. The calculations involve equating the time taken for light emitted when the star is moving away from Earth to the time taken when it is moving toward Earth, leading to three potential formulas for ω.

PREREQUISITES
  • Understanding of angular velocity in orbital mechanics
  • Familiarity with the speed of light and its implications in physics
  • Basic knowledge of relativity and the Michelson-Morley experiment
  • Ability to manipulate algebraic equations involving distance, velocity, and time
NEXT STEPS
  • Explore the implications of non-constant speed of light in theoretical physics
  • Study the Michelson-Morley experiment and its significance in proving the constancy of light speed
  • Investigate the mathematical derivation of angular velocity in binary star systems
  • Learn about Galilean relativity and its differences from Einstein's theory of relativity
USEFUL FOR

Astronomers, physicists, and students of theoretical physics who are interested in the properties of light, orbital mechanics, and the implications of relativity in astrophysical contexts.

Felipe Doria
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This is not schoolwork.
Imagine that light did not have a constant speed, but behaved in the manner expected from experience. Namely, if the source of the light is rushing toward you, the light will approach you faster; if the source is rushing away from you, the light will approach you slower. This is incorrect, of course, but it's worth investigating the consequences of a non-constant speed of light because the failure to observe those consequences is evidence that the speed of light is constant. With that backdrop, consider a binary star system situated a very large distance L from Earth. Let the angular velocity of the smaller star be ω, as it orbits the larger star in a circle of radius r.
What value of ω=v/r will result in the light emitted when the smaller star is traveling directly away from Earth reaching us at the same moment as the light emitted later, when the smaller star's orbit has it moving directly toward earth? (choose one)
a) ω=(c/r)*sqrt((πr)/(2L+2πr))
b) ω=(c/r)*((πr)/(2L+πr))
c) ω=(c/r)*sqrt((πr)/(2L+πr))

I think that the time it takes for the light emitted from the smaller star when it is traveling directly away from Earth has to be equal to the time it takes for the light emitted later plus the time it takes to complete half an orbit. So:
t1 = t2 + t3
L/(c-v) = L/(c+v) + pi*r/v

How can I get the answer from this? Thank you for your help.
 
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Felipe Doria said:
This is not schoolwork.
Imagine that light did not have a constant speed, but behaved in the manner expected from experience.
"from experience" the speed of light in invariant - but I get what you mean:

Namely, if the source of the light is rushing toward you, the light will approach you faster; if the source is rushing away from you, the light will approach you slower.
... you mean, what if light obeyed Galilean relativity.

This is incorrect, of course, but it's worth investigating the consequences of a non-constant speed of light because the failure to observe those consequences is evidence that the speed of light is constant.
See "Michealson-Morely experiment" for an example of this sort of calculation.

With that backdrop, consider a binary star system situated a very large distance L from Earth. Let the angular velocity of the smaller star be ω, as it orbits the larger star in a circle of radius r.
What value of ω=v/r will result in the light emitted when the smaller star is traveling directly away from Earth reaching us at the same moment as the light emitted later, when the smaller star's orbit has it moving directly toward earth? (choose one)
a) ω=(c/r)*sqrt((πr)/(2L+2πr))
b) ω=(c/r)*((πr)/(2L+πr))
c) ω=(c/r)*sqrt((πr)/(2L+πr))

I think that the time it takes for the light emitted from the smaller star when it is traveling directly away from Earth has to be equal to the time it takes for the light emitted later plus the time it takes to complete half an orbit.

The time is also the distance to the Earth divided by the velocity of the light.
 

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