Doppler Shift Light from another galaxy

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SUMMARY

The discussion focuses on the analysis of light from a distant galaxy exhibiting a Doppler shift, specifically an absorption line at 1118 nm compared to the Sun's 625 nm. The participant initially attempted to use classical Doppler equations but encountered inaccuracies due to the significant velocity of the galaxy, approximately 44% of the speed of light. The correct approach involves applying the Relativistic Doppler Shift formula, which accounts for velocities approaching the speed of light, using the relationship λ_s/λ_r = sqrt((1 + beta)/(1 - beta)), where beta = v/c.

PREREQUISITES
  • Understanding of Doppler effect principles
  • Familiarity with light wavelength measurements
  • Knowledge of classical and relativistic physics
  • Basic algebra for rearranging equations
NEXT STEPS
  • Study the Relativistic Doppler Shift equations in detail
  • Learn how to calculate redshift and blueshift in astrophysics
  • Explore the implications of relativistic effects on astronomical observations
  • Investigate the significance of absorption lines in spectroscopy
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Astronomers, astrophysics students, and anyone interested in understanding the effects of relativistic motion on light from distant celestial objects.

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When we analyze the light coming from a distant galaxy, we find a particular absorption line with a wavelength of 1118 nm. This same absorption line in light from the sun has a wavelength of 625 nm is this galaxy moving towards us or away from us?

Calculate the magnitude of the velocity of the galaxy relative to us.

I've tried all what I think are the Doppler equations for light, but can't seem to get the right answer.

When I plug in the values to λr = λc/(c − vr), I get 1.32198284 * 10^8 m / s, which the online homework says is wrong.
 
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Bave you tried:
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and
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?
 
If the classical approach (as you have used) returns a value for the velocity that is a significant fraction of the speed of light (in your case about 44% of c), then you'll want to employ the Relativistic Doppler Shift instead.

λ_s/λ_r = sqrt((1 + beta)/(1 - beta))

where: beta = v/c

This can be rearranged as:

v/c = (λ_s2 - λ_r2)/(λ_s2 + λ_r2)
 

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