What is the relation between redshift and absorption lines in galaxies?

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In summary, the redshift formula shows that different absorption lines from the same object will be redshifted by the same factor, but lines from different objects will have different redshift factors. This factor is determined by the object's relative velocity, gravitational redshifting, and Doppler effect.
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nietzsche
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I understand the concept, but not the math.

For example, let's say a galaxy is moving away from us, and we observe one absorption line at 400 nm, and another absorption line at 500 nm. Let's also say that we determine that the radiation was emitted originally at 200 nm and 300 nm respectively. Then according to the formula for redshift,

[tex]z = \frac{\lambda-\lambda_{0}}{\lambda_{0}} = \frac{500-300}{300} \approx 0.67[/tex]

and

[tex]z = \frac{400-200}{200} = 1[/tex]

Does this mean that every line measured will have a different redshift? Or am I missing something here?

Thanks in advance.
 
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  • #2
nietzsche said:
I understand the concept, but not the math.

For example, let's say a galaxy is moving away from us, and we observe one absorption line at 400 nm, and another absorption line at 500 nm. Let's also say that we determine that the radiation was emitted originally at 200 nm and 300 nm respectively. Then according to the formula for redshift,

[tex]z = \frac{\lambda-\lambda_{0}}{\lambda_{0}} = \frac{500-300}{300} \approx 0.67[/tex]

and

[tex]z = \frac{400-200}{200} = 1[/tex]

Does this mean that every line measured will have a different redshift? Or am I missing something here?

Thanks in advance.

The two lines you describe are redshifted by different factors. Specifically, the multiplier for redshifting one line is not the same for redshifting the other line. So one would have to assume the lines are not from the same object. For a given object, the wavelengths of all its lines are shifted by the same constant multiplier, and its value depends on several factors (object's relative velocity, gravitational redshifting, and Doppler effect).
 
  • #3
fleem said:
The two lines you describe are redshifted by different factors. Specifically, the multiplier for redshifting one line is not the same for redshifting the other line. So one would have to assume the lines are not from the same object. For a given object, the wavelengths of all its lines are shifted by the same constant multiplier, and its value depends on several factors (object's relative velocity, gravitational redshifting, and Doppler effect).

Thanks!
 

FAQ: What is the relation between redshift and absorption lines in galaxies?

What is redshift and how is it related to light?

Redshift is a phenomenon in which the light from an object appears to shift towards the red end of the electromagnetic spectrum. This is caused by the object's motion away from the observer, which stretches the wavelength of the light and causes it to appear redder.

How is redshift used to measure the distance of celestial objects?

By measuring the amount of redshift in an object's light, scientists can calculate its velocity and use that information to determine its distance. The farther away an object is, the faster it appears to be moving away from us, and the greater its redshift will be.

Can redshift be used to study the expansion of the universe?

Yes, the discovery of redshift in the light from distant galaxies was one of the key pieces of evidence for the expanding universe. By studying the redshift of different objects, scientists can track the rate of expansion and learn more about the structure and evolution of the universe.

Are there different types of redshift?

Yes, there are two main types of redshift: Doppler redshift and cosmological redshift. Doppler redshift is caused by the relative motion between an object and an observer, while cosmological redshift is a result of the expansion of the universe.

How does redshift contribute to our understanding of the Big Bang theory?

The Big Bang theory suggests that the universe began with a massive explosion, and redshift is one of the key pieces of evidence for this theory. By studying the redshift of light from distant galaxies, scientists can trace the expansion of the universe back in time and support the idea that it all began from a single point.

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