Redshift — Light Stretched by Expanding Space

Science

When astronomers look at distant galaxies, their light has been stretched to longer, redder wavelengths by the expansion of space itself. This cosmological redshift is not a Doppler effect — it is a signature of the universe growing as light travels through it.

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10
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Q1 Question 1 of 10

What is cosmological redshift?

Q2 Question 2 of 10

How is cosmological redshift fundamentally different from the Doppler effect?

Q3 Question 3 of 10

What is the redshift parameter z, and how is it calculated?

Q4 Question 4 of 10

If a galaxy has a redshift of z=1, what does this mean for the light we receive from it?

Q5 Question 5 of 10

What does a galaxy with a redshift of z=7 tell us?

Q6 Question 6 of 10

Why does the Andromeda galaxy (M31) show a blueshift rather than a redshift?

Q7 Question 7 of 10

How is redshift used as a proxy for both distance and lookback time?

Q8 Question 8 of 10

What does it mean when astronomers say a galaxy has a peculiar velocity?

Q9 Question 9 of 10

If astronomers detect a spectral line at 700 nm (red light) that was originally emitted at 500 nm (green light), what is the redshift z?

Q10 Question 10 of 10

Why do cosmological recession velocities sometimes appear to exceed the speed of light, and does this violate Einstein's relativity?