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What is redshift?

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Redshift is a phenomenon in physics commonly observed in astronomy. It refers to the shifting of light towards longer wavelengths, which happens when an object in space is moving away from an observer. This shift towards the red end of the spectrum is often used to determine the distance and speed of celestial objects in the universe.
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Redshift refers to the phenomenon where light from distant objects in space, such as galaxies and stars, appears redder than expected. This occurs because the objects are moving away from us, causing their light waves to stretch and shift towards the red end of the spectrum due to the Doppler effect. This effect is a key piece of evidence supporting the expansion of the universe.

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