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Red shift facts for kids

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Redshift
This picture shows redshift. On the left is light from the Sun. On the right is light from a far-off galaxy. Notice how the lines shift towards the red side of the spectrum because of redshift.

Redshift is a cool way astronomers figure out how far away objects are in the Universe. It's like a cosmic speedometer! Redshift is a type of Doppler effect, which you might have heard about with sound.

What is the Doppler Effect?

Imagine a train coming towards you. The sound it makes seems to get higher in pitch as it gets closer. This is because the sound waves are squished together. As the train moves away, the sound gets lower. The sound waves are stretched out.

The same thing happens with light when objects move very fast. If a star or galaxy is moving towards us, its light waves get squished. This makes the light look a bit more blue than it normally would. This is called blue shift.

If a star or galaxy is moving away from us, its light waves get stretched out. This makes the light look more red. That's why it's called "redshift"! The colors shift towards the red end of the light spectrum.

How Do Astronomers Use Redshift?

Astronomers can tell how much light has shifted because every chemical element, like hydrogen or oxygen, has a special "fingerprint" of light. No two elements have the same one!

They use a tool called a spectroscope to look at the light from a distant object. This tool breaks the light into its different colors, showing these unique "fingerprints" as spectral lines.

By comparing where these lines are to where they should normally be, astronomers can tell if an object is moving towards us or away from us. They can also figure out how fast it's going. The faster an object moves, the more its spectral lines shift from their normal spot.

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Kids robot.svg In Spanish: Corrimiento al rojo para niños

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