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How Do Scientists Utilize the Doppler Effect to Measure Cosmic Expansion?

Scientists use something called the Doppler Effect to see how the universe is getting bigger. They do this by looking at the light from faraway galaxies. Here’s how it works:

  1. Redshift and Blueshift:

    • When a galaxy is moving away from us, its light changes to the red side of the color spectrum. This is called redshift.
    • On the other hand, if a galaxy is getting closer, its light changes to the blue side. This is called blueshift.
  2. Calculating Speed:

    • The amount that the light shifts tells scientists how fast the galaxy is moving. They use a special formula to figure this out:

      v=cΔλλ0v = c \cdot \frac{\Delta \lambda}{\lambda_0}

    • In this formula, cc is the speed of light, Δλ\Delta \lambda is how much the light changes, and λ0\lambda_0 is the original light before it changed.

  3. Understanding Expansion:

    • By looking at many galaxies and their light shifts, scientists can get a better idea of how the universe is expanding. This helps them see how fast the universe is growing over time.

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How Do Scientists Utilize the Doppler Effect to Measure Cosmic Expansion?

Scientists use something called the Doppler Effect to see how the universe is getting bigger. They do this by looking at the light from faraway galaxies. Here’s how it works:

  1. Redshift and Blueshift:

    • When a galaxy is moving away from us, its light changes to the red side of the color spectrum. This is called redshift.
    • On the other hand, if a galaxy is getting closer, its light changes to the blue side. This is called blueshift.
  2. Calculating Speed:

    • The amount that the light shifts tells scientists how fast the galaxy is moving. They use a special formula to figure this out:

      v=cΔλλ0v = c \cdot \frac{\Delta \lambda}{\lambda_0}

    • In this formula, cc is the speed of light, Δλ\Delta \lambda is how much the light changes, and λ0\lambda_0 is the original light before it changed.

  3. Understanding Expansion:

    • By looking at many galaxies and their light shifts, scientists can get a better idea of how the universe is expanding. This helps them see how fast the universe is growing over time.

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