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  • Redshift Explained: Understanding the Expansion of the Universe
    The shift in light of a galaxy toward red wavelengths is called redshift.

    Here's why:

    * Doppler Effect: Redshift is a consequence of the Doppler effect, the same phenomenon that makes a siren sound higher pitched when it's coming towards you and lower pitched when it's moving away.

    * Light as a Wave: Light behaves as both a wave and a particle. As a wave, it has a specific wavelength (the distance between wave crests).

    * Expansion of the Universe: Galaxies are moving away from each other due to the expansion of the universe. As a galaxy moves away, its light is stretched, increasing the wavelength.

    * Red Shift: Since red light has a longer wavelength than blue light, the shift in light towards longer wavelengths appears redder, hence the term "redshift."

    Redshift is a fundamental tool in cosmology, allowing astronomers to:

    * Measure the distance to galaxies: The further away a galaxy is, the larger its redshift.

    * Study the expansion of the universe: Redshift provides evidence for the ongoing expansion of the universe.

    * Understand the age and evolution of the universe: By studying the redshift of distant galaxies, astronomers can learn about the early stages of the universe.

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