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The color of the Cosmic Microwave Background Radiation (CMB) appears to change over time due to the expansion of the universe, which causes the wavelengths of the radiation to stretch, leading to a redshift. As the universe expands, the CMB's peak wavelength shifts from the microwave region toward longer wavelengths, making it less energetic and altering its effective temperature. Additionally, advancements in observational technology and methods from 1965 to 2003 improved the precision of measurements, allowing for more detailed analysis of the CMB's properties and the influence of cosmic evolution on its characteristics.

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2mo ago

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