The Cosmic Microwave Background Radiation (CMB) is a faint glow of microwave radiation that permeates the universe, regarded as the remnant heat from the Big Bang, which occurred approximately 13.8 billion years ago. As the universe expanded, it cooled, and this radiation has stretched to longer wavelengths, now appearing as microwaves. The CMB is nearly uniform in all directions, with slight fluctuations that provide crucial information about the early universe's density variations, leading to the formation of galaxies. These fluctuations are described by a power spectrum, which can be analyzed to infer the universe's composition, age, and rate of expansion. The discovery of the CMB in 1965 by Arno Penzias and Robert Wilson provided strong evidence for the Big Bang theory, marking a pivotal moment in cosmology.
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