The Cosmic Microwave Background (CMB) radiation is predominantly observed in the microwave range due to the expansion of the universe, which has stretched the wavelengths from their original emission at about 3,000 kelvin. Initially, this radiation included visible light, but over 13 billion years, it has shifted to longer wavelengths. The CMB is a result of black body radiation from the early universe, and its intensity is now too low to be distinguished from noise by detection devices. Even if the CMB were in the visible spectrum, it would likely remain too faint to be seen, leaving the night sky black. The discussion highlights the challenges of detecting faint background radiation and the effects of cosmic expansion on electromagnetic radiation.