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Bill McKeeman
- 13
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What is known about how long it took to transition from an opaque universe to the release of the cosmic microwave background?
The opaque universe refers to the period of time in the early universe when it was filled with a dense and hot plasma of particles that made it impossible for light to travel through. This resulted in the universe being "opaque" or opaque to light.
The universe transitioned from being opaque to transparent through a process called recombination, which occurred approximately 380,000 years after the Big Bang. During recombination, the universe cooled down enough for electrons and protons to combine and form neutral atoms, allowing light to travel freely through the universe.
The cosmic microwave background (CMB) is the leftover radiation from the Big Bang that permeates the entire universe. It is often referred to as the "afterglow" of the Big Bang and is the oldest light in the universe.
The release of CMB is directly related to the transition from an opaque universe to a transparent one. As the universe became transparent, the CMB was able to travel freely and was released, filling the universe with a faint glow of microwave radiation.
Studying the CMB allows us to learn more about the early universe and its evolution. By analyzing the temperature and polarization patterns of the CMB, we can gather information about the composition, structure, and history of the universe, providing valuable insights into the fundamental laws of physics and the origin of the universe.