Definition:
"Cosmic microwave background radiation" (often shortened to CMB) is a scientific term that refers to a type of light that is found all over the universe. This light is a remnant from the hot beginning of the universe, known as the Big Bang, and it has cooled down over billions of years to an average temperature of about 2.725 Kelvin (which is very cold!).
In advanced discussions, you might hear scientists talk about the fluctuations or patterns in the cosmic microwave background radiation, which can provide insights into the structure of the universe and its expansion.
There aren't direct synonyms for "cosmic microwave background radiation," but related terms include: - Cosmic background radiation: A more general term that can refer to various forms of radiation in the universe. - Relic radiation: Another term used to describe the leftover radiation from the Big Bang.
This term does not have common idioms or phrasal verbs associated with it, as it is a highly specialized scientific term.
In summary, "cosmic microwave background radiation" is a crucial concept in understanding how our universe began and has evolved.