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  1. This remnant of the early universe is the cosmic microwave background radiation—the “three degree” (actually 2.728 K) background radiation—discovered in 1965 by American physicists Arno A. Penzias and Robert W. Wilson. Examine the big-bang model, the theory behind the evolution of the universe.

    • Planck Time

      big-bang model. In big-bang model …a certain epoch called...

  2. Jul 1, 2019 · The relic radiation of the Big Bang decoupled (picture heavy traffic suddenly clearing) nearly 400,000 years later, creating the resonant echo of radiation observed by Penzias and Wilson with...

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  4. en.wikipedia.org › wiki › Big_BangBig Bang - Wikipedia

    In 1964 the CMB was discovered, which convinced many cosmologists that the competing steady-state model of cosmic evolution was falsified, since the Big Bang models predict a uniform background radiation caused by high temperatures and densities in the distant past.

  5. The first moments after the Big Bang are literally hidden from us: the entire cosmos was too hot and dense for any light to pierce. However, signs of what happened then could be imprinted on the cosmic microwave background (CMB), a cold sea of light filling the modern universe.

  6. Another critical discovery was the observation of low levels of microwaves throughout space. Astronomers believe these microwaves, whose temperature is about -270 degrees Celsius, are the remnants of the extremely high-temperature radiation produced by the Big Bang.

  7. May 31, 2001 · Two experiments examining the detailed structure of the cosmic microwave background, the relic radiation from the Big Bang, have confirmed the basic model of how cosmologists believe the universe ...

  8. Oct 11, 2017 · A: No, the Big Bang itself is not something we can see. Q: What can we see? A: We can see the heat radiation that was there when the universe was young. We see this heat as it was about 380,000 years after the expansion of the universe began 13.8 billion years ago (which is what we refer to as the Big Bang).

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