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The cosmic microwave background radiation is an emission of uniform, black body thermal energy coming from all parts of the sky. The CMB has a thermal black body spectrum at a temperature of 2.725 48 ± 0.000 57 K. The spectrum peaks in the microwave frequency range.
- Cosmic background radiation
Cosmic background radiation is electromagnetic radiation...
- Hintergrundstrahlung
Analog zum kosmischen Mikrowellenhintergrund und...
- Cosmic microwave background radiation
The cosmic microwave background is the radiation that has...
- Cosmic background radiation
In 1964, US physicist Arno Allan Penzias and radio-astronomer Robert Woodrow Wilson discovered the cosmic microwave background (CMB), estimating its temperature as 3.5 K, as they experimented with the Holmdel Horn Antenna.
The Cosmic Microwave Background (CMB) is the cooled remnant of the first light that could ever travel freely throughout the Universe. This 'fossil' radiation, the furthest that any telescope can see, was released soon after the 'Big Bang'.
The cosmic microwave background (or CMB) fills the entire Universe and is leftover radiation from the Big Bang. When the Universe was born, nearly 14 billion years ago, it was filled with hot plasma of particles (mostly protons, neutrons, and electrons) and photons (light).