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The cosmic microwave background (CMB or CMBR) is microwave radiation that fills all space in the observable universe. It is a remnant that provides an important source of data on the primordial universe. With a standard optical telescope, the background space between stars and galaxies is almost completely … 詳細
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 … 詳細
Assuming the universe keeps expanding and it does not suffer a Big Crunch, a Big Rip, or another similar fate, the cosmic microwave background … 詳細
Early speculations
In 1931, Georges Lemaître speculated that remnants of the early universe may be observable as radiation, … 詳細The cosmic microwave background radiation and the cosmological redshift-distance relation are together regarded as the best available … 詳細
The CMB angular anisotropies are usually presented in terms of power per multipole. The angular the map of temperature across the sky, 詳細
Thermal (non-microwave background) temperature predictions
• 1896 – Charles Édouard Guillaume estimates the "radiation of the stars" to be 5–6 K 詳細CC-BY-SA ライセンスに準拠した Wikipedia テキスト Los Angeles - Wikipedia