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cosmic microwave background radiation

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(cosmology) the cooled remnant of the hot big bang that fills the entire universe and can be observed today with an average temperature of about 2.725 kelvin

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Type of thermal radiation; cosmic background radiation that is fundamental to observational cosmology because it is the oldest light in the universe, dating to the epoch of recombination
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An almost perfect black-body spectrum is exhibited by the cosmic microwave background radiation.
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Its goals were to investigate the cosmic microwave background radiation (CMB) of the universe and provide measurements that would help shape our understanding of the cosmos.
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An example is found in the cosmic microwave background radiation, which exhibits a dipole anisotropy from the Earth's motion relative to this black-body radiation field.
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This is the noise that Penzias and Wilson heard -- the oldest sound that you're ever going to hear, the cosmic microwave background radiation left over from the Big Bang.
Pindah. kamu berada di bawah penangkapanted2019 ted2019
Measurements of the effects of the cosmic microwave background radiation on the dynamics of distant astrophysical systems in 2000 proved the Copernican principle, that, on a cosmological scale, the Earth is not in a central position.
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For example, the cosmic microwave background radiation that we see right now was emitted at the time of photon decoupling, estimated to have occurred about 7005380000000000000♠380,000 years after the Big Bang, which occurred around 13.8 billion years ago.
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The Milky Way is moving with respect to the cosmic microwave background radiation (CMB) in the direction of the constellation Hydra with a speed of 550 km/s, and the Sun's resultant velocity with respect to the CMB is about 370 km/s in the direction of Crater or Leo.
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7 sinne gevind in 3 ms. Hulle kom uit baie bronne en word nie nagegaan nie.