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  2. Discovery of cosmic microwave background radiation - Wikipedia

    en.wikipedia.org/wiki/Discovery_of_cosmic...

    The discovery of cosmic microwave background radiation constitutes a major development in modern physical cosmology.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.

  3. Cosmic microwave background - Wikipedia

    en.wikipedia.org/wiki/Cosmic_microwave_background

    Assuming the universe keeps expanding and it does not suffer a Big Crunch, a Big Rip, or another similar fate, the cosmic microwave background will continue redshifting until it will no longer be detectable, [112] and will be superseded first by the one produced by starlight, and perhaps, later by the background radiation fields of processes ...

  4. Cosmic background radiation - Wikipedia

    en.wikipedia.org/wiki/Cosmic_background_radiation

    Background radiation is largely homogeneous and isotropic. A slight detectable anisotropy is present which correlates to galaxy filaments and voids. [2] [3] The discovery (by chance in 1965) of the cosmic background radiation suggests that the early universe was dominated by a radiation field, a field of extremely high temperature and pressure. [4]

  5. BOOMERanG experiment - Wikipedia

    en.wikipedia.org/wiki/BOOMERanG_experiment

    The experiment uses bolometers [3] for radiation detection. These bolometers are kept at a temperature of 0.27 kelvin.At this temperature the material has a very low heat capacity according to the Debye law, thus incoming microwave light will cause a large temperature change, proportional to the intensity of the incoming waves, which is measured with sensitive thermometers.

  6. Exploring The Universe: 20 Astronomy Questions To Test Your ...

    www.aol.com/lifestyle/space-explorer-challenge...

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  7. Project Echo - Wikipedia

    en.wikipedia.org/wiki/Project_Echo

    Project Echo was a pathfinder mission with the objective of testing new technologies and preparing for future missions. Spaceflight engineers used Echo to prove new ideas and test limits in aerodynamics, satellite shape and size, construction materials, temperature control and satellite tracking. [6]

  8. BICEP and Keck Array - Wikipedia

    en.wikipedia.org/wiki/BICEP_and_Keck_Array

    According to the project website: "BICEP Array will measure the polarized sky in five frequency bands to reach an ultimate sensitivity to the amplitude of IGW [inflationary gravitational waves] of σ(r) < 0.005" and "This measurement will be a definitive test of slow-roll models of inflation, which generally predict a gravitational-wave signal ...

  9. New test may detect Alzheimer's years before tau clumps ... - AOL

    www.aol.com/test-may-detect-alzheimers-years...

    New test may detect Alzheimer's years before tau clumps show up in scans. Tim Newman. February 14, 2025 at 10:38 AM. A new study looks at biomarkers that may help detect Alzheimer’s sooner.