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Cosmic microwave background radiation

Astronomy Cosmic DustCosmic Ray

annoying background noise using a special low noise antenna. The strange thing about the noise was that it was coming from every direction and did not seem to vary in intensity at all. They had discovered the Cosmic Microwave Background Radiation.

 


Cosmic Microwave Background Radiation: Radiation left over from the Big Bang. Because of the expansion of the Universe, the radiation is detected in the microwave portion of the spectrum, and has a temperature of only 2.7 K.

cosmic microwave background radiation The microwave radiation coming from all directions that is believed to be the redshifted glow of the Big Bang.

The Cosmic Microwave Background Radiation is a form of electromagnetic radiation that fills the whole of the universe. It has the characteristics of black body radiation at a temperature of 2.726 kelvins. It has a frequency in the microwave range.

The cosmic microwave background radiation can be explained only by the Big Bang theory. The background radiation is the relic of an early hot universe. The Steady State theory could not explain the background radiation, and so fell into disfavor.

This is the Cosmic Microwave Background Radiation (CMBR) astronomers observe in all directions of the sky and is one of the main pieces of evidence in support of the Big Bang theory.

Over time the cosmic microwave background radiation becomes weaker. Eventually it will be weak enough so that more Hawking radiation will be emitted than the energy of the background radiation being absorbed by the black hole.

WMAP image of the cosmic microwave background radiation anisotropy. It has the most precise thermal emission spectrum known and corresponds to a temperature of 2.725 kelvin (K) with an emission peak at 160.2 GHz.

horizon problem and the flatness problem, as well as generating the primordial density fluctuations that are required for structure formation to occur and which appear to have produced the famous ripples in the cosmic microwave background radiation.

* 1948 - George Gamow predicts the existence of the cosmic microwave background radiation by considering the behavior of primordial radiation in an expanding universe.
1950 to 1999 ...

In physical cosmology, the cosmic microwave background radiation CMB is a form of electromagnetic radiation filling the universe. With a traditional optical telescope, the space between stars and galaxies is pitch black....
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BOOMERANG (Balloon Observations Of Milli-metric Extragalactic Radiation And Geophysics) is an instrument designed to measure anisotropies in the Cosmic Microwave Background Radiation (CMBR).

After Penzias and Wilson found the Cosmic Microwave Background Radiation, astrophysicists began to study whether they could use its properties to study what the universe was like long ago.

Since the discovery of the cosmic microwave background radiation in 1965 it has been regarded as the best theory of the origin and evolution of the cosmos.

An experiment designed to measure the intensity of the cosmic microwave background radiation in different directions.

This was actually the first calculation of the temperature of the Cosmic Microwave Background Radiation, and was confirmed through observation over 20 years later.

However, the X-rays may also be generated by another means: As the electrons in the jet fly away from the quasar at near the , they move through the sea of cosmic microwave background radiation left over from the hot early phase of the .

Operating through 1993, COBE detected small temperature variations in the cosmic microwave background radiation that provided vital clues to the nature of the early universe and its evolution since the "big bang.

Recent observations (such as the BOOMERANG and MAXIMA cosmic microwave background radiation results, and various supernova observations) imply that the expansion of the Universe is accelerating.

MAP will measure minute temperature fluctuations (anisotropy) in the cosmic microwave background radiation (the radiant heat left over from the Big Bang) over the entire sky (these were originally detected by the COBE satellite).

than the big bang
2) the amounts of hydrogen and helium in the universe are similar to what would have been produced soon after the big bang
3) scientists have found a faint remnant of the big bang called the "cosmic microwave background radiation" - ...

of the cosmic background radiation) varies in value along axes in different directions - a physical measurement made in one direction differs from the measurement made in another direction. For example, the cosmic microwave background radiation (the ...

but has since cooled so that today its temperature is 3 K and its peak wavelength is near 1.1 millimeters (in the microwave portion of the spectrum). Also known as the 3-degree background radiation. Also called cosmic microwave background radiation, ...

See also: Background, Background radiation, Universe, Light, Time