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Cosmic Background Explorer

   Also found in: Dictionary/thesaurus, Acronyms, Wikipedia, Hutchinson 0.01 sec.
Cosmic Background Explorer: see infrared astronomy infrared astronomy, study of celestial objects by means of the infrared radiation they emit, in the wavelength range from about 1 micrometer to about 1 millimeter. All objects, from trees and buildings on the earth to distant galaxies, emit infrared (IR) radiation.
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Cosmic Background Explorer (COBE)

U.S. satellite that from 1989 to 1993 mapped the cosmic background radiation field. In 1964, microwave radiation was discovered that permeated the cosmos uniformly. This radiation provided spectacular support for the big bang theory, which held that the early universe was very hot. In order to test theories of the universe's history, cosmologists needed to know whether the field was truly the same in every direction. COBE's all-sky survey of the radiation showed slight “wrinkles” from density variations. These variations would have stimulated galaxy formation. A spectrometer showed that the background radiation's spectrum precisely matched the theory.



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In January 1990, John Mather of NASA's Goddard Space Flight Center got a standing ovation from colleagues when he unveiled data from NASA's Cosmic Background Explorer satellite showing that the radiation left over from the Big Bang perfectly matched that of a blackbody with a temperature of 2.
The engaging account for general readers features photos, diagrams, further reading, and a list of contributors to the Cosmic Background Explorer project.
Only the Cosmic Background Explorer satellite six years ago managed to look deeper in space, the project astronomers said.
 
 
 
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