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cosmological redshift

   Also found in: Wikipedia, Hutchinson 0.03 sec.
cosmological redshift [¦käz·mə¦läj·ə·kəl ′red‚shift]
(astronomy)
The red shift that can be ascribed entirely to the general expansion of space-time initiated by the big bang.


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Is it absurd to imagine that they might be slightly stretched or compressed as well, that the cosmological redshift might act differently on different wavelengths?
In the usual interpretation of cosmological redshift -- a well-known effect in which light from a rapidly receding source appears redder than it would had it remained at rest -- the greater the shift, the greater the object's distance from an observer.
 
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