blue shift
n.
A decrease in the wavelength of radiation emitted by an approaching celestial body as a consequence of the Doppler effect.
[From the fact that the shorter wavelengths of light are at the blue end of the visible spectrum.]
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A decrease in the wavelength of radiation emitted by an approaching celestial body as a consequence of the Doppler effect.
[From the fact that the shorter wavelengths of light are at the blue end of the visible spectrum.]
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Blue Shift refers to a shortening of a transmitted signal's wavelength, and/or an increase in its frequency. The name comes from the fact that the shorter-wavelength end of the optical spectrum is the blue (or violet) end, hence, when visible light is compacted in wavelength, it is "shifted towards the blue", or "blue-shifted". Since the longer-wavelength end of the visible electromagnetic spectrum is red, the opposite effect, of a lengthening of a signal's wavelength, is referred to as redshifting.
These terms and conventions ("blue" = compaction, "red"=stretching) are used even when referring to signals outside the optical range (for instance, radio waves, x-rays and gamma rays).
These effects are usually associated with relative motion between the signal source and the observer (a Doppler shift or Doppler effect), where a blueshift will be caused by the two moving towards each other. The term is also used informally to refer to a hypsochromic shift in photochemistry.
Redshift is much more noted due to its importance to modern astronomy. While the general redshift of starlight is seen as evidence for an expanding universe, there are a few examples of blue shift in astronomy:
These are the known possible causes of blue shift in astronomy:
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