Blue shift

Blue shift is the opposite of redshift, the latter being much more noted due to its importance to modern astronomy. It is also used informally to refer to a hypsochromic shift in photochemistry.

Blue shift is the phenomenon that the frequency of an electromagnetic wave (such as light) emitted by a source moving towards the observer is shifted towards the blue side of the electromagnetic spectrum (that is, its wavelength is decreased).

The phenomenon of shifting wavelengths in frames of reference moving relatively to each other is commonly known as Doppler shift or Doppler effect.

While the general redshift of starlight is seen as evidence for an expanding universe, there are a few examples of blue shift in astronomy:

The Andromeda Galaxy is moving towards our own Milky Way Galaxy within the Local Group; thus, when observed from earth, its light is undergoing a blue shift.

When observing spiral galaxies, the side spinning towards us will have a slight blue shift (see Tully-Fisher relation).

Also, Blazars are known to propel relativistic jets towards us, emitting synchrotron radiation and Bremsstrahlung that appears blue shifted.

Cause of blue shift in astronomy

These are the known possible causes of blue shift in astronomy:

Movement of the source towards us, as seen in (a) the edge of a rotating galaxy moving towards us (b) In blazars which propel relativistic jets towards us (c) Some galaxies and quasars [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005ApJ...618..601A&db_key=AST&data_type=HTML&format=&high=42ca922c9c07726
Gravitational effects. See gravitational redshift

Gourt Home::Gourt :: Blue shift

Cause of blue shift in astronomy

See also