If the source is moving towards the observer the wave is "squashed
up" so the wavelength is made smaller. The faster the source moves the more the
waves are squashed.
With sound this means that the pitch of the sound that
you hear is increased and with light the colour of the light that you see is shifted
towards the blue end of the spectrum.
If the source is moving away from the observer the wave is "stretched
out" and so the wavelength is made larger. The faster the source moves the more the
waves are stretched. With sound this means that the pitch of the sound that you hear
is decreased and with light the colour of the light that you see is shifted towards the
red end of the spectrum.
In astronomy the
Doppler effect is used to measure the motion of the galaxies. The faster a galaxy
moves the greater will be the shift in the colour of the light that you receive from it. If
the galaxy is moving away from us then the light from it will be shift towards the red
— this is known as Galactic Red Shift.
Since the Universe started with a Big
Bang most of the galaxies that you can see are moving away from us at high speed.
These speeds may be many tens of thousands of kilometres a second!
Radar speed trap
Red shift of the
galaxies
Siren of a train passing through a station
Change of pitch of a car
horn as it moves towards you and then away.