The Doppler Effect is the change in frequency of a wave (sound or light) due to the motion of the source or observer. The frequency (and hence pitch) of a sound appears to be higher when the source approaches the listener and lower when the source recedes from him.
It is due to the Doppler Effect that the whistle of a train appears shriller when it approaches a listener than when it moves away from him.
The Doppler Effect is very useful in Astronomy. It can be used to find out whether a star is approaching us or receding away from us. When a star is receding away from us, the light emitted from the star appears red (red light is of lower frequency than other colours). Thus the fact that the light emitted by the stars of distant galaxies suffers a red shift when observed from the earth, means that these galaxies are receding from our galaxy. This is the principle evidence in favour of the hypothesis of expanding universe.
Doppler Effect can also be used to detect or even measure the rotation of a star, e.g. the sun.
It is due to the Doppler Effect that the whistle of a train appears shriller when it approaches a listener than when it moves away from him.
The Doppler Effect is very useful in Astronomy. It can be used to find out whether a star is approaching us or receding away from us. When a star is receding away from us, the light emitted from the star appears red (red light is of lower frequency than other colours). Thus the fact that the light emitted by the stars of distant galaxies suffers a red shift when observed from the earth, means that these galaxies are receding from our galaxy. This is the principle evidence in favour of the hypothesis of expanding universe.
Doppler Effect can also be used to detect or even measure the rotation of a star, e.g. the sun.