The Doppler effect describes the apparent change in frequency of a wave when there is relative motion between the source and the observer.
When:
The source approaches, the waves are compressed → higher frequency (pitch rises).
The source moves away, the waves are stretched out → lower frequency (pitch drops).
It’s not the actual frequency changing — it’s how the observer perceives it, due to the motion affecting the wavefront spacing.
Radar and speed guns: Measure how fast cars or baseballs are moving.
Medical imaging (Doppler ultrasound): Measure blood flow velocity in arteries.
Astronomy: Determine if stars or galaxies are moving toward or away from Earth (redshift/blueshift).
Weather radar: Track movement of storm systems.
Navigation and sonar: Submarines and ships use Doppler shift to detect moving objects under water.
Mechanical waves (like sound):
Require a medium (air, water, etc.).
Doppler shift depends on motion relative to the medium, and you must consider both source and observer velocities relative to the medium.
Speed of sound depends on medium properties.
Electromagnetic waves (like light):
Can travel through a vacuum.
Doppler shift is due to relative motion only, and at high speeds, relativistic effects become important.
The speed of light is constant in all inertial frames (according to special relativity), so the equations differ from sound.
the nature of the Doppler effect for sound waves and electromagnetic waves
the representation of the Doppler effect in terms of wavefront diagrams when either the source or the observer is moving
the relative change in frequency or wavelength observed for a light wave due to the Doppler effect where the speed of light is much larger than the relative speed between the source and the observer
that shifts in spectral lines provide information about the motion of bodies like stars and galaxies in space.
the observed frequency for sound waves and mechanical waves due to the Doppler effect