The Doppler Effect
Why a siren sounds high on the way in and low on the way out — even though nothing about the sound itself has changed.
The Sound That Changes as It Passes You
Stand by the side of a road as an ambulance goes past. As it approaches, the siren sounds noticeably higher-pitched. The instant it passes and starts moving away, the pitch drops — like someone turned a dial. The siren itself never changed. The ambulance's electronics are producing the exact same frequency the whole time. What changed is your position relative to a moving source of sound waves, and that's enough to shift the frequency your ear receives.
This is the Doppler effect, and once you see the geometry behind it, the pitch-drop of a passing siren, the beep of a radar gun, and the redshifted light from a distant galaxy all turn out to be the same idea.
Picture the ambulance emitting sound wavefronts like ripples from a pebble dropped in a pond, once every period \(T\). But the ambulance is moving, so each new ripple starts from a slightly different spot — a bit closer to you than the last one. Ahead of the ambulance, the wavefronts get crowded closer together: a shorter wavelength reaches you, which means a higher frequency. Behind the ambulance, each wavefront starts a bit farther back, so the wavefronts stretch apart: a longer wavelength, a lower frequency. The speed of sound through the air itself never changes — only the spacing between wavefronts does.
Why the Direction of Motion Is Everything
Only the part of the motion that points directly along the line between source and observer matters. A source flying straight at you produces the maximum shift; a source moving past you but not toward or away from you — like a plane crossing directly overhead at the instant it's closest — produces almost no shift at that instant, even though it's moving fast. This is why the pitch of a passing siren doesn't jump instantly from high to low at one point; it slides smoothly through the moment of closest approach, when the along-the-line component of velocity passes through zero.
Notice also that the source and observer versions of the equation aren't quite symmetric — dividing by \((v-v_s)\) versus multiplying by \((v+v_o)\). At everyday speeds the difference is tiny, but it's a real feature of sound: it needs a physical medium to travel through, and the source and observer play different roles relative to that medium.
- While approaching, the source is moving toward you, so use the minus sign: \(f_o = f_s \dfrac{v}{v - v_s}\).
- Substitute: \(f_o = 600 \times \dfrac{340}{340 - 20} = 600 \times \dfrac{340}{320}\).
- Compute: \(600 \times 340 = 204{,}000\), and \(204{,}000 / 320 = 637.5\) Hz.
- While receding, switch to the plus sign: \(f_o = 600 \times \dfrac{340}{340 + 20} = 600 \times \dfrac{340}{360} = 204{,}000/360 \approx 566.7\) Hz.
- The source is stationary and the observer is moving toward it, so use the plus sign: \(f_o = f_s \dfrac{v + v_o}{v}\).
- Substitute: \(f_o = 500 \times \dfrac{340 + 10}{340} = 500 \times \dfrac{350}{340}\).
- Compute: \(500 \times 350 = 175{,}000\), and \(175{,}000 / 340 \approx 514.7\) Hz.
A passing siren also gets louder as it approaches and quieter as it recedes — but that's a separate effect (distance changing intensity), not the Doppler shift. The Doppler shift is specifically about frequency and pitch, and it happens even at constant distance if the motion has a component along the line of sight. Also remember these equations describe steady, constant-velocity motion in one medium; they break down as a source's speed approaches the speed of sound itself (that's where sonic booms come from), and light's Doppler shift — used for redshift in astronomy — needs a different, relativistic version of the formula rather than this sound-wave one.
Same Idea, Different Waves: Radar and Redshift
Police radar guns send out a radio wave, let it bounce off your moving car, and measure how much the reflected wave's frequency has shifted — that shift converts directly into your speed. Astronomers do something similar with light from distant galaxies: light from galaxies moving away from us arrives at a longer wavelength than emitted, shifted toward the red end of the spectrum, while light from things moving toward us shifts toward blue. It's the identical wavefront-spacing idea you just worked through with sound, just applied to a different kind of wave.
Check your understanding
- Pitch shifts because relative motion between source and observer compresses or stretches the spacing of wavefronts — the speed of sound in the medium itself never changes.
- An approaching source (or an observer moving toward a source) raises the frequency you hear; a receding one lowers it, and the shift is greatest when the motion is directly along the line between them.
- Two related equations cover the everyday cases: \(f_o = f_s \frac{v}{v \mp v_s}\) for a moving source, and \(f_o = f_s \frac{v \pm v_o}{v}\) for a moving observer.
- The same wavefront-spacing principle drives police radar speed guns and the redshift/blueshift astronomers use to measure how fast distant galaxies are moving.