Sound: Pressure in Flight (and a Build)

Pitch is frequency, loudness is amplitude, and a passing siren bends both rules audibly. Then: measure the speed of sound with a wall and a clap.

lesson 2 of 3 in this unit

Builds on: 4.1 Waves: Motion Without Transport

The two dials of a sound

Pitch is frequency. A young ear spans roughly 20 Hz to 20,000 Hz (the top eroding with age and headphone habits); a piano runs 27.5 to 4,186 Hz. Doubling the frequency raises the note exactly one octave — music is arithmetic your ear does for free. Loudness is amplitude — how hard the air is squeezed. Ears handle such a vast range that loudness is measured on the logarithmic decibel scale: every +10 dB is ×10 in energy. A 100 dB club is not “a bit” above an 85 dB limit; it is over thirty times the power.

Sound needs stuff

Pressure waves need something to squeeze. In a vacuum: silence — the film explosions are a courtesy. And the stiffer and lighter the medium’s springs, the faster the wave: ~343 m/s in room air, ~1,480 m/s in water, ~5,000 m/s in steel. Cowboys in films press an ear to the rail because the steel delivers the train’s rumble long before the air does.

The Doppler effect

A siren passes and its pitch visibly droops — eeee-yooow. The siren never changed; the geometry did. Moving toward you, the source partly chases its own waves, packing crests closer: shorter λ, higher pitch. Moving away, it stretches them. The effect belongs to every wave: radar guns Doppler microwaves off your car, bats do it to moths, and the redshift of galaxies — light stretched by recession — is the Doppler clue that the universe expands.

The build: clap at a wall

Sound’s speed is slow enough to measure in a courtyard. Stand 40+ metres from a big flat wall, clap, and the echo returns after the round trip: t = 2d/v — at 50 m, about 0.29 s. Too quick to time well once — so borrow the pendulum trick: clap in rhythm with your own echoes, so each clap lands exactly on the previous echo’s return. Your rhythm period is then exactly the round-trip time. Time 20 claps, divide, and:

v = 2·d / Tdistance there and back, over your clap period — expect within ~10% of 343 m/s
Sonar is this build, weaponised

Ships, bats and ultrasound scanners all run your courtyard experiment at higher frequency: send a pulse, time the echo, multiply by the known speed to get distance. You are calibrating the ruler they all use.

⚗️ Lab — The Siren Flyby

A sound source you can drive past a listener, with the wavefronts drawn honestly.

  • Park the source: perfect circles, steady pitch. Now drive — watch the circles crowd ahead and stretch behind.
  • Read the heard frequency before and after the pass; the drop is the eeee-yooow.
  • Push the source toward the speed of sound and watch the crests pile into a wall.
120 km/h
Approaching
775 Hz
Receding
638 Hz
Pitch drop at the pass
137 Hz
Works for
sound, radar, starlight — any wave

Work it by hand — 0 / 2

No multiple choice here: compute the value and type it. Suffixes like 2.5k or 20m are understood; answers within ±2% count.

1. You clap in rhythm with your echo off a wall 43 m away, and 20 claps take 5.0 s. What speed of sound does that give, in m/s? (v = 2d/T)
2. An ultrasound pulse in tissue (v ≈ 1,540 m/s) returns after 0.0001 s. How deep is the reflector, in metres?

Check your understanding

1. What does the frequency of a sound wave determine?

2. Why does a siren's pitch drop as it passes you?

3. Why is there no sound in space?

4. In the echo experiment, why clap in rhythm with the echoes instead of timing one echo?

5. Every +10 dB of loudness means…

Experiment checklist — 0 / 8