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Wave Behaviour - Doppler effect

Grade 11IBPhysics

Review the key concepts, formulae, and examples before starting your quiz.

🔑Concepts

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The Doppler effect is defined as the change in the observed frequency of a wave when there is relative motion between the source and the observer.

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For a source moving towards a stationary observer, the wavefronts ahead of the source are compressed, resulting in a shorter observed wavelength λ′\lambda' and a higher observed frequency f′f'.

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For a source moving away from a stationary observer, the wavefronts are spread out, resulting in a longer observed wavelength λ′\lambda' and a lower observed frequency f′f'.

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For electromagnetic waves (light), the Doppler effect is used in astronomy to determine the velocity of stars and galaxies. A 'red shift' occurs when a source moves away (ff decreases), and a 'blue shift' occurs when a source moves towards the observer (ff increases).

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In the IB syllabus, we distinguish between a moving source (where the wavelength physically changes in the medium) and a moving observer (where the relative speed of the wave changes for the observer).

📐Formulae

f′=f(vv∓vs)f' = f \left( \frac{v}{v \mp v_s} \right) (Moving source: −- for towards, ++ for away)

f′=f(v±vov)f' = f \left( \frac{v \pm v_o}{v} \right) (Moving observer: ++ for towards, −- for away)

Δf=vcf\Delta f = \frac{v}{c} f (Doppler shift for light, where v≪cv \ll c)

Δff=Δλλ≈vc\frac{\Delta f}{f} = \frac{\Delta \lambda}{\lambda} \approx \frac{v}{c} (Fractional shift for light)

💡Examples

Problem 1:

A police car siren emits a sound of frequency 1200 Hz1200\text{ Hz}. The car is traveling at 25 m s−125\text{ m s}^{-1} towards a stationary pedestrian. Calculate the frequency heard by the pedestrian. (Speed of sound v=340 m s−1v = 340\text{ m s}^{-1})

Solution:

Given: f=1200 Hzf = 1200\text{ Hz} vs=25 m s−1v_s = 25\text{ m s}^{-1} v=340 m s−1v = 340\text{ m s}^{-1}

Using the moving source formula (moving towards): f′=f(vv−vs)f' = f \left( \frac{v}{v - v_s} \right) f′=1200×(340340−25)f' = 1200 \times \left( \frac{340}{340 - 25} \right) f′=1200×(340315)f' = 1200 \times \left( \frac{340}{315} \right) f′≈1295.2 Hzf' \approx 1295.2\text{ Hz}

Explanation:

Since the source is moving toward the observer, the denominator (v−vs)(v - v_s) is smaller than vv, which correctly results in an observed frequency higher than the source frequency.

Problem 2:

Light from a distant galaxy is observed to have a wavelength of 658.2 nm658.2\text{ nm}. The known laboratory wavelength for this specific spectral line is 656.3 nm656.3\text{ nm}. Determine the velocity of the galaxy relative to Earth.

Solution:

Given: λlab=656.3 nm\lambda_{lab} = 656.3\text{ nm} λobs=658.2 nm\lambda_{obs} = 658.2\text{ nm} Δλ=658.2−656.3=1.9 nm\Delta \lambda = 658.2 - 656.3 = 1.9\text{ nm}

Using the light formula: Δλλ=vc\frac{\Delta \lambda}{\lambda} = \frac{v}{c} v=c×Δλλv = c \times \frac{\Delta \lambda}{\lambda} v=(3.00×108)×1.9656.3v = (3.00 \times 10^8) \times \frac{1.9}{656.3} v≈8.68×105 m s−1v \approx 8.68 \times 10^5\text{ m s}^{-1}

Explanation:

The observed wavelength is longer than the laboratory wavelength (red shift), indicating that the galaxy is moving away from Earth at approximately 868 km s−1868\text{ km s}^{-1}.