An ambulance is moving towards a stationary listener at a constant speed of 30 m s⁻¹ - NSC Physical Sciences - Question 6 - 2016 - Paper 1
Question 6
An ambulance is moving towards a stationary listener at a constant speed of 30 m s⁻¹. The siren of the ambulance emits sound waves having a wavelength of 0,28 m. Tak... show full transcript
Worked Solution & Example Answer:An ambulance is moving towards a stationary listener at a constant speed of 30 m s⁻¹ - NSC Physical Sciences - Question 6 - 2016 - Paper 1
Step 1
State the Doppler effect in words.
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Answer
The Doppler effect is the apparent change in frequency (or pitch) of sound detected by a listener, because the sound source and the listener have different velocities relative to the medium of sound propagation. This occurs due to the relative motion between the source of the sound and the observer.
Step 2
Calculate the frequency of the sound waves emitted by the siren as heard by the ambulance driver.
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Answer
Using the formula for wave speed:
v=fλ
we can rearrange to find the frequency:
f=λv
Substituting in the values:
fs=0.28340=1214.29 Hz
Step 3
Calculate the frequency of the sound waves emitted by the siren as heard by the listener.
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For the listener, we use the Doppler effect formula for sound when the source is moving towards a stationary observer:
f′=fsv−vsv+vo
Here, f′ is the frequency heard by the listener, v is the speed of sound, vo is the listener's speed (0 m s⁻¹), and vs is the speed of the ambulance (30 m s⁻¹):
Substituting the values:
f′=1214.29340−30340+0=1214.29310340≈1285.79 Hz
Step 4
How would the answer to QUESTION 6.1.3 change if the speed of the ambulance were LESS THAN 30 m s⁻¹?
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The frequency heard by the listener would DECREASE. This is because, as the speed of the ambulance decreases, the relative motion between the source and observer decreases, leading to a lower frequency being detected.
Step 5
Explain, in terms of the frequencies of the spectral lines, how it is possible to conclude that the star is moving away from the Earth.
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When observing the spectrum of a distant star, if the spectral lines are shifted towards the red end of the spectrum (redshift), it indicates that the star is moving away from the Earth. This effect occurs because the wavelengths of light emitted by the star stretch as it moves away, resulting in lower frequencies being detected compared to the frequencies when the star is stationary.