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Back to C: Wave behaviour

C.5 Doppler effect

Practice exam-style IB Physics questions for Doppler effect, aligned with the syllabus and grouped by topic.

Question 1
SL • Paper 1A
Easy
Non Calculator

A source emits waves of constant frequency. An observer detects a different frequency.

A.

Relative motion with a component along the line joining source and observer

B.

A change in the amplitude emitted by the source

C.

Relative motion perpendicular to the line joining source and observer only

D.

A change in the speed of the wave in the same medium

Question 2
SL • Paper 1A
Easy
Non Calculator

A galaxy is moving away from Earth at a speed much smaller than the speed of light.

A.

Its wavelength increases and its frequency decreases

B.

Its wavelength decreases and its frequency increases

C.

Both its wavelength and frequency increase

D.

Both its wavelength and frequency decrease

Question 3
SL • Paper 1A
Easy
Non Calculator

A point source of sound moves to the right through still air. Wavefronts are closer together on the right of the source than on the left.

A moving point source with circular wavefronts compressed in front of the source on the right and spread out behind it on the left; a stationary observer is positioned to the right.
A.

A frequency less than the emitted frequency

B.

The same frequency but a smaller amplitude

C.

The same frequency but a greater wave speed

D.

A frequency greater than the emitted frequency

Question 4
SL • Paper 1A
Easy
Non Calculator

A star moves across the sky with velocity perpendicular to the line joining it to Earth. In the low-speed Doppler treatment, what is the expected Doppler shift of its spectral lines?

A.

A shift to higher frequency and higher wavelength

B.

Zero, because there is no line-of-sight component of velocity

C.

A redshift, because all moving sources have longer wavelengths

D.

A blueshift, because the speed of light is constant

Question 5
SL • Paper 1A
Easy
Non Calculator

The same absorption-line pattern from hydrogen is observed in a galaxy spectrum at wavelengths longer than the laboratory wavelengths.

A.

The hydrogen atoms in the galaxy have different energy levels

B.

The galaxy emits sound waves as well as light waves

C.

The galaxy is approaching Earth along the line of sight

D.

The galaxy is receding from Earth along the line of sight

Question 6
SL • Paper 1A
Easy
Non Calculator

A source of sound is stationary in still air. An observer moves directly towards the source.

A.

The speed of sound in the air increases for the stationary source

B.

The wavelength in the air decreases because the observer is moving

C.

The observer detects a lower frequency and the wavelength in the air is unchanged

D.

The observer detects a higher frequency but the wavelength in the air is unchanged

Question 7
HL • Paper 1A
Easy
Non Calculator

A sound source moves directly away from a stationary observer through still air.

A.

$f'=f\left(\dfrac{v_w-u_s}{v_w}\right)$

B.

$f'=f\left(\dfrac{v_w}{v_w+u_s}\right)$

C.

$f'=f\left(\dfrac{v_w+u_s}{v_w}\right)$

D.

$f'=f\left(\dfrac{v_w}{v_w-u_s}\right)$

Question 8
HL • Paper 1A
Easy
Non Calculator

A stationary sound source emits frequency ff. An observer moves towards the source with speed uou_o through still air. The speed of sound is vwv_w.

A.

$f\left(\dfrac{v_w}{v_w+u_o}\right)$

B.

$f\left(\dfrac{v_w-u_o}{v_w}\right)$

C.

$f\left(\dfrac{v_w}{v_w-u_o}\right)$

D.

$f\left(\dfrac{v_w+u_o}{v_w}\right)$

Question 9
HL • Paper 1A
Easy
Non Calculator

In Doppler ultrasound, the ultrasound beam makes an angle heta heta to the direction of blood flow.

A.

When the beam is parallel to the blood flow

B.

It is independent of the angle of the beam

C.

When the beam is at 45° to the blood flow

D.

When the beam is perpendicular to the blood flow

Question 10
SL • Paper 2
Easy
Calculator
1.

Define the Doppler effect.

[1]
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2.

State why motion perpendicular to the line of sight does not produce a Doppler shift in the low-speed treatment.

[1]
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Question 11
SL • Paper 2
Easy
Calculator

An astronomical spectrum shows a familiar pattern of absorption lines shifted as a whole.

A laboratory absorption spectrum and two astronomical spectra with the same pattern shifted to longer and shorter wavelengths; wavelength increases left to right with labelled red and blue directions.
1.

State what is meant by a redshift.

[1]
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2.

State what is meant by a blueshift.

[1]
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3.

Explain why a whole pattern of shifted lines is more useful than a single shifted line for identifying the element.

[1]
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Question 12
SL • Paper 1A
Medium
Non Calculator

A spectral line with laboratory wavelength 500.00 nm is observed at 500.05 nm from a star. The speed of light is 3.00imes108extms13.00 imes10^8\, ext{m s}^{-1}.

A.

$3.0 imes10^4\, ext{m s}^{-1}$ away from Earth

B.

$3.0 imes10^5\, ext{m s}^{-1}$ towards Earth

C.

$3.0 imes10^4\, ext{m s}^{-1}$ towards Earth

D.

$3.0 imes10^5\, ext{m s}^{-1}$ away from Earth

Question 13
SL • Paper 1A
Medium
Non Calculator

A rotating star has one edge moving towards Earth and the opposite edge moving away.

A.

The line moves only to longer wavelengths

B.

The line disappears because the redshift cancels the blueshift

C.

The line moves only to shorter wavelengths

D.

The line is broadened because different edges have opposite Doppler shifts

Question 14
HL • Paper 1A
Medium
Non Calculator

A sound source of frequency 500 Hz moves directly towards a stationary observer at 20extms120\, ext{m s}^{-1}. The speed of sound is 340extms1340\, ext{m s}^{-1}.

A.

$471\, ext{Hz}$

B.

$560\, ext{Hz}$

C.

$500\, ext{Hz}$

D.

$531\, ext{Hz}$

Question 15
HL • Paper 1A
Medium
Non Calculator

A stationary source emits sound of frequency 400 Hz. An observer moving towards the source detects 408 Hz. The speed of sound is 340extms1340\, ext{m s}^{-1}.

A.

$20.0\, ext{m s}^{-1}$

B.

$13.6\, ext{m s}^{-1}$

C.

$6.8\, ext{m s}^{-1}$

D.

$3.4\, ext{m s}^{-1}$

Question 16
HL • Paper 1A
Medium
Non Calculator

Why is the approximate Doppler frequency shift in medical ultrasound reflected from moving blood cells proportional to 2u2u rather than uu?

A.

The ultrasound travels twice as fast after reflection

B.

The transmitted frequency is doubled by the transducer

C.

The blood cell first receives a shifted wave and then acts as a moving source of the reflected wave

D.

The blood speed is measured relative to two different media

Question 17
HL • Paper 1A
Medium
Non Calculator

A sound source approaches a stationary observer with speed usu_s in a medium where the sound speed is vwv_w. According to f=f(vw/(vwus))f'=f\left(v_w/(v_w-u_s)\right), what happens as usu_s approaches vwv_w from below?

A.

The observed frequency remains equal to the emitted frequency

B.

The speed of sound increases to keep the wavelength unchanged

C.

The wavefront spacing in front of the source approaches zero and the equation predicts a very large frequency

D.

The observed frequency approaches zero because the source catches the wave

Question 18
SL • Paper 2
Medium
Calculator

A source of sound moves at constant speed through still air.

Circular wavefronts from a point source moving horizontally through still air, showing compressed spacing in front and larger spacing behind; observers labelled in front of and behind the source.
1.

State how the spacing of wavefronts differs in front of and behind the source.

[1]
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2.

Explain why a stationary observer in front of the source detects a different frequency from the emitted frequency.

[1]
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Question 19
SL • Paper 2
Medium
Calculator

A spectral line has laboratory wavelength 656.3extnm656.3\, ext{nm}. It is observed from a star at 656.0extnm656.0\, ext{nm}. Use c=3.00imes108extms1c=3.00 imes10^8\, ext{m s}^{-1}.

1.

Determine the magnitude of the fractional wavelength shift.

[1]
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2.

Determine the line-of-sight speed of the star.

[1]
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3.

State whether the star is approaching or receding.

[1]
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Question 20
SL • Paper 2
Medium
Calculator

Compare the Doppler effect for sound in air with the Doppler effect for light in a vacuum.

1.

State one similarity.

[1]
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2.

State two differences.

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Question 21
SL • Paper 2
Medium
Calculator

The approximation Δf/fv/c\Delta f/f\approx v/c is often used for light.

1.

State the condition under which this approximation is valid.

[1]
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2.

State what type of treatment is required when the condition is not met.

[1]
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Question 22
HL • Paper 2
Medium
Calculator

A whistle emits sound of frequency 720 Hz while moving directly away from a stationary observer at 18extms118\, ext{m s}^{-1}. The speed of sound is 340extms1340\, ext{m s}^{-1}.

1.

Write the appropriate Doppler equation.

[1]
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2.

Calculate the observed frequency.

[1]
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Question 23
HL • Paper 2
Medium
Calculator

A stationary alarm emits sound of frequency 1000 Hz. A cyclist moving directly away from the alarm detects a frequency of 970 Hz. The speed of sound is 330extms1330\, ext{m s}^{-1}.

1.

Write the Doppler equation for this situation.

[1]
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2.

Determine the speed of the cyclist.

[1]
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Question 24
HL • Paper 2
Medium
Calculator

A sound source moves away from a stationary observer.

1.

State whether the plus or minus sign is used in the denominator of f=f(vw/(vw±us))f'=f(v_w/(v_w\pm u_s)).

[1]
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2.

Explain your choice without referring only to memory of the formula.

[1]
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Question 25
SL • Paper 1B
Medium
Non Calculator

The graph shows fractional frequency shift Δf/f\Delta f/f for light from laboratory sources moving directly towards a detector at different speeds.

Graph of fractional frequency shift for sources moving towards a detector at different speeds.
1.

Describe the relationship shown by the graph.

[1]
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2.

Use the gradient to estimate the speed of light.

[1]
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3.

State one reason why the graph would not remain valid at much larger source speeds.

[1]
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Question 26
SL • Paper 1B
Medium
Non Calculator

A ripple source moves across water. A photograph of the wavefronts is shown.

A top-view photograph-style diagram of circular water wavefronts from a source moving across the page, with wavefront spacing visibly smaller on one side and larger on the opposite side; three labelled observer positions around the source.
1.

Identify the direction of motion of the source.

[1]
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2.

State where an observer would detect the greatest frequency.

[1]
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3.

Explain how the photograph provides evidence for your answer to (b).

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Question 27
HL • Paper 1A
Medium
Non Calculator

A police radar emits microwaves of frequency 24.0extGHz24.0\, ext{GHz}. A car moves directly towards the radar at 25.0extms125.0\, ext{m s}^{-1}. Use Δf2vf/c\Delta f\approx 2vf/c with c=3.00imes108extms1c=3.00 imes10^8\, ext{m s}^{-1}.

A.

$2.0\, ext{kHz}$

B.

$0.40\, ext{kHz}$

C.

$4.0\, ext{kHz}$

D.

$40\, ext{kHz}$

Question 28
SL • Paper 2
Medium
Calculator

Light from a rotating star is observed from Earth.

A disk representing a rotating star with arrows showing one limb moving towards the observer and the opposite limb moving away; central region with velocity perpendicular to line of sight.
1.

State the Doppler shift of light from the limb moving towards Earth.

[1]
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2.

State the Doppler shift of light from the opposite limb moving away from Earth.

[1]
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3.

Explain why a spectral line from the whole disk is broadened.

[1]
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Question 29
SL • Paper 2
Medium
Calculator

Redshift measurements can be used to estimate distances to distant galaxies.

1.

Outline how the recessional speed is found from a spectral line shift.

[1]
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2.

Outline how this speed can then be used to estimate distance.

[1]
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3.

State one reason why redshift may not always be a simple Doppler shift due to motion through space.

[1]
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Question 30
HL • Paper 2
Medium
Calculator

A moving sound source and a moving sound observer can both produce Doppler shifts.

Two side-by-side sketches: a moving source with compressed/spread wavefronts and a stationary source with evenly spaced wavefronts crossed by a moving observer.
1.

State how a moving source affects the wavelength pattern in the medium.

[1]
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2.

State how a moving observer affects the wavelength pattern in the medium.

[1]
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3.

Explain why the equations for the two cases have different forms.

[1]
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Question 31
HL • Paper 2
Medium
Calculator

A Doppler ultrasound probe emits ultrasound of frequency 5.0extMHz5.0\, ext{MHz}. The reflected signal from blood has a frequency shift of 5.0extkHz5.0\, ext{kHz}. The speed of ultrasound in tissue is 1540extms11540\, ext{m s}^{-1} and the beam is at 6060^\circ to the flow.

Use Δf/f2ucosheta/vw\Delta f/f\approx 2u\cos heta/v_w.

Ultrasound transducer aimed at a blood vessel, showing the ultrasound beam at an angle theta to the direction of blood flow; labels for beam, vessel, and flow direction.
1.

Calculate the speed of the blood.

[1]
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2.

State why the angle is included in the equation.

[1]
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Question 32
HL • Paper 2
Medium
Calculator

A radar emits microwaves of frequency 24.0extGHz24.0\, ext{GHz}. The reflected signal from a vehicle has a frequency shift of 3.20extkHz3.20\, ext{kHz}. The vehicle moves directly along the radar beam. Use c=3.00imes108extms1c=3.00 imes10^8\, ext{m s}^{-1}.

1.

Write the approximate equation for the reflected radar shift.

[1]
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2.

Calculate the vehicle speed.

[1]
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Question 33
HL • Paper 2
Medium
Calculator

In Doppler ultrasound, an error is made in estimating the angle between the ultrasound beam and the blood-flow direction.

Ultrasound beam crossing a blood vessel with true angle and a smaller incorrectly assumed angle labelled; direction of blood flow indicated.
1.

State the velocity component measured by the Doppler shift.

[1]
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2.

Explain how using an angle that is too small affects the calculated blood speed.

[1]
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Question 34
SL • Paper 1B
Medium
Non Calculator

The table shows laboratory wavelengths and observed wavelengths for three absorption lines in the spectrum of a galaxy.

Spectral lineLaboratory wavelength / nmObserved wavelength / nm
Ca II K393.4399.3
Ca II H396.8402.8
H-beta486.1493.4
1.

For one line, determine the fractional wavelength shift.

[1]
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2.

Use the data to determine the approximate recessional speed of the galaxy.

[1]
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3.

Explain why using several lines is better than using one line.

[1]
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4.

State the direction of motion of the galaxy relative to Earth.

[1]
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Question 35
SL • Paper 1B
Medium
Non Calculator

A table gives redshift-derived recessional speeds and independently estimated distances for several galaxies.

GalaxyDistance / Mpcλ_lab / nmλ_obs / nmSpeed / km s⁻¹
A18656.3659.11280
B34656.3661.52380
C51656.3664.1
D68656.3661.82500
E92656.3670.46450
F125656.3675.48750
G148656.3679.110400
1.

Describe the trend in the data.

[1]
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2.

Use one galaxy’s spectral shift information to calculate its recessional speed.

[1]
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3.

Identify one galaxy that does not fit the overall trend well.

[1]
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4.

Suggest one reason why a galaxy might not lie exactly on the trend.

[1]
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Question 36
HL • Paper 1B
Medium
Non Calculator

A source of sound of constant emitted frequency moves directly towards a stationary microphone at different speeds. The speed of sound is known.

Observed frequency as a function of source speed for a sound source moving towards a stationary microphone.
1.

State the emitted frequency from the graph.

[1]
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2.

Use one data point to determine the speed of the source for a measured frequency.

[1]
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3.

Explain why the graph is not a straight line.

[1]
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4.

State what would change in the equation if the source moved away from the microphone.

[1]
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Question 37
HL • Paper 1B
Medium
Non Calculator

A stationary radar records frequency shifts from three vehicles moving directly along the radar beam.

VehicleTransmitted f / GHzShift magnitude / kHzReflected f
A24.01.60Higher
B24.02.40Lower
C24.01.20Higher
1.

Calculate the speed of one vehicle from its measured frequency shift.

[1]
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2.

Identify which vehicle is moving fastest.

[1]
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3.

Explain why the reflected radar shift contains a factor of two.

[1]
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Question 38
HL • Paper 2
Medium
Calculator

A stationary observer detects a sound frequency of 430 Hz from a source emitting 400 Hz. The source moves directly towards the observer through still air. The speed of sound is 340extms1340\, ext{m s}^{-1}.

1.

Write the Doppler equation for a moving source approaching a stationary observer.

[1]
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2.

Determine the speed of the source.

[1]
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3.

State why the moving-observer equation must not be used here.

[1]
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Question 39
SL • Paper 1B
Hard
Non Calculator

The diagram shows the measured wavelength of the same spectral line from different positions across the disk of a rotating star.

Position on diskx / stellar radiiMeasured wavelength / nm
Left limb-1.0656.10
Left inner-0.5656.20
Centre0.0656.30
Right inner+0.5656.40
Right limb+1.0656.50
1.

Identify the limb moving towards Earth.

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2.

Determine the maximum line-of-sight speed at the stellar limb.

[1]
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3.

Suggest why the central region of the disk has little or no Doppler shift.

[1]
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4.

Explain why the unresolved spectrum of the whole disk has a broadened line.

[1]
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Question 40
HL • Paper 1B
Hard
Non Calculator

A Doppler ultrasound system measures the frequency shift from blood flowing at the same speed while the probe angle is varied. The graph shows Δf\Delta f against cosheta\cos heta.

Doppler ultrasound data; emitted frequency f0 = 5.0 MHz and ultrasound speed in tissue c = 1540 m s^-1.
1.

Describe the relationship shown by the graph.

[1]
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2.

Use the gradient to determine the blood speed.

[1]
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3.

Explain the significance of the intercept.

[1]
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4.

Suggest one advantage of using Doppler ultrasound to measure blood flow.

[1]
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Question 41
HL • Paper 1B
Hard
Non Calculator

A stationary loudspeaker emits a constant frequency. A microphone moves directly towards the loudspeaker at different speeds. The graph shows observed frequency against microphone speed.

Observed frequency for a moving microphone approaching a stationary loudspeaker.
1.

Determine the emitted frequency.

[1]
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2.

Use the graph to determine the speed of sound in the air.

[1]
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3.

Explain why the graph is linear.

[1]
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4.

Predict the change to the graph if the microphone moved away from the loudspeaker.

[1]
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Question 42
SL • Paper 2
Hard
Calculator

A police siren is heard by a stationary pedestrian as a police car approaches and then passes.

A car with siren moving past a stationary pedestrian, showing compressed wavefronts ahead of the car and spread wavefronts behind; the pedestrian is shown before and after the car passes.
1.

Describe the change in frequency heard by the pedestrian before and after the car passes.

[1]
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2.

Explain the observation using wavefronts and the motion of the source.

[1]
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Question 43
SL • Paper 2
Hard
Calculator

A sound source and a sound observer may move relative to the air.

Two panels: one showing a stationary source with evenly spaced circular wavefronts and a moving observer, the other showing a moving source with compressed wavefronts ahead and spread wavefronts behind.
1.

Describe the wavefront pattern for a stationary source and a moving observer.

[1]
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2.

Compare this with the wavefront pattern and detected frequency for a moving source and a stationary observer.

[1]
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Question 44
HL • Paper 1B
Hard
Non Calculator

Two experiments use the same sound frequency and the same speed of sound. In experiment X the source moves towards a stationary detector. In experiment Y the detector moves towards a stationary source. The table gives observed frequency for the same set of speeds.

Approach speed / m s⁻¹Observed fX / HzObserved fY / Hz
0500.0500.0
20529.4531.3
40558.8566.7
60588.2607.1
80617.6653.8
100647.1708.3
1.

Identify which data set corresponds to the moving source.

[1]
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2.

Justify your answer using the mathematical forms of the Doppler equations.

[1]
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3.

For one speed, calculate the percentage difference between the observed frequencies in X and Y.

[1]
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4.

Suggest why the difference becomes more important at larger speeds.

[1]
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Question 45
SL • Paper 2
Hard
Calculator

Spectroscopy is used to investigate the motion of a distant galaxy. A laboratory spectral line at 486.1extnm486.1\, ext{nm} is observed at 489.0extnm489.0\, ext{nm} in the galaxy spectrum.

A comparison of a laboratory absorption spectrum and a galaxy absorption spectrum with the same line pattern shifted to longer wavelengths; the 486.1 nm line and its observed shifted position are labelled.
1.

Calculate the approximate line-of-sight speed of the galaxy.

[1]
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2.

Evaluate the use of spectral-line shifts for determining the motion and distance of galaxies.

[1]
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Question 46
SL • Paper 2
Hard
Calculator

A star of radius 7.0imes108extm7.0 imes10^8\, ext{m} rotates. A spectral line of laboratory wavelength 600.0extnm600.0\, ext{nm} is observed from one limb at 599.94extnm599.94\, ext{nm} and from the opposite limb at 600.06extnm600.06\, ext{nm}.

A rotating stellar disk with one limb labelled with a shorter observed wavelength and the opposite limb with a longer observed wavelength; the star radius is indicated.
1.

Explain why the two limbs show opposite wavelength shifts.

[1]
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2.

Estimate the rotational period of the star.

[1]
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Question 47
HL • Paper 2
Hard
Calculator

A sound source emits frequency 600 Hz in still air where the sound speed is 340extms1340\, ext{m s}^{-1}.

1.

Calculate the observed frequency when the source moves towards a stationary observer at 30extms130\, ext{m s}^{-1}.

[1]
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2.

Compare this with the observed frequency when an observer moves towards the stationary source at 30extms130\, ext{m s}^{-1}, and explain the difference.

[1]
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Question 48
HL • Paper 2
Hard
Calculator

A Doppler ultrasound probe sends waves of frequency 4.0extMHz4.0\, ext{MHz} into tissue. The speed of ultrasound in the tissue is 1540extms11540\, ext{m s}^{-1}. The beam is at 3030^\circ to the blood-flow direction and the measured reflected frequency shift is 7.2extkHz7.2\, ext{kHz}.

A medical ultrasound probe directed at a blood vessel with beam angle theta to blood flow; reflected wave shown returning to the probe.
1.

Determine the blood speed.

[1]
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2.

Discuss the physical origin and medical value of the Doppler ultrasound measurement.

[1]
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Question 49
HL • Paper 2
Hard
Calculator

Doppler radar and Doppler sound measurements are both used to determine speeds.

1.

radar of frequency 10.0extGHz10.0\, ext{GHz} detects a reflected frequency shift of 1.20extkHz1.20\, ext{kHz} from rain moving directly along the beam. Calculate the rain speed.

[1]
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2.

Evaluate similarities and differences between using Doppler radar and Doppler sound to measure motion.

[1]
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Question 50
HL • Paper 2
Hard
Calculator

An ambulance siren emits sound at 900 Hz. A stationary observer hears 960 Hz as the ambulance approaches. Take the speed of sound as 340extms1340\, ext{m s}^{-1}.

1.

Determine the speed of the ambulance.

[1]
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2.

The same observed frequency of 960 Hz could instead be produced by a moving observer approaching a stationary siren. Evaluate this statement quantitatively and physically.

[1]
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C.4 Standing waves and resonance