Doppler Effect - Definition, Formula, Examples, Uses, FAQs

Doppler Effect - Definition, Formula, Examples, Uses, FAQs

Vishal kumarUpdated on 02 Jul 2025, 04:48 PM IST

The Doppler Effect is a fascinating phenomenon observed when the source of a sound or light wave moves relative to an observer, leading to a change in the perceived frequency of the wave. The Doppler Effect is used in radar technology, medical imaging, and even in determining blood flow velocity in arteries. In this article, we will discuss what is Doppler Effect class 11, the Doppler effect in light, redshift, and blueshift, the Doppler effect formula, application of Doppler effect with solved examples.

This Story also Contains

  1. What is Doppler Effect Class 11 and Explain Doppler Effect?
  2. Doppler Effect Formula
  3. Doppler Effect in Light
  4. Red Shift
  5. Blue Shift
  6. Application Of Doppler Effect
  7. Limitations Of the Doppler Effect
  8. Solved Examples Based on the Doppler Effect
Doppler Effect - Definition, Formula, Examples, Uses, FAQs
Doppler Effect

What is Doppler Effect Class 11 and Explain Doppler Effect?

Doppler effect definition: The Doppler Effect is the change in the frequency or wavelength of a wave about an observer who is moving relative to the wave source. It occurs when the source of the wave (such as sound, light, or other waves) and the observer are in motion relative to each other.

Whenever there is a relative motion between a source of sound and the listener, the apparent frequency/wavelength of sound heard by the listener is different from the actual frequency/wavelength of sound emitted by the source.

When the distance between the source and listener is increasing the apparent frequency decreases. It means the apparent frequency is less than the actual frequency of sound. The reverse of this process is also true.

Doppler Effect Formula

The general expression for apparent frequency

$$
f^{\prime}=f \frac{v \pm v_o}{v \mp v_s}
$$

where,

  • $f^{\prime}$ is the observed frequency
  • $f$ is the actual frequency of the source
  • $v$ is the speed of sound in the medium
  • $v_o$ is the speed of the observer
  • $v_s$ is the speed of the source

Now, for different conditions, the value of apparent frequency will change.

There are some sign conventions for the velocities:

Along the direction Source to Listener is taken as positive and all velocities along the direction Listener to Source are taken as negative.

If the velocity of the medium is zero then the formula becomes

$$f^{\prime}=f \frac{v+v_{\text {listener }}}{v-v_{\text {source }}}$$

Also, read

Doppler Effect in Sound Waves Formula For Some Important Cases ($v$ is the speed of sound in medium)

(1) The source is moving towards the listener and the listener at rest then the formula becomes

$$
f^{\prime}=f\left(\frac{v}{v-v_{\text {source }}}\right)
$$

The sound waves are compacted as the source is moving towards the listener which increases the observed frequency in comparison with the source frequency.


(2) The source is moving away from the listener and the listener is at rest

$$
f^{\prime}=f\left(\frac{v}{v+v_{\text {source }}}\right)
$$

As the source is moving away from the listener the sound waves are spread thus decreasing the observed frequency relative to the original frequency.


(3) The source is at rest but the listener is moving away from the source $$
f^{\prime}=f\left(\frac{v-v_{\text {listener }}}{v}\right)
$$

$f^{\prime}$ decreases compared to the source frequency $f$


(4) The source is at rest but the listener is moving toward the source

$$
f^{\prime}=f\left(\frac{v+v_{\text {listener }}}{v}\right)
$$

As the listener is moving towards the source, observed frequency $f^{\prime}$ increases compared to the actual frequency.


(5) When the Source and listener are approaching each other

$$
f^{\prime}=f\left(\frac{v+v_{\text {listener }}}{v-v_{\text {source }}}\right)
$$

The observed frequency $f^{\prime}$ increases as compared to source frequency when both the source and listener are moving towards each other


(6) When the Source and listener move away from each other

$$
f^{\prime}=f\left(\frac{v-v_{\text {listener }}}{v+v_{\text {source }}}\right)
$$

The observed frequency $f^{\prime}$ decreases compared to the source frequency when the source and the listener are moving away from each other.

Note - Source and listener move perpendicular to the direction of sound wave propagation i.e., $f^{\prime}$ = $f$. It means there is no change in the frequency of the sound heard for the small displacement of the source and listener at a right angle to the direction of wave propagation but this is not true for large displacement. For a large displacement, the frequency decreases because the distance between the source of sound and the listener increases.

Doppler Effect in Light

In light of the observed frequency changes in connection with the relative motion of the source and listener. This is seen in two phenomena- red shift and blue shift.

Doppler effect in a light formula

$$
f^{\prime}=f \sqrt{\frac{1+\frac{v}{c}}{1-\frac{v}{c}}}
$$

OR

$$
\lambda^{\prime}=\lambda \sqrt{\frac{1-\frac{v}{c}}{1+\frac{v}{c}}}
$$

where,

  • $f^{\prime}$ is the observed frequency
  • $f$ is the source frequency
  • $\lambda^{\prime}$ is the observed wavelength
  • $\lambda$ is the source wavelength
  • $v$ is the relative velocity between the source and observer
  • $c$ is the speed of light in a vacuum
NEET Highest Scoring Chapters & Topics
This ebook serves as a valuable study guide for NEET exams, specifically designed to assist students in light of recent changes and the removal of certain topics from the NEET exam.
Download E-book

Commonly Asked Questions

Q: What is the "Doppler cooling" technique in atomic physics?
A:
Doppler cooling is a technique used to cool atoms to very low temperatures using laser light. It exploits the Doppler effect to selectively interact with atoms moving towards the laser beam. These atoms absorb photons and slow down, while atoms moving away are less likely to absorb photons. This process can cool atoms to temperatures just above absolute zero, enabling various quantum physics experiments.
Q: Can the Doppler effect be used to measure the rotation of planets?
A:
Yes, the Doppler effect can be used to measure the rotation of planets through a technique called Doppler imaging. By observing the slight frequency shifts in light from different parts of a planet's surface as it rotates, astronomers can map features and determine the planet's rotation rate. This technique is particularly useful for studying gas giants and stars.
Q: How does the Doppler effect influence the design of speed cameras?
A:
Speed cameras often use the Doppler effect to measure vehicle speeds. They emit radio waves or laser beams and measure the frequency shift of the reflected signals. The magnitude of this shift is directly related to the vehicle's speed, allowing for accurate speed measurements. Understanding the Doppler effect is crucial for designing and calibrating these systems to ensure accurate speed enforcement.
Q: Can the Doppler effect be used to measure the expansion rate of the universe?
A:
Yes, the Doppler effect, in the form of redshift measurements, is a key tool for measuring the expansion rate of the universe. By observing the redshift of distant galaxies and comparing it to their distance (determined by other methods), astronomers can calculate the Hubble constant, which describes the current expansion rate of the universe.
Q: Can the Doppler effect be used to detect gravitational waves?
A:
While gravitational wave detection doesn't directly use the Doppler effect, there are similarities. Gravitational waves cause minute changes in the distance between objects, which can be detected using laser interferometry. This process is analogous to detecting frequency shifts in the Doppler effect, as both involve measuring tiny changes in wave patterns caused by moving sources.

Red Shift

Consider the source is moving away from the observer. The observed wavelength increases while the source moves away shifting towards the red end of the light spectrum and frequency decreases. This phenomenon is called redshift.

$$
z=\frac{\lambda^{\prime}-\lambda}{\lambda}=\frac{v}{c}
$$
Using relativistic formula,

$$
z=\sqrt{\frac{1+\frac{v}{c}}{1-\frac{v}{c}}}-1
$$

Blue Shift

When the source is moving towards the observer the observed frequency becomes shorter and shifts to the blue side of the spectrum.

$$
z=\frac{\lambda-\lambda^{\prime}}{\lambda}=-\frac{v}{c}
$$

Using relativistic formula,

$$
z=1-\sqrt{\frac{1-\frac{v}{c}}{1+\frac{v}{c}}}
$$

where,

  • $z$ is the redshift parameter
  • $\lambda^{\prime}$ is the observed wavelength (longer, shifted towards red)
  • $\lambda$ is the original wavelength of the source
  • $v$ is the relative velocity of the source moving away from the observer
  • $c$ is the speed of light in a vacuum

Application Of Doppler Effect

The Doppler effect is used in the following ways:

  1. The Doppler effect (redshift and blueshift) is used to find the relative motion of celestial bodies.
  2. It helps in identifying the speed, distance, and direction of planets and stars relative to Earth.
  3. The Doppler effect is used in Doppler ultrasound to measure blood flow and heart function.
  4. The Doppler effect is used in LIDAR systems
  5. The Doppler effects are also used to study seismic waves.

Limitations Of the Doppler Effect

  1. The Doppler effect only happens when there is a relative motion between the source and the observer.
  2. The Doppler effect in sound waves depends on the medium.
  3. The Doppler effect formula is inaccurate at high relative velocities which is close to the speed of light.

Recommended Topic Video

Commonly Asked Questions

Q: Why doesn't the Doppler effect apply to transverse waves in a string?
A:
The Doppler effect doesn't apply to transverse waves in a string because these waves are confined to the medium (the string) and don't propagate through space like sound or light waves. The wave speed is determined by the properties of the string, and the relative motion between the source and observer doesn't affect the observed frequency.
Q: Why do we hear the Doppler effect but not see it in everyday life?
A:
We hear the Doppler effect more readily than we see it because the speed of sound (about 343 m/s in air) is much slower than the speed of light (about 3x10^8 m/s). Everyday objects can move at speeds comparable to sound, causing noticeable frequency shifts. However, objects would need to move at incredibly high speeds relative to light for us to perceive a visible Doppler effect.
Q: What's the difference between the classical and relativistic Doppler effect?
A:
The classical Doppler effect applies to sound waves and non-relativistic speeds, while the relativistic Doppler effect applies to light and objects moving at very high speeds. The relativistic version takes into account time dilation and length contraction effects from Einstein's theory of special relativity, leading to a more complex formula for frequency shift.
Q: How does the medium affect the Doppler effect?
A:
The medium affects the Doppler effect by determining the wave speed. The Doppler shift depends on the ratio of the relative motion to the wave speed. For sound waves, this means the effect can vary in different media (e.g., air vs. water). For electromagnetic waves like light, which don't require a medium, the effect is independent of the medium but depends on relative motion.
Q: How does the Doppler effect relate to the concept of Mach number?
A:
The Mach number is the ratio of an object's speed to the speed of sound in the medium. As an object approaches Mach 1 (the speed of sound), it creates a shock wave due to the compression of sound waves ahead of it. This is related to the Doppler effect, as the compressed waves result in a dramatic increase in observed frequency, culminating in the "sonic boom" when the object breaks the sound barrier.

Solved Examples Based on the Doppler Effect

Example 1: An observer is moving with half the speed of light towards a stationary microwave source emitting waves at a frequency of 10 GHz. What is the frequency of the microwave measured by the observer? (speed of light=3×108 ms−1)

1) 10.1 GHz

2) 12.1 GHz

3) 17.3 GHz

4) 15.3 GHz

Solution:

Doppler Effect

When a source of sound and a listener are in motion relative to each other, the frequency of the sound heard by the listener is not the same as the source frequency.

Doppler effect in light

$v^{\prime}=v \sqrt{\frac{1+\frac{v}{c}}{1-\frac{v}{c}}}=17.3 \mathrm{GHz}$

Hence, the answer is the option (3).

Example 2: An observer moves towards a stationary source of sound, with a velocity one­ fifth of the velocity of sound. What is the percentage( in % ) increase in the apparent frequency?

1) 20

2) 5

3) 0

4) 0.5

Solution:

By Doppler's effect

$\begin{gathered}v^{\prime}=\nu\left(\frac{v_s+v_0}{v_s}\right)=\nu+\frac{\nu}{5} \\ \qquad v^{\prime}=\frac{6 \nu}{5} \\ \text { Fractional increase }=\frac{v^{\prime}-v}{v}=\frac{6}{5}-1=\frac{1}{5} \\ \text { Percentage increase }=\frac{1}{5} \times 100=20 \%\end{gathered}$

Hence, the answer is the option (1).

Example 3: Two sources of sounds S1 and S2 produce sound waves of the same frequency 660 Hz. A listener is moving from source S1 towards S2 with a constant speed of u m/s and he hears 10 beats/s. The velocity of sound is 330 m/s. Then, u (in m/s) equals:

1) 2.5

2) 15.0

3) 5.5

4) 10

Solution:

Doppler Effect

When a source of the sound and a listener are in motion relative to each other, the frequency of the sound heard by the listener is not the same as the source frequency.

$\begin{gathered}f_0=660 \mathrm{H} 2 \\ f_1=\text { apparent frequency received from } \mathrm{S} 1=\frac{C-u}{C} f_0 \\ f_2=\text { apparent frequency received from } \mathrm{S} 2=\frac{C+u}{C} f_0 \\ f_2-f_1=\left[\frac{C+u}{C}-\frac{C-u}{C}\right] f_0 \\ \text { beat frequency }=\frac{2 u}{C} f_0=10 \\ \frac{2 u \times 660}{330}=10 \\ u=\frac{10 \times 330}{2 \times 660}=2.5 \mathrm{~m} / \mathrm{s}\end{gathered}$

Hence, the answer is the option (1).

Example 4: A source of sound emits sound waves at frequency f0. It is moving towards an observer with fixed speed vs(vs<v, where v is the speed of sound in air) If the observer were to move towards the source with speed v0, one of the following two graphs (A and B) will give the correct variation of the frequency f heard by the observer as v0 is changed.

The variation of f with v0 is given correctly by :

1. Graph A with slope $=f_0\left(\nu-\nu_s\right)$
2. Graph A with slope $=f_0\left(\nu+\nu_s\right)$
3. Graph B with slope $=f_0\left(\nu-\nu_s\right)$
4. Graph B with slope $=f_0\left(\nu+\nu_s\right)$

Solution:

Frequency of sound when source and observer are moving toward each other

$
\begin{aligned}
& \qquad \nu^{\prime}=\nu_0 \cdot \frac{C+V_0}{C-V_s} \\
& \text { wherein } \\
& C=\text { Speed of sound } \\
& V_0=\text { Speed of observer } \\
& V_s=\text { Speed of source } \\
& \nu_0=\text { Original Frequency } \\
& \nu^{\prime}=\text { apparent frequency }
\end{aligned}
$


Graph A with slope $=f_0\left(\nu-V_s\right)$

Hence, the answer is the option (1).

Example 5: A whistle producing sound waves of frequencies 9500 Hz and above is approaching a stationary person with speed $\nu$ ms-1 The velocity of sound in air is 300 ms-1. If the person can hear frequencies up to a maximum of 10000 Hz, the maximum value of ν up to which he can hear the whistle is :

1) 30 ms−1
2) 152 ms−1
3) 15/2 ms−1
4) 15 ms−1

Solution:

Frequency of sound when the observer is stationary and the source is moving towards the observer -

$
\nu^{\prime}=\nu_0 \cdot \frac{C}{C-V_s}
$

where
$C=$ the speed of sound
$V_s=$ speed of source
$\nu_0=$ original frequency
$\nu^{\prime}=$ apparent frequency

$
\frac{v^{\prime}}{v}=\frac{V_s}{V_s-v}
$


Where $V_s$ is the velocity of sound in air.

$\begin{gathered}\frac{10000}{9500}=\frac{300}{300-v} \\ (300-v)=285 \\ v=15 \mathrm{~m} / \mathrm{s}\end{gathered}$

Hence the answer is the option (4).

Frequently Asked Questions (FAQs)

Q: How does the Doppler effect influence the design of musical instruments?
A:
The Doppler effect doesn't directly influence the design of most musical instruments, as they typically produce stationary sound sources. However, some experimental instruments or techniques may incorporate moving sound sources to create Doppler-like effects. Additionally, understanding the Doppler effect is important for sound engineers and musicians when dealing with moving sound sources in live performances or recordings.
Q: How does the Doppler effect influence the design of musical synthesizers?
A:
While the Doppler effect isn't typically a primary consideration in synthesizer design, some advanced synthesizers incorporate Doppler-like effects to create more realistic or interesting sounds. For example, they might simulate the sound of a passing vehicle or create evolving textures by modulating pitch and amplitude in ways that mimic Doppler shifts.
Q: What is the "transverse Doppler effect" in special relativity?
A:
The transverse Doppler effect is a purely relativistic phenomenon that occurs when the source and observer have a relative motion perpendicular to the line of sight. Unlike the classical Doppler effect, it results in a frequency shift even when there's no radial motion. This effect is a direct consequence of time dilation in special relativity and becomes noticeable only at very high speeds.
Q: How does the Doppler effect relate to the concept of aberration of light?
A:
While the Doppler effect and aberration of light are both consequences of relative motion, they describe different phenomena. The Doppler effect causes a change in frequency or wavelength, while aberration causes an apparent change in the position of a light source. Both effects must be considered when observing fast-moving objects or light sources, especially in astronomical observations.
Q: Can the Doppler effect be used to measure the rotation of galaxies?
A:
Yes, the Doppler effect is crucial in measuring the rotation of galaxies. By observing the redshift and blueshift of spectral lines from different parts of a galaxy, astronomers can determine its rotation curve. This technique has led to important discoveries, such as the presence of dark matter in galaxies, as the observed rotation curves often don't match what would be expected based on visible matter alone.
Q: What is the "Doppler-free spectroscopy" technique?
A:
Doppler-free spectroscopy is a technique used to overcome the limitations of Doppler broadening in spectroscopic measurements. It typically involves using two counter-propagating laser beams to cancel out the Doppler effect. This allows for much higher resolution spectroscopy, revealing fine details of atomic and molecular energy levels that would otherwise be obscured by Doppler broadening.
Q: How does the Doppler effect relate to the concept of frame dragging in general relativity?
A:
While the Doppler effect and frame dragging are distinct phenomena, both involve the effects of motion on the behavior of waves or particles. Frame dragging, predicted by general relativity, is the dragging of spacetime by a rotating massive object. It can cause effects similar to the Doppler effect, such as frequency shifts in light or precession of orbits, but these are due to the curvature and rotation of spacetime rather than relative motion.
Q: Can the Doppler effect be used to measure stellar rotation rates?
A:
Yes, the Doppler effect is used to measure stellar rotation rates through a technique called Doppler imaging. As a star rotates, one side moves towards us while the other moves away, causing slight redshifts and blueshifts in the spectral lines from different parts of the star's surface. By analyzing these shifts, astronomers can determine the star's rotation rate and even map surface features like starspots.