You must have heard or read that our universe is expanding. Edwin Hubble noticed that the light from distant galaxies was shifted toward lower frequencies to the red end of the spectrum. When stars or galaxies are moving away from us, we see their color as red-shifted. This is called Doppler's effect. In this document, we will study this effect in detail.
What is Doppler's Effect?
The Doppler effect in physics refers to the alteration of the frequency of waves, such as sound, light, or others, as the source and observer move closer to or farther away from each other.
This phenomenon was first proposed by Christian Johann Doppler in 1842.
Doppler Effect
MULTIPLE CHOICE QUESTION
Try yourself: What is the Doppler effect?
A
The expansion of the universe observed by Edwin Hubble.
B
The alteration of the frequency of waves as the source and observer move closer to or farther away from each other.
C
The shift of light towards lower frequencies.
D
The red-shift observed in distant galaxies.
Correct Answer: B
- The Doppler effect refers to the alteration of the frequency of waves as the source and observer move closer to or farther away from each other. - It was first proposed by Christian Johann Doppler in 1842. - This effect can be observed in various types of waves, including sound and light. - When the source and observer are moving closer, the frequency of the waves increases, leading to a higher pitch or blue-shift in light. - Conversely, when the source and observer are moving farther away, the frequency of the waves decreases, resulting in a lower pitch or red-shift in light. - The Doppler effect has been instrumental in understanding the expansion of the universe, as observed by Edwin Hubble.
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Doppler Effect Formula
The Doppler effect refers to the perceived alteration in wave frequency resulting from the relative movement between the sound source and the observer. We can determine the apparent frequency in the Doppler effect by employing the following equation:
Doppler effect formula
The above equation changes in different situations depending on the velocities of the observer or the source of the sound.
Case 1: Stationary Source and Stationary Observer
The figure shows a stationary source of frequency n0 which produces sound waves in the air of wavelength l0 given as:
Although sound waves are longitudinal, here we represent sound weaves by the transverse displacement curve as shown in the figure to understand the concept in a better way.
As the source produces waves, these waves travel towards, stationary observer O in the medium (air) with speed v and wavelength l0.
As the observer is at rest here it will observe the same wavelength l0 is approaching it with speed v so it will listen to the frequency n given as:
This is why when a stationary observer list ends the sound from a stationary source of sound, it detects the same frequency sound that the source is producing. Thus no Doppler effect takes place if there is no relative motion between the source and the observer.
Case 2: Stationary Source and Moving Observer
The figure shows the case when a stationary source of frequency n0 produces sound waves that have a wavelength in the air given as:
These waves travel toward the moving observer with velocity v0 towards, the source. When sound waves approach the observer, they will receive the waves of wavelength l0 with speed v0 (relative speed).
Thus the frequency of sound heard by the observer can be given as
Apparent frequency nap = Similarly, we can say that if the observer is receding away from the source the apparent frequency heard by the observer will be given as
Case 3: Moving Source and Stationary Observer
The figure shows the situation when a moving source S of frequency n0 produces sound waves in medium (air) and the waves travel toward the observer with velocity v.
Here if we carefully look at the initial situation when the source starts moving with velocity vs as well as it starts producing waves.
The period of one oscillation is sec and in this duration source emits one wavelength l0 in the direction of propagation of waves with speed v, but in this duration, the source will also move forward by a distance vs.
Thus the effective wavelength of emitted sound in air is slightly compressed by this distance as shown in the figure. This is termed as the apparent wavelength of sound in a medium (air) by the moving source. This is given as:
Apparent wavelength
Now this wavelength will approach the observer with speed v ( O is at rest). Thus the frequency of sound heard by the observer can be given as, Apparent frequency :
Similarly, if the source is receding away from the observer, the apparent wavelength emitted by the source in the air toward the observer will be slightly expanded and the apparent frequency heard by the stationary observer can be given as
Case 4: Moving Source and Moving Observer
Let us consider the situation when both source and observer are moving in the same direction as shown in the figure at speeds vs and v0 respectively.
In this case, the apparent wavelength emitted by the source behind it is given as
Now this wavelength will approach the observer at relative speed v v0 thus the apparent frequency of sound heard by the observer is given as
By looking at the expression of apparent frequency given by the equation, we can easily develop a general relation for finding the apparent frequency heard by a moving observer due to a moving source as
Here + and - signs are chosen according to the direction of motion of the source and observer. For both source and observer v0 and vs are taken in equation with a -ve sign if they are moving in the direction of i.e. the direction of propagation of sound from a source to the observer. For both source and observer v0 and vs are taken with a -ve sign if they are moving in the direction opposite to i.e. opposite to the direction of propagation of sound from the source to the observer.
Doppler Effect in Reflected Sound
When a car is moving toward a stationary wall as shown in the figure, if the car sounds a horn, a wave travels towards the wall and is reflected from the wall.
When the reflected wave is heard by the driver, it appears to be of relatively high pitch. If we wish to measure the frequency of reflected sound then the problem must be handled in two steps.
Reflected sound
First, we treat the stationary wall as a stationary observer and the car as a moving source of sound of frequency n0. In this case, the frequency received by the wall is given as:
Now wall reflects this frequency and behaves like a stationary source of sound of frequency n1 and the car (driver) behaves like a moving observer with velocity vc. Here the apparent frequency heard by the car driver can be given as:
The same problem can also be solved in a different manner by using the method of sound images. In this procedure, we assume the image of the sound source behind the reflector. In the previous example we can explain this by the situation shown in the figure:
Doppler effect in reflected sound
Here we assume that the sound which is reflected by the stationary wall is coming from the image of the car which is at the back of it and coming toward it with velocity vc. Now the frequency of sound heard by car driver can directly be given as:
nap = n0
This method of images for solving problems of the Doppler effect is very convenient but is used only for velocities of source and observer which are very small compared to the speed of sound and it should not be used frequently when the reflector of sound is moving.
Doppler's Effect for Accelerated Motion
For the case of a moving source and a moving observer, we know the apparent frequency observer can be given as
Here v is the velocity of sound and v0 and vs are the velocity of observer and source respectively. When a source of the observer has accelerated or retarded motion then we use that value of v0 at which the observer receives the sound and for the source, we use that value of vs at which it has emitted the wave.
The alternative method of solving this case is the traditional method of compressing or expending the wavelength of sound by the motion of the source and using the relative velocity of sound with respect to the observer.
Doppler's Effect when the line of motion is different
Consider the situation shown in the figure. Two cars 1 and 2 are moving along perpendicular roads at speeds v1 and v2. When car 1 sounds a horn of frequency n0, it emits sound in all directions and says car 2 is at the position, shown in the figure, when it receives the sound.
In such cases we use velocity components of the cars along the line joining the source and observer thus the apparent frequency of sound heard by car 2 can be given as
Doppler's effect when the line of motion is different.
Applications of Doppler's Effect
A common misconception is that the Doppler effect is exclusively relevant to sound waves, but in reality, it applies to all kinds of waves, including light. Here, we've outlined a number of applications for the Doppler effect :
Sirens
Radar
Astronomy
Medical Imaging
Blood Flow Measurement
Satellite Communication
Vibration Measurement
Developmental Biology
Audio
Velocity Profile Measurement
Summary
The following table summarizes the important formulas of various cases of Doppler's effect:
The document Doppler's Effect : Definition, Formula and Applications is a part of the NEET Course Physics Class 11.
FAQs on Doppler's Effect : Definition, Formula and Applications
1. What exactly is Doppler's effect and why does sound change when an ambulance passes by?
Ans. Doppler's effect is the apparent change in frequency of a wave when the source or observer moves relative to each other. When an ambulance approaches, sound waves compress, increasing frequency and pitch. As it moves away, waves stretch, decreasing frequency and lowering pitch. This phenomenon occurs with all waves-sound, light, and electromagnetic radiation-and explains why sirens sound different depending on motion direction and speed.
2. How do I calculate the frequency change using the Doppler effect formula for NEET physics?
Ans. The Doppler's effect formula for sound is: f' = f(v ± vo)/(v ∓ vs), where f' is observed frequency, f is source frequency, v is sound velocity, vo is observer velocity, and vs is source velocity. Use (+) for observer approaching and (-) for receding. The signs reverse for source motion. Understanding which sign applies to your scenario-whether source or observer moves-is crucial for solving NEET problems correctly and avoiding common calculation errors.
3. What's the difference between Doppler shift for sound waves and light waves?
Ans. For sound waves, Doppler's effect depends on the medium's velocity and distinguishes between source and observer motion separately. For light waves, only relative motion matters since light travels through vacuum; the classical formula doesn't apply. Light uses relativistic Doppler equations accounting for time dilation. Additionally, light frequency shifts cause visible colour changes (redshift/blueshift), while sound produces audible pitch changes. Both follow the core principle but require different mathematical approaches.
4. Why do I keep getting Doppler effect problems wrong in practice tests?
Ans. Common mistakes include confusing when to add or subtract velocities in the formula, ignoring the medium's role in sound propagation, and forgetting that observer and source motions have different sign conventions. Students often apply the formula mechanically without understanding directional logic-approaching means compression (higher frequency), receding means expansion (lower frequency). Practise by sketching the scenario first, identifying relative motion direction, then applying signs carefully. Use EduRev's MCQ tests and visual worksheets to strengthen conceptual clarity.
5. How is Doppler's effect used in real life beyond ambulance sirens and what are its practical applications?
Ans. Doppler's effect applications include radar speed guns measuring vehicle velocity, astronomical observations detecting exoplanet motion and universe expansion through redshift, medical ultrasound measuring blood flow velocity, and police Doppler radar. Astrophysics relies heavily on spectral shifts to determine star motion and confirm the Big Bang theory. Meteorological Doppler radar tracks storm systems. Understanding these real-world applications helps students appreciate why Doppler's effect matters beyond exam questions and connects physics to everyday technology.
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