The Doppler Effect: Frequency Shift Due to Relative Motion
- Imagine standing by a road as a car speeds past.
- The sound of the engine is high-pitched as it approaches, but drops suddenly as it moves away.
- This change in pitch is a classic example of the Doppler effect.
Doppler effect
The Doppler effect is the change in the observed frequency of a wave when there is relative motion between the source and the observer
Note
The Doppler effect applies to all types of waves, including sound, light, and water waves.
Why Does the Frequency Change?
To understand the Doppler effect, we need to consider two scenarios:
- Stationary Source and Moving Observer
- Moving Source and Stationary Observer
Stationary Source and Moving Observer
- When a source is stationary, it emits wavefronts that spread out evenly in all directions.
- If the observer is moving towards the source, they encounter wavefronts more frequently, resulting in a higher observed frequency.
- Conversely, if the observer is moving away, they encounter wavefronts less frequently, leading to a lower observed frequency.
Tip
The wavelength remains unchanged in this scenario because the source is stationary.
Moving Source and Stationary Observer
- When the source is moving, the wavefronts are compressed in the direction of motion and stretched in the opposite direction.
- This causes the wavelength to decrease in front of the source and increase behind it.
Example
- Consider a car moving towards an observer while emitting sound waves.
- The wavefronts in front of the car are closer together, leading to a higher frequency for the observer.
- Behind the car, the wavefronts are spread out, resulting in a lower frequency.
Wavefront Representation: Visualizing the Doppler Effect
Stationary Source and Moving Observer
- In this scenario, the wavefronts are concentric circles centered around the stationary source.
- If the observer moves towards the source, they encounter wavefronts more frequently, resulting in a higher observed frequency.
- If the observer moves away, they encounter wavefronts less frequently, leading to a lower observed frequency.
Analogy
Think of wavefronts as runners on a track. If you run towards them, you meet them more often. If you run away, you meet them less frequently.
Moving Source and Stationary Observer
- When the source is moving, the wavefronts are no longer concentric.
- Instead, they are compressed in the direction of motion and stretched in the opposite direction.
- Observer in Front of the Source: The wavefronts are closer together, resulting in a higher frequency and shorter wavelength.
- Observer Behind the Source: The wavefronts are farther apart, leading to a lower frequency and longer wavelength.
Common Mistake
Don’t confuse frequency with intensity (loudness). The Doppler effect changes frequency, not intensity.
Note
Formulas showed in the image above are covered by HL students in the next section.
The Doppler Effect for Light: Redshift and Blueshift
- The Doppler effect also applies to light waves.
- However, because the speed of light is so much greater than everyday speeds, the effect is only noticeable when the relative velocity is a significant fraction of the speed of light.
Redshift and Blueshift
- Redshift:
- If a light source is moving away from the observer, the observed wavelength increases, and the frequency decreases.
- This is called a redshift because the light shifts towards the red end of the spectrum.
- If a light source is moving away from the observer, the observed wavelength increases, and the frequency decreases.
- Blueshift:
- If the source is moving towards the observer, the observed wavelength decreases, and the frequency increases.
- This is called a blueshift because the light shifts towards the blue end of the spectrum.
- If the source is moving towards the observer, the observed wavelength decreases, and the frequency increases.
Example
- Light from a distant galaxy is observed on Earth with a wavelength longer than that emitted.
- This indicates the galaxy is moving away from us, a key piece of evidence for the expanding universe.
Approximate Doppler Formula for Light
When the speed of the source or observer is much smaller than the speed of light, the change in frequency
Here,
Relativistic Doppler effect
Light emitted from a star has a wavelength of 500 nm. On Earth, it is observed at 505 nm. Is the star moving towards or away from Earth? Calculate its speed.
Solution
- Determine
: - Use the Approximate Formula:
- Calculate
:
The star is moving away from Earth at approximately
Reflection and Self-Assessment
Self review
- Can you explain the Doppler effect using wavefront diagrams for both a moving source and a moving observer?
- How does the Doppler effect differ for sound and light waves?
- What are some real-world applications of the Doppler effect?
Theory of Knowledge
How does the Doppler effect for light provide evidence for the expanding universe? Consider the role of redshift in cosmology.
The Doppler effect is a powerful concept that reveals how relative motion affects the waves we observe, from the sound of a passing car to the light from distant galaxies.