Review the key concepts, formulae, and examples before starting your quiz.
🔑Concepts
The Doppler effect is defined as the change in the observed frequency of a wave when there is relative motion between the source and the observer.
For a source moving towards a stationary observer, the wavefronts ahead of the source are compressed, resulting in a shorter observed wavelength and a higher observed frequency .
For a source moving away from a stationary observer, the wavefronts are spread out, resulting in a longer observed wavelength and a lower observed frequency .
For electromagnetic waves (light), the Doppler effect is used in astronomy to determine the velocity of stars and galaxies. A 'red shift' occurs when a source moves away ( decreases), and a 'blue shift' occurs when a source moves towards the observer ( increases).
In the IB syllabus, we distinguish between a moving source (where the wavelength physically changes in the medium) and a moving observer (where the relative speed of the wave changes for the observer).
📐Formulae
(Moving source: for towards, for away)
(Moving observer: for towards, for away)
(Doppler shift for light, where )
(Fractional shift for light)
💡Examples
Problem 1:
A police car siren emits a sound of frequency . The car is traveling at towards a stationary pedestrian. Calculate the frequency heard by the pedestrian. (Speed of sound )
Solution:
Given:
Using the moving source formula (moving towards):
Explanation:
Since the source is moving toward the observer, the denominator is smaller than , which correctly results in an observed frequency higher than the source frequency.
Problem 2:
Light from a distant galaxy is observed to have a wavelength of . The known laboratory wavelength for this specific spectral line is . Determine the velocity of the galaxy relative to Earth.
Solution:
Given:
Using the light formula:
Explanation:
The observed wavelength is longer than the laboratory wavelength (red shift), indicating that the galaxy is moving away from Earth at approximately .