Redshift: When a light-emitting object (like a galaxy) moves away from an observer, the light waves are stretched. This increase in wavelength shifts the light toward the red end of the visible spectrum.
Blueshift: When an object moves toward an observer, the light waves are compressed. This decrease in wavelength shifts the light toward the blue/violet end of the visible spectrum.
Cosmological Significance: Observations of redshift in distant galaxies provide primary evidence for the expansion of the universe, as almost all distant objects appear to be moving away from Earth.
| Feature | Approaching Source | Receding Source |
|---|---|---|
| Wavelength () | Decreases (Compressed) | Increases (Stretched) |
| Frequency () | Increases (Higher Pitch/Blue) | Decreases (Lower Pitch/Red) |
| Sound Perception | Higher Pitch | Lower Pitch |
| Light Perception | Blueshift | Redshift |
The Inverse Rule: Always remember that wavelength and frequency move in opposite directions. If a question states the wavelength has doubled, the frequency must have halved.
Direction of Motion: Identify the relative direction immediately. If the distance between the source and observer is closing, frequency must increase. If the distance is growing, frequency must decrease.
Sanity Check: Use the 'Siren Analogy.' Think of an ambulance passing you: the high-pitched 'wee-woo' (approaching) suddenly drops to a lower-pitched 'waw-waw' (receding) the moment it passes. This helps verify if your predicted shift direction is logical.
Spectrum Lines: In physics problems involving light, look for the shift of 'spectral lines' (absorption or emission lines). If they move toward the right (longer wavelengths), it is redshift.
Actual vs. Observed Frequency: A common mistake is thinking the source changes the frequency it emits. The source emits a constant frequency; the 'shift' only exists in the frame of the observer.
Speed vs. Frequency: The Doppler effect depends on velocity, not just position. An object very far away but stationary relative to you will show no Doppler shift, while a nearby object moving fast will show a significant one.
Volume vs. Pitch: In sound, students often confuse the loudness (amplitude) with the pitch (frequency). The Doppler effect specifically concerns pitch, not how loud the sound is.