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Doppler Effect for Sound and Light

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Doppler Effect for Sound and Light

1842

The Doppler effect is the apparent difference between the frequency at which sound or light waves leave a source and that at which they reach an observer, caused by relative motion of the observer and the wave source.

The Doppler effect for light was first described by the Austrian physicist Christian Doppler in 1842. He presented his ideas in a paper titled “On the Coloured Light of the Double Stars and Certain Other Stars of the Heavens,” proposing that the observed frequency of waves depends on the relative speed of the source and the observer. This principle was later first confirmed for sound experimentally by the Dutch scientist Christophorus Buys Ballot in 1845. In 1848 it was confirmed for  light. In 1868 we figured out which stars were coming and going for the first time.


That Science Story, 

was first published on TST 2 years ago.

The flashcard inspired by it is this.

Front: What property of sound changes when it moves from air to water?
Back: Speed (not frequency, not wavelength)
All this is part of the broader TST project.
When a source is corrected or expanded, it can be updated once at the tidbit level and reflected everywhere it appears.
This project separates research, synthesis, and reflection so that each can be improved independently without breaking coherence.

The end!

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