Expert reviewed • 22 November 2024 • 6 minute read
Ole Rømer made the first quantitative measurement of light's speed by observing Jupiter's moon Io. He noticed that Io's orbital period appeared to vary depending on Earth's motion relative to Jupiter. This variation occurred because:
The maximum time difference Rømer observed was 22 minutes, representing the time light took to travel across Earth's orbital diameter. While his calculated value of 200,000 km/s was imprecise due to uncertainties in Earth's orbital size, his work proved that light's speed was finite.
James Bradley discovered stellar aberration - an apparent displacement of stars due to Earth's orbital motion combined with light's finite speed. Using the equation:
Where:
Bradley calculated light's speed to be 301,000 km/s.
Hippolyte Fizeau developed the first terrestrial method using a rotating toothed wheel. The speed could be calculated using:
Where:
This method yielded 313,300 km/s.
Léon Foucault refined the measurement using rotating mirrors, achieving greater accuracy with a value of 298,000 km/s. His setup also demonstrated that light travels slower in water than in air, supporting the wave theory of light.
Following Maxwell's electromagnetic theory, Rosa and Dorsey calculated light's speed using electric and magnetic constants:
Where:
Their result: 299,788 km/s.
Evenson et al. achieved high precision using laser interferometry. The technique involves:
This yielded the highly accurate value of 299,792,457 m/s.
The speed of light's constancy in vacuum, as postulated by Einstein's Special Relativity, led to fundamental changes in how we define measurement units:
Special relativistic effects include:
Where primed quantities represent measurements in moving frames.