Rømer's Measurement of the Speed of Light

Initializing live version
Download to Desktop

Requires a Wolfram Notebook System

Interact on desktop, mobile and cloud with the free Wolfram Player or other Wolfram Language products.

Ole Rømer, a Danish astronomer, calculated the speed of light by observing the eclipses of Jupiter's moon during the years 1668–1674. A discrepancy was observed for the time between the eclipses, increasing when the Earth was moving away from Jupiter and decreasing when the Earth was approaching. In half a year, there are a total of 102 eclipses of Io, giving a maximum delay of 16.5 minutes (shown in the bottom-right plot). Rømer interpreted this as the difference in the times needed for the light to travel between Jupiter and Earth. He obtained a value of 214,000 km/s compared to the current value 299,792 km/s. The diameter of the Earth's orbit was not accurately known and there was also an error in the measurement of the delay. Nevertheless, it was a first confirmation that the speed of light is finite.

Contributed by: Enrique Zeleny (April 2010)
Open content licensed under CC BY-NC-SA


Snapshots


Details

The time delay of an eclipse of Io is given by

,

where and are the radii of the orbits of the Earth and Jupiter, is the angular velocity of Earth, represents the period of Io, and is Io's period; finally, is the distance when the Earth is closest to Jupiter and is the velocity of light.

[1] J. H. Shea, "Ole Rǿmer, the Speed of Light, the Apparent Period of Io, the Doppler Effect, and the Dynamics of Earth and Jupiter," Am. J. Phys., 66(7), 1988 pp. 561–569.



Feedback (field required)
Email (field required) Name
Occupation Organization
Note: Your message & contact information may be shared with the author of any specific Demonstration for which you give feedback.
Send