You might think we had to wait for modern physics to give us an answer, but Danish astronomer Ole Roemer measured the speed of light as early as 1676.
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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. Once it did, however, the speed of light could be easily calculated by taking the diameter of the Earth’s orbit and dividing it by the difference in time between the quickest and longest recorded For example, if we record the Io eclipse interval, i1, when Earth is at location L and the Io eclipse interval, i2, when Earth is at location K, the speed of light will be the distance between L and K divided by (i2-i1). Using this method, Roemer was able to measure the speed of light as 220,000,000 m/s. In 1983, an international commission on weights and measures set the speed of light in a vacuum at the calculation we use today: 299,792,458 meters per second (186,282 miles per second)—a speed From these findings, Romer could estimate the speed of light.
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Video showing how Ole Rømer attempted to derive the speed of light. Used in the Spitz Fulldome Curriculum for the SciDome planetarium, created by Dr. David B Modern accepted value for = 299,792,458 m/sec (186,292.03 miles per second), rounded off to = 300,000 km/sec (186,000 miles/sec). A better expression for the speed of light combining time and space is 1 meter of light travelled in 1/299,792,458 seconds. [ Mail this page to a friend ] 1983-06-01 See "Ole Rømer, the speed of light, the apparent period of Io, The Doppler effect and the dynamics of Earth and Jupiter" by James H. Shea, American Journal of Physics, 66, July 1998, p. 561-9 Next Stop , Roemer and the First Determination of the Velocity of Light (1676) M. Romer, and ; I Bernard Cohen; M. Romer.
By calculating the 2021-04-12 · In 1676, Rømer announced that the eclipse of Io scheduled for November 9 would be 10 minutes later than the time deduced on the basis of earlier eclipses of the same satellite.
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Olaf Roemer, a Danish astronomer, Made the first estimate of the speed of light in 1676. He did this by mea- suring length of time an eclipes occured in one of Jupiter’s moons. 3.
Fizeau calculated the speed of light to be 313,300 kilometres per second, which was within about five percent of the correct value (299,792.458 kilometers per second). Fizeau published the first results obtained by his method for determining the speed of light in 1849.
A better expression for the speed of light combining time and space is 1 meter of light travelled in 1/299,792,458 seconds. [ Mail this page to a friend ] 1983-06-01 See "Ole Rømer, the speed of light, the apparent period of Io, The Doppler effect and the dynamics of Earth and Jupiter" by James H. Shea, American Journal of Physics, 66, July 1998, p. 561-9 Next Stop , Roemer and the First Determination of the Velocity of Light (1676) M. Romer, and ; I Bernard Cohen; M. Romer.
Very good! Now, knowing how much Io's timing seemed to change and how much the distance from earth to Jupiter varied, Roemer was able to calculate a value
He reasoned that this could be because of the time light takes to travel from Jupiter to Earth. Rømer found the maximum variation in timing of these eclipses to be
The observed eclipses were furthest behind the predicted times when the earth was furthest from Jupiter.
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He cared about winning a prize to determine the longitude of a ship.
The speed of light was then estimated to account for the seven minute overall variation of the observed interval between successive eclipses. Roemer's estimate for the speed of light was 140,000 miles/second, which is remarkably good considering the method employed. The speed of light was then about 1.5 x 10 17 km/sec.
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The best way to do this was to use a very accurate clock Roemer needed to use those planets because the speed of light is just too quick to do it with anything smaller – something that Gallileo found when he tried to measure its speed by sending light 2021-02-27 Ole Rømer's (1676) method of using variations in the apparent period of Jupiter's moon, Io, to demonstrate that the speed of light is finite made use of what we would today call a ``Doppler'' method. He did this 166 years before Christian Doppler described what we now call the Doppler effect and the mechanism in 1842. Although the method Rømer conceived is unquestionably valid, his original Romer estimated that the speed of light was 214000 km/s.
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