Relativity Calculator
Almost from ancient times, light has been acknowledged as the transmitter of information to human eyes. Without light hardly anything is known about the "external world". Aristotle ( 384-322 BC ) conceived of light as ubiquitous and instantaneous whereas Empedocles of Acragas ( 492-432 BC ), Sicilian philosopher-physician-poet and Socrates contemporary, philosophized that the time of transit of light thru an intervening space and bringing information to an observer's eye is finite.
More recently, however, the first acknowledged quantitative determination of the finite speed of light was performed by Danish Olaf Roëmer ( 1644-1710 )
Olaf Roëmer
in December 7, 1676 and officially published in "Philosophical Transactions of the Royal Society, No. 136; June 25, 1677, by Olaf Roëmer". He observed that Jupiter had a transit orbit equivalent to 12 Earth-years and that between an Earth-winter and -summer Jupiter moved slightly [ 1/24th in its total transit orbit ] and hence remained relatively aligned with Earth during any 6-month period. Further, by observing the satellite motions of Jupiter's Io moon as Io entered and then exited from behind Jupiter's shadow when Earth and Jupiter were closest [ Earth summer position at H, see below ], it took approximately 42 hours and 28.6 minutes or ≈ 42.5 hours.
Roëmer's explanation, published June 25, 1677
source: NASA, December 7, 2002 with Io casting
its own shadow to its left. Io was first discovered by
Galileo Galilei on January 7, 1610.
Now as days passed and further observations were made, Roëmer calculated additional minutes to observe Io's reemergence from behind Jupiter's shadow as Earth and Jupiter moved further apart in their respective solar obits [ Earth's relative movement from position G to F. See above. ] In fact, at position F, the period of Io's reemergence was approximately 14 seconds longer! Contrariwise, the time elapses for Io's appearance from behind Jupiter's shadow would shorten as Earth moved relatively closer to Jupiter as from position K to L. At winter position E, the time neither shortened nor lengthened but however there was a delay of approximately 22 minutes as compared to summer position H. Interestingly winter position E represents 2.0 AUs or the diameter of Earth's solar transit which Giovanni Cassini calculated as ≈ 140,000,000 km in 1672. Roëmer therefore astutely calculated the finite speed of light as
[ note: the speed of light is denoted by c from the Latin celeritas meaning speed or swiftness. ]
These numbers which Roëmer used were of course best estimates and approximations calculated by him over several years. Nevertheless Danish Olaf Roëmer did indeed first demonstrate that c, speed of light, is finite and calculable. The modern transit time over 2.0 AUs for Io's reemergence is now accepted as ≈ 16 minutes 40 seconds.
The historical record in determining c :
• Empedocles of Acragas ( 492-432 BC ) philosophized that c is finite.• Danish Olaf Roëmer in 1676 is the acknowledged first to have determined c.
• Hippolyte Fizeau in 1849 performed the first successful measurement of c using an earthbound apparatus.
• Polish-born, Jewish American Albert Abraham Michelson together with Edward Morley determined that c = 299,796 km/sec (186,265 miles per second)
is finite and that no "ether" [ aether ] exists for which he became the first American in 1907 to receive a Nobel Prize in Physics.
• Modern accepted value for c = 299,792,458 m/sec ( 186,292.03 miles per second ), rounded off to c = 300,000 km/sec ( 186,000 miles/sec ).
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