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Simple Nature - Light and Matter

Simple Nature - Light and Matter

Simple Nature - Light and Matter

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An image of Jupiter <strong>and</strong>its moon Io (left) from the Cassiniprobe.c / The earth is moving towardJupiter <strong>and</strong> Io. Since thedistance is shrinking, it is takingless <strong>and</strong> less time for the light toget to us from Io, <strong>and</strong> Io appearsto circle Jupiter more quickly thannormal. Six months later, theearth will be on the opposite sideof the sun, <strong>and</strong> receding fromJupiter <strong>and</strong> Io, so Io will appearto revolve around Jupiter moreslowly.The first person to prove that light’s speed was finite, <strong>and</strong> todetermine it numerically, was Ole Roemer, in a series of measurementsaround the year 1675. Roemer observed Io, one of Jupiter’smoons, over a period of several years. Since Io presumably took thesame amount of time to complete each orbit of Jupiter, it could bethought of as a very distant, very accurate clock. A practical <strong>and</strong> accuratependulum clock had recently been invented, so Roemer couldcheck whether the ratio of the two clocks’ cycles, about 42.5 hoursto 1 orbit, stayed exactly constant or changed a little. If the processof seeing the distant moon was instantaneous, there would be noreason for the two to get out of step. Even if the speed of light wasfinite, you might expect that the result would be only to offset onecycle relative to the other. The earth does not, however, stay at aconstant distance from Jupiter <strong>and</strong> its moons. Since the distance ischanging gradually due to the two planets’ orbital motions, a finitespeed of light would make the “Io clock” appear to run faster as theplanets drew near each other, <strong>and</strong> more slowly as their separationincreased. Roemer did find a variation in the apparent speed of Io’sorbits, which caused Io’s eclipses by Jupiter (the moments when Iopassed in front of or behind Jupiter) to occur about 7 minutes earlywhen the earth was closest to Jupiter, <strong>and</strong> 7 minutes late when itwas farthest. Based on these measurements, Roemer estimated thespeed of light to be approximately 2 × 10 8 m/s, which is in the rightballpark compared to modern measurements of 3×10 8 m/s. (I’m notsure whether the fairly large experimental error was mainly due toimprecise knowledge of the radius of the earth’s orbit or limitationsin the reliability of pendulum clocks.)<strong>Light</strong> can travel through a vacuum.Many people are confused by the relationship between sound<strong>and</strong> light. Although we use different organs to sense them, there aresome similarities. For instance, both light <strong>and</strong> sound are typicallyemitted in all directions by their sources. Musicians even use visualmetaphors like “tone color,” or “a bright timbre” to describe sound.One way to see that they are clearly different phenomena is to notetheir very different velocities. Sure, both are pretty fast compared toa flying arrow or a galloping horse, but as we have seen, the speed oflight is so great as to appear instantaneous in most situations. Thespeed of sound, however, can easily be observed just by watching agroup of schoolchildren a hundred feet away as they clap their h<strong>and</strong>sto a song. There is an obvious delay between when you see theirpalms come together <strong>and</strong> when you hear the clap.The fundamental distinction between sound <strong>and</strong> light is thatsound is an oscillation in air pressure, so it requires air (or someother medium such as water) in which to travel. Today, we knowthat outer space is a vacuum, so the fact that we get light from thesun, moon <strong>and</strong> stars clearly shows that air is not necessary for the736 Chapter 12 Optics

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