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Figure 16-8 Roemer measured the time between eclipses as Io emerged from Jupiter s shadow During successive eclipses, Io s measured orbital period became increasingly smaller or larger depending on whether Earth was moving toward (from position 3 to 1) or away from (from position 1 to 3) Jupiter (Illustration not to scale)

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Measurements of the speed of light Roemer concluded that as Earth moved away from Jupiter, the light from each new appearance of Io took longer to travel to Earth because of the increasing distance to Earth Likewise, as Earth approached Jupiter, Io s orbital period seemed to decrease Roemer noted that during the 1825 days that it took Earth to travel from position 1 to position 3, as shown in Figure 16-8, there were (1852 days)(1 Io eclipse/18 days) 103 Io eclipses Thus, for light to travel the diameter of Earth s orbit, he calculated that it takes (103 eclipses )(13 s/eclipse) 13 103 s, or 22 min Using the presently known value of the diameter of Earth s orbit (29 1011 m), Roemer s value of 22 min gives a value for the speed of light of 29 1011 m/((22 min)(60 s/min)) 22 108 m/s Today, the speed of light is known to be closer to 30 108 m/s Thus, light takes 165 min, not 22 min, to cross Earth s orbit Nevertheless, Roemer had successfully proved that light moves at a finite speed Although many measurements of the speed of light have been made, the most notable were performed by American physicist Albert A Michelson Between 1880 and the 1920s, he developed Earth-based techniques to measure the speed of light In 1926, Michelson measured the time required for light to make a round-trip between two California mountains 35 km apart Michelson used a set of rotating mirrors to measure such small time intervals Michelson s best result was (2997996 000004) 108 m/s For this work, he became the first American to receive a Nobel prize in science The speed of light in a vacuum is a very important and universal value; thus it has its own special symbol, c Based on the wave nature of light, which you will study in the next section, the International Committee on Weights and Measurements has measured and defined the speed of light in a vacuum to be c 299,792,458 m/s For many calculations, the value c 300 108 m/s is precise enough At this speed, light travels 946 1012 km in a year This amount of distance is called a light-year.





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7 Use of Material Light Properties Why might you choose a window shade that is translucent Opaque 8 Illuminance Does one lightbulb provide more illuminance than two identical lightbulbs at twice the distance Explain 9 Luminous Intensity Two lamps illuminate a screen equally lamp A at 50 m, lamp B at 30 m If lamp A is rated 75 cd, what is lamp B rated 10 Distance of a Light Source Suppose that a lightbulb illuminating your desk provides only half the illuminance that it should If it is currently 10 m away, how far should it be to provide the correct illuminance

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11 Distance of Light Travel How far does light travel in the time it takes sound to travel 1 cm in air at 20 C 12 Distance of Light Travel The distance to the Moon can be found with the help of mirrors left on the Moon by astronauts A pulse of light is sent to the Moon and returns to Earth in 2562 s Using the measured value of the speed of light to the same precision, calculate the distance from Earth to the Moon 13 Critical Thinking Use the correct time taken for light to cross Earth s orbit, 165 min, and the diameter of Earth s orbit, 298 1011 m, to calculate the speed of light using Roemer s method Does this method appear to be accurate Why or why not

Object Circle Earth Pluto Comet Eccentricity (e) 0 0017 025 070 d (cm) Measured A Measured P Experimental e % Error

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