Maxwell's equations united the study of electromagnetism and optics. Light is the relatively narrow frequency band of electromagnetic waves to which our eyes are sensitive. Figure illustrates the spectrum of visible light. Wavelengths are usually measured in units of nanometers (1 nm = 10 −9 m) or in units of angstroms (1Å = 10 −10m). The colors of the visible spectrum stretch from violet, with the shortest length, to red, with the longest wavelength.
Figure 1 |
The spectrum of electromagnetic radiation, which includes visible light.
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Speed of light
Light travels at such a high speed, 3 × 10 8 m/sec, that historically it was difficult to measure. In the late 1600s, Claus Roemer observed differences in the period of the moons of Jupiter, which varied according to the position of the earth. He correctly assumed a finite speed of light. He deduced the annual variation was due to a changed distance between Jupiter and the earth; so a longer period indicated that the light had farther to travel. His estimate, 2.1 × 10 8 m/s, based on his value for the radius of the earth's orbit, was inaccurate, but his theories were sound. Armand Fizeau was the first to measure the speed of light on the earth's surface. In 1849, he used a rotating toothed wheel to find a close approximation of the speed of light, 3.15 × 10 8 m/s. As shown in Figure , a light beam passed through the wheel, was reflected by a mirror a distance ( d) away, and then again passed through an opening between cogs.
Figure 2 |
Fizeau's apparatus for measuring the speed of light.
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Assume the speed of the wheel is adjusted so that the light passing through the opening a then passes through opening b after reflection. If the toothed wheel spins at an angular velocity ω and the angle between the two openings is θ, then the time for light to travel 2 d is
and so the velocity of light may be calculated from
where c denotes the speed of light. More modern methods with lasers have made measurements accurate to at least nine decimal places.
Light and other elecromagnetic radiation can be polarized because the waves are transverse. An oscillatory motion perpendicular to the direction of motion of the wave is the distinguishing characteristic of transverse waves. Longitudinal waves, such as sound, cannot be polarized. Polarized light has vibrations confined to a single plane that is perpendicular to the direction of motion. A beam of light can be represented by a system of light vectors. In Figure 3, unpolarized light is radiating from a light bulb. The beam going to the top of the page is viewed along the direction of motion (as end‐on). The vectors in the beam traveling to the side of the page are seen perpendicular to the direction of motion (as a side view).