Physics for Geologists, Second edition
Physics for Geologists, Second edition
Physics for Geologists, Second edition
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4 Optics<br />
Light is an electromagnetic radiation. In some respects it behaves as waves; in<br />
others, as particles. Its speed in space, cg, is 299 792.4 km s-I, as is the speed<br />
of other types of electromagnetic radiation. This is an absolute constant, but<br />
light travels rather more slowly in air, much more slowly in transparent mate-<br />
rials such as crystals, glass and water. Radio waves are near one end of the<br />
range of electromagnetic radiations (wavelength h greater than 30 cm, fre-<br />
quency u less than lo9 Hz): y-rays are near the other end (h less than 10-l2 m,<br />
frequency greater than 100 x 1018 Hz). Within the visible range of light, there<br />
is a visible spectrum ranging from the longer-wavelength red to the shorter-<br />
wavelength violet, through orange, yellow, green, blue and indigo. h,,d is<br />
about 700 x lop9 m or 700 nm; hVi,l,, is about 400 nm. Outside this visible<br />
spectrum are infrared and ultraviolet. Infrared can be detected on photo-<br />
graphic film, and by its heat: ultraviolet can be detected because it excites<br />
light in the visible spectrum from some minerals and organic substances.<br />
The same relationship between wavelength, h, speed, c and frequency, u<br />
(the Greek letter nu), exists in electromagnetic radiation as in other waves,<br />
that is<br />
where c is the speed of light (but not necessarily as large as co). However,<br />
electromagnetic radiation does not always behave as waves. In that case,<br />
there is a relationship between the photon quantum energy E, the frequency<br />
of light, and Planck's constant, h,<br />
E = nhu, (4-2)<br />
where n is an integer. This is the basis of the quantum theory, initiated by<br />
Max Planck in 1900 - but we shall not go into it.<br />
Black objects are black because black absorbs practically all wavelengths<br />
that fall on it. White objects are white because white reflects practically all<br />
wavelengths that fall on it.<br />
Copyright 2002 by Richard E. Chapman