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Light is the final form of energy that we will study. Light behaves like a wave. In fact, light consists of perpendicular electric and magnetic fields that propagate (travel) through space. Since light is a wave, you can think of it as having a wavelength and an amplitude. The wavelength (abbreviated as lower-case Greek letter lambda, λ) of a wave describes the distance between two peaks in the wave. The amplitude of a wave is related to its intensity (the height of a peak). We will work with wavelength throughout the course, but won’t deal with amplitude again.

Waves can also be described in terms of frequency. The frequency of a wave is a measure of the number of peaks that pass by a particular point in space per unit time. The units for measuring frequency are inverse seconds (s ^{-1} ), which equals Hertz (Hz). Frequency is abbreviated using the lower-case Greek letter nu (ν).

All light waves move at the same speed in a vacuum (i.e., empty space). This speed is a fundamental constant which is abbreviated with a lower-case c. The speed of light is equal to about 3.0 x 10^8 m/s. The speed of light is equal to the product of a light wave’s wavelength (λ) in meters and frequency (ν) in s ^{-1} ; therefore c=λν (in m/s). An important consequence of this relationship is that the wavelength of a light wave is inversely proportional to its frequency. In other words, as wavelength increases, frequency decreases (and vice versa).

Shown below are the different regions of the electromagnetic spectrum (Figure 1). Where a particular type of light falls on the spectrum depends on its wavelength and frequency. The boundary between each region of the spectrum can be a bit fuzzy, and these regions are characterized mostly by how light within that region interacts with matter (Table 1). The study of light and its interaction with matter is a field known as spectroscopy.

Figure 1: Electromagnetic spectrum

Table 1: How light interacts with matter

Type of Radiation \lambda unit Interaction with Matter
radio kilometer (km), meter (m) Flip nuclear spin
microwave centimeter (cm), millimeter (mm) Causes molecular rotations
infrared (IR) micrometer ( \mu m) Causes molecular vibrations
visible nanometer (nm) electronic transitions
ultraviolet nanometer (nm) electronic transitions, can break certain chemical bonds
X-rays Angstrom (Å) ionizing radiation (ejection of electrons)
gamma rays Angstrom (Å) ionizing radiation (ejection of electrons)

(Note: You don’t need to memorize these details, but you should be familiar with them.)

You’ll need to know the different regions of the spectrum as well as their relative order: radio, microwaves, infrared, visible, ultraviolet, X-ray, and gamma rays (in order of decreasing wavelength and increasing frequency).

You’ll also need to know the relative order of the regions of the visible spectrum. A convenient acronym is ROYGBV which stands for red, orange, yellow, green, blue, violet, and is pronounced "roy-gee-biv". This acronym lists the regions of the visible spectrum in order of decreasing wavelength and increasing frequency.

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