The document discusses the principles and applications of diffraction. It defines diffraction as how waves spread out when passing through an aperture. The amount of diffraction depends on the ratio of the wavelength to the aperture width. A single slit produces a diffraction pattern of bright and dark fringes. Multiple slits produce an interference pattern as each slit acts as a point source. Diffraction gratings can be used to accurately measure wavelengths and produce spectra by separating wavelengths. Applications include measuring unknown wavelengths, identifying materials through their spectra, and determining the composition of stars and nebulae.