When light rays pass the edge of an opaque material, they tend to bend slightly around the edge of it. This bending, known as diffraction, is due to light acting not as a series of straight rays, but as waves.
The amount of bending is dependent on the wavelength and is different for different colours, as shown in the drawing below. Light passing through a very fine slit appears on a screen a short distance away as a white line with a band of colours on each side. Diffraction also is responsible for the ‘halo’ around the moon and the star-shaped patterns seen when you look at a distant bright light through a window screen.
In photography, diffraction around the edges of a lens diaphragm opening is responsible for the limitation of sharpness improvement when stopping down. Beyond a certain point, the use of smaller aperture no longer increases the sharpness of an image; instead the image actually becomes less sharp. In the same way, the image sharpness of a pinhole camera cannot be improved by making the pinhole smaller beyond a minimum diameter.

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