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A camera combines an image-forming arrangement with a surface that records the incident light. An optical lens collects many light rays from each object point and directs them toward a corresponding image point; a photographic emulsion or photodetector then records the image. The optical camera is the imaging part of this arrangement.

The simplest demonstration replaces the optical lens with an optical pinhole. In NASA's two-card activity, foil containing a small hole covers a window in one card, and a second white card receives the projected image of the Sun. Increasing the separation enlarges the image; making several holes produces several images. The receiving card is viewed from the side, rather than looking through the hole at the Sun.^[ref]

An optical pinhole selects narrow bundles of light rays without refraction. A finite hole also produces geometric blur, and an extremely small hole makes diffraction important. These competing effects explain why reducing the hole indefinitely does not produce unlimited spatial resolution.