Aperture

In <a href="/facts/Optics/p0vq4S1T">optics</a>, the aperture of an optical system (including a system consisting of a single lens) is a hole or an opening that primarily limits <a href="/facts/Light/jeofpMn4">light</a> propagated through the system. More specifically, the <a href="/facts/Entrance_pupil/8KSLrjSJ">entrance pupil</a> as the front side image of the aperture and <a href="/facts/Focal_length/brGIUkEY">focal length</a> of an <a href="/facts/Optical_system/p0vq4S1T">optical system</a> determine the cone angle of a bundle of <a href="/facts/Ray_(optics)/PgUEC7Sm">rays</a> that comes to a <a href="/facts/Focus_(optics)/QuRKfhg6">focus</a> in the <a href="/facts/Image_plane/46ydpCSb">image plane</a>.
An optical system typically has many openings or structures that limit ray bundles (ray bundles are also known as pencils of light). These structures may be the edge of a <a href="/facts/Lens_(optics)/ejlH6n5c">lens</a> or <a href="/facts/Mirror/wMu4u6BB">mirror</a>, or a ring or other fixture that holds an optical element in place or may be a special element such as a <a href="/facts/Diaphragm_(optics)/bwnWCojS">diaphragm</a> placed in the optical path to limit the light admitted by the system. In general, these structures are called stops, and the aperture stop is the stop that primarily determines the cone of rays that an optical system accepts (see <a href="/facts/Entrance_pupil/8KSLrjSJ">entrance pupil</a>). As a result, it also determines the ray cone angle and brightness at the image point (see <a href="/facts/Exit_pupil/gSQbtt60">exit pupil</a>). The aperture stop generally depends on the object point location; on-axis object points at different object planes may have different aperture stops, and even object points at different lateral locations at the same object plane may have different aperture stops (<a href="/facts/Vignetting/QMcCmUNw">vignetted</a>). In practice, many object systems are designed to have a single aperture stop at designed working distance and <a href="/facts/Field_of_view/Xp1G4CXF">field of view</a>.
In some contexts, especially in <a href="/facts/Photography/ezLPT43M">photography</a> and <a href="/facts/Astronomy/0ArJVM1p">astronomy</a>, aperture refers to the opening diameter of the aperture stop through which light can pass. For example, in a <a href="/facts/Telescope/BDwYahhR">telescope</a>, the aperture stop is typically the edges of the <a href="/facts/Objective_lens/6smChS48">objective lens</a> or mirror (or of the mount that holds it). One then speaks of a telescope as having, for example, a 100-centimetre (39 in) aperture. The aperture stop is not necessarily the smallest stop in the system. Magnification and demagnification by lenses and other elements can cause a relatively large stop to be the aperture stop for the system. In <a href="/facts/Astrophotography/NeWNUJEn">astrophotography</a>, the aperture may be given as a linear measure (for example, in inches or millimetres) or as the dimensionless ratio between that measure and the <a href="/facts/Focal_length/brGIUkEY">focal length</a>. In other photography, it is usually given as a ratio.
A usual expectation is that the term aperture refers to the opening of the aperture stop, but in reality, the term aperture and the aperture stop are mixed in use. Sometimes even stops that are not the aperture stop of an optical system are also called apertures. Contexts need to clarify these terms.
The word aperture is also used in other contexts to indicate a system which blocks off light outside a certain region. In astronomy, for example, a <a href="/facts/Photometry_(astronomy)/fnV9JdSa">photometric</a> aperture around a <a href="/facts/Star/euBFuo07">star</a> usually corresponds to a circular window around the image of a star within which the light intensity is assumed.

Aperture open-in-new

Aperture