aperture
A hole which restricts the diameter of the lightpath through one plane in an optical system.
aperture: the hole that controls how much light gets through
An aperture is a physical opening, typically circular or sometimes rectangular, that limits the diameter of a light beam passing through an optical system. In cameras, microscopes, telescopes, and projectors, the aperture sits at a specific plane in the optical path and acts as a constraint: light rays outside its diameter are blocked entirely, while those within it pass through to reach the sensor, specimen, or screen downstream. The size of this opening directly governs the brightness of the image, the depth of field, and the resolution of fine detail.
Apertures fall into two main categories: fixed and variable. A fixed aperture, ground into optical glass or molded into a lens barrel, cannot be adjusted and is sized for a specific application, such as a collimator or a relay lens. A variable aperture, controlled by an iris diaphragm or adjustable blade assembly, allows the operator to change the effective diameter during use. In photography, this variable aperture is expressed as an f-number: f/1.4, f/8, f/16, and so on. Smaller f-numbers (like f/1.4) represent larger physical apertures and admit more light; larger f-numbers (like f/16) represent smaller apertures and reduce light transmission but increase depth of field.
Aperture and optical performance
The diameter of an aperture profoundly affects both light transmission and image quality. A larger aperture passes more photons, brightening the image and reducing the exposure time needed in dim conditions, but it also admits more off-axis light and can introduce aberrations if the surrounding optics are not well-corrected. A smaller aperture rejects light from the margins of the lens, which often reduces spherical aberration and improves sharpness, but it also diffraction-limits fine detail at high magnifications. In microscopy, the numerical aperture, defined as n times the sine of half the cone angle of light converging to the specimen (where n is the refractive index of the medium), sets both the resolution and the light-gathering power; a high-NA objective (1.3 to 1.4 for oil immersion) resolves finer structures but requires more illumination than a low-NA dry objective (0.25 to 0.4).
Misalignment or contamination of an aperture stop can severely degrade image contrast and uniformity. Dust or fingerprints on the aperture surface scatter light into the optical path, creating haze and reducing contrast; this is why aperture stops in precision instruments are protected behind windows or sealed. In some systems, an aperture may be intentionally oversized during alignment to allow maximum light for viewing, then reduced to the correct diameter during final assembly. The term 'aperture stop' refers to the aperture that limits the cone angle of the axial light bundle; other apertures in the system may be larger and serve as 'field stops' to define the extent of the image rather than its brightness.
The name 'aperture' comes from Latin 'apertura', meaning 'opening'. In industrial optics, aperture size is always specified as a diameter in millimeters or as a ratio (f-number), never as a radius or area, because the relationship between diameter and light-gathering power is what matters in practice. When specifying an optical system, aperture is listed alongside focal length, wavelength, and numerical aperture to define the system's light-gathering capacity and diffraction-limited performance.