| 1. Fixed-Magnification Object-Space Telecentric Lens | The entrance pupil is positioned near infinity on the object side, making chief rays approximately parallel to the optical axis. The lens is optimized for one nominal magnification rather than continuous zooming. | Very stable around the specified working distance and nominal magnification. It is not intended to provide a broad zoom range. | High. Perspective distortion and magnification changes caused by moderate object-height variation are strongly reduced. | Usually designed for a fixed working distance, fixed image circle, and a defined sensor format. The usable depth range depends on numerical aperture and acceptable measurement error. | Repeatable dimensional inspection, low perspective error, and straightforward calibration in automated vision systems. | Limited flexibility if the working distance, sensor size, or required magnification changes. Telecentric optics can also be physically longer than ordinary imaging lenses. | Part gauging, edge measurement, semiconductor inspection, dimensional verification, and high-repeatability machine vision. |
| 2. Bi-Telecentric Lens | Telecentricity is provided in both object space and image space. Chief rays are approximately parallel to the optical axis on both sides of the optical system. | Extremely stable against small changes in object distance and image-side positioning when the system is used near its design conditions. | High. Object-side perspective effects are minimized, supporting accurate measurements of object dimensions and relative positions. | Designed to maintain nearly constant magnification while also reducing sensitivity to detector defocus or image-plane displacement. Often uses a comparatively complex multi-element optical layout. | High measurement consistency, low perspective error, and improved tolerance to small setup variations on both sides of the lens. | Typically larger, heavier, and more expensive than a comparable single-sided telecentric lens. Light transmission may be lower because of the additional optical elements and apertures. | Precision metrology, dimensional inspection, tolerance verification, flatness checks, connector inspection, and applications requiring stable scale reproduction. |
| 3. Large-Aperture Object-Space Telecentric Lens | Combines object-space telecentric geometry with a relatively large entrance pupil or clear aperture to collect more light and support higher optical throughput. | Magnification remains substantially less sensitive to object-depth changes than with a conventional non-telecentric lens, provided the object remains within the designed telecentric field. | High, subject to the specified telecentricity error and working range of the design. | Large aperture can provide higher numerical aperture, brighter images, and potentially higher resolving power. It may also reduce depth of field at a given magnification. | Useful for fast imaging, low-light inspection, high-speed line operation, and resolving fine features when illumination and sensor performance are sufficient. | Greater sensitivity to focus, alignment, aberrations, and illumination uniformity. The lens may be larger and more costly, and the reduced depth of field can complicate inspection of uneven parts. | High-speed production inspection, low-light measurement, fine-feature imaging, scientific imaging, and inspection of components with demanding resolution requirements. |