# Thin lens

A **thin lens** is an idealized lens whose thickness is negligible compared with its object and image distances, so that all refraction is treated as occurring at a single plane through the lens center. In this approximation the relationship between object distance, image distance, and focal length takes a simple algebraic form, the thin lens equation, which is broadly applicable to thin lenses (and, with suitable conventions, "thin" mirrors as well)<sup>[1](https://openstax.org/books/college-physics/pages/25-6-image-formation-by-lenses)</sup>.

| Key fact | Detail |
|---|---|
| Thin lens equation | \( \frac{1}{d_{\text{o}}} + \frac{1}{d_{\text{i}}} = \frac{1}{f} \), where \( d_{\text{o}} \) and \( d_{\text{i}} \) are object and image distances from the lens center and \( f \) is the focal length<sup>[1](https://openstax.org/books/college-physics/pages/25-6-image-formation-by-lenses)</sup> |
| Magnification | \( m = \frac{h_{\text{i}}}{h_{\text{o}}} = -\frac{d_{\text{i}}}{d_{\text{o}}} \); positive \( m \) means an upright image, negative means inverted<sup>[1](https://openstax.org/books/college-physics/pages/25-6-image-formation-by-lenses)</sup><sup> • </sup><sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup> |
| Sign conventions | \( d_{\text{i}} \) is positive for a real image (opposite side from the object) and negative for a virtual image; \( f \) is positive for a converging lens and negative for a diverging lens<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup> |
| Lensmaker's equation (thin lens in air) | \( \frac{1}{f} = (n-1)\left(\frac{1}{R_1} - \frac{1}{R_2}\right) \), with \( n \) the refractive index and \( R_1 \), \( R_2 \) the surface radii<sup>[3](https://www.ncbi.nlm.nih.gov/books/NBK594278/)</sup> |
| Converging behavior | An object beyond the focal length gives a real, inverted image; as the object approaches the focal plane the image distance diverges to infinity<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup> |
| Diverging behavior | The image distance is negative for all positive object distances: the image is virtual, on the same side as the object, and upright<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup> |
| Practical use | The lensmaker's equation determines the optical power of intraocular lenses implanted after cataract surgery; \( 1/f \) equals optical power in diopters<sup>[3](https://www.ncbi.nlm.nih.gov/books/NBK594278/)</sup> |

## The thin lens equation

The equation relates three quantities measured from the center of the lens: the object distance \( d_{\text{o}} \), the image distance \( d_{\text{i}} \), and the focal length \( f \)<sup>[1](https://openstax.org/books/college-physics/pages/25-6-image-formation-by-lenses)</sup>:

\[ \frac{1}{d_{\text{o}}} + \frac{1}{d_{\text{i}}} = \frac{1}{f} \]

The lateral magnification is defined as the ratio of image height to object height,<sup>[1](https://openstax.org/books/college-physics/pages/25-6-image-formation-by-lenses)</sup>

\[ m \equiv \frac{h_{\text{i}}}{h_{\text{o}}} = -\frac{d_{\text{i}}}{d_{\text{o}}} \]

The minus sign encodes orientation: if \( m > 0 \) the image has the same vertical orientation as the object (an upright image), and if \( m < 0 \) it has the opposite orientation (an inverted image)<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup>. The same magnification formula applies to mirrors<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup>.

**Sign conventions.** To use the equation consistently, three rules apply<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup>:

1. \( d_{\text{i}} \) is positive if the image is on the side opposite the object (a real image), otherwise negative (a virtual image).
2. \( f \) is positive for a converging lens and negative for a diverging lens.
3. A radius of curvature \( R \) is positive for a surface convex toward the object and negative for a surface concave toward the object.

## Derivation from two refracting surfaces

The thin-lens equation is obtained by treating the lens as two refracting surfaces in succession. The image formed by the first (left) surface, a virtual image \( Q' \) formed by extending the rays refracted at that surface backward, serves as the object for the second surface<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup>. Applying the single-surface refraction equation at each surface gives<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup>

\[ \frac{n_1}{d_{\text{o}}} + \frac{n_2}{d_{\text{i}}'} = \frac{n_2 - n_1}{R_1} \]

for the first surface, and a corresponding equation with the roles of \( n_1 \) and \( n_2 \) interchanged for the second. In the thin-lens approximation the lens thickness \( t \) is very small compared with the first image distance, \( t \ll d_{\text{i}}' \) (equivalently, \( t \ll R_1 \) and \( R_2 \)), the thickness-dependent terms cancel, and the result is<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup>

\[ \frac{n_1}{d_{\text{o}}} + \frac{n_1}{d_{\text{i}}} = (n_2 - n_1)\left(\frac{1}{R_1} - \frac{1}{R_2}\right) \]

For a lens in air (\( n_1 = 1 \)) this reduces to the thin lens equation with the focal length set by the right-hand side, which is the lensmaker's equation<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup>.

## The lensmaker's equation

The lensmaker's equation specifies how a lens may be formed from a material of refractive index \( n \) by grinding its surfaces to radii \( R_1 \) and \( R_2 \) to produce a desired focal length \( f \)<sup>[4](https://www.sciencedirect.com/topics/engineering/thin-lens)</sup>. For a thin lens in air it reads<sup>[3](https://www.ncbi.nlm.nih.gov/books/NBK594278/)</sup>

\[ \frac{1}{f} = (n-1)\left(\frac{1}{R_1} - \frac{1}{R_2}\right) \]

The full form includes a thickness correction,<sup>[3](https://www.ncbi.nlm.nih.gov/books/NBK594278/)</sup>

\[ \frac{1}{f} = (n-1) \left[ \frac{1}{R_1} - \frac{1}{R_2} + \frac{(n-1)\,d}{n \cdot R_1 \cdot R_2} \right] \]

where \( d \) is the lens thickness; for a thin lens the center thickness is negligible and the correction term drops out<sup>[3](https://www.ncbi.nlm.nih.gov/books/NBK594278/)</sup>. The reciprocal of the focal length, \( 1/f \), is the optical power measured in diopters<sup>[3](https://www.ncbi.nlm.nih.gov/books/NBK594278/)</sup>. The equation is used to design simple lenses of many shapes, including double-convex, double-concave, meniscus, and plano-convex or plano-concave forms, and to determine the optical power of intraocular lenses placed after cataract surgery<sup>[3](https://www.ncbi.nlm.nih.gov/books/NBK594278/)</sup>.

## Image formation

**Converging lens.** Plotting \( d_{\text{i}} = \left(\frac{1}{f} - \frac{1}{d_{\text{o}}}\right)^{-1} \) for a fixed \( f \) shows how the image moves as the object approaches the lens from infinity<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup>. An object much farther than \( f \) from the lens produces an image near the focal plane, because \( 1/d_{\text{o}} \) becomes negligible and \( d_{\text{i}} \approx f \)<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup>. As the object approaches the focal plane, the image distance diverges to positive infinity, since an object at the focal plane produces parallel rays that form an image at infinity<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup>. As long as the object lies beyond the lens's focal length, the image distance comes out positive, meaning the image is real, located across the lens from the object, and inverted<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup>.

**Diverging lens.** For a thin diverging lens with \( f = -1.0 \) cm as a worked example, the image distance is negative for all positive object distances: the image is virtual, on the same side of the lens as the object, and upright<sup>[2](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)</sup>.

**Ray tracing.** Three characteristic rays locate an image graphically<sup>[5](https://micro.magnet.fsu.edu/primer/lightandcolor/lensesintro.html)</sup>: a ray through the lens center passes undeviated; a ray parallel to the optical axis is refracted through the rear focal point; and a ray through the front focal point emerges parallel to the axis. The intersection of any two defines the image plane<sup>[5](https://micro.magnet.fsu.edu/primer/lightandcolor/lensesintro.html)</sup>. Ray tracing gives an approximate picture, while the thin lens equations supply numerical values, and the two methods give consistent results<sup>[1](https://openstax.org/books/college-physics/pages/25-6-image-formation-by-lenses)</sup>.

## Relation to thick lenses and real optical systems

Real lenses and compound systems have refracting surfaces that are not close together, and their behavior is described by principal planes. If object and image distances \( S_1 \) and \( S_2 \) are measured from reference planes \( H \) and \( H' \) rather than from the physical surfaces, any optical system obeys the thin-lens form<sup>[6](https://labs.phys.utk.edu/mbreinig/phys421/modules/m3/Refracting%20systems.html)</sup>

\[ \frac{1}{S_1} + \frac{1}{S_2} = \frac{1}{f_{\text{eff}}} \]

In the paraxial approximation, any optical system behaves like a single lens when referred to its overall principal planes<sup>[6](https://labs.phys.utk.edu/mbreinig/phys421/modules/m3/Refracting%20systems.html)</sup>. For a single thin lens the two principal planes coincide at the plane usually drawn to represent the lens<sup>[7](https://kestrel.nmt.edu/~rsonnenf/phys3034/Supp_Text/Ch18_MatrixOptics_Pedrotti.pdf)</sup>. The focal length is defined as the distance between the principal plane and the focal plane, and every lens has one such pair of planes on each side<sup>[5](https://micro.magnet.fsu.edu/primer/lightandcolor/lensesintro.html)</sup>.

The thin-lens relation also has an alternative form attributed to Newton. Using distances \( X_1 \) and \( X_2 \) measured from the focal points rather than the principal planes, similar triangles give<sup>[6](https://labs.phys.utk.edu/mbreinig/phys421/modules/m3/Refracting%20systems.html)</sup>

\[ X_1 \cdot X_2 = f \cdot f' \]

## Applications

The thin lens equations are used to analyze image formation quantitatively in the eye, where image formation and common vision correction are treated with the same geometric optics<sup>[8](https://openstax.org/books/college-physics-2e/pages/26-1-physics-of-the-eye)</sup>. In lens production, the lensmaker's equation combines refractive index, radii of curvature, and thickness to produce a lens with a targeted focal point based on the desired refraction<sup>[3](https://www.ncbi.nlm.nih.gov/books/NBK594278/)</sup>. The equations assume the lens is surrounded by the same medium (typically air) on both sides, which does not hold for microscope objectives using oil, water, or glycerin immersion<sup>[5](https://micro.magnet.fsu.edu/primer/lightandcolor/lensesintro.html)</sup>.

## References

1. [Image Formation by Lenses, College Physics, OpenStax](https://openstax.org/books/college-physics/pages/25-6-image-formation-by-lenses)
2. [Thin Lenses, University Physics Volume 3, OpenStax](https://openstax.org/books/university-physics-volume-3/pages/2-4-thin-lenses)
3. [Lensmaker's Equation, StatPearls, NCBI Bookshelf](https://www.ncbi.nlm.nih.gov/books/NBK594278/)
4. [Thin Lens, ScienceDirect Topics](https://www.sciencedirect.com/topics/engineering/thin-lens)
5. [Lenses and Geometrical Optics, Molecular Expressions Microscopy Primer, Florida State University](https://micro.magnet.fsu.edu/primer/lightandcolor/lensesintro.html)
6. [Refracting Systems, Physics 421, University of Tennessee](https://labs.phys.utk.edu/mbreinig/phys421/modules/m3/Refracting%20systems.html)
7. [Matrix Methods in Paraxial Optics, Pedrotti, New Mexico Tech](https://kestrel.nmt.edu/~rsonnenf/phys3034/Supp_Text/Ch18_MatrixOptics_Pedrotti.pdf)
8. [Physics of the Eye, College Physics 2e, OpenStax](https://openstax.org/books/college-physics-2e/pages/26-1-physics-of-the-eye)

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*Topic: Encyclopedia › Physical world and mathematics › Physics › Classical physics › Waves and optics › Geometrical optics and imaging › Lenses and image formation › Cardinal points and system descriptors › Thick-lens and thin-lens system parameters*

*Initially written Sep 17, 2026 · Reviewed: Oct 15, 2026 · Edited: Oct 15, 2026; Oct 25, 2026 · Last review: Oct 15, 2026*

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