Lens and Mirror Equation Calculator
Solve optics problems for converging lenses, diverging lenses, concave mirrors, and convex mirrors. Enter any two known values — object distance, image distance, or focal length — and the lens and mirror equation calculator computes the unknown, magnification, and full image classification (real/virtual, upright/inverted, enlarged/diminished). All calculations run locally in your browser with no signup required.
Select the optic type and what you want to solve for, then enter the two known values. The lens and mirror equation calculator applies the correct formula, computes image distance, magnification, and classifies the image as real/virtual and upright/inverted. All calculations run locally in your browser — no signup required.
Optic Type:
Solve for:
Enter the positive distance from object to lens/mirror
Enter the positive focal length magnitude (sign applied automatically for converging lens)
Equation Reference
Lens Equation
1/v − 1/u = 1/f
New Cartesian sign convention
Mirror Equation
1/v + 1/u = 1/f
New Cartesian sign convention
Magnification
m = −v / u (mirrors) | m = v / u (lenses)
m > 0 → upright; m < 0 → inverted
Radius of Curvature
R = 2f
Applies to spherical mirrors
Sign Convention (New Cartesian)
All calculations run locally in your browser. No data is ever sent to a server.
Why Use Our Lens and Mirror Equation Calculator?
Instant Lens and Mirror Equation Calculation
Select the optic type, choose what to solve for, enter two known values, and the lens and mirror equation calculator returns image distance, magnification, and full image classification instantly — no submit button needed.
Secure Lens Mirror Equation Calculator Online
Your values and calculations never leave your device. The lens and mirror equation calculator runs 100% client-side in your browser — no server, no account, no data collection of any kind.
Lens Mirror Equation Calculator — No Installation
Use the lens and mirror equation calculator directly in any modern browser with no downloads, no plugins, and no account required. Works on desktop and mobile — open the page and start solving optics problems immediately.
100% Free with Full Image Classification
The lens and mirror equation calculator is completely free with no signup, no usage limits, and no ads. Every result includes real/virtual classification, upright/inverted orientation, and enlarged/diminished size — all automatically determined.
Common Use Cases for Lens and Mirror Equation Calculator
Physics Homework and Exam Preparation
Students use the lens and mirror equation calculator to solve optics problems from textbooks and past papers. The equation reference panel shows which formula is applied and explains the sign convention, reinforcing understanding alongside worked examples.
Camera and Photography Optics
Photographers and optical engineers use the lens and mirror equation calculator to determine image distance for a given object distance and focal length. This helps in understanding depth of field, focus distance, and lens selection for specific shooting scenarios.
Telescope and Microscope Design
Optical instrument designers use the lens and mirror equation calculator to model the image-forming behaviour of individual lens and mirror elements. Solving for focal length from known object and image distances helps verify design specifications.
Concave Mirror Applications
Engineers working on solar concentrators, satellite dishes, and headlight reflectors use the lens and mirror equation calculator to determine the focal point and image position for concave mirror systems under various object distances.
Convex Mirror Safety Analysis
Traffic engineers and security system designers use the lens and mirror equation calculator to analyse convex mirror coverage. Convex mirrors always produce virtual, upright, diminished images — the calculator confirms this and quantifies the magnification.
Optics Lab Verification
Physics lab students use the lens and mirror equation calculator to verify experimental measurements. By entering measured object and image distances, they can calculate the experimental focal length and compare it to the manufacturer specification.
Understanding the Lens and Mirror Equation
What is the Lens and Mirror Equation?
The lens equation and mirror equation are fundamental formulas in geometric optics that relate three quantities: object distance (u), image distance (v), and focal length (f). For lenses, the equation is 1/v − 1/u = 1/f; for mirrors, it is 1/v + 1/u = 1/f — both using the New Cartesian sign convention. The magnification (m) is defined as m = v/u for lenses and m = −v/u for mirrors, and tells you the size and orientation of the image relative to the object. Our lens and mirror equation calculator online implements all four optic types — converging lens, diverging lens, concave mirror, and convex mirror — and automatically applies the correct sign convention so you only need to enter positive magnitudes.
How Our Lens and Mirror Equation Calculator Works
- Select the Optic Type: Choose from converging lens (convex), diverging lens (concave), concave mirror, or convex mirror. The lens and mirror equation calculator automatically applies the correct sign to the focal length based on your selection — you never need to remember which sign to use.
- Choose What to Solve For: Select image distance, object distance, or focal length as your unknown. Enter the two known values as positive magnitudes (or as signed values for image distance when solving for object distance or focal length). The lens and mirror equation calculator evaluates the formula in real time.
- Read the Full Result: The calculator displays the primary result, all four computed quantities (v, u, f, m), and a complete image classification — real or virtual, upright or inverted, and enlarged, diminished, or same size. All calculations run locally in your browser with no data sent to any server.
What the Lens and Mirror Equation Calculator Computes
- Image Distance (v): The signed distance from the lens or mirror to the image. Positive values indicate a real image on the transmission side of a lens or the reflection side of a mirror; negative values indicate a virtual image.
- Magnification (m):The ratio of image height to object height. A positive magnification means the image is upright; negative means inverted. |m| > 1 means enlarged; |m| < 1 means diminished.
- Image Classification: The calculator automatically determines whether the image is real or virtual, upright or inverted, and enlarged or diminished based on the computed magnification and image distance sign.
- Equation Reference: Every result shows the specific formula used and a sign convention summary, making the lens and mirror equation calculator a useful learning tool alongside textbook problems.
Important Notes About This Calculator
This lens and mirror equation calculator uses the New Cartesian sign convention, which is the most widely used convention in modern physics textbooks. Object distance is always taken as negative (object on the left of the optic), and the sign of the focal length is determined by the optic type — the calculator applies this automatically. The calculator assumes thin lens and spherical mirror approximations, which are valid when the lens thickness and mirror curvature are small compared to the object and image distances. For thick lenses or parabolic mirrors, more advanced ray-tracing methods are required.
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Frequently Asked Questions About Lens and Mirror Equation Calculator
A lens and mirror equation calculator is a tool that solves the thin lens equation (1/v − 1/u = 1/f) and the mirror equation (1/v + 1/u = 1/f) for any unknown — image distance, object distance, or focal length. It also computes magnification and classifies the image as real or virtual, upright or inverted, and enlarged or diminished. Our lens and mirror equation calculator online runs entirely in your browser with no signup, no server, and no data collection.
The lens equation is 1/v − 1/u = 1/f and applies to refracting optics (converging and diverging lenses). The mirror equation is 1/v + 1/u = 1/f and applies to reflecting optics (concave and convex mirrors). Both use the New Cartesian sign convention where object distance is always negative. The lens and mirror equation calculator applies the correct formula automatically based on your optic type selection.
Absolutely. The lens and mirror equation calculator runs 100% client-side in your browser. Your values and calculations are never transmitted to any server, stored in a database, or tracked in any way. Everything stays completely private on your device.
Yes — the lens and mirror equation calculator is 100% free with no signup, no account, and no usage limits. Solve as many optics problems as you need, completely free forever. There are no ads, no premium tiers, and no data collection.
The lens and mirror equation calculator uses the New Cartesian sign convention, which is standard in most modern physics textbooks. Distances are measured from the optical centre (lens) or pole (mirror). Object distance is always negative (object on the left). The sign of the focal length is applied automatically: positive for converging lenses and convex mirrors, negative for diverging lenses and concave mirrors.
In the New Cartesian convention, a positive image distance (v > 0) indicates a real image — one that can be projected on a screen. A negative image distance (v < 0) indicates a virtual image, which cannot be projected and appears to be behind the lens or mirror. The lens and mirror equation calculator determines this automatically and displays the classification clearly.
Magnification (m) is the ratio of image height to object height. A positive magnification means the image is upright (same orientation as the object); a negative magnification means the image is inverted. |m| > 1 means the image is larger than the object (enlarged); |m| < 1 means it is smaller (diminished); |m| = 1 means the image is the same size as the object.
Yes. The lens and mirror equation calculator supports all four optic types: converging lens, diverging lens, concave mirror, and convex mirror. For mirrors, the mirror equation (1/v + 1/u = 1/f) is used automatically. The sign convention for focal length is applied internally — concave mirrors have a negative focal length and convex mirrors have a positive focal length in the New Cartesian convention.
The thin lens equation assumes the lens thickness is negligible compared to the object and image distances, and that all rays are paraxial (close to the optical axis). The mirror equation assumes a spherical mirror with small curvature. For thick lenses, wide-angle optics, or parabolic mirrors, these equations are approximations and more advanced ray-tracing methods are needed for precise results.