Thin Lens Calculator
Apply the thin lens equation: 1/f = 1/p + 1/q. Solve for image distance given p and f, or focal length given p and q. Shows magnification.
Thin lens: 1/f = 1/p + 1/p'
The Gauss thin-lens equation links the focal length f, the object distance p and the image distance p': 1/f = 1/p + 1/p'. By convention, f > 0 for converging lenses (biconvex) and f < 0 for diverging lenses (biconcave). The linear magnification is A = -p'/p = i/o — negative means the image is inverted. Vergence (the unit used in eyeglass prescriptions) is V = 1/f in diopters (D), with f in meters. A normal emmetropic eye has about 60 D of refractive power. Example: an object 30 cm from a 10 cm lens gives 1/p' = 1/10 - 1/30 ⇒ p' = 15 cm, A = -0.5 (real, inverted, half size).
Applications
Eyeglasses and contact lenses (myopia uses diverging lenses with negative diopters, hyperopia uses converging with positive diopters, presbyopia after 40, astigmatism adds a cylindrical correction), progressive lenses, cameras (focal length × aperture), microscopes, telescopes (large objectives capture more light), and LASIK surgery, which reshapes the cornea to change its natural focal length.
FAQ
When is the image real or virtual? p' > 0 means a real image (formed on the opposite side, can be projected on a screen); p' < 0 means virtual (same side as the object, only seen through the lens — like a magnifying glass).
What are diopters? The unit of vergence: V = 1/f with f in meters. -2.00 D means a diverging lens with f = -50 cm (typical mild myopia).
Why does the same formula model the human eye? Because the eye behaves like a converging optical system (cornea + lens) projecting onto the retina. Refractive errors arise when the effective focal length doesn't match the eye's length.
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The results provided by this tool are for general informational and educational purposes only and do not constitute professional, financial, medical, legal, tax or accounting advice. Always confirm important decisions with a qualified professional and official sources.