Apply the mirror equation 1/f = 1/u + 1/v for spherical mirrors. Compute image distance, magnification, image type (real/virtual), orientation, and size. Visualize object & image positions with sign convention compliance.
The mirror equation relates object distance u, image distance v, and focal length f for spherical mirrors: 1/f = 1/u + 1/v. Derived from geometry under paraxial approximation, it forms the basis of geometrical optics. The linear magnification m = -v/u determines image size and orientation.
? Sign convention (Cartesian):
• Focal length: Concave → f > 0 | Convex → f < 0
• Object distance u > 0 (real object in front of mirror)
• Image distance v > 0 → real image (in front, inverted)
• v < 0 → virtual image (behind mirror, upright)
Using similar triangles for paraxial rays, the mirror equation emerges independent of mirror curvature to first order. For concave mirrors, the focal point is real (converging); for convex mirrors, the focus is virtual (diverging). This formula accurately predicts image formation for telescopes, shaving mirrors, rearview mirrors, and astronomical instruments.
A concave mirror with focal length 30 cm is used to concentrate sunlight. To produce a highly focused real image (intense spot) at the focal plane, the object (sun) is at infinity → image at focus. For extended objects, the cooker positions the pot near the focus. Our calculator helps determine how image distance changes with object placement, optimizing energy collection.
| Condition | Image Distance (v) | Magnification | Image Properties |
|---|---|---|---|
| Concave, u > 2f | f < v < 2f | |m| < 1, m negative | Real, inverted, diminished |
| Concave, u = 2f | v = 2f | |m| = 1, negative | Real, inverted, same size |
| Concave, f < u < 2f | v > 2f | |m| > 1, negative | Real, inverted, enlarged |
| Concave, u < f | v negative (virtual) | |m| > 1, positive | Virtual, upright, magnified |
| Convex (any u) | v negative, |v| < |f| | 0 < m < 1 | Virtual, upright, diminished |
The mirror equation was formalized by Ibn al-Haytham (Alhazen) in the 11th century and later developed by Kepler and Descartes. Its modern form is taught in every introductory physics course. This interactive tool promotes active learning, aligning with Next Generation Science Standards (NGSS).