The mirror formula relates the object distance (u), image distance (v), and focal length (f) of a spherical mirror:
This formula is valid for both concave and convex mirrors when the New Cartesian Sign Convention is applied.
Sign Convention Recap
- Distances are measured from the pole (P) of the mirror.
- Distances measured along the direction of incident light are taken as positive.
- Distances measured against the direction of incident light are taken as negative.
- Heights above the principal axis are positive; below are negative.

Geometrical Setup
Consider a concave mirror:
- C = Centre of curvature
- F = Focus
- P = Pole
- Object AB is placed at distance u from P.
- Image A′B′ is formed at distance v from P.
Draw two rays:
- Ray parallel to the principal axis → passes through focus (F).
- Ray through centre of curvature (C) → reflects back along the same path.
These rays intersect at A′, forming the image.
Step‑by‑Step Derivation
Step 1: Similar Triangles
From the ray diagram:
- Triangle ABP (object side) and triangle A′B′P (image side) are similar.
- Triangle A′B′F and triangle ABF are also similar.
Step 2: Ratio Relations
From similarity:
and
Step 3: Express Distances
- PB = u (object distance)
- PB′ = v (image distance)
- PF = f (focal length)
Using geometry:
and
Step 4: Equating Ratios
Since both ratios equal :
Step 5: Simplify
Cross‑multiply:
Divide throughout by :
Final Mirror Formula
This is the mirror formula, valid for both concave and convex mirrors.
Applications
- Concave mirrors: telescopes, headlights, shaving mirrors.
- Convex mirrors: vehicle side mirrors for wider field of view.
- Used in optical instruments to calculate image position without ray diagrams.

Conclusion
The mirror formula is derived using geometry and sign conventions, making it a universal relation for spherical mirrors. At Convex Classes Jaipur, we provide step‑by‑step derivations, diagrams, and solved examples so students can master concepts and score high in exams.



