Derivation of Mirror Formula | Convex Classes Jaipur
Derivation of Mirror Formula | Convex Classes Jaipur
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Derivation of Mirror Formula | Convex Classes Jaipur

by | Jan 10, 2026 | 0 comments

The mirror formula relates the object distance (u), image distance (v), and focal length (f) of a spherical mirror:

1f=1v+1u

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.
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iit 2026

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:

  1. Ray parallel to the principal axis → passes through focus (F).
  2. 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:

ABAB=PBPB

and

ABAB=FBFB

Step 3: Express Distances

  • PB = u (object distance)
  • PB′ = v (image distance)
  • PF = f (focal length)

Using geometry:

PBPB=uv

and

FBFB=uff

Step 4: Equating Ratios

Since both ratios equal ABAB:

uv=uff

Step 5: Simplify

Cross‑multiply:

uf=v(uf)

uf=uvvf

uvuf=vf

Divide throughout by uvf:

1f=1v+1u

Final Mirror Formula

1f=1v+1u

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.
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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.

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