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Q.(a) Using the necessary ray diagram, derive the mirror formula for a concave mirror.

(b) In the magnified image of a measuring scale (with equidistant markings) lying along the principal axis of a concave mirror, the markings are not equidistant. Explain.
CBSECBSE Class XII Board 2020Subjective· 3mImportance★★★★★
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Figure — The stem explicitly requires 'the necessary ray diagram' to derive the concave-mirror formula, so a labelled r
Figure — The stem explicitly requires 'the necessary ray diagram' to derive the concave-mirror formula, so a labelled r

The mirror formula 1f=1v+1u\frac{1}{f} = \frac{1}{v} + \frac{1}{u} relates object distance, image distance, and focal length for a concave mirror. When a scale lies along the principal axis, different points are at different object distances, producing unequal magnifications—hence non-equidistant image markings.


Part (a): Derivation of the Mirror Formula

The mirror formula connects three fundamental quantities: where you place an object (uu), where its image forms (vv), and the mirror's focal length (ff). The derivation rests on the geometry of similar triangles formed by rays reflecting off the mirror.

The Ray Diagram

Consider a concave mirror with pole PP, principal focus FF, and center of curvature CC. Place an object ABAB on the principal axis with AA on the axis and BB perpendicular to it.

        B'
        |
    F   |   C
----+---+---+----
    |       |
    |       B
    A'      A
    
    P (pole)

Two key rays from point BB:

  1. A ray parallel to the principal axis reflects through FF
  2. A ray through CC reflects back along itself

These rays intersect at B′B', forming the inverted image A′B′A'B'.

Setting up the geometry

Let:

  • Object distance: PA=−uPA = -u (negative by sign convention)
  • Image distance: PA′=−vPA' = -v (negative for real image)
  • Focal length: PF=−fPF = -f (negative for concave mirror)
  • Object height: AB=hAB = h
  • Image height: A′B′=h′A'B' = h' (negative for inverted image)

Step-by-step derivation

  1. Identify similar triangles from the parallel ray

    The incident ray from BB parallel to the axis and its reflected ray through FF create two similar triangles: △ABP\triangle ABP and △A′B′P\triangle A'B'P.

    From similarity:

B′A′BA=PA′PA\frac{B'A'}{BA} = \frac{PA'}{PA}

In terms of our variables:

h′h=vu\frac{h'}{h} = \frac{v}{u}

  1. Identify similar triangles involving the focal point

    Consider the ray through CC. The triangles △B′A′F\triangle B'A'F and △MNF\triangle MNF (where MNMN is the perpendicular from the parallel ray at the mirror surface) are similar.

    More directly, triangles △ABF\triangle ABF and △MPF\triangle MPF (where MM is on the mirror) give us:

B′A′MN=FA′FP\frac{B'A'}{MN} = \frac{FA'}{FP}

Since MN=AB=hMN = AB = h (the incident ray height equals object height):

h′h=v−ff\frac{h'}{h} = \frac{v-f}{f}

  1. Equate the two magnification expressions

    From steps 1 and 2:

vu=v−ff\frac{v}{u} = \frac{v-f}{f}

  1. Cross-multiply and simplify

vf=u(v−f)vf = u(v-f)

vf=uv−ufvf = uv - uf

uf=uv−vfuf = uv - vf

uf=v(u−f)uf = v(u-f)

  1. Divide throughout by uvfuvf

ufuvf=v(u−f)uvf\frac{uf}{uvf} = \frac{v(u-f)}{uvf}

1v=u−fuf\frac{1}{v} = \frac{u-f}{uf}

1v=uuf−fuf\frac{1}{v} = \frac{u}{uf} - \frac{f}{uf}

1v=1f−1u\frac{1}{v} = \frac{1}{f} - \frac{1}{u}

1f=1v+1u\frac{1}{f} = \frac{1}{v} + \frac{1}{u}

This is the mirror formula, valid for all spherical mirrors with appropriate sign conventions.

Tip

Remember: all distances are measured from the pole. For a concave mirror, uu, vv, and ff are all negative for real objects and real images in the standard (New Cartesian) sign convention.


Part (b): Non-equidistant Image Markings

When a measuring scale lies along the principal axis, each marking is at a different distance from the mirror. This creates a fascinating effect.

Why magnification varies along the axis

The linear magnification is given by:

m=−vum = -\frac{v}{u}

Since vv depends on uu through the mirror formula, different object distances produce different image distances—and crucially, different magnifications.

The mathematical reason

Consider two consecutive markings on the scale at distances u1u_1 and u2u_2 from the pole, separated by a small distance Δu=u2−u1\Delta u = u_2 - u_1. …

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