The distance between an object and a screen is 100 cm. A lens can produce real image of the object on the screen for two different positions between the screen and the object. The distance between these two positions is 40 cm. Find power of lens

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Published July 6, 2025
Physics
Optics
Geometrical Optics
Lens Formula
Bessel Method

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Detailed Explanation

1. What is happening?

A thin lens makes an image according to the lens formula

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

where

  • ff = focal length of lens,
  • uu = object distance from lens (taken negative in sign convention but we will work with magnitudes here),
  • vv = image distance from lens.

In Bessel's method, the distance between the object and the screen is fixed and called DD.

  • First position of lens: object distance u1u_1, image distance v1v_1.
  • Second position of lens: object distance u2u_2, image distance v2v_2.

Because the lens moves but object and screen stay, we always have

u+v=Du + v = D

for both positions. A nice result from the algebra (derived below) is

f=D2d24Df = \frac{D^2 - d^2}{4D}

where dd is the separation between the two sharp-image positions.

2. Why does that formula work?

  1. Start with u1+v1=Du_1 + v_1 = D and u2+v2=Du_2 + v_2 = D.
  2. Because the lens shifts by dd, one distance gets longer by dd while the other gets shorter by dd.
  3. Multiplying uu and vv for both cases and equating through the lens formula eliminates uu and vv, finally giving the compact relation above.

3. What the student must do in exam

  1. Identify DD (100 cm) and dd (40 cm).
  2. Plug into f=(D2d2)/(4D)f = (D^2 - d^2)/(4D).
  3. Convert ff from cm to metre.
  4. Power PP is 1/f1/f in dioptre (D).

Simple Explanation (ELI5)

Think of it like this

You have a torch (object) at one end of a 1-metre long bench and a white wall (screen) at the other end. You slide a magnifying glass (lens) somewhere in between so that a sharp bright spot of the torch appears on the wall. Surprisingly, you find two spots where the picture becomes sharp. Those two lens positions are 40 cm apart. From just these two distances, we can know how strong the magnifying glass is (its power), just like knowing the size of a cricket bat by two simple measurements.

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Step-by-Step Solution

Step-by-step calculation

Given: D=100 cmD = 100\ \text{cm}, d=40 cmd = 40\ \text{cm}

Formula from Bessel method

f=D2d24Df = \frac{D^2 - d^2}{4D}

Substitute the numbers

f=(100)2(40)24×100f = \frac{(100)^2 - (40)^2}{4 \times 100}

f=100001600400f = \frac{10000 - 1600}{400}

f=8400400f = \frac{8400}{400}

f=21 cmf = 21\ \text{cm}

Convert to metre

f=21 cm=0.21 mf = 21\ \text{cm} = 0.21\ \text{m}

Power of the lens

P=1f(in metre)P = \frac{1}{f\,(\text{in metre})}

P=10.214.76 dioptreP = \frac{1}{0.21} \approx 4.76\ \text{dioptre}

[\boxed{P \approx 4.8\ \text{D}}]

Examples

Example 1

Overhead projector focusing on a cinema screen

Example 2

Autofocus mechanism in DSLR cameras sliding internal lens groups

Example 3

Astronomers measuring telescope objective focal length without removing heavy mirrors

Example 4

Quality control in lens manufacturing where quick focal length check is needed

Visual Representation

References

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