Welcome to practical physicsPracticle physics - practical activities designed for use in the classroom with 11 to 19 year olds

Diffraction of light at a narrow opening


This is a simple and economic demonstration of the diffraction of light by a narrow opening, from which the wavelength of light can be determined.

Apparatus and materials

Diode laser (designed for educational use NOT a key chain laser) Class 2 either 635 mm or 670 mm

Thin aluminium foil (0.1mm thickness available as a sealed wrapper of a milk powder tin)

Stand with clamp

Meter scale

Sharp needle

Travelling microscope

Screen-white graph sheet pasted on cardboard

Health & Safety and Technical notes

The power of a class 2 laser is less than 1 mW. This is not harmful even if it is seen directly: the blink response gives adequate protection. Warning: cheap laser pointers have not been tested and cannot be relied upon to be Class 2.

Keeping the foil over a smooth plane surface, make a small circular hole in it by pressing the needle tip gently into the foil. The rectangular slit can be prepared by using two straight aluminium strips over transparent sticky tape. 



a Arrange the source (laser), aluminium foil with hole, and graph sheet pasted on cardboard as a screen, so that they lie in a straight line. Support the stands with the clamp as shown in the below diagram. 

Light source to screen

b Switch on the source and make fine adjustments so that the aperture in the foil is illuminated evenly. 
c Move the screen about 1 m from the aluminium foil, so that the diffraction pattern is within the graph sheet pasted on the screen.

Fringe pattern

The diffraction fringe pattern will be as shown above. 
d For the calculation of the wavelength of the source used: 

  • Note down the diameter of the first minimum, Y , with the help of graph sheet markings.  
  • Note the distance between the foil and the screen, D. 
  • Using a travelling microscope, measure the diameter of the hole or slit width used, X. 
  • Calculate the wavelength of the light source, λ, using the formula λ = XY/ 2D.

Teaching notes

1 Derivation 

Let S1S2 be the diameter of the hole, acting like secondary coherent sources. 

Secondary wave fronts coming from these undergo superposition (interference), leading to bright and dark fringes on the screen. 

First min and central max

The ray diagram is shown above. 
MN is the path difference between S1P’ & MP, where P is the centre of the first minimum and O is the centre of central maximum. 
Then MN = λ /2 ,…………………….(1) 
From triangle S1NM, sinӨ = MN/S1M = MN / (X/2), or MN = (X/2) sinӨ……………………(2) 
From triangle OMP, sinӨ = PO /MP ≈ Y1/ OM = Y1/ D………………………..(3), 
From (1),(2) &(3) 
Y1/ D = λ / X, or λ = X (2Y1) / 2D =XY/ 2D where the diameter of the first minimum, Y = 2Y1 
Hence λ =XY/ 2D 
Experimental results conducted at physics lab CMRIT BANGALORE: 

circular hole

For circular hole, X = 0. 018 cm, For rectangular slit, X = 0. 021 cm 
D = 177 cm, D = 215 cm 
Measured Y =1. 3 cm, Y =1. 35 cm 
will give 659 nm< λ <661 nm 
This is similar to the λ calculated by a diffraction grating experiment, at 653 nm. 

Actual diffection pattern

Actual diffraction pattern recorded by 3.1 Mega pixel digital camera, in the dark room is shown above. 

This experiment was submitted by Tukaram Shet, Senior Lecturer in Physics at CMRIT Bangalore.


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