A physics class is investigating the magnification produced by a converging lens. An illuminated object of height h0=3.0 cmh_0 = 3.0\text{ cm}h0=3.0 cm is set up. The distance uuu between the illuminated object and the lens is varied, and for each distance, the screen is adjusted until a sharp image of height hIh_{\text{I}}hI is formed. Measurements are recorded in Table 3.1. Table 3.1: | u/cmu / \text{cm}u/cm | hI/cmh_{\text{I}} / \text{cm}hI/cm | S=h0hIS = \frac{h_0}{h_{\text{I}}}S=hIh0 | | :---: | :---: | :---: | | 40.040.040.0 | 3.03.03.0 | | | 45.045.045.0 | 2.42.42.4 | | | 50.050.050.0 | 2.02.02.0 | | | 55.055.055.0 | 1.71.71.7 | | | 60.060.060.0 | 1.51.51.5 | | | 65.065.065.0 | 1.31.31.3 | | | 70.070.070.0 | 1.21.21.2 | |
Calculate the values of SSS for each of the distances uuu, rounding them to one decimal place, to complete Table 3.1.
A graph of SSS (on the yyy-axis) vs u/cmu / \text{cm}u/cm (on the xxx-axis) is plotted, yielding a straight line of best fit.
Determine the gradient GGG of this line using the two extreme points of the data: (40.0,1.0)(40.0, 1.0)(40.0,1.0) and (70.0,2.5)(70.0, 2.5)(70.0,2.5).
Calculate the focal length fff of the lens, where:
f=1G f = \frac{1}{G} f=G1216 exam-style questions on CIE IGCSE Physics 3.2 Light, covering 3.2.1a Reflection of light, 3.2.1b Images in a plane mirror, 3.2.2 Refraction of light, 3.2.2a Refraction of light, 3.2.2b Total internal reflection, 3.2.2c Refractive index and critical angle, 3.2.2d Optical fibres, 3.2.3a Converging and diverging lenses, 3.2.3b Ray diagrams and the nature of images, 3.2.3c Virtual images and the magnifying glass, 3.2.3d Correcting long-sightedness and short-sightedness, and 3.2.4 Dispersion of light. Each one has a worked solution and a mark scheme showing where the marks go.