SCIENCE • Form 5 • Chapter 7: Light and Optics
7.2 Optical Instruments
Optical instruments such as magnifying glasses, compound microscopes, and astronomical telescopes use convex lenses to form images suited to their specific functions. The size, orientation, and nature of the images depend on the position of the object relative to the focal point of each lens. Technological developments have also introduced ultra-thin lenses in everyday gadgets such as smartphones, CCTV systems, and DSLR cameras.
Learning Objectives
- Describe the image formation and characteristics of the final image produced by a microscope.
- Calculate the magnifying power of a compound microscope using the magnifying powers of its objective lens and eyepiece.
- Describe the image formation, image characteristics, and normal adjustment condition of an astronomical telescope.
- Explain the applications of lenses in optical instruments including DSLR cameras, CCTV cameras, and spy cameras.
How Optical Instruments Work
Both microscopes and telescopes utilise two convex lenses: an objective lens and an eyepiece. In a microscope, the objective lens forms a real, inverted, magnified image, which is positioned within the focal length of the eyepiece to produce a highly magnified virtual final image. In an astronomical telescope, parallel rays from an object at infinity form a real, inverted, diminished image at \(F_o\). In normal adjustment, \(F_o\) coincides with \(F_e\), making the distance between lenses equal to \(f_o + f_e\), and the eyepiece forms a magnified virtual image at infinity for relaxed viewing.
Formation of the Final Image by a Microscope
A compound microscope consists of two convex lenses: an objective lens and an eyepiece.
1. Objective Lens
Object position: between \(F_o\) and \(2F_o\). First image \(I_o\) position: further than \(2F_o\). First image characteristics: real, inverted, and magnified.
2. Eyepiece
The first image \(I_o\) acts as the object for the eyepiece. Object position: between \(F_e\) and the optical centre \(O\). Final image \(I\) position: further than \(F_e\). Final image characteristics: virtual, upright relative to the first image, and magnified. Relative to the original object, the final image is virtual, inverted, and magnified.
Determining the Magnifying Power of a Microscope
\[\text{Magnifying power of microscope} = \text{Magnifying power of objective lens} \times \text{Magnifying power of eyepiece}\]
Worked example: Eyepiece magnifying power = \(4\text{ times}\), objective lens magnifying power = \(40\text{ times}\). Calculation: \(40 \times 4 = 160\text{ times}\).
Formation of the Final Image by an Astronomical Telescope
A simple astronomical telescope consists of two convex lenses: an objective lens and an eyepiece.
1. Objective Lens
Object position: at infinity, so parallel incident rays arrive from a distant object. First image \(I_o\) position: at the focal point of the objective lens \(F_o\). First image characteristics: real, inverted, and diminished.
2. Eyepiece
The first image \(I_o\) acts as the object for the eyepiece and is positioned at the focal point of the eyepiece \(F_e\). Final image \(I\) position: at infinity. Final image characteristics: virtual, upright relative to the first image, and magnified. Relative to the distant object, the final image is virtual, inverted, and magnified at infinity.
Normal Adjustment
Distance between objective lens and eyepiece = \(f_o + f_e\), where \(f_o\) is the focal length of the objective lens and \(f_e\) is the focal length of the eyepiece. The purpose of normal adjustment is to enable the image at infinity to be viewed comfortably by the human eye.
Activity 7.3: Building a Simple Telescope Model
Materials and apparatus: hollow paper cylinder, cellophane tape, convex lens with focal length \(f_o \ge 10\text{ cm}\), convex lens with focal length \(f_e \le 2\text{ cm}\), ruler, scissors or knife, and pencil. The telescope cylinder must be made of opaque materials, not transparent or translucent, to prevent stray external light from entering and disturbing image clarity. The separation distance between lenses in normal adjustment is \(f_o + f_e\).
Application of Lenses in Modern Optical Instruments
Smartphones & CCTV
Flat lenses with thicknesses of only several microns, where \(1\text{ micron} = 0.001\text{ mm}\), reduce device thickness and size.
DSLR Cameras
Lens focal length directly affects the field of vision. The shorter the focal length of the lens, for example \(24\text{ mm}\), the wider the field of vision. A longer focal length lens, for example \(70\text{ mm}\), produces a narrower field of vision with greater magnification of distant subjects.
Safety & Security Devices
Miniature lenses are used in high-resolution CCTV and spy cameras inside safety devices.
Water Lens
A spherical drop or container of water can act as a convex lens functioning as a magnifying glass under sunlight.