7. Lenses
Complete solutions to the Exercise, with ray diagrams and step-by-step numericals. Maharashtra State Board (Balbharati), Std 10 Science and Technology Part 1.
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Exercise
| Column 1 | Column 2 | Column 3 |
|---|---|---|
| Farsightedness | Far away object can be seen clearly | Convex lens |
| Presbyopia | Problem of old age | Bifocal lens |
| Nearsightedness | Nearby object can be seen clearly | Concave lens |
Explanation:
- Farsightedness (hypermetropia): The eye sees distant objects clearly but not nearby objects. The image of a nearby object forms behind the retina. It is corrected by a convex lens, which converges the rays before they reach the eye.
- Presbyopia: With age, the ciliary muscles lose their ability to change the focal length of the eye lens, and the near point shifts farther away. When a person has both near and far defects, a bifocal lens is used: the upper part is concave (for distant vision) and the lower part is convex (for reading).
- Nearsightedness (myopia): The eye sees nearby objects clearly but distant objects appear indistinct. The image of a distant object forms in front of the retina. It is corrected by a concave lens, which diverges the rays.
Centres of curvature (C₁, C₂), radii of curvature (R₁, R₂), optical centre (O) and principal axis of a convex lens.
Rays parallel to the principal axis meet at the principal focus F₂. The distance OF₂ is the focal length f.
- Centre of curvature (C): The centres of the spheres whose parts form the surfaces of the lens. A lens with two spherical surfaces has two centres of curvature, C1 and C2.
- Radius of curvature (R): The radii R1 and R2 of the spheres whose parts form the surfaces of the lens.
- Principal axis: The imaginary line passing through both centres of curvature.
- Optical centre (O): The point inside the lens on the principal axis, through which light rays pass without changing their path.
- Principal focus (F): Rays parallel to the principal axis, after refraction through a convex lens, meet at a point on the principal axis. This point is the principal focus. A lens has two principal foci, F1 and F2.
- Focal length (f): The distance between the optical centre and the principal focus of the lens.
The object should be kept at 2F1, i.e. at a distance equal to twice the focal length (2f) from the lens.
Object AB at 2F₁ gives a real, inverted image A′B′ of the same size at 2F₂.
The ray BC parallel to the principal axis passes through F2 after refraction. The ray BO through the optical centre goes straight. They meet at B′. So the image A′B′ is formed at 2F2. It is real, inverted and of the same size as the object.
(a) Simple microscope is used for watch repairs.
- The parts of a watch are very small and cannot be seen clearly with the naked eye.
- A simple microscope is a convex lens of small focal length. When a small object is kept between its focus and the lens, it forms a virtual, erect and magnified image.
- So the watch repairer can see the tiny parts clearly in an enlarged form and repair them.
(b) One can sense colours only in bright light.
- The retina has two types of light-sensitive cells: rod-like cells and cone-like (conical) cells.
- Rod cells respond to the intensity of light, even faint light, but they do not give information about colour.
- Conical cells respond to colour, but they work only in bright light, not in faint light.
- Hence we can sense colours only in bright light.
(c) We can not clearly see an object kept at a distance less than 25 cm from the eye.
- The eye lens can change its focal length (power of accommodation), but only up to a limit.
- For a normal eye, the minimum distance of distinct vision (near point) is 25 cm.
- For an object closer than 25 cm, the eye lens cannot become rounded enough to reduce its focal length further. The image forms behind the retina.
- So the object is not seen clearly, even though it subtends a bigger angle at the eye.
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Astronomical telescope: the objective forms a real image at its focus, which the eyepiece magnifies.
- An astronomical (refracting) telescope has two convex lenses: the objective lens and the eyepiece. Their principal axes are along the same straight line, and they are fitted in a metallic tube so that the distance between them can be changed.
- The objective has a large diameter and a large focal length, so it collects maximum light from the distant object.
- Rays from a distant star or planet are nearly parallel. The objective refracts them and forms a real, inverted and small image at its focus.
- This image acts as the object for the eyepiece. It lies at (or just inside) the focus of the eyepiece.
- The eyepiece has a small size and small focal length. It refracts the rays again and forms a magnified final image, which the eye sees.
- With the same objective and different eyepieces, different magnifications can be obtained.
(a) Farsightedness and Nearsightedness
| Point | Farsightedness | Nearsightedness |
|---|---|---|
| Other name | Hypermetropia | Myopia |
| What is seen clearly | Distant objects | Nearby objects |
| Change in near/far point | Near point shifts farther than 25 cm | Far point shifts closer than infinity |
| Image formed | Behind the retina (for nearby objects) | In front of the retina (for distant objects) |
| Causes | Curvature of cornea and lens decreases; eyeball becomes flat (shorter) | Curvature of cornea and lens increases; eyeball elongates |
| Correction | Convex lens (positive power) | Concave lens (negative power) |
(b) Concave lens and Convex Lens
| Point | Concave lens | Convex lens |
|---|---|---|
| Shape | Thinner at the centre, thicker at the edges | Thicker at the centre, thinner at the edges |
| Effect on parallel rays | Diverges them (diverging lens) | Converges them (converging lens) |
| Image | Always virtual, erect and smaller | Real and inverted, or virtual and erect, depending on object position |
| Focal length and power | Negative | Positive |
| Use | Correcting nearsightedness, peep hole, torch | Correcting farsightedness, microscope, telescope, camera |
Iris:
- The iris is a dark, fleshy screen behind the cornea. It has a small hole of changing diameter at its centre, called the pupil.
- The iris controls the size of the pupil and so controls the amount of light entering the eye.
- In bright light, the pupil contracts; in dim light, it widens.
Muscles connected to the lens (ciliary muscles):
- These muscles change the shape, and therefore the focal length, of the eye lens.
- For distant objects, the muscles relax, the lens becomes flat and its focal length increases.
- For nearby objects, the muscles contract, the lens becomes more rounded and its focal length decreases.
- This power of accommodation lets us see objects clearly at different distances.
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(i) Doctor has prescribed a lens having power +1.5 D. What will be the focal length of the lens? What is the type of the lens and what must be the defect of vision?
Given: P = +1.5 D. To find: f
Focal length = +0.67 m. The power and focal length are positive, so it is a convex lens. A convex lens is used to correct farsightedness.
(ii) 5 cm high object is placed at a distance of 25 cm from a converging lens of focal length of 10 cm. Determine the position, size and type of the image.
Given: h1 = 5 cm, u = −25 cm, f = +10 cm (converging lens). To find: v, h2
v = 503 = +16.7 cm
h2h1 = vu ⇒ h2 = 16.7−25 × 5 = −3.3 cm
The image is formed at 16.7 cm on the other side of the lens. Its size is 3.3 cm. v is positive and h2 is negative, so the image is real and inverted (and smaller than the object).
(iii) Three lenses having power 2, 2.5 and 1.7 D are kept touching in a row. What is the total power of the lens combination?
The total power of the combination is 6.2 D.
(iv) An object kept 60 cm from a lens gives a virtual image 20 cm in front of the lens. What is the focal length of the lens? Is it a converging lens or diverging lens?
Given: u = −60 cm. The image is virtual and on the same side as the object, so v = −20 cm. To find: f
f = −30 cm
The focal length is −30 cm. It is negative, so the lens is a diverging (concave) lens.
Suggested slides for the presentation:
- Title: Binoculars — two telescopes side by side, one for each eye.
- Construction: Each half has a convex objective lens (large, collects light), two prisms (fold the light path and make the image erect), and a convex eyepiece (magnifies). A central focusing wheel moves the eyepieces.
- Working: The objective forms a real, inverted image. The prisms turn it upright using total internal reflection. The eyepiece magnifies this image.
- Why prisms: They make the image erect and fold the long light path, so binoculars are short and easy to hold.
- Meaning of “8 × 40”: magnification 8 times, objective diameter 40 mm.
- Uses: bird watching, wildlife viewing, sports events, ships and navy, army, astronomy.
- Advantage over a telescope: both eyes are used, which gives depth (3-D) and less strain.
Add pictures and a labelled diagram of the lens-and-prism arrangement to your slides.