Ray Optics and Optical Instruments NCERT Solutions are highly useful for students preparing for the Class 12 Physics board examination.
With the CBSE Class 12 Physics exam scheduled on 20th February 2026, this chapter becomes a must-revise topic due to its high weightage and scoring numericals. Ray Optics carries around 10 marks, making it an important contributor to the overall 80-mark theory paper.
As the board exams are approaching, focused practice and strong conceptual clarity are essential to avoid mistakes in numericals and ray diagrams. NCERT Solutions class 12 Chapter 9 Ray Optics and Optical Instruments help students revise efficiently by providing step-by-step solutions, accurate ray diagrams, and well-structured, exam-oriented answers aligned with the CBSE marking scheme.
Ray Optics NCERT Solutions for Class 12 Physics
Ray Optics NCERT Solutions are given here to help students understand reflection, refraction, total internal reflection, and optical instruments easily.
The solutions explain each concept clearly and focus on formula application, numerical problem-solving, and diagram-based answers, which are frequently asked in board exams. These solutions are especially useful for last-minute revision, helping students avoid common mistakes and improve speed and accuracy.
Physics Chapter 9 Ray Optics and Optical Instruments
NCERT Solutions for Chapter 9 Ray Optics and Optical Instruments provide complete coverage of all textbook questions, including derivations, ray diagrams, and numericals. Each solution follows the CBSE marking scheme, helping students understand how to present answers correctly to score full marks.
Class 12 Ray Optics and Optical Instruments NCERT Solutions (All Exercises)
Here are the questions along with the answers given at the end of the chapter. Students must understand each numerical and practice them thoroughly for CBSE Class 12th Physics Board exam:
Question 1. A small candle, 2.5 cm in size is placed at 27 cm in front of a concave mirror of radius of curvature 36 cm. At what distance from the mirror should a screen be placed in order to obtain a sharp image? Describe the nature and size of the image. If the candle is moved closer to the mirror, how would the screen have to be moved?
Solution : Size of the candle, h= 2.5 cm Image size = h’ Object distance, u= −27 cm Radius of curvature of the concave mirror, R= −36 cm Focal length of the concave mirror,
Image distance = v The image distance can be obtained using the mirror formula:
Therefore, the screen should be placed 54 cm away from the mirror to obtain a sharp image. The magnification of the image is given as:
The height of the candle’s image is 5 cm. The negative sign indicates that the image is inverted and real. If the candle is moved closer to the mirror, then the screen will have to be moved away from the mirror in order to obtain the image.
(b) An object 1.5 cm in size is placed on the side of the convex lens in the arrangement (a) above. The distance between the object and the convex lens is 40 cm. Determine the magnification produced by the two-lens system, and the size of the image.
Solution : Focal length of the convex lens, f1 = 30 cm Focal length of the concave lens, f2 = −20 cm Distance between the two lenses, d = 8.0 cm (a) When the parallel beam of light is incident on the convex lens first: According to the lens formula, we have:
Where,
= Object distance = ∞ v1 = Image distance
The image will act as a virtual object for the concave lens. Applying lens formula to the concave lens, we have:
Where,
= Object distance = (30 − d) = 30 − 8 = 22 cm
= Image distance
The parallel incident beam appears to diverge from a point that is
from the centre of the combination of the two lenses.
(ii) When the parallel beam of light is incident, from the left, on the concave lens first: According to the lens formula, we have:
Where,
= Object distance = −∞
= Image distance
The image will act as a real object for the convex lens. Applying lens formula to the convex lens, we have:
Where,
= Object distance = −(20 + d) = −(20 + 8) = −28 cm
= Image distance
Hence, the parallel incident beam appear to diverge from a point that is (420 − 4) 416 cm from the left of the centre of the combination of the two lenses. The answer does depend on the side of the combination at which the parallel beam of light is incident. The notion of effective focal length does not seem to be useful for this combination.
(b) Height of the image, h1 = 1.5 cm Object distance from the side of the convex lens,
According to the lens formula:
Where,
= Image distance
Magnification,
Hence, the magnification due to the convex lens is 3. The image formed by the convex lens acts as an object for the concave lens.
According to the lens formula:
Where,
= Object distance = +(120 − 8) = 112 cm.
= Image distance
Magnification,
Hence, the magnification due to the concave lens is
.
The magnification produced by the combination of the two lenses is calculated as:
The magnification of the combination is given as:
Where, h1 = Object size = 1.5 cm h2 = Size of the image
Hence, the height of the image is 0.98 cm.
Question 21. At what angle should a ray of light be incident on the face of a prism of refracting angle 60° so that it just suffers total internal reflection at the other face? The refractive index of the material of the prism is 1.524.
Solution : The incident, refracted, and emergent rays associated with a glass prism ABC are shown in the given figure.
Angle of prism, ∠A = 60° Refractive index of the prism, µ = 1.524
= Incident angle
= Refracted angle
= Angle of incidence at the face AC e = Emergent angle = 90° According to Snell’s law, for face AC, we can have:
It is clear from the figure that angle
According to Snell’s law, we have the relation:
Hence, the angle of incidence is 29.75°.
Question 22. A card sheet divided into squares each of size 1 mm2 is being viewed at a distance of 9 cm through a magnifying glass (a converging lens of focal length 9 cm) held close to the eye. (a) What is the magnification produced by the lens? How much is the area of each square in the virtual image? (b) What is the angular magnification (magnifying power) of the lens? (c) Is the magnification in (a) equal to the magnifying power in (b)? Explain.
Solution : Note : Here we took focal Length as 10 cm because if we take it as 9 cm then image distance will be zero ,which does not make any sense. (a) Area of each square, A = 1 mm2 Object distance, u = −9 cm Focal length of a converging lens, f = 9 cm For image distance v, the lens formula can be written as:
Magnification,
∴Area of each square in the virtual image = (10)2A = 102 × 1 = 100 mm2 = 1 cm2 (b) Magnifying power of the lens
(c) The magnification in (a) is not the same as the magnifying power in (b). The magnification magnitude is
and the magnifying power is
. The two quantities will be equal when the image is formed at the near point (25 cm).
Question 23. (a) At what distance should the lens be held from the figure in Exercise 9.29 in order to view the squares distinctly with the maximum possible magnifying power?
(b) What is the magnification in this case?
(c) Is the magnification equal to the magnifying power in this case? Explain.
Solution : (a) The maximum possible magnification is obtained when the image is formed at the near point (d = 25 cm). Image distance, v = −d = −25 cm Focal length, f = 10 cm Object distance = u According to the lens formula, we have:
Hence, to view the squares distinctly, the lens should be kept 7.14 cm away from them. (b) Magnification =
(c) Magnifying power =
Since the image is formed at the near point (25 cm), the magnifying power is equal to the magnitude of magnification.
Question 24. What should be the distance between the object in Exercise 9.23 and the magnifying glass if the virtual image of each square in the figure is to have an area of 6.25 mm2
. Would you be able to see the squares distinctly with your eyes very close to the magnifier?
Solution : Area of the virtual image of each square, A = 6.25 mm2 Area of each square, A0 = 1 mm2 Hence, the linear magnification of the object can be calculated as:
Focal length of the magnifying glass, f = 10 cm According to the lens formula, we have the relation:
The virtual image is formed at a distance of 15 cm, which is less than the near point (i.e., 25 cm) of a normal eye. Hence, it cannot be seen by the eyes distinctly.
Question 25. Answer the following questions:
(a) The angle subtended at the eye by an object is equal to the angle subtended at the eye by the virtual image produced by a magnifying glass. In what sense then does a magnifying glass provide angular magnification?
(b) In viewing through a magnifying glass, one usually positions one’s eyes very close to the lens. Does angular magnification change if the eye is moved back?
(c) Magnifying power of a simple microscope is inversely proportional to the focal length of the lens. What then stops us from using a convex lens of smaller and smaller focal length and achieving greater and greater magnifying power?
(d) Why must both the objective and the eyepiece of a compound microscope have short focal lengths?
(e) When viewing through a compound microscope, our eyes should be positioned not on the eyepiece but a short distance away from it for best viewing. Why? How much should be that short distance between the eye and eyepiece?
Solution : (a)Though the image size is bigger than the object, the angular size of the image is equal to the angular size of the object. A magnifying glass helps one see the objects placed closer than the least distance of distinct vision (i.e., 25 cm). A closer object causes a larger angular size. A magnifying glass provides angular magnification. Without magnification, the object cannot be placed closer to the eye. With magnification, the object can be placed much closer to the eye.
(b) Yes, the angular magnification changes. When the distance between the eye and a magnifying glass is increased, the angular magnification decreases a little. This is because the angle subtended at the eye is slightly less than the angle subtended at the lens. Image distance does not have any effect on angular magnification.
(c) The focal length of a convex lens cannot be decreased by a greater amount. This is because making lenses having very small focal lengths is not easy. Spherical and chromatic aberrations are produced by a convex lens having a very small focal length.
(d) The angular magnification produced by the eyepiece of a compound microscope is
Where, fe = Focal length of the eyepiece It can be inferred that if fe is small, then angular magnification of the eyepiece will be large. The angular magnification of the objective lens of a compound microscope is given as
Where,
= Object distance for the objective lens
= Focal length of the objective The magnification is large when
>
. In the case of a microscope, the object is kept close to the objective lens. Hence, the object distance is very little. Since
is small,
will be even smaller. Therefore,
and
are both small in the given condition.
(e)When we place our eyes too close to the eyepiece of a compound microscope, we are unable to collect much refracted light. As a result, the field of view decreases substantially. Hence, the clarity of the image gets blurred. The best position of the eye for viewing through a compound microscope is at the eye-ring attached to the eyepiece. The precise location of the eye depends on the separation between the objective lens and the eyepiece.
Question 26. An angular magnification (magnifying power) of 30X is desired using an objective of focal length 1.25 cm and an eyepiece of focal length 5 cm. How will you set up the compound microscope?
Solution : Focal length of the objective lens,
= 1.25 cm Focal length of the eyepiece, fe = 5 cm Least distance of distinct vision, d = 25 cm Angular magnification of the compound microscope = 30X Total magnifying power of the compound microscope, m = 30 The angular magnification of the eyepiece is given by the relation:
The angular magnification of the objective lens (mo) is related to me as:
= m
Applying the lens formula for the objective lens:
The object should be placed 1.5 cm away from the objective lens to obtain the desired magnification. Applying the lens formula for the eyepiece:
Where,
= Image distance for the eyepiece = −d = −25 cm
= Object distance for the eyepiece
Separation between the objective lens and the eyepiece
Therefore, the separation between the objective lens and the eyepiece should be 11.67 cm.
Question 27. A small telescope has an objective lens of focal length 140 cm and an eyepiece of focal length 5.0 cm. What is the magnifying power of the telescope for viewing distant objects when (a) the telescope is in normal adjustment (i.e., when the final image is at infinity)? (b) the final image is formed at the least distance of distinct vision (25 cm)? Solution : Focal length of the objective lens,
= 140 cm Focal length of the eyepiece, fe = 5 cm Least distance of distinct vision, d = 25 cm (a) When the telescope is in normal adjustment, its magnifying power is given as:
(b) When the final image is formed at d,the magnifying power of the telescope is given as:
Question 28. (a) For the telescope described in Exercise 9.34 (a), what is the separation between the objective lens and the eyepiece?
(b) If this telescope is used to view a 100 m tall tower 3 km away, what is the height of the image of the tower formed by the objective lens?
(c) What is the height of the final image of the tower if it is formed at 25 cm?
Solution : Focal length of the objective lens, fo = 140 cm Focal length of the eyepiece, fe = 5 cm (a) In normal adjustment, the separation between the objective lens and the eyepiece
(b) Height of the tower, h1 = 100 m Distance of the tower (object) from the telescope, u = 3 km = 3000 m The angle subtended by the tower at the telescope is given as:
The angle subtended by the image produced by the objective lens is given as:
Where, h2 = Height of the image of the tower formed by the objective lens
Therefore, the objective lens forms a 4.7 cm tall image of the tower. (c) Image is formed at a distance, d = 25 cm The magnification of the eyepiece is given by the relation:
Height of the final image
Hence, the height of the final image of the tower is 28.2 cm.
Question 29. A Cassegrain telescope uses two mirrors as shown in Fig. 9.33. Such a telescope is built with the mirrors 20 mm apart. If the radius of curvature of the large mirror is 220 mm and the small mirror is 140 mm, where will the final image of an object at infinity be?
Solution : The following figure shows a Cassegrain telescope consisting of a concave mirror and a convex mirror.
Distance between the objective mirror and the secondary mirror, d = 20 mm Radius of curvature of the objective mirror, R1 = 220 mm Hence, focal length of the objective mirror,
Radius of curvature of the secondary mirror, R1 = 140 mm Hence, focal length of the secondary mirror,
The image of an object placed at infinity, formed by the objective mirror, will act as a virtual object for the secondary mirror. Hence, the virtual object distance for the secondary mirror,
Applying the mirror formula for the secondary mirror, we can calculate image distance (v)as:
Hence, the final image will be formed 315 mm away from the secondary mirror.
Question 30. Light incident normally on a plane mirror attached to a galvanometer coil retraces backwards as shown in Fig. 9.36. A current in the coil produces a deflection of 3.5° of the mirror. What is the displacement of the reflected spot of light on a screen placed 1.5 m away?
Solution : Angle of deflection, θ = 3.5° Distance of the screen from the mirror, D = 1.5 m The reflected rays get deflected by an amount twice the angle of deflection i.e., 2θ= 7.0° The displacement (d) of the reflected spot of light on the screen is given as:
Hence, the displacement of the reflected spot of light is 18.4 cm.
Ray Optics Class 12 Important Concepts Explained
Along with the Exercise-Wise NCERT Solutions for Chapter 9, students should also learn about these important concepts included in the chapter:
What is Reflection of Light?
Reflection of light deals with the bouncing back of light rays from reflecting surfaces such as plane and spherical mirrors. Image formation is explained using ray diagrams and mirror formulae.
What is Refraction of Light?
Refraction is the bending of light when it passes from one medium to another due to a change in its speed. Laws of refraction and refractive index play a key role in solving numerical problems.
What is the use of Optical Instruments?
Optical instruments such as microscopes and telescopes use lenses and mirrors to produce magnified images. Their working is explained using ray diagrams and magnification formulae.