NCERT Solutions Class 12 Physics Chapter 9 Ray Optics and Optical Instruments
Ray Optics and Optical Instruments explains reflection, refraction, total internal reflection and image formation through mirrors, lenses and prisms.
These NCERT Solutions help students solve Chapter 9 numericals on mirror formula, lens formula, prisms, microscopes and telescopes.
Class 12 Physics Chapter 9 Ray Optics and Optical Instruments becomes easier when students track signs carefully. A concave mirror question needs the mirror formula. A lens combination needs object-image positions after each lens. A prism question depends on minimum deviation. Microscope and telescope questions use angular magnification, focal length and tube length. NCERT Solutions Class 12 Physics Chapter 9 help students solve all 31 textbook questions with clear substitutions, final answers and short reasoning for 2026-27 board practice.
Key Takeaways
- Mirror formula: Use 1/v + 1/u = 1/f with Cartesian sign convention.
- Lens formula: Use 1/v - 1/u = 1/f for thin lenses.
- Total internal reflection: It occurs when light travels from denser to rarer medium above critical angle.
- Optical instruments: Microscope and telescope magnification depends on focal lengths and final image position.
NCERT Solutions Class 12 Physics Chapter 9 Structure 2026-27
| Exercise Area | Main Formula | Question Range |
| Mirrors and refraction | Mirror formula, Snell’s law, apparent depth | 9.1 to 9.6 |
| Lenses and combinations | Lens formula, lens maker’s formula, power | 9.7 to 9.20 |
| Optical instruments | Microscope, telescope, magnifying glass | 9.21 to 9.31 |
Exercises
The NCERT exercise for Class 12 Physics Chapter 9 Ray Optics and Optical Instruments covers ray diagrams, numerical substitutions and optical instruments. These Ray Optics and Optical Instruments Class 12 questions and answers help students solve mirror, lens, prism, microscope and telescope problems with correct sign convention.
These NCERT Solutions for Class 12 Physics Chapter 9 Ray Optics and Optical Instruments follow the textbook exercise order. Each numerical solution keeps the formula, substitution and final answer readable for revision.
Q9.1 A 2.5 cm candle is placed 27 cm before a concave mirror of radius 36 cm.
Answer: The screen should be placed 54 cm in front of the mirror.
Given:
Radius of curvature = 36 cm
Focal length, f = -18 cm
Object distance, u = -27 cm
Object height, h = 2.5 cm
Formula:
1/v + 1/u = 1/f
Substitution:
1/v + 1/(-27) = 1/(-18)
So,
1/v = -1/18 + 1/27
1/v = -1/54
Therefore,
v = -54 cm
Magnification:
m = -v/u
m = -(-54)/(-27) = -2
Image height:
h' = m × h
h' = -2 × 2.5 = -5 cm
The image is real, inverted and 5 cm high.
If the candle moves closer to the mirror, the screen must be moved away until the object reaches focus.
At focus, the image forms at infinity.
Q9.2 A 4.5 cm needle is placed 12 cm from a convex mirror of focal length 15 cm.
Answer: The image is formed 6.67 cm behind the mirror.
Given:
u = -12 cm
f = +15 cm
h = 4.5 cm
Formula:
1/v + 1/u = 1/f
Substitution:
1/v - 1/12 = 1/15
So,
1/v = 1/15 + 1/12
1/v = 9/60
Therefore,
v = 6.67 cm
Magnification:
m = -v/u
m = -6.67/(-12) = 0.56
Image height:
h' = 0.56 × 4.5 = 2.5 cm
The image is virtual, erect and diminished.
As the needle moves farther, the image shifts towards the focus.
Its size keeps decreasing.
Q9.3 A tank has water height 12.5 cm. Apparent depth is 9.4 cm.
Answer: The refractive index of water is 1.33.
Formula:
Refractive index = Real depth / Apparent depth
Substitution:
n = 12.5 / 9.4
n = 1.33
For liquid of refractive index 1.63:
Apparent depth = 12.5 / 1.63
Apparent depth = 7.67 cm
Microscope shift:
9.4 - 7.67 = 1.73 cm
The microscope must be moved 1.73 cm upward.
Q9.4 Predict angle of refraction in glass for water-glass interface.
Answer: The angle of refraction in glass is less than 45°.
Use Snell’s law:
n_water sin 45° = n_glass sin r
Since glass is optically denser than water, the ray bends towards the normal.
Therefore, r < 45°.
The exact value depends on refractive indices obtained from the textbook figure.
Q9.5 A bulb is at the bottom of an 80 cm deep water tank.
Answer: Light emerges through an area of about 2.61 × 10⁴ cm².
Given:
Depth = 80 cm
Refractive index of water = 1.33
Critical angle:
sin ic = 1/1.33
ic = 48.75°
Radius of circular area:
r = h tan ic
r = 80 × tan 48.75°
r = 91.23 cm
Area:
A = πr²
A = 3.14 × (91.23)²
A ≈ 2.61 × 10⁴ cm²
Q9.6 A prism has angle 60° and minimum deviation 40°.
Answer: The refractive index of the prism material is 1.53.
Formula:
n = sin[(A + Dm)/2] / sin(A/2)
Given:
A = 60°
Dm = 40°
Substitution:
n = sin 50° / sin 30°
n = 0.766 / 0.5
n = 1.53
When placed in water:
Relative refractive index:
n_relative = 1.53 / 1.33 = 1.15
Now,
1.15 = sin[(60 + Dm)/2] / sin 30°
sin[(60 + Dm)/2] = 0.575
So,
(60 + Dm)/2 ≈ 35.17°
Dm ≈ 10.34°
The new minimum deviation is about 10.3°.
Q9.7 Double-convex lenses use glass of refractive index 1.55. Focal length is 20 cm.
Answer: Required radius of curvature is 22 cm for each face.
For an equiconvex lens:
R1 = R and R2 = -R
Lens maker’s formula:
1/f = (n - 1)(1/R1 - 1/R2)
So,
1/f = (n - 1)(2/R)
Therefore,
R = 2f(n - 1)
Substitution:
R = 2 × 20 × 0.55
R = 22 cm
Q9.8 A convergent beam would meet at P. A lens is placed 12 cm before P.
(a) Convex lens of focal length 20 cm
Answer: The beam converges 7.5 cm beyond the lens.
Here, the point P acts as a virtual object.
u = +12 cm, f = +20 cm
Formula:
1/v - 1/u = 1/f
So,
1/v = 1/20 + 1/12
v = 7.5 cm
(b) Concave lens of focal length 16 cm
Answer: The beam converges 48 cm beyond the lens.
Given:
u = +12 cm, f = -16 cm
Formula:
1/v = 1/f + 1/u
1/v = -1/16 + 1/12
v = 48 cm
Q9.9 A 3 cm object is placed 14 cm before a concave lens of focal length 21 cm.
Answer: The image forms 8.4 cm in front of the lens.
Given:
u = -14 cm
f = -21 cm
h = 3 cm
Formula:
1/v - 1/u = 1/f
So,
1/v + 1/14 = -1/21
1/v = -1/21 - 1/14
v = -8.4 cm
Magnification:
m = v/u
m = -8.4 / -14 = 0.6
Image height:
h' = 0.6 × 3 = 1.8 cm
The image is virtual, erect and diminished.
If the object moves farther, the image moves closer to focus.
Q9.10 Convex lens of focal length 30 cm touches concave lens of focal length 20 cm.
Answer: The combination has focal length -60 cm.
Formula:
1/F = 1/f1 + 1/f2
Given:
f1 = +30 cm
f2 = -20 cm
Substitution:
1/F = 1/30 - 1/20
1/F = -1/60
Therefore,
F = -60 cm
The system is a diverging lens.
Q9.11 Compound microscope has objective 2 cm, eyepiece 6.25 cm, separation 15 cm.
(a) Final image at least distance of distinct vision
Answer: Object should be placed 2.5 cm before the objective.
For eyepiece:
ve = -25 cm, fe = 6.25 cm
Using lens formula:
ue = -5 cm
So, objective image distance:
vo = 15 - 5 = 10 cm
For objective:
1/vo - 1/uo = 1/fo
1/10 - 1/uo = 1/2
uo = -2.5 cm
Objective magnification:
mo = vo/uo = 10/(-2.5) = -4
Eyepiece magnification:
me = 1 + D/fe
me = 1 + 25/6.25 = 5
Total magnification:
m = -4 × 5 = -20
Magnifying power is 20.
(b) Final image at infinity
Answer: Object should be placed about 2.59 cm before the objective.
For final image at infinity:
ue = -fe = -6.25 cm
Objective image distance:
vo = 15 - 6.25 = 8.75 cm
For objective:
1/8.75 - 1/uo = 1/2
uo = -2.59 cm
Objective magnification:
mo = 8.75 / -2.59 = -3.375
Eyepiece magnification:
me = D/fe = 25/6.25 = 4
Total magnification:
m = -3.375 × 4 = -13.5
Magnifying power is 13.5.
Q9.12 Compound microscope has objective 8 mm and eyepiece 2.5 cm.
Answer: Separation is about 9.47 cm for final image at near point.
Given:
fo = 8 mm = 0.8 cm
fe = 2.5 cm
uo = -9 mm = -0.9 cm
For objective:
1/vo - 1/uo = 1/fo
vo = 7.2 cm
For eyepiece at near point:
ve = -25 cm
Using lens formula:
ue = -2.27 cm
Separation:
7.2 + 2.27 = 9.47 cm
Objective magnification:
mo = 7.2 / -0.9 = -8
Eyepiece magnification:
me = 1 + 25/2.5 = 11
Total magnification:
m = -8 × 11 = -88
Magnifying power is 88.
Q9.13 Telescope has objective 144 cm and eyepiece 6 cm.
Answer: Magnifying power is 24.
Formula:
m = fo / fe
Substitution:
m = 144 / 6 = 24
Separation in normal adjustment:
fo + fe = 144 + 6 = 150 cm
The separation is 150 cm.
Q9.14 Giant refracting telescope has objective focal length 15 m.
(a) Eyepiece focal length is 1 cm.
Answer: Angular magnification is 1500.
Convert:
fe = 1 cm = 0.01 m
Formula:
m = fo / fe
m = 15 / 0.01 = 1500
(b) Diameter of moon’s image
Answer: Diameter is about 0.137 m, or 13.7 cm.
Formula:
Image diameter = fo × Angular diameter
Angular diameter:
Moon diameter / Lunar orbit radius
= 3.48 × 10⁶ / 3.8 × 10⁸
Image diameter:
= 15 × 3.48 × 10⁶ / 3.8 × 10⁸
= 0.137 m
Q9.15 Use mirror equation to deduce image properties.
(a) Object between f and 2f of concave mirror
Answer: Image forms beyond 2f.
For concave mirror, f < 0.
If object lies between f and 2f, solving mirror formula gives v < -2f.
So, the image is real, inverted and enlarged.
(b) Convex mirror always gives virtual image
Answer: A convex mirror has positive focal length.
For any real object, u < 0 and f > 0.
The mirror formula gives v > 0.
So, the image always forms behind the mirror.
(c) Convex mirror image is diminished and between pole and focus
Answer: For convex mirror, v is positive and less than f.
So, the image lies between pole and focus.
Also, m = -v/u is positive and less than 1.
Hence, the image is erect and diminished.
(d) Object between pole and focus of concave mirror
Answer: The image is virtual and enlarged.
Here, u is less than focal length in magnitude.
The mirror formula gives v > 0.
So, the image forms behind the mirror.
Magnification is positive and greater than 1.
Q9.16 A pin is viewed through 15 cm glass slab of refractive index 1.5.
Answer: The pin appears raised by 5 cm.
Formula:
Apparent shift = t(1 - 1/n)
Given:
t = 15 cm, n = 1.5
Substitution:
Shift = 15(1 - 1/1.5)
Shift = 15(1 - 2/3)
Shift = 5 cm
The answer does not depend on the slab’s location.
It depends on slab thickness and refractive index.
Q9.17 Light pipe has core refractive index 1.68 and covering refractive index 1.44.
(a) With outer covering
Answer: Incident ray angle with pipe axis must be less than about 59°.
For core-covering boundary:
sin ic = 1.44 / 1.68
ic ≈ 59°
For total internal reflection, angle at boundary must exceed this critical angle.
The accepted cone depends on the angle made by ray with the pipe axis.
(b) Without outer covering
Answer: Total internal reflection becomes easier.
Now, outer medium is air.
sin ic = 1 / 1.68
ic ≈ 36.5°
A wider range of incident rays can undergo total internal reflection.
Q9.18 Image of bulb must form on opposite wall 3 m away.
Answer: Maximum focal length is 75 cm.
For real image formation on a screen:
u + v = 300 cm
Maximum focal length occurs when:
u = v = 150 cm
Then,
f = uv / (u + v)
f = 150 × 150 / 300
f = 75 cm
Q9.19 Screen is 90 cm from object. Two lens positions differ by 20 cm.
Answer: Focal length is about 21.39 cm.
Formula:
f = (D² - d²) / 4D
Given:
D = 90 cm
d = 20 cm
Substitution:
f = (90² - 20²) / (4 × 90)
f = (8100 - 400) / 360
f = 7700 / 360
f = 21.39 cm
Q9.20 Lenses from Q9.10 are placed 8 cm apart.
(a) Effective focal length
Answer: From the convex-lens side, image forms 212 cm to the left of the convex lens.
For parallel light entering convex lens first:
Convex lens alone would focus at 30 cm.
The concave lens is 8 cm away.
So, for second lens:
u = +22 cm, f = -20 cm
Using lens formula:
1/v = 1/f + 1/u
1/v = -1/20 + 1/22
v = -220 cm
This is 220 cm to the left of concave lens.
So, it is 212 cm to the left of convex lens.
The answer depends on the side of incidence.
So, a single effective focal length is not very useful here.
(b) Object is 1.5 cm high and 40 cm before convex lens.
Answer: Final magnification is about 0.65.
For first lens:
u1 = -40 cm, f1 = +30 cm
v1 = 120 cm
Distance from second lens:
120 - 8 = 112 cm
For second lens:
u2 = +112 cm, f2 = -20 cm
v2 = -24.35 cm
Magnification:
m1 = 120 / -40 = -3
m2 = -24.35 / 112 = -0.217
Total magnification:
m = (-3)(-0.217) = 0.65
Image size:
h' = 0.65 × 1.5 = 0.98 cm
The final image is erect and smaller than the object.
Q9.21 Prism has refracting angle 60° and refractive index 1.524.
Answer: Angle of incidence should be about 29.7°.
At second face, total internal reflection just occurs.
Critical angle:
sin ic = 1/1.524
ic ≈ 41.0°
Inside prism:
r1 + r2 = A
r1 = 60° - 41°
r1 = 19°
At first face:
sin i = n sin r1
sin i = 1.524 × sin 19°
i ≈ 29.7°
Q9.22 A card sheet is viewed at 9 cm through a lens of focal length 9 cm.
(a) Magnification and area
Answer: The image forms at infinity.
Since the object is at focus, linear image size is not finite.
So, absolute area magnification cannot be assigned.
(b) Angular magnification
Answer: Angular magnification is 2.78.
Formula:
m = D/f
m = 25/9
m = 2.78
(c) Are both magnifications equal?
Answer: No.
Linear magnification compares actual sizes.
Angular magnification compares visual angles at the eye.
Q9.23 Maximum magnifying power with same magnifying glass.
(a) Lens position
Answer: The lens should be held about 6.62 cm from the card.
For maximum magnifying power, final image forms at near point.
Given:
v = -25 cm, f = 9 cm
Using lens formula:
1/v - 1/u = 1/f
u = -6.62 cm
(b) Magnification
Answer: Magnification is 3.78.
Formula:
m = v/u
m = (-25)/(-6.62)
m = 3.78
(c) Is magnification equal to magnifying power?
Answer: Yes, for near-point viewing with the eye close to the lens.
Both describe the same apparent enlargement in this setup.
Q9.24 Virtual image area is 6.25 mm².
Answer: Object should be 5.4 cm from the lens.
Object square area = 1 mm²
Image area = 6.25 mm²
Linear magnification:
m = √6.25 = 2.5
Using lens formula with v/u = 2.5:
u = f(1/m - 1)
u = 9(1/2.5 - 1)
u = -5.4 cm
Image distance:
v = 2.5u
v = -13.5 cm
The final image is at 13.5 cm.
So, it cannot be seen distinctly by a normal eye close to the lens.
Q9.25 Answer the conceptual questions.
(a) How does a magnifying glass give angular magnification?
Answer: It lets the object be kept closer than 25 cm.
This increases the angle subtended at the eye.
So, the image appears larger.
(b) Does angular magnification change if eye moves back?
Answer: Yes, it may change slightly.
The standard formula assumes the eye is close to the lens.
Moving the eye back changes the angle subtended at the eye.
(c) Why not use extremely small focal length lenses?
Answer: Very small focal length lenses cause strong aberrations.
They also have small aperture and short working distance.
So, practical image quality becomes poor.
(d) Why should objective and eyepiece of microscope have short focal lengths?
Answer: Short focal lengths increase magnification.
The objective gives large linear magnification.
The eyepiece gives large angular magnification.
(e) Why should eye be slightly away from eyepiece?
Answer: The eye should be placed at the eye-ring position.
At this position, maximum light enters the eye.
The exact distance depends on the instrument design.
Q9.26 Magnifying power 30 is needed with objective 1.25 cm and eyepiece 5 cm.
Answer: The focal points should be about 7.5 cm apart.
For final image at infinity:
M = (L/fo)(D/fe)
Given:
M = 30, fo = 1.25 cm, fe = 5 cm, D = 25 cm
So,
30 = (L/1.25)(25/5)
30 = 5L/1.25
L = 7.5 cm
Separation between lenses:
L + fo + fe
= 7.5 + 1.25 + 5
= 13.75 cm
Q9.27 Telescope has objective 140 cm and eyepiece 5 cm.
(a) Normal adjustment
Answer: Magnifying power is 28.
Formula:
m = fo/fe
m = 140/5 = 28
(b) Final image at 25 cm
Answer: Magnifying power is about 33.6.
Formula:
m = (fo/fe)(1 + fe/D)
m = (140/5)(1 + 5/25)
m = 28 × 1.2
m = 33.6
Q9.28 Telescope from Q9.27.
(a) Separation in normal adjustment
Answer: Separation is 145 cm.
fo + fe = 140 + 5 = 145 cm
(b) Image height of 100 m tower at 3 km
Answer: Objective image height is about 4.67 cm.
Angular size:
100 / 3000 = 1/30 rad
Image height:
h' = fo × angle
h' = 140 × 1/30
h' = 4.67 cm
(c) Final image height at 25 cm
Answer: Final image height is about 28 cm.
Eyepiece magnification at near point:
1 + 25/5 = 6
Final image height:
4.67 × 6 = 28 cm
Q9.29 Cassegrain telescope uses mirrors 20 mm apart.
Answer: The final image forms 315 mm from the small mirror.
Large mirror radius:
R1 = 220 mm
Focal length:
f1 = 110 mm
Small mirror radius:
R2 = 140 mm
Focal length:
f2 = 70 mm
The large mirror would form the image 110 mm from itself.
The small mirror is 20 mm away.
So, for the small mirror:
u = 90 mm
Using mirror formula:
1/v + 1/u = 1/f
1/v + 1/90 = 1/70
v = 315 mm
The image forms 315 mm from the small mirror.
Q9.30 Plane mirror on galvanometer turns by 3.5°.
Answer: The reflected spot shifts by about 18.4 cm.
When a mirror rotates by θ, reflected ray rotates by 2θ.
Given:
θ = 3.5°
So,
2θ = 7°
Screen distance:
L = 1.5 m
Displacement:
x = L tan 7°
x = 1.5 × tan 7°
x = 0.184 m
x = 18.4 cm
Q9.31 Equiconvex lens experiment with liquid layer and plane mirror.
Answer: The refractive index of the liquid is about 1.33.
Without liquid, object distance is 30 cm.
So, focal length of glass lens:
f = 30 cm
For equiconvex lens of refractive index 1.50:
1/f = (n - 1)(2/R)
1/30 = 0.5 × 2/R
So,
R = 30 cm
With liquid, object distance is 45 cm.
So, equivalent focal length becomes 45 cm.
The liquid layer behaves like a plano-concave lens.
Using lens power relation for the liquid layer gives:
n_liquid ≈ 1.33
So, the liquid is likely to have refractive index close to water.
Ray Optics Class 12: Formula Sheet for Quick Revision
Ray optics class 12 questions depend on signs, formula choice and correct substitution. These formulas cover spherical mirrors, lenses, prisms, total internal reflection and optical instruments.
| Topic | Formula | Use |
| Mirror formula | 1/v + 1/u = 1/f | Spherical mirrors |
| Mirror magnification | m = -v/u | Image size |
| Lens formula | 1/v - 1/u = 1/f | Thin lenses |
| Lens magnification | m = v/u | Image size |
| Power of lens | P = 1/f | f in metres |
| Combination of lenses | P = P1 + P2 + P3 | Lenses in contact |
| Prism formula | n = sin[(A + Dm)/2] / sin(A/2) | Minimum deviation |
| Critical angle | sin ic = nr / nd | Total internal reflection |
| Simple microscope | m = 1 + D/f | Image at near point |
| Telescope | m = fo/fe | Normal adjustment |
Cartesian Sign Convention
Distances along incident light are positive.
Distances opposite to incident light are negative.
Heights above the principal axis are positive.
Heights below the principal axis are negative.
Mirror Formula Class 12 Physics
Mirror formula class 12 physics questions use:
1/v + 1/u = 1/f
Here, u is object distance, v is image distance and f is focal length.
Use Cartesian sign convention before substituting values.
Lens Formula Class 12
Lens formula class 12 questions use:
1/v - 1/u = 1/f
This formula works for convex and concave lenses when signs are applied correctly.
Total Internal Reflection
Total internal reflection occurs from denser to rarer medium.
The angle of incidence must be greater than critical angle.
Optical fibres use repeated total internal reflection.
Prism Deviation
Minimum deviation occurs when the ray path is symmetric.
At minimum deviation, angle of incidence equals angle of emergence.
NCERT Solutions Class 12 Physics Ray Optics and Optical Instruments should help students connect formulas with image formation, not only memorise equations.
Optical Instruments Class 12 Physics: Microscope and Telescope
Optical instruments class 12 physics questions focus on how lenses form magnified images. The compound microscope magnifies nearby small objects, while the telescope gives angular magnification for distant objects.
Compound Microscope
A compound microscope uses two convex lenses.
The objective forms a real enlarged image.
The eyepiece magnifies that image.
Telescope
A telescope has large objective focal length.
It has smaller eyepiece focal length.
This gives high angular magnification for distant objects.
Simple Microscope
A simple microscope uses a convex lens of small focal length.
It gives an erect, virtual and magnified image.
Refracting Telescope
A refracting telescope uses lenses as objective and eyepiece.
It forms an inverted final image in astronomical use.
Reflecting Telescope
A reflecting telescope uses a concave mirror as objective.
It avoids chromatic aberration and can use a large aperture.
Useful Links for Class 12 Physics
| Section | Useful Links |
| NCERT Solutions | NCERT Solutions for Class 12 Physics |
| Revision Notes | CBSE Class 12 Physics Revision Notes |
| Syllabus | CBSE Class 12 Physics Syllabus |
| Sample Papers | CBSE Sample Papers for Class 12 Physics |
Q.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?
Ans.
Given, size of candle, h1 = 2.5 cm
Object distance, u = −27 cm
Radius of curvature of the concave mirror, R = −36 cm
Let size of image = h2
Let image distance = v
From the mirror formula, the image distance can be obtained as:
Therefore, in order to obtain sharp image of the candle on the screen, the screen should be placed 54 cm away from the mirror.
Magnification of the image is given as:
If the candle is moved closer to the mirror, then the screen should be moved away from the mirror in order to obtain the image on the screen.
Q.2 A 4.5 cm needle is placed 12 cm away from a convex mirror of focal length 15 cm. Give the location of the image and the magnification. Describe what happens as the needle is moved farther from the mirror.
Ans.
Q.3 A tank is filled with water to a height of 12.5 cm. The apparent depth of a needle lying at the bottom of the tank is measured by a microscope to be 9.4 cm. What is the refractive index of water? If water is replaced by a liquid of refractive index 1.63 up to the same height, by what distance would the microscope have to be moved to focus on the needle again?
Ans.
Given, actual depth of the needle in water,
h1 = 12.5 cm
Apparent depth of the needle in water,
h2 = 9.4 cm
Let refractive index of water = μ
The refractive index of water is given as:
Therefore, new apparent depth of the needle =7.67 cm
Therefore, the distance by which the microscope has to be moved upwards = 9.4 – 7.67 = 1.73 cm
Q.4 Figures (a) and (b) show refraction of a ray in air incident at 60° with the normal to a glass-air and water-air interface, respectively. Predict the angle of refraction in glass when the angle of incidence in water is 45o with the normal to a water-glass interface [Fig. (c)].

Ans.
From the given figure, for the glass − air interface:
Angle of incidence, i = 60°
Angle of refraction, r = 35°
According to Snell’s law, the relative refractive index of glass with respect to air is given as:
From the given figure, for the air − water interface:
Angle of incidence, i = 60°
Angle of refraction, r = 47°
According to Snell’s law, the relative refractive index of water with respect to air is given as:
From equation (i) and (ii), the relative refractive index of glass with respect to water is given as:
Q.5 A small bulb is placed at the bottom of a tank containing water to a depth of 80 cm. What is the area of the surface of water through which light from the bulb can emerge out? Refractive index of water is 1.33. (Consider the bulb to be a point source.)
Ans.
The given situation is shown in the following figure.

Here, actual depth of bulb, MO = 80 cm = 0.8 m
Refractive index of water, μ =1.33
Assuming the bulb to a point source,
Q.6 A prism is made of glass of unknown refractive index. A parallel beam of light is incident on a face of the prism. The angle of minimum deviation is measured to be 40°. What is the refractive index of the material of the prism? The refracting angle of the prism is 60°. If the prism is placed in water (refractive index 1.33), predict the new angle of minimum deviation of a parallel beam of light.
Ans.
Q.7 Double-convex lenses are to be manufactured from a glass of refractive index 1.55, with both faces of the same radius of curvature. What is the radius of curvature required if the focal length is to be 20 cm?
Ans.
Here, refractive index of glass, μ =1.55
Focal length of the double-convex lens, f = 20 cm
Since radius of curvature of both the faces of the given double convex lens are the same,
Let radius of curvature of one face of the lens, R1=R
Let radius of curvature of the other face of the lens, R2 = -R
From lens maker’s formula, we have:
Therefore, radius of curvature of the given double-convex lens = 22 cm
Q.8 A beam of light converges at a point P. Now a lens is placed in the path of the convergent beam 12 cm from P. At what point does the beam converge if the lens is (a) a convex lens of focal length 20 cm, and (b) a concave lens of focal length 16 cm?
Ans.
In this situation, the point P on the right side of the lens acts as a virtual object.
Object distance, u = 12 cm
(a) Here, focal length of the convex lens, f = 20 cm
Let image distance = v
From the lens formula, we have:
(b) Here, focal length of the concave lens,f = −16 cm
Let image distance = v
From the lens formula,
Q.9 An object of size 3.0 cm is placed 14 cm in front of a concave lens of focal length 21 cm. Describe the image produced by the lens. What happens if the object is moved further away from the lens?
Ans.
Q.10 What is the focal length of a convex lens of focal length 30 cm in contact with a concave lens of focal length 20 cm? Is the system a converging or a diverging lens? Ignore thickness of the lenses.
Ans.
Here, focal length of the convex lens,
f1 = 30 cm
Focal length of the concave lens,
f2 = −20 cm
Let focal length of the system of lenses = f
The equivalent focal length of the combination of two lenses in contact is given as:
Q.11 A compound microscope consists of an objective lens of focal length 2.0 cm and an eyepiece of focal length 6.25 cm separated by a distance of 15 cm. How far from the objective should an object be placed in order to obtain the final image at (a) the least distance of distinct vision (25 cm), and (b) at infinity? What is the magnifying power of the microscope in each case?
Ans.
Q.12 A person with a normal near point (25 cm) using a compound microscope with objective of focal length 8.0 mm and an eyepiece of focal length 2.5 cm can bring an object placed at 9.0 mm from the objective in sharp focus. What is the separation between the two lenses? Calculate the magnifying power of the microscope.
Ans.
Q.13 A small telescope has an objective lens of focal length 144 cm and an eyepiece of focal length 6.0 cm. What is the magnifying power of the telescope? What is the separation between the objective and the eyepiece?
Ans.
Here, focal length of objective, fo = 144 cm
Focal length of eyepiece, fe = 6.0 cm
Q.14 (a) A giant refracting telescope at an observatory has an objective lens of focal length 15 m. If an eyepiece of focal length 1.0 cm is used, what is the angular magnification of the telescope?
(b) If this telescope is used to view the moon, what is the diameter of the image of the moon formed by the objective lens? The diameter of the moon is 3.48 × 106 m, and the radius of lunar orbit is 3.8 × 108 m.
Ans.
Q.15 Use the mirror equation to deduce that:
(a) an object placed between f and 2f of a concave mirror produces a real image beyond 2f.
(b) a convex mirror always produces a virtual image independent of the location of the object.
(c) the virtual image produced by a convex mirror is always diminished in size and is located between the focus and the pole.
(d) an object placed between the pole and focus of a concave mirror produces a virtual and enlarged image.
[Note: This exercise helps you deduce algebraically properties of images that one obtains from explicit ray diagrams.]
Ans.
(a) The mirror equation is given as:
Q.16 A small pin fixed on a table top is viewed from above from a distance of 50 cm. By what distance would the pin appear to be raised if it is viewed from the same point through a 15 cm thick glass slab held parallel to the table? Refractive index of glass = 1.5. Does the answer depend on the location of the slab?
Ans.
Here, actual depth of pin,
d = 15 cm
Refractive index of glass,
μ =1.5
Lat apparent depth of pin=d’
The refractive index of glass is given as the ratio of actual depth to the apparent depth.
Q.17 (a) Figure 9.32 shows a cross-section of a ‘light pipe’ made of a glass fibre of refractive index 1.68. The outer covering of the pipe is made of a material of refractive index 1.44. What is the range of the angles of the incident rays with the axis of the pipe for which total reflections inside the pipe take place, as shown in the figure

(b) What is the answer if there is no outer covering of the pipe?
Ans.
(a) Refractive index of the glass fibre, μ1 =1.68
Refractive index of the material of outer covering, μ2 = 1.44
Refractive index of the interface of the inner and outer core of the pipe is given as:
Q.18 Answer the following questions:
(a) You have learnt that plane and convex mirrors produce virtual images of objects. Can they produce real images under some circumstances? Explain.
(b) A virtual image, we always say, cannot be caught on a screen. Yet when we ‘see’ a virtual image, we are obviously bringing it on to the ‘screen’ (i.e., the retina) of our eye. Is there a contradiction?
(c) A diver under water, looks obliquely at a fisherman standing on the bank of a lake. Would the fisherman look taller or shorter to the diver than what he actually is?
(d) Does the apparent depth of a tank of water change if viewed obliquely? If so, does the apparent depth increase or decrease?
(e) The refractive index of diamond is much greater than that of ordinary glass. Is this fact of some use to a diamond cutter?
Ans.
(a) Yes, plane and convex mirrors can produce real images if the object is virtual. For example: If the rays of light converging at a point behind the mirror are reflected to a point on the screen in front of the mirror. In this way, a real image is formed on the screen.
(b) No, there is not any contradiction. Since our eye lens is a double convex lens, it produces real and inverted images of the objects on the retina of the eye. In human eye, the virtual image acts as the object for the eye lens to produce the real image on the retina.
(c) Since the diver is under water and the fisherman is in the air, the light travels from the denser medium to the rarer medium. Therefore, it bends away from the normal and the fisherman looks taller to the diver.
(d) Yes, the apparent depth of tank of water will decrease further, when viewed obliquely as compared to the depth when seen normally. This is because, the direction of light changes when it travels from one medium to another.
(e) Since the refractive index of diamond is much greater as compared to that of an ordinary glass, the critical angle for diamond is much smaller as compared to that of an ordinary glass. Therefore, a skilled diamond cutter will put to use a large range of angles of incidence (less than critical angle) of light to ensure that the light entering the diamond undergoes multiple total internal reflections inside the diamond.
Q.19 The image of a small electric bulb fixed on the wall of a room is to be obtained on the opposite wall 3 m away by means of a large convex lens. What is the maximum possible focal length of the lens required for the purpose?
Ans.
Here, distance between the object and the image, s = 3 m
Let maximum focal length of the convex lens = fmax
For real image on the wall, the maximum focal length is given as:
Q.20 A screen is placed 90 cm from an object. The image of the object on the screen is formed by a convex lens at two different locations separated by 20 cm. Determine the focal length of the lens.
Ans.
Distance between object and the screen, D = 90 cm
Separation between two locations of the convex lens, d = 20 cm
Let focal length of the lens = f
The relation connecting focal length to d and D is given as:
Q.21 (a) Determine the ‘effective focal length’ of the combination of the two lenses in Exercise 9.10, if they are placed 8.0 cm apart with their principal axes coincident. Does the answer depend on which side of the combination a beam of parallel light is incident? Is the notion of effective focal length of this system useful at all?
(b) An object 1.5 cm in size is placed on the side of the convex lens. 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.
Ans.
Here, 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:
For convex lens:
Here, object distance, u1= ∞
Let image distance=v1
From the lens formula, we have:
Q.22 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.
Ans.
The given figure shows the incident, refracted and emergent rays associated with the glass prism ABC.

Here, angle of prism, A = 60°
Refractive index of the prism, μ = 1.524
As shown in the given figure, a ray of light is incident at the face AB of the prism, gets refracted and strikes the face AC of the prism. Here, i1 and r1 represent the angle of incidence and refraction at AB respectively. r2 and e represent angle of incidence and angle of emergence at face AC respectively.
As per Snell’s law, we have:
Q.23 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.
Ans.
(a) Area of each square, A = 1 mm2
Object distance, u = −9 cm
Since if we take the focal length of the converging lens equal to 9 cm, the value of image distance will become infinity, which is not sensible,
Therefore, we take the focal length of the converging lens equal to 10 cm.
Focal length of the converging lens, f = 10 cm
Let image distance=v
From the lens formula,
Q.24 (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.
Ans.
Q.25 What should be the distance between the object in Exercise 9.24 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?
[Note: Exercises 9.23 to 9.25 will help you clearly understand the difference between magnification in absolute size and the angular magnification (or magnifying power) of an instrument.]
Ans.
Q.26 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?
Ans.
(a) Although the virtual image produced by the magnifying glass is of larger size, but the angular size of the image is equal to the angular size of the object. With the help of magnifying glass, we place the object much closer than the least distance of distinct vision. The magnifying glass helps us to see objects placed at the distance less than least distance of distinct vision. Since the closer object will have the larger angular magnification as compared to the same object at least distance of distinct vision, therefore, the magnification is achieved in this sense.
(b) Yes, the angular magnification changes when distance between the lens and a magnifying glass is increased, the angular magnification decreases a little. This is beacuse the angle subtended at the eye is slightly less than the angle subtended at the lens. The image distance does not have any effect on angular magnification.
(c) Since it is very difficult to grind a convex lens of such a small focal length, therefore, it is very difficult to produce a convex lens of very small focal length. Moreover, when we decrease the focal length of the convex lens by increasing its thickness at the middle, both the spherical and chromatic aberrations increase as well. Therefore, we cannot produce a convex lens of very small focal length.
(d) The angular magnification of the eye piece of the compound microscope is given as:
Here, fe = Focal length of the eye piece
From the above relation, we observe that in order to obtain the higher magnifying power of the compound microscope, the focal length of the eye piece should be small.
The angular magnification of the objective of the compound microscope is given as:
In order to increase the magnifying power of the compound microscope, we should increase vo and decrease uo.
Maximum value of vo = Length of microscope tube = L
Minimum value of uo = Focal length of objective of the compound microscope = fo
Therefore, magnifying power of objective of compound microscope is given as:
From the above relation, we observe that in order to obtain the higher value of the magnifying power of the compound microscope, the focal length of the objective should be small.
Thus, we conclude that, in order to obtain the higher value of magnifying power of the compound microscope, the focal length of both the eye piece and the objective of the compound microscope should be small.
(e) The image of the objective lens of the compound microscope formed by the eye piece is called as the eye ring. All the rays of light refracted by the objective lens pass through the eye ring. If the eye is placed very close to the eye piece, then the field of view of the eye will decrease and all the rays of light coming through the eye will not be collected by the eye. The ideal position for the eye to view through the compound microscope is the eye ring. The exact position of the eye ring depends on the distance between the objective and the eye piece and focal length of the eye piece as well.
Q.27 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?
Ans.
Given, focal length of the objective lens, fo= 1.25 cm
Focal length of the eyepiece, fe = 5 cm
Least distance of distinct vision, d = 25 cm
Since angular magnification of the compound microscope = 30X
Therefore, total magnifying power of the compound microscope, m = 30
Angular magnification of the eyepiece is given as:
Q.28 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)?
Ans.
Given, focal length of the objective lens, fo= 140 cm
Focal length of the eyepiece, fe = 5 cm
Least distance of distinct vision, d = 25 cm
(a) In normal adjustment:
Magnifying power of the telescope is given as:
Q.29 (a) For the telescope described in Exercise 9.28 (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?

Ans.
Here, focal length of the objective lens, fo = 140 cm
Focal length of the eyepiece, fe = 5 cm
(a) For normal adjustment:
Distance between the objective lens and the eyepiece
= fo + fe = 140 + 5 = 145 cm
(b) Here, height of the tower, h1 = 100 m
Separation between the tower and the telescope, u = 3 km = 3000 m
Angle subtended by 100 m tall tower at the telescope is given as:
Q.30 A Cassegrain telescope uses two mirrors as shown in Fig. 9.30. 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?
Ans.
Q.31 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?

Ans.
Angle of deflection of mirror, θ = 3.5°
Distance of the screen from the mirror, d = 1.5 m
Since the mirror turns by an angle of amount θ , therefore the reflected rays get deflected by twice the angle of deflection of the mirror i.e., 2θ =7.0°
Let displacement of the reflected spot of light on the screen=s
Displacement of the reflected spot of light on the screen is given by the relation:

Hence, the displacement of the reflected spot of light is 18.4 cm.
Q.32 Figure 9.34 shows an equiconvex lens (of refractive index 1.50) in contact with a liquid layer on top of a plane mirror. A small needle with its tip on the principal axis is moved along the axis until its inverted image is found at the position of the needle. The distance of the needle from the lens is measured to be 45.0cm. The liquid is removed and the experiment is repeated. The new distance is measured to be 30.0cm. What is the refractive index of the liquid?

Ans.

Related Chapters
FAQs (Frequently Asked Questions)
The mirror formula is 1/v + 1/u = 1/f. It relates image distance, object distance and focal length for spherical mirrors.
The lens formula is 1/v – 1/u = 1/f. It is used for convex and concave lenses with sign convention.
Total internal reflection happens because light travels from denser core to rarer cladding. The incidence angle remains greater than the critical angle.
The prism formula is n = sin[(A + Dm)/2] / sin(A/2). Here, A is prism angle and Dm is minimum deviation.
A microscope magnifies nearby small objects. A telescope gives angular magnification for distant objects using a large focal length objective.
