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 .

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

Focal length of the concave mirror is given as:f = R2=-362 cm=-18 cm                     

Let size of image = h2
Let image distance = v
From the mirror formula, the image distance can be obtained as:

1v+1u=1f1v=1f1u=118cm+127cm=3+254cm=154cmImage distance,v=54 cm

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:

m=-h2h1=-v-u=vu-h22.5 cm=-54 cm -27 cm= 2Size of the image, h2=-5 cmThe image of the candle is real, inverted and magnified.

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.

Height of the needle, h1= 4.5 cmObject distance, u = -12 cmFocal length of the convex mirror, f = 15 cmLet image distance = vFrom the mirror formula, the image distance can be obtained as:1v+1u=1f                                                        1v=1f1u 1v= 115 cm+112 cm1v=4 + 560 cm=960 cmImage distance, v = 60 cm9 = 6.7 cmTherefore, the virtual image is formed at 6.7 cm behind the mirror. The magnification of the image is given as:m = h2h1 = –vu                                                      h24.5 cm= –6.7 cm12 cmh2 = –6.712 × 4.5 cm = 2.5 cmSize of the image, h2 = 2.5 cmm  =  h2h1= 2.5 cm4.5 cm = 0.56The image formed is virtual and erect.If the needle is moved farther from the mirror, then the image moves away from the mirror up to its principal focus and its magnification goes on decreasing.

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:

μ= Realdepth Apparentdepth = 12.5 9.4 =1.33 Forthesecondcase: Refractiveindexoftheliquid,μ=1.63 Realdepthofneedle=12.5cm Letapparentdepth=y Therelationforrefractiveindexisgivenas: μ= Realdepth Apparentdepth 1.63= 12.5 y y= 12.5 1.63 =7.67cm MathType@MTEF@5@5@+=feaaguart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbwvMCKfMBHbqedmvETj2BSbqefm0B1jxALjhiov2DaebbnrfifHhDYfgasaacH8MrFz0xbbf9q8WrFfeuY=Hhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0RYxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaaiaacaGaaeqabaWabeqaeaaakqaabeqaaiabeY7aTjabg2da9maalaaabaGaaeOuaiaabwgacaqGHbGaaeiBaiaaysW7caqGKbGaaeyzaiaabchacaqG0bGaaeiAaaqaaiaabgeacaqGWbGaaeiCaiaabggacaqGYbGaaeyzaiaab6gacaqG0bGaaGjbVlaabsgacaqGLbGaaeiCaiaabshacaqGObaaaiabg2da9maalaaabaGaaGymaiaaikdacaGGUaGaaGynaaqaaiaaiMdacaGGUaGaaGinaaaaaeaacqGH9aqpcaaIXaGaaiOlaiaaiodacaaIZaGaaGjbVlaaysW7caaMe8UaaGjbVlaaysW7caaMe8UaaGjbVlaaysW7caaMe8UaaGjbVlaaysW7caaMe8UaaGjbVlaaysW7caaMe8UaaGjbVlaaysW7caaMe8UaaGjbVlaaysW7caaMe8UaaGjbVlaaysW7caaMe8UaaGjbVlaaysW7caaMe8UaaGjbVlaaysW7aeaacaqGgbGaae4BaiaabkhacaaMe8UaaeiDaiaabIgacaqGLbGaaGjbVlaabohacaqGLbGaae4yaiaab+gacaqGUbGaaeizaiaaysW7caqGJbGaaeyyaiaabohacaqGLbGaaeOoaaqaaiaabkfacaqGLbGaaeOzaiaabkhacaqGHbGaae4yaiaabshacaqGPbGaaeODaiaabwgacaaMe8UaaeyAaiaab6gacaqGKbGaaeyzaiaabIhacaaMe8Uaae4BaiaabAgacaaMe8UaaeiDaiaabIgacaqGLbGaaGjbVlaabYgacaqGPbGaaeyCaiaabwhacaqGPbGaaeizaiaacYcacaaMe8UaeqiVd0Maeyypa0JaaGymaiaac6cacaaI2aGaaG4maaqaaiaabkfacaqGLbGaaeyyaiaabYgacaaMe8UaaeizaiaabwgacaqGWbGaaeiDaiaabIgacaaMe8Uaae4BaiaabAgacaaMe8UaaeOBaiaabwgacaqGLbGaaeizaiaabYgacaqGLbGaeyypa0JaaGymaiaaikdacaGGUaGaaGynaiaaysW7caWGJbGaamyBaaqaaiaabYeacaqGLbGaaeiDaiaaysW7caqGHbGaaeiCaiaabchacaqGHbGaaeOCaiaabwgacaqGUbGaaeiDaiaaysW7caqGKbGaaeyzaiaabchacaqG0bGaaeiAaiabg2da9iaadMhaaeaacaqGubGaaeiAaiaabwgacaaMe8UaaeOCaiaabwgacaqGSbGaaeyyaiaabshacaqGPbGaae4Baiaab6gacaaMe8UaaeOzaiaab+gacaqGYbGaaGjbVlaabkhacaqGLbGaaeOzaiaabkhacaqGHbGaae4yaiaabshacaqGPbGaaeODaiaabwgacaaMe8UaaeyAaiaab6gacaqGKbGaaeyzaiaabIhacaaMe8UaaeyAaiaabohacaaMe8Uaae4zaiaabMgacaqG2bGaaeyzaiaab6gacaaMe8UaaeyyaiaabohacaqG6aaabaGaeqiVd0Maeyypa0ZaaSaaaeaacaqGsbGaaeyzaiaabggacaqGSbGaaGjbVlaabsgacaqGLbGaaeiCaiaabshacaqGObaabaGaaeyqaiaabchacaqGWbGaaeyyaiaabkhacaqGLbGaaeOBaiaabshacaaMe8UaaeizaiaabwgacaqGWbGaaeiDaiaabIgaaaaabaGaeyinIWLaaGymaiaac6cacaaI2aGaaG4maiabg2da9maalaaabaGaaGymaiaaikdacaGGUaGaaGynaaqaaiaadMhaaaaabaGaeyinIWLaamyEaiabg2da9maalaaabaGaaGymaiaaikdacaGGUaGaaGynaaqaaiaaigdacaGGUaGaaGOnaiaaiodaaaaabaGaeyypa0JaaG4naiaac6cacaaI2aGaaG4naiaaysW7caqGJbGaaeyBaaaaaa@50FC@

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:

μ air glass = sin60 o sin35 o = 0.8660 0.5736 = 1.51 (i)

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:

μ air water = sin60 o sin47 o = 0.8660 0.7314 = 1.184 (ii)

From equation (i) and (ii), the relative refractive index of glass with respect to water is given as:

μglasswater=μglassairμwaterair=1.511.184=1.275(iii)

From the given figure, for the waterglass interface:Given, angle of incidence,i=45Let angle of refraction =r

According to Snell’s law, the refractive index of glass with respect to water is given as:μglasswater=sinisinr=sin45sinr(iv)From equation (iii) and (iv), we have:1.275=sin45sinrsinr=0.70711.275=0.5546r=sin1(0.5546)=33.68

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,

Area of the surface through which the light from the bulb can emerge out =Area of circle of radius, r = NP 2 = ON = OP Forangleofincidence,i = Criticalangle = C Angleofrefraction, r = 90 o AccordingtoSnell’slaw,therelationforrefractiveindexof waterisgivenas: μ= sinr sini 1.33 = sin90 o sinC = 1 sinC sin C = 1 1.33 = 0.75 C = sin -1 0.75 = 48 .6 o Fromthegivenfigure,inΔOPM,wehave: tani = OP OM OP = OM tan48 .6 o = 0.8 × 1.1345 = 0.907m Area of the surface through which the light from the bulb can emerge out=π r 2 = 3.14 OP 2 = 3.14 0.907 2 = 2.59 m 2

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.

Angle of minimum deviation,δm= 40°Angle of the prism,A = 60°Refractive index of water,μ = 1.33Let refractive index of the material of the prism =The angle of deviation is related to refractive index as:Relation connecting refractive index of the material of the prism and angle of deviation is given as:μP = sinA + δm2sinA2= sin60o + 40o2sin60o2= sin50osin30o= 1.532Refractive index of the material of the prism=1.532When the placed in water:Let new minimum angle of deviation=δmRefractive index of the material of the prism with respect to water is given as:μPw = μPμ= sinA + δm2sinA2sinA+δm2 = sinA2×μPμsinA+δm2 = sin60o2×1.5321.33= 12×1.5321.33= 0.5759= sin35.16osinA+δm2=sin35.16oA+δm2=35.16oA+δm‘=70.32oδm‘=70.32o– A=70.32o– 60o =10.32oTherefore, the new minimum angle of deviation of the parallel beam of light= 10.20°

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:

1 f = μ – 1 1 R 1 1 R 2 1 20 cm = 1.55 – 1 1 R + 1 R 1 20 cm = 0.55 × 2 R R = 0.55 × 2 × 20 cm = 22cm

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:

1v1u = 1f1v = 1f + 1u1v = 120 cm + 112 cm = 3 + 560 cmv = 60 cm8 = 7.5 cmThe image is formed at 7.5 cm to the right of the lens.

(b) Here, focal length of the concave lens,f = −16 cm
Let image distance = v
From the lens formula,

1 v 1 u = 1 f 1 v = 1 f + 1 u 1 v = – 1 16 cm + 1 12 cm 1 v = -3 + 4 48 cm = 1 48 v = 48cm Theimageisformedat48cmtotherightofthelens.

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.

Here, size of the object, h1= 3 cmObject distance, u = -14 cmFocal length of the concave lens, f = -21 cmLet image distance = vLet size of the object=h2From the lens formula, we have:

1v1u = 1f  1v = 1f + 1u= –121 cm114 cm= -2 – 342 cm = -542 cmv = –425 cm = -8.4 cmThe image formed is vertual, erect and 8.4 cm away from the lens on the same side as the object.Magnification of the lens is given by the relation:m = h2h1= vu h2 = -8.4 cm-14 cm × 3= 0.6 cm × 3 = 1.8 cm

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:

1f = 1f1+1f2= 130 cm120 cm= 2 – 360 cm=-160 cmf = -60 cmThe negative sign indicates it is a diverging lens withthe focal length of the combination of lenses=60 cm

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.

Here, focal length of the objective lens, f o = 2.0 cm Focal length of the eyepiece, f e = 6.25 cm Distance between the objective lens and the eyepiece, d = 15 cm ( a ) Least distance of distinct vision, d’ = 25 cm Image distance for the eyepiece, v e = -25 cm Let object distance for the eyepiece = u e From the lens formula, we have 1 v e 1 u e = 1 f e 1 u e = 1 v e 1 f e 1 u e = 1 -25 cm 1 6.25 cm = -1 5 cm u e = -5cm Image distance for the objective lens is given as v o = d + u e = 15 cm – 5 cm = 10 cm Object distance for the objective lens = u o From the lens formula, we have 1 v o 1 u o = 1 f o 1 u o = 1 v o 1 f o 1 u o = 1 10 cm 1 2 cm = -2 5 cm u o = -2.5cm Magnifyingpowerofthecompoundmicroscopeisgivenas: m = v o | u o | ( 1+ d’ f e ) = 10 cm 2.5 cm ( 1+ 25 cm 6.25 cm ) = 20 Magnifyingpowerofthecompoundmicroscope = 20

(b)Sincetheimageisformedatinfinity, Imagedistancefortheeyepiece, v e = Letobjectdistanceforthe eyepiece be u e Fromlensformula,wehave 1 v e 1 u e = 1 f e 1 1 u e = 1 6.25 u e =-6.25cm Imagedistancefortheobjectivelensisgivenas v o = d + u e v o = 15 cm – 6.25 cm = 8.75cm Letobjectdistancefortheobjective lens be u o Fromlensformula,wehave 1 v o 1 u o = 1 f o 1 u o = 1 v o 1 f o 1 u o = 1 8.75 cm 1 2 cm u o =- 17.5 6.75 cm = -2.59cm Magnifying power of the microscope is given as m = v o | u o | × v e | u e | m = 8.75 cm 2.59 cm × 25 cm 6.25 cm = 13.5 Therefore, magnifying power of the microscope is 13.51.

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.

Here, least distance of distinct vision, d = 25 cm Focal length of the objective of the compound microscope, fo = 8 mm = 0.8 cm Focal length of the eyepiece of the compound microscope, fe = 2.5 cm Object distance,u o = -9.0 mm = -0.9 cm From the lens formula, we have: 1 v e 1 u e = 1 f e 1 u e = 1 v e 1 f e Here,imagedistance, v e = -d = -25cm 1 u e = 1 -25 cm 1 2.5 cm = -1 – 10 25 cm = -11 25 cm u e = -25 11 = -2.27cm Incaseofobjectivelens: Fromlensformula,wehave: 1 v o 1 u o = 1 f o 1 v o = 1 f o + 1 u o = 1 0.8 cm 1 0.9 cm 1 v o = 0.9 – 0.8 0.72 cm = 0.1 0.72 v o = 0.72 0.1 = 7.2cm Thus, imagedistanceforobjective, v o =7.2cm Distancebetweenthetwolenses = u e +v o 2.27 cm + 7.2 cm = 9.47cm Magnifyingpowerofthemicroscopeisgivenas: m = v o u o 1+ d f e m = 7.2 cm 0.9 cm 1+ 25 cm 2.5 cm =88 Magnifyingpowerofthemicroscope = 88

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

m = f o f e = 144 cm 6 cm =24 Therefore, for normal adjustment, the magnifying power of the telescope = 24 Separation between the objective and the eyepiece is given as: L = fo + fe L = 144 cm + 6.0 cm = 150 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.

Here, focal length of the objective lens, fo = 15 m = 15 × 102 cmFocal length of the eyepiece, fe = 1.0 cma Angular magnification of the telescope is given as:m = fofe= 15×102 cm 10 cm = 1500                                         Therefore, angular magnification of the given refracting telescope = 1500b) Here, diameter of moon,D = 3.48 × 106 mRadius of lunar orbit,ra = 3.8 × 108 mLet diameter of the image of moon = dAngle subtended by the diameter of the moon is given as:θm = Diameter of the moonRadius of the lunar obbit=Dra=3.48×1063.8×108             Angle subtended by the image is given as:θI=Diameter of imageFocal length of objective lens=dfo = d15Since, angle subtended by the diameter of moon=anglesubtended by imageθm = θI3.48×1063.8×108 = d15d = 15 × 3.48×1063.8×108= 13.73×10-2 m = 13.73 cmSince, angle subtended by the diameter of the moon = angle subtended by the imageTherefore, the diameter of the image of the moon formed by the objective lens = 13.74 cm

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:

1 v + 1 u = 1 f 1 v = 1 f 1 u Foraconcavemirror,thefocallengthisnegative. f < 0 Sinceobjectliesontheleft, Objectdistance,u < 0 Sincetheobjectisplacedbetweenfand2f, 2f < u < f 1 2f > 1 u > 1 f 1 2f < – 1 u < – 1 f 1 f 1 2f < 1 f 1 u < 0 1 2f < 1 v < 0(i) 1 f 1 u = 1 v Equation(i)showsthat 1 v isnegative. Thevalueofvisnegative. Itimpliesthattherealimageisformed. Since, 1 2f < 1 v 2f > v -v > -2f Realimageisformedbeyond2f. (b)Fromthemirrorformulaforaconvexmirror,wehave: 1 f = 1 v + 1 u 1 v = 1 f 1 u (a) Sinceforaconvexmirror,thevalueoffocallengthis alwayspositiveandobjectdistance(u)isalwaysnegative. f > 0andu < 0 (b) Fromequation(a)and(b),weobtain: 1 v = 1 f 1 -u = 1 f + 1 u >0 1 v > 0 Thevalueofvispositive. Foraconvexmirror,whatevermaybethevalueofu, thevalueofimagedistance(v)alwaysremainspositive. Independentoftheobjectdistance,aconvexmirror alwaysformsvirtualimages. (c)Sincefocallengthofaconvexlensispositive. f > 0 Sincetheobjectliesontheleft, Objectdistance,u < 0 Fromthemirrorformulaforconvexmirror,weobtain: 1 f = 1 v + 1 u 1 v = 1 f 1 u Sincef > 0andu < 0 1 v > 1 f v < f Theimageformedbytheconvexmirrorisdiminishedand locatedbetweenthefocusandthepole. (d)Sincethefocallengthofaconcavemirrorisnegative, f < 0 Sincetheobjectisplacedontheleftoftheconcave mirror, u < 0 Fromthemirrorformulaforconcavemirror,weobtain: 1 f = 1 v + 1 u 1 v = 1 f 1 u Sincef < 0andu < 0 1 v = 1 -f 1 -u 1 v = 1 u 1 f (A) Since u < f 1 u > 1 f (B) Fromequation(A)and(B),weobtain: 1 v > 0 vispositive. Itshowsthattheimageisformedontherightsideof themirror. Thevirtualimageisformed. Foru < 0andv > 0.wehave: 1 u > 1 v v > u Magnificationisgivenas: m = v u Sincev > u Magnificationispositiveandtheenlargedimageis formed. Whenanobjectisplacedbetweenthepoleandfocus oftheconcavemirror,thevirtualandenlargedimage isformed.

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.

Refractiveindexofglass,μ = Realdepth Apparentdepth μ = d d’ d’ = d μ = 15 cm 1.5 =10cm Distance through which the pin appears to be raised = Realdepth – Apparentdepth = 15 cm – 10 cm = 5cm

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:

μ = μ2μ1 =1sinic                                                   Here, ic= Critical angle sin ic = μ1μ2=1.441.68 = 0.8571ic = sin-10.8571 = 59oTotal internal reflection takes place only when,Angle of incidence,i>ici.e., i>59oThe maximum value of angle of reflection is given as: rmax=90o-59o=31oFrom Snell’s law, we obtain:μ1=sin imaxsinrmaxsin imax = μ1 sin rmax=1.68 × sin31o= 0.8662 imax = sin-10.8662= 60oRange of angles of incident rays with the axis of pipe£60oThe lower limit of angle of incidence is decided by the ratioof diameter to length of the pipe.(b) If there is no outer covering of the pipe:Refractive index of the outer core of the pipe, μ1 = 1Refractive index of the inner core of the pipe, μ2= 1.68From Snell’s law, we obtain:μ = μ2μ1= 1sinicsinic‘=μ1μ2=11.68=0.5952ic=sin10.5952=36.5oHere, for angle of incidence,i=90oWe obtain, angle of reflection, r=36.5oi=90or=90o36.5o=53.5oSince the value of i>icAll the rays of light incident in the range 90o will undergo total internal reflection.

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:

f max = s 4 = 3 m 4 = 0.75m Therefore, the maximum focal length of the lens required for this purpose = 0.75 m

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:

f = D 2 – d 2 4D = 90 cm 2 20 cm 2 4×90 cm = 770 cm 36 = 21.39cm Therefore, focal length of the convex lens = 21.39 cm

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:

1v11u1=1f11v1=1f11u1=1301v1=30cmFor concave lens:In this case, the image will act as a virtual object.Here, object distance, u2= 30 – d =30 – 8=22 cmLet image distance=v2From lens formula for the concave lens, we obtain:1v21u2=1f21v2=1f21u2=122 cm120 cm=10 – 11220 cmv2 = -220 cmTherefore, the parallel incident beam appears to diverge from a point that is 220-4 216 cm fromthe centre of the system of the two lenses.ii When the parallel beam of light is incident from the left on the concave lens first:For concave lens:Here, object distance, u2=-Let image distance=v2From the lens formula, we have:1v21u2=1f21v2=1f2+1u2=1-20 cm1=-120 cmv2 = -20 cmFor convex lens:Here, object distance, u1=-20 cm + 8 cm = -28 cmLet image distance = v2From lens formula for the convex lens, we obtain:1v11u1=1f11v1=1f1+1u1=130 cm+1-28 cm=14-15420 cm=-1420 cmv2 = -420 cmTherefore, the parallel beam of incident light appears to diverge from a point 420-4=416 cmfrom the centre of the two lens system.b Given, height of the object, h1= 1.5 cmObject distance for convex lens, u1=- 40 cmFrom the lens formula, we obtain:1v11u1=1f11v1=1f1+1u1=130 cm140 cm=4-3120=1120v1=120 cmMagnitude of magnification produced by convex lens is given as:m1=v1u1=120 cm40 cm= 3Therefore, the magnitude of magnification produced by convex lens = 3The image formed by the convex lens acts as an object for the concave lens.For concave lens:Object distance,u2=120 cm – 8 cm = 112 cmFrom the lens formula,we obtain:1v21u2=1f21v2=1f2+1u2=1-20 cm+1112 cm=-112+202240 cm=-922240 cmv2=-224092 cmMagnitude of magnification produced by concave lens is given as:m2=v2u2=224092×1112=2092Net magnification of the lens combination, m=m1×m2=3×2092=0.652Height of image, h2 = emh1= 0.652×1.5 = 0.98 cm

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:

sine sin r 2 =μ sin r 2 = sine μ For total internal reflection at face AC: e=9 0 o sin r 2 = sin 90 o μ = sin 90 o 1.524 = 1 1.524 =0.6562 r 2 = sin 1 ( 0.6562 ) 41 o Sinceangleofprismisgivenas: A= r 1 + r 2 r 1 =A r 2 = 60 o 41 o = 19 o ForfaceAB: FromSnell’slaw,wehave: μ= sin i 1 sin r 1 sin i 1 =μsin r 1 =1.524×sin 19 o =0.496 i 1 = sin 1 ( 0.496 ) = 29.75 o Angleofincidence= 29.75 o MathType@MTEF@5@5@+=feaaguart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbwvMCKfMBHbqedmvETj2BSbqefm0B1jxALjhiov2DaebbnrfifHhDYfgasaacH8MrFz0xbbf9q8WrFfeuY=Hhbbf9v8qqaqFr0xc9pk0xbba9q8WqFfea0=yr0RYxir=Jbba9q8aq0=yq=He9q8qqQ8frFve9Fve9Ff0dmeaabaqaaiaacaGaaeqabaWabeqaeaaakqaabeqaamaalaaabaGaci4CaiaacMgacaGGUbGaamyzaaqaaiGacohacaGGPbGaaiOBaiaadkhadaWgaaWcbaGaaGOmaaqabaaaaOGaeyypa0JaeqiVd0gabaGaeyinIWLaci4CaiaacMgacaGGUbGaamOCamaaBaaaleaacaaIYaaabeaakiabg2da9maalaaabaGaci4CaiaacMgacaGGUbGaamyzaaqaaiabeY7aTbaaaeaacaqGgbGaae4BaiaabkhacaqGGaGaaeiDaiaab+gacaqG0bGaaeyyaiaabYgacaqGGaGaaeyAaiaab6gacaqG0bGaaeyzaiaabkhacaqGUbGaaeyyaiaabYgacaqGGaGaaeOCaiaabwgacaqGMbGaaeiBaiaabwgacaqGJbGaaeiDaiaabMgacaqGVbGaaeOBaiaabccacaqGHbGaaeiDaiaabccacaqGMbGaaeyyaiaabogacaqGLbGaaeiiaiaabgeacaqGdbGaaiOoaaqaaiaabwgacqGH9aqpcaqG5aGaaGimamaaCaaaleqabaGaae4BaaaaaOqaaiabgsJiCjGacohacaGGPbGaaiOBaiaadkhadaWgaaWcbaGaaGOmaaqabaGccqGH9aqpdaWcaaqaaiGacohacaGGPbGaaiOBaiaaiMdacaaIWaWaaWbaaSqabeaacaWGVbaaaaGcbaGaeqiVd0gaaaqaaiabg2da9maalaaabaGaaGPaVlGacohacaGGPbGaaiOBaiaaiMdacaaIWaWaaWbaaSqabeaacaWGVbaaaaGcbaGaaGymaiaac6cacaaI1aGaaGOmaiaaisdaaaaabaGaeyypa0ZaaSaaaeaacaaIXaaabaGaaGymaiaac6cacaaI1aGaaGOmaiaaisdaaaaabaGaeyypa0JaaGimaiaac6cacaaI2aGaaGynaiaaiAdacaaIYaaabaGaeyinIWLaamOCamaaBaaaleaacaaIYaaabeaakiabg2da9iGacohacaGGPbGaaiOBamaaCaaaleqabaGaeyOeI0IaaGymaaaakmaabmaabaGaaGimaiaac6cacaaI2aGaaGynaiaaiAdacaaIYaaacaGLOaGaayzkaaGaeyisISRaaGinaiaaigdadaahaaWcbeqaaiaad+gaaaaakeaacaqGtbGaaeyAaiaab6gacaqGJbGaaeyzaiaaysW7caqGHbGaaeOBaiaabEgacaqGSbGaaeyzaiaaysW7caqGVbGaaeOzaiaaysW7caqGWbGaaeOCaiaabMgacaqGZbGaaeyBaiaaysW7caqGPbGaae4CaiaaysW7caqGNbGaaeyAaiaabAhacaqGLbGaaeOBaiaaysW7caqGHbGaae4CaiaacQdacaaMe8oabaGaamyqaiabg2da9iaadkhadaWgaaWcbaGaaGymaaqabaGccqGHRaWkcaWGYbWaaSbaaSqaaiaaikdaaeqaaaGcbaGaeyinIWLaamOCamaaBaaaleaacaaIXaaabeaakiabg2da9iaadgeacqGHsislcaWGYbWaaSbaaSqaaiaaikdaaeqaaaGcbaGaeyypa0JaaGOnaiaaicdadaahaaWcbeqaaiaab+gaaaGccqGHsislcaaI0aGaaGymamaaCaaaleqabaGaam4BaaaaaOqaaiabg2da9iaaigdacaaI5aWaaWbaaSqabeaacaWGVbaaaaGcbaGaaeOraiaab+gacaqGYbGaaGjbVlaabAgacaqGHbGaae4yaiaabwgacaaMe8UaamyqaiaadkeacaGG6aaabaGaaeOraiaabkhacaqGVbGaaeyBaiaaysW7caqGtbGaaeOBaiaabwgacaqGSbGaaeiBaiaabEcacaqGZbGaaGjbVlaabYgacaqGHbGaae4DaiaabYcacaaMe8Uaae4DaiaabwgacaaMe8UaaeiAaiaabggacaqG2bGaaeyzaiaacQdaaeaacqaH8oqBcqGH9aqpdaWcaaqaaiGacohacaGGPbGaaiOBaiaadMgadaWgaaWcbaGaaGymaaqabaaakeaaciGGZbGaaiyAaiaac6gacaWGYbWaaSbaaSqaaiaaigdaaeqaaaaaaOqaaiabgsJiCjGacohacaGGPbGaaiOBaiaadMgadaWgaaWcbaGaaGymaaqabaGccqGH9aqpcqaH8oqBciGGZbGaaiyAaiaac6gacaWGYbWaaSbaaSqaaiaaigdaaeqaaaGcbaGaeyypa0JaaGymaiaac6cacaaI1aGaaGOmaiaaisdacqGHxdaTciGGZbGaaiyAaiaac6gacaaIXaGaaGyoamaaCaaaleqabaGaam4BaaaaaOqaaiabg2da9iaaicdacaGGUaGaaGinaiaaiMdacaaI2aaabaGaeyinIWLaamyAamaaBaaaleaacaaIXaaabeaakiabg2da9iGacohacaGGPbGaaiOBamaaCaaaleqabaGaeyOeI0IaaGymaaaakmaabmaabaGaaGimaiaac6cacaaI0aGaaGyoaiaaiAdaaiaawIcacaGLPaaaaeaacqGH9aqpcaaIYaGaaGyoaiaac6cacaaI3aGaaGynamaaCaaaleqabaGaam4BaaaaaOqaaiabgsJiCjaabgeacaqGUbGaae4zaiaabYgacaqGLbGaaGjbVlaab+gacaqGMbGaaGjbVlaabMgacaqGUbGaae4yaiaabMgacaqGKbGaaeyzaiaab6gacaqGJbGaaeyzaiabg2da9iaaikdacaaI5aGaaiOlaiaaiEdacaaI1aWaaWbaaSqabeaacaWGVbaaaaaaaa@6591@

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,

1 f = 1 v 1 u 1 v = 1 f + 1 u = 1 10 cm + 1 -9 cm = – 1 90 cm v = -90cm Magnificationoftheconverginglensisgivenas: m = v u = -90 -9 =10 Sinceareaofeachsquare,A = 1 mm 2 Areaofeachsquareinthevirtual image = m 2 A = 10 2 ×1 mm 2 =100 mm 2 =1 cm 2 (b)Magnifyingpoweroftheconverginglensisgivenas: m c = d u = 25 cm 9 cm = 2.8 (c) The magnification in (a) is not equal to the magnifying power in (b). The magnification can be equal to the magnifying power only if the image is formed at the least distance of distinct vision.

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.

( a ) The maximum possible magnification is obtained when the image is formed at the least distance of distinct vision ( d = 25 cm ). Here, image distance, v = -d = -25 cm Focal length of the lens, f = 10 cm Let object distance = u From the lens formula, we obtain 1 v 1 u = 1 f 1 u = 1 v 1 f 1 u = 1 -25 cm 1 10 cm = – 7 50 cm u = -7.14cm Therefore, in order to view the squares distinctly, the distance of lens from them = 7.14 cm ( b ) Magnification is given as m = | v u | m = 25 cm 7.14 cm = 3.5 ( c ) Magnifying power is given as Magnifying power, m P = d | u | m P = 25 cm 7.14 cm = 3.5 Since, the image is formed at the least distance of distinct vision ( 25 cm ), therefore, the magnifying power is equal to the magnitude of magnification in this case.

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.

Here, areal magnification of each square, A = 6 .25 mm 2 Therefore, the linear magnification is given as: m= 6 .25 mm 2 =2.5 mm Sincemagnitudeofmagnificationisgivenas: m = v u v = mu v = 2.5u Given,focallengthofmagnifyingglass,f=10cm Fromthelensformula,weobtain: 1 f = 1 v 1 u 1 10 = 1 2.5u 1 u = 1 u 1 2.5 -1 = 1 u -1.5 2.5 u = -1.5 ×10 cm 2.5 = -6cm Since,v = 2.5u v = 2.5×-6 cm = -15cm Since the virtual image is formed at 15 cm, which is less than the least distance of distinct vision for a normal eye 25 cm , therefore, the squares cannot be seen distinctly.

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:

me=1+dfe

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:

mo=vo|uo|

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:

mo=Lfo

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:

m e = 1+ d f e = 1+ 25 cm 5 cm =6 Angularmagnificationofthecompoundmicroscopeis givenas: m= m e m o 30=6× m o m o = 30 6 =5 Angularmagnificationoftheobjectivelens=5 Letobjectdistanceforobjectlens= u o Letimagedistanceforobjectlens= v o Relationfortheangularmagnificationoftheobjective isgivenas: m o = v o u o 5= v o u o v o =5 u o Fromthelensformulaforobjectivelens,weobtain: 1 v o 1 u o = 1 f o 1 5 u o 1 u o = 1 1.25 1 u o 1 5 +1 = 1 1.25 6 5 u o = 1 1.25 cm u o = 1.25 cm 1 × 6 5 =1.5 cm Objectdistanceforobjectivelens, u o =1.5cm(i) Since, v o =5 u o (ii) Fromequation(i)and(ii),weobtain: v o =5×1.5 =7.5cm Letimagedistanceforeyepiece= v e Letobjectdistanceforeyepiece= u e Fromlensformulaforeyepiece,weobtain: 1 v e 1 u e = 1 f e Imagedistanceforeyepiece, v e =d=25cm 1 u e = 1 v e 1 f e = 1 25 cm 1 5 cm = 6 25 u e = 25 6 = 4.17 cm Distancebetweenobjectivelensandeyepiece= u e + v e =4.17 cm+7.5 cm =11.67 cm Distancebetweenobjectivelensandeyepiece=11.67 cm

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:

m= f o f e = 140 cm 5 cm =28 (b)Whenfinalimageisformedatleastdistanceofdistinct vision: Magnifyingpowerofthetelescopeisgivenas: m= f o f e 1+ f e d = 140 cm 5 cm 1+ 5 cm 25 cm =28 1+0.2 =28×1.2 =33.6

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:

θ=htu=1003000=130rad(i)                                   Let height of the image formed by the objective=hiAngle subtended by the image of the tower formed by the objective lens is given as:θ=hifo=hi140rad(ii)From equation (i)and(ii), we obtain:130=hi140hi=14030=4.7cm(c) Here, final image distance, d=25 cmMagnification of the eye piece is given as:m=1+dfe=1+25 cm5 cm=6Height of the final image of tower=mhi=6×4.7 cm=28.2cm

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.

Given, distance between the objective mirror and the secondary mirror, d = 20 mm Radius of curvature of objective mirror, R 1 = 220 mm Therefore, focal length of the objective mirror is given as: f 1 = R 1 2 = 220 mm 2 = 110mm Radius of curvature of secondary mirror, R 1 = 140 mm Therefore, focal length of the secondary mirror is given as: f 2 = R 2 2 = 140 mm 2 = 70mm When the object is placed at infinity, the parallel rays of light coming from the object at infinity will collect at the focus of the object lens and act as the imaginary object for the secondary mirror. Forsecondarymirror,objectdistance, u = f o – d u = 110 mm – 20 mm = 90mm Letimagedistanceforsecondarymirror = v Fromthemirrorformulaforsecondarymirror,weobtain: 1 v + 1 u = 1 f 2 1 v = 1 f 2 1 u 1 v = 1 70 mm 1 90 mm 1 v = 2 630 mm v = 630 mm 2 = 315mm Finalimagedistancefromsecondarymirror = 315mm

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:

tan2θ= s 1.5 m s =1.5 m×tan 7 o =0.184m =18.4cm Displacementofthereflectedspotoflight=18.4cm

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.

Given, refractive index of equiconvex lens, = 1.50Focal length of equiconvex lens, f = 30 cmHere, the liquid in contact with the equiconvex lens acts as the mirror.Let refractive index of liquid in contact with the equiconvex lens = fFor the combination of the equiconvex lens and the liquid in contact with the equiconvex lens, the equivalent focal length is given as:1f=1f1+1f2                                                         145 cm=130 cm+1f21f2=145 cm130 cm=190cmf2=90cmFor the equiconvex lens:Let radius of curvature of one surface=RRadius of curvature of the other surface=RRefrative index of equiconvex lens,  μ=1.50From lens maker’s formula for equiconvex lens, we get1f1=μ11R1R130 cm=1.512RR=30 cm0.5×2=30cmLet refractive index of liquid=μ1Radius of curvature of the liquid on the side of equiconvexlens=30cmRadius of curvature of the liquid on the side of plane mirror=From the lens maker’s formula for the liquid, we obtain:1f2=μ111R1190 cm=μ11130 cm0μ11=13μ1=43=1.33Refractive index of the liquid=1.33

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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.