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NCERT Solutions for Class 12 Physics Chapter 9 Ray Optics and Optical Instruments

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NCERT Solutions for Class 12 Physics Chapter 9 Ray Optics and Optical Instruments - FREE PDF Download

NCERT for Chapter 9 Ray Optics and Optical Instruments Class 12 Solutions by Vedantu, explains the principles of light propagation, reflection, refraction, and the working of various optical instruments. You'll learn how the light interacts with different surfaces and media, forming the basis for understanding a wide range of optical phenomena. The chapter discusses the workings of lenses and mirrors, explaining how they form images and the mathematical formulas that describe these processes. With Vedantu's Class 12 Physics NCERT Solutions, you will find step-by-step explanations of all the exercises in your textbook, ensuring that you understand the concepts thoroughly.

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Glance on Class 12 Physics Chapter 9 - Ray Optics and Optical Instruments

  • Chapter 9 Physics Class 12 explores how light bends when passing from one medium to another, governed by Snell's law.

  • Understanding how light bounces off surfaces, following the law of reflection. Examining the conditions under which light is completely reflected within a medium, leads to applications like optical fibres.

  • Analysing the formation of images by concave and convex lenses and mirrors, including deriving mirror and lens formulas. Learn different types of telescopes, such as reflecting and refracting telescopes, and their use in astronomy.

  • Understanding the construction and working of simple and compound microscopes, and how they magnify objects.

  • This article contains chapter notes, important questions, exemplar solutions, exercises, and video links for Chapter 9 - Ray Optics and Optical Instruments, which you can download as PDFs.

  • There are 31 fully solved questions in the exercise of class 12th Physics Chapter 9 Ray Optics and Optical Instruments.

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Access NCERT Solutions for Class 12 Physics Chapter 9 – Ray Optics and Optical Instruments

1. A small candle, 2.5 cm in size is placed at 27 cm in front of a concave mirror of radius of curvature 36cm. 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: We have,

Size of the candle, h=2.5cm

Let image size =h

Object distance, u=27cm

concave mirror’s curvature radius, R=36cm

Focal length of the concave mirror, f=R2=18cm

Using mirror formula,

1u+1v=1f

1v=1f1u

Where, u is the object distance, 

v is the image distance and 

f is the focal length.

Now, we put given values,

1v=118127

1v=3+254

1v=154

v=54cm

Therefore, the screen should be 54 cm away from the mirror to get a sharp image.

The formula for magnification of image is given by:

m=hh=vu

h=vu×h

h=5427×2.5

h=5cm

The height of the image of the candle is 5 cm. The negative sign shows that the image is inverted and real.

If the candle is moved nearer to the mirror, then the screen will have to be moved far from the mirror in order to get the image.


2. A 4.5 cm needle is placed 12cm away from a convex mirror of focal length 15cm. Give the location of the image and the magnification. Describe what happens as the needle is moved farther from the mirror.

Ans: Given that,

Height of the needle, h1 = 4.5cm

Object distance, u = 12cm

Focal length of the convex mirror, f = 15cm

Image distance = v

Using mirror formula,

1u+1v=1f

1v=1f1u

Now, we put given values,

1v=115112

1v=4+560

1v=960

v=6.7cm

Hence, the needle’s image is 6.7 cm away from the mirror and it is on the mirror’s other side.

The formula for magnification of image is given by:

m=h2h1=vu

h2=vu×h1

h2=6.712×4.5

h2=2.5cm

The image’s height is 2.5cm. The positive sign shows that the image is virtual, erect, and diminished.

If the needle is moved away from the mirror, the image will also move farther from the mirror, and the size of the image will decrease gradually.


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 9.4cm. 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 that,

Actual depth of the needle in water, h1=12.5cm

Apparent depth of the needle in water, h2=9.4cm

Refractive index of water =μ

The formula for refractive index is given by:

μ=h1h2

Put the given values,

μ=12.59.4

μ1.33

Hence, the water’s refractive index is about 1.33.

When water is replaced by a liquid of refractive index, μ=1.63.

The actual depth of the needle will be the same, but it's apparent depth will vary.

Let y be the new apparent depth of the needle. 

We will use the relation given below:

μ=h1y

y=h1μ

y=12.51.63

y=7.67cm

We get the new apparent depth of the needle to be 7.67cm. It is less than h2. Therefore, the microscope should be moved up to focus the needle again.

The distance by which the microscope would be moved up= 9.4  7.67 = 1.73cm.


4. Figures (a) and (b) show the 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 a glass when the angle of incidence in water is 45 with the normal to a water-glass interface (figure (c)).


Refraction of light

Ans: Given that,

For the glass -air interface,

Angle of incidence, i= 60

Angle of refraction, r=35

We can use Snell’s law,

μga=sinisinr

μga=sin60sin35

μga=1.51……(i)

For the air-water interface,

Angle of incidence, i= 60

Angle of refraction, r=47

We can use Snell’s law,

μwa=sinisinr

μwa=sin60sin47

μwa=1.184……(ii)

Using (i) and (ii), the relative refractive index of glass with respect to water can be derived as:

μgw=μgaμwa

μgw=1.511.184

μgw=1.275

For the glass - water interface,

Angle of incidence, i= 45

Angle of refraction, =r

We can use Snell’s law,

μgw=sinisinr

1.275=sin45sinr

sinr=0.5546

r=sin1(0.5546)

r=38.68

Hence, the angle of refraction at the water – glass interface is 38.68.


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: Provided that,

Bulb’s actual depth in water, d1=80cm=0.8m

Water’s refractive index, μ=1.33

The following diagram represents the given setup:


Light rays coming from the bulb

Where i is the Angle of incidence 

r is the Angle of refraction, r=90

As the bulb acts as a point source, the emergent light would be considered as a circle of radius, R=AC2=AO=OB

Snell’s law may be used as follows:

μ=sinrsini

1.33=sin90sini

sini=11.33

i=48.75

Considering the given diagram, we have the relation:

tani=OCOB=Rd1

R=tan48.75×0.8

R=0.91m

Area of the surface of water =πR2=π(0.91)2=2.61m2

Clearly, the area of the water surface through which the light from the bulb could project is about 2.61m2.


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:  The minimum deviation angle and the angle of the prism is as shown in the figure given below: 


Refraction through prism

Angle of minimum deviation, δm=40 

Angle of the prism, A=60

Refractive index of water, μ=1.33

Refractive index of the material of the prism =μ

The relation between angle of deviation with refractive index is given by:

μ=sin(A+δm2)sin(A2)

μ=sin(60+402)sin(602)=sin50sin30

μ=1.532

Hence, the refractive index of the prism is 1.532.

Since the prism is placed in water, let δm be the new angle of minimum deviation for the same prism. 

The below figure shows the angle of the prism and the unknown minimum deviation angle.


Angle of deviation through prism

The refractive index of glass with respect to water is given by the relation:

μgw=μμ=sin(A+δm2)sin(A2)

μμsin(A2)=sin(A+δm2)

sin(A+δm2)=1.5321.33sin(602)=0.5759

A+δm2=sin1(0.5759)=35.16

60+δm=70.32

δm=10.32

Hence, the new minimum angle of deviation is 10.32.


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: Given that,

Refractive index of glass, μ=1.55

Focal length of the double-convex lens, f=20 cm

Radius of curvature of one face of the lens = R1

Radius of curvature of the other face of the lens = R2

Radius of curvature of the double-convex lens = R

R1=R; R2=R

We can use this formula:

1f=(μ1)[1R11R2]

120=(1.551)[1R+1R]

120=(0.55)[2R]

R=22cm

Hence, the radius of curvature of the double-convex lens is 22cm.


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 20cm?

Ans: Consider the given setup of a convex lens of focal length 20cm.


Light rays passing through concave lens
Here,

Object distance, u=+12 cm

Focal length of the convex lens, f=20 cm

Image distance =v

Using lens formula,

1v1u=1f

1v112=120

1v=120+112=860

v=608=7.5cm

Clearly, the image is formed 7.5cm away from the lens, toward its right.


b) a concave lens of focal length 16cm?

Ans: Consider the given setup of a concave lens of focal length 16cm.


concave mirror
Here,

Focal length of the concave lens, f=16cm

Image distance = v

Using lens formula,

1v1u=1f

1v=116+112

1v=3+448

1v=148

v=48cm

Clearly, the image is formed 48cm away from the lens, toward its right.


9. An object of size 3.0 cm is placed 14 cm in front of a concave lens of focal length 21cm. Describe the image produced by the lens. What happens if the object is moved further away from the lens?

Ans: Given that,

Size of the object, h1=3 cm

Object distance, u= 14 cm

Focal length of the concave lens, f=21 cm

Image distance = v

Using lens formula,

1v1u=1f

1v=121114

1v=2342

1v=542

v=425=8.4cm

Hence, the image is formed on the same side of the lens as the object, 8.4 cm away from it. The negative sign indicates that the image is erect and virtual. 

The formula for magnification of the image is given as:

m=h2h1=vu

h2=8.414×3=1.8cm

h2=1.8cm

Hence, the height of the image is 1.8 cm.

If the object is moved further away from the lens, then the virtual image will move towards the lens focus, but not beyond it. The image size will decrease with the increase in the distance of the object.


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: Given that,

Focal length of the convex lens, f1=30 cm

Focal length of the concave lens, f2=20 cm

Focal length of the system of lenses = f

The equivalent focal length of two lenses system in contact is given by:

1f=1f1+1f2

1f=130120=160

f=60cm

Hence, the focal length of the combination of lenses is 60 cm. The negative sign shows that the system of lenses acts as a diverging lens.


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)? What is the magnifying power of the microscope?

Ans: Given that,

Focal length of the objective lens, f1=2.0 cm

Focal length of the eyepiece, f2= 6.25 cm

Distance between the objective lens and the eyepiece, d = 15 cm

Least distance of distinct vision, d = 25 cm

lmage distance for the eyepiece, v2=25 cm

Object distance for the eyepiece = u2

Using lens formula,

1v21u2=1f2

1u2=1v21f2

1u2=12516.25

1u2=525

u2=5cm

The distance of image for the objective lens, v1=d+u2=155=10cm.

The distance of object for the objective lens =u1

Using lens formula,

1v11u1=1f1

1u1=1v11f1

1u1=11012

1u1=410

u1=2.5cm

Magnitude of the object distance, |u1|=2.5cm.

The compound microscope’s magnifying power is given by the relation:

m=v1|u1|(1+df2)

m=102.5(1+256.25)

m=4(1+4)=20

Hence, the magnifying power of the microscope is 20.


b) at infinity? What is the magnifying power of the microscope?

Ans: Given that, the final image is formed at infinity.

The distance of image of the eyepiece, v2= 

The distance of object of the eyepiece =u2

Using lens formula,

1v21u2=1f2

1u2=1v21f2

1u2=116.25

u2=6.25cm

The distance of image for the objective lens, v1=d+u2=156.25=8.75cm.

The distance of object for the objective lens =u1

Using lens formula,

1v11u1=1f1

1u1=1v11f1

1u1=18.7512

u1=2.59cm

Magnitude of the object distance, |u1|=2.59cm.

The compound microscope’s magnifying power is given by the relation:

m=v1|u1|(d|u2|)

m=8.752.59(256.25)

m=13.51

Hence, the magnifying power of the microscope is 13.51.


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: Given that,

Focal length of the objective lens, fo=8 mm=0.8 cm

Focal length of the eyepiece, fe=2.5 cm

The distance of the object for the Objective lens, uo=9.0 mm=0.9 cm

Least distance of distant vision, d=25 cm

Image distance for the eyepiece, ve=d=25 cm

Object distance for the eyepiece, ue

Using lens formula,

1ve1ue=1fe

1ue=1ve1fe

1ue=12512.5

1ue=1125

ue=2.27cm

Using lens formula, we can obtain image distance for the objective lens,vo, is given by:

1vo1uo=1fo

1vo=1uo+1fo

1vo=10.810.9

1vo=0.10.72

vo=7.2cm

The distance between the objective lens and the eyepiece,  |ue|+vo=2.27+7.2=9.47cm

The microscope’s magnifying power is given by the relation:

m=vo|uo|(1+dfe)

m=7.20.9(1+252.5)

m=8(1+10)=88

Hence, the magnifying power of the microscope is 88.


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: Given that,

Focal length of the objective lens, fo=144 cm

Focal length of the eyepiece, fe=6.0 cm

The telescope’s magnifying power is given by:

m=fofe

m=1446

m=24

The separation between the objective lens and the eyepiece is given by:

x=fo+fe

x=144+6=150cm

Hence, the magnifying power of the telescope is 24 and the distance between the objective lens and the eyepieces is 150cm.


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?

Ans: Given that,

Focal length of the objective lens, fo=15m=15×100=1500cm

Focal length of the eyepiece, fe= 1.0 cm

The telescope’s angular magnification is given as:

α=fofe

α=15001=1500

Hence, the refracting telescope’s angular magnification is 1500.


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: Given that,

Diameter of the moon, do=3.48×106m

Radius of the lunar orbit, ro=3.8×108m

Let d be the diameter of the moon image formed by the objective lens.

The angle subtended by the moon’s diameter is equal to the angle subtended by the image.

doro=dfo

3.48×1063.8×108=d15

d=13.74×102m=13.74cm

Hence, the diameter of the moon’s image formed by the objective lens is 13.74 cm.


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.

Ans: For a concave mirror, f<0.

When the object is placed on the left side of the mirror, then u<0.


convex mirror

Using mirror formula,

1u+1v=1f

1v=1f1u……(1)

If the object placed between f and 2f i.e.,2f<u<f:

12f>1u>1f

12f<1u<1f

1f12f<1f1u<0……(2)

Using equation (1), we get

12f<1v<0

Since 1v is negative, v is negative.

12f<1v

2f>v

v>2f

Therefore, image will lie beyond 2f.


b) a convex mirror always produces a virtual image independent of the location of the object.

Ans: For a convex mirror, f>0.

When the object is placed on the left side of the mirror, then u<0.


Light rays passing through glass slab

Using mirror formula,

1u+1v=1f

1v=1f1u

Using equation (2), we get:

1v<0

v>0

Thus, the image is formed on the mirror’s backside. 

Hence, a convex mirror always gives a virtual image, regardless of the object distance.


c) the virtual image produced by a convex mirror is always diminished in size and is located between the focus and the pole.

Ans: For a convex mirror, f>0.

Using mirror formula,

1u+1v=1f

1v=1f1u

But we have, u<0

1v>1f

v<f

Hence, the image formed is diminished and is located between the focus and the pole.


d) An object placed between the pole and the focus of a concave mirror produces a virtual and enlarged image.

Ans: For a concave mirror, f<0.

When the object is placed on the left side of the mirror, then u<0.

The object is placed between the focus and the pole.

f>u>0

1f<1u<0

1f1u<0

1v<0

v>0

The image is formed on the mirror’s right side. Hence, it is a virtual image.

For u<0,v>0 

1u>1v

v>u

Magnification, m=vu>1

Hence, the formed image is enlarged.


16. A small pin fixed on a tabletop 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: According to the question, 


Light rays through a glass pipe

Actual depth of the pin, d=15 cm

Apparent depth of the pin =d

Refractive index of glass, μ=1.5

The refractive index of glass is equal to the ratio of actual depth to the apparent depth, that is,

μ=dd

d=dμ

d=151.5=10cm

The distance at which the pin appears to be raised =dd=1510=5cm.

For a small incidence angle, this distance does not depend upon the slab location.


17. 

a) Figure 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?


convex lens placed at two different locations

Ans: Given that,

Refractive index of the glass fibre, μ1=1.68

Refractive index of the outer covering of the pipe, μ2=1.44

Angle of incidence = i

Angle Of refraction = r

Angle of incidence at the interface = i

The refractive index (μ) of the inner core - outer core interface is given as:

μ=μ2μ1=1sini

sini=μ1μ2

sini=1.441.68=0.8571

For the critical angle, total internal reflection (TIR) takes place only when i>i.

That is, when i>59.

Maximum angle of reflection, rmax=90i=9059=31.

Let imax be the maximum incidence angle.

The refractive index at the air – glass interface, μ1=1.68.

We can use the relation for the maximum angles of incidence and reflection as:

μ1=sinimaxsinrmax

sinimax=μ1×sinrmax

sinimax=1.68×sin31

sinimax=0.8652

imax60

Thus, all the ray’s incident at angles lying in the range 0<i<60  will suffer total internal reflection.


b) What is the answer if there is no outer covering of the pipe?

Ans: If the outer covering of the pipe is not present, then:

Refractive index of the outer pipe =μ1

Refractive index of air = 1

For the angle of incidence  i =90, we can use Snell’s law at the air – pipe interface as

μ2=sinisinr

1.68=sin90sinr

sinr=11.68

r=36.5

i=9036.5=53.5

Since, i>r, all incident rays will suffer total internal reflection.


18. 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: Given that,

Distance between the object and the image, d=3 m

Maximum focal length of the convex lens =fmax 

The maximum focal length is given by for real image:

fmax=d4

fmax=34=0.75m

Hence, for the required purpose, the maximum possible focal length of the convex lens is 0.75 m.


19. 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: The figure shows the given arrangement of convex lens.


Combination of two lens

Here,

Distance between the image (screen) and the object, D = 90 cm.

Distance between two locations of the convex lens, d = 20 cm.

Focal length of the lens = f

Focal length is related to d and D by:

f=D2d24D

f=9022024×90=77036

f=21.39cm

Clearly, the focal length of the convex lens is 21.39cm.


20. 

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?

Ans: Consider the diagram below which represents the combination of two lenses.


Two lens system

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

First, consider the case when the parallel beam of light falls on the convex lens.

Using lens formula, 

1v11u1=1f1

Where, object distance, u1=

Image distance =v1

1v1=1301=130

v1=30cm

The image will serve as a virtual object for the concave lens.

Using lens formula, 

1v21u2=1f2

Where, object distance =u2.

u2=308=22cm

Image distance =v2.

1v2=122120=1220

v2=220cm

The parallel incident beam seems to diverge from a point, that is, 220d2=2204=216cm from the centre of the combination of the two lenses.

Secondly, when the parallel beam of light falls, from the left, on the concave lens;

Using lens formula, 

1v21u2=1f2

Where, object distance, u2=.

Image distance =v2.

1v2=1201=120

v2=20cm

The image will serve as a real object for the convex lens.

Using lens formula, 

1v11u1=1f1

Where, object distance, =u1.

u1=(20+8)=28cm.

Image distance =v1.

1v1=130+128=1420

v1=420cm

Hence, the parallel incident beam seems to diverge from a point, that is =4204=416cm from the left of the centre of the combination of the two lenses. 

Thus, the answer does depend on the combination side at which the parallel beam of light is incident. The notion of effective focal length does not appear to be useful for this combination.


b) An object 1.5 cm in size is placed on the side of the convex lens in the arrangement (a) above. The distance between the object and the convex lens is 40cm. Determine the magnification produced by the two-lens system, and the size of the image.

Ans: Consider the given diagram of the previous arrangement as follows:


Light ray passing through a prism

Here, it is said that,

Height of the image, h1=1.5 cm

Object distance from the side of the convex lens, u1=40cm

|u1|=40cm

Using lens formula, 

1v11u1=1f1

1v1=130+140=1120

v1=120cm

Magnification, m=v1|u1|

m=12040=3

Hence, the magnification due to the convex lens is 3.

The image made by the convex lens acts as an object for the concave lens.

Using lens formula, 

1v21u2=1f2

Where, object distance =u2.

u2=1208=112cm.

Image distance =v2.

1v2=120+1112=922240

v2=224092cm

Magnification, m=|v1||u1|

m=224092×1112=2092

Hence, the magnification due to the concave lens is 2092.

The magnification due to the combination of the two lenses is calculated as:

m×m=3×2092=0.652

Thus,

h2h1=0.652

h2=0.652×1.5=0.98cm

Clearly, the height of the image is 0.98cm.


21. At what angle should a ray of light be incident on the face of a prism of refracting angle 60 so that it just suffers total internal reflection at the other face? The refractive index of the material of the prism is 1.524.

Ans: Consider the given figure below:


Combination of prisms

Angle of prism, A=60

i1 is the incidence angle.

r1 is the refracted angle.

r2 is the angle of incidence at the face AC.

eis the emergent angle, e=90.

Using Snell’s law,

μ=sinesinr2

1.524=sin90sinr2

sinr2=0.6562

r241

For refraction through prism, angle A=r1+r2.

We get,

r1=Ar2=6041

r1=19

Using Snell’s law,

μ=sini1sinr1

1.524=sini1sin19

sini1=0.496

i1=29.75

Hence, the incidence angle is 29.75.


22. A card sheet divided into squares each of size 1 mm2 is being viewed at a distance of 9 cm through a magnifying glass (a converging lens of focal length 9 cm) held close to the eye. 

a) What is the magnification produced by the lens? How much is the area of each square in the virtual image?

Ans: Given that,

Area of each square, A=1 mm2

Object distance, u=9cm

Focal length, f=10cm

Using lens formula,

1f=1v1u

110=1v19

v=90cm

Magnification, m=vu

m=9010=9

Area of each square in the virtual image =102A

102×1=100mm2=1cm2


b) What is the angular magnification (magnifying power) of the lens?

Ans: Magnifying power of the lens, m=d|u|

m=259=2.8


c) Is the magnification in (a) equal to the magnifying power in (b)? Explain.

Ans: The magnification in (a) is not the same as the magnifying power in (b).

The magnification magnitude is |vu| and the magnifying power is d|u|.

The two quantities will be same when the image is formed at the close point (25cm).


23. 

a) At what distance should the lens be held from the figure in Exercise 9.29 in order to view the squares distinctly with the maximum possible magnifying power?

Ans: The maximum possible magnification got when the image is made at the near point (d = 25 cm).

Image distance, v=d=25 cm

Focal length, f = 10 cm

Object distance = u

Using lens formula,

1f=1v1u

110=1251u

u=507cm=7.14cm

Hence, to view the squares distinctly, the lens should be kept 7.14cm away from them.


b) What is the magnification in this case?

Ans: Magnification, m=|vu|

m=25507=3.5


c) Is the magnification equal to the magnifying power in this case? Explain.

Ans: Magnifying power, m=du

m=25507=3.5=m

Since the image is made at the near point (25 cm), the magnifying power is equal to the magnification magnitude.


24. What should be the distance between the Object in Exercise 9.30 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?

Ans: Given that,

Area of the virtual image of each square, A=6.25 mm2

Area of each square, Ao=1 mm2

Hence, the linear magnification is given by:

m=AAo

m=6.251=2.5

But,

m=vu

v=2.5u

Focal length of the magnifying glass, f=10cm

Using lens formula,

1f=1v1u

110=12.5u1u

u=1.5×102.5cm=6cm

And,

v=2.5u

v=2.5×6=15cm

The virtual image is made at a distance of 15 cm, which is less than the near point of a normal eye. Hence it cannot be visible by the eye distinctly.


25. 

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?

Ans: Though the image size is larger than the object, the angular size of the image is equivalent to the angular size of the object. 

A magnifying glass supports one seeing the objects closer than the least distance of distinct vision. A closer object produces a larger angular size. 

A magnifying glass gives angular magnification. Without magnification, the object cannot be located closer to the eye. With magnification, the object can be set much closer to the eye.


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?

Ans: Yes, the angular magnification varies. 

When the length between the eye and a magnifying glass rises, the angular magnification reduces slightly because the subtended angle at the eye is imperceptibly less than the lenses. 

Image distance does not have any impact on angular magnification.


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?

Ans: The convex lens's focal length cannot be reduced by a more significant amount. 

This is because making lenses having tiny focal lengths is not easy. 

Spherical and chromatic aberrations are created by a convex lens having a petite focal length.


d) Why must both the objective and the eyepiece of a compound microscope have short focal lengths?

Ans: The angular magnification produced by the compound microscope’s eyepiece is:

[(25fe)+1]

Where, fe is the eyepiece's focal length.

It can be seen that if fe is small, then angular magnification of the eyepiece will be great.

The angular magnification of the compound microscope’s objective lens is given as fouo.

uo: Object distance for the objective lens

fo: Objective's focal length

The magnification is large when uo>fo

In the case of a microscope, the object is placed close to the objective lens. Hence, the object distance is tiny. 

Since uo is small, fo will be smaller. Therefore, fe and  fo are both small for the given condition.


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: We cannot collect much-refracted light when we put our eyes too close to the compound microscope's eyepiece. 

As a result, the field view reduces substantially. Hence, the image's clarity gets blurred. 

The best view of the eye for seeing through a compound microscope is at the eye-ring connected to the eyepiece. The exact location of the eye depends on the separation between the objective lens and the eyepiece.


26. An angular magnification (magnifying power) of 30X is desired using an objective of focal length 1.25 cm and an eyepiece of focal length 5 cm. How will you set up the compound microscope?

Ans: Given that,

Focal length of the objective lens, fo=1.25cm

Focal length of the eyepiece, fe=5 cm

Least distance of distinct vision, d = 25 cm

Angular magnification of the compound microscope = 30X

Total magnifying power of the compound microscope, m = 30

The eyepiece’s angular magnification is given by:

me=1+dfe

me=1+255

me=6

The objective lens angular magnification is given by:

m=mome

mo=mme

mo=306=5

We have, 

mo=vouo

5=vouo

vo=5uo……(1)

Using lens formula,

1fo=1vo1uo

11.25=15uo1uo

uo=1.5cm

And, vo=5uo=5×1.5=7.5cm

The object should be placed 1.5cm away from the objective lens to get the desired magnification.

Using lens formula,

1fe=1ve1ue

Where, ve=d=25cm

15=1251ue

ue=4.17cm

Separation between the eyepiece and the objective lens =|ue|+|vo|

|ue|+|vo|=4.17+7.5=11.67cm

Therefore, the separation between the eyepiece and the objective lens should be 11.67cm.


27. A small telescope has an objective lens of focal length 140 cm and an eyepiece of focal length 5.0 cm. What is the magnifying power of the telescope for viewing distant objects when

a) the telescope is in normal adjustment (i.e., when the final image is at infinity)?

Ans: Given that,

Focal length of the objective lens, fo=140cm

Focal length of the eyepiece, fe=5 cm

Least distance of distinct vision, d = 25 cm

When the telescope is in normal adjustment, formula for magnifying power is given by:

m=fofe

m=1405=28


b) the final image is formed at the least distance of distinct vision (25 cm)?

Ans: When the final image is formed at d, the formula for magnifying power of telescope is given by:

m=fofe(1+fed)

m=1405(1+525)=28[1+0.2]

m=33.6


28. 

a) For the telescope described in Exercise 9.34 (a), what is the separation between the objective lens and the eyepiece?

Ans: Given that,

Focal length of the objective lens, fo=140 cm

Focal length of the eyepiece, fe=5 cm

The separation between the objective lens and the eyepiece in normal adjustment =fo+fe=(140+5) cm=145cm


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? 

Ans: Given that,

Height of the tower, h1=100 m

Distance of the tower from the telescope, u = 3 km = 3000 m

The angle subtended by the tower at the telescope is given as:

θ=h1u

θ=1003000=130rad

The angle subtended by the image made by the objective lens is given by:

θ=h2fo

130=h2140

h2=4.7cm

Therefore, the objective lens forms a 4.7cm tall image of the tower.


c) What is the height of the final image of the tower if it is formed at 25 cm?

Ans: Given that,

Image is formed at a distance, d = 25cm

The eyepiece’s magnification is given by:

m=1+dfe

m=1+255

m=6

Height of the final image, =m×h2=6×4.7=28.2cm 

Hence, the final image’ height of the tower is 28.2cm.


29. A Cassegrain telescope uses two mirrors as shown in figure. Such a telescope is built with the mirrors 20 mm apart. If the radius of curvature of the large mirror is 220 mm and these all mirror is 140mm, where will the final image of an object at infinity be?


a telescope is built with the mirrors.png


Ans: A Cassegrain telescope contains two mirrors, one is an objective mirror and the second one is the secondary mirror. We need to find the distance of the final image from the secondary mirror. 

Given: distance between the objective mirror and the secondary mirror, d=20mm

Radius of curvature of the objective mirror, R1=220 mm

Hence, objective mirror’s focal length, f1=R12=110mm

Secondary mirror’s radius of curvature, R2=140 mm

Secondary mirror’s focal length, f2=R22=70mm

The image of an object set at infinity, made by the objective mirror, will serve as a virtual object for the secondary mirror.

Hence, the secondary mirror’s virtual object distance, u=f1d

u=11020=90mm

Using mirror formula,

1u+1v=1f2

1v=1f21u

Now, we put given values,

1v=170190

1v=97630

1v=2630

v=315mm

Clearly, the final image will be made 315 mm away from the secondary mirror.


30. Light incident normally on a plane mirror attached to a galvanometer coil retraces backwards as shown in figure. A current in the coil produces a deflection of 3.5 from the mirror. What is the displacement of the reflected spot of light on a screen placed 1.5 m away?


Light incident on plane mirror

Ans: Angle of deflection, θ=3.5

Screen distance from the mirror, D=1.5 m

The reflected rays will deflect by an amount twice the deflection angle,  2θ=7.

The displacement of the light’s reflected spot on the screen is given as:

tan2θ=d1.5

d=1.5×tan7=0.184m=18.4cm

Hence, the displacement of the reflected spot of light is 18.4 cm.


31. Figure 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 45.0 cm. The liquid is removed and the experiment is repeated. The new distance is measured to be 30.0 cm. What is the refractive index of the liquid?


Equiconvex lens in liquid layer

Ans: An equiconvex lens is in touch with a liquid layer on a plane mirror top. A small needle placed on the principal axis is moved along the axis until its inverted image will be at the position of the needle.

Convex lens focal length, f1=30 cm

The liquid will behave as a mirror. 

Liquid’s focal length = f2

System’s focal length, f = 45 cm

The equivalent focal length is given as:

1f=1f1+1f2

1f2=1f1f1

1f2=145130=190

f2=90cm

Let the lens’s refractive index be μ1 and curvature radius of one surface be R.

Hence, the curvature radius of the other surface is  R.

We use,

1f1=(μ11)[1R1R]

130=(1.51)[2R]

R=30cm

Let μ2 be the liquid’s refractive index.

Liquid’s curvature radius on the side of the plane mirror =.

Curvature radius of the liquid on the side of the lens, R= 30 cm.

We use,

1f2=(μ21)[1R1]

190=(μ21)[1300]

(μ21)=13

μ2=1.33

Clearly, the liquid’s refractive index is 1.33.


Key Points at a Glance

1. Straight-line Nature of Light:

  • In optics, light is conceptualized as a straight-line ray.

  • Every object is associated with an image in this optical model.


2. Reflection Phenomenon:

  • Reflection is the process of altering the course of light without changing the medium.

  • Upon striking a surface, light reflects back into the same medium from which it originated.


3. Reflection Laws:

  • Two fundamental laws govern reflection.

  • The angle of incidence (I) equals the angle of reflection (r).

  • At the point of incidence, the incident ray, reflected ray, and the normal to the reflecting surface lie in the same plane.


4. Spherical Mirrors:

  • Reflecting surfaces of spherical mirrors are enclosed within hollow spheres.

  • These mirrors come in two types: concave and convex.


Ray Optics and Optical Instruments Chapter Summary - Class 12 NCERT Solutions

  • Reflection is governed by the equation ∠i = ∠r′ and refraction by the Snell’s law, sinisinr=μ , where the incident ray, reflected ray, refracted ray and normal lie in the same plane, ⎧ is the refractive index of glass medium.


the refractive index of glass medium


  • The critical angle of incidence C for a ray incident from a denser to rarer medium, is that angle for which the angle of refraction is 90°. For i > C, total internal reflection occurs.


total internal reflection occurs


  • Cartesian Sign Convention: Distance measured in the same direction as the incident light are positive; those measured in the opposite direction are negative.  All distances are measured from the pole/optical centre of the mirror/lens on the principal axis. The heights measured upwards above x-axis and normal to the principal axis of the mirror/lens are taken as positive. The heights measured downwards are taken as negative.


The heights measured downwards are taken as negative


  • Mirror Equation:

1v+1u=1f

where u and v are object and image distances, respectively, and f is the focal length of the mirror. f is (approximately) half the radius of curvature R. f is negative for a concave mirror; f is positive for a convex mirror.


  • For a prism of the angle A, of refractive index  μ2 placed in a medium of refractive index μ1

μ21=μ2μ1=sin[(A+δm)2]sin(A2)

Where δm is the angle of minimum deviation.


the angle of minimum deviation


  • For refraction through a spherical interface (from medium 1 to 2 of refractive index
    μ1 and μ2 , respectively 

μ2vμ1u=μ2μ1R

Thin lens formula

1v1u=1f

Lens maker’s formula

1f=μ2μ1μ1(1R11R2)

Where, f is positive for a converging lens; f is negative for a diverging lens.


f is negative for a diverging lens


  • The power of a lens P=1f

The SI unit for power of a lens is dioptre (D) 

1 D = 1 m–1 .

If several thin lenses of focal length f1 , f2 , f3 ,.. are in contact, the effective focal length of their combination, is given by 1f=1f1+1f2+1f3+...

The total power of a combination of several lenses is

P = P1 + P2 + P3 + …


  • Dispersion is the splitting of light into its constituent colour.


the splitting of light into its constituent colour


  • Magnifying power m of a simple microscope is given by m=1+Df, where D = 25 cm is the least distance of distinct vision and f is the focal length of the convex lens. 

If the image is at infinity, m=Df.


the least distance of distinct vision and f is the focal length of the convex lens


  • For a compound microscope, the  magnifying power is  given by m=me×m0, where me=1+Dfe, is the magnification due to the eyepiece  and m0 is  the  magnification  produced  by  the  objective. Approximately,

m=Lf0=Dfe

Where fo and fe are the focal lengths of the objective and eyepiece, respectively, and L is the distance between their focal points.


the distance between their focal points


  • Magnifying power m of a telescope is the ratio of the angle ® subtended at the eye by the image to the angle 〈 subtended at the eye by the object. 

m=βα=f0fe

Where fo and fe are the focal lengths of the objective and eyepiece, respectively.


the objective and eyepiece


Overview of Deleted Syllabus for CBSE Class 12 Physics Ray Optics and Optical Instruments

Chapter

Dropped Topics

Ray Optics and Optical Instruments

9.3 Refraction (deleted only advanced sunrise and delayed sunset)

9.4.1 (i) Mirage

9.4.1 (ii) Diamond

9.7 Some Natural Phenomena Due to Sunlight

9.7.1 The Rainbow

9.7.2 Scattering of Light

Exercise 9.18



Conclusion

NCERT Class 11 Physics Chapter 2 Exercise Solutions on Ray Optics and Optical Instruments provided by Vedantu provides a thorough understanding of how light behaves and interacts with different media. The chapter covers fundamental principles and their applications, equipping students with the knowledge to understand and work with various optical instruments. This chapter introduces the fundamental concepts of ray optics, focusing on the behaviour of light as it travels through different media and interfaces. These concepts are essential for mastering the topic and are often tested in exams. From previous year's question papers, typically around 3–4 questions are asked from this chapter.


Other Study Material for CBSE Class 12 Physics Chapter 9



Chapter-Specific NCERT Solutions for Class 12 Physics

Given below are the chapter-wise NCERT Solutions for Class 12 Physics. Go through these chapter-wise solutions to be thoroughly familiar with the concepts.




Discover relevant links for NCERT Class 12 Physics in Hindi, offering comprehensive study materials, solutions, and resources to enhance understanding and aid in exam preparation.




Chapter-Specific NCERT Solutions for Class 12 Physics

Given below are the chapter-wise NCERT Solutions for Class 12 Physics. Go through these chapter-wise solutions to be thoroughly familiar with the concepts.


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FAQs on NCERT Solutions for Class 12 Physics Chapter 9 Ray Optics and Optical Instruments

1. Where can I get Solutions for Ray Optics Class 12?

Students can get Ray Optics class 12 NCERT solutions online on the website of Vedantu. It is downloadable for free. The solutions are provided in a simple manner with a clear explanation of concepts. Here students will find answers to all the NCERT questions.


The answers have been written by subject matter experts, to help students. Students will find accurate answers along with, illustrations, diagrams, comparison tables, and pictures in the explanation of every solution. The Ray optics class 12 NCERT solutions PDF is the best guide for every student when it comes to clearing of doubts. If students are pressed for time they can easily refer to the solutions given here thereby cutting their revision time by half.

2. How can I Study for Ray Optics Class 12?

Firstly, when it comes to studying anything remember that studying it three times helps. Three is the magic number you have to target. Once three revisions have been completed, work on the exercises at the back of the chapter. The Ray optics class 12 NCERT solutions will help students if they get stuck in any of the problems. The solutions are written in a lucid, practical style with diagrams and illustrations wherever necessary. Ray diagrams are drawn to explain the key points. Students will also find it helpful to go through past year papers and sample questions. They will need to practice ray diagrams for convex and concave mirrors if they want to score well. Ray Optics class 12 NCERT solutions PDF will help students in their exam preparation.

3. What is the Meaning of Ray Optics?

Ray optics deals with the propagation of light through media like a convex and concave lens. Some of the other topics covered in this chapter are refraction, mirror equation, and focal length of spherical mirrors. Additionally, three important phenomena of light are observed, namely, refraction, dispersion, and reflection. Students who are facing difficulty with Ray Optics class 12 NCERT should download and consult the Ray Optics class 12 solutions. This will benefit them greatly. Their conceptual understanding will improve by going through the solved questions. They will have a chance to compare, identify, and correct their mistakes by referring to the solutions.

4. What are the important topics of Class 12 Physics Chapter 9 Ray Optics and Optical Instruments?

Ray Optics is a vast and difficult chapter which requires proper guidance to understand each and every topic properly. Vedantu provides NCERT SOlutions to help students understand the chapter better and solve the questions based on the chapter effortlessly. In case students have any doubts, they can also refer to the online notes created by expert teachers at Vedantu. Students can also register for online classes where they can interact with the teacher and clear their doubts right away. A few of the important topics in the chapter are:

  • Total Internal Reflection

  • Refraction Through A Prism

  • Image formation by spherical lenses

  • Image formation by spherical mirrors

  • Telescope

  • Microscope

  • Eye

  • Natural Phenomena Due to Light

  • Power combination of lenses

5. What type of questions are asked from optics in the board exam?

Optics is a very important chapter for the Class 12 board exam as well as future reference and preparation of competitive exams. There are a few crucial topics that you definitely cannot afford to miss in the Chapter. Reflection of Light, Spherical Mirrors, Refraction of Light, Prism, Simple Microscope, Telescope, Lens and Optical Instruments are some of the important topics of the chapter. The type of questions asked from this chapter in board exams includes numerical and definitions. 

You can find the important questions for exam purposes from Vedantu's website, which will definitely help you to understand the types of questions usually asked in the board exams for class 12 Physics Chapter ray optics.

6. Is Ray Optics important for NEET?

Going by the chapter wise distribution of weightage for the NEET exam, approximately 5% of the total questions in the question papers of the past eight years have been asked from Ray Optics. A few important topics are:

  • Reflection

  • Refraction Through A Glass Slab

  • Total Internal Reflection

  • Refraction Through Spherical Surfaces And Lenses

  • Refraction, Dispersion Through A Prism

  • The Human Eye

  • Microscopes and Telescopes

7. What is the difference between ray optics and wave optics?

The main point of difference between Ray optics and Wave optics is:

Ray optics works with light as it travels in the path of a line, refracts from a given surface or reflects from it, and later continues as a straight line towards other surfaces. 

Wave optics is used as a standard to analyse the propagation of light when there exist a lot of photons.

You can learn in detail about the differences between the two topics from Vedantu's NCERT solutions for class 12 Physics Chapter 9, ray optics.

8. What are the most important topics in Ray Optics?

The most important topics in Ray optics are as follows:

  • Application Of Refraction

  • Total Internal Reflection 

  • Derivation Of Prism Refractive Index Formula

  • Derivation Of Refraction At A Spherical Surface

  • Applications Of Scattering 

  • Rayleigh Criteria

A good idea is to follow the NCERT solutions PDF provided by Vedantu to understand and take note of these important concepts to have a sure shot chance of scoring well in the exams.

9. What are optics and their types?

The discipline that studies the properties of a wave of light is called Optics. Optics can be further divided into three major subtypes:

  • Interference

  • Diffraction

  • Polarisation

One can access more about these topics on the Vedantu website and get all the required information free of cost and also utilise the Vedantu Mobile App.

10. What is the purpose of ray optics discussed in Ray Optics Class 12 NCERT Solutions?

Ray optics, also known as geometrical optics, studies the behaviour of light by treating it as a collection of rays. It helps us understand phenomena like reflection, refraction, and image formation by lenses and mirrors using geometric principles.

11. How many hours to complete Ray Optics NCERT Solutions?

The time to complete this chapter depends on your learning pace and background. It can take anywhere from a few hours to a week or more. Focus on understanding the concepts, solving practice problems, and referring to the NCERT solutions for clarification.

12. What is important in Class 12 Physics Chapter 9 Exercise Solutions?

Here are some key things to understand in ray optics:

  • Laws of reflection and refraction

  • Sign conventions for mirrors and lenses (focal length, object/image distance)

  • Mirror and lens equation for image formation

  • Ray diagrams for reflection and refraction

  • Applications of lenses and mirrors in optical instruments

13. What are the advantages of Ray Optics mentioned in Class 12 Ray Optics NCERT Solutions?

Ray optics is a powerful tool because:

  • It's a simple approach to understanding light behaviour for many practical applications.

  • It helps design and analyses optical instruments like telescopes, microscopes, and eyeglasses.

  • It lays the foundation for more advanced optics concepts like wave optics.

14. What is a ray of light called?

A ray of light isn't a formal scientific term, but it's a convenient way to visualize the propagation of light as a straight line.

15. Is Ray Optics Class 12 Physics Ch 9 NCERT Solutions tough?

The difficulty depends on your maths and physics background. Class 12 Physics Ray Optics NCERT Solutions involve applying geometric concepts and algebraic equations. With a solid foundation and practice, you can grasp the concepts effectively.

16. How can NCERT Solutions Chapter 9 Physics Class 12 help me learn the key concepts of ray optics?

By going through solved problems in Class 12 Physics Chapter 9 NCERT Solutions, you see how formulas and principles are applied to various scenarios. This helps solidify your understanding of core concepts like reflection, refraction, mirror and lens equations, and image formation.

17. What are the main topics covered in Class 12 Physics Chapter Ray Optics NCERT Solutions?

The main topics covered in Ch 9 Physics Class 12 include:

  • Laws of reflection and refraction

  • Image formation by plane and spherical mirrors

  • Lens formula and magnification for convex and concave lenses

  • Optical instruments like microscopes and telescopes

  • Phenomena such as dispersion, total internal reflection, and the working principles of optical fibres