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Ray Optics - 2 PPT Physics Class 12

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RAY OPTICS - II 
1. Refraction through a Prism
2. Expression for Refractive Index of Prism
3. Dispersion 
4. Angular Dispersion and Dispersive Power
5. Blue Colour of the Sky and Red Colour of the Sun
6. Compound Microscope
7. Astronomical Telescope (Normal Adjustment)
8. Astronomical Telescope (Image at LDDV)
9. Newtonian Telescope (Reflecting Type)
10.Resolving Power of Microscope and Telescope
Page 2


RAY OPTICS - II 
1. Refraction through a Prism
2. Expression for Refractive Index of Prism
3. Dispersion 
4. Angular Dispersion and Dispersive Power
5. Blue Colour of the Sky and Red Colour of the Sun
6. Compound Microscope
7. Astronomical Telescope (Normal Adjustment)
8. Astronomical Telescope (Image at LDDV)
9. Newtonian Telescope (Reflecting Type)
10.Resolving Power of Microscope and Telescope
Refraction of Light through Prism:
A
Refracting Surfaces
Prism
i
d
A
B C
e
O
P
Q
r
1
r
2
N
1
N
2
D
In quadrilateral  APOQ,
A + O = 180° …….(1) 
(since N
1
and N
2
are normal)
In triangle OPQ,
r
1 
+ r
2
+ O = 180° …….(2) 
In triangle DPQ,
d = (i - r
1
) + (e - r
2
)
d = (i + e) – (r
1
+ r
2
)   …….(3) 
From (1) and (2),
A = r
1 
+ r
2
From (3),
d = (i + e) – (A)
or
i + e = A + d
µ
Sum of angle of incidence and angle 
of emergence is equal to the sum of 
angle of prism and angle of deviation.
Page 3


RAY OPTICS - II 
1. Refraction through a Prism
2. Expression for Refractive Index of Prism
3. Dispersion 
4. Angular Dispersion and Dispersive Power
5. Blue Colour of the Sky and Red Colour of the Sun
6. Compound Microscope
7. Astronomical Telescope (Normal Adjustment)
8. Astronomical Telescope (Image at LDDV)
9. Newtonian Telescope (Reflecting Type)
10.Resolving Power of Microscope and Telescope
Refraction of Light through Prism:
A
Refracting Surfaces
Prism
i
d
A
B C
e
O
P
Q
r
1
r
2
N
1
N
2
D
In quadrilateral  APOQ,
A + O = 180° …….(1) 
(since N
1
and N
2
are normal)
In triangle OPQ,
r
1 
+ r
2
+ O = 180° …….(2) 
In triangle DPQ,
d = (i - r
1
) + (e - r
2
)
d = (i + e) – (r
1
+ r
2
)   …….(3) 
From (1) and (2),
A = r
1 
+ r
2
From (3),
d = (i + e) – (A)
or
i + e = A + d
µ
Sum of angle of incidence and angle 
of emergence is equal to the sum of 
angle of prism and angle of deviation.
Variation of angle of deviation with angle of incidence:
d
i
0
i = e
d
m
When angle of incidence increases,            
the angle of deviation decreases.  
At a particular value of angle of incidence 
the angle of deviation becomes minimum 
and is called ‘angle of minimum deviation’.
At d
m
, i = e and      r
1 
= r
2 
= r (say)
After minimum deviation, angle of deviation 
increases with angle of incidence.
Refractive Index of Material of Prism:
A = r
1
+ r
2
A = 2r
r = A / 2
i + e = A + d
2 i = A + d
m
i = (A + d
m
) / 2
According to Snell’s law,
sin i
µ = 
sin r
1
sin i
sin r
=
µ =
sin
(A + d
m
)
2
sin
A
2
Page 4


RAY OPTICS - II 
1. Refraction through a Prism
2. Expression for Refractive Index of Prism
3. Dispersion 
4. Angular Dispersion and Dispersive Power
5. Blue Colour of the Sky and Red Colour of the Sun
6. Compound Microscope
7. Astronomical Telescope (Normal Adjustment)
8. Astronomical Telescope (Image at LDDV)
9. Newtonian Telescope (Reflecting Type)
10.Resolving Power of Microscope and Telescope
Refraction of Light through Prism:
A
Refracting Surfaces
Prism
i
d
A
B C
e
O
P
Q
r
1
r
2
N
1
N
2
D
In quadrilateral  APOQ,
A + O = 180° …….(1) 
(since N
1
and N
2
are normal)
In triangle OPQ,
r
1 
+ r
2
+ O = 180° …….(2) 
In triangle DPQ,
d = (i - r
1
) + (e - r
2
)
d = (i + e) – (r
1
+ r
2
)   …….(3) 
From (1) and (2),
A = r
1 
+ r
2
From (3),
d = (i + e) – (A)
or
i + e = A + d
µ
Sum of angle of incidence and angle 
of emergence is equal to the sum of 
angle of prism and angle of deviation.
Variation of angle of deviation with angle of incidence:
d
i
0
i = e
d
m
When angle of incidence increases,            
the angle of deviation decreases.  
At a particular value of angle of incidence 
the angle of deviation becomes minimum 
and is called ‘angle of minimum deviation’.
At d
m
, i = e and      r
1 
= r
2 
= r (say)
After minimum deviation, angle of deviation 
increases with angle of incidence.
Refractive Index of Material of Prism:
A = r
1
+ r
2
A = 2r
r = A / 2
i + e = A + d
2 i = A + d
m
i = (A + d
m
) / 2
According to Snell’s law,
sin i
µ = 
sin r
1
sin i
sin r
=
µ =
sin
(A + d
m
)
2
sin
A
2
Refraction by a Small-angled Prism for Small angle of Incidence:
sin i
µ = 
sin r
1
sin e
µ = 
sin r
2
and
If i is assumed to be small, then r
1
, r
2
and e will also be very small.  
So, replacing sines of the angles by angles themselves, we get
i
µ = 
r
1
and
e
µ = 
r
2
i + e = µ (r
1
+ r
2
) = µ A
But  i + e = A + d
So, A + d = µ A
or
d = A (µ – 1)
Page 5


RAY OPTICS - II 
1. Refraction through a Prism
2. Expression for Refractive Index of Prism
3. Dispersion 
4. Angular Dispersion and Dispersive Power
5. Blue Colour of the Sky and Red Colour of the Sun
6. Compound Microscope
7. Astronomical Telescope (Normal Adjustment)
8. Astronomical Telescope (Image at LDDV)
9. Newtonian Telescope (Reflecting Type)
10.Resolving Power of Microscope and Telescope
Refraction of Light through Prism:
A
Refracting Surfaces
Prism
i
d
A
B C
e
O
P
Q
r
1
r
2
N
1
N
2
D
In quadrilateral  APOQ,
A + O = 180° …….(1) 
(since N
1
and N
2
are normal)
In triangle OPQ,
r
1 
+ r
2
+ O = 180° …….(2) 
In triangle DPQ,
d = (i - r
1
) + (e - r
2
)
d = (i + e) – (r
1
+ r
2
)   …….(3) 
From (1) and (2),
A = r
1 
+ r
2
From (3),
d = (i + e) – (A)
or
i + e = A + d
µ
Sum of angle of incidence and angle 
of emergence is equal to the sum of 
angle of prism and angle of deviation.
Variation of angle of deviation with angle of incidence:
d
i
0
i = e
d
m
When angle of incidence increases,            
the angle of deviation decreases.  
At a particular value of angle of incidence 
the angle of deviation becomes minimum 
and is called ‘angle of minimum deviation’.
At d
m
, i = e and      r
1 
= r
2 
= r (say)
After minimum deviation, angle of deviation 
increases with angle of incidence.
Refractive Index of Material of Prism:
A = r
1
+ r
2
A = 2r
r = A / 2
i + e = A + d
2 i = A + d
m
i = (A + d
m
) / 2
According to Snell’s law,
sin i
µ = 
sin r
1
sin i
sin r
=
µ =
sin
(A + d
m
)
2
sin
A
2
Refraction by a Small-angled Prism for Small angle of Incidence:
sin i
µ = 
sin r
1
sin e
µ = 
sin r
2
and
If i is assumed to be small, then r
1
, r
2
and e will also be very small.  
So, replacing sines of the angles by angles themselves, we get
i
µ = 
r
1
and
e
µ = 
r
2
i + e = µ (r
1
+ r
2
) = µ A
But  i + e = A + d
So, A + d = µ A
or
d = A (µ – 1)
Dispersion of  White Light through Prism:
The phenomenon of  splitting a ray of white light into its constituent colours
(wavelengths) is called dispersion and the band of colours from violet to red
is called spectrum (VIBGYOR).
d
r
A
B C
D
White 
light
d
v
Cause of Dispersion:
sin i
µ
v
= 
sin r
v
sin i
µ
r
= 
sin r
r
and
Since  µ
v
> µ
r
,   r
r
> r
v
So, the colours are refracted at different 
angles and hence get separated.
Screen
N
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FAQs on Ray Optics - 2 PPT Physics Class 12

1. What is ray optics?
Ans. Ray optics, also known as geometrical optics, is a branch of optics that studies the behavior of light as rays. It considers light as a straight line or ray that travels in a uniform medium and undergoes reflection, refraction, and absorption.
2. How does reflection occur in ray optics?
Ans. Reflection in ray optics occurs when a light ray bounces off a surface. It obeys the law of reflection, which states that the incident angle is equal to the reflected angle, and both lie in the same plane as the normal to the surface.
3. What is refraction in ray optics?
Ans. Refraction in ray optics is the bending of light as it passes from one medium to another. It occurs due to the change in the speed of light when it transitions between media with different optical densities. The bending is governed by Snell's law.
4. How can we determine the path of a light ray in ray optics?
Ans. In ray optics, the path of a light ray can be determined using two laws: the law of reflection and Snell's law of refraction. These laws provide mathematical relationships that allow us to predict the direction and angle of the ray after reflection or refraction.
5. What are the applications of ray optics?
Ans. Ray optics has numerous practical applications. It is used in the design of mirrors, lenses, and optical instruments like telescopes and microscopes. It is also employed in technologies such as fiber optics, laser systems, and optical communication.
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