CLASS: SS 2 THIRD TERM: E-LEARNING NOTES - Goodwill ...

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This material is NOT the property of Goodwill Group of Schools but has been adopted by the school management as additional teaching aid for teachers and students. Please this material should not be commercialized in any form without prior formal engagement with school management. This material was developed for the use of teachers and students of the Goodwill Group of Schools. All financial commitment has been duly fulfilled by the school management. It is prohibited therefore to commercialize this document in any form without prior formal discussion with the management. CLASS: SS 2 SUBJECT: PHYSICS THIRD TERM: E-LEARNING NOTES THIRD TERM SCHEME OF WORK WEEK TOPIC THEME: WAVES-MOTION WITHOUT MATERIAL TRANSFER 1. Revision/Production and Propagation of Waves: (a) Production of mechanical waves (b) Graphical representation of wave (c) Terms as applied to waves (d) Relationship between f, T and Ξ» (e) Simple solved problems on f, T and Ξ» 2. Types of waves&Wave equation ( y = Asin(Ο‰t – k) 3. Properties of Waves: (a)Reflection of waves (i)laws of reflection (b)Superposition of waves(i)Two waves in thesame direction (progressive wave) (ii)Two waves in oppositedirection(standing or stationary waves)(c)Refractionof waves: laws of refraction. 4. Light waves:(a)Sources of light (b)Light and matter (c)Transmission of light (d)Reflectionof light at(i)Plane mirror surfaces(ii)Curved mirrors(e)Formation of images by (i)Plane mirrors (ii)Curved mirrors (f)Laws of reflection (g)Parabolic mirror as application of reflection of light on curved surfaces. 5. Light waves: (a)Refraction of light through (i)Rectangular glass block (ii)Triangular prism(b) Laws refraction (c)Critical angle and total internal reflection (d)Angle ofdeviation(e)Sun’s energy and the radiation to the earth (f)Refraction of light through: (i)Converging lenses(ii)Diverging lenses. Dispersion of white light and colour mixing. 6. Application of lenses: (a)Human Eye (i) The human Eye (ii) Defects of vision (iii) Correction of defects. 7. MID – TERM BREAK 8. Application of lenses (contd):(b) The Camera (c) Comparing the human eye with the camera(d)Simple and compound microscope (e) Telescope (f)Simple periscope (g)filmprojector

Transcript of CLASS: SS 2 THIRD TERM: E-LEARNING NOTES - Goodwill ...

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additional teaching aid for teachers and students. Please this material should not be commercialized in any form without

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CLASS: SS 2 SUBJECT: PHYSICS

THIRD TERM: E-LEARNING NOTES

THIRD TERM SCHEME OF WORK

WEEK TOPIC

THEME: WAVES-MOTION WITHOUT MATERIAL TRANSFER

1. Revision/Production and Propagation of Waves: (a) Production of mechanical waves (b)

Graphical representation of wave (c) Terms as applied to waves (d) Relationship between

f, T and Ξ» (e) Simple solved problems on f, T and Ξ»

2. Types of waves&Wave equation ( y = Asin(Ο‰t – k𝒙)

3. Properties of Waves: (a)Reflection of waves (i)laws of reflection (b)Superposition of waves(i)Two waves in thesame direction (progressive wave) (ii)Two waves in oppositedirection(standing or stationary waves)(c)Refractionof waves: laws of refraction.

4. Light waves:(a)Sources of light (b)Light and matter (c)Transmission of light (d)Reflectionof light at(i)Plane mirror surfaces(ii)Curved mirrors(e)Formation of images by (i)Plane mirrors (ii)Curved mirrors (f)Laws of reflection (g)Parabolic mirror as application of reflection of light on curved surfaces.

5. Light waves: (a)Refraction of light through (i)Rectangular glass block (ii)Triangular prism(b) Laws refraction (c)Critical angle and total internal reflection (d)Angle ofdeviation(e)Sun’s energy and the radiation to the earth (f)Refraction of light through: (i)Converging lenses(ii)Diverging lenses. Dispersion of white light and colour mixing.

6. Application of lenses: (a)Human Eye (i) The human Eye (ii) Defects of vision (iii) Correction of defects.

7. MID – TERM BREAK

8. Application of lenses (contd):(b) The Camera (c) Comparing the human eye with the camera(d)Simple and compound microscope (e) Telescope (f)Simple periscope (g)filmprojector

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9. Sound Waves: (a) Sources of sound (b)Transformation of sound (c)Noise and music(d)Pitch, loudness andquality(e)Forced vibration (i)Resonance (ii)Harmonics and overtones (f)Speed of sound in (i)Solid (ii)Liquid (iii)Air (g)Velocityof sound; its measurement (h)Stationary waves.

10. Application of sound waves:(a)Wind instruments:(i)Clarinet (ii)Flute (iii)Saxophone (iv)Trumpet(b)Stringed instruments:(i)Guitar (ii)Sonometer (iii)Piano (c)Percussioninstruments (i)Drum(ii)Bell(iii)The talking drum (d)Echoes and their applications(e)Hearing Aids. Doppler Effect.

11. Revision

12. Exams

WEEK 1: DATE:…………….

SUBJECT: PHYSICS

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CLASS: SS 2:

TOPIC: REVISION &PRODUCTION AND PROPAGATION OF WAVES

CONTENTS

a. Revision

b. Production of mechanical waves

c. Graphical representation of wave

d. Terms as applied to waves

e. Relationship between f, T and Ξ»

f. Simple solved problems on f, T and Ξ»

Sub topic 1:Production of mechanical waves

A wave is a disturbance which travels through a medium and transfers energy from one

point to another without causing any permanent displacement of the medium itself. If you

drop a stone into water in a basin or swimming pool, ripples or waves will be seen spreading

outward from the source of the disturbance. As the waves generated spread out, they transfer

energy from one point to the other without the water moving in the direction of the ripples.

See diagrams below.

Waves can also be produced when one ties one end of a rope to a wall, hold the other end and

make it to move up and down rapidly. Alternatively, get a long string and place both ends to

Stone ripples

Water source of disturbance

Dir

ecti

on

of

pro

pag

atio

n

Dir

ecti

on

of

pro

pag

atio

n

Waves propagated along water

rope

Hand move rope up and

down to generate the

wave form

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two fixed points as shown below. Pluck the string i.e pull it either vertically downward or

upward and release it. A wave will be generated.

Class activity

1. Educator should use ripple tank to produce plane and circular waves or a large bowl

containing water could be used as alternative

2. Educator should guide the students as they produce mechanical waves using a rope or a

suitable string.

Subtopic 2: Terms used in Describing Waves

A wave can be represented as shown in the diagram below.

Terms as applied to wave motion

Production of mechanical waves

Y

P Ξ» Q

a

O x

Ξ»

General representation of a wave

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a. Crest: This is a region of maximum upward displacement of the particles of the

medium.

b. Trough: This is a region of maximum downward displacement of the particles of the

medium

c. Phase: The particles of a wave are said to be in phase when they are at the same

vertical distance from their mean position and are moving in the same direction.

d. Amplitude (a): It is the maximum displacement of the particles as measured from the

mean position.

e. Period (T): This is the time taken by a particle to complete one circle or oscillation. Its

unit is seconds. It can also be defined as the time taken for the wave to cover one

wavelength. i.e from point P to Q or from Point O to R in the diagram above.

π‘π‘’π‘Ÿπ‘–π‘œπ‘‘ 𝑇 =π‘‘π‘–π‘šπ‘’

(π‘›π‘’π‘šπ‘π‘’π‘Ÿ π‘œπ‘“ π‘œπ‘ π‘π‘–π‘™π‘™π‘Žπ‘‘π‘–π‘œπ‘›)

𝑇 =𝑑

𝑛

f. Frequency ( f ): This is defined as the number of circles the wave makes in one

second. It is measured in Hertz (Hz)

𝑓 =𝑛

𝑑

C r c r r c r c r c

(b) Propagated sound wave in air

B A

From a to B is a cycle. The time for

the wave to move from A to B is

called PERIOD

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g. Wavelength (Ξ» ): This is the distance between two successive crests or troughs in phase.

It can also be defined as the distance covered by the wave after completing a circle. It is

measured in metres. In the diagram, the wavelength Ξ» is the distance (P Q) or (O R).

h. Wave velocity (v): This is the distance (π‘₯) the wave travels with time (t). its unit is m/s.

𝑣 =π‘‘π‘–π‘ π‘‘π‘Žπ‘›π‘π‘’

π‘‘π‘–π‘šπ‘’

During one cycle, the distance travelled = wavelength

Time to complete one cycle = period.

Therefore;

𝑣 =π‘€π‘Žπ‘£π‘’π‘™π‘’π‘›π‘”π‘‘β„Ž

π‘π‘’π‘Ÿπ‘–π‘œπ‘‘

𝑣 =πœ†

𝑇

Since frequency is inverse of period f = 1/T

𝑣 = πœ†π‘“

Example 1

A wave travels a distance of 100m in 5 seconds. The distance between successive crests of the

wave is 25cm. calculate the frequency of the wave.

Solution:

Distance = 100m, time = 5 seconds Ξ» = 25cm = (25/100) = 0.25m

Velocity = distance / time

= 100 / 5 = 20m/s

V = f Ξ»

F = v / Ξ»

f = 20 / 0.25 = 80Hz

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Example 2

A radio station broadcasts at a frequency of 200 kHz. If the speed of the wave is 3.0 x 108 m/s,

calculate the period and the wavelength of the wave.

Solution

Frequency, f = 200kHz = 200000Hz, velocity, v = 3.0 x 108 m/s

Period, T = 1/f = 1/ 200000 = 5 x 10 – 6 seconds

V = f Ξ»

Wavelength, Ξ» = v/f

= 3 x 108/ 2 x 105 = 1.5 x 103m

Example 3

A vibrating source which has a frequency of 500Hz produces a sound whose velocity in air is

330m/s. determine the distance which the sound travels when the source completes 100

vibrations.

Solution

𝒇 =𝒏

𝒕

πŸ“πŸŽπŸŽ =𝟏𝟎𝟎

𝒕

𝒕 = 𝟎. 𝟐 𝒔𝒆𝒄

π’•π’‰π’Šπ’” π’Šπ’” 𝒕𝒉𝒆 π’•π’Šπ’Žπ’† 𝒇𝒐𝒓 𝒕𝒉𝒆 π’˜π’‚π’—π’† 𝒕𝒐 π’„π’π’Žπ’‘π’π’†π’•π’† 𝟏𝟎𝟎 π’„π’šπ’„π’π’†

𝒗 =𝒅

𝒕

πŸ‘πŸ‘πŸŽ =𝒅

𝟎. 𝟐

𝒅 = πŸ”πŸ”. 𝟎 π’Ž

Alternative solution,

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Frequency f = 500Hz or 500 circles per second.

If the source makes 500 circles in a second, then it will take the source (100/500) seconds to

make 100 circles = 0.2s

Speed (v) = distance (s) / time (t)

Therefore s = v t = 330 x 0.2 = 66m

Evaluation

1. Define wave and represent its motion by a diagram

2. Calculate the frequency of a wave if its period is 0.25s

3. Five circles are formed in 2s, what is the period of the wave?

Weekend assignment

1. Reading assignment: Read on transverse and longitudinal

2. What is wave motion?

Objectives

1. Which of the following

statements about wave is/are correct?

i. A wavefront is a line which contains

all particles whose vibrations are in

phase.

ii. The direction of propagation of a

wave is the line drawn parallel to

the wavefront.

iii. A wavefront is a circle which is

common to all particles that are to

be in the same state

of disturbance.

(A) I only (B) ii only (C) I, ii and iii

(D) I and ii only (E) ii and iii only.

2. A stone is dropped into the middle

of a pool of water. Which of the

following statements is/are correct?

i. Spherical waves are set up in the

water.

ii. The water moves outwards to the

sides of the pool.

iii. Energy is transmitted outwards

from the center of disturbance.

(A) I only (B) ii only (C) iii only

(D) I and iii only (E) ii and iii only.

3. The S.I units of frequency, period

and amplitude of a wave are

respectively

(A) hertz, second and centimeter.

(B) second, meter and hertz

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(C) meter, hertz and second

(D) hertz, second and meter

4. The period of a wave is 0.02second.

Calculate its wavelength if its speed

is 330m/s.

(A) 6.6m (B) 5.0m (C) 4.0m

(D) 3.3m (E) 2.0m

. 5. The distance between two points in

phase on a progressive wave is 5cm.

If the speed of the wave is 0.020m/s.

Calculate its period.

(A) 4.00s (B) 2.50s

(C) 0.25s (D) 0.04s

6. A periodic pulse travels a distance

of 20.0m in 1.00s. If the frequency

is 2.0 x 103Hz, calculate the

wavelength.

(A) 1.0 x 10-3m (B) 1.0 x 10-2m

(C) 2.0 x 10-2m (D) 1.0 x 102Hz

WEEK 2: DATE:…………….

SUBJECT: PHYSICS

CLASS: SS 2

TOPIC: WAVES ( CONT’D)

CONTENTS

1. Types of waves

2. Wave equation ( y = Asin(Ο‰t – k𝒙)

Sub topic 1: Types of waves

Waves can be classified under Transverse waves and Longitudinalwaves. If the direction of

propagation of the particles of the wave is perpendicular to the direction of vibration of the

medium, the wave is transverse. Examples of transverse waves are, water waves and waves

produced by plucking a string. If we consider material medium, waves can be classified under

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mechanical waves and electromagnetic waves. Mechanical waves require a material medium

for propagation e.g water waves and waves in a string while electromagnetic waves do not

require material medium for propagation. Examples of these waves are; radio waves, light

waves, x-rays e.t.c.

(a) Original undisturbed position of air

Direction of travel of wave

Direction of vibration of medium

(b) longitudinal wave

Direction of vibration of the particles

Direction of travel of wave

(a) Transverse wave

C r c r r c r c r c

(b) Propagated sound wave in air

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If the direction of travel of the wave is the same as the direction of vibration of the medium,

the wave is longitudinal. Sound waves are example of longitudinal waves. In longitudinal waves,

the vibrating particles behave like a spiral spring that has a series of compressed regions and

spaced out regions travelling along it. Series of compressed regions are called compression (c)

while series of spaced out regions are called rarefaction (r). See diagram (b) below.

Sub topic 3: Equation of a travelling wave

The equation of a travelling wave can be written mathematically as

y = 𝑠𝑖𝑛 πœƒ or 𝑦 = π‘π‘œπ‘  πœƒ

Angular velocity πœ” =πœƒ

𝑑 radians per seconds. πœƒ = πœ”π‘‘

y = 𝑠𝑖𝑛 πœ”π‘‘ or 𝑦 = π‘π‘œπ‘  πœ”π‘‘

Generally, A travelling wave with amplitude β€˜A’ and constant angular velocity πœ” can be written

𝑦 = 𝐴𝑠𝑖𝑛( πœ”π‘‘ Β± Ø)………………………………………..eqn 1

Ø is a constant for a wave that did not start from the origin

Ø is constant angular distance called phase constant which is related to linear distance x by

Ø =2πœ‹π‘₯

Ξ» ------------------------------------------------------eqn 2

2πœ‹

Ξ» = k. which we call wave number. Substituting eqn 2 into eqn 1, we have

𝑦 = 𝐴𝑠𝑖𝑛(πœ”π‘‘ Β±2πœ‹π‘₯

Ξ») = 𝐴𝑠𝑖𝑛(πœ”π‘‘ Β± π‘˜π‘₯)-------------------------eqn 3

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If we substitute πœ” =2πœ‹

𝑇 and π‘˜ =

2πœ‹

Ξ» into eqn 3, it becomes

𝑦 = 𝐴𝑠𝑖𝑛 (2πœ‹π‘‘

TΒ±

2πœ‹π‘₯

Ξ»)

Or 𝑦 = 𝐴𝑠𝑖𝑛2πœ‹ (𝑑

TΒ±

π‘₯

Ξ»)---------------------------------------------eqn 4

Or 𝑦 = 𝐴 sin2πœ‹

Ξ»(

Ξ»t

TΒ± π‘₯)----------------------------------------------eqn 5

Recall that v = f Ξ»

Ξ» = vt, therefore eqn 5 becomes

𝑦 = 𝐴 sin2πœ‹

Ξ»(𝑣𝑑 Β± π‘₯)--------------------------------------------------eqn 6

+ π‘“π‘œπ‘Ÿ π‘€β„Žπ‘’π‘› π‘‘β„Žπ‘’ π‘€π‘Žπ‘£π‘’ 𝑖𝑠 π‘π‘Ÿπ‘œπ‘π‘Žπ‘”π‘Žπ‘‘π‘–ng in the negative x-direction

βˆ’ π‘“π‘œπ‘Ÿ π‘€β„Žπ‘’π‘› π‘‘β„Žπ‘’ π‘€π‘Žπ‘£π‘’ 𝑖𝑠 π‘π‘Ÿπ‘œπ‘π‘Žπ‘”π‘Žπ‘‘π‘–π‘›π‘” 𝑖𝑛 π‘‘β„Žπ‘’ positive x- direction

Solved problems

Example 4

A travelling wave is given by the equation y = 0.03 Sin ( 2.2 π‘₯ βˆ’ 3.5t ) where y and π‘₯ are in

metres and t is in seconds. Find the amplitude, the wavelength, the frequency, the period and

the speed of the wave.

Solution

To solve this problem, we compare the equation with eqn 3

𝑦 = 𝐴𝑠𝑖𝑛(πœ”π‘‘ Β± π‘˜π‘₯) (eqn 3)

y = 0.03 Sin ( 2.2 π‘₯ βˆ’ 3.5t )

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Thus, amplitude A = 0.03m, angular frequencyπœ” = 3.5 rad – s k = 2.2 m – 1

Ξ» =2Ο€

k= 2 Γ—

3.142

2.2= 2.86m

Period T = 2Ο€

πœ”= 2 x

3.142

3.5= 1.80s

The speed of the wave is given by

v = fΞ» =Ξ»

T=

2.86

1.80=1.59m – s

Example 5

The wavelength of a travelling wave is 5m at a frequency of 12 Hz.

i. What is the wave velocity?

ii. If there is a crest at π‘₯ = 3m at time t, find three other positions of the crest at that

instant

iii. What time later will there be another crest at π‘₯ = 3m ?

iv. If the amplitude of the wave is 1.5m, write the equation of the wave.

Solution

i. v = fΞ» = 12 x 5 = 60 m/s

ii. the crests are at one wavelength apart, so there are crests at π‘₯ = 3m, π‘₯ = (3 + 5)m, π‘₯ =

( 3 + 5 + 5)m and π‘₯ = ( 3 + 5 + 5 + 5)m. i.e π‘₯ = 3m, 13m and 18m

iii. A crest will arrive again at π‘₯ = 3m after one period T = 1

𝑓=

1

12= 0.083𝑠

iv. The wave equation can be written as 𝑦 = 𝐴 sin2πœ‹

Ξ»(𝑣𝑑 βˆ’ π‘₯)

A = 1.5m, v = 60m/s, Ξ» = 5.0m

Hence, 𝑦 = 1.5 sin2πœ‹

5(60𝑑 βˆ’ π‘₯) or 𝑦 = 1.5 sin 2πœ‹ (12𝑑 βˆ’

π‘₯

5).

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Weekend assignment

1. Differentiate between transverse and longitudinal waves with examples

2. Mention 5 terms associated with waves and explain them

3. The equation of a wave is given as 𝑦 = 0.5sin (3πœ‹π‘₯ + 50πœ‹π‘‘). Where x and y are in

metres and t is in seconds. Find (a) The amplitude (b) the wave number k and (c) the

wavelength of the wave.

4. A wave covers 30cm in 5s, if the distance between a crest and its neighbouring

trough is 1.5cm, (a) What is the wavelength? (b) How many circles can be formed in

15s?

5. The equation, y = Asin2πœ‹/πœ†(vt –x) represents a wave train in which y is the vertical

displacement of a particle at distance X from the origin in the medium through which

the wave is travelling. Explain, with the aid of a diagram, what A and Ξ» represent.

6. The equation y = asin(wt-kx) represents a plane wave travelling in a medium along

the

x-direction, y being the displacement at the point x at time t.

i. Given that x is in meters and t is in seconds, state the units of k and w.

ii. What physical quantity does w/k represent? Justify your answer.

iii. State whether the wave is travelling in the positive or negative x-direction.

7. The equation, y = 5sin(3x – 4t), where y is in millimeters, x is in meters and t in

seconds

represents a wave motion. Determine the i. frequency ii. Period iii. Speed of the

wave.

Objectives

1. Which of the following is not a

property of longitudinal waves?

(A) Compression (B) Reflection

(C) Refraction (D) polarization

(E) Diffraction.

3. When the direction of vibration of

the particles of a medium is

perpendicular to the direction of

travel of a wave, the wave

transmitted is known as

(A) sound wave (B) transverse

wave

(C) longitudinal wave

(D) stationary wave

(E) mechanical wave.

4. Which of the following are

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longitudinal waves?

i. Ripples on the surface of water

ii. waves produced by a tuning fork

vibrating in air.

iii. light waves.

iv. waves produced by flute.

(A) I and ii only (B) I and iii only

(C) ii and iii only (D) ii and iv only

(E) iii and iv only.

8. Which of the following are

transverse wave?

i. Ripples on water

ii. sound waves in air.

iii. light waves from the sun.

(A) ii only (B) I and ii only

(C) ii and iii only

(D) I and iii only

(E) I, ii and iii

9. Which of the following wave

characteristics can be used to

distinguish a transverse wave from a

longitudinal wave?

(A) Reflection (B) Refraction

(C) Diffraction (D) Polarization

(E) interference.

10. Which of the following is not a

mechanical wave?

(A) wave propagated in stretched

string.

(B) Waves in closed pipes

(C) Radio waves

(D) Water waves

(E) sound waves.

11. Which of the following statements

about a progressive mechanical wave

is correct?

(A) it can be plane polarized.

(B) its energy is localized at specific

points of its profile.

(C) it does not require material

medium for its propagation.

(D) its frequency remains constant

as it travels between different

media.

12. .

13. In a wave, the maximum

displacement of particles from their

equilibrium positions is called

(A) frequency (B) Amplitude

(C) Period (D) wavelength

(E) Wave velocity.

14. The amplitude of a wave is the

(A) distance travelled by the wave in

a complete cycle of its motion.

(B) maximum displacement of the

wave particle from the

equilibrium position.

(C) separation of two adjacent

particles vibrating in phase.

(D) distance between two

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successive troughs of the wave.

16. The diagram below represents part

of a wave motion in air, If the wave

travels with a speed of 300m/s,

calculate the frequency of the wave.

y (cm)

0 x(cm)

3m

17. which of the following staments is

not true of the diagram shown

below

s A B

0

C D

(A) The two points A and B are in

phase.

(B) Distance AB is half the

wavelength of the wave.

(C) Ac and BD are the amplitudes

of the wave.

(D) The two points A and B

represents the wave crests.

(E) The wave has four crests.

18. The diagram below shows a

waveform in which energy is

transferred from A to B in a time of

2.5 x 10-3s. calculate the frequency

of the wave.

A B

(A) 2.0 x 103Hz (B) 1.0 x 103Hz

(C) 4.0 x 10-2Hz (D) 1.0 x 10-3Hz

(E) 5.0 x 10-4Hz

19. Dcm

5

0 0.05 0.10 0.15 0.20 0.25 t/s

5

The diagram above represents the

displacement D versus time t, graph

of a progressive wave. Deduce the

frequency of the wave?

(A) 20Hz (B) 225.0Hz

(C) 270.0Hz (D) 750.0Hz

20. Sixty complete waves pass a

particular point in 4s. If the distance

between three successive troughs of

the waves is 15m, calculate the

speed of the waves?

(A) 300m/s (B) 225.0m/s

(C) 112.5m/s (D) 75.0m/s

(E) 16.0m/s

23. The distance between two points P

and Q along a wave is 0.05m. If the

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wave length of the wave is 0.10m,

determine the angle between P and

Q in radians.

(𝐴) 0.1 πœ‹ (B) πœ‹

(𝐢) 2 πœ‹(𝐷) 10 πœ‹

24. A progressive wave has a

wavelength of 50cm. Calculate the

phase difference between two

points at a distance of 20cm apart.

(𝐴) 10/3 πœ‹ (B) 5/2πœ‹

(𝐢) 4/5πœ‹(𝐷) 2/3 πœ‹

(𝐷) πœ‹/3

2526. The change of the direction of a

wavefront because of a change in

the velocity of the wave in another

medium is called

(A) refraction (B) reflection

(C) diffraction (D) interference

27. In which of the following is a

stationary wave produced?

i. A vibrating tuning fork held near

the end of a resonate tube closed

at the end.

ii. A string tightly stretched between

two points and plucked at its

middle.

iii. The prongs of a tuning fork

vibrating in air

(A) I only (B) ii only

(C) I and ii only

28. Two identical waves travelling in

the same direction are

superimposed,

what should be the phase difference

between the waves for maximum

destructive interference to occur?

(A) 200 (B) 450 (C) 1800

(D) 2250 (E) 2700

29. Water waves are generated by

dropping stones at regular intervals

at a point in a pool of water. The

first crest reaches another point, 8m

away in 4s. If the distance between

two successive crests is 0.5m, the

frequency of the wave is

(A) 2Hz (B) 4Hz (C) 8Hz

(D) 16Hz

30. In the wave equation

y = Eosin(200t- πœ‹x), Eo represents

the

(A) amplitude (B) frequency

(C) period (D) wavelenght

WEEK 3

DATE:…………….

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SUBJECT: PHYSICS

CLASS: SS 2

TOPIC: PROPERTIES OF WAVES

CONTENTS

1. Reflection and refractionof waves

2. . Interference, diffraction and polarization of waves

3. Progressive and stationary waves

Subtopic 1: Reflection and Refraction of waves

Reflection occurs in waves when they encounter an obstacle and are made to propagate in the

opposite direction as shown in the diagram below

Reflection also occurs in sound and light waves. Sound heard after reflection of sound waves is

called an echo.

Refraction of waves

Refraction occurs when the wave is made to travel through two media of different densities.

Refraction is the change in the speed and direction of the waves as they cross the boundary

between two media of different densities. The incident angle ( i ) is the angle the direction of

the incident wave front makes with the normal ( N ) at the boundary surface. The angle of

refraction (r) is the angle the direction of the refracted ray makes with the normal ( N) to the

plane boundary.

Incident wave

Plane reflector

Normal to the reflector

Reflected wave

Reflection by a plane surface

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The refractive index 1n2 of medium 1 with respect to medium 2 is given as

1n2 = Speed of wave in medium 1

Speed of wave in medium 2

If the waves pass from deep water to shallow water, the refractive index is given as

1n2 = Speed in deep water

Speed in shallow water

The refractive index 1n2 is also given as

1n2=𝑠𝑖𝑛 𝑖

𝑠𝑖𝑛 π‘Ÿ

Evaluation

1. Define reflectionand refraction of waves

2. With the aid of a labeled diagram, explain what you understand by (a) normal (b)

angle of incidence (c) angle of refraction when light travels from air to glass

Subtopic 2. Interference, diffraction and polarization of waves

Interference of waves: Interference is a phenomenon whereby two or more waves of the

same frequency, amplitude and wavelength traveling in the same direction are superimposed

or overlap. We have two types of interference namely, constructive and destructive

interference. For constructive interference, the two waves are superimposed in the same

phase. i.e crests on crests or troughs on troughs. This will lead to increased or maximum

Direction of incident wave front

Angle of incidence ( I )

N

Boundary interface

Angle of refraction ( r )

Refracted wave front

Refraction of waves at plane boundary

Medium 1

Medium 2

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disturbance. The lines joining the points where there is constructive interference are called

antinodal lines. While the lines joining the points where the waves are out of phase i.e where

the crests of one wave overlap with the troughs of another wave are called nodal lines. Here

the resultant disturbance is zero. Here the waves appear stationary. See diagrams below.

Nodal line (destructive interference) Antinodal line (constructive interference

Interference of circular waves

Diffraction of waves

Diffraction is the bending or spreading of waves around corners when the traveling waves

encounter obstacles with a hole (aperture). The bending of the waves depend on the size of the

aperture. If the width of the aperture is smaller than the wavelength, the waves will bend and

spread out more as shown in the diagram below.

Evaluation

1. Define the following terms: (i) Diffraction (ii) interference of waves

Diffraction

Incident wave

Diffraction of waves

S1 Wave sources

From dippers

S2

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2. Explain the effect of the width of an obstacle on diffraction of waves

3. Explain what you understand by destructive and constructive interference as applied to

wave motion.

Polarization of waves

Polarization is a phenomenon that differentiates transverse waves from longitudinal waves.

Polarization takes place in transverse waves only. A wave is said to be plane polarized if it is

constraint to vibrate in one plane. Polarization occurs with light waves and other

electromagnetic waves such radio waves, x-rays, infra-red radiation, e.t.c.

Polarized light can be produced using a polarizer such as Tourmaline crystal, Quartz or Polaroid.

A polarizer will only allow light vibrations of only one direction to pass through it. Any other

vibrations will be absorbed. See diagram below. Since the plane of polarization is vertical, only

vibrations in the vertical directions will pass through the polarizer.

Another means of polarizing light waves is by reflection. If light is incident at angle of 570 on

the polished surface of a glass plate, the light will be reflected in one plane. This is plane

polarization of light. This angle is called the Brewster angle.

Practical application of Polaroid

Polaroid are used in sun glasses to control or reduce the intensity of incident light and to

eliminate reflected light. Polaroid can also be used to eliminate light glare from window panes,

Unpolarized light

plane Polarized light polarized light

vibrations in all directions

Polarization of waves

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glass doors, polished table top, also how chemical substance polarize light has also been used in

salt analysis e.t.c.

Progressive and stationary waves

A progressive wave is a wave that travels and continues to spread out from the source of

disturbance. A standing or stationary wave is a wave that is produced when two waves of the

same frequency and amplitude superimposed or overlap. The superposition of two waves of

the same frequency and amplitude that are exactly out of phase leads to the formation of a

region of zero resultant disturbance as shown in the diagrams below.

Superposition of two waves of the same frequency and wave length traveling in the same

direction and in phase

A

Wave 1

B

Wave 2

C

Wave 1 & 2

D

Resultant wave

E F G H

Wave 1 wave 2 wave 1 & 2 resultant wave

Superposition of two waves of the same frequency and wavelength traveling in the same direction

which are exactly out of phase

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Stationary wave

Stationary waves are obtained as a result of the combination or superposition of an incident

wave and its reflected wave which is of the same frequency and wavelength and are exactly out

of phase. Thus, the crest of the incident wave coincides with the trough of the reflected wave

and vice-versa. See diagram below. N are called nodes of the stationary wave. The

displacement at this point is always zero. Points β€˜AN’ are the antinodes. These are points of

maximum displacement. We therefore define node as a point on a stationary wave where there

is no movement of the medium. Antinode is a point on the stationary wave where there is

maximum displacement of the medium. The nodes and antinodes are Ξ»

2 apart

Evaluation

1. How are stationary waves obtained?

2. With the aid of a diagram, explain node and antinode as applied to stationary waves

Weekend assignment

1. Reading assignment: Read on sources of light, transmission of light and image formation

by curved mirrors

Incident wave reflected wave

Source of wave obstacle

Ξ»

4

N N N

Ξ»

2

3Ξ»

4

Ξ»

Stationary wave

AN AN AN AN

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2. Distinguish between progressive and stationary waves. What is the distance between

two nodes and between a node and an antinode in terms of the wavelength of the

wave?

3. What is plane polarized wave? How can plane polarized light be produced and

detected?

WEEK 4:

DATE:…………….

SUBJECT: PHYSICS

CLASS: SS11

TOPIC: LIGHT WAVES

CONTENTS

1. Sources of light

2. Transmission of light

3. Reflection of light

4. Formation of images by plane and curved mirrors

Sub topic 1: Sources of light

Light has a number of sources. Some are man-made while others are natural. Examples of man

made sources of light include: light from candles and light from electric bulbs. Natural sources of

light are; the sun, stars, glow-worms, e.t.c. these sources of light can be grouped into luminous

and non luminous sources. Luminous bodies or objects generate and emit light by themselves.

E.g stars, sun electric lamps e.t.c. Non luminous objects or bodies depend on man-made or

natural sources. E.g the moon.

Sub topic 2: Transmission of light

Light is an example of electromagnetic waves because it does not require a material medium for

propagation. Some materials allow light to pass through them easily while others do not.

Materials that allow light to pass through them so that objects can be seen are called transparent

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materials. E.g glass and water. Non transparent bodies that allows small amount of light to pass

through them such that objects are not seen clearly are called translucent materials or bodies.

Examples of such bodies are, frosted glass or tinted glass. Those that will not allow light to pass

through them at all are called opaque bodies. Example is wood.

Rays and beams of light

The direction or path along which light energy travels is called a ray of light. A collection of

light rays is called a beam.

Ray of lightBeam of light

We have three types of beam of light namely, parallel beam of light, convergent beam of light

and divergent beam of light. For parallel beam of light, the rays are parallel to one another. E.g

beam from search light. If the rays converge or meet at a point, the beam is called convergent

beam. In divergent beam, the rays spread out or appear to have originated from a source say p.

E.g rays from torch light. See diagrams below.

p

Parallel beam of light convergent beam of light Divergent

beam of light

Note that light rays travel in a straight line. This is what is called rectilinear propagation of light.

Your teacher will demonstrate this with you using a ray box.

Rectilinear propagation of light.

This means that light travels in a straight line. i.e light ray propagation along a straight line.

Evidence in support of rectilinear propagation of light.

1. Formation of shadow: when light rays from a source fall on a opaque object, the outline

of the shadow of object is formed as shown below

Point light

source

screen

shadow

Opaque

object

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For point light source, the shadow formed has a uniform intensity. For a broad light source, the

shadow has two distinct region: umbra and preumbra.

2. Formation of eclipse: eclipse is formed when the sun, the moon and the earth are

collinear such that the shadow of the moon/earth is cast on the earth/moon. There are

two types of eclipse:

I. Solar eclipse: this occur when the sun, the moon and the earth are on a straight

line such that the moon is between the sun and the earth and the shadow of the

moon is cast on the earth.

The sun act like a broad light source. Part of the earth corresponding to b will

experience total darkness. Parts of the earth corresponding to c and a will experience

partial darkness. It occurs during the day

Broad light

source

screen

shadow

Opaque

object umbra

preumbra

a

b

c

Sun earth

moon

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If the distance between the moon and the earth is so great such that the light ray from

the sun grazing the moon intersect before reaching the earth., the eclipse form as a

pattern of a ring of light. This eclipse is called is called Annular Eclipse.

( ring of light will occur around the region a.)

ii. lunar eclipse (eclipse of the earth): This is when the sun the moon and the earth are

collinear such that the earth is between the sun and the moon and the shadow of the

earth is cast on the moon. it occurs during the night.

3. Pin hole camera: this device is a rectangular pin with a pin on one of its faces and a film/

screen on the face opposite to the pin hole. Light rays from an object will through the

pinhole and form the image of the object on the screen. The image formed has the

following property:

(a) Image is real

(b) Image is inverted

(c) Image is diminished if the distance of the object from the pinhole is greater than the

length of the camera. Otherwise, the image will be magnified.

(d) Magnification m of the image formed is given as:

π‘š =β„Žπ‘–

β„Ž0

π‘š =𝑣

𝑒

β„Žπ‘–

β„Ž0=

𝑣

𝑒

Where;

hi - is the height (or size) of image.

h0 - is the height (or size) of the object

v - image distance (or distance between the pinhole and the screen)

u – object distance.

Earth a

sun

Moon

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(e) The smaller the size of the pinhole, the sharper the image. Ifthe size of the pinhole is too

big, the image will be blur.

(f) To increase the magnification of the image of a pinhole camera, move the object close to

the pnhole.

Examples:

1. The length of a pin-hole camera is 12cm. it is used to photograph an object 60cm

away from the hole, and 80cm high. Calculate the height of the image and

magnification produced.

Solution

β„Žπ‘–

β„Ž0=

𝑣

𝑒

Height of object h0 = 80 cm

Object distance u = 60 cm

Image distance v = 12 cm

Height of image hi = ?

β„Žπ‘–

80=

12

60

β„Žπ‘– =80 Γ— 12

60

β„Žπ‘– = 16 π‘π‘š

Example 2.

An object of height 40cm is placed 0.80m in front of a pin-hole camera of length 16cm.

what is the magnification and height of the image produced?

Solution

screen

pinhole

Object h0

hi image

v

u

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β„Žπ‘–

β„Ž0=

𝑣

𝑒

Height of object h0 = 40 cm

Object distance u = 0.8 m = 80 cm

Image distance v = 16 cm

Height of image hi = ?

Magnification m = ?

β„Žπ‘–

40=

16

80

β„Žπ‘– =40 Γ— 16

80

β„Žπ‘– = 8 π‘π‘š

Evaluation

1. The distance between the pinhole and the screen of a pinhole camera is 12.5 cm and the

plate is 20 cm long. T what minimum distance from the pinhole must a 1.8 m tall man

stand if a full-length photo is required?

2. A body of height 6 cm and it is placed 40 cm in front of pinhole camera 16 cm in length.

What is the height of the image?

Sub topic 3: Reflection of light

As earlier discussed, light waves undergo reflection. The nature of the reflection depends on

the type of surface the light is incident on. Thus, we have two types of reflections namely,

regular reflection and diffused reflection. If the reflections are such that the rays are parallel to

one another and are in one direction, we have regular reflection. This happens when light is

incident on a polished or smooth surface. If on the other hand, the rays of light are incident on

a rough surface, the rays will be reflected in different directions. This type of reflection is called

diffused reflection. These are shown in the diagrams below.

Laws of reflection of light

There are two laws of reflection. These are

rough surface

Smooth surface

Regular reflectionDiffused reflection

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1. The incident ray, the reflected ray and the normal at the point of incidence all lie in the

same plane

2. The angle of incidence (i) is equal to the angle of reflection (r)

Educator should carry out a simple experiment to investigate these laws of reflection.

Sub topic 4: Formation of images by plane mirrors and curved mirrors

1. Image formed by a Plane mirror. The way a plane mirror forms an image of an object

placed in front of it is illustrated in the diagram below.

The incident rays OA and OB from the tip O, of the object strike the mirror at point A and B and

are reflected as AC and AD respectively. When the points AC and BD are extended backwards,

they will intersect at point I. That is why an observer at point E sees the upright image of the

Image ( I ) N Object ( O )

Mirror

A

B

C

D

E

Formation of image by a plane mirror

Incident ray Reflected ray

normal

i r

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object as if it were located at I behind the mirror. The ray ON normal or perpendicular to the

mirror is reflected back along ON. On produced meets the other two rays at I such that ON = NI.

This image formed is a virtual image because the rays do not intersect to form the image. Thus

there exist two types of images. Virtual image and real image. A virtual image is the one that is

formed by the apparent intersection of light rays while a real image is the one that is formed by

the actual intersection of light rays. One major difference between a virtual and a real image is

that real image can be caught on a screen while virtual image cannot be caught on a screen.

Class activity

Educator should teach the students how to locate the image of a pin placed in front of a plane

mirror.

Characteristics of images formed by a plane mirror

1. The image is virtual

2. It is far behind the mirror as the object is in front of it

3. It is virtual

4. It is the same size as the object

5. It is upright and laterally inverted

Images formed by inclined mirrors

When an object is placed in front of two mirrors that are inclined to each other, a number of

images can be viewed by an observer. The number of images (n) is given by the equation

𝑛 =360

πœƒβˆ’ 1

where πœƒ is the angle of inclination of the two mirrors. For example if πœƒ = 600, then number of

images (n) =360

πœƒβˆ’ 1 =

360

60βˆ’ 1 = 6 βˆ’ 1 = 5

Class activity

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Place a pin in front of two mirrors inclined at an angle of 450. View and record down the images

formed. Repeat the experiment for two other angles ( 600, 900). Test your result using the

formula method. What do you notice?

Evaluation

1. Mention 4 sources of light you know

2. What do you understand by rectilinear propagation of light?

3. Differentiate between virtual and real image

4. Give 4 characteristics of images formed by a plane mirror

Applications/uses of plane mirror

1. Periscope.

The simple periscope is a practical application of reflection of light by plane mirrors. It

consists of two mirrors which are placed parallel to each other, one at the top and the

other beneath and inclined at an angle of 45o to each other as shown in the diagram below.

Simple periscope

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Parallel rays from an object β€˜O’ strike mirror β€˜A’ at an angle of 45o and are reflected

perpendicularly through an angle of 45o (law of reflection) to mirror B. As the rays strike

mirror β€˜B’, they again get reflected through the same angle of 45o. Thus, an observer at point β€˜E’

can see the object β€˜O’ clearly. The simple periscope is used in warfare especially in sea or water.

It is also used for looking over barriers. The periscope produces multiple images. This is a

disadvantage. Modern periscope uses a triangular glass prism with refractive angle 900 instead

of plane mirrors.

2. Kaleidoscope: This is a toy in which multiple images are formed by two plane mirrors inclined at

angle 600. The mirrors are fixed between at one end of a tube and colour paper are placed

there. The image of the paper viewed through the other end of the tube are seen symmetrically

in a circle. By shaking the tube, different pattern can be seen each time.

3. Sextant: optical instrument used for the measurement of angular distance between any

two objects. The operation of the sextant depends upon superimposition of the images of

the two objects whose distance is being measured. This is achieved by means of an

optical system consisting of a telescope and two mirrors, one fixed and one movable.

4. It is used in supermarkets to display multiple images of items.

5. it used for dressing mirrors.

Reflection of light by curved or spherical mirrors

Apart from plane mirrors, curved or spherical mirrors also reflect light rays. There are two types

of spherical mirrors. They are convex mirror and concave mirror. If the reflecting surface is

curved inside, the mirror is concave mirror or converging mirror. If the reflecting surface is

curved outward, it is called convex or diverging mirror. Ask your teacher to show you these

spherical mirrors.

Terms as applied to spherical mirrors

The Polep of the mirror is the centre of the reflecting surface of the curved mirror.

The Aperture is the width AB of the mirror. The centre of curvature C is the centre of the

sphere of which the mirror is a part

Silvered surface reflecting surface

Reflecting surface silvered surface

Concave mirror Convex mirror

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The Radius of Curvaturer is the radius of the sphere of which the mirror forms a part. It is the

distance CP

The Principal Axis is the line PC from the pole to the to the centre of curvature

The Principal FocusF of a concave mirror is that point on the Principal Axis where rays parallel

and close to the principal axis converges to after reflection

The Principal FocusF of a convex mirror is that point on the Principal Axis where rays parallel

and close to the Principal Axis appear to diverge from after reflection.

The Focal Lengthf is the distance PF between the principal axis and the Principal Focus.

The Focal Lengthf is half of the Radius of Curvaturer

𝒇 =𝒓

𝟐

Reflecting surface

Reflecting surface

Parallel incident rays C F P

Reflected converging rays

Reflection of light rays by a concave mirror

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Formation of images by curve mirrors.

The nature and position of the image formed by a concave mirror is dependent upon the place

the object is placed in front of the mirror. We note these facts when drawing ray diagrams.

1. A ray parallel to the principal axis passes through the principal focus after reflection

2. A ray through the centre of curvature is reflected back along the same path

3. A ray passing through the principal focus is reflected parallel to the principal axis

The point of intersection of any two of these rays is enough to determine the position of the

image. Let us consider some cases.

Object placed beyond C

(a) Object placed beyond C

A Mirror

O C F P

B

I

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(b) Object placed at C

A Mirror

O C F P

B

The image is real, inverted, same size as the object and formed at C

I

(c) Object placed between C and F

Mirror

C O F P

B

The image is real, inverted, enlarged and formed beyond C

I

A

(d) Object placed at F

A Mirror

C O F P

The image is at infinity

∞

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For convex mirror irrespective of the position of the object, the image is always virtual,

diminished, erect and formed behind the mirror.

Uses of curved mirrors

1. Parabolic mirrors are used for car head lamps, search lamp.

2. Convex mirror is used as a driving mirror because of its wider aperture

3. Concave mirror of long focal length are used as shaving mirror

4. Concave mirror of large diameter are used in reflecting telescope.

5. Concave mirror of large diameter are also used as solar collector for solar ovens and

some solar water heater.

Mirror formula

(e) Object placed between F and P

A Mirror

C F O P I

The image is virtual, upright, magnified and formed at the back of the mirror

F C

I O

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(a) If a concave mirror forms a real image, then the object distance (u), image distance (v)

and focal length f will be positive. If the image formed is virtual, then v will be negative.

For real image formed, the mirror formula for a concave mirror is given as

1

𝑓=

1

𝑒+

1

𝑣 .

If image is virtual, then v will be negative and the mirror formula becomes

1

𝑓=

1

π‘’βˆ’

1

𝑣

Magnification m is given by

π‘š = π‘–π‘šπ‘Žπ‘”π‘’ π‘‘π‘–π‘ π‘‘π‘Žπ‘›π‘π‘’ π‘“π‘Ÿπ‘œπ‘š π‘‘β„Žπ‘’ π‘šπ‘–π‘Ÿπ‘Ÿπ‘œπ‘Ÿ

π‘œπ‘π‘—π‘’π‘π‘‘ π‘‘π‘–π‘ π‘‘π‘Žπ‘›π‘π‘’ π‘“π‘Ÿπ‘œπ‘š π‘‘β„Žπ‘’ π‘šπ‘–π‘Ÿπ‘Ÿπ‘œπ‘Ÿ=

β„Žπ‘’π‘–π‘”β„Žπ‘‘ π‘œπ‘Ÿ 𝑠𝑖𝑧𝑒 π‘œπ‘“ π‘–π‘šπ‘Žπ‘”π‘’

β„Žπ‘’π‘–π‘”β„Žπ‘‘ π‘œπ‘Ÿ 𝑠𝑖𝑧𝑒 π‘œπ‘“ π‘œπ‘π‘—π‘’π‘π‘‘

π‘š =β„Žπ‘–

β„Ž0=

𝑣

𝑒

Magnification is related to object distance u and focal length f by the equation

π‘š =𝑓

𝑒 βˆ’ 𝑓

(b) For a convex mirror that always forms virtual image, principal focus is virtual therefore

its focal length is negative but the object distance is positive. Hence its mirror formula is

given as

1

βˆ’π‘“=

1

π‘’βˆ’

1

𝑣

Solved problems

Example 1

Example 3

An object is placed at a distance of 10.0cm in front of a concave mirror of focal length

15cm. what is the position and nature of the image formed?

Solution

u = 10.0cm, v = ? f = 15cm

Using the mirror formula

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1

𝑓=

1

𝑒+

1

𝑣 ,

1

15=

1

10+

1

𝑣

1

𝑣=

1

15βˆ’

1

10

1

𝑣= βˆ’

1

30

v = - 30cm

Therefore the image is formed 30cm behind the mirror and it is virtual since v is

negative

Example 4

A converging mirror forms an image which is twice the size of the object. Given that the

focal length of the mirror is 5cm, calculate the object distance and the image distance.

Solution

Magnification m = 2, f = 5cm, u = ? v = ?

m = v/u

2 = v/u

V =2u

Considering the mirror formula

1

𝑓=

1

𝑒+

1

𝑣

1

𝑓=

1

𝑒+

1

2𝑒

1

5=

1

𝑒+

1

2𝑒

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1

5=

3

2𝑒

2u = 15

u = 7.5cm

since v = 2u

v = 2 x 7.5 = 15cm

Example 5

An object is placed 30cm from a concave mirror of focal length 15cm. find the linear

magnification of the image produced

Solution

Object distance u = 30cm, focal length f = 15cm

Applying the mirror formula,

1

𝑓=

1

𝑒+

1

𝑣

1

15=

1

𝑒+

1

30

1

𝑒=

1

15+

1

30=

2 βˆ’ 1

30=

1

30

u = 30cm

magnification m = 𝑣

𝑒=

30

30= 1.0π‘π‘š

Note: Educator should carry out an experiment to determine the focal length of a

concave mirror with the students

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Evaluation:

1. Define these terms as applied to curved mirror. Radius of curvature, centre of

curvature, pole, focal length and principal focus of a concave mirror

2. Differentiate between convergent and divergent beam

3. Differentiate between concave and convex mirror

4. Draw the ray diagram of an object placed between C and P and explain its

characteristics

Week end assignment:

1. Draw a ray diagram of an object placed in front of a convex mirror and explain the

characteristics of the image formed.

2. An object of height 3cm is placed 10cm in front of a concave mirror of focal length 5cm.

using scale diagram, determine the position, height, nature of magnification of the

image that will be produced.

3. State one advantage and one disadvantage of using a convex mirror as a driving mirror

4. Explain the term parallax as applied to optics. Describe the method of non-parallax to

locate the position of an image in a plane mirror.

5. With a labeled diagram, describe the mode of operation of a pin-hole camera. Comment

on the effects of the size of the pin-hole on the image formed by the camera.

Objectives

1. The image of an optical pin placed at the principal focus of a concave mirror will be

formedbetween the principal focus and the pole

a. at the centre of curvature

b. between the principal focus and the centre of curvature

c. at infinity

d.

2. A man 1.8m tall stands 3m away from a pin hole camera. If the distance between the pin

hole and the screen of the camera is 0.3m, calculate the height of the image of the man

produced by the camera.

A 0.18m B. 0.50m C. 1.62m D. 18.00m

3. The image in a pin-hole camera is always

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A. Diminished B. enlarged

B. C. upright D. inverted

4. Which of the following statement is/are correct about the image formed by a plane

mirror?

i. The magnification produced is 1

ii. The image distance is the same as the object distance.

iii. The image is real.

iv. The image is laterally inverted.

A i only B. ii only C. iii only D. i and iii only

5. An image which can be formed on the screen is said to be

A. real B. virtual C.blurred D.inverted

. An object is placed between two mirrors which are inclined at an angle of 1200 and facing each

other. Determine the number of images observed in the two mirrors.

A. 1 B. 2 C 3 D. 4

8. A concave mirror of radius of curvature 20cm has a pin placed at 15cm from the pole. What

will be the magnification of the image produced?

A. 4.00 B. 2.00 C.1.33 D.1.50

9. A parallel beam of light is to be obtained from the headlamp of a car. At which of the

following positions should the source of light be placed from the pole of its spherical mirror?

A. At the focal point

B. At the centre of curvature

C. Beyond the centre of curvature

D. Between the focal point and the pole

WEEK 5:

DATE:…………….

SUBJECT: PHYSICS

CLASS: SS11

TOPIC: REFRACTION OF LIGHT WAVES

CONTENTS

1. Refraction of light through rectangular glass block and triangular glass prism

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2. Laws of refraction

3. Critical angle and total internal reflection of light

4. Sun’ s energy and the radiation to the earth

5. Refraction of light through converging and diverging lenses

6. Dispersion of white light and colour mixing.

Sub topic 1: Refraction of light through a rectangular glass block and a triangular glass

prism.

(a) Refraction through a rectangular glass prism

Refraction is a change in direction of light rays as the rays travel from one medium to

another media of different density. Refraction takes place when light travels from air to

glass or from air to water.

OA is the incident ray, OB is the refracted ray. Angle of incidence ( i ) is the angle the ray makes

with the normal ON in air. Angle of refraction OB is the angle the refracted ray OB makes with

the normal ON in the second medium.

The refractive index of glass with respect to air ang is given as

ang=𝑠𝑖𝑛𝑖

π‘ π‘–π‘›π‘Ÿ

Refractive index in terms of wavelength is given as

A Normal (N)

Incident ray (OA)

i Medium 1 e.g air

O

Refracted ray

Medium 2 (glass block)

Refraction of light through rectangular glass block

r

B

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Refractive index n = wavelength of light in medium 1 = Ξ»1

its wavelength in medium 2 Ξ»2

Refraction of light can be used to explain a number of phenomena such as mirage,

apparentdepth of a swimming pool, bending of a straight object e.g metre rule when immersed

partially

Mathematically, real depth, apparent depth and refractive index β€˜n’ are related by the equation

π‘Ÿπ‘’π‘“π‘Ÿπ‘Žπ‘π‘‘π‘–π‘£π‘’ 𝑖𝑛𝑑𝑒π‘₯ 𝑛 =π‘Ÿπ‘’π‘Žπ‘™ π‘‘π‘’π‘π‘‘β„Ž (𝑅)

π‘Žπ‘π‘π‘Žπ‘Ÿπ‘’π‘›π‘‘ π‘‘π‘’π‘π‘‘β„Ž(𝐴)

𝑛 =𝑅

𝐴

Displacement of the object β€˜d’ = Real depth β€˜R’ – Apparent depth β€˜A’

Therefore d = R – A

A = R / n

d = R – A = R – R/n = R(1 – 1/n)

d = R(1 – 1/n)

Evaluation

1. What do you understand by refraction of light?

2. When a ray of light travels from air to glass, what is the formula for calculating the

refractive index of glass with respect to air?

water

image

object d - displacement

A – apparent depth Real depth R

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Sub topic 2: Laws of refraction

We have two laws of refraction. They are,

1. The incident ray, the refracted ray and the normal at the point of incidence all lie in the

same plane

2. The ratio of the sine of angle of incidence to the sine of angle of refraction is constant

for a given pair of media.

The second law is known as Snell’s law of refraction. Refractive index can also be written as

ang=π‘£π‘’π‘™π‘œπ‘π‘–π‘‘π‘¦ π‘œπ‘“ π‘™π‘–π‘”β„Žπ‘‘ 𝑖𝑛 π‘Žπ‘–π‘Ÿ

π‘£π‘’π‘™π‘œπ‘π‘–π‘‘π‘¦ π‘œπ‘“ π‘™π‘–π‘”β„Žπ‘‘ 𝑖𝑛 π‘”π‘™π‘Žπ‘ π‘ 

ang=π‘£π‘Ž

𝑣𝑔

Where ang is refractive index of glass with respect to air.

Educator should verify Snell’s law in the laboratory with the students using a rectangular

glass block.

Example 1

A fish appears to be 2m below the surface of a pond when viewed directly from above. How

far below the surface of the pond is the fish? (Refractive index of water = 1.33)

Solution

Apparent depth = 2m, refractive index n = 1.33

Using the formula: refractive index n = real depth / apparent depth,

Real depth = refractive index x apparent depth = 1.33 x 2 = 2.66m

Example 2

The wavelength of red light in air is 7 x 10 -7m. (a) What is its wavelength in a glass of

refractive index 1.5 (b) What is its speed in the glass. (speed of light in air is 3 x 108m/s)

Solution

Wavelength of red light Ξ»R = 7 x 10 – 7m. Wavelength in glass = Ξ» . Refractive index = n =

1.5

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(a) n = Ξ»R / Ξ»

1.5 = 7 x 10 – 7

Ξ»

Ξ» = 7 x 10 – 7 = 4.7 x 10 – 7 m

1.5

(b) n = V1

V2 where V1 = speed of light in air and V2 = speed of light in glass

1.5 = 3 x 108m/s

V2

V2 = 2 x108m/s.

Example 3

An object is placed directly below a glass block of thickness 3.0 cm.Calculate the lateral

displacement of the object if the refractive index of the glass is 1.5 (JAMB)

Solution

The thickness of the glass is the real depth (R) = 3.0cm, refractive index n = 1.5

Therefore

𝑑 =𝑅(𝑛 βˆ’ 1)

𝑛

𝑑 =3(1.5 βˆ’ 1)

1.5

𝑑 =3 Γ— 0.5

1.5

𝑑 = 1.0 π‘π‘š

Example 4

A ray of light strikes the surface of glass at an angle of incidence of 600. Find the angle of

refraction in the glass. (refractive index of glass is 1.5)

Solution

𝒏 =π’”π’Šπ’π’Š

π’”π’Šπ’π’“

𝟏. πŸ“ =π’”π’Šπ’πŸ”πŸŽ

π’”π’Šπ’π’“

π’”π’Šπ’π’“ =π’”π’Šπ’πŸ”πŸŽ

𝟏. πŸ“

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𝒓 = π’”π’Šπ’βˆ’πŸ (𝟎. πŸ–πŸ”πŸ”

𝟏. πŸ“)

𝒓 = πŸ‘πŸ“. πŸ“πŸŽ

(b) Refraction of light through a triangular glass prism

Refraction of light through a triangular glass prism can be studied practically. To do these,

we need the following apparatus/materials: triangular glass prism, four optical pins,

drawing paper, protractor, and ruler. The procedure is as follows

i. Place the triangular glass prism on the drawing paper and trace its outline ABC

ii. Remove the prism and draw a normal to pass through the point p on line AB

iii. Draw a line RP such that angle of incidence i = 300

iv. Place two pins at points T and G on line RP. The pins should be reasonably separated

and replace the prism on its outline ABC.

v. Looking through side AC, place the third pin at D such that it is in a straight line with the

images of the first two pins. Place the last pin at point H so that the four pins are in a

straight line.

vi. Remove the prism and draw a line through DH to meet AC at Y and extend it to a point

W as shown in the diagram below.

A Refracting angle (A)

W Angle of deviation (d)

Angle of incidence N Angle of emergent (e)

i O

T D

G

H

B C

Refraction of light through a triangular glass block

r Y

angle of refraction

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The experiment can be repeated for four other values of i = 350, 400, 450, and 500 to verify

Snell’s law. If we tabulate the results determining e, sin i and sin r and plot a graph of sin i on

the vertical axis against sin r on the horizontal axis, the slope of the graph will give the

refractive index of the glass. This value should be equal to or approximately 1.5. Also, if we plot

a graph of angle of deviations against angles of incidence i, we should obtain a minimum angle

of deviation ( dm ). This the smallest angle of deviation produced by the prism. At minimum

deviation, the light rays passes symmetrically through the prism. Under this condition, the angle

of refraction at points O and Ywill be the same. In terms of angle of minimum deviation ( dm),

refractive index n is given as:

𝑛 =sin (

π‘‘π‘š+𝐴

2)

sin(𝐴

2)

Students should carry out the experiment using equilateral triangular prism stating precautions

necessary to obtain accurate results

Evaluation

1. State the laws of refraction of light

2. State refractive index formula in terms of angle of minimum deviation

Sub topic 3: Critical angle and total internal reflection of light

When light travels from an optically denser medium e.g glass to an optically less dense medium

e.g air, refraction occurs with faint or weak internally reflected ray in the denser medium fig. a.

As the angle of incidence i increases, the strong refracted ray bends towards the glass- air

interface. For a particular angle of incidence, the refracted ray lies on the air-glass interface fig.

b. the angle of incidence for which this happens is called critical angle. We therefore define

critical angle as the angle of incidence in the denser medium for which the angle of refraction

is 900 when light travels from an optically denser medium to an optically less dense medium.

If this angle is increased, the ray will be reflected internally in the denser medium fig. c. This is

what we called total internal reflection. For total internal reflection to occur, two conditions

must be satisfied.

1. Light must travel from an optically denser medium to an optically less dense medium

2. The angle of incidence in the denser medium must be greater than the critical.

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Refractive index in terms of total internal reflection is given as

n = 1

𝑠𝑖𝑛𝐢 where n is refractive index of glass with respect to air and C is critical angle.

Applications of total internal reflection

1. Periscope

2. Mirage

3. Optical fibres

4. Fish’s view

5. Changing the direction of light using triangular prism.

Some solved problems

Example 5

The refractive index of glass is 1.5. What is the critical angle for glass-air boundary?

Solution

Refractive index n = 1.5, critical angle = C

𝑛 =1

𝑠𝑖𝑛𝐢

𝐢 = π‘ π‘–π‘›βˆ’1 (1

𝑛)

𝐢 = π‘ π‘–π‘›βˆ’1 (1

1.5)

𝐢 = 41. 80

Example 6

Less dense

dense c

Less dense

dense Less dense

dense

Total

internal

reflection

Weak

reflection

Fig a Fig b Fig c

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An equilateral glass prism of refractive index 1.5 produces a minimum deviation when a ray

of light strikes on one face. Calculate (a) the angle of incidence (b) the angle of minimum

deviation.

Solution

Since the prism is equilateral, refracting angle A = 600 and angle of refraction r = 60/2 =

300

(a) At the instant the prism produces a minimum deviation, angle of incidence I,

𝑖 =𝐴 + π‘‘π‘š

2

While the angle of refraction at this instant is r

π‘Ÿ =𝐴

2

Since the refractive angle of the prism A = 600.

π‘Ÿ =60

2

π‘Ÿ = 300

Snell’s law

𝑛 =𝑠𝑖𝑛𝑖

π‘ π‘–π‘›π‘Ÿ

1.5 =sin 𝑖

𝑠𝑖𝑛30

𝑖 = π‘ π‘–π‘›βˆ’1(1.5 Γ— 𝑠𝑖𝑛30)

𝑖 = 48. 60

(b) But,

𝑖 =𝐴 + π‘‘π‘š

2

48.6 =60 + π‘‘π‘š

2

97.2 = 60 + π‘‘π‘š

π‘‘π‘š = 37. 20

Evaluation

1. Explain these terms: critical angle and total internal reflection of light

2. State the conditions for total internal reflection of light to occur

Refraction of light through lenses

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We have two types of lenses namely:

Converging or convex lens and diverging or concave lens. A converging lens is thicker at the

middle than at the edge while a diverging lens is thinner at the middle than at the edge.Lenses

come in different shapes and sizes. Your teacher will show you different types of lenses.

Terms as applied to lenses

The optical centre centre of a lens is that point through the lens where rays pass through

undeviated.

The Principal Axis is the line joining that passes through the optical centre of the lens and

joining the centres of curvature of its surfaces.

The Principal FocusF of a converging or convex lens is that point on the Principal Axis where

rays parallel and close to the principal axis converge after refraction through the lens

The Principal FocusF of a concave or diverging lens is that point on the Principal Axis where

rays parallel and close to the Principal Axis appear to diverge from after refraction through the

lens.

The Focal Lengthf is the distance between the optical centre and the Principal Focus.

The power p of a lens is equal to the reciprocal of the focal length. When f is in metres, it is

measured in Dioptres.

Construction of rays for images formed by lenses

Any two of these rays can be used to obtain the position and nature of the image applying the

fact that

1. A ray from the object, parallel to the principal axis, refracts through the lens and passes

through the principal focus

Convex lens Concave lens

2f f f 2f

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2. A ray from the object which passes through the optical centre does so undeviated.

3. A ray from the object through the principal focus will be parallel to the principal axis

after refraction.

Images formed by a convex lens

1. Object placed beyond 2f of the lens

2. Object placed at less than 2f

3. Object placed at 2f

Converging lens

Object β€˜O’ image I

O f f I

Image is real, inverted, diminished

And formed between f and 2f

C

Converging lens

Object β€˜O’ image I

O f f I

The image is real, inverted , magnified and formed beyond 2f

C

2f f f 2f

2f f f 2f

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4. Object placed between f and C

Object placed at F

Converging lens

Object β€˜O’ image I

O f f I

The image is real, inverted same size

as the object and formed at 2f

C

Image I Converging lens

O f f

Object β€˜O’

The image is virtual, erect, magnified and formed beyond f on the same side with the object

C

Converging lens

Object β€˜O’ image I

f f

The image is formed at infinity

C

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For a concave lens, the image formed is always virtual, erect and diminished irrespective of the

position of the object.

Lens formula

The focal length β€˜f’, image distance β€˜v’ and object distance β€˜u’ are related by the formula

1

𝑓=

1

𝑒+

1

𝑣

π‘šπ‘Žπ‘”π‘›π‘–π‘“π‘–π‘π‘Žπ‘‘π‘–π‘œπ‘› π‘š =π‘–π‘šπ‘Žπ‘”π‘’ β„Žπ‘’π‘–π‘”β„Žπ‘‘

π‘œπ‘π‘—π‘’π‘π‘‘ β„Žπ‘’π‘–π‘”β„Žπ‘‘=

π‘–π‘šπ‘Žπ‘”π‘’ π‘‘π‘–π‘ π‘‘π‘Žπ‘›π‘π‘’

π‘œπ‘π‘—π‘’π‘π‘‘ π‘‘π‘–π‘ π‘‘π‘Žπ‘›π‘π‘’

π‘š =β„Žπ‘–

β„Ž0=

𝑣

𝑒

It can be shown that

π‘š =𝑣 βˆ’ 𝑓

𝑓

Concave lens

Object

Image

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Sign conventions for lenses

1. Focal length for convex or converging lens is positive

2. Focal length for concave or diverging lens is negative

3. For virtual image or erected image, v is negative

4. For real or inverted image, v is positive.

Solved problems

Example 1

A diverging lens has a focal length of 15.0cm. an object 1.5cm high is positioned 30cm in front

of the lens. Find (a) the image distance (b) the height of the image and (c) the magnification

Solution

f = - 15cm (diverging lens), object distance u = 30cm, height of object ho = 1.5cm, image

distance v=? height of image hi =?

Using the lens formula:

1

𝑓=

1

𝑒+

1

𝑣

βˆ’1

15=

1

30+

1

𝑣

1

𝑣=

βˆ’1

15βˆ’

1

30= βˆ’

3

30

𝑣 = βˆ’30

3= βˆ’10π‘π‘š

( this minus sign means the image formed is virtual and erect)

(b) Magnification m =hi

ho=

v

u

hi

1.5=

10

30,

hi Γ— 30 = 1.5 Γ— 10

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hi = 1.5 Γ—10

30

hi = 0.5cm

Example 2

The image of a pin formed by a diverging lens of focal length 10cm is 5cm from the lens.

Calculate the distance of the pin from the lens ( SSCE)

Solution

image distance v = - 5.0cm, object distance u = ? Focal length f = - 10cm (diverging lens)

Using the lens formula

1

𝑓=

1

𝑒+

1

𝑣

1

βˆ’π‘“=

1

π‘’βˆ’

1

𝑣

1

βˆ’10=

1

π‘’βˆ’

1

5

1

𝑒=

1

5βˆ’

1

10=

1

10

u = 10cm.

Example 3

A real image of an object formed by a converging lens of focal length 15cm is three times the

size of the object. What is the distance of the object from the lens. (SSCE)

Solution

Using the formula

m = 𝑓

π‘’βˆ’π‘“

m = 3, f = 15cm, u = ?

3 =15

π‘’βˆ’15

15 = 3(𝑒 βˆ’ 15) = 3𝑒 βˆ’ 45

3𝑒 = 45 + 15

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3𝑒 = 60

𝑒 =60

3= 20π‘π‘š

Example 4

Find the focal length of a lens with power 0.4D

Solution

Power 𝑝 =1

𝑓

0.4 =1

𝑓

𝑓 =1

0.4= 2.5π‘š

𝑓 = 250 π‘π‘š

( since f is positive, the lens is a converging lens)

Educator should carry out an experiment to determine the focal length of a lens

DISPERSION OF WHITE LIGHT

Generally, white light has a band of wavelengths of different colours. This β€˜β€™band’’ is called

β€˜spectrum of white light’.

This phenomenon was first discovered by Sir Isaac Newton in Cambridge in 1666 by making a

small circular opening in a shutter in a dark room and placed a prism near the hole. In this way,

the light was refracted on to the opposite wall. The colours produced were in the order of:

Red, Orange, Yellow, Green, Blue, Indigo, Violet (ROYGBIV).

This therefore shows that a prism can β€˜separate’ or β€˜disperse’ white light into its various colours

or wavelengths.

E

Red

violet screen

Glass prism Source

of

white

light

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In the above diagram, the white light has been separated into the seven colours, called

β€˜β€™spectrum of white light’’, though not pure.

Dispersion is therefore defined as the separation of white light into its component colours.

This separation is due to the fact that different colours of white light travels at different speed

through the glass.

Production of Pure Spectrum

To produce a pure spectrum, a converging lens is placed in between the source of light and the

prism in such that the distance between the source of light and the lens is the focal length of

the lens. Another lens is placed in between the prism and screen to collect the parallel beams

of different colours on the screen.

In this way, a pure spectrum would be produced on the screen.

COLOUR MIXING

All the colours that the eye sees can be made by mixing the three basic colours, called the

β€˜β€™primary colours’’. These colours are red, blue and green.

Mixing any two of these colours will produce a β€˜β€™secondary colour’’. Secondary colours include

magenta, cyan and yellow. All the three colours mixed together will produce a β€˜β€™white light’’.

Narrow

split

Converging

lens

Glass

prism

Converging

lens

screen

red blue magenta

white

cyan yellow

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π‘Žπ‘‘π‘‘π‘–π‘‘π‘–π‘£π‘’ π‘π‘œπ‘™π‘œπ‘’π‘Ÿ π‘šπ‘–π‘₯𝑖𝑛𝑔 βˆ’ π‘™π‘–π‘”β„Žπ‘‘

The mixing of coloured light is called β€˜β€™additive mixing’’. This is the operation in which colour

movies is based on.

COLOURED FILTERS AND PIGMENTS

Coloured filters are made from coloured glass or plastic. A coloured filter transmits its own

colour but absorbs any other colour which falls on it.

An object can only be seen when light is reflected from it into the eye. The substance which

gives an object its colour is called a pigment. A pigment absorbs all colours except its own

which it reflects.

A black pigment absorbs all colour but reflects none. A white pigment reflects all colours.

Coloured objects like paints (pigments) used by painters can also be mixed together.

The mixing of coloured pigments is known as β€˜β€™subtractive mixing’’.

RED RED

GREEN BLUE BLUE YELLOW

orange

green

purple yellow

cyan

magenta

white black

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π‘Žπ‘‘π‘‘π‘–π‘‘π‘–π‘£π‘’ π‘π‘œπ‘™π‘œπ‘’π‘Ÿ π‘šπ‘–π‘₯𝑖𝑛𝑔 βˆ’ π‘™π‘–π‘”β„Žπ‘‘π‘ π‘ π‘’π‘π‘‘π‘Ÿπ‘Žπ‘π‘‘π‘–π‘£π‘’ π‘π‘œπ‘™π‘œπ‘’π‘Ÿ π‘šπ‘–π‘₯𝑖𝑛𝑔 βˆ’ π‘π‘Žπ‘–π‘›π‘‘π‘ 

In the additive colour mixing,

Red + Blue + Green = White

Also, Red + Cyan = White

Blue + Yellow = White

Green + Magenta = White

Since the colours which add together to produce white light are complementary colours, then,

Red is complementary to Cyan

Blue is complementary to Yellow

Green is complementary to Magenta.

Weekend assignment:

Objectives .

1. A converging lens of focal length 15cm forms a virtual image at a point 10cm from the lens.

Calculate the distance of the object from the lens.

A. 10.00cm B. 6.00cm C. 5.00cm D. 1.50cm

2. In a compound microscope, the image formed by the objective lens is at a distance of 3.0cm

from the eye lens. If the final image is at 25.0cm from the eye lens, calculate the focal length of

the eye lens.

A. 0.3cm B. 2.7cm C. 3.4cm D. 8.3cm

3. Which of the following conditions is necessary for the occurrence of total internal reflection of

light?

A. Light must travel from an optically less dense to a denser medium

B. The angle of incidence must be equal to the critical angle

C. The angle of incidence must be greater than the critical angle.

D. The angle of refraction must be 900

4. A converging lens produces an image four times as large as an object placed 25cm from the

lens.

Calculate its focal length.

A. 100cm B. 33cm C. 29cm D. 20cm

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5. The horizontal floor of a water reservoir appears to be 1.0m deep when viewed vertically

From above. If the refractive index of water is 1.35, calculate the real depth of the reservoir.

A. 2.35m B. 1.35m C. 1.00m D. 0.35m

6. A converging lens has a focal length of 5cm. Determine its power.

A. +20.0D B. +0.2D C. -20.0D D. -0.2D

WEEK 6:

DATE:…………….

SUBJECT: PHYSICS

CLASS: SS11

TOPIC: APPLICATION OF LENSES: THE HUMAN EYE

CONTENTS

1. Description of the human eye

2. Eye defects and their corrections

3. Comparison of the human eye and camera

Sub topic 1. Description of the human eye

The human eye is a very sensitive organ of the body, it is protected by a ring of bones or socket,

eye lids and eye lashes. The diagram below shows the essential parts of the human eye.

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The human eye

The eye lens focus light entering the eye onto the retina. The ciliary muscle is attached to the eye

lens and changes the shape of the lens in accordance with the distance of the object in focus. The

retina is a light sensitive area located at the back of the eye. It acts as a screen. The yellow spot

on the retina is the most sensitive spot to light. The least sensitive portion is the blind spot. The

retina is connected to the brain by the optical nerves. The aqueous humor is the transparent liquid

between the lens and the cornea and the vitreous humour is a jelly-like liquid between the lens

and the rest of the eye ball. The iris acts as a stop or diaphragm of variable size. The pupil is a

circular aperture in the iris. The cornea is the transparent front part of the eye, that serves as a

protective covering which refracts most of the light that is entering the eye.

Accommodation is the ability of the eye lens to focus objects at different distances onto the

retina. The nearest point at which an object is clearly seen by an eye is known as the near point

and the farthest point of clear vision is known as the far point. People with normal vision have

the nearest distance at which objects can comfortably be seen at about 25cm from the eye.

Evaluation

1. Mention 5 parts of the human eye

2. Define the term accommodation

Sub topic 2: Eye defects

Long sight (hypermetropia) and short sight (myopia) are two common eye defects. When a

person cannot see objects clearly at a close range except objects that are far away, the person is

suffering from hypermetroia. This happens when the eyeball becomes too short or inability of the

eye lens to focus the light rays onto the retina. His nearest point is more than 25cm. The rays

from objects at a distance of 25cm from the eyes converge and are brought to focus behind the

retina. This can be corrected by using a convex lens of appropriate focal length that will make

the rays from the object converge on the retina. See diagram below.

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Short sight (myopia)

A person suffering from myopia will not be able to see far away objects clearly because rays

from the object are bought to a focus or converge in front of the retina. Only objects close to the

eyes can be seen clearly. Such a person has an eyeball that is too long or eye lenses that are too

convergent. This eye defect can be corrected by using a suitable diverging lens. That is a

diverging lens of appropriate focal length.

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Short-sightedness and its correction

Summarily;

Eyes defects Cause Description Correction 1. Shortsightedness

(myopia)

Eyeball is

too long

Eyes can see object close to it but

not object too far from it. Light

ray from distant object converges

in front of the retina (instead of

converging on the retina.

By using a diverging

lens.

2. Longsightedness

(hypermetropia

Eyeball is

too

Eyes ca see distant object but not

object close to the eye. Light ray

from object closed to the eye

converges behind the retina

(instead of converging on the

retina)

By using a converging

lens

3. Presbyopia Weak

ciliary

muscle

The weak ciliary muscle result in

loss of accommodation property

of the eye. It often comes with old

age

Can be corrected

using bifocal lens

4. Astigmatism Uneven

curvature

of the eye

Surface of the eye lens is uneven.

This prevent the light ray entering

the eyes to focus at a single point.

Can be corrected

using special

cylindrical lens

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lens This result in blur image.

Evaluation

1. Differentiate between long sight and short sight

2. What type of lens is normally used to correct the defects?

Some solved problems

Example 1

Calculate the focal length of a lens needed by a woman whose near point is50cm from her eyes,

assuming that the least distance of distinct vision for a normal eye is 25cm

Solution

for the woman to see an object clearly at 25cm from the eye, the image must be formed at 50cm

on the same side of the lens at her near point.

u = 25cm. v = -50cm (image is virtual).

Using the lens formula:

1

𝑓=

1

𝑒+

1

𝑣

1

𝑓=

1

25βˆ’

1

50

1

𝑓=

2 βˆ’ 1

50

1

𝑓=

1

50

f = 50.0cm

Example 2

A short sighted person cannot see distinctly objects beyond 80cm from his eye. What is the focal

of the correcting lens he needs to see distant objects clearly?

Solution

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For the short-sighted person, an object at infinity must be made to appear to be at his far point

which is 80cm away. The image of the distant object must be formed on the same side of the lens

as the objects.

Therefore v = - 80cm, u = ∞,

Using the lens formula:

1

𝑓=

1

𝑒+

1

𝑣

1

𝑓=

1

βˆžβˆ’

1

80

f = -80cm

Weekend assignment

1. Reading assignment: read on wind and stringed instruments

2. Explain two other eye defects.

WEEK 7: MID – TERM BREAK

WEEK 8:

DATE:…………….

SUBJECT: PHYSICS

CLASS: SS 2

TOPIC: APPLICATION OF LENSES (CONTD): CONTENT: - The Camera - Comparing the human eye with the camera

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- Simple and compound microscope - Telescope - Simple periscope (SEE APPLICATIONS MIRROR) - film projector

THE CAMERA

The camera is a device for taking photographs of an object. It consists of

1. A light proof box with a converging lens in front of it and a light sensitive film at the back. The

distance between the lens and the film can be varied so that objects in front of the lens can

always be focused on the film by the converging lens.

2. A shutter of variable speed between the lens and the film to admit or shuts off light from the

film.

3. An aperture that regulates the amount of light energy getting to the film

4. A diaphragm that regulates the size of the aperture

When taking a photograph of an object, the camera lens will be pointed at the object and the

focusing ring is used to adjust the distance between the lens and the film until a sharp image of

the object is obtained on the film. A button is then pressed so that the shutter quickly opens and

closes, exposing the film, for a brief period to light from the object.

Evaluation

1. Mention 4 parts of a simple camera and explain their functions

2. Explain how a camera is used to take photographs of an object.

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Sub topic 2: Comparison of the human eye with camera

(a) Similarities between the human eye and camera

1. The human eye is impregnated with black pigment within while the camera consists of a

light-tight box painted black inside

2. The human eye has the retina which is light sensitive. The camera has a film which is

also light sensitive

3. Both have converging lens systems to focus light from an external object

4. The iris in human eye performs the same function as diaphragm in camera. i.e both

regulates the amount of light entering the eye/camera respectively

5. The pupil in human eye performs the same function as the aperture in camera

Differences between the human eyes and the camera

s/n Human eyes Camera 1 Lens has a variable focal length Lens has a fixed focal length

2 Image distance is fixed Image distances could be varied

3 It is a biological organ It is a mechanical devices

4 It may suffer from defect It can’t suffer eye defect

5 It position does not change. It remains

in the eye socket

It position can be changed

Summarily;

A camera device that can be used to record the image of object. Light ray from objects are

formed on a light sensitive material /film.

The image formed by a camera is

(a) Inverted

(b) Diminished

aperture

shutter

film diaphragm

lens

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(c) Real

Evaluation

1. Mention 4 similarities between the human eye and camera

2. Mention 4 differences between the human eye and camera

Subtopic 3: Simple microscope

A converging lens acts as a simple microscope (magnifier) or magnifying glass as shown below.

If an object is placed in front of the lens between the optical centre and the principal focus, the

image formed will be enlarged, erect and virtual. The magnifying glass is used for reading tiny

writings and for viewing specimens in the laboratory

Magnifying glass

Summarily;

A simple microscope sometimes called a magnifying glass. It consists of a single converging

lens with a long focal length. The object is position between the principal focal and the optical

pole. The image produced is:

Magnified

Erect

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Virtual

The compound microscope

The compound microscope consists of two converging lenses, the objective lens and the eye

piece. The two lenses have short focal length. When an object is placed in front of the objective

lens, a magnified, inverted and real image of an object OA will be produced if well illuminated.

The eye piece is moved so that IB is nearer to it than its principal focus. A magnified but virtual

image PQ of IB is formed at Q with the eye piece lens acting as a magnifying glass for an object

at I. Thus the object OA is enlarged by the action of the two lenses.

The magnifying power m of the compound microscope is given as m = m1 x m2 = PQ/AO.

The compound microscope

Summarily; A compound consist of two converging lens of short focal length. The lens close to the

object is called objective lens, while the lens close to eyes through which the final image is

viewed is called the eyepiece. The focal length of the eyepiece is longer than the focal length of

the objective lens. The final image produced by the compound microscope is:

Magnified

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Inverted

virtual

Solved problem

A compound microscope has lenses of focal lengths 1.0cm and 3.0cm. an object is placed 1.2cm from

the object lens and the final image is formed 25.0cm from the eye piece. Calculate the distance between

the two lenses

Solution

Let the distance between the two lenses be ycm

Focal length of objective lens f0 = 1.0cm,

focal length of eye piece fo = 3.0cm,

object distance for objective lens uo = 1.2cm

object distance for eye-piece ue = ?

image distance for objective lens vo = ?

image distance for eye piece ve = 25.0cm

for objective lens,

1

π‘“π‘œ=

1

π‘£π‘œ+

1

π‘’π‘œ

1

1=

1

π‘£π‘œ+

1

1.2

1

π‘£π‘œ=

1

1βˆ’

1

1.2= 1 βˆ’ 0.833 = 0.167

1

π‘£π‘œ= 0.167

Vo= 6cm

For eye-piece, ve is negative ( final image is always virtual)

1

𝑓𝑒= βˆ’

1

𝑣𝑒+

1

𝑒𝑒

1

𝑓𝑒+

1

𝑣𝑒=

1

𝑒𝑒

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1

𝑒𝑒=

1

3+

1

25

1

𝑒𝑒=

1

3+

1

25

1

𝑒𝑒=

25 + 3

75

1

𝑒𝑒=

28

75

𝑒𝑒 =75

28= 2.7π‘π‘š

But y is distance between the two lenses = 𝑒𝑒 + 𝑣𝑒 = 6 + 2.7 = 8.7π‘π‘š

Evaluation

1. Differentiate between the compound microscope and the simple microscope

2. Mention two similarities between the simple microscope and the compound microscope

The astronomical telescope

The astronomical telescope is used for viewing celestial bodies like stars, planets, moon

e.t.c. it consists of two converging lens that are mounted so that they have a common

axis. The objective lens has a longer focal length than the eye-piece. This arrangement

makes the telescope to have a high magnifying power. In the diagram below, rays from

distant objects coming to the objective lens arrive as parallel rays, inclined at a small

angle to the principal axis. A real image of the object is formed at the principal focus fo of

the objective lens figure a. The eye piece can be adjusted so that the image lies within a distance of one

focal length. The eye piece acts as a magnifier and produces a magnified image PI QI of the distant

object. The final image is inverted. If the lenses are arranged so that the principal focus of the objective

lens coincides with that of the eye piece, the image of the distant object will be at infinity as shown in

figure b. The telescope in this arrangement is said to be in normal view.

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The Astronomical Telescope

The slide projector

A slide projector uses a convex lens to form a real, magnified and an inverted image of a slide or

film on a screen. The slide (object) is placed between f and 2f from the projection lens. Its

essential parts are

1. A small and powerful source of light with a converging mirror placed behind it.

The converging mirror directs light rays towards the slide.

2. A condenser (a combination of two Plano-convex lenses). The condenser collects

the light rays from the light source and to converge them onto the slide so that

every part of the slide is well illumination. It also protects the slide from the heat

of the lamp.

3. A slide carrier where the object can be placed upside down so that it will appear

erect on the screen

4. A focusing lens that is placed near the lens

5. A white screen that receives the image.

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The slide projector

Evaluation

1. Mention 4 components of the slide projector

2. Which instrument is used to view celestial bodies?

Week end assignment

1. Mention 4 differences between the simple camera and the slide projector

2. Draw a labeled diagram of the terrestrial telescope and explain how it works

WEEK 9:

TOPIC: SOUND WAVES

CONTENTS

1. Sources of sound

2. Transmission of sound

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3. Characteristics of sound

4. Forced vibrations

5. Solved problems

Sub topic 1: Sources of sound

Sound is a form of wave motion which is conveyed through an elastic medium from a vibrating

body to a listener. It is a longitudinal wave. Sound has a number of sources including sound from

animals, moving aircraft, vehicles, vibrating turning fork, e.t.c

Sound wave is also a mechanical wave. That is, it cannot travel through vacuum. There must be a

material medium for its to propagate. Astronauts on the moon can only communicate each other

via walkie-talkie even at close distance because there is no air molecule to propagate sound wave

on the moon.

Sub topic 2: Transmission of sound

Sound waves are produced from vibrating systems and travels as a series of compressions and

rarefactions as discussed earlier. Sound waves do not travel through a vacuum. It requires a

material medium. Your teacher will show you a simple experiment to investigate this fact. Speed

of sound varies from medium to medium because it depends on the density, elasticity and

temperature of the transmitting medium. For example, the speed of sound in air is about 330m/s

at 00 C. in water it is about 1500 m/s. in steel rods, it can be as high as 5000m/s. wind also affect

the speed of sound in relation to a listener. A louder sound is heard if the direction of travel of

the wind is the same as the direction of propagation of the sound. If the two directions are

opposite, the sound will decrease. In air the speed of sound increases by about 0.6m/s for each

degree rise in temperature. The rise is much less in solids and liquids

As mentioned earlier, the speed of sound varies with density and the elastic properties of the

medium. Experiment shows that, the velocity β€˜v’ of sound is proportional to the Young’s

modulus (E) of elasticity and the density, β€˜d’ according to the equation:

𝑣 ∝ √𝐸

𝑑

. In gas, it is independent of pressure and proportional to the absolute temperature of the gas.

𝑣 ∝ βˆšπ‘‡

Some applications of sound waves

1. Echoes: an echo is a sound heard after the reflection of sound waves from a plane

surface. Echo can be used to determine the speed of sound in air.

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2. Echo sounding devices: Sonar is an echo sounding device which can be used on a ship to

determine the depth of the sea. When a sound wave is sent into the sea bed, it get

reflected back in time β€˜t’ seconds after striking the sea bed. The time of travel of the

wave can be measured using a stop watch and since the speed of sound in water is

known, the depth of the sea can thus be calculated using the equation: speed (v) =

distance (π‘₯) /time (t). since distance =2 π‘₯,

π‘₯ =𝑣𝑑

2

3. Exploration of natural resources(oil and gas): geophysicists can use the principle of

echo to detect the presence of mineral resources in the ground. To do these, a small

explosion is set off on or just below the earth’s surface. The sound waves will be

reflected by different layers of underground rocks. The Geologists can use the nature of

each echo and the time it takes each echo to reach the surface to detect the presence of

some mineral resources.

4. Reverberation :Reverberation is a phenomenon that occurs as a result of multiple

reflections of sound waves from walls, roof and floor of a large hall. Some rooms and

halls are padded to minimized or control reverberation.

5. Beat:This is a phenomenon whereby two notes of nearly equal frequency (pitch) are

sounded together resulting to a rise and fall of intensity of the sound. This happens as a

result of constructive interference of sound. The beat frequency is the difference in the

frequencies.

6. Doppler Effect:This is a change in frequency (pitch) of a source when there is a relative

motion between the source and the observer. For example, if you are stationary, and

an ambulance with siren passes with speed, you will observe a sudden drop in the pitch

of the sound.

Evaluation

1. Light require a material medium for its propagation true of false

2. Mention 5 sources of light

3. What is an echo? Give 2 applications of echo

Source of

sound x

reflector

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Sub topic 3: Characteristics of sound

A musical note is a sound which originates from a source that is vibrating at certain set

frequencies. Noise is produced by sources vibrating with no definite frequency. Musical notes

are characterized by pitch, quality and loudness.

Pitch: Pitch is the characteristic of a note which enables us to differentiate a high note from a

low one. Pitch depend on frequency

Quality: The quality of a note is the characteristic that distinguishes it from another note of the

same pitch and loudness when played on musical instruments. The quality of the note β€˜C’ played

on a piano is different from that of the middle β€˜C’ played on a violin. Musical instruments consist

of sound of different frequencies blended together. That is why they cannot give out pure tones.

The strongest audible frequency in the instrument is the fundamental frequency β€˜fo’ others are

integral multiples of fo such as, 2fo, 3fo, 4fo. e.t.c. These are called overtones or harmonics.

Intensity and loudness: The intensity of sound at a certain place is the rate of flow of energy

per unit area perpendicular to the direction of the sound wave.

Loudness: is a sensation in the mind of an individual observer, depending on the intensity of

sound.

Summarily;

Characteristics of sound Factor affecting the characteristic

1 Pitch Frequency

2 Intensity /loudness Amplitude

3 Quality Harmonics

Note that not all sounds can be heard by the human ear. The human ear can respond to sounds

of frequencies ranging between 20Hz to 20000Hz. Sounds with frequencies much above these

are called ultra sounds

Resonance: This is a phenomenon whereby a vibrating body makes another body to vibrate

when its frequency of vibration is the same with the natural frequency of the second body.

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Sub topic 4: Forced vibration

A vibration is said to be free if a body is disturbed in a short period of time and allowed to

vibrate with its own natural frequency. Examples are the vibration of a turning fork and a

loaded test tube oscillating in water. The vibration is said to be forced if the body is continually

disturbed so that it does not vibrate with its own natural frequency. Musical instruments such

as flutes, drums, are either open or closed pipes. A closed pipe is closed at one end only while

an open pipe is closed at both ends. Experiments show that the frequency of vibration of air in

these pipes increases as the length of air column decreases. i.e f ∝1

𝑙

Vibrations in a closed pipe:Forced vibration can be demonstrated using a tall tube filled with

water. The column or length of air can be varied by letting water out of it. A column of air in the

tube will have its own natural frequency of vibration. Suppose we have a turning fork of

frequency fo and we set it to vibrate over a column of air in the tube with length β€˜l1’. If the

length of the air column is gradually increased by running off water, a large sound will be heard.

(forced vibration). When this happens it means the air column now vibrates with a frequency

that is the same with that of the turning fork. The incident wave will be reflected at the closed

end of the tube and the reflected wave will combine with the original wave to produce a

standing wave. The close end is a node since the air at that point cannot move. The open end is

an antinode. This resonance is the first one.

The wavelength Ξ» is given as 𝑙 =Ξ»

4 or Ξ» = 4𝑙

Since 𝑣 = 𝑓 Ξ»

c = end correction

c

Incident

Wave 𝑙1 =πœ†

4

𝑙2 =3πœ†

4

Overtones of a closed pipe

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The fundamental frequency fo is given as

π‘“π‘œ =𝑣

Ξ»=

𝑣

4𝑙

Where v is the speed of the sound in air. f0 is the fundamental frequency of the closed pipe.

If we further increase the air column by running off water from the tube, a point will be

reached when another loud sound will be heard. In this position, a second node will be formed

so that the wavelength at this point is obtained from

𝑙 =3Ξ»

4 or Ξ» =.

4𝑙

3

The frequency 𝑓1 at this point is given as:

𝑓1 =𝑣

πœ†

𝑓1 =𝑣4𝑙

3

𝑓1 =3𝑣

4𝑙

𝑠𝑖𝑛𝑐𝑒 𝑓0 =𝑣

4𝑙 𝑓1 = 3𝑓0

This frequency 𝑓1 = 3π‘“π‘œ is called the third harmonic or first overtone of a closed pipe. A

harmonic is a note with frequency equal to an integral multiple of that of the fundamental

note. The next overtones are 5π‘“π‘œ, 7π‘“π‘œ, 9π‘“π‘œ and so on. Only odd harmonics are present.

If we consider the end correction β€˜c’, At first resonance,

Ξ»

4= 𝑙1 + 𝑐

At second resonance,

3Ξ»

4= 𝑙2 + 𝑐

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The end correction β€˜c’ arises from the fact that the antiinode at the top does not exactly

coincides with the top of the tube but projects slightly above it by a length β€˜c’. if we subtract

equation 1 from equation 2, the end correction will be eliminated so that

Ξ»

2= 𝑙2 βˆ’ 𝑙1. Hence,

Ξ» = 2(𝑙2 βˆ’ 𝑙1)

but 𝑣 = 𝑓 Ξ»

Therefore v = 2f(𝑙2 – 𝑙1 ). With this equation, the velocity of sound can be obtained from the

values of 𝑙2 , 𝑙1 and the frequency β€˜f’ of thee turning fork.

Note the above set up is a resonance tube experiment which can be used to determine the

velocity of sound in air.

Vibrations in an open pipe.

In an open pipe, the two ends of the pipe must end in an antinode. The first harmonic or the

fundamental note has a mid-point as the node. Hence, 𝑙 =Ξ»

2 or Ξ» = 2𝑙. The fundamental

frequency is given as:

𝑓0 =𝑣

2𝑙λ

The second harmonic has frequency

𝑓1 =𝑣

Ξ»=

𝑣

𝑙=

2𝑣

2𝑙= 2𝑓0

The third harmonic is 𝑓2 =𝑣

Ξ»=

3𝑣

2𝑙= 3𝑓0

The next harmonics are: 4π‘“π‘œ, 5π‘“π‘œ, 6π‘“π‘œ and so on. Thus, for open pipes all harmonics are

possible.

(a) (b) (c)

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Note: The velocity of sound wave in air using resonance tube is given as v = 2f(𝑙2 – 𝑙1 )

Where v= velocity of sound in air, f is frequency of the vibrating air column, 𝑙1 is first

resonant length. 𝑙2 is length of second resonant.

Overtones in strings

Musical instruments such as guitar, violin,… produce sound when string attached to a sound

box vibrate. The frequency of the sound produced is depends on the following factors

Length of string: the frequency is inversely proportional to the length of the string.

𝑓 ∝1

𝑙

𝑓1

𝑓2=

𝑙2

𝑙1

Tension in the string: the frequency is directly proportional to the square root of the

tension in the string.

𝑓 ∝ βˆšπ‘‡

𝑓1

𝑓2= √

𝑇1

𝑇2

Linear density of the string: the frequency is inversely proportional to linear density of

the string.

𝑓 ∝1

βˆšπœ‡

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𝑓1

𝑓2= √

πœ‡2

πœ‡1

Linear density of the string can be defined as the ratio of the mass of the string to its

linear.

π‘™π‘–π‘›π‘’π‘Žπ‘Ÿ 𝑑𝑒𝑛𝑠𝑖𝑑𝑦 πœ‡ =π‘šπ‘Žπ‘ π‘ (π‘š)

π‘™π‘’π‘›π‘”π‘‘β„Ž(𝑙)

πœ‡ =π‘š

𝑙

Velocity: the velocity of sound wave in string is given as

𝑣 = βˆšπ‘‡

πœ‡

Where T is the tension in the string and

ΞΌ – linear density of the string.

When the string vibrates in its fundamental mode

Distance between successive node:

𝑙 =πœ†

2

πœ† = 2𝑙

𝑏𝑒𝑑 π‘“π‘Ÿπ‘’π‘žπ‘’π‘’π‘›π‘π‘¦ 𝑓 =𝑣

πœ†

π‘Žπ‘›π‘‘ 𝑣 = βˆšπ‘‡

πœ‡

𝑓 =1

2π‘™βˆš

𝑇

πœ‡

𝑓0 ==1

2π‘™βˆš

𝑇

πœ‡

For the first overtone (2nd harmonic)

L

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𝑓1 =1

𝐿√

𝑇

πœ‡

For the second overtone ( 3rd harmonics)

π’‡πŸ =πŸ‘

πŸπ‘³βˆš

𝑻

𝝁

For the nth overtone ;

𝒇𝒏 = (𝒏 + 𝟏)π’‡πŸŽ

Solved problems

Example 1.

The frequency of a fundamental note from a closed pipe is 200Hz. What is the frequency of the

next possible note from the same pipe?

Solution

For a closed pipe, the possible harmonics are f0, 3f0, 5f0 e.t.c f0 = 200Hz

The frequency of the next harmonic is 3f0 = 3 x 200Hz = 600Hz.

Example 2

A pipe of length 45cm is closed at one end. Calculate the fundamental frequency of the sound

wave generated in the pipe if the velocity of sound in air is 360m/s (neglect end correction)

Jamb.

Solution

For a closed pipe, 𝑙 =πœ†

4𝑙 = 45π‘π‘š given

Therefore πœ† = 4 Γ— 45 = 180π‘π‘š = 1.8π‘š.

𝑣 = 𝑓 πœ†

𝑓 =𝑣

πœ†

360

1.8= 200𝐻𝑧

L

L

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Example 3

The shortest length of the air column in a resonance tube at resonance is 0.12m and the next

resonance length is 0.37m. Calculate the frequency of the vibration. (speed of sound in air is

340m/s).

Solution

v = 340m/s, 𝑙1 = 0.12m, 𝑙2 = 0.37m, f =?

Using the formula

v = 2f(𝑙2 – 𝑙1)

f = v / 2(𝑙2 – 𝑙1)

= 340/2(0.37 – 0.12)

= 680Hz.

Example 4

A string of length 20cm fixed at both ends and set into vibration. If the velocity of sound in air is

340m/s, calculate (a) the wave length (b) the fundamental frequency (c) the second harmonic

frequency.

Solution

(a) Length of string β€˜π‘™β€² = 20π‘π‘š = 0.2π‘š, velocity of sound = 340m/s, wavelength β€˜πœ†β€² =?

𝑙 =πœ†

2

πœ† = 2𝑙 = 2 Γ— 0.2 = 0.4π‘š

(b) v = fo Ξ»o

340 = fo x 0.4

fo = 340/0.4 = 850Hz

(c) The second harmonic is 2fo = 2 x 850 = 1700Hz

Example 5

A string has a length of 80cm and a mass of 1.92 x 10 – 3 What is the tension in the string, if its

fundamental frequency is 156.25Hz?

Solution

fo=1

2π‘™βˆš(

𝑇

π‘š)

Fundamental frequency fo = 156.25Hz , Length of string = 80cm = 0.80m, Tension T = ? Mass per unit

length of string β€˜m’ = 1.92 x 10 – 3 / 0.80 = 2.4 x 10– 3kg/m,

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156.25 =1

2Γ—0.8√

𝑇

2.4Γ—10βˆ’3

Squaring both sides, 156.252 = (1

(2Γ—0.8))2 Γ— (

𝑇

2.4Γ—10βˆ’3 )

24,414.0625 =0.625 Γ— 𝑇

0.0024

24,414.0625 x 0.0024 = 0.390625 x T

T = 24,414.0625 x 0.0024/0.390625 =150N.

Week end assignment:

1. Reading assignment: read on the human eye ( comparison of the eye and camera),

defects of the human eye and their corrections

2. Give three differences between music and noise

3. Give three applications of resonance.

4. Describe a simple experiment to determine the speed of sound in air using the principle

of echo.

5. A pipe closed at one end is sounding its fundamental note. If the length of the pipe is

10cm, calculate the wavelength of the note. (neglect end correction of the pipe).

Answer = 40cm

WEEK: 10

DATE:…………….

SUBJECT: PHYSICS

CLASS: SS 2

TOPIC: APPLICATION OF SOUND WAVES: (MUSICAL INSTRUMENTS)

CONTENTS

1. Wind instruments

2. String instruments

3. Percussion instruments

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additional teaching aid for teachers and students. Please this material should not be commercialized in any form without

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Sub topic 1: Wind instruments

Wind instruments are classified as aerophones. They produce sounds when air is blown into

them. Sound is produced in these instruments because the air column in them vibrates. Whether

the instrument is a closed pipe or an open pipe, the air column determines the quality of the note

produced. The frequency β€˜f’ of the note depends mainly on the length β€˜π‘™β€™ of the vibrating column

and it is inversely proportional to it, i.e ∝1

𝑙. a short column of air will produce a high pitch while

a long column of air will produce a high pitch. Typical examples of wind instruments are, flutes,

clarinets, saxophones, trumpets, mouth organ e.t.c

Trumpets saxophone

Sub topic 2: String instruments

String instruments are also called chordophones. They are instruments that use stretched strings

or chords and operates based on the equation:

𝑓 =1

2π‘™βˆš(

𝑇

π‘š). This means that the frequency is inversely proportional to the length β€˜π‘™ β€˜of the

string, directly proportional to the square root of the tension β€˜T’ on the string and inversely

proportional to the square root of the mass β€˜m’ per unit length of the string. For example

vibrating length of a thick and loose guitar string will produce a low frequency note. But thin,

short and taut strings will produce high frequency notes. These instruments produce sound as a

result of the vibrations of the strings in them. The strings of these instruments can vibrate as a

whole and also in loops so that both fundamental and various harmonics are produced. The

quality of the sound produced is upon the combination of the fundamental harmonic and other

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additional teaching aid for teachers and students. Please this material should not be commercialized in any form without

prior formal engagement with school management. This material was developed for the use of teachers and students of the

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harmonics. Typical examples of string instruments are; sonometer, the guitar, the piano, violin,

harps.

Harp Guitar Violin

Sub topic 3: Percussion instruments

These are musical instruments that you can hit, strike, or scrape. They produce sound

when they vibrate. Instruments under this category include; xylophone, talking drum,

tambourine, bell, xylophone, e.t.c

Talking drum Steel Drum Tambourine

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additional teaching aid for teachers and students. Please this material should not be commercialized in any form without

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therefore to commercialize this document in any form without prior formal discussion with the management.

Bell Xylophone

BEAT

When two notes of nearly equal frequency are sounded together, the resulting sound is a periodic

rise and fall in loudness. These alteration in loudness are known as beats. Beats are due to

interference of the wave produced by two notes.

The frequency f of beats is the number of intense sound heard per second.

𝑓 =1

𝑇

Uses of Beats

1. It is used to determine the frequency of a tuning fork or to measure an unknown frequency.

2. Beats could be used to tune an instrument. E.g, piano.

DOPPLER EFFECT.

When the siren on a moving police car buzzes at the car passes a stationary observer, the sound shifts

from a lower pitch roar to a high pitch screen as the car approaches but shift from a high-pitch sound to a

lower pitch sound as the car moves away. This characteristic shift in frequency of sound due to relative

moving between a sound of a wave and the observer is called DOPPLER EFFECT. This effect was first

studied in detailed by an Austrian Physicist and Mathematician Christian Johann Doppler (1803-1853)

Doppler effect can be define as an alteration in the observed frequency of a sound due to motion of

either the source or the observer.

The doppler effect occurs to only for sound but for any wave when there is relative motion between the

observers and the source. There are doppler shifts in the frequency of sound light and water waves.

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additional teaching aid for teachers and students. Please this material should not be commercialized in any form without

prior formal engagement with school management. This material was developed for the use of teachers and students of the

Goodwill Group of Schools. All financial commitment has been duly fulfilled by the school management. It is prohibited

therefore to commercialize this document in any form without prior formal discussion with the management.

Doppler shift can be used to determine velocity such as when ultrasound is reflected from blood in a

medical diagnostic. The recession of galaxies is determined by the shift in the frequencies of light

received from them and has implied much about the origins of the universe.

For a stationary observer and a source moving at speed v

π‘œπ‘π‘ π‘’π‘Ÿπ‘£π‘’π‘Ÿ π‘“π‘Ÿπ‘’π‘žπ‘’π‘’π‘›π‘π‘¦ π‘“π‘œπ‘π‘  = 𝑓𝑠 (𝑐

𝑐 Β± 𝑣)

βˆ’ π‘“π‘œπ‘Ÿ π‘Žπ‘π‘π‘Ÿπ‘Žπ‘β„Žπ‘–π‘›π‘” π‘ π‘œπ‘’π‘Ÿπ‘π‘’

+ π‘“π‘œπ‘Ÿ π‘Ÿπ‘’π‘π‘’π‘‘π‘‘π‘–π‘›π‘” π‘ π‘œπ‘’π‘Ÿπ‘π‘’

fs – frequency of the wave

c - speed of the wave

v – speed of the source

(Note: use minus when the source is moving toward to observer. Use plus when the source is moving

away from the observer)

for a stationary source and a moving observer

π‘‚π‘π‘’π‘Ÿπ‘£π‘’π‘Ÿ π‘“π‘Ÿπ‘’π‘žπ‘’π‘’π‘›π‘π‘¦ π‘“π‘œπ‘π‘  = 𝑓𝑠 (𝑐 Β± 𝑣

𝑐)

βˆ’ π‘“π‘œπ‘Ÿ π‘Ÿπ‘’π‘π‘’π‘‘π‘–π‘›π‘” π‘œπ‘π‘ π‘’π‘Ÿπ‘£π‘’π‘Ÿ

+ π‘“π‘œπ‘Ÿ π‘Žπ‘π‘π‘Ÿπ‘œπ‘Žπ‘β„Žπ‘–π‘›π‘” π‘œπ‘π‘ π‘’π‘Ÿπ‘£π‘’π‘Ÿ

(note: use minus when the observer is moving away from the source. Use plus when the observer is

moving toward the source)

Evaluation

1. What is the difference between percussion and string instruments?

2. Mention 3 wind instruments

3. Mention 3 string instruments

4. Mention 3 percussion instruments

Week end assignment

1. Reading assignment: read on molecular theory of matter

This material is NOT the property of Goodwill Group of Schools but has been adopted by the school management as

additional teaching aid for teachers and students. Please this material should not be commercialized in any form without

prior formal engagement with school management. This material was developed for the use of teachers and students of the

Goodwill Group of Schools. All financial commitment has been duly fulfilled by the school management. It is prohibited

therefore to commercialize this document in any form without prior formal discussion with the management.

2. Identify the different cultural groups in Nigeria and their local musical instruments.

WEEK 11: Revision

WEEK 12: Exams

REFERENCE TEXTS:

1. Senior Secondary School Physics by P.N. Okeke et al. 2011.

2. New School Physics for Senior Secondary Schools by Anyakoha, M.W. 2010

4. Science Teachers Association of Nigeria Physics for Senior Secondary School, Book 1. New

Edition; 2012.

5. Melrose Physics for Senior Secondary School, Book 1 by Akano, O and Onanuga, O.O. 2012.