ICSE Class 10 Physics Chapter 6 Spectrum Notes | PDF Download

ICSE Class 10 Physics Chapter 6 Spectrum Notes

Prepare for your ICSE Class 10 Physics examination with these complete Spectrum Notes based on the latest ICSE syllabus. These notes cover every important concept including the electromagnetic spectrum, infrared rays, ultraviolet rays, X-rays, gamma rays, visible spectrum, properties, uses, detection methods, and previous year exam questions in an easy-to-understand format.

Our ICSE Class 10 Physics Chapter 6 Spectrum Notes PDF are specially designed for quick revision and board exam preparation. Each topic is explained with simple language, diagrams, tables, memory tricks, and important points frequently asked in ICSE examinations.

Rohit Academy offers expert-curated ICSE Class 10 Physics Study Materials including ICSE Spectrum Chapter Notes, diagrams, and key formulas for better understanding.

ICSE Class 10 Chapter 6 Spectrum Ex 6(A) Solutions
ICSE Class 10 Chapter 6 Spectrum Ex 6(A) Solutions
ICSE Class 10 Chapter 6 Spectrum Ex 6(A) Solutions
ICSE Class 10 Physics Chapter 6 – Spectrum Previous Year Questions

Definition
Deviation is the change in the direction of a light ray when it passes through a prism.

Formula:
Total deviation (δ) = δ1 + δ2
Where:

  • δ1 = Deviation at the first surface
  • δ2 = Deviation at the second surface
ICSE Class 10 Physics Chapter 6 Spectrum img13

(i) Angle of incidence (i) : deviation first  decreases, becomes minimum at the  angle of minimum deviation, then  increases as i increases.

(ii) Angle of prism (A) : larger A gives larger deviation.

(iii) Refractive index / colour (μ or λ) : higher μ (shorter wavelength) gives larger deviation.

  • When white light passes through a prism, different colours deviate by different amounts because the refractive index of the prism varies with the wavelength of light.
  • Different colours travel with different speeds inside glass.
    • Shorter wavelength → Higher refractive index → Greater deviation
    • Longer wavelength → Lower refractive index → Smaller deviation
  • Colour is a subjective property of light and is determined by its wavelength.
  • Red colour  ⇨ Highest Wavelength ⇨ Maximum Velocity ⇨ Least Deviation ⇨ least frequency 
  • Violet colour  ⇨ least Wavelength ⇨ Minimum Velocity ⇨ maximum Deviation  ⇨  maximum frequency
Colour Deviation
Violet Maximum
Indigo High
Blue High
Green Moderate
Yellow Less
Orange Lower
Red Minimum

White light consists of seven colours.

ICSE Class 10 Physics Chapter 6 Spectrum img16
Colour Wavelength (Approx.) Frequency (Approx.)
Violet 400 – 446 nm Highest
Indigo 446 – 464 nm High
Blue 464 – 500 nm High
Green 500 – 578 nm Medium
Yellow 578 – 592 nm Medium
Orange 592 – 620 nm Low
Red 620 – 800 nm Lowest
  • Shortest wavelength: Violet (≈400 nm)
  • Longest wavelength: Red (≈800 nm)
  • Highest frequency: Violet
  • Lowest frequency: Red
  • Maximum deviation: Violet
  • Minimum deviation: Red

Formula
c = fλ

Where,

  • c = Speed of light
  • f = Frequency
  • λ = Wavelength

Definition
Dispersion is the splitting of white light into its constituent colours when it passes through a prism.

Definition
The band of seven colours obtained on passing white light through a prism is called the spectrum.

ICSE Class 10 Physics Spectrum img2

Sir Isaac Newton passed sunlight through a small opening and then through a glass prism.

Observation
A band of seven colours appeared on a white screen.

Conclusion

  • White light is a mixture of seven colours.
  • Each colour has a different wavelength.
  • White light is polychromatic.
  • Light of different colours has different wavelengths and speeds in glass.
  • Different colours deviate by different angles at the first surface of the prism.
  • Violet deviates the most; Red deviates the least.
  • At the second surface, only refraction occurs colours spread further to form the spectrum.
  • Dispersion occurs at the first surface of the prism.
  • Refraction takes place at both surfaces.
  • A prism does not create colours.
  • It only separates colours already present in white light.
  • Speed is maximum for red light.
  • Speed is minimum for violet light.

As wavelength increases,

  • Speed increases
  • Refractive index decreases
  • The Electromagnetic Spectrum (EMS) is the complete range of electromagnetic waves arranged according to their wavelength or frequency.
  • The visible spectrum is only a small part of the electromagnetic spectrum. Waves beyond the visible region are called the invisible spectrum.

Increasing Wavelength (Decreasing Frequency)

  1. Gamma Rays
  2. X-rays
  3. Ultraviolet Rays
  4. Visible Light
  5. Infrared Rays
  6. Microwaves
  7. Radio Waves

Increasing Frequency (Decreasing Wavelength)
Radio Waves → Microwaves → Infrared → Visible Light → Ultraviolet → X-rays → Gamma Rays

ICSE Class 10 Physics Chapter 6 Spectrum img18

c = fλ

Where:

  • c = Speed of light = 3 × 108 m/s
  • f = Frequency
  • λ = Wavelength

Frequency remains unchanged because it is determined by the source of the wave.

  • They do not require a material medium.
  • They travel in vacuum at 3 × 10⁸ m/s.
  • They are transverse waves.
  • They obey reflection and refraction.
  • Their frequency remains constant when entering another medium.
  • They are not deflected by electric or magnetic fields.
  • 1 nm = 10–9 m
  • 1 Å = 10–10 m
  • 1 nm = 10 Å
Name of the wave Wavelength Frequency
Gamma rays \(Less\ than\ 0.1\ Å\) \(\left(or,\ 0.01\ nm\right)\) \(Greater\ than\ 3\times{10}^{19}\ \ Hz\)
X-rays \(0.1\ Å\ to\ 100\ Å\)\(\left(or,\ \ 0.01\ nm\ to\ 10\ nm\right)\) \(3\times{10}^{19}\ to\ \ 3\times{10}^{16}\ Hz\)
Ultraviolet \(100\ Å\ to\ 4000 Å\)\(\left(or,\ \ 10\ nm\ to\ 400\ nm\right)\) \(3\times{10}^{16}\ to\ \ 7.5\times{10}^{14}\ Hz\)
Visible Light \(4000\ Å\ to\ 8000 Å\)\(\ \left(or,\ \ 400\ nm\ to\ 800\ nm\right)\) \(7.5\ \times{10}^{14}\ to\ \ 3.75\times{10}^{14}\ Hz\)
Infrared waves \(8000\ Å\ to\ 10^7 Å\)\(\left(or,\ \ 800\ nm\ to\ {10}^6\ nm\right)\)  \(3.75\ \times{10}^{14}\ \ to\ \ 3\times{10}^{11}\ Hz\)
Microwaves \(10^7\ Å\ to\ 10^{11} Å\)\(\left(or,\ \ {10}^6\ nm\ to\ {10}^{10}\ nm\right)\)  \(3\ \times{10}^{11}\ \ to\ \ 3\times{10}^7\ Hz\)
Radio waves \(more\ than\ 10^{11} Å\)\(\left(or,\ \ {10}^{10}\ nm\right)\)  \(below\ 3\ \times{10}^7\)
ICSE Class 10 Physics Chapter 6 Spectrum img15

❖ Source of gamma rays:

  • Radioactive substances
  • Cosmic rays

❖ Properties of gamma rays:

  • Shortest wavelength
  • Most energetic electromagnetic radiations
  • Highest frequency
  • Highest penetrating power
  • Cause fluorescence
  • Can pass through thick metal sheets
  • Harmful to living tissues

❖ Uses of gamma rays:

  • Cancer treatment (Radiotherapy)
  • Detecting cracks in metal
  • Industrial radiography

❖ Source of X-rays:

  • Produced when fast electrons strike a heavy metal target

❖ Method of detection of X-rays:

  • X-rays are detected by the fluorescence produced on a zinc sulphide screen.

❖ Properties of X-rays:

  • Highly penetrating
  • Affect photographic plates
  • Cause fluorescence
  • Pass through flesh but are absorbed by bones

❖ Uses of X-rays: 

  • Detect bone fractures
  • Dental diagnosis
  • CT Scan
  • To study the atomic arrangement in crystals and complex molecules
  • Security scanning

❖ Source of UV:

  • Sun
  • Electric arc
  • Mercury vapour lamp
  • Electric sparks

❖ Method of detection of UV:

  • UV rays are detected by their chemical effect on silver chloride, dyes, and photographic plates.
  • The ultraviolet spectrum is obtained using a quartz prism, as quartz transmits UV rays, whereas glass absorbs them.

❖ Properties of UV:

  • Pass through quartz
  • Absorbed by glass
  • Cause fluorescence
  • Affect photographic plates
  • Chemically active
  • Scattered by dust

Harmful Effects of UV:

  • Skin cancer
  • Eye damage
  • Sunburn

❖ Uses of UV:

  • Sterilization
  • Detect fake currency
  • Detect purity of gems
  • Vitamin D production

Source of Visible Light:

  • Sun
  • Electric bulb
  • Flame
  • White hot objects

Method of detection of Visible Light: 

  • Seen by human eye

❖ Uses of Visible Light: 

  • Vision
  • Photography
  • Photosynthesis
  • Optical instruments

❖ Source of Infrared waves:

  • Hot bodies
  • Heated iron
  • Fire
  • Sun

❖ Method of detection of Infrared waves:

  • Blackened bulb thermometer – Shows a rise in temperature due to the heating effect of infrared rays.
  • Thermopile – Produces a deflection when infrared rays fall on it.
  • Rock-salt prism – Used to obtain the infrared spectrum because glass absorbs infrared rays.

❖ Properties of Infrared waves: 

  • Strong heating effect
  • Less scattered by atmosphere
  • Pass through rock salt
  • Absorbed by glass
  • Detected using thermopile

❖ Harmful Effects of Infrared waves:

  • High exposure may cause skin burns.

❖ Uses of Infrared waves:

  • TV remote controls – Used to transmit signals to electronic devices.
  • Night photography – Used to take photographs in darkness.
  • Physiotherapy – Used for heat treatment to relieve pain and improve blood circulation.
  • Infrared lamps – Used in dark rooms for photographic development.
  • Fog photography – Used because infrared rays are scattered less by fog and mist.
  • Military signalling – Used for secret communication as infrared rays are invisible.

Source of Microwaves:

  • Crystal oscillators
  • Electronic devices

❖ Uses of Microwaves:

  • Satellite communication.
  • Atomic and molecular structure analysis.
  • Microwave ovens (cooking).
  • Radar communication.

    ❖ Properties of Radio waves: 

    • Longest wavelength
    • Lowest frequency
    • Lowest energy

    ❖ Uses of Radio waves:

    • Radio broadcasting
    • Television transmission
    • Radar communication
    • Wireless communication
    • Shortest wavelength: Gamma rays
    • Longest wavelength: Radio waves
    • Highest frequency: Gamma rays
    • Lowest frequency: Radio waves
    • Highest energy: Gamma rays
    • Lowest energy: Radio waves
    • Visible light range: 400 – 800 nm
    • Speed of all electromagnetic waves in vacuum: 3 × 108 m/s
    • Ultraviolet rays pass through quartz but not glass.
    • Infrared rays pass through rock salt but are absorbed by glass.
    • Microwaves are used in satellite communication and microwave ovens.
    • Radio waves are used for radio and television broadcasting.

    Definition
    Scattering of light is the process in which light is absorbed by tiny particles and then re-emitted in different directions.
    It occurs due to the presence of air molecules, dust particles, smoke, and tiny water droplets in the Earth’s atmosphere.

    • If particles are very fine, they scatter mainly the blue  colour of light (shorter wavelength).
    • Medium sized particles scatter mainly the red colour  (longer wavelength).
    • Even larger particles scatter all the colours of light that is why it appears white.

    For particles smaller than the wavelength of light,

    I 1λ4I\propto \ \frac{1}{{\lambda }^{4}}

    Where:

    • I = Intensity of scattered light
    • λ = Wavelength of light

    Conclusion

    • Shorter wavelength → More scattering
    • Longer wavelength → Less scattering

    Therefore,

    • Violet light is scattered the most.
    • Red light is scattered the least.
    • Violet has the shortest wavelength (≈400 nm).
    • Red has the longest wavelength (≈800 nm).
    • Since scattering is inversely proportional to the fourth power of wavelength, violet is scattered much more than red.

    The relation I 1λ4I\propto \ \frac{1}{{\lambda }^{4}} is valid only when the scattering particles are smaller than the wavelength of the incident light.
    If the particles are larger than the wavelength (such as water droplets in clouds), all colours are scattered almost equally.

    ICSE Class 10 Physics Chapter 6 Spectrum img17

    Reason

    • During sunrise and sunset, sunlight travels the longest distance through the atmosphere.
    • Blue and violet light are scattered away before reaching our eyes.
    • Mostly red light reaches the observer.

    ❖ Result

    • The Sun appears red or orange.

    Reason

    • At noon, the Sun is nearly overhead.
    • Sunlight travels the shortest distance through the atmosphere.
    • Very little scattering occurs.

    Result

    • The sky appears white.

    Reason

    • The upper layer of atmosphere contains very fine particles of water vapours and gases. These particles scatter short-wavelength light (blue and violet) more than red light.
    • The scattered blue light reaches our eyes from all directions.

    ❖ Result

    • The sky appears blue.

    Reason

    Without an atmosphere:

    • No air molecules are present.
    • No scattering occurs.

    Result

    • The sky appears black, as seen from the Moon or outer space.

    Reason

    Clouds contain:

    • Water droplets
    • Ice crystals
    • Dust particles

    These particles are larger than the wavelength of visible light, so they scatter all colours equally.

    Result

    • Clouds appear white.

    Reason

    • Red light has the longest wavelength.
    • It is scattered the least.
    • It can travel a greater distance through fog, smoke, rain, and dust.

    ❖ Applications

    • Traffic signals
    • Railway signals
    • Warning lights
    • Emergency vehicles

    To help you revise quickly, we are providing ICSE Class 10 Spectrum Physics Notes PDF Download with key concepts, Selina Solutions, and important questions.

    Revise the ICSE Class 10 Spectrum Physics Notes PDF daily, practice diagrams, and solve numericals regularly. With consistent preparation, you can easily score full marks in this chapter.

    ICSE Class 10 Physics
    ICSE Class 10 Chemistry
    ICSE Class 10 Mathematics
    ICSE Class 10 Biology
    ICSE Class 10 Physics Chapter 1 – Force Notes
    ICSE Class 10 Physics Chapter 2 – Work, Energy and Power Notes
    ICSE Class 10 Physics Chapter 3 – Machines Notes
    ICSE Class 10 Physics Chapter 4 – Refraction of Light at Plane Surfaces Notes
    ICSE Class 10 Physics Chapter 5 – Refraction through Lens Notes
    ICSE Class 10 Physics Chapter 6 – Spectrum Notes
    ICSE Class 10 Physics Chapter 7 – Sound Notes
    ICSE Class 10 Physics Chapter 8 – Current Electricity Notes
    ICSE Class 10 Physics Chapter 9 – Electrical Power and Household Circuits Notes
    ICSE Class 10 Physics Chapter 10 – Electro-magnetism Notes
    ICSE Class 10 Physics Chapter 11 – Calorimetry Notes
    ICSE Class 10 Physics Chapter 12 – Radioactivity  Notes
    Previous 1