Understanding Ray Optics and Optical Instruments

Ray Optics and Optical Instruments 2021 ( Physics Ray Optics and Optical Instruments )

Jaya Sharma
Updated on Aug 11, 2025 13:22 IST

By Jaya Sharma, Assistant Manager - Content

Ray optics, or geometrical optics, is one of the main branches of optics that deals with the propagation of light as rays. When it is assumed that light travels in a straight line, predicting the behaviour of light becomes easier. 

ray optics

Optical instruments are designed on the principles of ray optics and are used in many applications from day-to-day life to advanced research. Such instruments as microscopes, cameras, and telescopes are optical instruments that have revolutionised the world. Once you have completed the Ray optics and optical instruments class 12 notes, you can start practising the ray optics class 12 NCERT solutions to perform well in the entrance exams.

Table of content
  • What is Reflection?
  • What is Refraction?
  • Total Internal Reflection
  • What is Raman Scattering?
  • What are Spherical Mirrors?
  • Important Formulae in Ray Optics and Optical Instruments
  • FAQs on Derivation of lens formula
View More
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What is Reflection?

Reflection describes how light waves bounce off a surface. When a wave comes across a boundary between two different media, a part of the wave energy is reflected back into original medium. The rest of the light wave is either absorbed or transmitted through boundary.

The reflection of light is governed by two laws: first law of reflection and second law of reflection. CBSE board students must be well aware of these laws since many questions based on them, are asked directly in the paper.

  1. The first law of reflection states that the incident ray, the reflected ray and the normal to the surface at the point of incidence all lie in the same plane.
  2. Second law of reflection states that angle of incidence is equal to angle of reflection. 

        θ        i     =         θ        r   

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What is Refraction?

Refraction is a phenomenon that occurs when light changes its direction on passing from one medium to another. Here, the refractive index of both media are different. This phenomenon causes a number of optical effects and it is crucial in the functioning of prisms, lenses as well as other optical instruments. 

Refraction occurs because the speed of light changes in different media. When light is passing from one medium to another, its speed changes, which causes the light to bend. This bending is known as refraction.

1. Refraction at spherical surfaces and by lenses 

Refraction at spherical surfaces and by lenses is a concept in optics that explains the way light rays will change direction as they pass through curved surfaces and lenses. This phenomenon explains how lenses form images and their use in different optical instruments like telescopes, cameras and eyeglasses. 

Whenever light passes from one medium to another through spherical surface, refraction occurs as per the curvature of surface and refractive index of two media. For a spherical surface, the relation between object distance (u), image distance (v), radius of curvature (R) and refractive indices of 2 media is given by:  

               n 2        v           -             n 1        u           =                      n 2          -          n 1               R        

2. Refraction Through a Prism

IIT JAM exam will ask questions based on the phenomenon of refraction through the prism instead of asking questions directly on refraction.

refraction through a prism

A prism is a transparent optical element that has flat, polished surfaces that are angled in a way to refract light. Refraction through a prism demonstrates how light changes its direction when it passes through different media. Refraction through a prism takes place in the following way:

  • Light enters the prism as an incident ray and it travels from one medium into another medium.
  • As incident ray hits the first surface of prism, it will undergo refraction. The phenomenon of refraction is the bending of light as it passes from one medium to another with a different refractive index. This index measures how much a material can bend the light.
  • The angle at which light bends is dependent on angle of incidence and refractive indices of two media.

               n        1                sin      (             θ        1           )      =             n        2                sin      (             θ        2           )   

Here:

  •         n      1    and          n      2    are refractive indices of first and second media, respectively
  •         θ        1    and          θ        2    are angles of incidence and refraction, respectively.
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Total Internal Reflection

Total internal reflection occurs when a light travels from a medium with a higher refractive index to a medium with lower refractive index. In this situation, the light strikes the boundary at an angle greater than critical angle. This results in light being reflected back into original medium without any refraction. 

In mathematical terms (important for NEET exam students), total internal reflection will occur if the angle of incidence is greater than the critical angle. This critical angle is the angle of incidence at which the angle of refraction is         90      °   

Critical angle will be calculated with the following formula:

               θ          c           =             sin                          1                                                  n            2                              n            1                        

Physics Ray Optics and Optical Instruments

Try these practice questions

Q1:

At a certain place the angle of dip is 30° and the horizontal component of earth’s magnetic field is 0.5 G. The earth’s total magnetic field (in G), at the certain place, is:

Q2:

Light travels in two media M1 and M2 with speeds 1.5 × 108 ms1 and 2.0 × 108 ms1 respectively. The critical angle between them is:

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What is Raman Scattering?

Raman scattering or Raman effect is a phenomenon in spectroscopy that involves inelastic scattering of photons by molecules that are excited to higher energy levels. When light interacts with molecules, most of the scattered light and incident light have same wavelength. This is known as Rayleigh scattering. Many questions based on this type of scattering are asked in the IISER exam and therefore, students must be well aware of the terminology.

However, a small fraction of light gets scattered at different wavelengths because of the interactions with molecular vibrations. This inelastic scattering is known as Raman scattering. This is a relatively weak effect that requires sensitive detectors and strong light sources like lasers. 

What are Spherical Mirrors?

Spherical mirrors are optical devices having curved surfaces that are part of a sphere. These mirrors include concave and convex mirrors.

  1. Concave mirrors have surface that is curved inwards. Its reflective surface is on the side that faces the center of sphere. The curvature of this mirror causes the incident light rays to converge at a focal point. Based on the position of object which is relative to mirror's focal point and center of curvature, these mirrors can produce both real and virtual images. JEE Main exam students must also know about the diagrams of the images formed by this type of mirror.
  2. Convex mirrors have a surface that is curved outward, just like the outer surface of a sphere. These mirrors always form virtual images that are upright and diminished. The images appear as if they are located behind the mirror. Convex mirror images are smaller than the object in real life.
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Important Formulae in Ray Optics and Optical Instruments

Let us take a look at the formulae in ray optics and optical instruments that are important for CUET exam and GATE entrance exam.

1. Lens Formula

This formula relates object distance (u), image distance (v) and focal length (f) of a lens. Lens formula determines the position and nature of image formed by lens.  It is given by:

               1        f           =             1        v           -             1        u         Here:

  • f is the focal length of the lens
  • v is the image distance
  • u is the object distance

2. Beer-Lambert Law

This law relates the absorption of light with the properties of material through which light is travelling. It is a law used in spectroscopy to analyze concetration of substances in solution. Beer-Lambert law is expressed as:

A = ϵ⋅c⋅l

  • A is absorbance that measures amount of light absorbed by sample
  • ϵ is molar absorptivity or extinction coefficient, the constant that depends on nature of substance and wavelength of light
  • c is the concentration of absorbing species in sample
  • l is the path length or distance that light travels through sample

3. Lambert's Cosine Law

This law describes the relationship between intensity of light that falls on a surface and angle at which it strikes. This law states that illuminance on surface is proportional to cosine of angle of incidence. Lambert's Cosine law explains why surfaces appear brighter when a light strikes them in a perpendicular direction. It also explains why surfaces appear darker when light strikes at oblique angle.

        I      =             I        0                cos      (      θ      )    Here: 

  •         I      0    is the light source intensity which is perpendicular to the surface
  • I is the illuminance on surface which is the amount of light that falls on a unit area of surface
  • θ is the angle of incidence between direction of light and surface
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FAQs on Derivation of lens formula

Let us take a look at some of the important questions based on ray optics and optical instruments class 12 notes from the exam point of view:

Q&A Icon
Commonly asked questions
Q:  

What happens when light is refracted through a prism?

A: 

The following happens when light refracts from a prism:

  • When a white light passes through prism, it is separated into its constituent colours. This separation occurs because different colours of light are refracted in different amounts. This is known as dispersion.
  • Prism's refractive index varies with the wavelength of light. This causes shorter wavelengths to bend more than longer wavelengths. Due to the variation in bending, spread of colours is visible in rainbow. 
  • After being dispersed within the prism, light rays reach second surface of the prism. Here, light rays again undergo refraction as they exit the prism and re-enter air.
  • Light rays bend from their normal path as they pass from glass to air. This second refraction results in the separation of colours.
  • The light rays emerge out of the prism as a spectrum of colour. The angle between incident ray and the emergent ray is known as the angle of deviation. 
Q:  

Explain the working principle of a Telescope.

A: 

A telescope functions on the working principle of gathering light form distant source and then, forming image which can be magnified for observation. Based on their design, there are two types of telescopes including refracting telescopes and reflecting telescopes. A refracting telescope has a front lens called as objective lens. This front lens is a convex lens that collects light from distant objects and then bend it to the focal point. In a reflecting telescope, a concave mirror is the primary mirror that collects light and then, reflects it to a focal point.

Q:  

What is the function of a Camera Lens?

A: 

A camera lens focuses the light onto a light-sensitive surface like film or a digital sensor for capturing an image. The camera lens gathers as much light as possible for forming a clear and bright image. This lens focuses the collected light on a specific point like camera's film or its digital sensor. The focus is achieved due to the curvature of lens and the arrangement of its optical elements. This lens refracts light rays so that they converge at focal plane where film/sensor is located.

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