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We can see objects around us because of the light reflected or emitted by them. Nature has given us eyes, which can detect a small region of electromagnetic radiation spectrum, known as visible light. Light travels with great speed in a straight line.
Optics is a branch of physics that deals with the study of nature, production, and propagation of light.
Optics is divided into categories:
- Ray optics or Geometrical optics
- Wave optics or Physical optics
Light is a wave. Although a light wave spreads as it moves away from its source, we can approximate its path as a straight line. Under this approximation, we show light as a ray and the study of light as a ray is called Ray optics or Geometrical optics. CBSE Class 12 Physics Notes for Chapter 9 Ray Optics are given in the article below for easy preparation and understanding of the concepts involved.
Read More:
| Additional Resources for Preparation | |
|---|---|
| Ray Optics and Optical Instruments | NCERT Solutions for Class 12 Physics Chapter 9 Ray Optics and Optical Instruments |
| Ray Optics MCQs | Ray Optics Important Questions |
Class 12 Physics Chapter 9 Notes - Ray Optics
Light
- The visible part of the electromagnetic spectrum is called Light.
- Light always travels in a straight line.
- The speed of light in vacuum or air is 3 x 108 m/s.
- The straight line in which the light travels is known as a Ray of Light.
- The bundle of parallel rays of light is called a Beam of Light.
Laws of Reflection
- According to the law of reflection, the angle of incidence (∠i) is equal to the angle of reflection (∠r).
- The incident ray, the reflected ray, and the normal, all lie in the same plane.
- After reflection, the velocity, wavelength, and frequency of the light remain the same.

Laws of reflection
Spherical Mirrors
- Concave Mirror: It is a part of a hollow sphere that converges the rays of light.
- Convex Mirror: It is a part of a hollow sphere that diverges the rays of light.

Spherical Mirrors
Terms Related to Spherical Mirrors
- Pole (P): Mid-point of the mirror.
- Center of Curvature (C): Center of the sphere of which the mirror is a part.
- Radius of Curvature (R): Distance between pole and center of curvature.
- Principal axis: A line passing through pole and center of curvature.
- Focus (F): The image point on the principal axis for an object at infinity.
- Focal length (f): Distance between pole and focus.
Sign Convention
- All distances are measured from the pole.
- Distances measured in the direction of the incident ray are taken as “Positive”.
- Distances measured in the direction opposite of the incident ray are taken as “Negative”.
- Distances above the principal axis are taken as “Positive”.
- Distances below the principal axis are taken as “Negative”.

Sign conventions for spherical mirrors
Image Formation by Concave Mirror
| Position of Object | Position of Image | Nature of Image | Size of Image |
|---|---|---|---|
| At infinity | At F | Real and Inverted | Very Small |
| Beyond C | Between F and C | Real and Inverted | Small |
| At C | At C | Real and Inverted | Same size |
| Between C and F | Beyond C | Real and Inverted | Large |
| At F | At Infinity | Real and Inverted | Very large |
| Between F and P | Behind the mirror | Virtual and Erect | Large |
Image Formation by Convex Mirror
| Position of Object | Position of Image | Nature of Image | Size of Image |
|---|---|---|---|
| At Infinity | At focus (behind the mirror) | Virtual and Erect | Very small |
| Between infinity and P | Between P and F (behind the mirror) | Virtual and Erect | Small |
Relation Between Focal Length and Radius of Curvature
- Formula:
f = R/2
Where
- f is the focal length
- R is the radius of curvature
- This formula is valid for both concave and convex mirrors
- For a plane mirror, f = ∞ and also R = ∞
Mirror Formula
- The relation between the focal length of a lens, object distance, and image distance is known as the mirror formula.
- Formula:
1/f = 1/u + 1/v
Where
- f is the focal length
- u is the distance of the object
- v is the distance of the image
- This formula is valid for both concave and convex mirrors.
Magnification
- It is the ratio of the height of the image to the height of the object.
- Formula:
m = h’/h
Where
- m is the magnification
- h’ is the height of the image
- h is the height of the object
- It is positive for erect images.
- It is negative for inverted images.
Refraction of Light
- The bending of the ray of light passing from one medium to another medium is called refraction.
- A ray of light bends towards the normal while traveling from a rarer to a denser medium.
- A ray of light bends away from the normal while traveling from a denser to a rarer medium.

Refraction of light
Snell’s Law
- Snell’s law states that the ratio of the sine of the angle of incidence to the sine of the angle of refraction is constant.
- This constant is known as the Refractive Index.
- Formula:
sin i / sin r = μ
Where
- i is the angle of incidence
- r is the angle of refraction
- μ is the refractive index
Total Internal Reflection (TIR)
- The phenomenon in which a ray of light traveling from a denser to a rarer medium is sent back to the same denser medium is known as Total Internal Reflection.
- Condition for TIR:
- Light travels from denser medium to rarer medium.
- The angle of incidence must be greater than the critical angle.

Total Internal Reflection
Relation Between Refractive Index and Critical Angle
- Formula:
sin C = 1/μ
Where
- C is the critical angle
- μ is the refractive index
Refraction from Spherical Surface
- Refraction Formula:
(μ2 - μ1)/R = μ2/v - μ1/u
Where
- μ1 is the refractive index of the medium from which light rays are coming
- μ2 is the refractive index of the medium in which light rays are entering
- u is the object distance
- v is the image distance
- R is the radius of curvature.
The Lens
- A lens is a transparent medium bounded by two refracting surfaces such that at least one surface is curved.
- Types of Lens:
- Concave Lens: It is also known as a Diverging lens.
- Convex Lens: It is also known as a Converging lens.

Concave and Convex Lenses
Lens Maker’s Formula
1/f = (μ - 1) [1/R1 - 1/R2]
Where
- f is the focal length of the lens
- μ is the refractive index
- R1 is the radius of curvature of the first refractive surface
- R2 is the radius of curvature of the second refractive surface

Lens Maker’s Formula
Lens Formula
- Formula:
1/f = 1/v - 1/u
Where
- f is the focal length of the lens
- u is the distance of the object from the lens
- v is the distance of the image from the lens
Image Formation by Convex Lens
| Position of Object | Position of Image | Nature of Image | Size of Image |
|---|---|---|---|
| At infinity | At F | Real and Inverted | Very Small |
| Between Infinity and 2F | Between F and 2F | Real and Inverted | Small |
| At 2F | At 2F | Real and Inverted | Same size |
| Between 2F and C | Beyond 2F | Real and Inverted | Large |
| At F | At Infinity | Real and Inverted | Very large |
| Between F and Optical center | On the same side of object | Virtual and Erect | Large |
Image Formation by Concave Lens
| Position of Object | Position of Image | Nature of Image | Size of Image |
|---|---|---|---|
| At Infinity | At focus | Virtual and Erect | Very small |
| Between infinity and Optical center | Between focus and the optical center | Virtual and Erect | Small |
Magnification of Lens
- Formula:
m = h’/h = v/u
Where
- m is the magnification
- h’ is the height of the image
- h is the height of the object
- v is the image distance
- u is the object distance
Power of a Lens
- The power of a lens is the ability of a lens to converge or diverge rays of light falling on it.
- It is the reciprocal of the focal length of the lens.
- Formula:
- P = 1/f
Where
- P is the power of the lens
- f is the focal length of the lens in meters.
- The SI unit of power of the lens is Dioptre (D).
Prism Formula
- Formula:
μ = sin [(A +\(\delta\) m)/2] / sin (A/2)
Where
- μ is the refractive index of the prism
- \(\delta\)m is the angle of minimum deviation.
- A is the prism angle.

Prism
Microscope
- It is an optical instrument used to see very small objects.
- Types:
Simple Microscope
- It is a convex lens of lesser focal length.
- It is also called a magnifying glass or reading lens.
- Magnification, when the final image is formed at least a distance of distinct vision (D) is
mD = [1 + D/f]max
- Magnification, when the final image is formed at infinity is
m∞ = [D/f]min
Compound Microscope
- It consists of two converging lenses called objective and eye lens.
- The final image formed is magnified, virtual, and inverted.
- Magnification, when the final image is formed at least a distance of distinct vision (D) is
mD = - vo/uo [1 + D/fe]
- Magnification, when the final image is formed at infinity is
m∞ = - vo/uo [D/fe]
Astronomical Telescope
- This type of telescope is used to see heavenly bodies.
- The focal length of the object is greater than the focal length of the eyepiece.
- The final image is virtual, inverted, and small.
- Magnification, when the final image is formed at least a distance of distinct vision (D) is
mD = - fo/fe [1 + fe/D]
- Magnification, when the final image is formed at infinity is
m∞ = - fo/fo
There are Some important List Of Top Physics Questions On Ray Optics And Optical Instruments Asked In CBSE CLASS XII





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