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Class 10: Light: Reflection and Refraction, complete article (In Brief Edition)

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যেকোনো ভাষায় এটি অনুবাদ করতে, ডানদিকে তিনটি লাইনে ক্লিক করুন এবং তারপর অনুবাদ করুন!

इसे किसी भी भाषा में अनुवाद करने के लिए दाहिनी ओर तीन पंक्तियों पर क्लिक करें और फिर अनुवाद करें!

これを任意の言語に翻訳するには、右側の 3 本線をクリックして翻訳してください.

Pour traduire cela dans n'importe quelle langue, cliquez sur les trois lignes à droite puis traduisez !

Light: Reflection and Refraction

Light is a form of energy that creates the sensation of vision. It travels in straight lines (Rectilinear Propagation). But what happens when it hits a wall? Or when it enters a glass of water? This is where Physics gets interesting.

For Class 10 students, this chapter is the foundation of Optics. We will break this down into three major conceptual pillars: Reflection, Refraction, and Lenses.


Part 1: Reflection of Light

Reflection is the bouncing back of light rays when they strike a polished surface. The most common example is a mirror.

1. Laws of Reflection

Whether the surface is flat (plane mirror) or curved (spherical mirror), these two laws are universal:

  • First Law: The angle of incidence (∠i) is always equal to the angle of reflection (∠r).
  • Second Law: The incident ray, the reflected ray, and the normal (the perpendicular line at the point of incidence) all lie in the same plane.
📷 Click here to View Diagram: Laws of Reflection

(Opens in a new tab)

2. Real vs. Virtual Images

Before we look at mirrors, you must understand the two types of images formed:

Real Image Virtual Image
Formed when light rays actually meet. Formed when light rays appear to meet (when extended backwards).
Can be obtained on a screen (like a cinema projector). Cannot be obtained on a screen (like your face in a mirror).
Always Inverted (Upside down). Always Erect (Upright).

3. Spherical Mirrors

Spherical mirrors are parts of a hollow sphere. There are two types:

  • Concave Mirror (Converging): The reflecting surface is curved inwards. It collects light to a single point called the Focus.
    Application: Used by dentists to see large images of teeth, shaving mirrors, and solar furnaces.
  • Convex Mirror (Diverging): The reflecting surface is curved outwards. It spreads light out.
    Application: Rear-view mirrors in cars because they give a much wider field of view than plane mirrors.
📷 Click here to View Diagram: Concave Mirror Ray Tracing

4. The Mirror Formula

To find the position of the image mathematically, we use the mirror formula:

1/v + 1/u = 1/f

Magnification (m): This tells us how much larger or smaller the image is compared to the object.

m = h'/h = -v/u
Sign Convention Tip: Imagine the pole of the mirror is the origin (0,0) of a graph.
  • Light always comes from the Left.
  • u (Object distance): Always Negative (-).
  • f (Concave): Negative (-).
  • f (Convex): Positive (+).

Part 2: Refraction of Light

Refraction is the bending of light when it travels from one transparent medium to another (e.g., Air to Glass). This happens because light travels at different speeds in different media.

1. The Rules of Bending

  • Rare to Dense (Air to Water): Speed slows down → Light bends TOWARDS the normal.
  • Dense to Rare (Glass to Air): Speed speeds up → Light bends AWAY FROM the normal.

2. Refraction through a Rectangular Glass Slab

When light passes through a glass slab, it refracts twice (Air→Glass, then Glass→Air). The final emergent ray is parallel to the original incident ray, but it is shifted sideways. This shift is called Lateral Displacement.

📷 Click here to View Diagram: Refraction through Glass Slab

3. Refractive Index (n)

The refractive index is a measure of how much a medium slows down light. It is derived from Snell's Law.

sin i / sin r = Constant (n)

Absolute Refractive Index:

nm = Speed of light in Vacuum (c) / Speed of light in Medium (v)

Example: The refractive index of diamond is 2.42. This means light travels 2.42 times slower in diamond than in vacuum!


Part 3: Spherical Lenses

Mirrors reflect light; Lenses refract light. A lens is a piece of transparent material bound by at least one curved surface.

1. Convex vs. Concave Lens

  • Convex Lens (Converging): Thicker at the center, thinner at the edges. It brings parallel rays to a Focus. It is used in cameras and to correct Hypermetropia (farsightedness).
  • Concave Lens (Diverging): Thinner at the center, thicker at the edges. It spreads light out. It is used in peepholes and to correct Myopia (nearsightedness).
📷 Click here to View Diagram: Convex vs Concave Lens Action

2. The Lens Formula

Be careful! The sign changes here compared to the mirror formula.

1/v - 1/u = 1/f

Magnification (m):

m = h'/h = v/u

3. Power of a Lens

The power of a lens is its ability to converge or diverge light rays. It is the reciprocal of the focal length.

P = 1 / f (in meters)

The SI unit of Power is Dioptre (D).

  • Power of Convex Lens = Positive (+)
  • Power of Concave Lens = Negative (-)

Summary Cheat Sheet for Numericals

Use this table to quickly solve any board exam problem:

Quantity Concave Mirror Convex Mirror Convex Lens Concave Lens
u (Object) Always (-) Always (-) Always (-) Always (-)
f (Focal Length) (-) (+) (+) (-)
v (Real Image) (-) N/A (+) N/A
v (Virtual Image) (+) (Behind mirror) (+) (Behind mirror) (-) (Same side) (-) (Same side)

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