Light: Reflection & Refraction - Rapid Revision Notes

Light

  • Rectilinear Propagation of Light: Light travels in a straight line.
  • Speed of Light: Denoted as cc, approximately 3×1083 \times 10^8 m/s.

Reflection

  • Definition: The bouncing back of light from a shiny surface (e.g., mirror or water).
  • Laws of Reflection:
    • The incident ray, the reflected ray, and the normal all lie in the same plane.
    • Angle of incidence i\angle i = Angle of reflection r\angle r

Mirrors

  • Plane Mirror:
    • Smooth, polished surface with minimal bumps.
    • Image Characteristics:
      • Always virtual and erect.
      • Image size equals object size.
      • Image distance behind the mirror equals object distance in front.
      • Laterally inverted.
  • Spherical Mirror: A mirror whose reflecting surface is part of a hollow sphere of glass.
    • Concave Mirror: Reflecting surface is curved inwards.
    • Convex Mirror: Reflecting surface is curved outwards.

Spherical Mirrors: Key Terms

  • Pole (P): The center of the reflecting surface.
  • Center of Curvature (C): The center of the sphere of which the mirror is a part.
  • Radius of Curvature (R): The radius of the sphere of which the mirror is a part.
  • Principal Axis: The straight line through the pole and center of curvature.
  • Principal Focus (F): The point where parallel rays converge (concave) or appear to diverge from (convex) after reflection.
  • Focal Length (f): Distance between the pole and the principal focus.
  • Aperture: Diameter of the reflecting surface.
  • Relationship between R and f for Concave Mirror: R=2fR = 2f
  • Relationship between R and f for Convex Mirror: R=2fR = 2f

Ray Diagrams: Rules

  • A ray parallel to the principal axis will pass through the focus after reflection.
  • A ray passing through the principal focus will become parallel to the principal axis after reflection.
  • A ray passing through the center of curvature will retrace its path after reflection.
  • A ray incident at the pole is reflected back making the same angle with the principal axis.

Concave and Convex Mirrors: Image Formation

  • Concave Mirror:
    • Object at infinity: Image at focus, highly diminished, real and inverted.
    • Object beyond C: Image between F and C, diminished, real and inverted.
    • Object at C: Image at C, same size, real and inverted.
    • Object between F and C: Image beyond C, enlarged, real and inverted.
    • Object at F: Image at infinity, highly enlarged, real and inverted.
    • Object between P and F: Image behind the mirror, enlarged, virtual and erect.
  • Convex Mirror:
    • Object at infinity: Image at focus, highly diminished, virtual and erect.
    • Object at any other position: Image between P and F, diminished, virtual and erect.

Uses of Concave and Convex Mirrors

  • Concave Mirrors:
    • Torches, searchlights, vehicle headlights.
    • Shaving mirrors.
    • Dentist's mirrors.
    • Solar furnaces.
  • Convex Mirrors:
    • Rear-view mirrors in vehicles (preferred because they provide erect, diminished images and have a wider field of view).

Important Formulas and Sign Convention

  • Object Placement: Object typically to the left of the mirror.
  • Distance Measurement: Measured from the pole of the mirror.
  • Coordinate System:
    • Positive x-axis: Right of origin.
    • Negative x-axis: Left of origin.
    • Positive y-axis: Above principal axis.
    • Negative y-axis: Below principal axis.
  • Image Height (h’):
    • Positive: Virtual images.
    • Negative: Real images.
  • Magnification (m):
    • Negative: Real images.
    • Positive: Virtual images.
  • Mirror Formula: 1f=1v+1u\frac{1}{f} = \frac{1}{v} + \frac{1}{u}, where ff is the focal length, vv is the image distance, and uu is the object distance.
  • Magnification Formula: m=hh=vum = \frac{h'}{h} = -\frac{v}{u}, where hh' is the image height and hh is the object height.

Problem-Solving Steps for Mirrors

  1. Identify Given Values: Determine what the question is asking and the given values of uu, vv, and ff. Typically, two of these will be provided.
  2. Apply Mirror Formula: Use the mirror formula to find the unknown value.
  3. Magnification Analysis:
    • m > 0: Image is upright.
    • m < 0: Image is inverted.
    • Concave Mirror:
    • ff = always -ve
      • u = always -ve
      • v = -ve (real)
      • = +ve (virtual)
  • Convex Mirror
    • f = always +ve
    • u = always −ve
    • v = always +ve (virtual)
  1. Deduce Nature of Image: From the sign of ff, identify the type of mirror. From the sign of vv, determine the nature of the image formed by a concave mirror.
  2. Apply Magnification Formula: If magnification is required, use the magnification formula. The value of mm indicates the nature of the image, and allows calculation of hh and hh'.
    • h = +ve
    • h′ = +ve (upright, virtual)
    • = −ve (inverted, real)
    • h = +ve
    • h′ = +ve (virtual and upright)
  3. Additional Insights from Magnification: The value of 'm' also provides insight into the type of mirror.

Refraction of Light

  • Definition: The change in direction of light as it passes from one transparent medium to another.
  • Laws of Refraction:
    • The incident ray, the refracted ray, and the normal to the interface of two transparent media at the point of incidence, all lie in the same plane.
    • Snell's Law of Refraction: States the relationship between the angles of incidence and refraction and the refractive indices of the two media.
  • Refractive Index: Measurement of how much a light ray bends when it passes from one medium to another.

Lenses

  • Definition: A transparent material bound by two surfaces, at least one of which is spherical.
  • Types:
    • Convex Lens: Thicker in the middle (converging lens).
    • Concave Lens: Thicker at the edges (diverging lens).

Lenses: Key Terms

  • Centre of Curvature (C, C1, C2): The center of the sphere from which the lens surface is a part.
  • Principal Axis: An imaginary straight line passing through the two centers of curvature.
  • Optical Centre (O): The central point of a lens where a ray of light passes without deviation.
  • Aperture: The effective diameter of the circular outline of a spherical lens.
  • Principal Focus (F, F1, F2): The point where rays parallel to the principal axis converge (convex) or appear to diverge from (concave).
  • Focal Length (f): The distance between the principal focus and the optical centre of a lens.

Ray Diagrams: Rules for Lenses

  • A ray of light from the object, parallel to the principal axis, after refraction through a convex lens, passes through the principal focus on the other side of the lens, or appears to diverge from the principal focus in case of a concave lens.
  • A ray of light passing through a principal focus, after refraction through a convex lens, will emerge parallel to the principal axis. A ray of light directed towards the principal focus, after refraction through a concave lens, will emerge parallel to the principal axis.
  • A ray of light passing through the optical centre of a lens will emerge without any deviation.

Convex Lens: Image Formation

  • Object at infinity: Image at F2, highly diminished, real and inverted.
  • Object beyond 2F1: Image between F2 and 2F2, diminished, real and inverted.
  • Object at 2F1: Image at 2F2, same size, real and inverted.
  • Object between F1 and 2F1: Image beyond 2F2, enlarged, real and inverted.
  • Object at F1: Image at infinity, highly enlarged, real and inverted.
  • Object between O and F1: Image on the same side as the object, enlarged, virtual and erect.

Concave Lens Image Formation

  • Object at infinity: Image at F1, highly diminished, virtual and erect.
  • Object at any other position: Image between F1 and O, diminished, virtual and erect.

Uses of Convex & Concave Lenses

  • Convex Lenses:
    • Overhead projectors
    • Cameras
    • Focusing sunlight
    • Simple telescopes
    • Projectors
    • Microscopes
    • Magnifying glasses
  • Concave Lenses:
    • Spyholes in doors
    • Eyeglasses
    • Some telescopes

Important Formulas for Lenses

  • All measurements are taken from the optical centre of the lens.
  • Focal length of a convex lens = positive.
  • Focal length of a concave lens = negative.
  • Lens Formula: 1f=1v1u\frac{1}{f} = \frac{1}{v} - \frac{1}{u}
  • Magnification: m=hh=vum = \frac{h'}{h} = \frac{v}{u}
  • Power of Lens: P=1fP = \frac{1}{f}, where ff is in meters. SI unit is Dioptre (D).
    • 1 Dioptre is the power of a lens whose focal length is 1 meter.
    • 1D=1m11D = 1m^{-1}
    • Power of a convex lens = positive.
    • Power of a concave lens = negative.

Problem-Solving Steps for Lenses

  1. Identify Given Values: Determine what the question is asking and the given values of uu, vv, and ff. Typically, two of these will be provided.

  2. Apply Lens Formula: Use the lens formula to find the unknown value.

    • (m > 0): image is upright.
    • (m < 0): The image is inverted
  3. Deduce Nature of Image: From the sign of ff, identify the type of lens. From the sign of vv, determine the nature of the image formed by a convex lens.

    • Concave Convex
      • f = always +ve
      • u = always −ve
      • v = +ve (real image)
      • = −ve(virtual image)
      • f = always −ve
      • u = always −ve
      • v = always −ve
  4. Apply Magnification Formula: If magnification is required, use the magnification formula. The value of mm indicates the nature of the image, and allows calculation of hh and hh'.

  5. Power of a lens asked then formula and sign conventions used:

    • P (convex lens) = positive
    • P (concave lens) = negative.
    • f = always +ve
    • f = always −ve

Additional Types of Questions

  • Screen-Based Questions: Problems involving slide projectors. The position of the screen needed for the slide projector to remain in focus.
  • Refractive Index and Speed of Light Questions: Refractive indexes of a particular medium and the speed of light in the medium; determine the speed of light in another medium.
  • Formula Used: n=cvn = \frac{c}{v}, where nn is the refractive index, cc is the speed of light in vacuum, and vv is the speed of light in the medium.