1. Basic Terminology of Ray Optics

  • Ray: The path along which light energy travels; represented as a straight line with an arrow.
  • Beam: A collection of rays. A parallel beam comes from a distant source; a convergent beam meets at a point; a divergent beam spreads out from a point.
  • Wavefront: The locus of all points in a wave that are in the same phase. Rays are always perpendicular to wavefronts.
  • Normal: A line perpendicular to the surface at the point of incidence.
  • Angle of Incidence (i): Angle between the incident ray and the normal at the point of incidence.
  • Angle of Reflection (r): Angle between the reflected ray and the normal at the point of incidence.

2. Laws of Reflection

The two laws of reflection hold for all types of reflecting surfaces — plane, concave, and convex:

  • First Law: The incident ray, the reflected ray, and the normal to the surface at the point of incidence all lie in the same plane.
  • Second Law: The angle of incidence equals the angle of reflection: i=r.

These laws hold for all wavelengths of light and are independent of the medium in which the light travels.

Reflection from a Plane Mirror — Key Results

Property Detail
Image type Virtual and erect
Image size Same as object (magnification m=+1)
Image distance Equal to object distance (image is as far behind mirror as object is in front)
Laterally inverted? Yes — left and right are interchanged
Mirror rotated by θ Reflected ray rotates by 2θ
Number of images (two mirrors at angle θ) n=360°θ1 (if 360°θ is even)
Minimum mirror length to see full image Half the height of the person — independent of distance from mirror

3. Spherical Mirrors — Terminology

A spherical mirror is a mirror whose reflecting surface is a part of a hollow sphere. Two types:

  • Concave mirror: Reflecting surface is on the inner (cave) side of the sphere — converging mirror.
  • Convex mirror: Reflecting surface is on the outer side of the sphere — diverging mirror.

Important Terms

Term Symbol Definition
Centre of Curvature C Centre of the sphere of which the mirror is a part
Radius of Curvature R Radius of the sphere; distance from pole to C
Pole P Midpoint of the reflecting surface of the mirror
Principal Axis Line joining pole P and centre of curvature C
Principal Focus F Point where parallel rays (close to principal axis) converge after reflection (concave) or appear to diverge from (convex)
Focal Length f Distance from pole to focus: f=R/2
Aperture Diameter of the circular boundary of the mirror

Key relation: f=R2 — focal length is half the radius of curvature. This holds for both concave and convex mirrors.

4. Sign Convention

The New Cartesian Sign Convention is essential for applying the mirror formula correctly. All distances are measured from the pole P:

  • Distances measured in the direction of incident light (usually left to right) are positive.
  • Distances measured opposite to the direction of incident light are negative.
  • Heights measured above the principal axis are positive.
  • Heights measured below the principal axis are negative.
Quantity Concave Mirror Convex Mirror
Object distance u Always ve (object in front) Always ve (object in front)
Focal length f ve (focus in front of mirror) +ve (focus behind mirror)
Radius of curvature R ve +ve
Image distance v (real image) ve (in front of mirror) Never forms real image
Image distance v (virtual image) +ve (behind mirror) +ve (behind mirror)

5. Mirror Formula and Magnification

Mirror Formula

The relationship between object distance u, image distance v, and focal length f:

1v+1u=1f=2R

This formula is valid for all positions of the object and for both concave and convex mirrors, provided the sign convention is followed consistently.

Derivation of Mirror Formula (for Concave Mirror)

Consider a concave mirror with pole P, focus F, and centre C. For an object at point O beyond C, an image forms at I. Using similar triangles from the geometry of the ray diagram:

From similar triangles ABF and MPF:
ABMP=BFFP

Since MP=AB (where B is the image) and FP=f, BF=vf (using magnitudes):
ABAB=BFFP=vff   ... (1)

From similar triangles formed by object and image (using principal axis geometry):
ABAB=OBOB=uv   ... (2)

From (1) and (2): uv=vff
uf=v(vf)=v2vf
Dividing both sides by uvf:
1v+1u=1f   ✓

Linear Magnification

The ratio of the height of the image (h) to the height of the object (h):

m=hh=vu

Value of m Image Characteristics
m>0 (positive) Virtual and erect image
m<0 (negative) Real and inverted image
|m|>1 Image is enlarged (magnified)
|m|<1 Image is diminished
|m|=1 Image is same size as object

6. Ray Diagrams — Rules for Image Construction

Any two of the following standard rays are used to locate the image formed by a spherical mirror:

  • Ray 1 — Parallel to principal axis: After reflection, passes through F (concave) or appears to come from F (convex).
  • Ray 2 — Through/towards F: After reflection, emerges parallel to the principal axis.
  • Ray 3 — Through/towards C: Reflects back along the same path (normal incidence — angle of incidence = 0°).
  • Ray 4 — Incident at pole: Reflects making the same angle with the principal axis on the other side (like a plane mirror at that point).

7. Image Formation by Concave Mirror — All Cases

Object Position Image Position Nature Size Application
At infinity At F Real, inverted Point-sized Solar furnace, reflecting telescope
Beyond C (object >2f) Between F and C Real, inverted Diminished Rear-view mirror (no, that's convex)
At C (u=2f) At C Real, inverted Same size (m=1) Used in optics experiments
Between F and C (f<u<2f) Beyond C Real, inverted Enlarged Projectors
At F (u=f) At infinity Real, inverted Highly enlarged Search lights, headlights, torches
Between P and F (u<f) Behind mirror Virtual, erect Enlarged Shaving/makeup mirrors, dentist mirrors

8. Image Formation by Convex Mirror

A convex mirror always forms a virtual, erect, and diminished image — regardless of object position. The image is always between P and F (behind the mirror).

Object Position Image Position Nature Size
At infinity At F (behind mirror) Virtual, erect Point-sized
Anywhere in front of mirror Between P and F (behind mirror) Virtual, erect Diminished

Why Convex Mirrors are Used as Rear-View Mirrors

  • Always gives an erect image — easy to interpret while driving.
  • Diminished image gives a wider field of view — more area visible in a smaller mirror.
  • Image is always virtual — unambiguous and does not confuse the driver.

9. Power of a Mirror

The power of a mirror is defined as the reciprocal of its focal length (in metres):

P=1f    (unit: Dioptre, D)

  • Concave mirror: f is negative → P is negative.
  • Convex mirror: f is positive → P is positive.
  • Note: The sign convention for mirror power is opposite to that of lenses. For mirrors, the power is 1/f in some conventions — always clarify with the sign convention used.

10. Important Derived Results

Object at C of Concave Mirror

When u=2f (object at centre of curvature):

1v+12f=1f       v=2f

Image forms at C itself — same size, real, inverted. m=vu=2f2f=1. ✓

Mirror Moved Towards/Away from Object

Differentiating the mirror formula with respect to time (for a moving mirror or moving object):

1v2dvdt1u2dudt=0       vimage=v2u2vobject=m2vobject

The velocity of the image = m2 times the velocity of the object. This result is used in JEE problems on moving objects/mirrors.

Number of Images in Two Inclined Mirrors

Angle θ between mirrors Number of images
60° 5
72° 4
90° 3
120° 2
180° (parallel mirrors)
0° (facing each other)