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Mirror Formula and Magnification

Jul 25, 2025

Overview

This lecture covers the mirror formula, magnification, and the sign convention for spherical mirrors, with examples for both concave and convex mirrors.

Spherical Mirrors and Their Types

  • Spherical mirrors are of two types: concave (converging) and convex (diverging).
  • Concave mirrors reflect light inward; convex mirrors reflect light outward.

Sign Convention for Spherical Mirrors

  • All distances are measured from the mirror's pole (vertex).
  • Distances measured in the direction of incident light are positive.
  • Distances measured opposite to the direction of incident light are negative.
  • For mirrors, object distances (u) are usually negative (object left of mirror).
  • For concave mirrors, focal length (f) is negative; for convex mirrors, f is positive.
  • Heights above the principal axis are positive; below are negative.

Mirror Formula

  • The mirror formula relates object distance (u), image distance (v), and focal length (f):
    1/f = 1/v + 1/u
  • Used for both concave and convex mirrors by applying proper signs.

Magnification Formula

  • Magnification (m) is the ratio of image height (h') to object height (h):
    m = h'/h = -v/u
  • Negative magnification means the image is inverted; positive magnification means it is erect.

Example Problem (Application)

  • Given: Object height = 1 cm, object distance u = -9 cm, concave mirror f = -6 cm.
  • Apply mirror formula: 1/f = 1/v + 1/u to find image distance v.
  • Calculate magnification using m = -v/u, then find image height h' = m Γ— h.
  • Determine if image is real or virtual, magnified or diminished, inverted or erect based on sign and values.

Key Terms & Definitions

  • Concave mirror β€” spherical mirror that converges light, reflective surface curved inward.
  • Convex mirror β€” spherical mirror that diverges light, reflective surface curved outward.
  • Pole (P) β€” central point on the mirror’s surface.
  • Principal axis β€” imaginary line passing through pole and center of curvature.
  • Focal length (f) β€” distance from pole to focus.
  • Object distance (u) β€” distance from object to pole.
  • Image distance (v) β€” distance from image to pole.
  • Magnification (m) β€” ratio of image height to object height.

Action Items / Next Steps

  • Practice numericals using mirror and magnification formulas.
  • Review sign conventions for different mirror setups.
  • Complete textbook exercises on spherical mirrors.