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Formula Sheet: Spherical Mirrors

Spherical Mirrors: Complete Formula Sheet

Mirror Fundamentals

Types of Spherical Mirrors

  • Concave Mirror (Converging): Reflects light inward; center of curvature and focal point are in front of the mirror (real side)
  • Convex Mirror (Diverging): Reflects light outward; center of curvature and focal point are behind the mirror (virtual side)

Key Definitions

  • Center of Curvature (C): Center of the sphere from which the mirror is a section
  • Radius of Curvature (r): Distance from mirror surface to center of curvature
  • Focal Point (F): Point where parallel rays converge (concave) or appear to diverge from (convex)
  • Focal Length (f): Distance from mirror surface to focal point
  • Principal Axis: Line passing through center of curvature and center of mirror
  • Object Distance (do or so): Distance from object to mirror surface
  • Image Distance (di or si): Distance from image to mirror surface
  • Object Height (ho): Height of the object
  • Image Height (hi): Height of the image

Primary Mirror Equations

Focal Length and Radius of Curvature

\[f = \frac{r}{2}\]
  • f = focal length
  • r = radius of curvature
  • The focal point is located halfway between the mirror surface and center of curvature
  • Units: meters (m), centimeters (cm)

Mirror Equation (Gaussian Form)

\[\frac{1}{f} = \frac{1}{d_o} + \frac{1}{d_i}\]
  • f = focal length
  • do = object distance from mirror
  • di = image distance from mirror
  • All distances measured from the mirror surface along the principal axis
  • Alternative notation: \(\frac{1}{f} = \frac{1}{s_o} + \frac{1}{s_i}\)

Alternative Forms of Mirror Equation

\[d_i = \frac{f \cdot d_o}{d_o - f}\]
\[d_o = \frac{f \cdot d_i}{d_i - f}\]
\[f = \frac{d_o \cdot d_i}{d_o + d_i}\]

Sign Conventions

Standard Sign Convention (Real is Positive)

  • Focal Length (f):
    • Positive (+) for concave mirrors (converging)
    • Negative (-) for convex mirrors (diverging)
  • Object Distance (do):
    • Positive (+) when object is in front of mirror (real object) - standard case
    • Negative (-) when object is behind mirror (virtual object) - rare
  • Image Distance (di):
    • Positive (+) when image is in front of mirror (real image)
    • Negative (-) when image is behind mirror (virtual image)
  • Heights (ho, hi):
    • Positive (+) when upright
    • Negative (-) when inverted

Magnification

Linear Magnification Formula

\[m = -\frac{d_i}{d_o} = \frac{h_i}{h_o}\]
  • m = magnification (dimensionless)
  • di = image distance
  • do = object distance
  • hi = image height
  • ho = object height
  • The negative sign accounts for image inversion

Magnification Interpretation

  • |m| > 1: Image is enlarged (magnified)
  • |m| <>: Image is reduced (diminished)
  • |m| = 1: Image is same size as object
  • m > 0: Image is upright (erect) relative to object
  • m <>: Image is inverted relative to object

Image Height Formula

\[h_i = -m \cdot h_o = -\frac{d_i}{d_o} \cdot h_o\]

Image Characteristics by Mirror Type

Concave Mirror (f > 0)

  • Object beyond C (do > r or do > 2f):
    • Real, inverted, diminished image
    • Image between F and C
    • di positive, |m| < 1,="" m=""><>
  • Object at C (do = r or do = 2f):
    • Real, inverted, same size image
    • Image at C
    • di = do = 2f, |m| = 1, m <>
  • Object between C and F (2f > do > f):
    • Real, inverted, enlarged image
    • Image beyond C
    • di positive, |m| > 1, m <>
  • Object at F (do = f):
    • No image formed (rays parallel after reflection)
    • di = ∞
  • Object between F and mirror (do <>:
    • Virtual, upright, enlarged image
    • Image behind mirror
    • di negative, |m| > 1, m > 0

Convex Mirror (f <>

  • Object anywhere in front of mirror:
    • Virtual, upright, diminished image
    • Image always behind mirror between F and mirror surface
    • di negative, |m| < 1,="" m=""> 0
  • Convex mirrors always produce virtual, upright, reduced images regardless of object position

Power of a Mirror

Mirror Power Formula

\[P = \frac{1}{f}\]
  • P = power of the mirror
  • f = focal length in meters
  • Units: diopters (D) where 1 D = 1 m-1
  • Positive power: concave (converging) mirror
  • Negative power: convex (diverging) mirror

Ray Tracing Rules

Principal Rays for Concave Mirrors

  • Ray 1 (Parallel Ray): Ray parallel to principal axis reflects through focal point F
  • Ray 2 (Focal Ray): Ray through focal point F reflects parallel to principal axis
  • Ray 3 (Central Ray): Ray through center of curvature C reflects back on itself
  • Ray 4 (Vertex Ray): Ray striking mirror vertex reflects symmetrically about principal axis

Principal Rays for Convex Mirrors

  • Ray 1 (Parallel Ray): Ray parallel to principal axis reflects as if coming from focal point F (behind mirror)
  • Ray 2 (Focal Ray): Ray directed toward focal point F (behind mirror) reflects parallel to principal axis
  • Ray 3 (Central Ray): Ray directed toward center of curvature C (behind mirror) reflects back along same path

Special Cases and Conditions

Object at Infinity

\[d_o \to \infty \implies d_i = f\]
  • Parallel rays from distant object converge at focal point
  • Used to locate focal point experimentally
  • Magnification approaches zero

Object at Focal Point

\[d_o = f \implies d_i \to \infty\]
  • Reflected rays are parallel
  • No real or virtual image formed
  • Used in searchlights and flashlights

Plane Mirror (Special Case)

\[r \to \infty \implies f \to \infty\] \[d_i = -d_o\] \[m = +1\]
  • Image is virtual, upright, same size, and same distance behind mirror
  • Can be considered limiting case of spherical mirror with infinite radius

Multiple Mirror Systems

Two Mirror System

  • Image from first mirror becomes object for second mirror
  • Total magnification: \(m_{total} = m_1 \times m_2\)
  • Apply mirror equation sequentially for each mirror
  • Distance to second mirror measured from position of first image

Spherical Aberration

Paraxial Approximation

  • Mirror equations valid only for paraxial rays: rays close to and nearly parallel to principal axis
  • Assumes small angles: sin θ ≈ tan θ ≈ θ (in radians)
  • Spherical aberration: rays far from principal axis focus at different points
  • Minimized by using mirrors with small aperture or parabolic mirrors

Important Relationships and Notes

Key Concepts for MCAT

  • Real images: formed by actual convergence of light rays; can be projected on screen; always inverted for single mirror
  • Virtual images: formed by apparent divergence of light rays; cannot be projected; always upright for single mirror
  • Concave mirrors can produce both real and virtual images depending on object position
  • Convex mirrors always produce virtual, upright, diminished images
  • For real images: light actually passes through image location
  • For virtual images: light appears to come from image location but does not actually pass through it

Problem-Solving Strategy

  1. Identify mirror type (concave or convex) and determine sign of f
  2. Identify given quantities and assign proper signs
  3. Choose appropriate equation(s)
  4. Solve algebraically before substituting numbers
  5. Check sign of result for physical meaning
  6. Verify image characteristics make sense for given configuration

Common MCAT Applications

  • Makeup/shaving mirrors: concave mirrors with object inside focal length (virtual, enlarged, upright image)
  • Security/surveillance mirrors: convex mirrors (wide field of view, virtual, reduced image)
  • Telescopes: concave mirrors to collect and focus light
  • Dental mirrors: may use either type depending on application
  • Headlight reflectors: concave mirrors with light source at focal point
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