OpticsTopic #35 of 35

Refraction and Lenses

Snell's law, total internal reflection, lenses, and the lens equation.

Overview

Refraction is the bending of light as it passes from one medium to another. Lenses use refraction to form images and are essential components in cameras, eyeglasses, microscopes, and telescopes.

Index of Refraction

n=cvn = \frac{c}{v}

Where:

  • cc = speed of light in vacuum (3×1083 \times 10^8 m/s)
  • vv = speed of light in medium
  • n1n \geq 1 (n=1n = 1 for vacuum)

Common Values

Materialnn
Vacuum1.00
Air1.0003
Water1.33
Glass1.5
Diamond2.42

Snell's Law

n1sin(θ1)=n2sin(θ2)n_1 \sin(\theta_1) = n_2 \sin(\theta_2)

Where:

  • n1,n2n_1, n_2 = indices of refraction
  • θ1\theta_1 = angle of incidence
  • θ2\theta_2 = angle of refraction

Bending Direction

  • From less dense to more dense (n1<n2n_1 < n_2): bends toward normal
  • From more dense to less dense (n1>n2n_1 > n_2): bends away from normal

Total Internal Reflection

Occurs when light goes from denser to less dense medium at angles greater than critical angle.

Critical Angle

sin(θc)=n2n1(for n1>n2)\sin(\theta_c) = \frac{n_2}{n_1} \quad \text{(for } n_1 > n_2\text{)}

Applications: fiber optics, prisms, diamond brilliance

Lenses

Converging (Convex) Lens

  • Thicker in the middle
  • Positive focal length
  • Converges parallel rays to focal point

Diverging (Concave) Lens

  • Thinner in the middle
  • Negative focal length
  • Diverges parallel rays (appear to come from focal point)

Lensmaker's Equation

1f=(n1)(1R11R2)\frac{1}{f} = (n-1)\left(\frac{1}{R_1} - \frac{1}{R_2}\right)

Where R1,R2R_1, R_2 are radii of curvature of the surfaces.

Thin Lens Equation

1do+1di=1f\frac{1}{d_o} + \frac{1}{d_i} = \frac{1}{f}

Same as mirror equation!

Magnification

m=hiho=didom = \frac{h_i}{h_o} = -\frac{d_i}{d_o}

Same conventions as mirrors:

  • m>0m > 0: upright
  • m<0m < 0: inverted
  • m>1\lvert m \rvert > 1: enlarged

Converging Lens - Image Formation

Object PositionImage PositionImage Type
Beyond 2FBetween F and 2FReal, inverted, diminished
At 2FAt 2FReal, inverted, same size
Between F and 2FBeyond 2FReal, inverted, enlarged
At FAt infinity
Inside FSame sideVirtual, upright, enlarged

Diverging Lens - Image Formation

  • Always virtual
  • Always upright
  • Always diminished
  • Between lens and F (same side as object)

Power of a Lens

P=1fP = \frac{1}{f}

Unit: Diopter (D) = m⁻¹

  • Positive PP: converging lens
  • Negative PP: diverging lens

Lenses in Combination

Close Together

Ptotal=P1+P2+P3+P_{\text{total}} = P_1 + P_2 + P_3 + \cdots 1feq=1f1+1f2+\frac{1}{f_{\text{eq}}} = \frac{1}{f_1} + \frac{1}{f_2} + \cdots

Separated by Distance dd

Use image from first lens as object for second.

Ray Diagrams for Lenses

Converging Lens Rules

  1. Parallel ray → refracts through F (far side)
  2. Ray through F (near side) → refracts parallel
  3. Ray through center → passes straight through

Diverging Lens Rules

  1. Parallel ray → refracts as if from F (near side)
  2. Ray toward F (far side) → refracts parallel
  3. Ray through center → passes straight through

Examples

Example 1: Snell's Law

Light goes from air to glass (n=1.5n = 1.5) at 45°.

sin(θ2)=n1sin(θ1)n2=1×sin(45°)1.5=0.7071.5=0.471\sin(\theta_2) = \frac{n_1 \sin(\theta_1)}{n_2} = \frac{1 \times \sin(45°)}{1.5} = \frac{0.707}{1.5} = 0.471 θ2=28.1°\theta_2 = 28.1°

Example 2: Critical Angle

Find critical angle for glass-air interface (nglass=1.5n_{\text{glass}} = 1.5).

sin(θc)=nairnglass=11.5=0.667\sin(\theta_c) = \frac{n_{\text{air}}}{n_{\text{glass}}} = \frac{1}{1.5} = 0.667 θc=41.8°\theta_c = 41.8°

Example 3: Converging Lens - Real Image

A lens (f=20f = 20 cm) has an object at do=60d_o = 60 cm.

1di=1f1do=120160=360160=260\frac{1}{d_i} = \frac{1}{f} - \frac{1}{d_o} = \frac{1}{20} - \frac{1}{60} = \frac{3}{60} - \frac{1}{60} = \frac{2}{60} di=30 cm (real, opposite side)d_i = 30 \text{ cm (real, opposite side)} m=3060=0.5 (inverted, diminished)m = -\frac{30}{60} = -0.5 \text{ (inverted, diminished)}

Example 4: Converging Lens - Virtual Image

Same lens, object at do=10d_o = 10 cm (inside F).

1di=120110=120220=120\frac{1}{d_i} = \frac{1}{20} - \frac{1}{10} = \frac{1}{20} - \frac{2}{20} = -\frac{1}{20} di=20 cm (virtual, same side)d_i = -20 \text{ cm (virtual, same side)} m=2010=2 (upright, magnified)m = -\frac{-20}{10} = 2 \text{ (upright, magnified)}

Example 5: Diverging Lens

A lens (f=15f = -15 cm) has an object at do=30d_o = 30 cm.

1di=115130=230130=330\frac{1}{d_i} = \frac{1}{-15} - \frac{1}{30} = -\frac{2}{30} - \frac{1}{30} = -\frac{3}{30} di=10 cm (virtual, same side)d_i = -10 \text{ cm (virtual, same side)} m=1030=0.33 (upright, diminished)m = -\frac{-10}{30} = 0.33 \text{ (upright, diminished)}

Example 6: Lens Combination

Two lenses (f1=10f_1 = 10 cm, f2=20f_2 = 20 cm) are in contact.

P=10.1+10.2=10+5=15 DP = \frac{1}{0.1} + \frac{1}{0.2} = 10 + 5 = 15 \text{ D} f=115 m=6.67 cmf = \frac{1}{15} \text{ m} = 6.67 \text{ cm}

Example 7: Vision Correction

A nearsighted person can't see beyond 100 cm. What lens corrects to infinity?

Object at infinity should form image at 100 cm (far point):

1+11=1f\frac{1}{\infty} + \frac{1}{-1} = \frac{1}{f} f=1 m=100 cmf = -1 \text{ m} = -100 \text{ cm} P=1 D (diverging lens)P = -1 \text{ D (diverging lens)}

Sign Convention Summary

QuantityPositiveNegative
dod_oObject in frontObject behind
did_iImage behind (real)Image in front (virtual)
ffConverging lensDiverging lens
RRCenter on opposite sideCenter on same side