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Library / Foundations: Physics / FPH-31

Foundations: Physics

Double-slit fringe spacing

Spacing of interference fringes on a screen.

Ref
FPH-31
Rev
v1
Field
Foundations: Physics
Result
w [mm]

Fringe spacing w on a distant screen depends on wavelength λ, screen distance D and slit separation s. Use for small angles and coherent light.

Light passing through two slits makes bright and dark bands; the bands are further apart for longer wavelengths and closer slits.

Calculator

Solve for
mm
nm
380750
m
0.510
mm
0.12
  • Fringe spacing in metres0.0024 m
  • Fringes within 10 mm4.167

What drives the result

Each variable is moved across its typical range while the others stay at the values above. The longest bar is the key driver.

Fringe spacing (mm) current value 2.4 mm
DScreen distanceKey driver
0.612
sSlit separation
0.612
λWavelength
1.523
  • Measure the fringe spacing and you can find the wavelength of the light.
  • Red light gives wider fringes than blue.
Chart data as tables

Ranked variables

VariableTypical rangeLowest resultHighest resultSwing (mm)Local stepChange in result
D Screen distance0.5 to 10 m0.61211.4+10%+10 %
s Slit separation0.1 to 2 mm0.61211.4+10%−9.09 %
λ Wavelength380 to 750 nm1.5231.48+10%+10 %

Sweep of Screen distance

Screen distance (m)Fringe spacing (mm)
0.50.6
0.72710.8725
1.0571.269
1.5381.845
2.2362.683
3.2523.902
4.7295.674
6.8778.252
1012

Sweep one variable

Fringe spacing (mm)Hover, touch, or use the arrow keys on the chart
024681012 0.512510 Screen distance (m), log scale now 2.4

Variables and how each one contributes

w

Fringe spacing

Result · mm

What the equation gives you. Everything else feeds it.

λ

Wavelength

nm · typical 380 to 750

Wavelength of the light. Directly proportional.

D

Screen distance

m · typical 0.5 to 10

Distance from slits to screen. Directly proportional.

s

Slit separation

mm · typical 0.1 to 2

Distance between the slits. Inversely proportional.

Worked example with the values above

  1. Convert units: λ = 6×10−7 m, s = 5×10−4 m.
  2. w = λD/s = 6×10−7 × 2 / 5×10−4 = 0.0024 m.
  3. w = 2.4 mm.

Assumptions and limits

  • Small angles and D much larger than s.
  • Coherent, monochromatic light.

Common mistakes

  • Mixing nm, mm and m.
  • Measuring to the wrong fringe.

Statistics and uncertainty

Measuring several fringes and dividing by their count reduces the reading error on w.

Where it is used

  • Measuring wavelengths.
  • Laser and optics calibration.

Maths you need

  • Interference: path difference
  • Unit conversion: nm, mm and m

Related formulas

Practise this formula