Follow the experiment, change the light, and discover why the energy of emitted electrons depends on frequency—not simply on brightness.
Guided lessonInteractive model5–8 minutes
STEP 1 · OBSERVE
What happens when light strikes a metal?
Light arrives as photons. If an individual photon has enough energy to overcome the metal's work function, an electron can escape from the surface.
Observe the photons reaching the cathode. Emission depends on photon energy.
Explore the light
200 nm · UV700 nm · Red
LowerHigher
Work function is a model value in electronvolts (eV).
Photon energy3.10 eV
Work function, φ2.28 eV
Maximum kinetic energy0.82 eV
Stopping potential0.82 V
The photon energy exceeds the work function, so photoemission is possible.
GRAPHICAL ANALYSIS
Finding Planck's constant from the photoelectric effect
Live graph
Einstein's equation predicts a straight-line relationship between maximum kinetic energy and frequency: Kmax = hν − φ. The gradient gives Planck's constant when the axes are expressed in SI units.
Gradient, ΔKmax/Δν4.136 × 10⁻¹⁵ eV·s
Planck's constant, h6.626 × 10⁻³⁴ J·s
Threshold frequency, ν₀5.51 × 10¹⁴ Hz
The line's gradient represents Planck's constant. The horizontal-axis intercept gives the threshold frequency for the selected metal.