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Physics

Blackbody Radiation Calculator

Calculate Wien peak wavelength and Stefan-Boltzmann radiation power.

Last validated: 2026-02-14

Blackbody Radiation Calculator estimates peak wavelength and emitted power from temperature using blackbody relations. It is useful in physics coursework and thermal-emission intuition building. The tool gives quick numerical outputs from core formulas. Use it to validate hand calculations and scenario comparisons.

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Input Pattern

Enter values in the left panel, keep units explicit, run the calculation, then copy or share the result. Invalid fields are highlighted immediately.

Blackbody Inputs

Result

Peak wavelength (Wien): 499.616 nm

Radiant exitance sigma*T^4: 64168769.431116 W/m²

Total power (area * sigma*T^4): 64168769.431116 W

How to use this tool

  1. Enter absolute temperature and any required area/emissivity inputs.
  2. Run the calculator to compute peak wavelength and radiated power metrics.
  3. Compare outputs across temperature values to analyze trends.

Worked Example

Auto-generated from the tool's current default or entered inputs.

Example Inputs

  • Temperature k: 5800.0
  • Area m2: 1.0
  • Peak wavelength m: 4.996158543103448e-07
  • Peak wavelength nm: 499.6158543103448
  • Radiant exitance w m2: 64168769.43111582

Expected Outputs

  • Temperature k: 5800
  • Area m2: 1
  • Peak wavelength m: 0
  • Peak wavelength nm: 499.615854

Interpretation

Scenario Compare (A vs B)

Use this to compare two input sets and quantify change in key outputs.

Scenario A

Scenario B

Confidence and limitations

Formula References

Assumptions

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