Thermal Expansion Calculator
Calculate linear or volumetric thermal expansion of materials due to temperature change.
Thermal Expansion Converts Temperature Change into Strain
Most materials change dimensions when temperature changes because average atomic spacing changes with thermal energy. For a uniform isotropic material over a modest range, linear expansion is ΔL=αL0ΔT. The corresponding thermal strain is εth=αΔT. For isotropic solids, the volumetric expansion coefficient is approximately 3α when coefficients are small.
The coefficient α depends on material and temperature. Expansion formulas describe free dimensional change; if supports prevent that movement, thermal stress can develop instead. Different materials joined together can bend or stress because their coefficients differ.
| Symbol | Meaning | Why it appears / units |
|---|---|---|
| α | Linear expansion coefficient | 1/K or 1/°C. |
| L0 | Initial length | Any length unit consistent with ΔL. |
| ΔT | Temperature change | K or °C difference. |
| ΔL | Length change | Same length unit as L₀. |
Expansion scales linearly with original length and temperature change in the simple model. A long structure can therefore require significant movement allowance even when strain is only a few hundred parts per million.
Free thermal expansion should reverse sign when the temperature change reverses. With positive α, heating gives positive ΔL and cooling gives negative ΔL under the usual sign convention. Keep α in reciprocal degrees consistent with the chosen temperature-difference unit.
Worked Examples
Common Mistakes
Linear expansion depends on ΔT from the reference state, not on the final Kelvin temperature itself.
A coefficient listed as 12ppm/K equals 12×10⁻⁶/K.
Thermal expansion coefficients can vary with temperature and phase, so tabulated constant values have limited ranges.
Frequently Asked Questions
Formula Explorer connections
Interpretation: This formula tracks heat, temperature, work, entropy or transport in a thermodynamic system. Assumption: Use absolute temperature where required and consistent energy units. Constant properties, equilibrium, ideal gases or negligible losses may be assumed.