Ideal Gas Law Calculator

Solve for pressure, volume, temperature, or moles using the ideal gas law PV = nRT.

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The Ideal Gas Law in Context

The ideal gas law is a cornerstone of thermodynamics and physical chemistry, combining Boyle's Law (pressure and volume are inversely related at constant temperature), Charles's Law (volume and temperature are directly related at constant pressure), and Avogadro's Law (volume and moles are directly related at constant pressure and temperature) into a single elegant equation.

The constant R is universal—it is the same for all ideal gases regardless of chemical identity. Its magnitude in SI units, 8.314 J/(mol·K), reflects the conversion between mechanical work (pressure × volume) and thermal energy. At the particle level, the Boltzmann constant k_B plays an analogous role, with R simply being k_B scaled by Avogadro's number.

Real gases deviate from ideality under conditions where particles are close together and forces matter: high pressure and low temperature. The van der Waals equation corrects for these deviations and is accurate enough for most engineering applications involving common gases like nitrogen, oxygen, and carbon dioxide. For extreme conditions—such as inside gas giants or cryogenic systems—more complex equations of state like the Peng-Robinson or Redlich-Kwong models are required.

Explore more physics and chemistry tools: calculate motion energy with our Kinetic Energy Calculator, analyze acidity with the pH Calculator, or study radioactive decay with the Half-Life Calculator.

References & Further Reading

Frequently Asked Questions

The ideal gas law is a fundamental equation of state in physics and chemistry that relates the pressure (P), volume (V), temperature (T), and amount of substance (n) of an ideal gas: PV = nRT. An ideal gas is a theoretical model in which gas particles occupy no volume and experience no intermolecular forces. While no real gas is perfectly ideal, the law provides an excellent approximation at low pressures and high temperatures where particles are far apart and interactions are negligible.

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