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Chemistry

Ideal Gas Law Calculator

Solve pressure, volume, moles, or temperature with PV=nRT.

Formula reviewed: 2026-02-14 Chemistry

Use this free online Ideal Gas Law Calculator to solve for pressure, volume, temperature, or moles using PV = nRT. It is useful for classwork, lab checks, design screening, and engineering sanity checks where units and assumptions must stay visible. The form focuses on Mode, Pressure (atm), Volume (L), Moles (mol), Temperature (K) and returns Ideal Gas Law Inputs, Result, so you can move from input to answer without setting up a spreadsheet or custom script. Run one realistic example, adjust the inputs, and compare how the result changes before you copy or share it. Check units and formula assumptions carefully; for safety-critical or code-governed work, validate the result with authoritative references.

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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.

How to use this tool

  1. Enter Mode, Pressure (atm), Volume (L), Moles (mol), Temperature (K) for the ideal gas law calculator, keeping units, dates, or text format consistent with the form labels.
  2. Choose the relevant mode, unit, or option values before running so the output answers the right version of the question.
  3. Click "Run the tool" and review Ideal Gas Law Inputs, Result for the primary output.
  4. Verify units and assumptions, especially before using the result for design, lab, or safety-sensitive work.

Ideal Gas Law Inputs

Use PV = nRT (R = 0.082057 L*atm/mol*K).

Result

Solved value: 1.223265

The Ideal Gas Law

Pressure, Volume, Temperature, and Amount

The ideal gas law, PV = nRT, connects pressure, volume, amount of gas, and absolute temperature. It combines several simpler gas relationships into one equation: pressure rises when gas is compressed, volume expands with temperature, and more moles mean more particles contributing to pressure.

The constant R depends on the units used. Temperature must be absolute, usually Kelvin, because gas volume and molecular kinetic energy relate to distance above absolute zero rather than Celsius or Fahrenheit offsets. Unit consistency is not a detail; it is part of the law.

The Molecular Picture

The ideal gas model imagines particles moving randomly, colliding elastically, and occupying negligible volume compared with the container. Pressure comes from countless molecular impacts on container walls. Temperature reflects average kinetic energy.

This microscopic view explains the macroscopic equation. Raising temperature increases particle speeds and therefore pressure if volume is fixed. Increasing volume gives particles more space, reducing collision frequency with the walls. Adding moles adds more particles and raises pressure if volume and temperature stay constant.

When Gases Behave Ideally

Many gases behave approximately ideally at low pressure and high temperature, where particles are far apart and intermolecular forces are relatively small. Air near room conditions is often close enough for practical estimates.

The model becomes weaker at high pressure, low temperature, or near phase changes. Real molecules have volume and attractions. In those situations, equations such as van der Waals or compressibility-factor corrections may be needed. Ideal gas results are a baseline, not a universal truth.

Applications and Cautions

The ideal gas law appears in chemistry stoichiometry, ventilation, cylinders, balloons, engines, weather, lab experiments, and safety calculations. It can estimate gas amount from pressure and volume or predict how pressure changes with temperature.

Care is especially important with sealed containers. Heating a fixed-volume gas raises pressure, sometimes dangerously. Gas calculations should respect rated equipment limits, material compatibility, and real-gas behavior when conditions are extreme.

How to interpret the result

Confidence and limitations

Formula References

Assumptions

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