Ideal Gas Law · Heat Transfer · Phase Changes · Laws of Thermodynamics
P = pressure (Pa) · V = volume (m³) · n = moles · R = 8.314 J/(mol·K) · T = temperature (K)
Adjust variables — pressure is calculated
Particles collide elastically — higher temperature = faster particles
Heat added to raise m kg by ΔT degrees
Q/t = k·A·ΔT/d (W)
Heat flows through direct contact between particles. Fast in metals (free electrons), slow in insulators.
Warm fluid rises, cool fluid sinks — creating circulation currents. How ovens, oceans, and weather work.
Electromagnetic waves carry energy without needing matter. How the Sun's heat reaches Earth through space.
Solid → Liquid. Occurs at melting point (0°C for water). Requires energy = latent heat of fusion.
Liquid → Gas. Boiling: at 100°C (1 atm). Evaporation: at any temperature at the surface.
Solid → Gas directly, skipping liquid. Dry ice (CO₂) sublimates at −78.5°C at 1 atm.
Gas → Liquid. Releases the same latent heat that was absorbed during vaporisation.
The most efficient possible heat engine operating between two temperatures. Real engines are always less efficient due to friction and other irreversibilities.
The study of heat, work, temperature, and energy. It governs everything from steam engines to refrigerators to the Sun — any system that converts energy between forms.
PV = nRT relates pressure, volume, moles, and temperature for an "ideal" gas (point particles, no intermolecular forces). Real gases deviate at high pressures and low temperatures. R = 8.314 J/(mol·K).
Using PV = nRT, if you double the temperature (in Kelvin) of a gas at constant volume, what happens to the pressure? Try it with the Ideal Gas Law tool. Then explain it using the particle model.