Resources | Subject Notes | Chemistry
This section explores the fundamental properties of matter in its different states – solid, liquid, and gas. We will delve into the arrangement and motion of particles within these states, the associated energies, the processes of changing between states, and the relationships governing the behaviour of gases.
The state of matter is determined by the arrangement and motion of its constituent particles (atoms, ions, or molecules). Different states exhibit distinct characteristics in these aspects.
The kinetic theory provides a model for understanding the macroscopic properties of gases based on the microscopic behaviour of their particles. Key assumptions include:
The kinetic energy of particles in a substance is related to its temperature. The average kinetic energy of particles in a gas is directly proportional to the absolute temperature (in Kelvin).
$$KE_{avg} = \frac{3}{2} k T$$
where:
Changes of state involve the absorption or release of heat energy. These processes are accompanied by a change in the arrangement and motion of particles.
Melting occurs at a specific temperature called the melting point. Heat energy is absorbed to overcome the intermolecular forces holding the solid together.
Freezing occurs at the melting point. Heat energy is released as intermolecular forces become stronger and particles arrange into a crystalline structure.
Boiling occurs at a specific temperature called the boiling point. Heat energy is absorbed to overcome the remaining intermolecular forces and allow particles to escape into the gaseous phase.
Condensation occurs at the boiling point. Heat energy is released as particles slow down and intermolecular forces become dominant, causing them to cluster together in a liquid state.
Sublimation occurs when a solid directly changes into a gas without passing through the liquid phase. This happens when the particles in the solid have enough kinetic energy to overcome the intermolecular forces.
Deposition occurs when a gas directly changes into a solid without passing through the liquid phase. This happens when the particles in the gas lose enough kinetic energy to form a crystalline structure.
Gas laws describe the relationship between the macroscopic properties of gases – pressure (P), volume (V), temperature (T), and number of moles (n).
At constant temperature and number of moles, the pressure of a gas is inversely proportional to its volume.
$$P \propto \frac{1}{V}$$
or
$$P_1 V_1 = P_2 V_2$$
At constant pressure and number of moles, the volume of a gas is directly proportional to its absolute temperature.
$$V \propto T$$
or
$$\frac{V_1}{T_1} = \frac{V_2}{T_2}$$
At constant volume and number of moles, the pressure of a gas is directly proportional to its absolute temperature.
$$P \propto T$$
or
$$\frac{P_1}{T_1} = \frac{P_2}{T_2}$$
Combines Boyle's Law, Charles's Law, and Gay-Lussac's Law.
$$\frac{P_1 V_1}{T_1} = \frac{P_2 V_2}{T_2}$$
Relates pressure, volume, temperature, and the number of moles of a gas through the ideal gas constant (R).
$$PV = nRT$$
where: