Equilibrium means a state of balance. In chemistry, equilibrium is when the observable properties (like colour, temperature, pressure, or concentration) do not change over time.
Physical equilibrium exists when a substance exists in more than one phase, and there is no chemical change. Examples include:
(i) Solid–Liquid Equilibrium
H₂O(solid) ⇌ H₂O(liquid)
Rate of melting = Rate of freezing
(ii) Liquid–Vapour Equilibrium
H₂O(liquid) ⇌ H₂O(vapour)
Rate of vaporization = Rate of condensation
NOTE: Triple point of water is the temperature and pressure where solid, liquid, and gas states of water coexist: 273.15 K
(iii) Solid–Vapour Equilibrium
NH₄Cl(solid) ⇌ NH₄Cl(vapour)
This process is sublimation, and reverse is called deposition or desublimation.
(iv) Solid–Solution Equilibrium
Sugar(solid) ⇌ Sugar(solution)
In a saturated solution, the rate of dissolution = rate of precipitation
(v) Gas–Liquid Equilibrium
Solubility of a gas in a liquid depends on:
At constant temperature, the mass of a gas dissolved in a liquid is directly proportional to the pressure of the gas above the liquid. Gas solubility decreases with increasing temperature. Occurs during physical changes.
Examples:
Chemical equilibrium occurs in reversible chemical reactions.
Examples:
Dynamic in nature – both forward and backward reactions continue at equal rates
Electrolytes
Examples of weak electrolyte equilibrium:
For a general reaction: aA + bB ⇌ cC + dD
The equilibrium constant is: Kₑq = [C]c [D]d / [A]a [B]b
Interpreting Kₑq Values:
Note: Kₑq is constant at a given temperature, but changes if the temperature changes.
(Session 2025 - 26)