Gibbs Energy Change and Equilibrium
✨ Key Ideas
Gibbs free energy (G) helps us predict two important things about chemical reactions:
- 🎯 Whether a reaction happens spontaneously
- ⚡ How much useful work we can get from it
🧪 Equilibrium Condition
At equilibrium, the system’s free energy is at its minimum, and:
This means for a reaction like \( A + B \rightleftharpoons C + D \), the forward and reverse reactions perfectly balance each other ⚖️.
🔗 The Magic Equation
For reactions where all substances are in their standard states, we use:
Where:
– \( \Delta_r G^\circ \) = standard Gibbs energy change
– \( R \) = gas constant (8.314 J/mol·K)
– \( T \) = temperature in Kelvin
– \( K \) = equilibrium constant
🔥🌡️ How Heat (ΔH°) and Chaos (ΔS°) Affect Reactions
ΔH° | ΔS° | Spontaneity |
---|---|---|
– (exothermic) | + (more disorder) | ✅ Spontaneous at all temperatures |
– (exothermic) | – (more order) | ✅ Spontaneous at low temperatures ❌ Not spontaneous at high temperatures |
+ (endothermic) | + (more disorder) | ❌ Not spontaneous at low temperatures ✅ Spontaneous at high temperatures |
+ (endothermic) | – (more order) | ❌ Never spontaneous |
Note: “Low” and “high” temperatures depend on the specific reaction!
📊 Equilibrium Constant Tips
- If \( K \gg 1 \) (large K): Reaction favors products 🟢
- If \( K \ll 1 \) (small K): Reaction favors reactants 🔴
- Exothermic reactions (ΔH° negative) usually have large K
- Endothermic reactions (ΔH° positive) usually have small K
💡 Problem Solving Toolkit
Example 1: Finding ΔG° from K
For \( \frac{3}{2}O_2(g) \rightarrow O_3(g) \) at 298 K with \( K_p = 2.47 \times 10^{-29} \):
Example 2: Finding K from ΔG°
For \( 2NH_3(g) + CO_2(g) \leftrightharpoons NH_2CONH_2(aq) + H_2O(l) \) with ΔG° = -13.6 kJ/mol at 298 K:
Example 3: Finding K from dissociation
For \( N_2O_4(g) \rightleftharpoons 2NO_2(g) \) at 60°C with 50% dissociation:
– Mole fractions: \( x_{N_2O_4} = \frac{0.5}{1.5} \), \( x_{NO_2} = \frac{1}{1.5} \)
– Partial pressures: \( p_{N_2O_4} = \frac{0.5}{1.5} \ \text{atm} \), \( p_{NO_2} = \frac{1}{1.5} \ \text{atm} \)
🚀 NEET Must-Knows
- Equilibrium condition: \( \Delta_r G = 0 \) ⚖️
- Master the equation: \( \Delta G^\circ = -RT \ln K \) 🔑
- Predict spontaneity using ΔH° and ΔS° signs (Table 5.4) 🔥❄️
- Calculate K from ΔG° (and vice versa) 🧮
- Find K for dissociation reactions (like N₂O₄ example) 🧪
💎 Key Takeaway
Gibbs energy is your reaction “thermometer” 🌡️ – it tells you if a reaction will run (ΔG < 0), stay stuck (ΔG > 0), or chill at equilibrium (ΔG = 0)! Combine it with K to predict reaction outcomes.