Spontaneity and Free Energy Applications - Complete Interactive Lesson
Part 1: Introduction to Gibbs Free Energy
⚡ Gibbs Free Energy and Spontaneity
Part 1 of 7 — ΔG = ΔH − TΔS
Topics in This Part
Section
⚡ Defining Gibbs Free Energy
Where Does This Come From?
⚡ The Spontaneity Criterion
Why Gibbs Free Energy Is So Useful
What "Free" Means
🔑 Key Concept: Mastering this material will strengthen your foundation for both the AP Chemistry exam and more advanced chemistry topics.
What You'll Master in Part 1
Understanding the core concepts covered in Part 1
Applying these ideas to solve practice problems
Building toward AP exam readiness for this topic
⚡ Defining Gibbs Free Energy
G=H−TS
The change in Gibbs free energy at constant temperature:
ΔG=ΔH
⚡ The Spontaneity Criterion
ΔG
Meaning
ΔG<0
Spontaneous (thermodynamically favorable)
ΔG=0
At equilibrium
⚡ Temperature and Spontaneity
From ΔG=ΔH−TΔS, we see that temperature affects spontaneity through the TΔS term:
At low temperatures: ΔH dominates ( is small)
Gibbs Free Energy Concept Quiz 🎯
Gibbs Free Energy Calculations 🧮
1)ΔH=−100 kJ, ΔS=+50 J/K, T=298 K. Calculate in kJ. (to 3 significant figures)
Gibbs Free Energy Concepts 🔽
Exit Quiz — Gibbs Free Energy ✅
Part 2: ΔG = ΔH − TΔS
🔀 Four ΔH/ΔS Combinations
Part 2 of 7 — Always, Never, or Temperature-Dependent
Topics in This Part
Section
📌 The Four Cases
Case 1: ΔH < 0, ΔS > 0 — Always Spontaneous ✅
Case 2: ΔH > 0, ΔS < 0 — Never Spontaneous ❌
Case 3: ΔH < 0, ΔS < 0 — Spontaneous at Low T 🥶
Case 4: ΔH > 0, ΔS > 0 — Spontaneous at High T 🔥
🔑 Key Concept: Mastering this material will strengthen your foundation for both the AP Chemistry exam and more advanced chemistry topics.
What You'll Master in Part 2
Understanding the core concepts covered in Part 2
Applying these ideas to solve practice problems
Building toward AP exam readiness for this topic
📌 The Four Cases
Case 1: ΔH < 0, ΔS > 0 — Always Spontaneous ✅
ΔG
Part 3: Spontaneity & Temperature
🏗️ Standard Free Energy of Formation
Part 3 of 7 — Calculating ΔG° from Tables
Topics in This Part
Section
⚡ Standard Free Energy of Formation (ΔG°f)
The Master Equation
Key Rule
Sample Values
🧪 Worked Example
🔑 Key Concept: Mastering this material will strengthen your foundation for both the AP Chemistry exam and more advanced chemistry topics.
What You'll Master in Part 3
Understanding the core concepts covered in Part 3
Applying these ideas to solve practice problems
Building toward AP exam readiness for this topic
Part 4: Standard Free Energy of Formation
⚖️ ΔG and Equilibrium
Part 4 of 7 — ΔG° = −RT ln K
Topics in This Part
Section
🔑 The Key Equation
What This Equation Tells Us
Important Nuance
📌 Solving for K from ΔG°
Worked Example
🔑 Key Concept: Mastering this material will strengthen your foundation for both the AP Chemistry exam and more advanced chemistry topics.
What You'll Master in Part 4
Understanding the core concepts covered in Part 4
Applying these ideas to solve practice problems
Building toward AP exam readiness for this topic
🔑 The Key Equation
Part 5: ΔG and Equilibrium
📊 Non-Standard Conditions — ΔG = ΔG° + RT ln Q
Part 5 of 7 — Real-World Free Energy
Topics in This Part
Section
⚡ The Non-Standard Free Energy Equation
Recall: Q vs K
📌 Interpreting ΔG, Q, and K
Key Insight
The Big Picture
🔑 Key Concept: Mastering this material will strengthen your foundation for both the AP Chemistry exam and more advanced chemistry topics.
What You'll Master in Part 5
Understanding the core concepts covered in Part 5
Applying these ideas to solve practice problems
Building toward AP exam readiness for this topic
⚡ The Non-Standard Free Energy Equation
Part 6: Problem-Solving Workshop
🛠️ Problem-Solving Workshop — Gibbs Free Energy
Part 6 of 7 — Practice and Integration
Practice Makes Perfect
This workshop features multi-step problems that mirror the AP Chemistry exam format. Each problem requires you to combine concepts from previous parts and show your work clearly.
🔑 Why this matters: The AP Chemistry exam rewards students who can apply concepts to unfamiliar problems — structured practice is the best preparation.
What You'll Master in Part 6
Working through complete multi-step problems from start to finish
Building problem-solving strategies you can apply on the AP exam
Identifying which concepts to apply and in what order
🛠️ Problem-Solving Flowchart
💡 Tip: On the AP exam, identify what you're given first, then choose the correct equation.
What Are You Given? → What Method to Use?
Given
Method
ΔH and (or )
Part 7: Synthesis & AP Review
🎯 Synthesis & AP Review — Gibbs Free Energy
Part 7 of 7 — Mastering the Connections
Bringing It All Together
This comprehensive review connects every concept from Parts 1–6 with AP-style problems. The questions are designed to mirror what you'll see on the actual exam — multi-step, multi-concept, and requiring clear written explanations.
🔑 Why this matters: AP Chemistry exam questions rarely test one concept in isolation — success requires connecting ideas across topics.
What You'll Master in Part 7
Solving AP-style questions that integrate multiple concepts from this unit
Writing clear, concise explanations using proper chemistry terminology
Identifying and avoiding common AP exam traps and mistakes
🌡️ The Web of Thermodynamic Equations
Core Equations
🔑 Key Concept: These five equations form the complete Gibbs free energy toolkit for AP Chemistry.
| Equation | When to Use |
|----------|-------------|
| ΔG=ΔH | Calculate ΔG from enthalpy and entropy |
| | Calculate from tables |
| | Connect free energy to equilibrium |
| | Non-standard conditions |
| | Connect to electrochemistry (Topic 4) |
−
T
Δ
S
🔑 Key Equation: This is the master equation of Gibbs free energy — it combines enthalpy and entropy into a single criterion for spontaneity.
Where Does This Come From?
Recall: ΔSuniverse=ΔSsystem+ΔSsurroundings
And: ΔSsurroundings=−ΔHsystem/T
So: ΔSuniverse=ΔSsys−ΔHsys/T
Multiply by −T:
−TΔSuniverse=ΔHsys−TΔSsys=ΔG
Since ΔSuniverse>0 for spontaneous processes:
ΔG<0(spontaneous)
ΔG>0
Nonspontaneous (reverse reaction is spontaneous)
🔑 Key Concept: Memorize this table — it's the foundation for every Gibbs free energy problem on the AP exam.
Why Gibbs Free Energy Is So Useful
It accounts for both enthalpy and entropy
It is a property of the system only — no need to calculate ΔSsurroundings
It connects directly to equilibrium and electrochemistry
What "Free" Means
"Free energy" is the maximum amount of energy available to do useful work (non-PV work) in a reaction.
wmax=ΔG
If ΔG=−100 kJ, the reaction can do at most 100 kJ of useful work.
TΔS
At high temperatures: TΔS dominates (TΔS is large)
⚠️ Warning: Temperature must always be in Kelvin in thermodynamic equations. Also ensure ΔH and TΔS use the same units (both kJ or both J).
The Crossover Temperature
When ΔG=0 (equilibrium):
T=ΔSΔH
This is the temperature at which the reaction switches between spontaneous and nonspontaneous.
Example
Problem: For ice melting: ΔH=+6.01 kJ/mol, ΔS=+22.0 J/(mol·K)
Solution:
T=22.06010=273 K=0°C
Above 273 K: melting is spontaneous (ΔG<0). Below 273 K: freezing is spontaneous.
ΔG
2)ΔH=+200 kJ, ΔS=+500 J/K, T=500 K. Calculate ΔG in kJ.
3) A reaction has ΔH=+30 kJ and ΔS=+100 J/K. At what temperature (in K) is ΔG=0?
=
(negative)−
T(positive)=
always negative
Both terms favor spontaneity
Spontaneous at all temperatures
Example: combustion of hydrocarbons
Case 2: ΔH > 0, ΔS < 0 — Never Spontaneous ❌
ΔG=(positive)−T(negative)=always positive
Both terms oppose spontaneity
Never spontaneous (the reverse reaction is always spontaneous)
Example: the reverse of combustion
Case 3: ΔH < 0, ΔS < 0 — Spontaneous at Low T 🥶
ΔG=(negative)−T(negative)
Exothermic but entropy-decreasing
At low T: ∣ΔH∣>∣TΔS∣ → ΔG<0
At high T: ∣TΔS∣>∣ΔH∣ → ΔG>0
Example: freezing of water
Case 4: ΔH > 0, ΔS > 0 — Spontaneous at High T 🔥
ΔG=(positive)−T(positive)
Endothermic but entropy-increasing
At high T: ∣TΔS∣>∣ΔH∣ → ΔG<0
At low T: ∣ΔH∣>∣TΔS∣ → ΔG>0
Example: melting of ice, vaporization
📋 Summary Table
ΔH
ΔS
ΔG
Spontaneous?
−
+
Always −
Always ✅
+
−
Always +
Never ❌
−
−
− at low T, + at high T
Low T only 🥶
+
+
+ at low T, − at high T
High T only 🔥
🔑 Key Concept: This table appears on nearly every AP Chemistry exam. Memorize all four cases and be ready to identify which case applies from ΔH/ΔS signs.
The Crossover Temperature
For Cases 3 and 4, the temperature where ΔG=0:
Tcrossover=ΔSΔH
💡 Tip: This equation only gives a physically meaningful (positive) temperature when ΔH and ΔS have the same sign (Cases 3 and 4).
🧪 Real-World Examples
Case 1 (Always Spontaneous): Combustion
CH4(g)+2O2(g)→CO2(g)+2H2O(g)
ΔH<0 (releases heat)
ΔS>0 (Δngas, but products are more complex — actually can be slightly negative for this specific reaction at standard conditions)
Case 3 (Low T): Freezing Water
H2O(l)→H2O(s)
ΔH<0 (releases heat — exothermic)
ΔS<0 (liquid → solid, more ordered)
Spontaneous only below 273 K
Case 4 (High T): Melting Ice
H2O(s)→H2O(l)
ΔH>0 (absorbs heat — endothermic)
ΔS>0 (solid → liquid, more disordered)
Spontaneous only above 273 K
Four Cases Quiz 🎯
Classify the Reaction 🧮
For each combination, type "always", "never", "low T", or "high T" for when the reaction is spontaneous:
1)ΔH<0, ΔS>0
2)ΔH>0, ΔS>0
3)ΔH>0, ΔS<0
Spontaneity and Temperature 🔽
Exit Quiz — Four Cases ✅
⚡ Standard Free Energy of Formation (ΔG°f)
The free energy change when one mole of a compound is formed from its elements in their standard states at standard conditions.
The Master Equation
ΔG°rxn=∑n⋅ΔG°f(products)−∑m⋅
Key Rule
ΔG°f=0 for all elements in their standard states
🔑 Key Concept: Same convention as ΔH°f — elements in their standard states are the reference point.