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Thermodynamics - Interactive Lesson | Study Mondo
Thermodynamics - Complete Interactive Lesson Part 1: Enthalpy & Hess's Law Thermodynamics
Part 1 of 5 — Enthalpy (Δ H \Delta H Δ H ) & Hess's Law
System vs. Surroundings
System: The reaction or process under study
Surroundings: Everything else (including the calorimeter/solution)
First Law of Thermodynamics: Energy is conserved: Δ E universe = 0 \Delta E_{\text{universe}} = 0 Δ E universe = 0 ; Δ E sys = − Δ E surr \Delta E_{\text{sys}} = -\Delta E_{\text{surr}} Δ E sys = − Δ E surr
Enthalpy (H H H )
Enthalpy change Δ H \Delta H Δ H = heat transferred at constant pressure.
Δ H = H products − H reactants \Delta H = H_{\text{products}} - H_{\text{reactants}} Δ H = H products − H reactants
Δ H \Delta H Δ H Name Energy transfer Negative (Δ H < 0 \Delta H < 0 Δ H < 0 ) Exothermic Releases heat to surroundings Positive (Δ H > 0 \Delta H > 0 Δ H > 0 ) Endothermic
Calorimetry at constant pressure:
q = m c Δ T q = mc\Delta T q = m c Δ T
where m m m = mass (g), c c c = specific heat (J/g·°C), Δ T = T final − T initial \Delta T = T_{\text{final}} - T_{\text{initial}} Δ T = T final − T .
For the reaction: Δ H rxn = − q solution \Delta H_{\text{rxn}} = -q_{\text{solution}} Δ H rxn = − q solution (the sign flip — if the solution warms, the reaction is exothermic)
Standard Enthalpy of Formation (Δ H ° f \Delta H°_f Δ H ° f )
Δ H ° f \Delta H°_f Δ H ° f = enthalpy change when 1 mole of a compound is formed from its elements in their standard states.
By convention: Δ H ° f = 0 \Delta H°_f = 0 Δ H ° f = 0 for pure elements in standard states.
Hess's Law:
Δ H ° rxn = ∑ n Δ H ° f ( products ) − ∑ m Δ H ° f ( reactants ) \Delta H°_{\text{rxn}} = \sum n \Delta H°_f(\text{products}) - \sum m \Delta H°_f(\text{reactants}) Δ H ° rxn = ∑ n Δ H ° f
Hess's Law (Path Independence)
Enthalpy is a state function — Δ H \Delta H Δ H depends only on initial and final states, not the path.
Method: Reactions can be added/subtracted like algebraic equations to obtain a target reaction.
Rules for manipulating reactions:
If a reaction is reversed , flip the sign of Δ H \Delta H Δ H
If a reaction is multiplied by a factor, multiply Δ H \Delta H Δ H by the same factor
Worked Example
Find Δ H \Delta H Δ H for: C ( s ) + 1 2 O 2 ( g ) → CO ( g ) \text{C}(s) + \frac{1}{2}\text{O}_2(g) \to \text{CO}(g) C ( s ) + 2 1 O
Given:
(1) C ( s ) + O 2 ( g ) → CO 2 ( g ) \text{C}(s) + \text{O}_2(g) \to \text{CO}_2(g) C ( s ) + O 2 ( g ) → CO 2 ( g ; kJ
Reverse reaction (2): CO 2 ( g ) → CO ( g ) + 1 2 O 2 ( g ) \text{CO}_2(g) \to \text{CO}(g) + \frac{1}{2}\text{O}_2(g) CO 2 ( g ) → CO ( g ) + 2 ; kJ
Add to reaction (1):
C ( s ) + O 2 + CO 2 → CO 2 + CO + 1 2 O 2 \text{C}(s) + \text{O}_2 + \text{CO}_2 \to \text{CO}_2 + \text{CO} + \frac{1}{2}\text{O}_2 C ( s ) + O 2 + CO 2 →
C ( s ) + 1 2 O 2 ( g ) → CO ( g ) \text{C}(s) + \frac{1}{2}\text{O}_2(g) \to \text{CO}(g) C ( s ) + 2 1 O 2 ( g
Δ H = − 393.5 + 283.0 = − 110.5 kJ \Delta H = -393.5 + 283.0 = \mathbf{-110.5\text{ kJ}} Δ H = − 393.5 + 283.0 = − 110.5 kJ
Bond Enthalpy Approximation
Δ H rxn ≈ ∑ ( bonds broken ) − ∑ ( bonds formed ) \Delta H_{\text{rxn}} \approx \sum (\text{bonds broken}) - \sum (\text{bonds formed}) Δ H rxn ≈ ∑ ( bonds broken ) − ∑ ( bonds formed )
Breaking bonds requires energy (+); forming bonds releases energy (−). This gives an estimate; less accurate than using Δ H ° f \Delta H°_f Δ H ° f values.
Key Takeaways — Part 1
Δ H < 0 \Delta H < 0 Δ H < 0 : exothermic (releases heat); Δ H > 0 \Delta H > 0 Δ H > 0 : endothermic (absorbs heat)
Calorimetry: q = m c Δ T q = mc\Delta T q = m c Δ T ;
Part 2: Entropy & Laws of Thermodynamics Thermodynamics
Part 2 of 5 — Entropy (Δ S \Delta S Δ S ), Spontaneity & the Laws of Thermodynamics
Entropy (S S S )
Entropy is a measure of disorder or randomness of a system.
Δ S = S products − S reactants \Delta S = S_{\text{products}} - S_{\text{reactants}} Δ S = S
Part 3: Gibbs Free Energy, Keq & Cell Potential Thermodynamics
Part 3 of 5 — Gibbs Free Energy, K e q K_{eq} K e q & Cell Potential
Gibbs Free Energy (G G G )
Δ G = Δ H − T Δ S \Delta G = \Delta H - T\Delta S Δ G =
Part 4: Phase Changes & Heating Curves Thermodynamics
Part 4 of 5 — Phase Changes, Heating Curves & Colligative Properties
Phases and Phase Changes
The six phase transitions:
Transition Direction Δ H \Delta H Δ H Δ S \Delta S Δ S Fusion (melting) solid → liquid + (endothermic) + Freezing liquid → solid − (exothermic) − Vaporization liquid → gas + (endothermic) + Condensation
Part 5: Mixed MCAT Review Thermodynamics
Part 5 of 5 — Mixed MCAT Review
High-Yield Checklist
✅ Δ H \Delta H Δ H : exothermic (−) releases heat; endothermic (+) absorbs heat
✅ Hess's Law: Δ H \Delta H Δ H is a state function; add reactions algebraically
✅ Δ S > 0 \Delta S > 0 Δ S > 0 : more disorder (gas formed, dissolution, mixing, heating)
✅ Δ G = Δ H − T Δ : negative = spontaneous
Absorbs heat from surroundings
initial
(
products
)
−
∑ m Δ H ° f ( reactants )
2
(
g
)
→
CO ( g )
)
Δ H 1 = − 393.5 \Delta H_1 = -393.5 Δ H 1 = − 393.5 (2) CO ( g ) + 1 2 O 2 ( g ) → CO 2 ( g ) \text{CO}(g) + \frac{1}{2}\text{O}_2(g) \to \text{CO}_2(g) CO ( g ) + 2 1 O 2 ( g ) → CO 2 ( g ) ; Δ H 2 = − 283.0 \Delta H_2 = -283.0 Δ H 2 = − 283.0 kJ 1
O 2
(
g
)
Δ H = + 283.0 \Delta H = +283.0 Δ H = + 283.0
CO 2 +
CO +
2 1 O 2
)
→
CO ( g )
Δ H rxn = − q soln \Delta H_{\text{rxn}} = -q_{\text{soln}} Δ H rxn = − q soln
Hess's Law: Δ H \Delta H Δ H is a state function; add reactions algebraically Reverse a reaction → flip sign of Δ H \Delta H Δ H ; multiply by factor → multiply Δ H \Delta H Δ H Formation enthalpy: Δ H ° rxn = ∑ n Δ H ° f ( products ) − ∑ m Δ H ° f ( reactants ) \Delta H°_{\text{rxn}} = \sum n\Delta H°_f(\text{products}) - \sum m\Delta H°_f(\text{reactants}) Δ H ° rxn = ∑ n Δ H ° f ( products ) − ∑ m Δ H ° f ( reactants ) Δ H ° f = 0 \Delta H°_f = 0 Δ H ° f = 0 for elements in standard statesproducts
−
S reactants
Δ S \Delta S Δ S Meaning Positive (Δ S > 0 \Delta S > 0 Δ S > 0 ) Increased disorder Negative (Δ S < 0 \Delta S < 0 Δ S < 0 ) Decreased disorder
Predicting the Sign of Δ S \Delta S Δ S Δ S > 0 \Delta S > 0 Δ S > 0 (entropy increases) when:
Gases are produced from solids/liquids (Δ n gas > 0 \Delta n_{\text{gas}} > 0 Δ n gas > 0 )
A solid dissolves to form aqueous ions
Temperature increases (for any substance)
A substance vaporizes or melts
Mixing occurs
Gas occupies larger volume
Δ S < 0 \Delta S < 0 Δ S < 0 (entropy decreases) when:
Gases are consumed (Δ n gas < 0 \Delta n_{\text{gas}} < 0 Δ n gas < 0 , e.g., 3 mol gas → 1 mol gas)
A substance crystallizes/freezes
Complex molecules form from simpler ones (polymerization)
Laws of Thermodynamics Zeroth Law: If A is in thermal equilibrium with B, and B with C, then A is in equilibrium with C. (Defines temperature)
First Law: Energy is conserved. Δ E universe = 0 \Delta E_{\text{universe}} = 0 Δ E universe = 0 .
Δ U = q + w ( internal energy = heat + work ) \Delta U = q + w \quad (\text{internal energy} = \text{heat} + \text{work}) Δ U = q + w ( internal energy = heat + work )
where w = − P Δ V w = -P\Delta V w = − P Δ V for expansion/compression work.
Second Law: The entropy of the universe always increases for spontaneous processes.
Δ S universe = Δ S sys + Δ S surr > 0 ( spontaneous ) \Delta S_{\text{universe}} = \Delta S_{\text{sys}} + \Delta S_{\text{surr}} > 0 \quad (\text{spontaneous}) Δ S universe = Δ S sys + Δ S surr > 0 ( spontaneous )
Third Law: The entropy of a perfect crystal at absolute zero (0 K) is exactly zero. This establishes an absolute reference for entropy measurements.
Standard Molar Entropy (S ° S° S ° ) S ° > 0 S° > 0 S ° > 0 for all pure substances (third law). More complex molecules have higher S ° S° S ° values.
Δ S ° rxn = ∑ n S ° ( products ) − ∑ m S ° ( reactants ) \Delta S°_{\text{rxn}} = \sum n S°(\text{products}) - \sum m S°(\text{reactants}) Δ S ° rxn = ∑ n S ° ( products ) − ∑ m S ° ( reactants )
Spontaneity — First Look A process is spontaneous if it can proceed without continuous external input of energy.
Caution: Spontaneous does NOT mean fast (kinetics is separate from thermodynamics).
Exothermic processes (Δ H < 0 \Delta H < 0 Δ H < 0 ) tend to be spontaneous — enthalpy drives spontaneity
Disorder increasing (Δ S > 0 \Delta S > 0 Δ S > 0 ) tends to be spontaneous — entropy drives spontaneity
But both factors matter — see Gibbs free energy (Part 3)
Δ H \Delta H Δ H Δ S \Delta S Δ S Spontaneous? − + Always spontaneous + − Never spontaneous − − Depends on T (low T favors) + + Depends on T (high T favors)
Entropy & Laws of Thermodynamics 🎯
Key Takeaways — Part 2
Entropy increases when gases form, substances dissolve, temperature rises, or mixing occurs
Entropy decreases when gases condense, substances crystallize, or complexity increases
Second Law: Δ S universe > 0 \Delta S_{\text{universe}} > 0 Δ S universe > 0 for all spontaneous processes
Third Law: S = 0 S = 0 S = 0 for perfect crystal at 0 K; all S ° > 0 S° > 0 S ° > 0 at room temperature
Spontaneous ≠ fast; thermodynamics says nothing about how quickly a reaction occurs
Δ H < 0 \Delta H < 0 Δ H < 0 favors spontaneity; Δ S > 0 \Delta S > 0 Δ S > 0 favors spontaneity; temperature controls the trade-off
Δ
H
−
T Δ S
Δ G \Delta G Δ G combines both enthalpy and entropy to predict spontaneity:
Δ G \Delta G Δ G Process Δ G < 0 \Delta G < 0 Δ G < 0 Spontaneous (thermodynamically favorable) Δ G = 0 \Delta G = 0 Δ G = 0 At equilibrium Δ G > 0 \Delta G > 0 Δ G > 0 Non-spontaneous (requires energy input)
Temperature governs which effect wins when Δ H \Delta H Δ H and Δ S \Delta S Δ S have the same sign.
Standard Gibbs Free Energy (Δ G ° \Delta G° Δ G ° ) Δ G ° = Δ H ° − T Δ S ° \Delta G° = \Delta H° - T\Delta S° Δ G ° = Δ H ° − T Δ S °
Also calculable from formation values:
Δ G ° = ∑ n Δ G ° f ( products ) − ∑ m Δ G ° f ( reactants ) \Delta G° = \sum n\Delta G°_f(\text{products}) - \sum m\Delta G°_f(\text{reactants}) Δ G ° = ∑ n Δ G ° f ( products ) − ∑ m Δ G ° f ( reactants )
Relationship Between Δ G ° \Delta G° Δ G ° and K e q K_{eq} K e q Δ G ° = − R T ln K \Delta G° = -RT\ln K Δ G ° = − RT ln K
where R = 8.314 R = 8.314 R = 8.314 J/mol·K, T T T in Kelvin.
Δ G ° \Delta G° Δ G ° K K K Meaning < 0 < 0 < 0 K > 1 K > 1 K > 1 Products favored at equilibrium = 0 = 0 = 0 K = 1 K = 1 K = 1 Reactants and products roughly equal > 0 > 0 > 0 K < 1 K < 1 K < 1 Reactants favored at equilibrium
Large negative Δ G ° \Delta G° Δ G ° → large K K K → reaction runs nearly to completion.
Relationship to Cell Potential (E ° cell E° _{\text{cell}} E ° cell ) For electrochemical reactions:
Δ G ° = − n F E ° cell \Delta G° = -nFE°_{\text{cell}} Δ G ° = − n FE ° cell
n n n = moles of electrons transferred
F = 96,485 F = 96{,}485 F = 96 , 485 C/mol (Faraday constant)
E ° cell E°_{\text{cell}} E ° cell measured in volts (V)
Connection between Δ G ° \Delta G° Δ G ° , K K K , and E ° cell E°_{\text{cell}} E ° cell :
Δ G ° = − R T ln K = − n F E ° cell \Delta G° = -RT\ln K = -nFE°_{\text{cell}} Δ G ° = − RT ln K = − n FE ° cell
Sign of E ° cell E°_{\text{cell}} E ° cell Δ G ° \Delta G° Δ G ° Spontaneous? E ° cell > 0 E°_{\text{cell}} > 0 E ° cell > 0 Negative Yes E ° cell < 0 E°_{\text{cell}} < 0 E ° cell < 0 Positive No E ° cell = 0 E°_{\text{cell}} = 0 E ° cell = 0 Zero At equilibrium
Δ G \Delta G Δ G at Non-Standard ConditionsWhen the system is not at standard conditions:
Δ G = Δ G ° + R T ln Q \Delta G = \Delta G° + RT\ln Q Δ G = Δ G ° + RT ln Q
At equilibrium, Δ G = 0 \Delta G = 0 Δ G = 0 and Q = K Q = K Q = K , which yields Δ G ° = − R T ln K \Delta G° = -RT\ln K Δ G ° = − RT ln K (as above).
Coupled Reactions In biochemistry, non-spontaneous reactions are driven by coupling with spontaneous ones:
Example: Glucose phosphorylation (Δ G ° = + 13.8 \Delta G° = +13.8 Δ G ° = + 13.8 kJ) is coupled with ATP hydrolysis (Δ G ° = − 30.5 \Delta G° = -30.5 Δ G ° = − 30.5 kJ):
Δ G ° total = 13.8 + ( − 30.5 ) = − 16.7 kJ (spontaneous) \Delta G°_{\text{total}} = 13.8 + (-30.5) = -16.7\text{ kJ} \quad \text{(spontaneous)} Δ G ° total = 13.8 + ( − 30.5 ) = − 16.7 kJ (spontaneous)
This is how cells use ATP to drive energetically unfavorable biochemical reactions.
Gibbs Free Energy, K e q K_{eq} K e q & E ° cell E°_{\text{cell}} E ° cell 🎯
Key Takeaways — Part 3
Δ G = Δ H − T Δ S \Delta G = \Delta H - T\Delta S Δ G = Δ H − T Δ S : negative Δ G \Delta G Δ G = spontaneous
Δ G ° = − R T ln K \Delta G° = -RT\ln K Δ G ° = − RT ln K : negative Δ G ° \Delta G° Δ G ° → K > 1 K > 1 K > 1 (products favored)
Δ G ° = − n F E ° cell \Delta G° = -nFE°_{\text{cell}} Δ G ° = − n FE ° cell : positive E ° cell E°_{\text{cell}} E ° cell → negative → spontaneous galvanic cell
At equilibrium: Δ G = 0 \Delta G = 0 Δ G = 0 , Q = K Q = K Q = K
Non-standard conditions: Δ G = Δ G ° + R T ln Q \Delta G = \Delta G° + RT\ln Q Δ G = Δ G ° + RT ln Q
Coupled reactions: add Δ G ° \Delta G° Δ G ° values; ATP hydrolysis drives non-spontaneous biochemical reactions
The Δ G \Delta G Δ G , K K K , and E ° cell E°_{\text{cell}} E ° cell are all interconnected — if you know one, you can find the others
Sublimation solid → gas + (endothermic) +
Deposition gas → solid − (exothermic) −
At the phase transition temperature (e.g., boiling point), Δ G = 0 \Delta G = 0 Δ G = 0 :
Δ G = Δ H − T Δ S = 0 ⇒ T transition = Δ H Δ S \Delta G = \Delta H - T\Delta S = 0 \Rightarrow T_{\text{transition}} = \frac{\Delta H}{\Delta S} Δ G = Δ H − T Δ S = 0 ⇒ T transition = Δ S Δ H
Heating Curves A heating curve shows temperature vs. heat added for a substance.
Slanted region: Temperature rises; q = m c Δ T q = mc\Delta T q = m c Δ T ; specific heat governs slope
Flat region (plateau): Phase change at constant T; q = n Δ H fus q = n\Delta H_{\text{fus}} q = n Δ H fus or q = n Δ H vap q = n\Delta H_{\text{vap}} q = n Δ H vap
Steeper slope = lower specific heat; gentle slope = higher specific heat
Specific heats to know (MCAT):
Water (liquid): 4.18 4.18 4.18 J/g·°C (highest of common substances)
Steam: 2.01 2.01 2.01 J/g·°C
Ice: 2.09 2.09 2.09 J/g·°C
Δ H fus \Delta H_{\text{fus}} Δ H fus (water) = 6.01 6.01 6.01 kJ/mol
Δ H vap \Delta H_{\text{vap}} Δ H vap (water) = 40.7 40.7 40.7 kJ/mol
Example calculation: Heat to convert 18.0 g (1.00 mol) of ice at −10°C to steam at 110°C:
Heat ice: 18.0 × 2.09 × 10 = 376.2 18.0 \times 2.09 \times 10 = 376.2 18.0 × 2.09 × 10 = 376.2 J
Melt ice: 1.00 × 6010 = 6010 1.00 \times 6010 = 6010 1.00 × 6010 = 6010 J
Heat water: 18.0 × 4.18 × 100 = 7524 18.0 \times 4.18 \times 100 = 7524 18.0 × 4.18 × 100 = 7524 J
Boil water: 1.00 × 40,700 = 40,700 1.00 \times 40{,}700 = 40{,}700 1.00 × 40 , 700 = 40 , 700 J
Heat steam: 18.0 × 2.01 × 10 = 361.8 18.0 \times 2.01 \times 10 = 361.8 18.0 × 2.01 × 10 = 361.8 J
Total = 376.2 + 6010 + 7524 + 40,700 + 361.8 ≈ 54,972 J ≈ 55.0 kJ 376.2 + 6010 + 7524 + 40{,}700 + 361.8 \approx \mathbf{54{,}972\text{ J} \approx 55.0\text{ kJ}} 376.2 + 6010 + 7524 + 40 , 700 + 361.8 ≈ 54 , 972 J ≈ 55.0 kJ
Phase Diagrams A phase diagram plots pressure vs. temperature; shows stable phase regions divided by boundary curves.
Point/Line Meaning Triple point All three phases coexist Critical point Gas and liquid become indistinguishable Solid-liquid line Melting points at various pressures Liquid-gas line Boiling points at various pressures
Water is unusual: Solid-liquid line has negative slope (ice is less dense than water; increasing pressure melts ice).
Colligative Properties (Review) Colligative properties depend on the number of solute particles , not their identity.
Property Formula Key notes Boiling point elevation Δ T b = K b m i \Delta T_b = K_b m i Δ T b = K b mi Higher BP than solvent Freezing point depression Δ T f = K f m i \Delta T_f = K_f m i Δ T f = K f mi Lower FP than solvent Osmotic pressure Π = i M R T \Pi = iMRT Π = i MRT R = 0.0821 R = 0.0821 R = 0.0821 L·atm/mol·KVapor pressure lowering Δ P = χ solute P ° solvent \Delta P = \chi_{\text{solute}} P°_\text{solvent} Δ P = χ solute P ° solvent Raoult's law
i i i = van 't Hoff factor (particles per formula unit); m m m = molality (mol solute / kg solvent).
Phase Changes & Heating Curves 🎯
Key Takeaways — Part 4
Endothermic phase changes: melting, vaporization, sublimation (require heat input)
Exothermic phase changes: freezing, condensation, deposition (release heat)
Phase transition temperature: T = Δ H / Δ S T = \Delta H / \Delta S T = Δ H /Δ S (where Δ G = 0 \Delta G = 0 Δ G = 0 )
Heating curve plateaus = phase transitions at constant T; sloped regions = q = m c Δ T q = mc\Delta T q = m c Δ T
Water: c liq = 4.18 c_{\text{liq}} = 4.18 c liq = 4.18 ; c steam = 2.01 c_{\text{steam}} = 2.01 c steam = 2.01 ; J/g·°C;
Phase diagram: triple point (all 3 coexist); critical point (gas/liquid no distinction)
Water's negative solid-liquid slope = unique (ice less dense than liquid water)
S \Delta G = \Delta H - T\Delta S Δ G = Δ H − T Δ S
✅ Δ G ° = − R T ln K = − n F E ° cell \Delta G° = -RT\ln K = -nFE°_{\text{cell}} Δ G ° = − RT ln K = − n FE ° cell
✅ Phase transitions: exothermic going toward solid; endothermic going toward gas ✅ Heating curve: plateaus at phase transitions (q = n Δ H q = n\Delta H q = n Δ H ); slopes = q = m c Δ T q = mc\Delta T q = m c Δ T ✅ Colligative properties: Δ T b = K b m i \Delta T_b = K_b m i Δ T b = K b mi ; Δ T f = K f m i \Delta T_f = K_f m i Δ T f = K f mi ; Π = i M R T \Pi = iMRT Π = i MRT Mixed Thermodynamics — MCAT-Style Questions 🎯
Thermodynamics — Complete Topic Summary
Part 1: Enthalpy, exothermic/endothermic, calorimetry (q = m c Δ T q = mc\Delta T q = m c Δ T ), Hess's Law, standard enthalpies of formation.
Part 2: Entropy, predicting sign ( Δ S ) \text{sign}(\Delta S) sign ( Δ S ) , First/Second/Third Laws, entropy at phase transitions, spontaneity matrix.
Part 3: Gibbs free energy (Δ G = Δ H − T Δ S \Delta G = \Delta H - T\Delta S Δ G = Δ H − T Δ S ), relationship to K e q K_{eq} K e q (Δ G ° = − R T ln K \Delta G° = -RT\ln K Δ G ° = − RT ln K ), relationship to cell potential (Δ G ° = − n F E ° \Delta G° = -nFE° Δ G ° = − n FE ° ), coupled reactions.
Part 4: Phase changes (endo/exothermic), heating curves, specific heats of water, phase diagrams, triple point, critical point, colligative properties review.
Part 5: Integrated MCAT practice.
Most Tested MCAT Thermodynamics Concepts
Δ G = 0 \Delta G = 0 Δ G = 0 at equilibrium or phase transition temperature
Δ G ° , K , E ° cell \Delta G°, K, E°_{\text{cell}} Δ G ° , K , E ° cell are all related: − n F
c ice = 2.09 c_{\text{ice}} = 2.09 c ice = 2.09
Δ H vap ≫ Δ H fus \Delta H_{\text{vap}} \gg \Delta H_{\text{fus}} Δ H vap ≫ Δ H fus E ° = Δ G ° = − R T ln K -nFE° = \Delta G° = -RT\ln K − n FE ° = Δ G ° = − RT ln K
Spontaneous at all T: when Δ H < 0 \Delta H < 0 Δ H < 0 and Δ S > 0 \Delta S > 0 Δ S > 0
Heating curve plateaus — never confuse with temperature changes Phase transition: T transition = Δ H / Δ S T_{\text{transition}} = \Delta H/\Delta S T transition = Δ H /Δ S
Colligative properties depend on number of particles, not identity