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🎯⭐ INTERACTIVE LESSON

Thermodynamics

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Thermodynamics - Complete Interactive Lesson

Part 1: Enthalpy & Hess's Law

Thermodynamics

Part 1 of 5 — Enthalpy (ΔH\Delta 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: ΔEuniverse=0\Delta E_{\text{universe}} = 0; ΔEsys=−ΔEsurr\Delta E_{\text{sys}} = -\Delta E_{\text{surr}}

Enthalpy (HH)

Enthalpy change ΔH\Delta H = heat transferred at constant pressure.

ΔH=Hproducts−Hreactants\Delta H = H_{\text{products}} - H_{\text{reactants}}

ΔH\Delta HNameEnergy transfer
Negative (ΔH<0\Delta H < 0)ExothermicReleases heat to surroundings
Positive (ΔH>0\Delta H > 0)EndothermicAbsorbs heat from surroundings

Calorimetry at constant pressure:

q=mcΔTq = mc\Delta T

where mm = mass (g), cc = specific heat (J/g·°C), ΔT=Tfinal−Tinitial\Delta T = T_{\text{final}} - T_{\text{initial}}.

For the reaction: ΔHrxn=−qsolution\Delta H_{\text{rxn}} = -q_{\text{solution}} (the sign flip — if the solution warms, the reaction is exothermic)

Standard Enthalpy of Formation (ΔH°f\Delta H°_f)

ΔH°f\Delta H°_f = enthalpy change when 1 mole of a compound is formed from its elements in their standard states.

By convention: ΔH°f=0\Delta H°_f = 0 for pure elements in standard states.

Hess's Law: ΔH°rxn=∑nΔH°f(products)−∑mΔH°f(reactants)\Delta H°_{\text{rxn}} = \sum n \Delta H°_f(\text{products}) - \sum m \Delta H°_f(\text{reactants})

Hess's Law (Path Independence)

Enthalpy is a state function — ΔH\Delta 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:

  1. If a reaction is reversed, flip the sign of ΔH\Delta H
  2. If a reaction is multiplied by a factor, multiply ΔH\Delta H by the same factor

Worked Example

Find ΔH\Delta H for: C(s)+12O2(g)→CO(g)\text{C}(s) + \frac{1}{2}\text{O}_2(g) \to \text{CO}(g)

Given:

  • (1) C(s)+O2(g)→CO2(g)\text{C}(s) + \text{O}_2(g) \to \text{CO}_2(g); ΔH1=−393.5\Delta H_1 = -393.5 kJ
  • (2) CO(g)+12O2(g)→CO2(g)\text{CO}(g) + \frac{1}{2}\text{O}_2(g) \to \text{CO}_2(g); ΔH2=−283.0\Delta H_2 = -283.0 kJ

Reverse reaction (2): CO2(g)→CO(g)+12O2(g)\text{CO}_2(g) \to \text{CO}(g) + \frac{1}{2}\text{O}_2(g); ΔH=+283.0\Delta H = +283.0 kJ

Add to reaction (1):

C(s)+O2+CO2→CO2+CO+12O2\text{C}(s) + \text{O}_2 + \text{CO}_2 \to \text{CO}_2 + \text{CO} + \frac{1}{2}\text{O}_2

C(s)+12O2(g)→CO(g)\text{C}(s) + \frac{1}{2}\text{O}_2(g) \to \text{CO}(g)

ΔH=−393.5+283.0=−110.5 kJ\Delta H = -393.5 + 283.0 = \mathbf{-110.5\text{ kJ}}

Bond Enthalpy Approximation

ΔHrxn≈∑(bonds broken)−∑(bonds formed)\Delta H_{\text{rxn}} \approx \sum (\text{bonds broken}) - \sum (\text{bonds formed})

Breaking bonds requires energy (+); forming bonds releases energy (−). This gives an estimate; less accurate than using ΔH°f\Delta H°_f values.

Enthalpy & Hess's Law 🎯

Key Takeaways — Part 1

  • ΔH<0\Delta H < 0: exothermic (releases heat); ΔH>0\Delta H > 0: endothermic (absorbs heat)
  • Calorimetry: q=mcΔTq = mc\Delta T; ΔHrxn=−qsoln\Delta H_{\text{rxn}} = -q_{\text{soln}}
  • Hess's Law: ΔH\Delta H is a state function; add reactions algebraically
  • Reverse a reaction → flip sign of ΔH\Delta H; multiply by factor → multiply ΔH\Delta H
  • Formation enthalpy: ΔH°rxn=∑nΔH°f(products)−∑mΔH°f(reactants)\Delta H°_{\text{rxn}} = \sum n\Delta H°_f(\text{products}) - \sum m\Delta H°_f(\text{reactants})
  • ΔH°f=0\Delta H°_f = 0 for elements in standard states

Part 2: Entropy & Laws of Thermodynamics

Thermodynamics

Part 2 of 5 — Entropy (ΔS\Delta S), Spontaneity & the Laws of Thermodynamics

Entropy (SS)

Entropy is a measure of disorder or randomness of a system.

ΔS=Sproducts−Sreactants\Delta S = S_{\text{products}} - S_{\text{reactants}}

ΔS\Delta SMeaning
Positive (ΔS>0\Delta S > 0)Increased disorder
Negative (ΔS<0\Delta S < 0)Decreased disorder

Predicting the Sign of ΔS\Delta S

ΔS>0\Delta S > 0 (entropy increases) when:

  1. Gases are produced from solids/liquids (Δngas>0\Delta n_{\text{gas}} > 0)
  2. A solid dissolves to form aqueous ions
  3. Temperature increases (for any substance)
  4. A substance vaporizes or melts
  5. Mixing occurs
  6. Gas occupies larger volume

ΔS<0\Delta S < 0 (entropy decreases) when:

  1. Gases are consumed (Δngas<0\Delta n_{\text{gas}} < 0, e.g., 3 mol gas → 1 mol gas)
  2. A substance crystallizes/freezes
  3. 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. ΔEuniverse=0\Delta E_{\text{universe}} = 0.

ΔU=q+w(internal energy=heat+work)\Delta U = q + w \quad (\text{internal energy} = \text{heat} + \text{work})

where w=−PΔVw = -P\Delta V for expansion/compression work.

Second Law: The entropy of the universe always increases for spontaneous processes.

ΔSuniverse=ΔSsys+ΔSsurr>0(spontaneous)\Delta S_{\text{universe}} = \Delta S_{\text{sys}} + \Delta S_{\text{surr}} > 0 \quad (\text{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°>0S° > 0 for all pure substances (third law). More complex molecules have higher S°S° values.

ΔS°rxn=∑nS°(products)−∑mS°(reactants)\Delta S°_{\text{rxn}} = \sum n S°(\text{products}) - \sum m S°(\text{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 (ΔH<0\Delta H < 0) tend to be spontaneous — enthalpy drives spontaneity
  • Disorder increasing (ΔS>0\Delta S > 0) tends to be spontaneous — entropy drives spontaneity
  • But both factors matter — see Gibbs free energy (Part 3)
ΔH\Delta HΔS\Delta SSpontaneous?
−+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: ΔSuniverse>0\Delta S_{\text{universe}} > 0 for all spontaneous processes
  • Third Law: S=0S = 0 for perfect crystal at 0 K; all S°>0S° > 0 at room temperature
  • Spontaneous ≠ fast; thermodynamics says nothing about how quickly a reaction occurs
  • ΔH<0\Delta H < 0 favors spontaneity; ΔS>0\Delta S > 0 favors spontaneity; temperature controls the trade-off

Part 3: Gibbs Free Energy, Keq & Cell Potential

Thermodynamics

Part 3 of 5 — Gibbs Free Energy, KeqK_{eq} & Cell Potential

Gibbs Free Energy (GG)

ΔG=ΔH−TΔS\Delta G = \Delta H - T\Delta S

ΔG\Delta G combines both enthalpy and entropy to predict spontaneity:

ΔG\Delta GProcess
ΔG<0\Delta G < 0Spontaneous (thermodynamically favorable)
ΔG=0\Delta G = 0At equilibrium
ΔG>0\Delta G > 0Non-spontaneous (requires energy input)

Temperature governs which effect wins when ΔH\Delta H and ΔS\Delta S have the same sign.

Standard Gibbs Free Energy (ΔG°\Delta G°)

ΔG°=ΔH°−TΔS°\Delta G° = \Delta H° - T\Delta S°

Also calculable from formation values: ΔG°=∑nΔG°f(products)−∑mΔG°f(reactants)\Delta G° = \sum n\Delta G°_f(\text{products}) - \sum m\Delta G°_f(\text{reactants})

Relationship Between ΔG°\Delta G° and KeqK_{eq}

ΔG°=−RTln⁡K\Delta G° = -RT\ln K

where R=8.314R = 8.314 J/mol·K, TT in Kelvin.

ΔG°\Delta G°KKMeaning
<0< 0K>1K > 1Products favored at equilibrium
=0= 0K=1K = 1Reactants and products roughly equal
>0> 0K<1K < 1Reactants favored at equilibrium

Large negative ΔG°\Delta G° → large KK → reaction runs nearly to completion.

Relationship to Cell Potential (E°cellE° _{\text{cell}})

For electrochemical reactions:

ΔG°=−nFE°cell\Delta G° = -nFE°_{\text{cell}}

where:

  • nn = moles of electrons transferred
  • F=96,485F = 96{,}485 C/mol (Faraday constant)
  • E°cellE°_{\text{cell}} measured in volts (V)

Connection between ΔG°\Delta G°, KK, and E°cellE°_{\text{cell}}:

ΔG°=−RTln⁡K=−nFE°cell\Delta G° = -RT\ln K = -nFE°_{\text{cell}}

Sign of E°cellE°_{\text{cell}}ΔG°\Delta G°Spontaneous?
E°cell>0E°_{\text{cell}} > 0NegativeYes
E°cell<0E°_{\text{cell}} < 0PositiveNo
E°cell=0E°_{\text{cell}} = 0ZeroAt equilibrium

ΔG\Delta G at Non-Standard Conditions

When the system is not at standard conditions:

ΔG=ΔG°+RTln⁡Q\Delta G = \Delta G° + RT\ln Q

At equilibrium, ΔG=0\Delta G = 0 and Q=KQ = K, which yields ΔG°=−RTln⁡K\Delta G° = -RT\ln K (as above).

Coupled Reactions

In biochemistry, non-spontaneous reactions are driven by coupling with spontaneous ones:

Example: Glucose phosphorylation (ΔG°=+13.8\Delta G° = +13.8 kJ) is coupled with ATP hydrolysis (ΔG°=−30.5\Delta G° = -30.5 kJ):

ΔG°total=13.8+(−30.5)=−16.7 kJ(spontaneous)\Delta G°_{\text{total}} = 13.8 + (-30.5) = -16.7\text{ kJ} \quad \text{(spontaneous)}

This is how cells use ATP to drive energetically unfavorable biochemical reactions.

Gibbs Free Energy, KeqK_{eq} & E°cellE°_{\text{cell}} 🎯

Key Takeaways — Part 3

  • ΔG=ΔH−TΔS\Delta G = \Delta H - T\Delta S: negative ΔG\Delta G = spontaneous
  • ΔG°=−RTln⁡K\Delta G° = -RT\ln K: negative ΔG°\Delta G° → K>1K > 1 (products favored)
  • ΔG°=−nFE°cell\Delta G° = -nFE°_{\text{cell}}: positive E°cellE°_{\text{cell}} → negative ΔG°\Delta G° → spontaneous galvanic cell
  • At equilibrium: ΔG=0\Delta G = 0, Q=KQ = K
  • Non-standard conditions: ΔG=ΔG°+RTln⁡Q\Delta G = \Delta G° + RT\ln Q
  • Coupled reactions: add ΔG°\Delta G° values; ATP hydrolysis drives non-spontaneous biochemical reactions
  • The ΔG\Delta G, KK, and E°cellE°_{\text{cell}} are all interconnected — if you know one, you can find the others

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:

TransitionDirectionΔH\Delta HΔS\Delta S
Fusion (melting)solid → liquid+ (endothermic)+
Freezingliquid → solid− (exothermic)−
Vaporizationliquid → gas+ (endothermic)+
Condensationgas → liquid− (exothermic)−
Sublimationsolid → gas+ (endothermic)+
Depositiongas → solid− (exothermic)−

At the phase transition temperature (e.g., boiling point), ΔG=0\Delta G = 0:

ΔG=ΔH−TΔS=0⇒Ttransition=ΔHΔS\Delta G = \Delta H - T\Delta S = 0 \Rightarrow T_{\text{transition}} = \frac{\Delta H}{\Delta S}

Heating Curves

A heating curve shows temperature vs. heat added for a substance.

Key features:

  1. Slanted region: Temperature rises; q=mcΔTq = mc\Delta T; specific heat governs slope
  2. Flat region (plateau): Phase change at constant T; q=nΔHfusq = n\Delta H_{\text{fus}} or q=nΔHvapq = n\Delta H_{\text{vap}}
  3. Steeper slope = lower specific heat; gentle slope = higher specific heat

Specific heats to know (MCAT):

  • Water (liquid): 4.184.18 J/g·°C (highest of common substances)
  • Steam: 2.012.01 J/g·°C
  • Ice: 2.092.09 J/g·°C
  • ΔHfus\Delta H_{\text{fus}}(water) = 6.016.01 kJ/mol
  • ΔHvap\Delta H_{\text{vap}}(water) = 40.740.7 kJ/mol

Example calculation: Heat to convert 18.0 g (1.00 mol) of ice at −10°C to steam at 110°C:

  1. Heat ice: 18.0×2.09×10=376.218.0 \times 2.09 \times 10 = 376.2 J
  2. Melt ice: 1.00×6010=60101.00 \times 6010 = 6010 J
  3. Heat water: 18.0×4.18×100=752418.0 \times 4.18 \times 100 = 7524 J
  4. Boil water: 1.00×40,700=40,7001.00 \times 40{,}700 = 40{,}700 J
  5. Heat steam: 18.0×2.01×10=361.818.0 \times 2.01 \times 10 = 361.8 J

Total = 376.2+6010+7524+40,700+361.8≈54,972 J≈55.0 kJ376.2 + 6010 + 7524 + 40{,}700 + 361.8 \approx \mathbf{54{,}972\text{ J} \approx 55.0\text{ kJ}}

Phase Diagrams

A phase diagram plots pressure vs. temperature; shows stable phase regions divided by boundary curves.

Point/LineMeaning
Triple pointAll three phases coexist
Critical pointGas and liquid become indistinguishable
Solid-liquid lineMelting points at various pressures
Liquid-gas lineBoiling 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.

PropertyFormulaKey notes
Boiling point elevationΔTb=Kbmi\Delta T_b = K_b m iHigher BP than solvent
Freezing point depressionΔTf=Kfmi\Delta T_f = K_f m iLower FP than solvent
Osmotic pressureΠ=iMRT\Pi = iMRTR=0.0821R = 0.0821 L·atm/mol·K
Vapor pressure loweringΔP=χsoluteP°solvent\Delta P = \chi_{\text{solute}} P°_\text{solvent}Raoult's law

ii = van 't Hoff factor (particles per formula unit); mm = 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=ΔH/ΔST = \Delta H / \Delta S (where ΔG=0\Delta G = 0)
  • Heating curve plateaus = phase transitions at constant T; sloped regions = q=mcΔTq = mc\Delta T
  • Water: cliq=4.18c_{\text{liq}} = 4.18; csteam=2.01c_{\text{steam}} = 2.01; cice=2.09c_{\text{ice}} = 2.09 J/g·°C; ΔHvap≫ΔHfus\Delta H_{\text{vap}} \gg \Delta H_{\text{fus}}
  • 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)

Part 5: Mixed MCAT Review

Thermodynamics

Part 5 of 5 — Mixed MCAT Review

High-Yield Checklist

  • ✅ ΔH\Delta H: exothermic (−) releases heat; endothermic (+) absorbs heat
  • ✅ Hess's Law: ΔH\Delta H is a state function; add reactions algebraically
  • ✅ ΔS>0\Delta S > 0: more disorder (gas formed, dissolution, mixing, heating)
  • ✅ ΔG=ΔH−TΔS\Delta G = \Delta H - T\Delta S: negative = spontaneous
  • ✅ ΔG°=−RTln⁡K=−nFE°cell\Delta G° = -RT\ln K = -nFE°_{\text{cell}}
  • ✅ Phase transitions: exothermic going toward solid; endothermic going toward gas
  • ✅ Heating curve: plateaus at phase transitions (q=nΔHq = n\Delta H); slopes = q=mcΔTq = mc\Delta T
  • ✅ Colligative properties: ΔTb=Kbmi\Delta T_b = K_b m i; ΔTf=Kfmi\Delta T_f = K_f m i; Π=iMRT\Pi = iMRT

Mixed Thermodynamics — MCAT-Style Questions 🎯

Thermodynamics — Complete Topic Summary

Part 1: Enthalpy, exothermic/endothermic, calorimetry (q=mcΔTq = mc\Delta T), Hess's Law, standard enthalpies of formation.

Part 2: Entropy, predicting sign(ΔS)\text{sign}(\Delta S), First/Second/Third Laws, entropy at phase transitions, spontaneity matrix.

Part 3: Gibbs free energy (ΔG=ΔH−TΔS\Delta G = \Delta H - T\Delta S), relationship to KeqK_{eq} (ΔG°=−RTln⁡K\Delta G° = -RT\ln K), relationship to cell potential (ΔG°=−nFE°\Delta G° = -nFE°), 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

  1. ΔG=0\Delta G = 0 at equilibrium or phase transition temperature
  2. ΔG°,K,E°cell\Delta G°, K, E°_{\text{cell}} are all related: −nFE°=ΔG°=−RTln⁡K-nFE° = \Delta G° = -RT\ln K
  3. Spontaneous at all T: when ΔH<0\Delta H < 0 and ΔS>0\Delta S > 0
  4. Heating curve plateaus — never confuse with temperature changes
  5. Phase transition: Ttransition=ΔH/ΔST_{\text{transition}} = \Delta H/\Delta S
  6. Colligative properties depend on number of particles, not identity