By the end of this chapter you'll be able to…

  • 1Distinguish system, surroundings, state functions, and path functions
  • 2Apply the first law and relate enthalpy and internal energy (delta-H = delta-U + delta-n_g RT)
  • 3Use Hess's law and bond enthalpies to calculate reaction enthalpies
  • 4Explain entropy and the second and third laws of thermodynamics
  • 5Use Gibbs free energy (delta-G = delta-H - T delta-S) to judge spontaneity
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Why this chapter matters
Chemical thermodynamics predicts whether a reaction will happen and how much heat it involves. Enthalpy, Hess's law, entropy, and Gibbs free energy give the criterion of spontaneity that underlies equilibrium, electrochemistry, and biochemistry.

Before you start — revise these

A 5-minute refresher here will save you 30 minutes of confusion below.

Thermodynamics

'Thermodynamics is the only physical theory of universal content which I am convinced will never be overthrown.' — Albert Einstein

1. Chapter Overview

Chemical THERMODYNAMICS deals with ENERGY CHANGES accompanying chemical reactions. Unlike the Physics thermodynamics chapter (which focuses on heat engines), this chapter focuses on REACTION ENTHALPY, BOND ENERGIES, HESS'S LAW, ENTROPY, GIBBS FREE ENERGY, and the CRITERION OF SPONTANEITY. These concepts tell you WHETHER a reaction will occur and how MUCH heat is involved.


2. Thermodynamic Terms

  • System: The PART of the universe under study
    • Open: exchanges matter AND energy
    • Closed: exchanges energy ONLY
    • Isolated: exchanges NEITHER
  • Surroundings: Everything OUTSIDE the system
  • State Functions: Depend ONLY on the state, NOT the path (P, V, T, U, H, S, G)
  • Path Functions: Depend on the PATH taken (Heat Q, Work W)

3. Internal Energy (U) and Enthalpy (H)

First Law of Thermodynamics

  • ΔU = Q + W (Chemistry convention: W = work done ON the system)
  • ΔU = Q — PΔV (for pressure-volume work only)

Enthalpy Definition

  • H = U + PV (Enthalpy = Internal energy + Pressure-Volume work)
  • ΔH = ΔU + Δn_gRT (at constant P)
  • ΔH = Q_p (heat at constant pressure)
  • ΔU = Q_v (heat at constant volume)

Exothermic vs Endothermic

TypeΔH signHeatExamples
ExothermicNegativeHeat releasedCombustion, respiration
EndothermicPositiveHeat absorbedMelting, decomposition

4. Enthalpy Changes in Reactions

Standard Enthalpy of Reaction (Δ_rH°)

  • Enthalpy change when reaction occurs with ALL substances in their STANDARD states
  • Standard state: 1 bar pressure, pure substance at specified T

Standard Enthalpy of Formation (Δ_fH°)

  • Enthalpy change when ONE MOLE of compound is formed from its ELEMENTS in their standard states
  • Δ_fH° of elements in standard state = 0 (reference)
  • Example: C(s) + O₂(g) → CO₂(g), Δ_fH° = -393.5 kJ/mol

Standard Enthalpy of Combustion (Δ_cH°)

  • Enthalpy change when ONE MOLE of substance is completely burned in oxygen

Bond Enthalpy

  • AVERAGE energy required to break a specific type of bond
  • Δ_rH° = Σ(Bond enthalpies of reactants) — Σ(Bond enthalpies of products)
  • Average values: C—H = 413, C≡C = 839, O=O = 498 kJ/mol

5. Hess's Law of Constant Heat Summation

  • Statement: The total enthalpy change for a reaction is INDEPENDENT of the PATH
  • ΔH for the overall reaction = ΣΔH of individual steps
  • Application: Used to calculate ΔH for reactions that are DIFFICULT to measure directly

Worked Problem

Q: Calculate Δ_fH° of CO using: (1) C + O₂ → CO₂, ΔH₁ = -393.5 kJ; (2) CO + ½O₂ → CO₂, ΔH₂ = -283 kJ. A: Target: C + ½O₂ → CO. ΔH = ΔH₁ — ΔH₂ = -393.5 — (-283) = -110.5 kJ/mol.


6. Entropy (S) and the Second Law

  • Entropy: Measure of RANDOMNESS or DISORDER
  • Second Law: Total entropy of the universe ALWAYS INCREASES for a spontaneous process
  • ΔS_system + ΔS_surroundings > 0 for spontaneous process

Entropy Changes

  • Solids < Liquids < Gases (increasing entropy)
  • S° increases with temperature
  • S° of a PERFECT crystal at 0 K = 0 (Third Law of Thermodynamics)

7. Gibbs Free Energy (G) and Spontaneity

Definition

  • G = H — TS
  • ΔG = ΔH — TΔS

Criterion of Spontaneity

ΔHΔSΔG = ΔH — TΔSResult
-+ALWAYS negativeSpontaneous at ALL T
+-ALWAYS positiveNon-spontaneous at ALL T
--Negative at LOW TSpontaneous at low T
++Negative at HIGH TSpontaneous at high T

Key Points

  • If ΔG < 0: Process is SPONTANEOUS (feasible)
  • If ΔG = 0: System is at EQUILIBRIUM
  • If ΔG > 0: Process is NON-SPONTANEOUS (reverse is spontaneous)

Standard Gibbs Free Energy

  • Δ_rG° = ΣΔ_fG°(products) — ΣΔ_fG°(reactants)
  • Δ_rG° = -RT ln K (K = equilibrium constant)
  • At equilibrium: Δ_rG = 0

Worked Problem

Q: For a reaction, ΔH = 100 kJ and ΔS = 200 J/K. Is it spontaneous at 300 K? A: ΔG = 100 — 0.2 × 300 = 100 — 60 = 40 kJ. ΔG > 0 → NON-SPONTANEOUS at 300 K. At T > 500 K: ΔG becomes negative → spontaneous.


8. Comparison: Physics vs Chemistry Thermodynamics

AspectPhysics (Class 11)Chemistry (Class 11)
FocusHeat engines, efficiencyReaction spontaneity, ΔH
W signΔU = Q — WΔU = Q + W (or Q — PΔV)
Key conceptCarnot efficiencyΔG = ΔH — TΔS
ApplicationsEngine cyclesChemical reactions

9. Common Mistakes

  1. Sign convention confusion: Physics: ΔU = Q — W. Chemistry: ΔU = Q + W (W = work ON system). Be CAREFUL about the convention used
  2. ΔH°_f of elements is ZERO only in standard state: O(g) ≠ O₂(g)! Δ_fH° of O(g) is +249 kJ/mol
  3. Entropy of vaporisation >> entropy of fusion: Gas has much higher disorder than liquid
  4. ΔG < 0 means spontaneous, NOT fast: Thermodynamics tells us FEASIBILITY, not RATE (kinetics)
  5. Hess's law applies because H is a state function: The path doesn't matter, only initial and final states

10. CBSE Exam Focus

  1. Enthalpy, internal energy — relation ΔH = ΔU + ΔnRT (3-mark)
  2. Hess's law numerical problems (5-mark)
  3. Bond enthalpy calculations (3/5-mark)
  4. ΔG, ΔH, ΔS — numerical problems on spontaneity (5-mark)
  5. Standard enthalpy of formation, combustion, neutralisation
  6. Relationship between ΔG° and equilibrium constant

11. Key Formulas

  • ΔU = Q + W = Q — PΔV (at constant P)
  • ΔH = ΔU + Δn_gRT
  • Δ_rH° = ΣΔ_fH°(products) — ΣΔ_fH°(reactants)
  • Δ_rH = Σ(Bond energy)_reactants — Σ(Bond energy)_products
  • ΔG = ΔH — TΔS
  • ΔG° = -RT ln K
  • ΔG = ΔG° + RT ln Q (Q = reaction quotient)

12. Self-Test (5+ Q&A)

Q1: For the reaction N₂ + 3H₂ → 2NH₃, ΔH = -92.4 kJ at 298 K. Find ΔU if Δn_g = -2. A: ΔH = ΔU + Δn_gRT → -92.4 = ΔU + (-2)(8.314×298)/1000 → -92.4 = ΔU — 4.96 → ΔU = -87.44 kJ.

Q2: Calculate Δ_fH° of C₂H₆ given: C(s) + O₂ → CO₂ ΔH = -393.5; H₂ + ½O₂ → H₂O ΔH = -285.8; C₂H₆ + 7/2O₂ → 2CO₂ + 3H₂O ΔH = -1560 kJ. A: Δ_fH°[C₂H₆] = 2(-393.5) + 3(-285.8) — (-1560) = -787 — 857.4 + 1560 = -84.4 kJ/mol.

Q3: For a reaction, ΔH = 30 kJ, ΔS = 100 J/K. Find temperature at which it becomes spontaneous. A: At equilibrium ΔG = 0. T = ΔH/ΔS = 30000/100 = 300 K. Spontaneous ABOVE 300 K (ΔH +, ΔS +).

Q4: Is bond breaking endothermic or exothermic? A: ENDOTHERMIC — energy is absorbed to break bonds. Bond FORMATION is exothermic (energy released).

Q5: What is the significance of ΔG = 0? A: ΔG = 0 means the system is at EQUILIBRIUM. No net change occurs. The forward and reverse rates are equal.


13. Conclusion

Chemical thermodynamics provides TOOLS for predicting reaction feasibility and energy changes. Enthalpy tells us about heat flow; Hess's law allows CALCULATION of otherwise unmeasurable reaction enthalpies. Entropy introduces the DIRECTION of spontaneous change. Gibbs free energy COMBINES enthalpy and entropy into a single SPONTANEITY criterion. These concepts are ESSENTIAL for understanding chemical equilibrium, electrochemistry, and biochemistry.

Key formulas & results

Everything you need to memorise, in one card. Screenshot this for revision.

First law of thermodynamics
delta-U = Q + W = Q - P delta-V
Chemistry convention: W is work done ON the system.
Enthalpy-internal energy relation
delta-H = delta-U + delta-n_g RT
delta-n_g = moles of gaseous products minus reactants.
Hess's law / bond enthalpy
delta-rH = sum(bond energies reactants) - sum(bond energies products)
Reaction enthalpy is path-independent because H is a state function.
Gibbs free energy
delta-G = delta-H - T delta-S; delta-G = -RT ln K
delta-G < 0 spontaneous, = 0 equilibrium, > 0 non-spontaneous.
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Common mistakes & fixes

These are the exact errors that cost students marks in board exams. Read them once, save yourself the trouble.

WATCH OUT
Mixing up the physics and chemistry sign conventions
In chemistry delta-U = Q + W (W done ON the system); in physics delta-U = Q - W. State the convention before solving.
WATCH OUT
Assuming delta-fH of all forms of an element is zero
Only the element in its standard state has delta-fH = 0; delta-fH of O(g) is +249 kJ/mol, not zero.
WATCH OUT
Thinking a spontaneous reaction must be fast
delta-G < 0 means feasible, not fast. Rate is governed by kinetics, not thermodynamics.
WATCH OUT
Forgetting to convert delta-S units
delta-S is usually in J/K while delta-H is in kJ; convert to the same units before computing delta-G.

Practice problems

Try each one yourself before tapping "Show solution". Active recall > rereading.

Q1MEDIUM· Enthalpy
For N2 + 3H2 -> 2NH3, delta-H = -92.4 kJ at 298 K. Find delta-U given delta-n_g = -2.
Show solution
delta-H = delta-U + delta-n_g RT. -92.4 = delta-U + (-2)(8.314 x 298)/1000 = delta-U - 4.96. So delta-U = -87.44 kJ.
Q2HARD· Hess's Law
Calculate delta-fH of C2H6 given delta-cH(C) = -393.5, delta-fH(H2O) = -285.8, and delta-cH(C2H6) = -1560 kJ/mol.
Show solution
delta-fH(C2H6) = 2(-393.5) + 3(-285.8) - (-1560) = -787 - 857.4 + 1560 = -84.4 kJ/mol.
Q3MEDIUM· Spontaneity
For a reaction delta-H = 30 kJ and delta-S = 100 J/K. Find the temperature above which it becomes spontaneous.
Show solution
At equilibrium delta-G = 0, so T = delta-H/delta-S = 30000/100 = 300 K. Since delta-H and delta-S are both positive, the reaction is spontaneous above 300 K.
Q4EASY· Concept
Is bond breaking endothermic or exothermic, and what about bond formation?
Show solution
Bond breaking is endothermic (energy must be supplied); bond formation is exothermic (energy is released).
Q5EASY· Concept
What is the significance of delta-G = 0?
Show solution
delta-G = 0 means the system is at equilibrium -- there is no net change and the forward and reverse rates are equal.

5-minute revision

The whole chapter, distilled. Read this the night before the exam.

  • State functions (U, H, S, G) depend only on state; heat and work are path functions.
  • delta-H = Q_p, delta-U = Q_v, and delta-H = delta-U + delta-n_g RT.
  • Exothermic: delta-H negative; endothermic: delta-H positive.
  • Hess's law: total delta-H is independent of path because H is a state function.
  • Entropy increases solid < liquid < gas; second law: universe entropy rises for spontaneous change.
  • Third law: entropy of a perfect crystal at 0 K is zero.
  • delta-G = delta-H - T delta-S; delta-G < 0 spontaneous, = 0 equilibrium, > 0 non-spontaneous; delta-G = -RT ln K.

CBSE marks blueprint

Where the marks come from in this chapter — so you can plan your prep.

Typical chapter weightage: 7-9 marks across the chapter

Question typeMarks eachTypical countWhat it tests
Hess's law numericals3-51Calculating reaction and formation enthalpies
Gibbs energy / spontaneity3-51delta-G = delta-H - T delta-S and temperature dependence
First law / enthalpy relation2-31delta-H = delta-U + delta-n_g RT
Prep strategy
  • Master the chemistry sign convention for the first law
  • Practise Hess's law and bond-enthalpy calculations
  • Memorise the delta-H/delta-S spontaneity table
  • Always check units before computing delta-G

Where this shows up in the real world

This chapter isn't just an exam topic — it lives in the world around you.

Fuels and energy

Enthalpies of combustion tell engineers how much energy fuels release, guiding fuel choice and engine design.

Industrial processes

Gibbs energy and temperature dependence decide the conditions for processes like the Haber synthesis of ammonia.

Biochemistry

Free-energy changes govern whether metabolic reactions like ATP hydrolysis are spontaneous in living cells.

Exam strategy

Battle-tested tips from teachers and toppers for this chapter.

  1. Write the relevant formula and convention before substituting numbers
  2. Track signs carefully in Hess's law cycles
  3. Convert delta-S to kJ/K when combining with delta-H
  4. State the spontaneity conclusion explicitly from the sign of delta-G

Going beyond the textbook

For olympiad aspirants and curious learners — topics that build on this chapter.

  • Derive the temperature dependence of K from delta-G = -RT ln K and the van't Hoff equation.
  • Explore how coupled reactions drive thermodynamically unfavourable steps in biology.

Where else this chapter is tested

CBSE board isn't the only one — other exams test this chapter too.

CBSE Class 11 Chemistry examHigh
JEE Main and Advanced (Thermodynamics)High
NEET ChemistryHigh

Questions students ask

The real ones — pulled from the Q&A community and tutor sessions.

If delta-H is negative and delta-S positive, delta-G is always negative (spontaneous at all temperatures). If both are positive, the reaction is spontaneous only at high temperature; if both negative, only at low temperature. If delta-H is positive and delta-S negative, it is never spontaneous. The crossover temperature is T = delta-H/delta-S.

Thermodynamics (delta-G) only tells us whether a reaction is feasible, not how fast it goes. A reaction with a large activation energy barrier can have delta-G < 0 yet proceed immeasurably slowly -- for example, the conversion of diamond to graphite. Rate is the domain of chemical kinetics, not thermodynamics.
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