myclass24
myclass24your class. your pace.
NCERT SOLUTIONS

Chapter 6: Thermodynamics

Get NCERT Solutions for Class 11 Chemistry Chapter 6. Learn energy changes, enthalpy, work, heat, and thermodynamic laws.

read this first

NCERT Solutions for Class 11 Chemistry Chapter 6: Thermodynamics

Chapter 6 of Class 11 Chemistry, Thermodynamics, deals with one of the most profound subjects in science — the study of energy and how it transforms. Every reaction in chemistry, every process in biology, every engine in engineering is governed by the laws of thermodynamics. Yet for many Class 11 students, this chapter feels abstract and difficult. The NCERT solutions on Myclass24 are specifically designed to change that. Each concept — from internal energy and enthalpy to entropy and Gibbs free energy — is explained clearly with worked examples and connections to real chemistry. 

You will not just learn that ΔG = ΔH − TΔS; you will understand what it means for a reaction to be spontaneous, and under what conditions endothermic reactions can still occur naturally. The chapter also covers the laws of thermodynamics, standard enthalpy of various processes, Hess's Law of constant heat summation, and Kirchhoff's equation. Students preparing for CBSE boards, JEE, or NEET will find thermodynamics questions to be among the most formula-intensive — but with the right preparation, they are also among the most scoring. The NCERT solutions at Myclass24 are updated to match the current NCERT syllabus and are accessible 24/7 from anywhere in India, whether you are in Varanasi, Coimbatore, Amritsar, or Ranchi.

Download PDF: NCERT Solutions for Class 11 Chemistry Chapter 6 Thermodynamics

NCERT Solutions — Class 11 Chemistry Chapter 6: Thermodynamics

Enthalpy calculations, Hess's Law, Gibbs energy, spontaneity criteria | Free PDF on Myclass24

Chapter 6 Detailed Notes: Thermodynamics Laws, Enthalpy & Spontaneity

Basic Terminology in Thermodynamics
Before diving into laws, it is important to be clear about the vocabulary. The system is the part of the universe being studied; everything else is the surroundings. Systems can be open (exchange of energy and matter), closed (only energy exchange), or isolated (no exchange). A process is isothermal if temperature is constant, isobaric if pressure is constant, isochoric if volume is constant, and adiabatic if there is no heat exchange with the surroundings. State functions (like internal energy U, enthalpy H, entropy S) depend only on the current state of the system, not the path taken. One can check out all chapters of NCERT Solutions for Class 11 Chemistry and all subjects of NCERT Solutions for Class 11 from the Myclass24 page. 

First Law of Thermodynamics
The First Law states that energy can neither be created nor destroyed — only converted from one form to another. Mathematically: ΔU = q + w, where ΔU is the change in internal energy, q is heat absorbed by the system, and w is work done on the system. Work done by expansion against constant external pressure: w = −PₑₓₜΔV. At constant volume (isochoric process), no work is done, so ΔU = qᵥ.

ProcessConditionKey Relationship
IsothermalΔT = 0ΔU = 0 (ideal gas); q = −w
Adiabaticq = 0ΔU = w
IsobaricΔP = 0q_p = ΔH
IsochoricΔV = 0w = 0; ΔU = q_v

Enthalpy (H) and Thermochemistry
Enthalpy is defined as H = U + PV. At constant pressure: ΔH = ΔU + PΔV. Since most reactions in chemistry occur at constant (atmospheric) pressure, ΔH is the heat exchanged. If ΔH is negative, the reaction is exothermic (releases heat); if positive, it is endothermic (absorbs heat). The relationship between ΔH and ΔU is: ΔH = ΔU + Δnᵍ × RT, where Δnᵍ is the change in moles of gaseous species.

Type of EnthalpyDefinitionExample
Enthalpy of Formation (ΔH°f)Formation of 1 mol compound from elementsH₂ + ½O₂ → H₂O; ΔH°f = −286 kJ/mol
Enthalpy of Combustion (ΔH°c)Complete combustion of 1 mol substanceCH₄ + 2O₂ → CO₂ + 2H₂O
Enthalpy of NeutralisationNeutralisation of strong acid + strong base≈ −57.1 kJ/mol always
Enthalpy of AtomisationBreaking 1 mol substance into gaseous atomsNa(s) → Na(g); ΔH = 108.4 kJ/mol
Bond EnthalpyEnergy to break 1 mol of bond in gaseous phaseC−H bond ≈ 413 kJ/mol

Hess's Law of Constant Heat Summation
Hess's Law states that the total enthalpy change of a reaction is the same, regardless of whether it occurs in one step or multiple steps. This allows calculation of ΔH for reactions that are difficult to measure directly. It is essentially a consequence of enthalpy being a state function. Using Hess's Law, we can calculate lattice enthalpies (Born-Haber cycle), bond enthalpies, and enthalpy of formation for complex compounds.

Second Law and Entropy
The Second Law states that the total entropy of an isolated system always increases during a spontaneous process. Entropy (S) is a measure of disorder or randomness in a system. ΔS = q_rev / T. For a spontaneous process: ΔS_universe = ΔS_system + ΔS_surroundings > 0. Melting ice, dissolving salt, and expanding gases are all examples of entropy increasing.

Gibbs Free Energy and Spontaneity
Gibbs free energy (G) combines enthalpy and entropy to predict whether a process is spontaneous at a given temperature: ΔG = ΔH − TΔS. A reaction is spontaneous if ΔG < 0, non-spontaneous if ΔG > 0, and at equilibrium if ΔG = 0.

ΔHΔSSpontaneity
Negative (−)Positive (+)Always spontaneous
Negative (−)Negative (−)Spontaneous at low T
Positive (+)Positive (+)Spontaneous at high T
Positive (+)Negative (−)Never spontaneous

Third Law of Thermodynamics: The entropy of a perfect crystal at absolute zero (0 K) is zero. This establishes an absolute scale for entropy.

  • R (gas constant) = 8.314 J mol⁻¹ K⁻¹
  • Standard state: 298 K (25°C) and 1 bar pressure
  • For a reaction: ΔH°rxn = ΣΔH°f (products) − ΣΔH°f (reactants)
  • ΔG° = −RT ln K (connects thermodynamics with equilibrium constant)
Class 11 Chemistry Chapter 6 Thermodynamics Enthalpy Gibbs Energy NCERT Solutions

Content prepared by Myclass24 | NCERT Solutions for Class 11 Chemistry | Updated for latest CBSE syllabus

FAQs for NCERT Solutions Class 11 Chemistry Chapter 6 Thermodynamics