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CBSE 13 min read23 October 2026

CBSE Class 11 Chemistry Formulas and Equations Chapter Wise 2027 — Complete List

All CBSE Class 11 Chemistry formulas organized by chapter: Some Basic Concepts, Atomic Structure, Chemical Bonding, States of Matter, Thermodynamics, Equilibrium, Redox, s-Block, p-Block, Hydrocarbons. Every formula with units and context.

In short: Class 11 Chemistry is the foundation year — every formula you learn here carries into Class 12, competitive exams like JEE and NEET, and even college chemistry. This post covers every important formula and equation organized by NCERT chapter: from mole concept to hydrocarbons. Physical Chemistry chapters (1–7) are formula-heavy; Organic and Inorganic chapters rely more on reactions and trends. Bookmark this for daily 15-minute revision sessions.

Chapter 1: Some Basic Concepts of Chemistry

FormulaExpressionUse
Mole concept1 mole = 6.022 × 10²³ particles (Avogadro's number, Nₐ)Converting between particles and moles
Molar massM = mass of 1 mole of substance (g/mol)Relating mass to moles
Number of molesn = given mass / molar mass = W/MCore calculation
Number of particlesN = n × Nₐ = (W/M) × 6.022 × 10²³Finding atoms/molecules from mass
MolarityM = moles of solute / volume of solution in litresSolution concentration
Molalitym = moles of solute / mass of solvent in kgTemperature-independent concentration
Mole fractionxₐ = nₐ/(nₐ + n_b)Composition of mixtures
Mass percentage(mass of solute / mass of solution) × 100Percentage concentration
Empirical formulaSimplest whole-number ratio of atomsFrom percentage composition
Molecular formulan × empirical formula (n = molecular mass / empirical formula mass)Actual formula of compound
Limiting reagentReagent that produces the least amount of productStoichiometry problems
Percentage yield(actual yield / theoretical yield) × 100Efficiency of reaction

Mole concept is tested in every exam. For a broader study approach, see how to study chemistry: organic, inorganic, physical.


Chapter 2: Structure of Atom

FormulaExpressionNotes
Atomic numberZ = number of protonsDefines the element
Mass numberA = protons + neutronsIsotopes differ in A
Wavelength-frequencyc = νλc = 3 × 10⁸ m/s
Energy of photonE = hν = hc/λh = 6.626 × 10⁻³⁴ J·s
Photoelectric effecthν = φ + ½mv²φ = work function
De Broglie wavelengthλ = h/mv = h/pWave-particle duality
Heisenberg uncertaintyΔx × Δp ≥ h/4πCannot know both x and p precisely
Bohr's radiusrₙ = 0.529 × n²/Z ÅHydrogen-like atoms
Bohr's energyEₙ = −13.6 × Z²/n² eVNegative = bound state
Bohr's velocityvₙ = 2.18 × 10⁶ × Z/n m/sSpeed of electron
Wave numberν̄ = 1/λ = Rₕ[1/n₁² − 1/n₂²]Rₕ = 1.097 × 10⁷ m⁻¹
Quantum numbersn (principal), l (azimuthal, 0 to n−1), mₗ (magnetic, −l to +l), mₛ (spin, ±½)Electron address
Max electrons in shell2n²n=1→2, n=2→8, n=3→18
Max electrons in subshell2(2l+1)s→2, p→6, d→10, f→14

Chapter 3: Classification of Elements and Periodicity in Properties

This chapter is trend-based rather than formula-based. Key quantitative relationships:

PropertyTrend Along Period (→)Trend Down Group (↓)
Atomic radiusDecreasesIncreases
Ionization enthalpyIncreasesDecreases
Electron gain enthalpyBecomes more negative (generally)Becomes less negative
ElectronegativityIncreasesDecreases
Metallic characterDecreasesIncreases
Non-metallic characterIncreasesDecreases

Key formulas:

  • IE₁ < IE₂ < IE₃ (successive ionization enthalpies increase)
  • Electronegativity (Pauling scale): difference determines bond polarity

Chapter 4: Chemical Bonding and Molecular Structure

ConceptFormula / RuleNotes
Formal chargeFC = valence electrons − non-bonding electrons − ½(bonding electrons)Determines best Lewis structure
Bond orderBO = (bonding electrons − antibonding electrons)/2Higher BO = stronger bond
Dipole momentμ = q × d (charge × distance)Unit: Debye (D)
% ionic character(observed μ / calculated μ for 100% ionic) × 100Fajan's rules
Hybridization½[V + M − C + A]V=valence electrons, M=monovalent atoms, C=cation charge, A=anion charge
sp hybridization2 electron pairs → linear (180°)BeCl₂, C₂H₂
sp² hybridization3 electron pairs → trigonal planar (120°)BF₃, C₂H₄
sp³ hybridization4 electron pairs → tetrahedral (109.5°)CH₄, NH₃ (107°), H₂O (104.5°)

Chapter 5: States of Matter

Gas Laws

LawFormulaCondition
Boyle's LawP₁V₁ = P₂V₂Constant T and n
Charles's LawV₁/T₁ = V₂/T₂Constant P and n
Gay-Lussac's LawP₁/T₁ = P₂/T₂Constant V and n
Avogadro's LawV ∝ nConstant T and P
Ideal Gas EquationPV = nRTR = 8.314 J/(mol·K) = 0.0821 L·atm/(mol·K)
Combined Gas LawP₁V₁/T₁ = P₂V₂/T₂Constant n
Dalton's LawP_total = p₁ + p₂ + p₃ + ...Partial pressures
Partial pressurepᵢ = xᵢ × P_totalxᵢ = mole fraction
Graham's Lawr₁/r₂ = √(M₂/M₁)Rate of diffusion
Kinetic energyKE = (3/2)kT per molecule = (3/2)RT per molek = R/Nₐ
Root mean square speedu_rms = √(3RT/M)M in kg/mol
Average speedu_avg = √(8RT/πM)
Most probable speedu_mp = √(2RT/M)u_mp < u_avg < u_rms
Van der Waals equation(P + an²/V²)(V − nb) = nRTa = intermolecular forces, b = volume correction
Compressibility factorZ = PV/nRTZ = 1 for ideal gas

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Chapter 6: Thermodynamics

FormulaExpressionNotes
First LawΔU = q + wq = heat, w = work
Work (expansion)w = −P_ext × ΔV (irreversible); w = −nRT ln(V₂/V₁) (reversible isothermal)Negative w = work done BY system
EnthalpyH = U + PV; ΔH = ΔU + ΔnₘRTΔnₘ = moles of gaseous products − reactants
Heat capacityq = nCΔT; Cp − Cv = RCp = constant pressure, Cv = constant volume
Hess's LawΔH_reaction = Σ ΔH_f(products) − Σ ΔH_f(reactants)Enthalpy is a state function
Bond enthalpyΔH = Σ bond enthalpies (reactants) − Σ bond enthalpies (products)Breaking bonds is endothermic
Lattice enthalpyBorn-Haber cycleRelates lattice energy to measurable quantities
EntropyΔS = q_rev/TMeasure of disorder
Gibbs free energyΔG = ΔH − TΔSΔG < 0 → spontaneous
Gibbs criteriaΔG < 0 → spontaneous; ΔG = 0 → equilibrium; ΔG > 0 → non-spontaneous
Equilibrium temperatureT = ΔH/ΔS (when ΔG = 0)At this T, reaction is at equilibrium

Chapter 7: Equilibrium

Chemical Equilibrium

FormulaExpressionNotes
Equilibrium constant (Kc)Kc = [products]ⁿ/[reactants]ᵐConcentrations at equilibrium
Equilibrium constant (Kp)Kp = (partial pressures of products)/(partial pressures of reactants)For gaseous reactions
Relation Kp and KcKp = Kc(RT)^ΔnΔn = gaseous product moles − gaseous reactant moles
Reaction quotientQ = same form as K but with any concentrationsQ < K → forward; Q > K → backward
ΔG° and KΔG° = −RT ln KLinks thermodynamics to equilibrium
Le Chatelier's PrincipleSystem shifts to oppose the changeQualitative — no formula

Ionic Equilibrium

FormulaExpression
Degree of dissociationα = dissociated amount / initial amount
Ostwald dilution lawKa = Cα² / (1−α) ≈ Cα² (for weak electrolyte)
pHpH = −log[H⁺]
pOHpOH = −log[OH⁻]
RelationpH + pOH = 14 (at 25°C)
Ionic product of waterKw = [H⁺][OH⁻] = 10⁻¹⁴ at 25°C
Henderson-HasselbalchpH = pKa + log([salt]/[acid]); pOH = pKb + log([salt]/[base])
Buffer capacityRatio [salt]/[acid] determines buffering range
Solubility productKsp = [cation]ᵐ[anion]ⁿ (for MₘAₙ)
Common ion effectAddition of common ion suppresses dissociation

Chapter 8: Redox Reactions

ConceptFormula / Rule
Oxidation number rulesFree element = 0; monoatomic ion = charge; H = +1 (except metal hydrides = −1); O = −2 (except peroxides = −1, OF₂ = +2)
Balancing by oxidation numberIdentify oxidation and reduction half-reactions; balance electrons transferred
Balancing by half-reaction (ion-electron)Balance atoms, then charge using e⁻, then combine
n-factor (equivalent concept)For acid: basicity; for base: acidity; for redox: electrons transferred per molecule

Chapter 9: Hydrogen

Key reactions (not formula-heavy):

  • Electrolysis of water: 2H₂O → 2H₂ + O₂
  • H₂ + Cl₂ → 2HCl (in presence of light)
  • Water hardness: Ca(HCO₃)₂ → CaCO₃ + H₂O + CO₂ (temporary, on boiling)

Chapters 10–11: s-Block and p-Block Elements

These chapters focus on reactions and trends, not formulas. Key quantitative:

PropertyFormula
Diagonal relationshipLi ~ Mg, Be ~ Al, B ~ Si
Solubility trend (s-block hydroxides)Increases down the group
Solubility trend (s-block carbonates)Decreases down the group (Group 2)
Thermal stability of carbonatesIncreases down the group

Chapter 12: Organic Chemistry — Some Basic Principles

ConceptFormula / Rule
Degree of unsaturation (DBE)DBE = (2C + 2 + N − H − X)/2
Homologous seriesCₙH₂ₙ₊₂ (alkanes), CₙH₂ₙ (alkenes/cycloalkanes), CₙH₂ₙ₋₂ (alkynes)
IUPAC namingLongest chain + substituent positions + functional group suffix
Inductive effect (+I, −I)Through sigma bonds; decreases with distance
Electromeric effect (+E, −E)Temporary shift of π electrons under influence of attacking reagent
HyperconjugationNo-bond resonance; stability: 3° > 2° > 1° carbocation

Chapter 13: Hydrocarbons

Reaction TypeGeneral EquationConditions
Combustion (alkanes)CₙH₂ₙ₊₂ + (3n+1)/2 O₂ → nCO₂ + (n+1)H₂OComplete combustion
Halogenation (alkanes)CH₄ + Cl₂ → CH₃Cl + HClUV light, free radical mechanism
Addition of H₂ to alkenesCₙH₂ₙ + H₂ → CₙH₂ₙ₊₂Ni/Pt/Pd catalyst
Addition of HBr (Markovnikov)CH₃CH=CH₂ + HBr → CH₃CHBrCH₃Ionic addition, H to C with more H
Anti-Markovnikov (Peroxide effect)CH₃CH=CH₂ + HBr → CH₃CH₂CH₂BrPeroxide (ROOR), only with HBr
Ozonolysis (alkenes)R₁R₂C=CR₃R₄ → R₁R₂C=O + R₃R₄C=OO₃ then Zn/H₂O
Addition to alkynesHC≡CH + 2H₂ → CH₃CH₃Ni catalyst
Lindlar's catalyst (partial)HC≡CH + H₂ → CH₂=CH₂ (cis)Pd/BaSO₄ with quinoline (poisoned)
Birch reductionC₆H₆ + Na/liquid NH₃ + alcohol → 1,4-cyclohexadienePartial reduction of benzene

Quick Summary — Formula Count by Chapter

ChapterApprox. FormulasPriority
Some Basic Concepts12🔴 High
Atomic Structure14🔴 High
Chemical Bonding8🟡 Medium
States of Matter15🔴 High
Thermodynamics12🔴 High
Equilibrium14🔴 High
Redox4🟢 Low
s-Block & p-BlockReactions only🟡 Medium
Organic Principles6🟡 Medium
HydrocarbonsReactions🟡 Medium

For strategic study ordering, see the how to study smart not hard guide.


Frequently Asked Questions

How many formulas are there in CBSE Class 11 Chemistry?

There are approximately 85–90 important formulas and equations across all chapters. The most formula-dense chapters are States of Matter (15), Atomic Structure (14), Equilibrium (14), Thermodynamics (12), and Some Basic Concepts (12). Organic Chemistry chapters have more reactions than formulas.

Should I memorize all formulas or understand the derivations?

For Class 11, understanding is more important than memorization because these formulas appear again in Class 12 and competitive exams. That said, you must be able to recall and apply them quickly. The best approach: understand once, then practice 10 numericals per formula to make recall automatic.

Which Class 11 Chemistry formulas are most important for JEE/NEET?

The ideal gas equation (PV = nRT), Gibbs free energy (ΔG = ΔH − TΔS), Kp-Kc relationship, Bohr model equations, and the mole concept formulas are tested heavily in both JEE and NEET. Every single formula from Thermodynamics and Equilibrium appears in entrance exams.

Is Class 11 Chemistry harder than Class 12?

The formula density is similar, but Class 11 introduces many concepts from scratch (mole concept, atomic orbitals, thermodynamic laws) whereas Class 12 builds on them. Students who struggle in Class 11 often find Class 12 easier because the foundation is set. Build that foundation strong using these formulas.

How do I revise all Class 11 Chemistry formulas before the exam?

Spend 15 minutes daily: Day 1 — Chapter 1–2, Day 2 — Chapter 3–4, Day 3 — Chapter 5–6, Day 4 — Chapter 7, Day 5 — Chapters 8–11, Day 6 — Chapters 12–13, Day 7 — full formula test from memory. Repeat this 7-day cycle until the exam.

Are there any differences between CBSE and JEE syllabus for Class 11 Chemistry?

The NCERT syllabus is the base for both. JEE goes deeper in certain topics — more complex equilibrium problems, advanced thermodynamics calculations, and additional organic reaction mechanisms. But every CBSE formula listed here is also relevant for JEE Main.


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