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

  • 1Compare Thomson, Rutherford, and Bohr atomic models and their limitations
  • 2Apply Bohr's energy and radius formulas and the Rydberg equation for spectral lines
  • 3Explain dual nature of matter (de Broglie) and the Heisenberg uncertainty principle
  • 4Assign the four quantum numbers and describe orbital shapes and nodes
  • 5Write electronic configurations using Aufbau, Pauli, and Hund's rules, including the Cr and Cu exceptions
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Why this chapter matters
This chapter takes you inside the atom -- from Dalton's sphere to the quantum mechanical model. The evolution of atomic models, Bohr's theory, wave-particle duality, quantum numbers, orbitals, and electronic configurations underpin the periodic table and chemical bonding, and are heavily tested in JEE and NEET.

Before you start — revise these

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

Structure of Atom

'The atom is the basic building block of matter. But inside the atom lies a strange and fascinating world.' — Quantum Physics

1. Chapter Overview

This chapter takes you INSIDE the atom — beyond Dalton's indivisible sphere to the world of PROTONS, NEUTRONS, ELECTRONS, and the QUANTUM MECHANICAL model. You will study the EVOLUTION of atomic models (Thomson, Rutherford, Bohr), the WAVE-PARTICLE duality of matter, QUANTUM NUMBERS (the 'address' of an electron), ATOMIC ORBITALS, and ELECTRONIC CONFIGURATIONS.


2. Subatomic Particles

ParticleSymbolCharge (C)Mass (kg)Discoverer
Electrone⁻-1.602 × 10⁻¹⁹9.1 × 10⁻³¹J.J. Thomson (1897)
Protonp⁺+1.602 × 10⁻¹⁹1.672 × 10⁻²⁷E. Goldstein (1886)
Neutronn⁰01.675 × 10⁻²⁷J. Chadwick (1932)

Atomic Number and Mass Number

  • Atomic Number (Z) = Number of PROTONS in the nucleus
  • Mass Number (A) = Number of PROTONS + Number of NEUTRONS
  • Isotopes: Same Z, different A (same element, different number of neutrons)

3. Atomic Models — A Historical Journey

Thomson's Model (Plum Pudding Model)

  • Atom as a SPHERE of positive charge with electrons EMBEDDED
  • Failed to explain Rutherford's experimental results

Rutherford's Model (Gold Foil Experiment)

  • Most α-particles passed straight through → atom is EMPTY space
  • Some α-particles were DEFLECTED → small, dense POSITIVE nucleus
  • A few BOUNCED BACK → nucleus is VERY dense
  • Drawbacks: Could not explain STABILITY of atom (electron would spiral into nucleus) or atomic SPECTRA

Bohr's Model (for Hydrogen)

Postulates:

  1. Electrons move in STATIONARY circular orbits (shells) around nucleus
  2. Angular momentum is QUANTIZED: mvr = nh/2π (n = 1, 2, 3...)
  3. Energy is emitted/absorbed ONLY when electron JUMPS between orbits

Bohr's Radius: r_n = n² × a₀ (a₀ = 0.529 Å = Bohr radius for n = 1) Bohr's Energy: E_n = -13.6/n² eV = -2.18×10⁻¹⁸/n² J Spectral Lines: ΔE = hν = E_f — E_i

Worked Problem: Calculate the energy of the n = 3 level in hydrogen. A: E₃ = -13.6/9 = -1.51 eV.


4. Dual Nature of Matter and Radiation

Planck's Quantum Theory

  • Energy is quantised: E = hν (h = 6.626 × 10⁻³⁴ J·s)
  • h = Planck's constant

Photoelectric Effect (Einstein)

  • Light ejects electrons from metal surface
  • KE_max = hν — hν₀ (ν₀ = threshold frequency)
  • Proves particle nature of light (photons)

de Broglie's Hypothesis

  • Matter has wave-like properties
  • λ = h/p = h/mv (de Broglie wavelength)
  • EVERY moving particle has an associated wavelength

Heisenberg's Uncertainty Principle

  • It is IMPOSSIBLE to simultaneously know the EXACT position and EXACT momentum of a particle
  • Δx × Δp ≥ h/4π
  • Fundamental LIMITATION, not a measurement issue

Worked Problem

Q: Find de Broglie wavelength of an electron moving at 2 × 10⁶ m/s. (m = 9.1 × 10⁻³¹ kg) A: λ = h/mv = 6.626×10⁻³⁴/(9.1×10⁻³¹ × 2×10⁶) = 3.64 × 10⁻¹⁰ m = 3.64 Å.


5. Quantum Mechanical Model

Quantum Numbers (The Electron's Address)

Quantum NumberSymbolValuesSignificance
Principaln1, 2, 3...Shell size and ENERGY
Azimuthall0 to n-1Subshell SHAPE (s, p, d, f)
Magneticm_l-l to +lOrbital ORIENTATION
Spinm_s+½ or -½Electron SPIN direction

Shapes of Orbitals

  • s-orbital (l = 0): SPHERICAL
  • p-orbital (l = 1): DUMBBELL shape (p_x, p_y, p_z)
  • d-orbital (l = 2): CLOVERLEAF shape (5 orientations)
  • f-orbital (l = 3): Complex shapes (7 orientations)

Nodes

  • Radial nodes = n — l — 1
  • Angular nodes = l
  • Total nodes = n — 1

6. Electronic Configuration

Filling Order — Aufbau Principle

  • Electrons fill orbitals in INCREASING order of energy
  • Energy order: 1s < 2s < 2p < 3s < 3p < 4s < 3d < 4p < 5s < 4d < 5p < 6s...
  • Mnemonic: (n + l) rule — lower (n + l) fills first

Pauli's Exclusion Principle

  • NO two electrons in an atom can have the SAME set of all four quantum numbers
  • Each orbital can hold MAXIMUM 2 electrons with OPPOSITE spins

Hund's Rule of Maximum Multiplicity

  • Electrons occupy ALL orbitals of a subshell SINGLY before pairing
  • Maximises TOTAL spin (most stable)

Electronic Configurations of Key Elements

ElementZConfiguration
H11s¹
He21s²
C61s² 2s² 2p²
N71s² 2s² 2p³
O81s² 2s² 2p⁴
Na111s² 2s² 2p⁶ 3s¹
Fe261s² 2s² 2p⁶ 3s² 3p⁶ 4s² 3d⁶

Exceptions

  • Cr (Z=24): [Ar] 4s¹ 3d⁵ (NOT 4s² 3d⁴) — HALF-FILLED stability
  • Cu (Z=29): [Ar] 4s¹ 3d¹⁰ (NOT 4s² 3d⁹) — FULLY-FILLED stability

7. Common Mistakes

  1. Bohr's model FAILS for multi-electron atoms: It works well only for H and H-like ions (He⁺, Li²⁺)
  2. 4s fills BEFORE 3d (Aufbau), but 3d has LOWER energy than 4s in actual atoms
  3. Nodes are regions of ZERO probability: Not 'minimum' probability
  4. m_s = ±½, NOT the values +1 and -1: These are for spin, not charge
  5. Heisenberg principle ≠ measurement error: It is a FUNDAMENTAL property of quantum systems

8. CBSE Exam Focus

  1. Bohr's model — radius, energy derivation (5-mark)
  2. de Broglie wavelength numericals (3-mark)
  3. Quantum numbers — writing sets for electrons (3-mark)
  4. Electronic configuration of elements (1/3-mark)
  5. Heisenberg uncertainty principle — numericals (3-mark)
  6. Photoelectric effect numericals

9. Key Formulas

  • E_n = -13.6/n² eV (hydrogen)
  • ΔE = hν = hc/λ
  • λ = h/mv (de Broglie)
  • Δx × Δp ≥ h/4π
  • mvr = nh/2π (Bohr quantisation)
  • R_H = 1.097 × 10⁷ m⁻¹ (Rydberg constant)
  • 1/λ = R_H(1/n₁² — 1/n₂²)

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

Q1: Find the wavelength of the Hα line (transition from n=3 to n=2) in the Balmer series. (R_H = 1.097 × 10⁷ m⁻¹) A: 1/λ = R_H(1/4 — 1/9) = R_H(5/36) = 1.097×10⁷ × 5/36 = 1.524×10⁶ m⁻¹. λ = 656.3 nm.

Q2: Write the four quantum numbers for the 3p¹ electron of aluminium (Z=13). A: Al: 1s² 2s² 2p⁶ 3s² 3p¹. n=3, l=1, m_l can be -1,0,+1 (typically +1), m_s = +½.

Q3: Calculate the uncertainty in position if Δv = 0.001 m/s for an electron (m = 9.1×10⁻³¹ kg). A: Δp = mΔv = 9.1×10⁻³⁴. Δx ≥ h/(4πΔp) = 6.626×10⁻³⁴/(4×3.14×9.1×10⁻³⁴) = 0.058 m.

Q4: State and explain Hund's rule with an example. A: Hund's rule: Electrons fill each orbital singly with parallel spins before pairing. Example: Carbon (1s² 2s² 2p²) — the two 2p electrons go into separate p orbitals with parallel spins.

Q5: Why is Cr's configuration [Ar]4s¹3d⁵ instead of 4s²3d⁴? A: Half-filled d⁵ configuration has EXTRA STABILITY due to exchange energy and symmetry. One electron from 4s promotes to 3d to achieve this stable configuration.


11. Conclusion

The structure of the atom has EVOLVED from Thomson's sphere to the quantum mechanical model. Bohr's model, while limited, introduces the crucial idea of QUANTISATION. The quantum mechanical model, with its orbital concept and quantum numbers, provides a COMPLETE description of electron distribution in atoms. Electronic configuration determines the CHEMICAL PROPERTIES of elements — making this chapter fundamental to understanding the periodic table and chemical bonding.

Key formulas & results

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

Bohr energy levels (hydrogen)
E_n = -13.6/n^2 eV = -2.18 x 10^-18 / n^2 J
Negative sign shows the electron is bound; works only for H and H-like ions.
Rydberg equation
1/lambda = R_H (1/n1^2 - 1/n2^2), R_H = 1.097 x 10^7 m^-1
Gives the wavelengths of hydrogen spectral lines (Lyman, Balmer, etc.).
de Broglie wavelength
lambda = h/mv
Every moving particle has an associated wavelength (wave-particle duality).
Heisenberg uncertainty principle
delta-x x delta-p >= h/4pi
A fundamental limit -- position and momentum cannot both be known exactly.
Nodes
Radial nodes = n - l - 1; Angular nodes = l; Total nodes = n - 1
Nodes are regions of zero probability of finding the electron.
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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
Applying Bohr's model to multi-electron atoms
Bohr's model works only for hydrogen and H-like ions (He+, Li2+); it fails for atoms with more than one electron.
WATCH OUT
Thinking nodes are regions of minimum probability
Nodes are regions of ZERO probability of finding the electron, not minimum probability.
WATCH OUT
Treating the uncertainty principle as a measurement error
It is a fundamental property of quantum systems, not a limitation of our instruments.
WATCH OUT
Writing Cr as [Ar]4s2 3d4
Cr is [Ar]4s1 3d5 and Cu is [Ar]4s1 3d10 due to the extra stability of half-filled and fully-filled d subshells.

Practice problems

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

Q1HARD· Spectra
Find the wavelength of the H-alpha line (n=3 to n=2) in the Balmer series. (R_H = 1.097 x 10^7 m^-1)
Show solution
1/lambda = R_H(1/4 - 1/9) = 1.097x10^7 x 5/36 = 1.524x10^6 m^-1. lambda = 656.3 nm.
Q2MEDIUM· de Broglie
Find the de Broglie wavelength of an electron moving at 2 x 10^6 m/s (m = 9.1 x 10^-31 kg).
Show solution
lambda = h/mv = 6.626x10^-34 / (9.1x10^-31 x 2x10^6) = 3.64 x 10^-10 m = 3.64 Angstrom.
Q3MEDIUM· Quantum Numbers
Write the four quantum numbers for the 3p electron of aluminium (Z=13).
Show solution
Al: 1s2 2s2 2p6 3s2 3p1. For the 3p electron: n=3, l=1, m_l = +1 (any of -1, 0, +1), m_s = +1/2.
Q4HARD· Uncertainty
Calculate the uncertainty in position if the uncertainty in velocity is 0.001 m/s for an electron (m = 9.1 x 10^-31 kg).
Show solution
delta-p = m x delta-v = 9.1x10^-34. delta-x >= h/(4 pi delta-p) = 6.626x10^-34 / (4 x 3.14 x 9.1x10^-34) = 0.058 m.
Q5MEDIUM· Reasoning
Why is chromium's configuration [Ar]4s1 3d5 instead of [Ar]4s2 3d4?
Show solution
A half-filled 3d5 subshell has extra stability due to symmetrical distribution and exchange energy, so one 4s electron shifts to 3d to achieve the more stable half-filled configuration.

5-minute revision

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

  • Subatomic particles: electron (Thomson), proton (Goldstein), neutron (Chadwick).
  • Atomic number Z = protons; mass number A = protons + neutrons; isotopes share Z.
  • Rutherford: atom is mostly empty with a small dense positive nucleus; Bohr added quantised orbits.
  • Bohr: E_n = -13.6/n^2 eV; works only for H and H-like ions.
  • Dual nature: lambda = h/mv (de Broglie); Heisenberg: delta-x x delta-p >= h/4pi.
  • Quantum numbers: n (shell), l (subshell shape), m_l (orientation), m_s (spin).
  • Configurations follow Aufbau, Pauli's exclusion, and Hund's rule; Cr and Cu are exceptions.

CBSE marks blueprint

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

Typical chapter weightage: 8-10 marks across the chapter

Question typeMarks eachTypical countWhat it tests
Bohr model / spectra3-51Energy levels and the Rydberg equation
Dual nature / uncertainty31de Broglie and Heisenberg numericals
Quantum numbers / configurations1-31-2Assigning quantum numbers and writing configurations
Prep strategy
  • Memorise E_n = -13.6/n^2 and the Rydberg equation
  • Practise de Broglie and uncertainty numericals with units
  • Learn the Aufbau order and the (n+l) rule
  • Remember the Cr and Cu exceptions

Where this shows up in the real world

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

Spectroscopy

Atomic spectra (from Bohr's model) let scientists identify elements in stars, flames, and chemical samples.

Electron microscopy

The de Broglie wavelength of electrons enables electron microscopes to image objects far smaller than light can resolve.

Lasers and LEDs

Electron transitions between quantised energy levels are the basis of lasers, LEDs, and fluorescent lighting.

Exam strategy

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

  1. State the formula before substituting in numericals
  2. Keep track of units (eV vs J, m vs Angstrom)
  3. For configurations, use noble-gas shorthand and check the exceptions
  4. Define nodes and quantum numbers precisely

Going beyond the textbook

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

  • Derive Bohr's radius and energy expressions from the quantisation of angular momentum.
  • Investigate the Schrodinger wave equation and the physical meaning of psi-squared (probability density).

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 (Atomic Structure)Very High
NEET ChemistryVery High

Questions students ask

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

By the Aufbau (n+l) rule, 4s (n+l = 4) fills before 3d (n+l = 5) because 4s has lower energy when empty. Once electrons occupy 3d, however, 3d drops below 4s, which is why 4s electrons are removed first during ionisation.

Rutherford's model could not explain the stability of the atom -- according to classical physics, an orbiting electron would continuously radiate energy and spiral into the nucleus. It also could not explain the line spectra of atoms. Bohr's quantised orbits resolved this for hydrogen.
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Last reviewed on 29 May 2026. Written and reviewed by subject-matter experts — read about our process.
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