Class 12 Physics Chapter 12 Atoms

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February 23, 2026

One of the most important chapters in Class 12 Physics is Atoms. This chapter explains the structure of atoms, atomic models, quantization of energy, atomic spectra and other key concepts that form the backbone of modern physics.

In these notes, we cover all NCERT topics, formulas and examples in a concise, exam-oriented and student-friendly way. You’ll also find practice questions to strengthen your understanding.

Atoms and Nuclei Class 12 Notes PDF

These notes are perfect for last-minute revision, quick formula recall or full marks prep without stress. Download from below:

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S. No. Headings
1 Structure of the Atom
2 Early Models of the Atom
3 Atomic Spectra
4 Energy Levels and Spectral Series
5 Bohr’s Model and Energy Quantization
6 Dual Nature of Matter (de Broglie Hypothesis)
7 Heisenberg’s Uncertainty Principle

Structure of the Atom

Atoms are the building blocks of matter. Each atom has:

  • A nucleus at the center, containing protons and neutrons.
  • Electrons orbiting the nucleus in energy levels or shells.

The arrangement of electrons determines the chemical and physical properties of the atom.

Subatomic Particles:

Particle Charge Location Role
Proton (p) +1 Nucleus Determines atomic number
Neutron (n) 0 Nucleus Adds stability, determines atomic mass
Electron (e) -1 Orbits Determines chemical behavior, can form ions

Early Models of the Atom

Understanding atoms evolved over time through key models:

a) Thomson’s Model (Plum Pudding, 1897)

  • Atom = positively charged pudding with electrons as plums.
  • Disproved by Rutherford’s experiment.

b) Rutherford’s Model (1911)

  • Gold foil experiment β†’ atom has a dense, positively charged nucleus.
  • Electrons revolve around the nucleus.
  • Most of the atom is empty space.

c) Bohr’s Model (1913)

  • Electrons move in fixed orbits (quantized energy levels).
  • Energy is absorbed or emitted only when electrons jump between levels.

Atomic Spectra

When electrons move between energy levels, atoms emit or absorb light β†’ this produces atomic spectra.

a) Types of Spectra

  1. Continuous Spectrum: All wavelengths emitted by solids, liquids or dense gases.
  2. Line Spectrum: Discrete wavelengths; emitted by gases.

Example: Hydrogen spectrum – unique lines related to electron transitions.

b) Rydberg Formula (Hydrogen Spectrum)

1/Ξ» = RH (1/n21 - 1/n22)

Where:

  • Ξ» = wavelength of emitted light
  • RH = Rydberg constant (~1.097 Γ— 10^7 m⁻¹)
  • n1, n2 = principal quantum numbers

Energy Levels and Spectral Series - Class 12 Physics

1. Energy Levels of Electrons

  • Electrons in an atom don’t move randomly; they occupy specific energy levels or shells around the nucleus.
  • These energy levels are quantized, meaning an electron can only have certain allowed energies.
  • The energy of an electron in the (n)-th orbit of hydrogen is given by:

En = - 13.6eV/n2

Where:

  • Ec = energy of the electron in the n-th orbit
  • n = principal quantum number (1, 2, 3, …)
  • A negative sign indicates the electron is bound to the nucleus.

Idea: Electrons can jump between levels, but cannot exist between them.

2. Electron Transitions

  • When an electron absorbs energy, it jumps from a lower energy level to a higher one β†’ absorption spectrum.
  • When an electron falls from a higher energy level to a lower one, it emits light β†’ emission spectrum.
  • The energy difference between levels determines the wavelength of emitted or absorbed light:

Ξ”E = Ehigher - Elower = hv

Where:

  • h = Planck’s constant
  • v = frequency of light

Spectral Series

In hydrogen, electrons moving to a specific lower level produce spectral series:

Series Final Orbit (n1) Wavelength Region Electron Transitions (n2 to n1)
Lyman 1 Ultraviolet (UV) n β‰₯ 2 β†’ 1
Balmer 2 Visible light n β‰₯ 3 β†’ 2
Paschen 3 Infrared (IR) n β‰₯ 4 β†’ 3
Brackett 4 Infrared (IR) n β‰₯ 5 β†’ 4
Pfund 5 Infrared (IR) n β‰₯ 6 β†’ 5

‍

Tips for exams:

  • Lyman β†’ UV, Balmer β†’ Visible, Paschen β†’ IR
  • Often, numericals ask for wavelength using Rydberg formula.

Bohr’s Model and Energy Quantization

  • Electrons occupy fixed energy levels β†’ cannot exist in between.
  • Energy of electron in (n)-th orbit:

En = - 13.6eV/n2

Bohr’s Postulates:

  1. Electrons move in stable orbits without energy loss.
  2. Energy is quantized.
  3. Energy is absorbed/emitted when electrons jump between orbits.

Dual Nature of Matter (de Broglie Hypothesis)

  • Louis de Broglie (1924) β†’ particles like electrons have wave properties.
  • Wavelength of a particle:

Ξ» = h/mv

  • Confirmed by electron diffraction experiments (Davisson & Germer, 1927).

Heisenberg’s Uncertainty Principle

  • Due to wave-particle duality β†’ cannot know exact position and momentum of a particle simultaneously:

Ξ”x.Ξ”p β‰₯h/4Ο€

  • Highlights limits of measurement at the quantum scale.

And that’s a wrap on Atoms and Nuclei Class 12 from atomic structure and subatomic particles to energy levels, spectra and quantum concepts, it’s all here. No more flipping between NCERT chapters or trying to decode formulas at midnight.

With this Atoms Physics Class 12 Notes PDF, you’ve now got everything simplified, sorted and 100% board-friendly. These Class 12 Atoms Notes make revision faster, easier and stress-free, giving you Atom Class 12 Physics Notes that are perfect for last-minute prep and full marks.

FAQs

Q1. What are the main subatomic particles in an atom?

Ans. Protons, neutrons and electrons. Protons are positively charged, neutrons are neutral and electrons are negatively charged.Β 

Q2. How does Bohr’s model explain atomic spectra?

Ans. Electrons occupy quantized orbits and emit or absorb energy only when jumping between levels. This produces line spectra, like the hydrogen spectrum.

Q3. What is the significance of spectral series like Lyman, Balmer and Paschen?

Ans. These series represent electron transitions to specific energy levels and help in identifying elements.Β 

Q4. What is the de Broglie hypothesis?

Ans. It states that matter has wave properties. The wavelength of a particle is given by Ξ» = h/ mv.Β 

Q5. What is Heisenberg’s Uncertainty Principle?

Ans. It’s impossible to know a particle’s exact position and momentum simultaneously: Ξ”xΒ·Ξ”p β‰₯ h/4Ο€.

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