Bohr's Atomic Model

Master Bohr's postulates, orbital radii, electron velocities, and energy levels for hydrogen-like atoms.

Introduction

In 1913, Niels Bohr proposed a revolutionary model of the atom that successfully explained the hydrogen spectrum. While later superseded by quantum mechanics, Bohr’s model remains essential for JEE and provides intuitive understanding of atomic structure.

Oppenheimer's Atomic Understanding
In Oppenheimer (2023), the scientists’ understanding of atomic structure started with Bohr’s model! The film shows how these “planetary” orbits of electrons helped physicists unlock nuclear energy. Bohr even appears as a character, discussing quantum theory with Oppenheimer. The discrete energy levels you’ll learn here are the foundation of understanding how atoms work!

Interactive: Bohr Model Visualization

Click the buttons to see energy absorption and emission as electrons jump between orbits:


Bohr’s Postulates

Postulate 1: Quantized Orbits

Electrons revolve around the nucleus in fixed circular orbits called stationary states or energy levels. While in these orbits, electrons do not radiate energy.

Postulate 2: Quantized Angular Momentum

The angular momentum of an electron is quantized:

$$\boxed{mvr = n\frac{h}{2\pi} = n\hbar}$$

where:

  • $n$ = principal quantum number (1, 2, 3, …)
  • $\hbar$ = reduced Planck’s constant = $\frac{h}{2\pi}$

Postulate 3: Energy Transitions

Energy is absorbed or emitted only when an electron jumps between orbits:

$$\boxed{\Delta E = E_2 - E_1 = h\nu}$$
  • Absorption: electron jumps to higher orbit (n₁ → n₂, where n₂ > n₁)
  • Emission: electron falls to lower orbit (n₂ → n₁)
Neon Signs in Stranger Things
Ever wondered why neon signs in Stranger Things (2024) glow with specific colors? That’s Bohr’s 3rd postulate in action! When electricity excites atoms, electrons jump to higher orbits. When they fall back down, they emit light of EXACTLY the right frequency. Different atoms = different colors. The Upside Down’s eerie lighting? All atomic physics!

Interactive Demo: Bohr’s Model

Watch how electrons transition between energy levels. See absorption and emission in action:


Derivation of Key Formulas

For a hydrogen-like atom with nuclear charge $Ze$:

Balancing Forces

Centripetal force = Electrostatic attraction:

$$\frac{mv^2}{r} = \frac{kZe^2}{r^2}$$

where $k = \frac{1}{4\pi\epsilon_0} = 9 \times 10^9$ N·m²/C²

Combining with Angular Momentum

From $mvr = n\hbar$, we get $v = \frac{n\hbar}{mr}$

Substituting and solving:


Results for Hydrogen-like Atoms

1. Radius of nth Orbit

$$\boxed{r_n = \frac{0.529 \times n^2}{Z} \text{ Å}}$$

or in SI units:

$$r_n = \frac{n^2 h^2 \epsilon_0}{\pi m Z e^2}$$

Key observations:

  • Radius increases as $n^2$
  • Radius decreases with increasing $Z$
  • First Bohr radius ($a_0$) for H = 0.529 Å

2. Velocity in nth Orbit

$$\boxed{v_n = \frac{2.18 \times 10^6 \times Z}{n} \text{ m/s}}$$

Key observations:

  • Velocity decreases as $\frac{1}{n}$
  • Velocity increases with $Z$
  • Electron in 1st orbit of H has velocity ≈ c/137

3. Energy of nth Orbit

$$\boxed{E_n = -\frac{13.6 \times Z^2}{n^2} \text{ eV}}$$

or in Joules:

$$E_n = -\frac{2.18 \times 10^{-18} \times Z^2}{n^2} \text{ J}$$

Key observations:

  • Energy is negative (bound state)
  • Energy increases (becomes less negative) with n
  • Ground state energy of H = -13.6 eV
  • At n = ∞, E = 0 (ionization)
Memory Aid

Remember the magic numbers:

  • 0.529 Å for radius
  • 2.18 × 10⁶ m/s for velocity
  • 13.6 eV for energy

Energy Level Diagram

graph BT
    A[n=1: -13.6 eV] --> B[n=2: -3.4 eV]
    B --> C[n=3: -1.51 eV]
    C --> D[n=4: -0.85 eV]
    D --> E[n=∞: 0 eV]
    
    style A fill:#e74c3c
    style E fill:#2ecc71
nEnergy (eV)Radius (Å)Velocity (m/s)
1-13.60.5292.18 × 10⁶
2-3.42.1161.09 × 10⁶
3-1.514.7610.727 × 10⁶
4-0.858.4640.545 × 10⁶
00

Important Relationships

Energy Ratios

For hydrogen-like atoms:

$$\frac{E_{n_1}}{E_{n_2}} = \frac{n_2^2}{n_1^2}$$

Orbital Period

Time for one revolution:

$$T_n = \frac{2\pi r_n}{v_n} \propto \frac{n^3}{Z^2}$$

Frequency of Revolution

$$f_n = \frac{v_n}{2\pi r_n} \propto \frac{Z^2}{n^3}$$

Calculations

Example 1: Comparing Radii

Problem: Find the radius of the 3rd orbit of Li²⁺.

Solution: For Li²⁺: Z = 3, n = 3

$$r_3 = \frac{0.529 \times 3^2}{3} = \frac{0.529 \times 9}{3} = 1.587 \text{ Å}$$

Note: This equals the first Bohr radius of hydrogen times 3!

Example 2: Energy Difference

Problem: Calculate the energy required to excite an electron from n=2 to n=4 in hydrogen.

Solution:

$$\Delta E = E_4 - E_2 = -\frac{13.6}{16} - \left(-\frac{13.6}{4}\right)$$ $$\Delta E = -0.85 + 3.4 = 2.55 \text{ eV}$$

Ionization Energy

Ionization energy is the energy needed to remove an electron from ground state to infinity:

$$IE = E_\infty - E_1 = 0 - (-13.6 Z^2) = 13.6 Z^2 \text{ eV}$$

For hydrogen: IE = 13.6 eV = 2.18 × 10⁻¹⁸ J

For JEE

Common hydrogen-like species:

  • H (Z=1): IE = 13.6 eV
  • He⁺ (Z=2): IE = 54.4 eV
  • Li²⁺ (Z=3): IE = 122.4 eV

Practice Problems

  1. Calculate the velocity of electron in the 2nd orbit of He⁺.

  2. In which orbit of hydrogen atom will the electron have the same energy as in the first orbit of Li²⁺?

  3. Find the ratio of kinetic energies of electrons in the 1st and 3rd orbits of hydrogen.

Quick Check
Total energy of electron in nth orbit = -½ × Potential energy = -(Kinetic energy). Verify this!


Within Atomic Structure

Cross-Subject: Physics Connections

Cross-Subject: Math Connections