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Bohr's Model of Atom | Structure of Atom Class 11 Notes

Bohr's Model of Atom | Structure of Atom Class 11 Notes

Bohr's Model of Atom

Structure of Atom | Postulates, Formulas, and Hydrogen Spectrum

1. Main Postulates of Bohr's Theory

Niels Bohr proposed a model for the Hydrogen atom based on Planck's Quantum Theory.

  1. Stationary Orbits: Electrons revolve around the nucleus in fixed circular paths called orbits or shells ($K, L, M, N...$). Energy does not radiate while in these orbits.
  2. Quantization Condition: An electron can revolve only in those orbits where its angular momentum ($L$) is an integral multiple of $h/2\pi$. $$ mvr = \frac{nh}{2\pi} $$
  3. Energy Transitions: Energy is absorbed or emitted only when an electron jumps from one orbit to another. $$ \Delta E = E_2 - E_1 = h\nu $$

2. Important Formulas (For Hydrogen-like Species)

A. Radius of $n^{th}$ Orbit ($r_n$)

$$ r_n = 0.529 \frac{n^2}{Z} \, \mathring{A} $$

Radius $\propto n^2$ and Radius $\propto 1/Z$.

B. Velocity of Electron ($v_n$)

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

Velocity $\propto Z$ and Velocity $\propto 1/n$.

C. Energy of Electron ($E_n$)

$$ E_n = -13.6 \frac{Z^2}{n^2} \, eV/atom $$

Or in Joules: $E_n = -2.18 \times 10^{-18} \frac{Z^2}{n^2} \, J/atom$.

Note: Negative sign indicates the electron is bound to the nucleus.

3. Hydrogen Spectrum

The wave number ($\bar{\nu}$) of emitted radiation when an electron drops from $n_2$ to $n_1$ is given by the Rydberg Formula:

$$ \bar{\nu} = \frac{1}{\lambda} = R_H Z^2 \left[ \frac{1}{n_1^2} - \frac{1}{n_2^2} \right] $$

Where $R_H \approx 109677 \, cm^{-1}$ (Rydberg Constant).

Spectral Series

Series Ground State ($n_1$) Excited State ($n_2$) Region
Lyman 1 2, 3, 4... Ultraviolet (UV)
Balmer 2 3, 4, 5... Visible
Paschen 3 4, 5, 6... Infrared (IR)
Brackett 4 5, 6, 7... Infrared (IR)
Pfund 5 6, 7, 8... Far Infrared

4. Limitations of Bohr's Model

  • It could not explain the spectra of multi-electron atoms (e.g., Helium atom).
  • It could not explain the splitting of spectral lines in magnetic fields (Zeeman Effect) or electric fields (Stark Effect).
  • It violates the Heisenberg Uncertainty Principle (defines exact position and velocity simultaneously).

Practice Quiz

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