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1 Some Basic Concepts of Chemistry 2 Structure of Atom 3 Classification of Elements and Periodicity in Properties 4 Chemical Bonding and Molecular Structure 5 Thermodynamics 6 Equilibrium 7 Redox Reactions 8 Organic Chemistry – Some Basic Principles and Techniques 9 Hydrocarbons

2 Structure of Atom

2.1 Discovery of Sub-atomic Particles 2.2 Atomic Models 2.3 Developments Leading to the Bohr’s Model of Atom 2.4 Bohr’s Model for Hydrogen Atom 2.5 Towards Quantum Mechanical Model of the Atom 2.6 Quantum Mechanical Model of Atom

Bohr’s Model for Hydrogen Atom

NCERT Reference: Chapter 2, Pages 40–44
Learning Objective: Understand how Bohr’s quantized circular orbits explain hydrogen’s spectrum, how to use radius and energy expressions, and why the model has limitations.

Quick Notes:

  • Bohr explained hydrogen's atomic structure using quantized circular orbits.
  • Electrons can only occupy discrete energy levels without radiating energy.
  • Energy is emitted or absorbed only when the electron jumps between levels.
  • Bohr’s model explains line spectrum of hydrogen well, but fails for atoms with more than one electron and can't account for fine spectra or quantum mechanics.

Full Notes:

Background to Bohr’s Model

Classical mechanics, as used in Rutherford’s model, could not explain the stability of atoms or the line spectra of hydrogen.

Bohr introduced a new atomic model in 1913, combining classical ideas with quantum postulates to overcome these issues.

Postulates of Bohr’s Atomic Model

1. Stable Circular Orbits (Stationary States)
Electrons revolve around the nucleus in circular orbits with fixed radii and energy, called stationary states, without emitting radiation as they move.

2. Quantization of Angular Momentum
Only orbits are permitted where the electron’s angular momentum is an integral multiple of h/2π.

Formula:

NCERT 11 Chemistry Bohr angular momentum quantization diagram showing m e v r = n h over 2π.

mₑ × v × r = n × h / (2π)  (Equation 2.11)

3. Emission or Absorption of Radiation
Electrons can jump between energy levels by emitting or absorbing a photon of radiation.

The energy gaps can be described by the Bohr’s Frequency Rule formula:

NCERT 11 Chemistry Bohr frequency rule diagram showing ν equals ΔE divided by h.

ν = ΔE / h = (E₂ – E₁) / h  (Equation 2.10)

Energy and Radius of Bohr Orbits for Hydrogen

Note - you don’t need to know the derivations or advanced theory behind these equations, just how they can be used and what they describe

For hydrogen atom (Z = 1), Bohr showed:

Radius of nth orbit:

NCERT 11 Chemistry Bohr radius relation showing r n equals n squared times a0.

rn = n² × a₀ (Equation 2.12)

(Where 1 Å = 10−10 m)

This means the radius of the first stationary state (n=1) is 52.9pm. This is called the Bohr Radius or Bohr Orbit.

And, as n increases, the distance of the orbit the electron is in is further from the nucleus.

Energy of nth orbit:

NCERT 11 Chemistry hydrogen energy-level expression E n equals negative 2.18 × 10⁻¹⁸ times 1 over n squared.

Note - the 1 in the formula comes from atomic number of hydrogen (given a positive charge from the nucleus of 1).

En = − 2.18 × 10−18 × (1 / n²) J
Meaning for E1 (lowest possible energy state) = − 2.18 × 10−18 J

Note:

For other species with only 1 electron (such as He+, Li2+, Be3+) we can use the following formula:

NCERT 11 Chemistry one-electron ion energy expression E n equals negative 2.18 × 10⁻¹⁸ times Z squared over n squared.

En = −2.18 × 10−18 × (Z² / n²) J  (Equation 2.14)

As Z increases, the energy of the electron gets more negative. This means its harder to remove from the atom (or ion) in its stationary state.

The radii of an orbit can also be determined using:

NCERT 11 Chemistry Bohr orbit radii relation r n equals 52.9 times n squared over Z picometres.

rn = 52.9 × (n² / Z) pm  (Equation 2.15)

2.4.1 Explanation of Line Spectrum of Hydrogen

In hydrogen atoms, electrons don’t emit a continuous spectrum of light. Instead, we see a line spectrum – sharp, distinct lines of specific wavelengths. This is because electrons only occupy specific orbits with fixed energy, as Bohr proposed.

Why Do These Lines Appear?

Energy of a Transition

When an electron moves from energy level nᵢ (initial) to n𝒇 (final), the energy difference is:

NCERT 11 Chemistry transition energy diagram showing ΔE equals E f minus E i.

ΔE = E𝒇 – Eᵢ (Equation 2.16)

From Bohr’s model, the energy of each orbit is:

NCERT 11 Chemistry equation E n equals negative 2.18 times 10 to the power minus 18 times 1 over n squared.

En = −2.18 × 10−18 × (1 / n²) J (Equation 2.13)

Substituting into ΔE gives:

NCERT 11 Chemistry ΔE expression showing −2.18 × 10⁻¹⁸ times (1 over n f squared minus 1 over n i squared).

ΔE = −2.18 × 10−18 × (1 / n𝒇² – 1 / nᵢ²) J (Equation 2.17)

Frequency of Emitted or Absorbed Radiation

The frequency ν of the emitted or absorbed radiation is related to energy by Planck’s equation:

NCERT 11 Chemistry Planck relation diagram ν equals ΔE divided by h linking photon frequency to energy gap.

ν = ΔE / h (Equation 2.18)

Substituting ΔE from Equation 2.17:

NCERT 11 Chemistry combined frequency formula leading to R H times (1 over n i squared minus 1 over n f squared).

ν = RH × (1 / nᵢ² – 1 / n𝒇²) where RH = 3.29 × 1015 Hz (Equation 2.19)

This gives the frequency of the spectral line.

Wave Number (ṽ) and Line Spectrum

Wavenumber is the number of waves per unit length, and is defined as:

NCERT 11 Chemistry wavenumber definition ṽ equals ν over c equals ΔE over h c.

ṽ = ν / c = ΔE / (hc)

Substitute in the constants and formula for ΔE:

NCERT 11 Chemistry Rydberg wavenumber formula ṽ equals 1.09677 × 10⁷ times (1 over n i squared minus 1 over n f squared) per metre.

ṽ = RH / c × (1 / nᵢ² – 1 / n𝒇²)
ṽ = 1.09677 × 107 × (1 / nᵢ² – 1 / n𝒇²) m−1 (Equation 2.21)

This is the Rydberg formula, used to calculate wavelengths of spectral lines in hydrogen.

What to Remember

Spectral Series of Hydrogen:

Each series corresponds to transitions ending at a specific lower level:

NCERT 11 Chemistry hydrogen spectral series diagram showing Lyman UV, Balmer visible, Paschen IR and higher series.
Series Name Final Level (n1) Region of Spectrum
Lyman 1 Ultraviolet
Balmer 2 Visible
Paschen 3 Infrared
Brackett 4 Infrared
Pfund 5 Infrared

Example Balmer emission

An electron falling from n = 3 to n = 2 → emits visible light (Balmer series).

2.4.2 Limitations of Bohr’s Model

Although successful for hydrogen, Bohr’s model fails in multiple ways:

  1. Could Not Explain Multi-Electron Systems
    • Bohr’s equations and energy levels only apply to hydrogen or hydrogen-like ions (e.g. He+, Li2+)
    • Spectra of more complex atoms do not fit Bohr’s model
  2. Spectral Fine Structure Not Explained
    • Actual hydrogen spectral lines are split into multiple closely spaced lines (fine structure)
    • Bohr's model predicts single lines only
    • Fine structure is explained only by relativistic corrections and spin (quantum mechanics)
  3. Zeeman and Stark Effects Not Accounted For
    • When atoms are placed in magnetic (Zeeman) or electric (Stark) fields, their spectral lines split further
    • Bohr's model provides no explanation for these effects
  4. No Explanation for Heisenberg Uncertainty or Dual Nature
    • Bohr treated electrons as particles in fixed orbits, ignoring their wave nature
    • This contradicts the Heisenberg Uncertainty Principle, which says we can’t simultaneously know position and momentum of an electron exactly
  5. Incompatible with Quantum Mechanics
    • Bohr’s model is semi-classical, using classical orbits with quantum jumps
    • It violates modern quantum mechanics, which describes electrons as probability clouds (orbitals), not fixed orbits

Conclusion
Bohr’s model was a major breakthrough and laid the groundwork for quantum theory by introducing the idea of quantized energy levels. It successfully explained:

But it failed to extend to multi-electron systems and did not incorporate the wave-particle duality, fine spectral features, or quantum mechanical principles, which were later addressed in more advanced models like Schrödinger’s.

Summary