Radii & Velocity Derivations
Niels Bohr's 1913 model of the hydrogen atom was a landmark in the history of atomic physics. By combining classical mechanics with a bold quantum postulate — that electrons occupy only certain discrete, stable orbits — Bohr was able to derive exact expressions for the radius and speed of an electron in any allowed orbit. These results explained the observed line spectra of hydrogen and hydrogen-like ions with extraordinary precision. The two key results of Bohr's derivation are the orbital radius formula, , and the orbital velocity formula, , where is the principal quantum number and is the atomic number. Both relationships emerge naturally from balancing the Coulomb electrostatic force against the centripetal force requirement, and then applying Bohr's angular momentum quantization condition . Understanding these derivations is essential not only for solving numerical problems about orbit sizes and electron speeds, but also for appreciating how the model connects classical physics to early quantum ideas. Although the Bohr model is ultimately superseded by quantum mechanics, the quantitative relationships it produces for hydrogen-like species remain numerically accurate and are widely used in introductory atomic physics and chemistry.
- Setting Up the Force Balance
- Applying Bohr's Quantization Condition
- Solving for the Orbital Radius
- Solving for the Orbital Velocity
- Physical Interpretation and Proportionality Summary
Setting Up the Force Balance
Consider an electron of mass and charge moving in a circular orbit of radius around a nucleus of charge . Two conditions must be satisfied simultaneously. First, the electrostatic (Coulomb) attraction provides exactly the centripetal force needed to keep the electron in circular motion: . Rearranging gives , which links the electron's speed and orbit radius .
Applying Bohr's Quantization Condition
Bohr postulated that only orbits where the electron's angular momentum is an integer multiple of the reduced Planck constant are allowed: , where is the principal quantum number. This is the radical quantum postulate that breaks from classical mechanics. Solving for : .
Solving for the Orbital Radius
Substitute into the force-balance equation . This gives , which simplifies to . Solving for : . The constant Å is known as the Bohr radius. This immediately reveals : orbits grow as the square of and shrink for heavier nuclei.
Solving for the Orbital Velocity
Now substitute back into the angular momentum condition : . Since where , the combination m/s, the ground-state speed in hydrogen. Thus , confirming . Electrons move faster in higher- atoms and slower in higher shells.
Physical Interpretation and Proportionality Summary
The two derived proportionalities have clear physical meanings. : increasing spreads the orbit further from the nucleus (electron cloud expands), while increasing pulls the orbit inward (stronger nuclear attraction). : a more highly charged nucleus accelerates the electron to higher speed, while moving to a higher shell requires the electron to slow down to satisfy the angular momentum condition. For hydrogen () in the ground state (): Å and m/s, which is about 0.73% the speed of light — fast but still non-relativistic, validating the classical mechanical approach.
The Key Equation
- r_n — Orbital radius of nth shell (metres (m) or ångströms (Å)): Distance from the nucleus to the electron in the nth allowed orbit for a nucleus of charge Z.
- a_0 — Bohr radius (Å (1 Å = 10⁻¹⁰ m)): The smallest possible orbit radius in hydrogen; Å.
- n — Principal quantum number (dimensionless): A positive integer (1, 2, 3, …) labelling the allowed orbital shells; n=1 is the ground state.
- Z — Atomic number (dimensionless): Number of protons in the nucleus; determines the nuclear charge experienced by the electron.
- v_n — Orbital velocity of nth shell (m/s): The speed of the electron in the nth allowed orbit; it depends on nuclear charge and shell number.
- v_1 — Ground-state orbital speed (hydrogen) (m/s): m/s; also equals where is the fine-structure constant.
Worked Example
Problem. Calculate (a) the radius and (b) the orbital speed of the electron in the He⁺ ion (Z = 2) in its n = 3 shell. Express the radius in ångströms and the speed as a fraction of the speed of light.
Answer. Orbital radius r₃ ≈ 2.38 Å; orbital speed v₃ ≈ 1.46 × 10⁶ m/s (≈ 0.49% of the speed of light).
Origins · 1 minNiels Henrik David Bohr and how this was discovered
Bohr proposed his quantum model of the hydrogen atom in 1913, introducing the postulate that electrons occupy discrete, non-radiating orbits with quantized angular momentum. From this single assumption he derived the correct Rydberg formula for hydrogen spectral lines, explained the stability of atoms, and calculated orbital radii and velocities — all from first principles. He was awarded the Nobel Prize in Physics in 1922. Bohr was also an enthusiastic football (soccer) player and his younger brother Harald Bohr represented Denmark in the 1908 Olympics, winning a silver medal. Niels was reportedly the better goalkeeper of the two.
Related Concepts
- Bohr Energy Levels: — The orbital radius and velocity derivations feed directly into calculating the total energy of each Bohr orbit, which explains the hydrogen emission spectrum.
- Quantization of Angular Momentum () — Bohr's angular momentum postulate is the key step that selects allowed orbits and is used in every step of the radius and velocity derivations.
- Hydrogen Emission Spectrum and the Rydberg Equation — The quantized radii and energies directly explain why hydrogen emits light only at specific wavelengths, giving series like Lyman, Balmer, and Paschen.
- Quantum Numbers and Electron Configuration — The principal quantum number n introduced by Bohr is the foundation for the full set of quantum numbers used in modern atomic orbital theory.
- Coulomb's Law and Electrostatic Force — The Coulomb force between nucleus and electron is the centripetal force in Bohr's model; understanding its form is essential for Step 1 of the derivation.