Physics · Atoms

Bohr Model of the Hydrogen Atom

Rutherford's nuclear atom was mechanically stable on paper but could neither survive classical electromagnetism nor explain the sharp line spectrum of hydrogen. In 1913 Niels Bohr resolved both failures with three bold postulates, set out in NCERT Class XII §12.4 and NIOS §24.2. The model fixes the electron in quantised orbits of radius $r_n \propto n^2/Z$, speed $v_n \propto Z/n$ and energy $E_n = -13.6\,Z^2/n^2$ eV — the exact relations NEET tests almost every year.

Why Rutherford's atom failed

Rutherford's nuclear model pictured the electron orbiting the nucleus like a planet around the sun, the Coulomb attraction supplying the centripetal force. NCERT §12.4 identifies two fatal objections. First, an electron moving in a circle is continuously accelerated, and classical electromagnetic theory requires an accelerating charge to radiate. The electron should therefore lose energy continuously, spiral inward and collapse into the nucleus — so the atom could not be stable.

Second, as the electron spiralled in, its frequency of revolution would change continuously, so the emitted light would span a continuous band of frequencies. This contradicts the observed hydrogen spectrum, which consists of sharp discrete lines. Classical physics, in short, could explain neither the stability of the atom nor its line spectrum.

SVG Figure 1

The classical catastrophe: an accelerating electron radiates and spirals into the nucleus.

+ e⁻ radiated energy Continuous radiation → continuous spectrum → unstable atom.

The three postulates

Bohr kept Rutherford's nucleus but grafted on the new quantum ideas of Planck and Einstein. He accepted that classical electromagnetism does not govern atomic-scale processes, and stated his theory as three postulates (NCERT §12.4).

PostulateStatementKey relation
I — Stationary orbits The electron revolves only in certain stable orbits without emitting radiation. Each such state has a definite total energy and is called a stationary state. No radiation in a stationary state
II — Quantised angular momentum Only those orbits are allowed for which the orbital angular momentum is an integral multiple of $h/2\pi$. L = mvr = nh/2π
III — Frequency / transition An electron may jump from a higher to a lower allowed orbit, emitting a photon whose energy equals the difference between the two states. hν = Eᵢ − E_f

The second postulate is the engine of the model. With Planck's constant $h = 6.6 \times 10^{-34}$ J s, the quantisation condition is

$$ L = m v_n r_n = \dfrac{nh}{2\pi}, \qquad n = 1, 2, 3, \dots $$

Here $n$ is the principal quantum number. Because $L$ can take only the discrete values $h/2\pi,\, 2h/2\pi,\, 3h/2\pi, \dots$, the allowed radii and energies are also discrete. The third postulate then ties these discrete energies to the discrete frequencies seen in the spectrum, $h\nu = E_i - E_f$ with $E_i > E_f$.

Radius of the nth orbit

The radius is not assumed — it is forced by combining classical mechanics with the second postulate. Start from the dynamical condition that NCERT §12.4 inherits from the Rutherford model: for a stable circular orbit the Coulomb attraction between the nucleus ($+Ze$) and the electron ($-e$) supplies exactly the centripetal force,

$$ \dfrac{1}{4\pi\varepsilon_0}\,\dfrac{Ze^2}{r_n^{\,2}} \;=\; \dfrac{m v_n^{\,2}}{r_n} \qquad\Longrightarrow\qquad m v_n^{\,2} \;=\; \dfrac{1}{4\pi\varepsilon_0}\,\dfrac{Ze^2}{r_n}. \tag{1} $$

This single equation contains two unknowns, $r_n$ and $v_n$, so classical physics alone cannot fix the orbit — any radius would do. Bohr's second postulate removes the freedom by quantising the angular momentum:

$$ m v_n r_n = \dfrac{nh}{2\pi} \qquad\Longrightarrow\qquad v_n = \dfrac{nh}{2\pi m r_n}. \tag{2} $$

Substituting $v_n$ from (2) into (1) eliminates the velocity. The left side becomes $m\!\left(\dfrac{nh}{2\pi m r_n}\right)^{2} = \dfrac{n^2 h^2}{4\pi^2 m r_n^{\,2}}$, and setting that equal to the right side of (1) gives

$$ \dfrac{n^2 h^2}{4\pi^2 m r_n^{\,2}} = \dfrac{1}{4\pi\varepsilon_0}\,\dfrac{Ze^2}{r_n} \qquad\Longrightarrow\qquad r_n = \dfrac{n^2 h^2 \varepsilon_0}{\pi m Z e^2}. \tag{3} $$

Equation (3) is NCERT Eq. 12.7. Collecting the constants for the ground state of hydrogen ($n = 1$, $Z = 1$) gives the Bohr radius, which NCERT and NIOS §24.2.1 both quote as $a_0 = 5.3 \times 10^{-11}$ m. Writing the result in terms of $a_0$,

$$ r_n = \dfrac{n^2}{Z}\,(0.529\ \text{Å}), \qquad a_0 = 0.529\ \text{Å} = 5.3 \times 10^{-11}\ \text{m}. $$

Because $r_n \propto n^2$ at fixed $Z$, the $n = 2$ and $n = 3$ orbits of hydrogen sit at $4a_0$ and $9a_0$; and because $r_n \propto 1/Z$, a more highly charged nucleus pulls every orbit inward.

NCERT Example 12.3

It is found that 13.6 eV is required to separate a hydrogen atom into a proton and an electron. Compute the orbital radius and the velocity of the electron.

Total energy $E = -13.6$ eV $= -2.2 \times 10^{-18}$ J. Substituting into the energy expression gives the orbital radius $r = 5.3 \times 10^{-11}$ m, and the velocity relation then yields $v = 2.2 \times 10^{6}$ m/s. These are the ground-state Bohr radius and speed of the hydrogen electron.

Velocity and energy of the electron

The orbital speed follows immediately by feeding the quantised radius (3) back into the quantisation condition (2), $v_n = nh/(2\pi m r_n)$. Substituting $r_n = n^2 h^2 \varepsilon_0 / \pi m Z e^2$ and cancelling one power of $n$ gives

$$ v_n = \dfrac{nh}{2\pi m}\cdot\dfrac{\pi m Z e^2}{n^2 h^2 \varepsilon_0} = \dfrac{Z e^2}{2\varepsilon_0 n h} \qquad\Longrightarrow\qquad v_n \propto \dfrac{Z}{n}. $$

The electron therefore moves fastest in the innermost orbit and in atoms of larger nuclear charge, and slows as $n$ rises. For hydrogen in the ground state ($n = Z = 1$) the constants evaluate to $v_1 \approx 2.2 \times 10^{6}$ m/s, the value NCERT Example 12.3 quotes.

To find the energy, add the kinetic and potential parts. From the force balance (1), the kinetic energy of the electron is

$$ K = \tfrac{1}{2}m v_n^{\,2} = \dfrac{1}{2}\cdot\dfrac{1}{4\pi\varepsilon_0}\,\dfrac{Ze^2}{r_n} = +\,\dfrac{Ze^2}{8\pi\varepsilon_0 r_n}. $$

The electrostatic potential energy of the attractive nucleus–electron pair is negative and twice as large in magnitude:

$$ U = -\dfrac{1}{4\pi\varepsilon_0}\,\dfrac{Ze^2}{r_n} = -\,\dfrac{Ze^2}{4\pi\varepsilon_0 r_n} = -2K. $$

Hence the total energy $E_n = K + U = K - 2K = -K$ — the relation NCERT Eq. 12.4 records as $E = -\dfrac{Ze^2}{8\pi\varepsilon_0 r_n}$. Inserting the quantised radius (3) for $r_n$ collapses the constants into the headline result (NCERT Eq. 12.8–12.10):

$$ E_n = -\dfrac{m Z^2 e^4}{8\varepsilon_0^{\,2} n^2 h^2} = -\dfrac{13.6\,Z^2}{n^2}\ \text{eV} \qquad\Longrightarrow\qquad E_n \propto -\dfrac{Z^2}{n^2}. $$

Two features deserve emphasis. The energy is negative, signifying that the electron is bound — work must be done on it to reach the $E = 0$ free state; positive energy would mean an unbound electron. And the bookkeeping $K = -E_n$, $U = 2E_n$ holds in every orbit, so the binding energy in any level is numerically equal to its kinetic energy. This $K : E = 1 : -1$ ratio is itself a recurring NEET question.

λ Go deeper

Why must $L$ be a multiple of $h/2\pi$? See De Broglie's explanation of Bohr's second postulate, where standing electron waves fit the orbit.

Energy levels of hydrogen

For hydrogen ($Z = 1$), $E_n = -13.6/n^2$ eV. The energy is most negative in the ground state and rises toward zero as $n$ increases; at $n = \infty$ the energy is $0$ eV, corresponding to the electron removed and at rest (NCERT §12.4.1).

nEₙ (eV)StateEₙ − E₁ (eV)
1−13.6Ground state0
2−3.40First excited10.2
3−1.51Second excited12.09
0Free electron13.6 (ionisation)

The minimum energy needed to free the ground-state electron is therefore $13.6$ eV — the ionisation energy of hydrogen, in excellent agreement with experiment. The excited levels crowd together as $n$ grows, since the spacing falls off as $1/n^2$. The energy delivered to or absorbed by the atom in any process is always a difference between two of these levels.

Worked Example

Using $E_n = -13.6/n^2$ eV, find (a) the energy needed to excite a hydrogen atom from its ground state to the first excited state, and (b) the ionisation energy of a hydrogen atom already in the $n = 2$ state.

(a) The first excited state is $n = 2$, so $E_2 = -13.6/4 = -3.40$ eV. The excitation energy is $E_2 - E_1 = -3.40 - (-13.6) = 10.2$ eV — the energy of a photon that can lift the electron to $n = 2$, matching the $\text{E}_n - \text{E}_1$ column of the table above.

(b) Ionising from $n = 2$ means taking the electron from $E_2 = -3.40$ eV to $E_\infty = 0$. The energy required is $0 - (-3.40) = 3.40$ eV — only a quarter of the $13.6$ eV needed from the ground state, because the $n = 2$ electron is already four times less tightly bound.

SVG Figure 2

Energy-level ladder for hydrogen with $E_n = -13.6/n^2$ eV; a transition $n=3 \to n=2$ emits a photon $h\nu = E_3 - E_2$.

n=∞, 0 eV n=4 n=3, −1.51 n=2, −3.40 n=1, −13.6 photon, hν = E₃ − E₂ energy →

Scaling with n and Z

Most NEET problems on the Bohr model reduce to a single skill: reading off how $r_n$, $v_n$ and $E_n$ scale with the quantum number $n$ and the nuclear charge $Z$. The table below collects all three for a hydrogenic atom.

QuantityExpressionScalingHydrogen ground state
Radiusrₙ = (n²/Z)·0.529 Å$\propto n^2/Z$$5.3 \times 10^{-11}$ m
Velocityvₙ ∝ Z/n$\propto Z/n$$2.2 \times 10^{6}$ m/s
EnergyEₙ = −13.6 Z²/n² eV$\propto -Z^2/n^2$$-13.6$ eV
Angular momentumL = nh/2π$\propto n$$h/2\pi$
SVG Figure 3

Quantised circular orbits with radii in the ratio $1 : 4 : 9$ for $n = 1, 2, 3$.

+ n=1 (r) n=2 (4r) n=3 (9r) Radii scale as n²; orbits drawn to relative scale for hydrogen.
NEET Trap

Mixing up the n and Z exponents

The three relations carry different powers of $n$ and $Z$, and swapping them is the most common error. Keep them distinct: radius grows as $n^2$ but falls as $1/Z$; velocity falls as $1/n$ but grows as $Z$; energy falls in magnitude as $1/n^2$ and grows as $Z^2$. Angular momentum is the simplest — it depends only on $n$, in units of $h/2\pi$, and is independent of $Z$.

$r_n \propto \dfrac{n^2}{Z}$  ·  $v_n \propto \dfrac{Z}{n}$  ·  $E_n \propto -\dfrac{Z^2}{n^2}$  ·  ground state of H $= -13.6$ eV.

Limitations of the model

Bohr's model brilliantly reproduces the gross features of hydrogen, but NCERT §12.6 lists its boundaries. It applies only to hydrogenic atoms — a nucleus of charge $+Ze$ with a single electron, such as H, He⁺ and Li²⁺. It cannot be extended even to two-electron helium, because it accounts only for the nucleus-electron force and ignores the electron-electron repulsions that appear in multi-electron atoms.

The model also cannot explain the relative intensities of spectral lines — why some transitions are stronger than others. And as the "Points to Ponder" note, the sharp orbital picture conflicts with the uncertainty principle; it was later replaced by full quantum mechanics, in which Bohr's orbits become regions of high probability for finding the electron.

Quick Recap

Bohr model in one screen

  • Rutherford's atom fails: an accelerating electron radiates, spirals in, and would give a continuous spectrum.
  • Three postulates: stationary non-radiating orbits; quantised angular momentum $L = nh/2\pi$; transitions with $h\nu = E_i - E_f$.
  • Radius $r_n = (n^2/Z)\,(0.529\ \text{Å})$; Bohr radius (H, $n=1$) $\approx 5.3 \times 10^{-11}$ m.
  • Velocity $v_n \propto Z/n$; ground-state hydrogen speed $\approx 2.2 \times 10^{6}$ m/s.
  • Energy $E_n = -13.6\,Z^2/n^2$ eV; hydrogen ground state $-13.6$ eV; ionisation energy $13.6$ eV.
  • Valid only for single-electron (hydrogenic) atoms; cannot give line intensities.

NEET PYQ Snapshot — Bohr Model of the Hydrogen Atom

Real NEET questions on Bohr radius, orbital energy and the kinetic-to-total energy ratio.

NEET 2023

The radius of the innermost orbit of a hydrogen atom is 5.3 × 10⁻¹¹ m. What is the radius of the third allowed orbit of hydrogen?

  • (1) 4.77 Å
  • (2) 0.53 Å
  • (3) 1.06 Å
  • (4) 1.59 Å
Answer: (1) 4.77 Å

Since $r_n \propto n^2$ at fixed $Z$, $r_3 = 9\,r_1 = 9 \times 5.3 \times 10^{-11}$ m $= 47.7 \times 10^{-11}$ m $= 4.77$ Å.

NEET 2022

Let T₁ and T₂ be the energies of an electron in the first and second excited states of hydrogen. By Bohr's model, the ratio T₁ : T₂ is

  • (1) 4 : 1
  • (2) 4 : 9
  • (3) 9 : 4
  • (4) 1 : 4
Answer: (3) 9 : 4

First excited state is $n = 2$, second excited state is $n = 3$. With $E_n \propto 1/n^2$, $T_1 : T_2 = (1/4) : (1/9) = 9 : 4$.

NEET 2018

The ratio of kinetic energy to total energy of an electron in a Bohr orbit of the hydrogen atom is

  • (1) 1 : 1
  • (2) 1 : −1
  • (3) 2 : −1
  • (4) 1 : −2
Answer: (2) 1 : −1

In a Bohr orbit the kinetic energy $K = +Ze^2/8\pi\varepsilon_0 r$ and the total energy $E = -Ze^2/8\pi\varepsilon_0 r$, so $K = -E$ and $K : E = 1 : -1$.

FAQs — Bohr Model of the Hydrogen Atom

Quick answers to the points NEET most often tests on the Bohr model.

What are the three postulates of Bohr's model?

First, an electron can revolve in certain stable orbits without emitting radiation; these are the stationary states, each with a definite energy. Second, only those orbits are allowed for which the angular momentum is an integral multiple of h/2π, that is L = nh/2π. Third, an electron may jump from one allowed orbit to another of lower energy, emitting a photon whose energy equals the difference between the states, hν = Eᵢ − E_f.

Why does the electron not radiate energy in a Bohr stationary orbit?

Bohr's first postulate simply asserts that the electron in a stationary orbit does not emit radiant energy, in direct contradiction to classical electromagnetic theory. Classically an accelerating charge must radiate, so the electron should spiral into the nucleus. Bohr abandoned that classical requirement for atomic-scale processes; the non-radiating orbit is a postulate, not something derived from earlier physics.

How does the orbit radius depend on n and Z in the Bohr model?

The radius of the nth orbit is rₙ = (n²/Z) × 0.529 Å. It grows as the square of the principal quantum number and shrinks inversely with the atomic number. For hydrogen (Z = 1) the n = 1 radius is the Bohr radius, about 5.3 × 10⁻¹¹ m, and the n = 2 and n = 3 radii are 4 and 9 times larger.

What is the ground state energy of the hydrogen atom and what does the negative sign mean?

The ground state (n = 1) energy of hydrogen is −13.6 eV. The negative sign signifies that the electron is bound to the nucleus; energy must be supplied to free it. Removing the electron from the ground state to infinity requires 13.6 eV, which is the ionisation energy of hydrogen.

How does the orbital velocity vary with n and Z?

The orbital speed of the electron varies as vₙ ∝ Z/n. It is largest in the innermost orbit and in atoms of higher nuclear charge, and it decreases as the electron moves to higher orbits. For hydrogen in the ground state the speed is about 2.2 × 10⁶ m/s.

Why does the Bohr model fail for atoms heavier than hydrogen?

The Bohr model applies only to hydrogenic atoms — a nucleus of charge +Ze with a single electron. It cannot be extended even to two-electron atoms such as helium because it accounts only for the nucleus-electron force and ignores the electron-electron forces that appear in multi-electron atoms. It also cannot explain the relative intensities of spectral lines.