Q.The gravitational attraction between electron and proton in a hydrogen atom is weaker than the coulomb attraction by a factor of about 10−40. An alternative way of looking at this fact is to estimate the radius of the first Bohr orbit of a hydrogen atom if the electron and proton were bound by gravitational attraction. You will find the answer interesting.
Concept understanding — Bohr Model Quantization
Why does an electron not spiral into the nucleus?
Imagine you're pushing a child on a swing. If you push at random moments, the swing jerks and slows down. But if you push exactly in rhythm with the swing's natural motion, each push adds energy smoothly and the swing goes higher and higher. The swing "prefers" to move at specific frequencies — its natural modes.
An electron orbiting a nucleus is similar, but with a crucial twist from the quantum world. Classical physics says an accelerating charge (like an electron going in a circle) must continuously radiate energy. If that were true, the electron would lose energy, spiral into the nucleus, and atoms would collapse in a flash of light. But atoms are stable. So something is fundamentally different.
The radical idea: allowed orbits only
Niels Bohr proposed in 1913 that the electron cannot occupy just any orbit. It can only exist in certain stationary states — orbits where it does not radiate energy. These are like the swing's natural frequencies, but for an electron.
The key condition that picks out these special orbits is called quantization of angular momentum.
L=n2πh,n=1,2,3,…
Here L is the orbital angular momentum of the electron, h is Planck's constant, and n is a positive integer called the principal quantum number.
What this means physically
Angular momentum for a circular orbit is L=mvr, where m is the electron mass, v its speed, and r the orbit radius. So the quantization condition becomes:
mvr=n2πh
This is not a formula you derive — it is a postulate, a rule that nature follows. Bohr had no deeper explanation for why this rule works; he simply noticed it gave the right answers for hydrogen's spectrum.
The quantity 2πh appears so often that it has its own symbol: ℏ (h-bar). So the condition is often written as L=nℏ.
What it predicts
Combining this quantization with Newton's law for circular motion (centripetal force = Coulomb attraction) gives:
- Radius of the nth orbit: rn=n2a0, where a0=0.529A˚ is the Bohr radius (the smallest orbit, n=1).
- Energy of the nth orbit: En=−n213.6eV
The negative sign means the electron is bound to the nucleus. As n increases, the orbit gets larger and the energy becomes less negative (closer to zero).
The key insight for exams
Bohr quantization is not a derivation — it is a condition you apply. When you see a problem about hydrogen-like atoms (one electron), you:
- Write mvr=nℏ
- Write the force balance: rmv2=r2kZe2 (for nuclear charge Ze)
- Solve for r and v in terms of n
Bohr's model works perfectly only for single-electron systems: H, He+, Li2+, etc. It fails for multi-electron atoms because it ignores electron-electron repulsion and the wave nature of electrons.
Why "quantization"?
The word comes from the Latin quantus — "how much." In classical physics, angular momentum can take any value. In Bohr's atom, it comes only in discrete packets (quanta) of size ℏ. This is the first hint that at the atomic scale, nature is not continuous but granular.
The electron does not spiral because it cannot lose energy gradually — it can only jump from one allowed orbit to another, emitting or absorbing a photon of exactly the right energy. Between these jumps, it simply exists in a stationary state, defying classical expectations.
Bohr's quantization of angular momentum is one of the defining postulates covered in the NCERT Class 12 Physics Atoms chapter, and students frequently search for "Bohr model quantization condition and derivation" or "Bohr's model important questions" while preparing for CBSE boards and JEE Main/NEET. This concept is also a common launching point for numerical problems on orbital radius and energy levels of hydrogen-like atoms tested across competitive exams.
Why this formula?
Why Angular Momentum is Quantised in the Bohr Model
The Bohr model's most famous result — that angular momentum comes only in integer multiples of 2πh — is not an arbitrary assumption. It follows directly from a single, elegant idea: the electron's wave must close on itself.
The core problem Bohr faced
By 1913, physicists knew two things that seemed contradictory:
- Rutherford's nuclear model showed electrons orbiting the nucleus.
- Maxwell's equations predicted that any accelerating charge (like an orbiting electron) must radiate energy, spiral inward, and collapse in about 10−11 seconds.
Atoms are stable. Something was missing.
Bohr's breakthrough was to combine the newly discovered quantum idea (Planck's constant h) with classical mechanics, but only for allowed orbits. The key constraint came from thinking of the electron not as a tiny planet, but as a standing wave.
The de Broglie wavelength argument (the cleanest derivation)
A few years after Bohr, de Broglie proposed that every moving particle has a wavelength:
λ=ph=mvh
For an electron in a circular orbit of radius r, the circumference is 2πr. For the wave to be stable — not cancelling itself out — the circumference must contain an integer number of wavelengths:
2πr=nλ,n=1,2,3,…
Substitute λ=h/(mv):
2πr=n⋅mvh
Rearrange:
mvr=n⋅2πh
That's it. The left side mvr is the angular momentum L. So:
L=nℏ,where ℏ=2πh
This is not a separate postulate — it is a consequence of requiring the electron wave to be a standing wave. If the wave doesn't close on itself, it interferes destructively and the orbit cannot exist.
Why this fixes the energy levels
Once angular momentum is quantised, the rest follows from classical physics. For a circular orbit, the centripetal force is provided by the Coulomb attraction:
rmv2=4πϵ01r2e2
Combine this with mvr=nℏ and solve for r and E:
rn=me24πϵ0ℏ2⋅n2=a0n2
En=−8ϵ02h2me4⋅n21=−n213.6 eV
A common mistake is to think Bohr derived the quantization rule from first principles. He didn't — he postulated it. The de Broglie standing-wave argument came later and provides the physical reason for the postulate, but it is still a postulate in the full quantum theory.
The deeper reason: it's not really about orbits
The Bohr model is ultimately wrong — electrons don't orbit in neat circles. But the quantization of angular momentum survives in the full quantum mechanical treatment (Schrödinger equation) as the condition that the wavefunction must be single-valued. For the hydrogen atom, the angular momentum quantum number l can take values 0,1,2,…,n−1, and the magnitude is l(l+1)ℏ, not nℏ.
Yet the Bohr model's key insight — that only certain discrete states are allowed — remains the foundation of atomic physics. The formula L=nℏ is the simplest example of a quantum number, and it correctly predicts the hydrogen spectrum to within fine-structure corrections.
The Bohr quantization condition L=nℏ is a boundary condition on the electron wave, not a dynamical law. It says: for the electron to exist in a stable state, its wave must fit perfectly around the nucleus. This is the same principle that governs standing waves on a string or in an organ pipe — only certain wavelengths survive.
The Bohr-model derivation for the orbit radius never actually depends on the force being electrical -- only on it being an inverse-square central force -- so the same derivation goes through with the Coulomb force constant ke2 replaced by the gravitational analogue Gmemp.
r1≈1.2×1029 m -- vastly larger than the size of the observable universe, showing just how much weaker gravity is than the Coulomb force at atomic scales.
Replacing the Coulomb force ke2/r2 with the gravitational force Gmemp/r2 in the Bohr derivation gives a 'gravitational Bohr radius' of about 1.2×1029 m for n=1 -- enormously larger than an atom, or even the observable universe.
Step 1 -- Redo the Bohr derivation with gravity as the central force.
In the ordinary Bohr model, the centripetal force balance is
rmv2=r2ke2,k=4πε01
and angular momentum quantisation gives mvr=n2πh. Combining these (exactly as in the text's derivation of the Bohr radius) gives
rn=4π2mke2n2h2
Nothing about this derivation actually used the fact that the force was electrical -- only that it was a 1/r2 attractive force between the electron (mass me) and a much heavier fixed centre. So if the electron and proton were instead bound purely by gravity, we simply replace the Coulomb coupling ke2 by the gravitational coupling Gmemp:
rngrav=4π2me(Gmemp)n2h2=4π2Gme2mpn2h2
Step 2 -- Evaluate for n=1.
Using h=6.63×10−34 J s, G=6.67×10−11 N m2kg−2, me=9.11×10−31 kg, mp=1.67×10−27 kg:
r1grav=4π2Gme2mph2≈1.2×1029 m
Step 3 -- Put the number in perspective.
1.2×1029 m is about a thousand times larger than the radius of the observable universe (∼4×1026 m). This dramatically illustrates the exercise's opening fact -- gravity is weaker than the Coulomb attraction between an electron and proton by a factor of about 10−40 -- an atom held together by gravity alone, at the same quantum number, would be unimaginably larger than anything that actually exists.
r1grav≈1.2×1029 m
- JKBOSE Class 12 Annual Regular Examination 2024Set SZ3 marksQ.On the basis of Bohr's atomic model, find an expression for radius of nth orbit of a hydrogen atom.
›Reveal solutionSolution
Equating the Coulomb attraction to the required centripetal force, and combining it with Bohr's quantization of angular momentum, gives the radius of the nth orbit as r_n = n²h²ε0/(πme²) — increasing as the square of the orbit number n.
Step 1 — Centripetal force condition: In Bohr's model, an electron of mass m and charge −e moves in a circular orbit of radius r around the nucleus (charge +e for hydrogen), held in orbit by the electrostatic (Coulomb) force acting as the centripetal force:
(1/4πε0) × e²/r² = mv²/r
⟹ mv² = e² / (4πε0 r) ... (1)
Step 2 — Bohr's quantization postulate: The angular momentum of the electron is quantized in integral multiples of h/2π:
mvr = nh/2π ⟹ v = nh / (2πmr) ... (2)
Step 3 — Combine (1) and (2): Substitute v from (2) into (1):
m × [nh/(2πmr)]² = e²/(4πε0 r)
n²h² / (4π²mr²) = e² / (4πε0 r)
Multiplying both sides by r and rearranging for r:
n²h² / (4π²mr) = e² / (4πε0)
r = n²h² × 4πε0 / (4π²me²)
r_n = n²h²ε0 / (πme²)
This shows the orbit radius increases as the square of the quantum number n (r_n ∝ n²) — for hydrogen, r1 works out to about 0.53 Å (the Bohr radius), r2 = 4 × 0.53 Å, and so on.
✓Final answerr_n = n²h²ε0 / (πme²) — derived from equating the Coulomb force to the centripetal force and using Bohr's angular-momentum quantization mvr = nh/2π.
- JKBOSE Class 12 Annual Regular Examination 2023Set ANNUAL3 marksQ.Write the postulates of Bohr's modal of hydrogen atom.
›Reveal solutionSolution
Bohr's model of the hydrogen atom rests on three postulates: stable non-radiating orbits, quantized angular momentum (mvr = nh/2pi), and photon emission/absorption only during transitions between orbits (h*nu = delta-E).
Niels Bohr proposed the following postulates to explain the stability of atoms and the discrete (line) spectrum of hydrogen, combining classical mechanics with early quantum ideas:
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Postulate of stationary (stable) orbits: An electron in an atom revolves around the nucleus only in certain specific, permitted circular orbits, called stationary orbits, without radiating energy - even though it is accelerating (contrary to classical electromagnetic theory, which would predict continuous energy loss and the electron spiralling into the nucleus). In these orbits, the necessary centripetal force is provided by the electrostatic (Coulomb) attraction between the electron and the nucleus.
-
Postulate of quantization of angular momentum: Only those orbits are permitted (stable) for which the angular momentum of the electron is an integral multiple of h/(2pi): L = mvr = nh/(2*pi), where n = 1, 2, 3, ... is the principal quantum number, m is electron mass, v its orbital speed, r the orbit radius, and h is Planck's constant.
-
Postulate of frequency condition (radiation postulate): An atom radiates (emits) energy only when an electron makes a transition from a higher-energy stationary orbit to a lower-energy one, and it absorbs energy when the electron jumps from a lower to a higher orbit. The energy of the photon emitted or absorbed equals the difference in energy of the two orbits: h*nu = E2 - E1 (or E_i - E_f), where nu is the frequency of the emitted/absorbed radiation and h is Planck's constant. While the electron remains in a given stationary orbit, no radiation occurs regardless of its acceleration.
These three postulates together successfully explained the stability of the hydrogen atom and correctly predicted its observed line spectrum (Balmer, Lyman series, etc.).
✓Final answerBohr's postulates: (i) electrons move in stable, non-radiating circular orbits;
(ii) angular momentum is quantized, L = nh/(2pi);
(iii) radiation is emitted/absorbed only during a transition between orbits, with photon energy h*nu = E2 - E1.
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- JKBOSE Class 12 Annual Regular Examination 2022Set SZ3 marksQ.Write down the postulates of Bohr's model of hydrogen atom.
›Reveal solutionSolution
Bohr postulated stationary orbits with quantised angular momentum, and that spectral lines arise from photon emission/absorption during transitions between these orbits.
Niels Bohr proposed the following postulates for the hydrogen atom, combining classical mechanics with quantum ideas:
-
Stationary (stable) orbits: An electron in an atom revolves around the nucleus in certain fixed, stable circular orbits without radiating energy, contrary to what classical electromagnetic theory (an accelerating charge should continuously radiate energy) would predict. These allowed orbits are called stationary states.
-
Quantisation of angular momentum: The electron can revolve only in those orbits for which its orbital angular momentum is an integral multiple of h/2π:
mvr=2πnh,n=1,2,3,…
where n is called the principal quantum number.
-
Emission/absorption on transition: An electron can transition ("jump") from one stationary orbit to another. When it jumps from a higher energy orbit (E2) to a lower one (E1), it emits a photon of energy equal to the energy difference; conversely, it absorbs a photon of that energy to jump from the lower to the higher orbit:
hν=E2−E1
These postulates successfully explained the discrete line spectrum of hydrogen (the various spectral series such as Lyman, Balmer, Paschen) and gave correct values for the energy levels and radius of the hydrogen atom.
✓Final answerBohr's three postulates: stationary non-radiating orbits; quantised angular momentum mvr=nh/2π; photon of energy hν=E2−E1 emitted/absorbed on transition between orbits.
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- JKBOSE Class 12 Annual Regular Examination 2021Set SZ3 marksQ.State the basic postulates of Bohr's model of atom.
›Reveal solutionSolution
Bohr combined classical mechanics with quantum ideas: electrons orbit without radiating, only in orbits with quantised angular momentum, and photons are emitted/absorbed only during a jump between orbits.
Niels Bohr proposed three basic postulates to explain the stability of atoms and the discrete line spectra observed (overcoming the problem that a classically accelerating orbiting electron should radiate energy continuously and spiral into the nucleus):
1. Postulate of stationary orbits: An electron in an atom can revolve only in certain special, discrete circular orbits, called stationary states or orbits, without radiating energy, even though it is undergoing centripetal acceleration. In these orbits, the electrostatic force of attraction between the nucleus and electron provides the necessary centripetal force:
4πε01r2Ze2=rmv2
2. Postulate of quantisation of angular momentum: Only those orbits are allowed for which the angular momentum of the electron is an integral multiple of h/2π:
L=mvr=2πnh,n=1,2,3,…
where n is called the principal quantum number.
3. Postulate of quantum jumps (frequency condition): An atom radiates (or absorbs) energy only when an electron jumps from a higher energy orbit to a lower one (or vice versa). The energy of the emitted/absorbed photon equals the difference in energy between the two orbits:
hν=Ei−Ef
where Ei and Ef are the energies of the initial and final orbits.
These three postulates together successfully explained the stability of the hydrogen atom and the observed discrete spectral lines (Lyman, Balmer, Paschen series, etc.).
✓Final answerBohr's postulates: electrons move in non-radiating stationary orbits; angular momentum is quantised as L=nh/2π; energy is emitted/absorbed as a photon only during a transition between orbits, hν=Ei−Ef.
- JKBOSE Class 12 Annual Regular Examination 2020Set SZ3 marksQ.State postulates of Bohr's theory of Hydrogen atom.
›Reveal solutionSolution
Bohr's three postulates fix stable non-radiating orbits with quantised angular momentum, and explain spectral lines as photon emission/absorption during orbit jumps.
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Stationary orbits postulate: An electron in an atom revolves around the nucleus in certain fixed circular orbits, called stationary orbits, without radiating any energy, even though it is accelerating (which classically should cause continuous radiation and spiral collapse into the nucleus).
-
Quantisation of angular momentum: Only those orbits are permitted for which the angular momentum of the electron is an integral multiple of h/2π (h being Planck's constant):
mvr = nh/2π, n = 1, 2, 3, …
where n is called the principal quantum number.
-
Frequency condition (transition postulate): An electron can jump from one stationary orbit to another. When it jumps from a higher energy orbit E₂ to a lower energy orbit E₁, the energy difference is emitted as a photon of frequency ν given by
hν = E₂ − E₁
Conversely, the atom absorbs a photon of exactly this energy to jump from E₁ to E₂.
✓Final answer(1) Electrons move in fixed non-radiating stationary orbits. (2) Angular momentum is quantised, mvr = nh/2π. (3) Energy is emitted/absorbed only on transition between orbits, hν = E₂ − E₁.
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