Q.The radius of the innermost electron orbit of a hydrogen atom is 5.3×10−11 m. What are the radii of the n=2 and n=3 orbits?
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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 …
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 …
The key idea is that in the Bohr model, the radius of the n-th orbit is quantized as rn=n2r1, where r1 is the radius of the innermost orbit (n=1).
Given r1=5.3×10−11 m:
- For n=2: r2=22×r1=4×5.3×10−11=2.12×10−10 m. …
In the Bohr model, the radius of an electron orbit scales as n2 times the Bohr radius r1. Given r1=5.3×10−11 m, the radii for n=2 and n=3 are 2.12×10−10 m and 4.77×10−10 m, respectively.
The Bohr model of the hydrogen atom is built on a simple but powerful idea: the electron can only occupy certain allowed orbits where its angular momentum is an integer multiple of 2πh. This quantization condition leads directly to a neat scaling law for orbit radii.
For a hydrogen-like atom (one electron orbiting a nucleus of charge +Ze), the centripetal force comes from the Coulomb attraction:
rmv2=4πε01r2Ze2
Combine this with Bohr’s quantization of angular momentum:
mvr=n2πh
Solving these two equations eliminates v and gives the radius of the nth orbit:
rn=4π2me24πε0h2⋅Zn2=a0Zn2
where a0=5.3×10−11 m is the Bohr radius — the radius of the innermost orbit (n=1) for hydrogen (Z=1).
rn=n2⋅r1
This is the key: the radius grows as the square of the principal quantum number n. No need to re-derive constants each time — once you know r1, all higher orbits follow immediately.
Now let’s apply it step by step.
-
Identify the given data.
The innermost orbit radius r1=5.3×10−11 m. This is the Bohr radius for hydrogen.
-
Write the general relation.
For hydrogen (Z=1):
rn=n2⋅r1
- Find r2 (for n=2). …
Method: Direct Application of Bohr's Radius Formula
Bohr's model tells us that the radius of an electron orbit in a hydrogen atom is proportional to n2, where n is the principal quantum number. The innermost orbit (n=1) has a known radius r1=5.3×10−11 m.
The formula is:
rn=n2⋅r1
Steps:
-
Identify the given data
r1=5.3×10−11 m
We need r2 and r3.
-
Apply the formula for n=2
r2=22⋅r1=4×(5.3×10−11)=2.12×10−10 m
- Apply the formula for n=3 r3=32⋅r1=9×(5.3×10−11)=4.77×10−10 m …
The most common mistake here is forgetting that the Bohr radius scales as n2, not n. Students often multiply the given radius by n instead of n2, so for n=2 they write 2×5.3×10−11 m, and for n=3 they write 3×5.3×10−11 m. That is wrong.
Why it happens: The formula rn=n2r1 comes directly from the quantization condition mvr=nℏ combined with the Coulomb force balance. The n2 dependence is a key result — it is not obvious from a quick glance, so students misremember it as linear.
How to avoid: Always write the proportionality explicitly before plugging numbers:
rn∝n2
Then, for n=2:
r2=22×r1=4×5.3×10−11 m=2.12×10−10 m
For n=3:
r3=32×r1=9×5.3×10−11 m=4.77×10−10 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:
…
- 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:
-
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.
…
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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.
…
-
- 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.
…
- 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.
- 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. …
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