NCERT Solutions for Class 12 Physics Chapter 12: Atoms
All 9 exercise questions of the latest NCERT textbook (2026–27 reprint) solved like a topper’s answer-sheet — Thomson and Rutherford models, alpha-particle scattering, Bohr’s postulates, energy levels, speeds and radii of hydrogen orbits and the hydrogen spectral series — with energy-level diagrams linked to the exact NCERT pages, comparison tables, complete revision notes and exam tips.
Chapter at a glance — complete revision notes
12.1 Introduction
- By the nineteenth century enough evidence had accumulated for the atomic hypothesis. J. J. Thomson (1898) proposed the first model (the “plum pudding” / watermelon model): the positive charge is uniformly distributed over the whole atom (size ≈ 10⁻¹⁰ m) with the negatively charged electrons embedded in it, the atom being neutral. Light from rarefied gases (neon sign, mercury vapour lamps) has only certain discrete wavelengths (a line spectrum, characteristic of each element), unlike the continuous spectrum of a hot solid — a clue to the internal structure of the atom. Balmer (1885) found an empirical formula for a group of hydrogen lines.
- Rutherford (a student of Thomson) proposed in 1906 an experiment on the scattering of α-particles; it was performed around 1911 by Hans Geiger and Ernst Marsden (Marsden, 20, had not yet earned his bachelor’s degree), leading to Rutherford’s planetary (nuclear) model: all the positive charge and most of the mass in a small nucleus, with electrons revolving like planets. It could not explain why atoms emit only discrete wavelengths — the problem solved by Bohr’s quantum ideas.
12.2 Alpha-particle scattering and Rutherford’s nuclear model of the atom
- Geiger–Marsden experiment (Figs 12.1, 12.2): α-particles (from ²¹⁴₈₃Bi, ≈ 5.5 MeV) are collimated and directed at a thin gold foil (2.1 × 10⁻⁷ m thick) in a vacuum chamber; a rotatable detector (zinc sulphide screen and microscope) counts the scattered particles at different angles. Results (Fig. 12.3): most α-particles pass through undeviated; only about 0.14 % scatter by more than 1° and about 1 in 8000 deflect by more than 90°.
- Interpretation: to turn an α-particle back, a very large repulsive force is needed — due to a small, dense, positively charged nucleus; the electrons, so light, do not appreciably affect the α-particles. The positive charge and most of the mass of the atom are concentrated in a nucleus of size ≈ 10⁻¹⁵ m (the electrons being at a distance of 10,000 to 100,000 times the size of the nucleus), so most of the atom is empty space. The scattering data fit the theoretical curve based on the nuclear model (single scattering by a nucleus of charge Ze, Z = 79 for gold; the gold nucleus is ~50 times heavier than the α-particle so it is assumed stationary).
12.2.1 Alpha-particle trajectory (Fig. 12.4)
The force is the Coulomb repulsion F = (1/4πε₀)(2Ze²/r²); the trajectory depends on the impact parameter b — the perpendicular distance of the initial velocity vector from the centre of the nucleus: a head-on collision (b ≈ 0) gives scattering through 180°, large b gives small deflection. The distance of closest approach for a head-on collision: ½mv² = (1/4πε₀)(2Ze²/d) ⇒ d = (1/4πε₀)(2Ze²)/K; for a 7.7 MeV α-particle on gold d = 3.0 × 10⁻¹⁴ m (30 fm), an upper limit for the nuclear radius (the actual radius is ~6 fm). Example 12.1: if the solar system had the same proportions as the atom (orbit/nucleus ≈ 10⁵), the Earth’s orbit would be 7 × 10¹³ m — more than 100 times the actual radius: the atom contains a much greater fraction of empty space than the solar system.12.2.2 Electron orbits
The electrostatic attraction provides the centripetal force: mv²/r = e²/(4πε₀r²), i.e. r = e²/(4πε₀mv²); K = ½mv² = e²/(8πε₀r), U = −e²/(4πε₀r), so the total energy E = K + U = −e²/(8πε₀r), negative: the electron is bound. Example 12.3: 13.6 eV is required to separate hydrogen into a proton and an electron ⇒ E = −13.6 eV ⇒ orbital radius r = 5.3 × 10⁻¹¹ m and speed 2.2 × 10⁶ m s⁻¹.
12.3 Atomic spectra
- Each element has a characteristic emission line spectrum (excited gas at low pressure). When white light passes through the gas, the absorption spectrum shows dark lines at precisely the wavelengths found in the emission spectrum. Hydrogen series (Fig. 12.5): Balmer series (visible): 1/λ = R(1/2² − 1/n²), n = 3, 4, 5, … with the Rydberg constant R = 1.097 × 10⁷ m⁻¹; the other series: Lyman (UV, final level 1), Paschen (final 3), Brackett (final 4), Pfund (final 5) (infrared). General: 1/λ = R(1/p² − 1/n²), n > p.
- Failure of Rutherford’s model: an electron in circular motion is accelerated; according to classical electromagnetic theory it should radiate and lose energy, spiralling into the nucleus (Fig. 12.6), emitting radiation of continuously changing frequency (a continuous spectrum) — contrary to the stable atoms and line spectra observed. Example 12.4: the classical frequency for the orbit of radius 5.3 × 10⁻¹¹ m: ν = v/(2πr) = 6.6 × 10¹⁵ Hz.
12.4 Bohr model of the hydrogen atom
- Bohr (1913), who had studied in Rutherford’s laboratory in 1912, added quantum ideas to Rutherford’s model with three postulates: (i) an electron in an atom revolves in certain stable orbits (stationary states) without radiating energy, in spite of its acceleration; (ii) only those orbits are allowed for which the angular momentum is an integral multiple of h/2π: L = mvr = nh/2π (n = 1, 2, 3, …, the principal quantum number); (iii) the electron can make a transition from one stationary state to another of lower energy with the emission of a photon of energy hν = E_i − E_f (and absorbs a photon of the same energy to go up).
- Results: radius of the n-th orbit r_n = n² (h/2π)²(4πε₀)/(m e²) = n² a₀, with the Bohr radius a₀ = 0.529 Å = 5.3 × 10⁻¹¹ m (r₁); speed v_n = e²/(2ε₀ n h) = v₁/n (v₁ = 2.19 × 10⁶ m s⁻¹ ≈ c/137); 12.4.1 energy levels: E_n = −me⁴/(8ε₀²h²) (1/n²) = −13.6 eV/n² (ground state E₁ = −13.6 eV, E₂ = −3.4 eV, E₃ = −1.51 eV, E₄ = −0.85 eV…; ionisation energy 13.6 eV); K = −E, U = 2E. The Rydberg constant comes out as R = me⁴/(8ε₀²h³c) = 1.03 × 10⁷ m⁻¹ (close to the empirical value).
- Ground and excited states: the lowest energy state (n = 1) is the ground state; the others are excited states with lifetimes ~10⁻⁸ s before returning to lower levels by photon emission.
12.5 The line spectra of the hydrogen atom (Fig. 12.7)
- With hν = E_i − E_f: 1/λ = (me⁴/8ε₀²h³c)(1/n_f² − 1/n_i²), reproducing the Balmer and other series. Energy-level diagram (Fig. 12.7): Lyman series (transitions to n = 1, ultraviolet), Balmer (to n = 2, visible), Paschen (to n = 3), Brackett (to n = 4), Pfund (to n = 5) (infrared). An electron in a low level can be excited by absorbing a photon of exactly the right energy (absorption spectrum) or by collision with an electron of enough energy. The model is successful for hydrogen and hydrogen-like ions but cannot be extended to multi-electron atoms.
12.6 De Broglie’s explanation of Bohr’s second postulate of quantisation
- One of Bohr’s postulates (L = nh/2π) was unexplained until de Broglie (1923) proposed that an electron moving in a circular orbit is a standing wave: the circumference must contain an integral number of wavelengths: 2πr_n = nλ (Fig. 12.8), and with λ = h/mv this gives mvr_n = nh/2π. The wave picture also explains why the electron does not radiate in a stationary orbit (a standing wave does not carry energy). (Bohr’s postulates remain approximate; the full quantum mechanical atom is described by wave mechanics — Schrödinger.)
Summary & key points (NCERT)
- Thomson’s model (uniform positive sphere with embedded electrons) vs Rutherford’s nuclear model (explaining large-angle scattering); instability and the continuous-spectrum problem of the classical nuclear atom; Bohr’s postulates; r_n ∝ n², v_n ∝ 1/n, E_n ∝ −1/n²; hydrogen spectral series; de Broglie’s standing-wave explanation of L = nh/2π.
Choose the correct alternative from the clues given at the end of the each statement: (a) The size of the atom in Thomson’s model is ………. the atomic size in Rutherford’s model. (much greater than/no different from/much less than.) (b) In the ground state of ………. electrons are in stable equilibrium, while in ………. electrons always experience a net force. (Thomson’s model/ Rutherford’s model.) (c) A classical atom based on ………. is doomed to collapse. (Thomson’s model/ Rutherford’s model.) (d) An atom has a nearly continuous mass distribution in a ………. but has a highly non-uniform mass distribution in ………. (Thomson’s model/ Rutherford’s model.) (e) The positively charged part of the atom possesses most of the mass in ………. (Rutherford’s model/both the models.)
Concept and context. Thomson’s model (1898) pictures the atom as a sphere of uniformly distributed positive charge (radius ≈ 10⁻¹⁰ m, the size of the atom) in which the electrons are embedded like plums in a pudding; the positive charge and the mass are spread over the whole atom. Rutherford’s nuclear model (1911), inferred from the Geiger–Marsden α-particle scattering experiment (about 1 α-particle in 8000 deflects by more than 90°), concentrates all the positive charge and almost all the mass in a tiny nucleus (≈ 10⁻¹⁵ m) with the electrons revolving around it at distances of the order of the atomic size (10⁻¹⁰ m). Each blank below is answered using these two pictures.
| Part | Answer | Reason |
|---|---|---|
| (a) Size of the atom in Thomson’s model … the atomic size in Rutherford’s model | no different from | in Thomson’s model the atom is a sphere of diameter ~10⁻¹⁰ m; in Rutherford’s model the electron orbits have a radius of ~10⁻¹⁰ m, which defines the size of the atom (the nucleus itself is ~10⁻¹⁵ m) — the two models give the same atomic size |
| (b) Stable equilibrium in the ground state / always a net force | Thomson’s model (stable equilibrium); Rutherford’s model (net force) | in Thomson’s model the electron sits at the centre of the positive sphere in equilibrium (net force zero, restoring force if displaced — a stable equilibrium); in Rutherford’s model the electron always experiences the attractive Coulomb force of the nucleus (it needs this net force as the centripetal force to stay in its orbit) |
| (c) A classical atom doomed to collapse | Rutherford’s model | the orbiting electron is accelerated and, by classical electromagnetic theory, radiates energy and spirals into the nucleus |
| (d) Nearly continuous mass distribution / highly non-uniform mass distribution | Thomson’s model (continuous); Rutherford’s model (non-uniform) | Thomson: mass spread throughout the sphere; Rutherford: almost all the mass in the tiny nucleus, the rest of the atom nearly empty space |
| (e) The positively charged part possesses most of the mass in … | both the models | in Thomson’s model the positive sphere carries the mass (the electrons are very light, 1/1836 of a proton), and in Rutherford’s model the nucleus carries it |
- Detail for (a): the radius of the nucleus (10⁻¹⁵ m) is about 10⁵ times smaller than the orbit radius; the “size of the atom” is the orbit size ≈ 10⁻¹⁰ m in the Rutherford model and the radius of the positive sphere ≈ 10⁻¹⁰ m in the Thomson model — equal.
- Detail for (b): in Thomson’s model the force on an electron displaced r from the centre of a uniformly positive sphere is proportional to r and directed towards the centre (like a spring): the equilibrium at the centre is stable and the electron can oscillate with a definite frequency. In Rutherford’s model, there is no position of zero force; the electron survives only because it is moving (centripetal acceleration).
- Detail for (c): an electron revolving around the nucleus is continuously accelerated; the radiation would take away its energy, so the orbit radius would shrink and the electron would spiral into the nucleus — and the emission would be a continuous spectrum, contradicting both the stability of atoms and the line spectra (NCERT Example 12.4: ν ≈ 6.6 × 10¹⁵ Hz initially).
- Detail for (d): Thomson’s model could not explain the large-angle scattering of α-particles, because a smeared charge cannot exert a strong enough force to turn an α-particle back; the non-uniform (nuclear) distribution of Rutherford’s model can.
Conclusion: (a) no different from; (b) Thomson’s model / Rutherford’s model; (c) Rutherford’s model; (d) Thomson’s model / Rutherford’s model; (e) both the models.
Suppose you are given a chance to repeat the alpha-particle scattering experiment using a thin sheet of solid hydrogen in place of the gold foil. (Hydrogen is a solid at temperatures below 14 K.) What results do you expect?
Concept and context. In the Geiger–Marsden experiment (NCERT Fig. 12.1) the large-angle scattering of α-particles (about 1 in 8000 by more than 90°) by gold atoms arises because the α-particle (mass 4 u, charge 2e) is repelled by a very massive, highly charged nucleus (gold: Z = 79, mass ≈ 197 u ≈ 50 times heavier than the α-particle) which hardly recoils. A hydrogen nucleus is a single proton (mass ≈ 1 u, charge +e), lighter than the incident α-particle. The nature of the scattering therefore changes completely.
- Heavier projectile, lighter target: the mass of an α-particle (≈ 4 u) is about four times that of the proton (≈ 1 u). In an elastic collision with a nearly stationary particle that is lighter than the projectile, momentum conservation shows the projectile cannot be turned back or deflected through a large angle: the maximum deflection angle of the α-particle satisfies sin θ_max = m_p/m_α = 1/4, so θ_max ≈ 14.5°. It is like a bowling ball hitting a table-tennis ball — the heavy object ploughs on almost undisturbed while the light one is knocked away.
- Weaker Coulomb force: the charge of a hydrogen nucleus (+e) is also small (compared with +79e of gold), so the repulsive force on the α-particle (F = (1/4πε₀)(2e × e)/r²) is much weaker and the closest-approach energy barrier much smaller: the α-particle (even at a few MeV) can approach very close to the proton and still lose only a small part of its momentum.
- Expected result: no large-angle scattering (no back-scattering at all); almost all α-particles go straight through the thin solid hydrogen sheet with only small deflections (below about 14.5°), and the hydrogen nuclei (protons) are knocked out of the sheet in the forward direction — these recoil protons could be detected. The conclusions drawn from gold (a small massive positive nucleus) therefore could not have been drawn from a hydrogen target.
| Feature | Gold foil | Solid hydrogen foil |
|---|---|---|
| Target nucleus | Z = 79, mass ≈ 197 u (≈ 50 × m_α) | Z = 1, mass ≈ 1 u (≈ m_α/4) |
| Large-angle scattering (> 90°) | yes (≈ 1 in 8000) | none |
| Maximum deflection of the α-particle | up to 180° (head-on) | ≈ 14.5° (sin θ = m_p/m_α) |
| Recoil of the target nucleus | negligible | large (protons knocked forward) |
| Conclusion | shows the nuclear atom | no information on the nucleus |
- Why gold was chosen: a heavy, high-Z, malleable metal that can be rolled into a very thin foil (2.1 × 10⁻⁷ m, a few thousand atoms thick) so that single scattering by the nucleus dominates.
- Also: energy conservation: the momentum transferred to a light proton is small, so the α-particle loses only a modest amount of energy.
Conclusion: with a solid hydrogen foil no large-angle scattering would be observed — the α-particles would pass through with only small deflections (at most ≈ 14.5°) while the lighter protons recoil forward — so the experiment would not reveal the nuclear structure as gold does.
A difference of 2.3 eV separates two energy levels in an atom. What is the frequency of radiation emitted when the atom makes a transition from the upper level to the lower level?
Concept and context. According to Bohr’s third postulate, when an atom makes a transition from a higher energy state of energy E_i to a lower one of energy E_f, it emits a photon whose energy equals the difference between the energies of the two states: hν = E_i − E_f (NCERT Section 12.4). The frequency of the emitted radiation therefore follows directly from the energy gap: ν = (E_i − E_f)/h. Conversely, an atom can absorb a photon of exactly this frequency to move up.
Given: E_i − E_f = 2.3 eV = 2.3 × 1.6 × 10⁻¹⁹ J = 3.68 × 10⁻¹⁹ J; h = 6.63 × 10⁻³⁴ J s.
- Photon energy: hν = 3.68 × 10⁻¹⁹ J.
- Frequency: ν = (3.68 × 10⁻¹⁹)/(6.63 × 10⁻³⁴) = 5.55 × 10¹⁴ Hz.
ν = ΔE/h = 5.55 × 10¹⁴ Hz
| Quantity | Value |
|---|---|
| Energy gap ΔE | 2.3 eV = 3.68 × 10⁻¹⁹ J |
| Frequency ν = ΔE/h | 5.55 × 10¹⁴ Hz |
| Wavelength λ = c/ν = 1240/2.3 nm | 540 nm (green) |
| Region of the spectrum | visible (green) |
- Check: λ = hc/ΔE = 1240 eV nm/2.3 eV = 539 nm; 3 × 10⁸/5.55 × 10¹⁴ = 5.4 × 10⁻⁷ m ✓.
- Meaning: energy gaps of a few eV between the levels of atoms produce visible light (1.8–3.1 eV); smaller gaps give infrared and larger gaps ultraviolet, as in the series of hydrogen.
Conclusion: the frequency of the radiation emitted is 5.55 × 10¹⁴ Hz (green light of wavelength about 540 nm).
The ground state energy of hydrogen atom is −13.6 eV. What are the kinetic and potential energies of the electron in this state?
Concept and context. In the Bohr (and Rutherford) model the electron of a hydrogen atom moves in a circular orbit of radius r under the attractive Coulomb force which provides the centripetal force: mv²/r = e²/(4πε₀r²). From this, the kinetic energy is K = ½mv² = e²/(8πε₀r), the electrostatic potential energy (zero at infinity) is U = −e²/(4πε₀r), so U = −2K and the total energy is E = K + U = −e²/(8πε₀r) = −K (NCERT Section 12.2.2, Eqs 12.3–12.4). The total energy is negative: the electron is bound to the nucleus. Hence K = −E and U = 2E.
Given: total energy of the ground state E = −13.6 eV.
- Kinetic energy: K = −E = +13.6 eV (= 2.2 × 10⁻¹⁸ J).
- Potential energy: U = 2E = −27.2 eV (= −4.4 × 10⁻¹⁸ J).
- Check: K + U = 13.6 − 27.2 = −13.6 eV = E ✓.
K = +13.6 eV ; U = −27.2 eV
| Energy | Expression | Value in the ground state |
|---|---|---|
| Kinetic K | e²/(8πε₀r) = −E | +13.6 eV |
| Potential U | −e²/(4πε₀r) = 2E | −27.2 eV |
| Total E | −e²/(8πε₀r) | −13.6 eV |
| Ionisation energy | −E | 13.6 eV |
- Virial relation: for an inverse-square force law, 2K = −U (the “virial theorem”) — the result is general for all Bohr orbits: K_n = 13.6/n² eV, U_n = −27.2/n² eV.
- Meaning of E = −13.6 eV: 13.6 eV of energy must be supplied to the electron to free it (E = 0 at rest at infinity): the ionisation energy of hydrogen.
Conclusion: the kinetic energy of the electron is +13.6 eV and its potential energy is −27.2 eV.
A hydrogen atom initially in the ground level absorbs a photon, which excites it to the n = 4 level. Determine the wavelength and frequency of photon.
Concept and context. By Bohr’s third postulate an atom can absorb a photon only if its energy exactly equals the difference between two stationary-state energies: hν = E_f − E_i. The energy of the n-th level of hydrogen is E_n = −13.6 eV/n²: E₁ = −13.6 eV, E₂ = −3.40 eV, E₃ = −1.51 eV, E₄ = −0.85 eV (NCERT Fig. 12.7). The photon needed to excite the atom from n = 1 to n = 4 has energy E₄ − E₁.
Given: n_i = 1, n_f = 4; E_n = −13.6/n² eV; h = 6.63 × 10⁻³⁴ J s; c = 3 × 10⁸ m s⁻¹.
- Energy of the photon: ΔE = E₄ − E₁ = −0.85 − (−13.6) = 12.75 eV (= 12.75 × 1.6 × 10⁻¹⁹ = 2.04 × 10⁻¹⁸ J).
- Frequency: ν = ΔE/h = (2.04 × 10⁻¹⁸)/(6.63 × 10⁻³⁴) = 3.08 × 10¹⁵ Hz.
- Wavelength: λ = c/ν = (3 × 10⁸)/(3.08 × 10¹⁵) = 9.74 × 10⁻⁸ m = 97.4 nm (also 1240/12.75 = 97.3 nm).
ΔE = 12.75 eV ; ν = 3.08 × 10¹⁵ Hz ; λ ≈ 97 nm
| Quantity | Value |
|---|---|
| Energy of the photon | 12.75 eV |
| Frequency | 3.08 × 10¹⁵ Hz |
| Wavelength | 97.4 nm |
| Region | ultraviolet (Lyman series: n = 4 → 1 line when the atom returns) |
- Check with the Rydberg formula: 1/λ = R(1/1² − 1/4²) = 1.097 × 10⁷ × 15/16 = 1.028 × 10⁷ m⁻¹ ⇒ λ = 97.3 nm ✓.
- After absorption the atom (in the excited state n = 4) may return to the ground state in one step (emitting the same 97.3 nm photon) or by cascading through intermediate levels (4 → 3 → 2 → 1, etc.), giving several spectral lines (Lyman, Balmer, Paschen series).
Conclusion: the photon has energy 12.75 eV, frequency 3.08 × 10¹⁵ Hz and wavelength ≈ 97 nm (ultraviolet).
(a) Using the Bohr’s model calculate the speed of the electron in a hydrogen atom in the n = 1, 2, and 3 levels. (b) Calculate the orbital period in each of these levels.
Concept and context. In the Bohr model the electron revolves in a circular orbit satisfying (i) the centripetal force condition mv²/r = e²/(4πε₀r²) and (ii) the quantisation of angular momentum mvr = nh/2π. Together these give the radius r_n = n² a₀ (a₀ = 5.3 × 10⁻¹¹ m, the Bohr radius) and the speed v_n = e²/(2ε₀nh) = v₁/n where v₁ = 2.19 × 10⁶ m s⁻¹ (the speed in the first orbit ≈ c/137). The orbital period T_n = 2πr_n/v_n = 2π n² a₀/(v₁/n) = n³T₁ with T₁ = 2πa₀/v₁.
Given: v₁ = e²/(2ε₀h) = (1.6 × 10⁻¹⁹)²/(2 × 8.85 × 10⁻¹² × 6.63 × 10⁻³⁴) = 2.18 × 10⁶ m s⁻¹; r₁ = 5.3 × 10⁻¹¹ m.
(a) Speeds
- n = 1: v₁ = 2.18 × 10⁶ m s⁻¹ (≈ c/137).
- n = 2: v₂ = v₁/2 = 1.09 × 10⁶ m s⁻¹.
- n = 3: v₃ = v₁/3 = 7.27 × 10⁵ m s⁻¹.
(b) Orbital periods
- n = 1: r₁ = 5.3 × 10⁻¹¹ m; T₁ = 2πr₁/v₁ = (2 × 3.14 × 5.3 × 10⁻¹¹)/(2.18 × 10⁶) = 1.52 × 10⁻¹⁶ s.
- n = 2: r₂ = 4r₁ = 2.12 × 10⁻¹⁰ m; T₂ = 2πr₂/v₂ = (2 × 3.14 × 2.12 × 10⁻¹⁰)/(1.09 × 10⁶) = 1.22 × 10⁻¹⁵ s (= 8T₁).
- n = 3: r₃ = 9r₁ = 4.77 × 10⁻¹⁰ m; T₃ = 2πr₃/v₃ = (2 × 3.14 × 4.77 × 10⁻¹⁰)/(7.27 × 10⁵) = 4.12 × 10⁻¹⁵ s (= 27T₁).
| Level n | Radius r_n (m) | Speed v_n (m/s) | Period T_n (s) | Frequency of revolution (Hz) |
|---|---|---|---|---|
| 1 | 5.3 × 10⁻¹¹ | 2.18 × 10⁶ | 1.52 × 10⁻¹⁶ | 6.6 × 10¹⁵ |
| 2 | 2.12 × 10⁻¹⁰ | 1.09 × 10⁶ | 1.22 × 10⁻¹⁵ | 8.2 × 10¹⁴ |
| 3 | 4.77 × 10⁻¹⁰ | 7.27 × 10⁵ | 4.12 × 10⁻¹⁵ | 2.4 × 10¹⁴ |
- Scaling laws: r_n ∝ n², v_n ∝ 1/n, T_n ∝ n³, E_n ∝ −1/n². The speed of the electron falls as it goes to higher orbits; the revolution frequency falls as n⁻³.
- Relativity check: v₁/c = 2.18 × 10⁶/3 × 10⁸ = 0.7 % — the non-relativistic Bohr treatment is a good approximation (fine-structure constant α = v₁/c ≈ 1/137).
Conclusion: (a) v = 2.18 × 10⁶, 1.09 × 10⁶ and 7.27 × 10⁵ m s⁻¹; (b) T = 1.52 × 10⁻¹⁶ s, 1.22 × 10⁻¹⁵ s and 4.12 × 10⁻¹⁵ s for n = 1, 2, 3 respectively.
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?
Concept and context. In the Bohr model the radius of the n-th stationary orbit of hydrogen is r_n = n² r₁ where r₁ = a₀ = (h/2π)²(4πε₀)/(me²) = 5.3 × 10⁻¹¹ m is the Bohr radius. The radius thus increases as the square of the principal quantum number — a consequence of the quantisation of angular momentum (mvr = nh/2π) combined with the Coulomb force law.
- n = 2: r₂ = 2² × r₁ = 4 × 5.3 × 10⁻¹¹ = 2.12 × 10⁻¹⁰ m (≈ 0.212 nm).
- n = 3: r₃ = 3² × r₁ = 9 × 5.3 × 10⁻¹¹ = 4.77 × 10⁻¹⁰ m (≈ 0.477 nm).
r₂ = 4r₁ = 2.12 × 10⁻¹⁰ m ; r₃ = 9r₁ = 4.77 × 10⁻¹⁰ m
| n | r_n = n² r₁ | Radius |
|---|---|---|
| 1 | 1 × r₁ | 5.3 × 10⁻¹¹ m |
| 2 | 4 × r₁ | 2.12 × 10⁻¹⁰ m |
| 3 | 9 × r₁ | 4.77 × 10⁻¹⁰ m |
| 4 | 16 × r₁ | 8.48 × 10⁻¹⁰ m |
- Interpretation: higher orbits are much larger — the n = 3 orbit has a radius nine times that of the ground state; the atom swells as the electron is excited (the size ~10⁻¹⁰ m of the ground-state atom).
- Derivation: from mv²/r = e²/4πε₀r² and mvr = nh/2π: v = nh/(2πmr) ⇒ m (nh/2πmr)²/r = e²/(4πε₀r²) ⇒ r = n²h²ε₀/(πme²) ∝ n².
Conclusion: the radii of the second and third Bohr orbits are 2.12 × 10⁻¹⁰ m and 4.77 × 10⁻¹⁰ m.
A 12.5 eV electron beam is used to bombard gaseous hydrogen at room temperature. What series of wavelengths will be emitted?
Concept and context. Hydrogen atoms at room temperature are in the ground state (n = 1, E₁ = −13.6 eV). An incident electron can excite an atom by collision if its kinetic energy is at least equal to the energy needed to raise the atom to a higher level (the excess energy stays with the electron). The energy needed to excite from n = 1 to the n-th level is E_n − E₁ = 13.6(1 − 1/n²) eV: 10.2 eV (n = 2), 12.09 eV (n = 3), 12.75 eV (n = 4), … Because the bombarding electrons have only 12.5 eV, the atoms can be excited to levels up to n = 3 (12.09 eV ≤ 12.5 eV) but not to n = 4 (12.75 eV > 12.5 eV). The excited atoms then return to lower levels, emitting photons of wavelengths given by hν = E_i − E_f.
Step 1 — highest level reachable
- E₃ − E₁ = −1.51 − (−13.6) = 12.09 eV < 12.5 eV ✓ (n = 3 can be reached).
- E₄ − E₁ = −0.85 − (−13.6) = 12.75 eV > 12.5 eV ✗ (n = 4 cannot be reached).
Step 2 — possible transitions from n = 3 (and n = 2)
- 3 → 1 (Lyman series): ΔE = 12.09 eV; λ = hc/ΔE = 1240/12.09 = 102.6 nm (ultraviolet). Check with Rydberg: 1/λ = 1.097 × 10⁷ (1 − 1/9) = 9.75 × 10⁶ m⁻¹ ⇒ 102.6 nm.
- 2 → 1 (Lyman series): ΔE = 10.2 eV; λ = 1240/10.2 = 121.6 nm (ultraviolet). Check: 1.097 × 10⁷ (1 − 1/4) = 8.23 × 10⁶ ⇒ 121.5 nm.
- 3 → 2 (Balmer series): ΔE = 1.89 eV; λ = 1240/1.89 = 656 nm (red, Hα line). Check: 1.097 × 10⁷ (1/4 − 1/9) = 1.524 × 10⁶ ⇒ 656.3 nm.
| Transition | Series | Energy (eV) | Wavelength | Region |
|---|---|---|---|---|
| 3 → 1 | Lyman | 12.09 | 102.6 nm | ultraviolet |
| 2 → 1 | Lyman | 10.2 | 121.6 nm | ultraviolet |
| 3 → 2 | Balmer (first line, Hα) | 1.89 | 656.3 nm | visible (red) |
- Answer in words: two lines of the Lyman series (102.5 nm and 121.5 nm) and the first line of the Balmer series (656.3 nm) are emitted — three lines in all.
- Why not more: reaching n = 4 or higher needs at least 12.75 eV, more than the 12.5 eV available; hence the Paschen, Brackett and Pfund series (which end on n = 3, 4, 5) and the higher lines of the Balmer series do not appear.
- Role of collision: in an inelastic collision the electron gives up exactly the excitation energy (12.09 eV or 10.2 eV) and keeps the rest of its energy.
Conclusion: the beam can excite hydrogen only up to n = 3, so the emitted wavelengths belong to the Lyman series (102.6 nm and 121.6 nm) and the Balmer series (first line, 656 nm).
In accordance with the Bohr’s model, find the quantum number that characterises the earth’s revolution around the sun in an orbit of radius 1.5 × 10¹¹ m with orbital speed 3 × 10⁴ m/s. (Mass of earth = 6.0 × 10²⁴ kg.)
Concept and context. Bohr’s second postulate states that the angular momentum of an electron in a stationary orbit is an integral multiple of h/2π: L = mvr = nh/2π (n = 1, 2, 3 …, the principal quantum number). Although the postulate was proposed for atomic electrons, the same quantisation applied (formally) to the Earth’s revolution around the Sun gives an enormous quantum number — which illustrates the correspondence principle: for macroscopic systems the quantum numbers are so large that the discreteness of the allowed values is utterly unobservable, and the classical (continuous) description holds.
Given: m = 6.0 × 10²⁴ kg; v = 3 × 10⁴ m s⁻¹; r = 1.5 × 10¹¹ m; h = 6.63 × 10⁻³⁴ J s.
- Angular momentum of the Earth: L = mvr = (6.0 × 10²⁴)(3 × 10⁴)(1.5 × 10¹¹) = 2.7 × 10⁴⁰ kg m² s⁻¹.
- Quantum number: n = L/(h/2π) = 2πL/h = (2 × 3.14 × 2.7 × 10⁴⁰)/(6.63 × 10⁻³⁴) = (1.70 × 10⁴¹)/(6.63 × 10⁻³⁴).
- n ≈ 2.6 × 10⁷⁴.
n = 2π m v r / h ≈ 2.6 × 10⁷⁴
| Quantity | Value |
|---|---|
| L = mvr | 2.7 × 10⁴⁰ kg m² s⁻¹ |
| ħ = h/2π | 1.055 × 10⁻³⁴ J s |
| n = L/ħ | 2.6 × 10⁷⁴ |
- Significance: successive allowed values (n and n + 1) differ by only one part in 10⁷⁴ — the “quantisation” of the Earth’s orbital angular momentum is completely undetectable; hence quantum effects are not seen in the planetary motion and Newtonian mechanics is perfectly adequate.
- Contrast: for the electron in hydrogen the quantum numbers are 1, 2, 3 …, with the discreteness of energy levels very evident (13.6 eV, 3.4 eV …).
Conclusion: the quantum number characterising the Earth’s revolution around the Sun is n ≈ 2.6 × 10⁷⁴ — so large that quantisation of its orbit is of no practical consequence.