આ MCQ મોડ્યુલ આના પર આધારિત છે: NCERT Exercises and Solutions: Atoms
NCERT Exercises and Solutions: Atoms
આ મૂલ્યાંકન આના પર આધારિત હશે: NCERT Exercises and Solutions: Atoms
મૂલ્યાંકન બનાવવામાં તેમની સામગ્રી સામેલ કરવા ચિત્રો, PDF અથવા Word દસ્તાવેજ અપલોડ કરો.
NCERT Exercises and Solutions: Atoms
Chapter 12 — Summary & Key Formulae
- Thomson's plum-pudding atom (1898): a uniform positive sphere with embedded electrons.
- Geiger-Marsden α-scattering on gold (1909): most α pass straight; 1/8000 deflect > 90°; some bounce back.
- Rutherford's nuclear atom (1911): tiny dense positive nucleus (< 10⁻¹⁴ m); electrons orbit at ~10⁻¹⁰ m.
- Classical instability — orbiting electrons should radiate and spiral in. Bohr (1913) added quantum postulates.
- Bohr's stationary orbits: L = nℏ. Bohr radius a₀ = 0.529 Å. E_n = −13.6/n² eV.
- Photons emitted on transitions: hν = E_i − E_f. Rydberg formula 1/λ = R(1/n_f² − 1/n_i²) with R = 1.097×10⁷ m⁻¹.
- Five spectral series: Lyman (UV, n_f=1), Balmer (visible, n_f=2), Paschen, Brackett, Pfund (IR).
- de Broglie (1924): the quantisation rule arises because matter waves form standing waves on the orbit (2πr = nλ).
- Bohr's model fails for multi-electron atoms, line intensities, fine structure, and Zeeman/Stark effects. Schrödinger's wave mechanics (1926) supersedes it.
| Quantity | Symbol | Equation / value |
|---|---|---|
| Bohr radius | a₀ | 5.29×10⁻¹¹ m = 0.529 Å |
| Radius of n-th orbit | r_n | n² a₀ / Z |
| Speed of n-th orbit | v_n | (αc)·Z/n where α ≈ 1/137 |
| Energy of n-th level | E_n | −13.6 Z²/n² eV |
| Ionisation energy of H | I | 13.6 eV |
| Bohr quantisation | L | nℏ = nh/(2π) |
| Rydberg formula | 1/λ | R(1/n_f² − 1/n_i²) |
| Rydberg constant | R | 1.097 × 10⁷ m⁻¹ |
| de Broglie standing-wave | 2πr | nλ |
| Distance of closest approach | r₀ | (1/4πε₀)·(2Ze²)/((1/2)mv²) |
| Photon energy ↔ wavelength | E | 1240/λ(nm) eV |
NCERT Exercises — Worked Solutions
(a) The size of the atom in Thomson's model is …………… that in Rutherford's model. (b) In the ground state of …………… electrons are in stable equilibrium, while in …………… electrons always experience a net force.
(b) Thomson's model electrons are in stable equilibrium (positive jelly balances electron repulsion). In Rutherford's model electrons orbit and continuously experience the central Coulomb force.
(Hydrogen is a solid below 14 K.) What results do you expect?
What is the shortest wavelength present in the Paschen series of spectral lines?
\(1/\lambda = R/9 = (1.097\times10^{7})/9 = 1.219\times10^{6}\) m⁻¹.
λ = 8.205×10⁻⁷ m = 820.5 nm (near IR).
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?
λ = c/ν = 3×10⁸/5.56×10¹⁴ ≈ 540 nm — green visible light.
The ground state energy of hydrogen atom is −13.6 eV. What are the kinetic and potential energies of the electron in this state?
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 the photon.
ν = ΔE/h = 2.04×10⁻¹⁸/6.626×10⁻³⁴ = 3.08×10¹⁵ Hz.
λ = c/ν = 3×10⁸/3.08×10¹⁵ = 97.4 nm — Lyman-γ, in the far UV.
(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.
v₁ = 2.19×10⁶ m/s; v₂ = 1.095×10⁶ m/s; v₃ = 7.30×10⁵ m/s.
(b) T_n = 2πr_n/v_n = 2π(n²a₀)/(v₁/n) = (2π a₀ n³)/v₁.
T₁ = 2π × 5.29×10⁻¹¹/2.19×10⁶ = 1.52×10⁻¹⁶ s.
T₂ = 2³ × T₁ = 1.22×10⁻¹⁵ s.
T₃ = 27 × T₁ = 4.10×10⁻¹⁵ s.
T₁ ≈ 1.52×10⁻¹⁶ s.
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?
r₂ = 4 × 5.3×10⁻¹¹ = 2.12×10⁻¹⁰ m.
r₃ = 9 × 5.3×10⁻¹¹ = 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?
Possible levels: E₃ = −1.51 eV (allowed, since 12.09 eV is enough); E₄ = −0.85 eV (NOT allowed, 12.75 eV needed).
So the highest level reached is n = 3. Possible transitions: 3 → 1 (Lyman), 3 → 2 (Balmer-α), 2 → 1 (Lyman-α).
Wavelengths: 102.6 nm, 656.3 nm, 121.5 nm respectively. Lyman series (UV) and Balmer-α (visible red) will be emitted.
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.)
For such a colossal n, the levels are spaced by ΔE/E ~ 1/n² = 10⁻¹⁵⁰ — utterly indistinguishable. The orbit looks classical and continuous, exactly as we observe.
An α-particle of kinetic energy 7.7 MeV approaches a gold nucleus head-on. Calculate the distance of closest approach. (Z = 79; e = 1.6×10⁻¹⁹ C.)
\(r_0 = (1/4\pi\varepsilon_0)\,(2Ze^2/K) = (8.99\times10^{9})(2 \times 79 \times (1.6\times10^{-19})^{2})/(7.7\times10^{6}\times1.6\times10^{-19})\)
= (8.99×10⁹)(4.05×10⁻³⁶)/(1.232×10⁻¹²) = 2.95 × 10⁻¹⁴ m.
The ground-state binding energy of hydrogen is 13.6 eV. What wavelength of light is just sufficient to ionise a ground-state hydrogen atom?
Calculate the wavelength of the photon emitted when a singly-ionised helium ion (He⁺, Z = 2) makes a transition from n = 2 to n = 1.
λ = 1/3.29×10⁷ = 30.4 nm. (Compare hydrogen Lyman-α at 121.6 nm — He⁺ photon is 4× more energetic.)
Use the data below to compute every key quantity for an electron in the n = 5 Bohr orbit of hydrogen.
| Quantity | Formula | Your answer |
|---|---|---|
| Radius r₅ | n² a₀ | ? |
| Speed v₅ | v₁/n | ? |
| Energy E₅ | −13.6/n² | ? |
| Period T₅ | n³ T₁ | ? |
| de Broglie λ | h/(mv) | ? |
| 2πr₅/λ | n | ? |
v₅ = 2.19×10⁶/5 = 4.38×10⁵ m/s.
E₅ = −13.6/25 = −0.544 eV.
T₅ = 125 × 1.52×10⁻¹⁶ = 1.90×10⁻¹⁴ s.
λ = h/(m_e v₅) = 6.626×10⁻³⁴/(9.11×10⁻³¹ × 4.38×10⁵) = 1.66×10⁻⁹ m.
2πr₅/λ = 2π × 13.23×10⁻¹⁰/1.66×10⁻⁹ = 5 ✓.
Interactive — Pick a Transition, See the Photon
Slide the upper and lower quantum numbers to see the wavelength and the spectral series of the resulting photon.
656 nm
1.89 eV
Balmer
Competency-Based Questions — Mixed Revision
Q1. The ratio of the radii of the first three Bohr orbits in hydrogen is:
Q2. Which spectral series of hydrogen lies entirely in the ultraviolet region?
Q3. (Short Answer) State two limitations of Bohr's model.
Q4. (Fill in the blank) The Rydberg constant has the value ______ m⁻¹.
Q5. (HOT) An electron in the n = 4 state of hydrogen jumps down to n = 1 either directly or via intermediate states. How many distinct photons are possible? List them.
Assertion–Reason — Mixed Revision
Options: (A) Both true, R correct explanation of A. (B) Both true, R not the correct explanation. (C) A true, R false. (D) A false, R true.
Assertion: The energy of an electron in a Bohr orbit is the same as for the corresponding free-particle orbit at the same radius.
Reason: Bohr's quantisation does not affect the kinetic and potential energies for given r.
Assertion: The ionisation energy of hydrogen is exactly +13.6 eV.
Reason: The energy of the ground state is E₁ = −13.6 eV.
Assertion: de Broglie's hypothesis successfully explains why angular momentum is quantised in Bohr's model.
Reason: The matter wave of an electron must form a standing wave on the orbit.
Frequently Asked Questions - NCERT Exercises and Solutions: Atoms
What are the key NCERT exercise types in Chapter 12 Atoms?
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What are the most-asked CBSE board questions from Chapter 12?
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Physics — CBSE Class XII Sample Paper 1 (2025-26)
Section A · Section B · Section C · Section D · Section E