Practice MCQs for Class 11 Chemistry Chapter 02 Structure of Atom
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Multiple Choice Questions
(a) the critical frequency
(b) the threshold frequency
(c) the Rydberg frequency
(d) the resonance frequency
Show Answer & Explanation
Answer: (b) the threshold frequency
Explanation:
1. Each metal has a characteristic minimum frequency ν0.
2. If the incident frequency is below ν0, no electrons are ejected however intense the light is or however long it falls on the surface.
Teacher's Note:
1. The work function is W0 = hν0.
2. Different metals have different threshold frequencies.
(a) the frequency of the incident light
(b) the work function of the metal
(c) the intensity of the incident light
(d) the wavelength of the incident light
Show Answer & Explanation
Answer: (c) the intensity of the incident light
Explanation:
1. K.E. = hν − hν0, so it depends on the frequency (or wavelength) and on the metal.
2. Intensity only changes the number of photons, and so the number of electrons ejected, not their kinetic energy.
Teacher's Note:
1. Brighter light gives more electrons, not faster ones.
2. Higher frequency gives faster electrons.
(a) 1.99 × 10−19 J
(b) 5.30 × 10−19 J
(c) 3.31 × 10−19 J
(d) 0 J
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Answer: (a) 1.99 × 10−19 J
Explanation:
1. K.E. = h(ν − ν0) = 6.626 × 10−34 × (8 − 5) × 1014.
2. K.E. = 6.626 × 10−34 × 3 × 1014 = 1.99 × 10−19 J.
Teacher's Note:
1. Subtract the threshold frequency from the incident frequency.
2. K.E. is zero only when ν equals ν0.
(a) 2 × 1018
(b) 2 × 1015
(c) 2 × 1025
(d) 2 × 1020
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Answer: (d) 2 × 1020
Explanation:
1. Energy of one photon = hc/λ = 6.626 × 10−34 × 3 × 108 ÷ 4 × 10−7 = 4.97 × 10−19 J.
2. Photons per second = 100 ÷ 4.97 × 10−19 = 2.0 × 1020.
Teacher's Note:
1. Power is energy per second (1 W = 1 J s−1).
2. Divide the total energy per second by the energy of one photon.
(a) 2 × 1018
(b) 2 × 109
(c) 2 × 10−18
(d) 2 × 1027
Show Answer & Explanation
Answer: (a) 2 × 1018
Explanation:
1. Energy of one photon = hc/λ = 6.626 × 10−34 × 3 × 108 ÷ 4 × 10−7 = 4.97 × 10−19 J.
2. Number = 1 ÷ 4.97 × 10−19 = 2.0 × 1018.
Teacher's Note:
1. Convert 4000 Å to 4 × 10−7 m.
2. Number of photons = total energy ÷ energy per photon.
(a) a continuous spectrum
(b) a line absorption spectrum only
(c) a line emission spectrum
(d) a band absorption spectrum
Show Answer & Explanation
Answer: (c) a line emission spectrum
Explanation:
1. Excited atoms return to lower levels and emit radiation of definite wavelengths only.
2. This gives bright lines on a dark background, a line emission spectrum, which is a fingerprint of the element.
Teacher's Note:
1. White light from a bulb gives a continuous spectrum.
2. Dark lines on a bright background form an absorption spectrum.
(a) −6.54 × 10−18 J
(b) −2.42 × 10−19 J
(c) −7.26 × 10−19 J
(d) +2.42 × 10−19 J
Show Answer & Explanation
Answer: (b) −2.42 × 10−19 J
Explanation:
1. En = −2.18 × 10−18 ÷ n2 J.
2. For n = 3, E = −2.18 × 10−18 ÷ 9 = −2.42 × 10−19 J.
Teacher's Note:
1. The energy is always negative for a bound electron.
2. Divide by n squared, not by n.
(a) −5.45 × 10−19 J
(b) −8.72 × 10−18 J
(c) −1.09 × 10−18 J
(d) −2.18 × 10−18 J
Show Answer & Explanation
Answer: (d) −2.18 × 10−18 J
Explanation:
1. En = −2.18 × 10−18 × Z2/n2 J.
2. For Z = 2 and n = 2: E = −2.18 × 10−18 × 4/4 = −2.18 × 10−18 J.
Teacher's Note:
1. Z2/n2 = 1 here, so the energy equals that of H in n = 1.
2. Always substitute both Z and n.
(a) 159 pm
(b) 17.6 pm
(c) 476 pm
(d) 52.9 pm
Show Answer & Explanation
Answer: (c) 476 pm
Explanation:
1. rn = 52.9 × n2/Z pm.
2. For n = 3 and Z = 1: r = 52.9 × 9 = 476 pm (0.476 nm).
Teacher's Note:
1. The radius grows as n2.
2. r1 = 52.9 pm is the Bohr radius.
(a) 70.5 pm
(b) 211.6 pm
(c) 17.6 pm
(d) 158.7 pm
Show Answer & Explanation
Answer: (a) 70.5 pm
Explanation:
1. rn = 52.9 × n2/Z pm.
2. For n = 2 and Z = 3: r = 52.9 × 4/3 = 70.5 pm.
Teacher's Note:
1. A larger Z shrinks the orbit.
2. Do not forget to divide by Z.
(a) h/2π
(b) 9h/2π
(c) h/6π
(d) 3h/2π
Show Answer & Explanation
Answer: (d) 3h/2π
Explanation:
1. Angular momentum is quantised: mvr = nh/2π.
2. For n = 3, it is 3h/2π.
Teacher's Note:
1. The angular momentum is an integral multiple of h/2π.
2. It is proportional to n, not n2.
(a) Balmer series
(b) Lyman series
(c) Paschen series
(d) Brackett series
Show Answer & Explanation
Answer: (a) Balmer series
Explanation:
1. Balmer lines arise when electrons fall to n = 2 from higher levels (n = 3, 4, 5 ...).
2. Lyman lines are in the ultraviolet; Paschen, Brackett and Pfund lines are in the infrared.
Teacher's Note:
1. Lyman: n = 1, Balmer: n = 2, Paschen: n = 3, Brackett: n = 4, Pfund: n = 5.
2. Only Balmer is visible.
(a) 4
(b) 10
(c) 5
(d) 15
Show Answer & Explanation
Answer: (b) 10
Explanation:
1. Number of lines = n(n − 1)/2 for a fall from level n to the ground state.
2. For n = 5: 5 × 4/2 = 10.
Teacher's Note:
1. Count all possible jumps, not only those to n = 1.
2. For n = 6 the number would be 15.
(a) 486 nm
(b) 122 nm
(c) 656 nm
(d) 1875 nm
Show Answer & Explanation
Answer: (c) 656 nm
Explanation:
1. 1/λ = R(1/22 − 1/32) = 1.097 × 107 × 5/36 = 1.524 × 106 m−1.
2. λ = 6.56 × 10−7 m = 656 nm.
Teacher's Note:
1. Use n1 = 2 and n2 = 3.
2. This red line is called H-alpha.
(a) the electron carries a negative charge
(b) the energy is zero near the nucleus
(c) of repulsion between electrons
(d) the electron is bound; its energy is lower than that of a free electron at rest, taken as zero
Show Answer & Explanation
Answer: (d) the electron is bound; its energy is lower than that of a free electron at rest, taken as zero
Explanation:
1. A free electron at rest infinitely far away (n = ∞) is assigned zero energy.
2. As the electron comes closer, energy is released and its energy falls below zero, so the bound electron has negative energy. The most negative value is at n = 1.
Teacher's Note:
1. Negative energy means a stable, bound state.
2. The ground state is the lowest, most negative level.
(a) 54.4 eV
(b) 13.6 eV
(c) 27.2 eV
(d) 122.4 eV
Show Answer & Explanation
Answer: (a) 54.4 eV
Explanation:
1. Ionisation energy = 13.6 × Z2 eV for a one-electron species in n = 1.
2. For He+, Z = 2: 13.6 × 4 = 54.4 eV.
Teacher's Note:
1. The energy needed is proportional to Z2.
2. Li2+ would need 13.6 × 9 = 122.4 eV.
(a) It cannot explain the line spectrum of hydrogen
(b) It cannot explain the spectra of atoms with more than one electron
(c) It does not use quantised energy levels
(d) It does not give the radius of the first orbit
Show Answer & Explanation
Answer: (b) It cannot explain the spectra of atoms with more than one electron
Explanation:
1. Bohr's model works well for hydrogen and hydrogen-like ions only.
2. It cannot explain multi-electron spectra, the splitting of lines in magnetic and electric fields, or chemical bonding, and it ignores the dual nature of matter and the uncertainty principle.
Teacher's Note:
1. It gave the correct hydrogen spectrum and orbit radius.
2. Its fixed circular orbits conflict with the uncertainty principle.
(a) 2.04 × 10−19 J
(b) 1.36 × 10−18 J
(c) 4.09 × 10−19 J
(d) 4.09 × 10−18 J
Show Answer & Explanation
Answer: (c) 4.09 × 10−19 J
Explanation:
1. ΔE = 2.18 × 10−18 × (1/22 − 1/42) J.
2. ΔE = 2.18 × 10−18 × 3/16 = 4.09 × 10−19 J.
Teacher's Note:
1. Take 1/nf2 − 1/ni2, with nf the lower level.
2. The emitted photon has this energy.
(a) 3.0 × 108 m s−1
(b) 2.18 × 108 m s−1
(c) 6.6 × 103 m s−1
(d) 2.18 × 106 m s−1
Show Answer & Explanation
Answer: (d) 2.18 × 106 m s−1
Explanation:
1. The speed in the nth orbit is vn = 2.188 × 106 × Z/n m s−1.
2. For n = 1 and Z = 1 this is 2.188 × 106 m s−1, about 1/137 of the speed of light.
Teacher's Note:
1. Speed falls as n increases.
2. It is much less than the speed of light.
(a) n = 4 to n = 2
(b) n = 3 to n = 1
(c) n = 3 to n = 2
(d) n = 2 to n = 1
Show Answer & Explanation
Answer: (a) n = 4 to n = 2
Explanation:
1. For He+, 1/λ = R × 4 × (1/n12 − 1/n22). For hydrogen n = 2 to n = 1: 1/λ = R × 3/4.
2. For n = 4 to n = 2 in He+: 4 × (1/4 − 1/16) = 4 × 3/16 = 3/4. The two match.
Teacher's Note:
1. The factor Z2 = 4 makes He+ levels four times as far apart.
2. Equate the two expressions and test the options.
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