Download JEE MCQs for JEE Chemistry: Structure Of Atom
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Chapter-wise Objective Questions: Structure Of Atom
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Multiple Choice Questions
(a) Half of the potential energy
(b) Twice the potential energy
(c) One-fourth of the potential energy
(d) None of these
Show Answer & Explanation
Answer: (a) Half of the potential energy
Explanation:
1. In a Bohr orbit KE = +Ze²/2r (in CGS) and PE = −Ze²/r.
2. So
3. KE
4. = ½
5. PE
6. , and the total energy equals −KE.
Teacher's Note:
1. Remember the three relations: KE = −E, PE = 2E and PE = −2 KE.
(a) Electrons
(b) Protons
(c) A nucleus
(d) Neutrons
Show Answer & Explanation
Answer: (c) A nucleus
Explanation:
1. Most α-particles passed straight through but a few were deflected through large angles.
2. This showed that the positive charge and mass are concentrated in a tiny, dense nucleus.
Teacher's Note:
1. Convert every quantity to moles or equivalents first.
2. Then apply the stoichiometric ratio or the definition asked for.
(a) Nucleus
(b) Atom
(c) Electron
(d) Neutron
Show Answer & Explanation
Answer: (a) Nucleus
Explanation:
1. The distance of closest approach of α-particles to the nucleus gave an estimate of the nuclear size (about 10−15 m).
Teacher's Note:
1. Eliminate options that disagree with the basic definition.
2. Confirm the remaining option by a quick calculation.
(a) The spectrum of the hydrogen atom only
(b) The spectrum of an atom or ion containing one electron only
(c) The spectrum of the hydrogen molecule
(d) The solar spectrum
Show Answer & Explanation
Answer: (b) The spectrum of an atom or ion containing one electron only
Explanation:
1. Bohr's theory works for hydrogen-like species such as H, He+, Li2+, which have a single electron.
2. It fails for multi-electron atoms.
Teacher's Note:
1. Read the data carefully and write the relevant formula before substituting.
2. Check units and the order of magnitude of the answer.
(a) The force of repulsion on the moving α-particle is small
(b) The force of attraction on the α-particle to the oppositely charged electrons is very small
(c) There is only one nucleus and a large number of electrons
(d) The nucleus occupies a much smaller volume compared to the volume of the atom
Show Answer & Explanation
Answer: (d) The nucleus occupies a much smaller volume compared to the volume of the atom
Explanation:
1. Deflection occurs only when an α-particle passes very close to the nucleus.
2. The nucleus is about 10−5 times the size of the atom, so close approaches are rare.
Teacher's Note:
1. Convert every quantity to moles or equivalents first.
2. Then apply the stoichiometric ratio or the definition asked for.
(a) R∞/4
(b) R∞/2
(c) 2R∞
(d) R∞
Show Answer & Explanation
Answer: (b) R∞/2
Explanation:
1. The Rydberg constant is proportional to the reduced mass μ of the system.
2. For positronium μ = m·m/(m + m) = m/2.
3. So R = R∞/2.
Teacher's Note:
1. Eliminate options that disagree with the basic definition.
2. Confirm the remaining option by a quick calculation.
(a) Energy is absorbed
(b) Energy is released
(c) Energy is sometimes absorbed and sometimes released
(d) Energy is neither absorbed nor released
Show Answer & Explanation
Answer: (b) Energy is released
Explanation:
1. The K shell is lower in energy than the L shell.
2. A fall to a lower level releases energy as a photon.
Teacher's Note:
1. Read the data carefully and write the relevant formula before substituting.
2. Check units and the order of magnitude of the answer.
(a) A beam of protons
(b) α-rays
(c) A beam of neutrons
(d) X-rays
Show Answer & Explanation
Answer: (c) A beam of neutrons
Explanation:
1. Be + He → C + n; the radiation is undeflected, so it carries no charge.
2. It is a beam of neutrons (Chadwick, 1932).
Teacher's Note:
1. Convert every quantity to moles or equivalents first.
2. Then apply the stoichiometric ratio or the definition asked for.
(a) Increases as we move away from the nucleus
(b) Decreases as we move away from the nucleus
(c) Remains the same as we move away from the nucleus
(d) None of these
Show Answer & Explanation
Answer: (a) Increases as we move away from the nucleus
Explanation:
1. E_n = −13.6/n² eV is negative and increases (becomes less negative) as n increases.
2. The energy is highest (zero) at infinite distance.
Teacher's Note:
1. Eliminate options that disagree with the basic definition.
2. Confirm the remaining option by a quick calculation.
(a) Emission spectrum
(b) Absorption spectrum
(c) Line spectrum of hydrogen
(d) Fine spectrum
Show Answer & Explanation
Answer: (d) Fine spectrum
Explanation:
1. Bohr's model explains the main lines of hydrogen. Fine structure, where each line is split into very close components, needs sub-shells (Sommerfeld) and relativistic treatment.
Teacher's Note:
1. Read the data carefully and write the relevant formula before substituting.
2. Check units and the order of magnitude of the answer.
(a) −41 kJ/mol
(b) −1312 kJ/mol
(c) −164 kJ/mol
(d) −82 kJ/mol
Show Answer & Explanation
Answer: (d) −82 kJ/mol
Explanation:
1. E_n is proportional to 1/n².
2. E_4 = E_2 × (2²/4²) = −328 × 4/16 = −82 kJ/mol.
Teacher's Note:
1. Convert every quantity to moles or equivalents first.
2. Then apply the stoichiometric ratio or the definition asked for.
(a) −13.6/n4 eV
(b) −13.6/n3 eV
(c) −13.6/n² eV
(d) −13.6/n eV
Show Answer & Explanation
Answer: (c) −13.6/n² eV
Explanation:
1. For hydrogen, E_n = −13.6/n² eV.
2. For example, n = 1 gives −13.6 eV and n = 2 gives −3.4 eV.
Teacher's Note:
1. Eliminate options that disagree with the basic definition.
2. Confirm the remaining option by a quick calculation.
(a) 3 × 10−23 kg m s−1
(b) 3.33 × 1022 kg m s−1
(c) 1.452 × 10−44 kg m s−1
(d) 6.89 × 1043 kg m s−1
Show Answer & Explanation
Answer: (a) 3 × 10−23 kg m s−1
Explanation:
1. Momentum p = h/λ.
2. p = 6.6 × 10−34/2.2 × 10−11 = 3 × 10−23 kg m s−1.
Teacher's Note:
1. Read the data carefully and write the relevant formula before substituting.
2. Check units and the order of magnitude of the answer.
(a) UV field
(b) IR field
(c) Visible field
(d) Far IR field
Show Answer & Explanation
Answer: (a) UV field
Explanation:
1. Lyman lines arise from transitions to n = 1 and have the shortest wavelengths.
2. They lie in the ultraviolet region.
Teacher's Note:
1. Convert every quantity to moles or equivalents first.
2. Then apply the stoichiometric ratio or the definition asked for.
(a) Fifth Bohr orbit to second one
(b) Fifth Bohr orbit to first one
(c) Fourth Bohr orbit to second one
(d) Fourth Bohr orbit to first one
Show Answer & Explanation
Answer: (a) Fifth Bohr orbit to second one
Explanation:
1. Balmer lines end at n = 2.
2. First line 3 → 2, second 4 → 2, third 5 → 2.
Teacher's Note:
1. Eliminate options that disagree with the basic definition.
2. Confirm the remaining option by a quick calculation.
(a) −5.44 × 10−19 J
(b) −5.44 × 10−19 kJ
(c) −5.44 × 10−19 cal
(d) −5.44 × 10−19 eV
Show Answer & Explanation
Answer: (a) −5.44 × 10−19 J
Explanation:
1. E_2 = −13.6/4 = −3.4 eV.
2. In joules: −3.4 × 1.6 × 10−19 = −5.44 × 10−19 J.
Teacher's Note:
1. Read the data carefully and write the relevant formula before substituting.
2. Check units and the order of magnitude of the answer.
(a) 0.79 Å
(b) 1.59 Å
(c) 3.18 Å
(d) 4.77 Å
Show Answer & Explanation
Answer: (d) 4.77 Å
Explanation:
1. r_n = 0.53 n² Å.
2. r_3 = 0.53 × 9 = 4.77 Å.
Teacher's Note:
1. Convert every quantity to moles or equivalents first.
2. Then apply the stoichiometric ratio or the definition asked for.
(a) 3.08 × 1015 s−1
(b) 2.00 × 1015 s−1
(c) 1.54 × 1015 s−1
(d) 1.03 × 1015 s−1
Show Answer & Explanation
Answer: (a) 3.08 × 1015 s−1
Explanation:
1. ΔE = 2.18 × 10−18 (1/1² − 1/4²) = 2.18 × 10−18 × 15/16 = 2.044 × 10−18 J.
2. ν = ΔE/h = 2.044 × 10−18/6.625 × 10−34 = 3.08 × 1015 s−1.
Teacher's Note:
1. Eliminate options that disagree with the basic definition.
2. Confirm the remaining option by a quick calculation.
(a) 406 nm
(b) 192 nm
(c) 91 nm
(d) 9.1 × 10−8 nm
Show Answer & Explanation
Answer: (c) 91 nm
Explanation:
1. 1/λ = R(1/1² − 1/∞²) = R.
2. λ = 1/1.097 × 107 = 9.12 × 10−8 m = 91 nm.
Teacher's Note:
1. Read the data carefully and write the relevant formula before substituting.
2. Check units and the order of magnitude of the answer.
(a) n1 = 1 and n2 = 2, 3, 4
(b) n1 = 3 and n2 = 4, 5, 6
(c) n1 = 1 and n2 = 3, 4, 5
(d) n1 = 2 and n2 = 3, 5
Show Answer & Explanation
Answer: (b) n1 = 3 and n2 = 4, 5, 6
Explanation:
1. The Paschen series ends on the third orbit, so n1 = 3.
2. The electron falls from n2 = 4, 5, 6, ... to n1 = 3.
Teacher's Note:
1. Convert every quantity to moles or equivalents first.
2. Then apply the stoichiometric ratio or the definition asked for.
(a) He+ (n = 2)
(b) Li2+ (n = 2)
(c) Li2+ (n = 3)
(d) Be3+ (n = 2)
Show Answer & Explanation
Answer: (d) Be3+ (n = 2)
Explanation:
1. r ∝ n²/Z.
2. He+: 4/2 = 2; Li2+ (n = 2): 4/3; Li2+ (n = 3): 9/3 = 3; Be3+: 4/4 = 1.
3. Only Be3+ (n = 2) matches hydrogen n = 1 (ratio 1).
Teacher's Note:
1. Eliminate options that disagree with the basic definition.
2. Confirm the remaining option by a quick calculation.
(a) 4π²mr²/nh
(b) nh/4π²mr
(c) nh/4π²mr²
(d) h/2πmr
Show Answer & Explanation
Answer: (a) 4π²mr²/nh
Explanation:
1. Angular momentum mvr = nh/2π, so v = nh/2πmr.
2. Time period T = 2πr/v = 2πr × 2πmr/nh = 4π²mr²/nh.
Teacher's Note:
1. Read the data carefully and write the relevant formula before substituting.
2. Check units and the order of magnitude of the answer.
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FAQs
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