Multiple Choice Questions (MCQs) for JEE Chemistry: Structure Of Atom
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Practice Structure Of Atom MCQs for JEE Chemistry
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Multiple Choice Questions
(a) more than doubles
(b) doubles exactly
(c) halves
(d) is unchanged
Show Answer & Explanation
Answer: (a) more than doubles
Explanation:
1. \(KE_2 = 2h\nu-W = 2(h\nu-W)+W > 2KE_1\).
2. Only option (a) agrees with this working.
Teacher's Note:
1. The de Broglie relation lambda = h/mv and the Heisenberg relation dx.dp = h/4pi are the two tools here; for an electron accelerated through V volts, lambda = sqrt(150/V) in angstrom.
(a) 0.1 g
(b) 1000 kg
(c) \(10^{-3}\) g
(d) 0.1 kg
Show Answer & Explanation
Answer: (d) 0.1 kg
Explanation:
1. \(m = h/(4\pi\Delta x\Delta v) = 6.626\times10^{-34}/(4\pi\times10^{-10}\times5.27\times10^{-24}) = 0.1\) kg.
2. Only option (d) agrees with this working.
Teacher's Note:
1. The de Broglie relation lambda = h/mv and the Heisenberg relation dx.dp = h/4pi are the two tools here; for an electron accelerated through V volts, lambda = sqrt(150/V) in angstrom.
(a) \(1.11\times10^{9}\) cm/s
(b) \(1.11\times10^{6}\) cm/s
(c) \(1.11\times10^{5}\) cm/s
(d) \(1.11\times10^{11}\) cm/s
Show Answer & Explanation
Answer: (a) \(1.11\times10^{9}\) cm/s
Explanation:
1. \(\Delta v = \Delta p/m = 10^{-18}/9\times10^{-28} = 1.11\times10^{9}\) cm/s.
2. Only option (a) agrees with this working.
Teacher's Note:
1. The de Broglie relation lambda = h/mv and the Heisenberg relation dx.dp = h/4pi are the two tools here; for an electron accelerated through V volts, lambda = sqrt(150/V) in angstrom.
(a) using better instruments
(b) using photons of higher energy
(c) no method; it is a fundamental limit
(d) using photons of lower wave number
Show Answer & Explanation
Answer: (c) no method; it is a fundamental limit
Explanation:
1. The limit \(\Delta x\,\Delta p \ge h/4\pi\) follows from the wave nature of matter and does not depend on the apparatus.
2. Only option (c) agrees with this working.
Teacher's Note:
1. The de Broglie relation lambda = h/mv and the Heisenberg relation dx.dp = h/4pi are the two tools here; for an electron accelerated through V volts, lambda = sqrt(150/V) in angstrom.
(a) 2r\(_1\), 3r\(_1\), 4r\(_1\)
(b) 4r\(_1\), 9r\(_1\), 16r\(_1\)
(c) 8r\(_1\), 27r\(_1\), 64r\(_1\)
(d) r\(_1\)^2, r\(_1\)^3, r\(_1\)^4
Show Answer & Explanation
Answer: (b) 4r\(_1\), 9r\(_1\), 16r\(_1\)
Explanation:
1. \(r_n = n^2r_1\) gives 4, 9, 16 times r\(_1\).
2. Only option (b) agrees with this working.
Teacher's Note:
1. In the Bohr model remember r proportional to n squared over Z, v proportional to Z over n, and E proportional to minus Z squared over n squared. Ratios between species are then quick to find.
(a) 1 : 2 : 3
(b) 3 : 4 : 6
(c) 6 : 4 : 3
(d) 2 : 3 : 4
Show Answer & Explanation
Answer: (c) 6 : 4 : 3
Explanation:
1. For the same n, \(r\propto1/Z\): \(1/2:1/3:1/4 = 6:4:3\).
2. Only option (c) agrees with this working.
Teacher's Note:
1. In the Bohr model remember r proportional to n squared over Z, v proportional to Z over n, and E proportional to minus Z squared over n squared. Ratios between species are then quick to find.
(a) 0.17 A
(b) 1.27 A
(c) 0.57 A
(d) 0.99 A
Show Answer & Explanation
Answer: (a) 0.17 A
Explanation:
1. \(r = 0.53/Z = 0.53/3 = 0.177\) A.
2. Only option (a) agrees with this working.
Teacher's Note:
1. In the Bohr model remember r proportional to n squared over Z, v proportional to Z over n, and E proportional to minus Z squared over n squared. Ratios between species are then quick to find.
(a) u/4
(b) 4u
(c) 16u
(d) u/16
Show Answer & Explanation
Answer: (b) 4u
Explanation:
1. \(v\propto1/n\), so \(v_1 = 4v_4 = 4u\).
2. Only option (b) agrees with this working.
Teacher's Note:
1. In the Bohr model remember r proportional to n squared over Z, v proportional to Z over n, and E proportional to minus Z squared over n squared. Ratios between species are then quick to find.
(a) The energy of the electron decreases as the orbit number increases
(b) The kinetic energy is half the magnitude of the potential energy
(c) The kinetic energy is the negative of the total energy
(d) The ionisation energy of H in the first excited state is minus one-fourth of the ground-state energy
Show Answer & Explanation
Answer: (a) The energy of the electron decreases as the orbit number increases
Explanation:
1. Energy \(= -13.6Z^2/n^2\) increases (becomes less negative) with n, so the first statement is false
2. The others are true: \(KE = -E = |PE|/2\), and \(IE(n=2) = 3.4\) eV \(= -E_1/4\).
Teacher's Note:
1. In the Bohr model remember r proportional to n squared over Z, v proportional to Z over n, and E proportional to minus Z squared over n squared. Ratios between species are then quick to find.
(a) directly proportional to n\(^2\)
(b) inversely proportional to Z\(^2\)
(c) neither directly proportional to n\(^2\) nor inversely proportional to Z\(^2\)
(d) both of these
Show Answer & Explanation
Answer: (c) neither directly proportional to n\(^2\) nor inversely proportional to Z\(^2\)
Explanation:
1. \(KE = 13.6Z^2/n^2\) eV, which varies as \(1/n^2\) and as \(Z^2\).
2. Only option (c) agrees with this working.
Teacher's Note:
1. In the Bohr model remember r proportional to n squared over Z, v proportional to Z over n, and E proportional to minus Z squared over n squared. Ratios between species are then quick to find.
(a) +3.4 eV
(b) -13.6 eV
(c) +13.6 eV
(d) +1.51 eV
Show Answer & Explanation
Answer: (d) +1.51 eV
Explanation:
1. \(KE = -E = +1.51\) eV.
2. Only option (d) agrees with this working.
Teacher's Note:
1. In the Bohr model remember r proportional to n squared over Z, v proportional to Z over n, and E proportional to minus Z squared over n squared. Ratios between species are then quick to find.
(a) -164 kJ/mol
(b) -328 kJ/mol
(c) -41 kJ/mol
(d) -1312 kJ/mol
Show Answer & Explanation
Answer: (b) -328 kJ/mol
Explanation:
1. \(E\propto1/n^2\): \(E_2 = E_4\times16/4 = -82\times4 = -328\) kJ/mol.
2. Only option (b) agrees with this working.
Teacher's Note:
1. In the Bohr model remember r proportional to n squared over Z, v proportional to Z over n, and E proportional to minus Z squared over n squared. Ratios between species are then quick to find.
(a) Li\(^{2+}\)
(b) Be\(^{3+}\)
(c) He\(^+\)
(d) Li\(^+\)
Show Answer & Explanation
Answer: (a) Li\(^{2+}\)
Explanation:
1. \(13.6Z^2/9 = 13.6\) gives \(Z = 3\), so the species is Li\(^{2+}\).
2. Only option (a) agrees with this working.
Teacher's Note:
1. In the Bohr model remember r proportional to n squared over Z, v proportional to Z over n, and E proportional to minus Z squared over n squared. Ratios between species are then quick to find.
(a) H
(b) He\(^+\)
(c) Li\(^{2+}\)
(d) Be\(^{3+}\)
Show Answer & Explanation
Answer: (b) He\(^+\)
Explanation:
1. For hydrogen this line is at about 4861 A, and \(\lambda\propto1/Z^2\)
2. \(4861/1216 = 4\), so Z = 2.
Teacher's Note:
1. In the Bohr model remember r proportional to n squared over Z, v proportional to Z over n, and E proportional to minus Z squared over n squared. Ratios between species are then quick to find.
(a) 13.6x eV
(b) 40.5x eV
(c) -10.2x eV
(d) 12.09x eV
Show Answer & Explanation
Answer: (d) 12.09x eV
Explanation:
1. In units of x the level scheme is that of hydrogen (first excitation 10.2x eV), so the second excitation energy is \(13.6(1-1/9)x = 12.09x\) eV.
2. Only option (d) agrees with this working.
Teacher's Note:
1. In the Bohr model remember r proportional to n squared over Z, v proportional to Z over n, and E proportional to minus Z squared over n squared. Ratios between species are then quick to find.
(a) 2
(b) 3
(c) 4
(d) 1
Show Answer & Explanation
Answer: (c) 4
Explanation:
1. \(13.6Z^2/4 = 54.4\) gives \(Z^2 = 16\), Z = 4.
2. Only option (c) agrees with this working.
Teacher's Note:
1. In the Bohr model remember r proportional to n squared over Z, v proportional to Z over n, and E proportional to minus Z squared over n squared. Ratios between species are then quick to find.
(a) visible region
(b) ultraviolet region
(c) X-ray region
(d) infrared region
Show Answer & Explanation
Answer: (d) infrared region
Explanation:
1. Paschen lines end at n = 3 and have energies below those of the Balmer series, so they are infrared.
2. Only option (d) agrees with this working.
Teacher's Note:
1. For spectral lines use 1/lambda = R Z^2 (1/n1^2 - 1/n2^2). The lowest n1 fixes the series (1 Lyman, 2 Balmer, 3 Paschen), and n(n-1)/2 gives the total number of possible lines.
(a) 1315 A
(b) 1215 A
(c) 1415 A
(d) 1515 A
Show Answer & Explanation
Answer: (b) 1215 A
Explanation:
1. \(\bar\nu = R(1-1/4) = 82258.5\) cm\(^{-1}\), so \(\lambda = 1.2157\times10^{-5}\) cm \(= 1215\) A.
2. Only option (b) agrees with this working.
Teacher's Note:
1. For spectral lines use 1/lambda = R Z^2 (1/n1^2 - 1/n2^2). The lowest n1 fixes the series (1 Lyman, 2 Balmer, 3 Paschen), and n(n-1)/2 gives the total number of possible lines.
(a) 1459 A
(b) 4052 A
(c) 1459 nm
(d) 4052 nm
Show Answer & Explanation
Answer: (c) 1459 nm
Explanation:
1. The series limit has \(\bar\nu = R/16\), so \(\lambda = 16/109678 = 1.459\times10^{-4}\) cm \(= 1459\) nm.
2. Only option (c) agrees with this working.
Teacher's Note:
1. For spectral lines use 1/lambda = R Z^2 (1/n1^2 - 1/n2^2). The lowest n1 fixes the series (1 Lyman, 2 Balmer, 3 Paschen), and n(n-1)/2 gives the total number of possible lines.
(a) Lyman series
(b) Balmer series
(c) Paschen series
(d) Pfund series
Show Answer & Explanation
Answer: (b) Balmer series
Explanation:
1. All lines ending at n = 2 form the Balmer series.
2. Only option (b) agrees with this working.
Teacher's Note:
1. For spectral lines use 1/lambda = R Z^2 (1/n1^2 - 1/n2^2). The lowest n1 fixes the series (1 Lyman, 2 Balmer, 3 Paschen), and n(n-1)/2 gives the total number of possible lines.
(a) c/1370
(b) c/13.7
(c) c/1.37
(d) c/137
Show Answer & Explanation
Answer: (d) c/137
Explanation:
1. \(v = 2.18\times10^{6}\) m/s and \(c = 3\times10^{8}\) m/s give \(v/c = 1/137\).
2. Only option (d) agrees with this working.
Teacher's Note:
1. For spectral lines use 1/lambda = R Z^2 (1/n1^2 - 1/n2^2). The lowest n1 fixes the series (1 Lyman, 2 Balmer, 3 Paschen), and n(n-1)/2 gives the total number of possible lines.
(a) 15
(b) 12
(c) 14
(d) 10
Show Answer & Explanation
Answer: (a) 15
Explanation:
1. The levels involved are 2, 3, 4, 5, 6, 7, which is six levels, giving \(6\times5/2 = 15\) lines.
2. Only option (a) agrees with this working.
Teacher's Note:
1. For spectral lines use 1/lambda = R Z^2 (1/n1^2 - 1/n2^2). The lowest n1 fixes the series (1 Lyman, 2 Balmer, 3 Paschen), and n(n-1)/2 gives the total number of possible lines.
(a) the fourth orbit of Li\(^{2+}\)
(b) the second orbit of He\(^+\)
(c) the second orbit of Li\(^{2+}\)
(d) the fourth orbit of He\(^+\)
Show Answer & Explanation
Answer: (d) the fourth orbit of He\(^+\)
Explanation:
1. \(E\propto Z^2/n^2\)
2. H, n = 2: 1/4
3. He\(^+\), n = 4: 4/16 = 1/4.
Teacher's Note:
1. For spectral lines use 1/lambda = R Z^2 (1/n1^2 - 1/n2^2). The lowest n1 fixes the series (1 Lyman, 2 Balmer, 3 Paschen), and n(n-1)/2 gives the total number of possible lines.
(a) n = 3 to n = 5
(b) n = 1 to n = 2
(c) n = 2 to n = 1 (emits)
(d) n = infinity to n = 1 (emits)
Show Answer & Explanation
Answer: (b) n = 1 to n = 2
Explanation:
1. Absorption of 10.2 eV is needed for 1 to 2
2. The 3 to 5 jump needs only 0.97 eV, and the other two release energy.
Teacher's Note:
1. For spectral lines use 1/lambda = R Z^2 (1/n1^2 - 1/n2^2). The lowest n1 fixes the series (1 Lyman, 2 Balmer, 3 Paschen), and n(n-1)/2 gives the total number of possible lines.
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