Practice MCQs for JEE Chemistry Structure Of Atom
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Multiple Choice Questions
(a) V/3
(b) V
(c) 3V
(d) 9V
Show Answer & Explanation
Answer: (b) V
Explanation:
1. \(v\propto Z/n\)
2. For H(n = 1) it is 1; for Li\(^{2+}\)(Z = 3, n = 3) it is 1
3. So the speed is V.
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) Potential energy of two opposite charges increases when they come closer
(b) Kinetic energy of the electron increases when it moves to a lower orbit
(c) Potential energy of the electron increases when it moves to a higher orbit
(d) An 11 eV photon cannot free the electron from the first excited state of He\(^+\)
Show Answer & Explanation
Answer: (a) Potential energy of two opposite charges increases when they come closer
Explanation:
1. Potential energy of opposite charges \(-kq_1q_2/r\) becomes more negative (decreases) as they approach, so the first statement is false
2. The other three are true: KE \(=-E\) rises as n falls; PE \(=2E\) rises with n; and the binding energy of n = 2 in He\(^+\) is 13.6 eV, more than 11 eV.
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
(b) 1 : 4
(c) 2 : 1
(d) 1 : 8
Show Answer & Explanation
Answer: (d) 1 : 8
Explanation:
1. \(T\propto n^3\), so \(T_1:T_2 = 1:8\).
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) 1 : 4
(b) 1 : 8
(c) 4 : 1
(d) 8 : 1
Show Answer & Explanation
Answer: (b) 1 : 8
Explanation:
1. \(r\propto n^2\), so \(n = 1\) and \(n = 2\)
2. \(T\propto n^3\) gives 1 : 8.
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) \(+\dfrac{3e^2}{8\pi\varepsilon_0r}\)
(b) \(-\dfrac{3e^2}{8\pi\varepsilon_0r}\)
(c) \(+\dfrac{3e^2}{4\pi\varepsilon_0r}\)
(d) \(-\dfrac{3e^2}{4\pi\varepsilon_0r}\)
Show Answer & Explanation
Answer: (a) \(+\dfrac{3e^2}{8\pi\varepsilon_0r}\)
Explanation:
1. For nuclear charge Ze, \(KE = Ze^2/(8\pi\varepsilon_0r)\), positive
2. With Z = 3 this is \(3e^2/8\pi\varepsilon_0r\).
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 and 3
(b) 3 and 5
(c) 2 and 5
(d) 2 and 4
Show Answer & Explanation
Answer: (d) 2 and 4
Explanation:
1. \(E_n = -13.6/n^2\): \(E_2 = -3.4\) and \(E_4 = -0.85\) eV, difference 2.55 eV. No other pair of the given levels has a gap of 2.55 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) 54.4 eV
(b) 40.8 eV
(c) 13.6 eV
(d) 122.4 eV
Show Answer & Explanation
Answer: (a) 54.4 eV
Explanation:
1. \(\Delta E_{1\to2} = \tfrac34\times IE = 40.8\) eV, so \(IE = 54.4\) eV (this is He\(^+\), Z = 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) y
(b) z
(c) all are equal
(d) x
Show Answer & Explanation
Answer: (d) x
Explanation:
1. Energy gaps: x \(= 1-1/9 = 0.889\), y \(= 1/4-1/16 = 0.1875\), z \(= 1/9-1/25 = 0.071\) (in units of 13.6 eV)
2. The largest gap gives the shortest wavelength.
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) 8 V
(b) 16 V
(c) 12 V
(d) 4 V
Show Answer & Explanation
Answer: (c) 12 V
Explanation:
1. First excitation energy \(= \tfrac34\times\) ionisation energy \(= 0.75\times16 = 12\) V.
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) 32
(b) 18
(c) 8
(d) 50
Show Answer & Explanation
Answer: (a) 32
Explanation:
1. \(r = 8.46\) A \(= 0.529n^2\), so \(n^2 = 16\) and n = 4
2. The shell holds \(2n^2 = 32\) electrons.
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) 4
(c) 5
(d) 3
Show Answer & Explanation
Answer: (d) 3
Explanation:
1. Energy \(= 3.85\) eV \(= 54.4(1/n^2-1/(n+2)^2)\), so the bracket is about 0.0708
2. For n = 3, \(1/9-1/25 = 0.0711\); n = 2 gives 0.188 and n = 4 gives 0.0347.
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) 656 nm and 410 nm
(b) 486 nm and 434 nm
(c) 656 nm and 486 nm
(d) 122 nm and 103 nm
Show Answer & Explanation
Answer: (c) 656 nm and 486 nm
Explanation:
1. \(1/\lambda = R(1/4-1/9)\) gives 656 nm (3 to 2) and \(R(1/4-1/16)\) gives 486 nm (4 to 2)
2. These Balmer lines are the two longest.
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) 3
(b) 2
(c) 4
(d) 1
Show Answer & Explanation
Answer: (b) 2
Explanation:
1. \(1/\lambda = R_HZ^2(1-1/4)\), so \(Z^2 = 1/(3\times10^{-8}\times1.097\times10^{7}\times0.75) = 4.05 \approx 4\) and Z = 2 (He\(^+\)).
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) 21
(b) 28
(c) 22
(d) 36
Show Answer & Explanation
Answer: (c) 22
Explanation:
1. H, n = 2: \(2\times1/2 = 1\) line
2. He\(^+\), n = 4: \(4\times3/2 = 6\) lines
3. Li\(^{2+}\), n = 6: \(6\times5/2 = 15\) lines
4. Total \(1+6+15 = 22\).
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 number of electrons making the transition
(b) the energy difference of the transition
(c) the nuclear charge only
(d) the velocity of the electron
Show Answer & Explanation
Answer: (b) the energy difference of the transition
Explanation:
1. \(\lambda = hc/\Delta E\), so \(\lambda\) varies inversely with the energy difference between the two levels.
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) n - 1
(b) n
(c) n - 2
(d) n(n + 1)
Show Answer & Explanation
Answer: (a) n - 1
Explanation:
1. Each Lyman line ends at n = 1 and starts from one of the other n - 1 levels.
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) 4
(b) 5
(c) 3
(d) 10
Show Answer & Explanation
Answer: (c) 3
Explanation:
1. Visible lines end at n = 2: 5-2, 4-2 and 3-2
2. That is 3 lines.
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) 9x/5
(b) 36x/5
(c) 5x/9
(d) 5x/36
Show Answer & Explanation
Answer: (b) 36x/5
Explanation:
1. Lyman limit: \(1/x = R\)
2. First Balmer line: \(1/\lambda = R(1/4-1/9) = 5R/36\), so \(\lambda = 36/5R = 36x/5\).
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) 12.15 eV
(b) 11.49 eV
(c) 12.46 eV
(d) 12.63 eV
Show Answer & Explanation
Answer: (a) 12.15 eV
Explanation:
1. Two Balmer lines (n to 2 and one more) means the highest level is n = 4 (4-2 and 3-2)
2. Binding energy \(= 13.6/16 = 0.85\) eV, so \(KE = 13-0.85 = 12.15\) eV.
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) \(7R/144\)
(b) \(7R/9\)
(c) \(7R/16\)
(d) \(R/144\)
Show Answer & Explanation
Answer: (b) \(7R/9\)
Explanation:
1. For Be\(^{3+}\) (Z = 4): \(\bar\nu = 16R(1/9-1/16) = 16R\times7/144 = 7R/9\).
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) the ultraviolet region, because the energies are four times those in hydrogen
(b) the visible region, as for hydrogen
(c) the infrared region
(d) the X-ray region only
Show Answer & Explanation
Answer: (a) the ultraviolet region, because the energies are four times those in hydrogen
Explanation:
1. For He\(^+\), \(\bar\nu = 4R(1/4-1/n^2)\), four times as large as the hydrogen Balmer value
2. The first line \(5R/9\) has \(\lambda \approx 164\) nm, which is ultraviolet.
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) ultraviolet region
(b) visible region
(c) microwave region
(d) infrared region
Show Answer & Explanation
Answer: (d) infrared region
Explanation:
1. \(\bar\nu = 1.10\times10^{5}(1/25-1/100) = 3300\) cm\(^{-1}\), so \(\lambda = 3.03\times10^{-4}\) cm \(\approx 3030\) nm
2. This is infrared.
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) 6
(b) 8
(c) 5
(d) 7
Show Answer & Explanation
Answer: (b) 8
Explanation:
1. The series ends at n = 4 (\(E_4 = -0.85\) eV)
2. Highest energy photon from level x: \(0.85-13.6/x^2 = 0.6375\), so \(13.6/x^2 = 0.2125\) and \(x^2 = 64\), x = 8.
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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Practice MCQs for JEE Chemistry Structure Of Atom
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