2 - Atomic Structure (Engg) Sol
2 - Atomic Structure (Engg) Sol
INTEXT EXERCISE: 1
1. Hydrogen atom contains 1 proton, 1 electron and no m
8.
e = 1.5 × 10 e = 1.6 × 10-19
-8
neutrons.
\ m = 1.5 × 10-8 × 1.6 × 10-19 = 2.4 × 10-27 kg
2. Cathode Rays have constant b m
e l ratio.
\ m = 2.4 × 10-24 g
(e/m) e e/me
3. (e/m) = 2e/(4 # 1836m
3672
= 1 9. Charge on oil drop = - 6.39 × 10-19 C
a e)
a -1.602 × 10-19 C is charge on one electron
4. Factual.
\ - 6.39 × 10-19 C is charge on
5. rN + 10 -13 cm and ratom + 10 -8 cm
- 6.39 # 10 -19
Volume of nucleus
= = 4 electrons.
Volume fraction = Total vol. of atom - 1.602 # 10 -19
10. From a particle scattering experiment, distance of
(4/3) r (10 -13) 3
= = 10 -15 closest approach of a particle with nucleus came out
(4/3) r (10 -8) 3 to be of the order of 10-14 m. This scattering followed
6. R = RoA1/3 = 1.3 × 641/3 = 5.2 fm Coulomb’s law and gave the size of the nucleus to
7. Speed of cathode rays is less than speed of light. be < 10-14m.
INTEXT EXERCISE: 2
c 3 # 10 8 7. According to Planck’s Quantum Theory the
1. m = y = = 0.75 m minimum energy which can be absorbed from an
400 # 106
EM wave
2. Violet colour has minimum wavelength so maximum
energy. hc
=
m
hc
3. I.E. of one sodium atom = 8. E \
1
m m
& I.E. of one mole Na atom \ l1 = 2000 and l2 = 4000
hc 6.62 # 1034 # 3 # 108 # 6.02 # 10 23
N A = m
m 242 # 10 -9
E
\ E1 = 2 = 2
m1
= 494.65 kJ. mol.
2
9. u = 6 × 1014 Hz
4. Energy absorbed = 40 J/s
Now, c = ul
\ Energy released (as EM waves) =0.8×40= 32 J/s 1 y
\ y= = c
\ 32 × 20 =
nhc m
m
6×1014
⇒ n = 2 × 1021
\ y= = 2×106 m -1
3×108
1
5. y =
m hc
10. Eabsorbed = 500 = Ereleased
1
\ y= = 2 × 106 m-1 hc hc
500×10 -9 m Now, Ereleased = 800 +
m
6. 4 waves are passing through a given point in 2s. 1 1 1
= 500 - 800
a Frequence = no. of waves / sec. m
\ Frequency = 4/2 = 2 Hz ⇒
1
=
3
m 4000
\ l = 1333.3 nm
2.2 Chemistry
INTEXT EXERCISE: 3
6. S1 : Potential energy of the two opposite charge
1. r a b nZ l As Z increases, radius of 1st orbit decreases.
2
22
\ (n12 - n 22) = 24 = 13.6× 2 = 6.04 eV (i)
3
So, n1 = 5 and n2 = 1 d) Ionisation potential of He+
= 13.6×2 2 = 54.4 V (iii)
INTEXT EXERCISE: 4
Z2 (1) 2 For last line of Pachen series
1. E n = E1 E5 =- 13.6 # =- 0.54 eV
y 2 = R H (3) 2 < 2 - F= R
1 1
n2 (5) 2
(3) (3) 2
hc 1
2. m = 9E ` ma 9E R
Thus, difference = 4
3. Infrared lines = total lines – visible lines – UV lines
6 (6 - 1) 8. (He+)2 → 4 = (Li 2+) n 4 " n3
Total lines = 2 = 15 Z n n 2 2 4
\ Z1 = n 24 = n13 or 3 = n 4 = n3
visible lines = 4 (6 → 2, 5 → 2, 4 → 2, 3 → 2) 2
UV lines = 5 (6 → 1, 5 → 1, 4 → 1, 3 → 1, 2 → 1) \ n4 = 3 and n3 = 6.
\ Transition in Li2+ ion = 3 → 6
4. When electron falls from n to 1, total possible
9. y1 = Rc Z 2 c 2 - 2 m = Rc Z 2 ,
1 1
number of lines = n – 1.
n1 3
5. Visible lines ⇒ Balmer series (5 → 2, 4 → 2, 3 → 2)
y 2 = Rc Z 2 c 2 - 2 m = 4 Rc Z 2 .
1 1 3
So, 3 lines.
1 2
y3 = Rc Z 2 c 2 - 2 m = 4 Rc Z 2
6. According to energy, E 4 " 1 > E3 " 1 > E 2 " 1 > E3 " 2 . 1 1 1
2 3
According to energy, Violet > Blue > Green > Red. \ u 1 - u 2 = u 3.
\ Red line ⇒ 3 → 2 transition.
10. Visible lines ⇒ Balmer series ⇒ only in H atoms.
7. For 1st line of Balmer series In H like species, e.g. He+, we cannot make
generalizations of certain lines lying in the visible
y1 = R H (3) 2 < 2 - F = 9R b 5 l = 5 R
1 1
(2) (3) 2 36 4 region.
Atomic Structure 2.3
INTEXT EXERCISE: 5
1. For photoelectric effect to take place, 6. P.E.E. occurs only if uin > uo
Elight > f K.E. ∝ uin not velocity of photoelectron.
\
hc
$
hc
or m # m 0 . 7. K.E.max = huin - f
m m0
2. Photoelectric effect is a random phenomena. So, 8. uincident = u1
electron may come out with a kinetic energy less K. E. =
hc
-z
than or equal to (hu – w) as some energy is lost m1
hc z
while escaping out. \ stopping potential = -
m1 e e
3. If u > u0, emission takes place with a maximum K.E. when uincident = u2
of hu-huo. The K.E. is independent of the intensity hc z
but the number of photoelectrons increases with stopping potential = -
m2 e e
intensity.
\ stopping potential increase by e c
hc 1 - 1 m
hc m 2 m1
4. = 1 + z ...(1)
m
hc 9. | Max K.E. | = | stopping potential |
3# = 4 + z ...(2)
m
\ K.E.max = 1.5 eV also f = 2.5 eV
from, e.q., (1) and (2) z = 0.5 eV
\ Eincident = 1.5 + 2.5 = 4 eV
5. Number of lines in Balmer series = 2 10. K.E.mzx = Ein - f = 6 - 2.1 eV
\ n = 4 (lines will be 4 → 2, 3 → 2). = 3.9 eV
KE of ejected photoelectrons
\ stopping potential = - 3.9 eV
13.6
= Ephoton - En = 13 - 2 = 13 - 0.85 = 12.15 eV.
4
INTEXT EXERCISE: 6
-34
h 6.625 # 10 # h
7. 9p $ 9x = 4r
1. m = mv = 0.2 # 5 3600 . 10 -30 m.
6.62 # 10 -34
2.
m1
= V2 =
V 200 2 ⇒ 9x = = 5.27 # 10 -30 m.
m2 1 50 = 1 . 4 3.14 # 1 # 10 -5
#
3. r1 = 0.529 A c my mx vx my m vx 16
8. = & 1 = (0.25m )x (0.75v = 3 .
r3 = 0.529 # (3) 2 Ac = 9x mx my vy x x)
2rr 2r (9x)
So, m = n = 3 = 6rx. h
9. m = mv
o
12.3
4. m = A gives the De-Broglie wavelength of an mp m v
V = map vap m = 4mp
ma
electron accelerated by V volts.
mp 4m v 1 va vp 8
n n n 2 4 = m pav pa 2 = 4 # vp va = 1
5. m \ Z ` Z1 = Z2 or 3 = 6 (n = 4 of C5+ ion) ma
1 2
h 10. l = v
6. For a charged particle m = h h
2mqV
then m = mv or m2 = m
1
\ m\ . h
V
So, m= m
INTEXT EXERCISE: 7
h
\ No. of unpaired electron = 4.
1. Orbital angular momentum = , (, + 1) 2r = 0.
X26 : 1s22s22p63s23p63d84s2.
\ l = 0 (s orbital).
To get 4 unpaired electrons, outermost configuration
2. Cu:1s 2 2s 2 2p6 3s 2 3p6 3d10 4s1 . will be 3d6.
\ Cu 2+:1s 2 2s 2 2p6 3s 2 3p6 3d9 or 6Ar@ 3d9 .
\ No. of electrons lost = 2 (from 4s2).
3. Magnetic moment = n (n + 2) = 24 B.M.
\ n = 2.
2.4 Chemistry
4. Zn2+ : [Ar]3d10 (0 unpaired electrons). h
8. Orbital angular momentum = , (, + 1) 2r
Fe 2+
: [Ar]3d (4 unpaired electrons) maximum.
6
Now for 2s orbitals, l = 0
Ni 3+
: [Ar]3d7 (3 unpaired electrons). \ Orbital angular momentum = 0
Cu+ : [Ar]3d10 (0 unpaired electrons). 9. 17
Cl- : [Ne]3s23p6
5. d7 : 3 unpaired electrons Last electron enters 3p orbital.
n
\ Total spin = ! 2 = ! 2 .
3
\ , = 1 and m = 1, 0, - 1.
10. n = 3 can have l= 0, 1, 2
6. X23 : 1s22s22p63s23p63d34s2.
if l = 0 ⇒ orbital angular momentum = 0
No. of electron with , = 2 are 3 (3d3) .
2h
if l= 1 ⇒ orbital angular momentum = 2r
7. Cr (Zn = 24)
electronic configuration is :1s 2 2s 2 2p6 3s 2 3p6 4s1 3d5 6h
if l= 2 ⇒ orbital angular momentum = 2r
So, no. of electron in , = 1 i.e., p subshell is 12 and
no. of electron in , = 2 i.e., d subshell is 5.
INTEXT EXERCISE: 8
1. For 6g orbitals, n = 6 and l = 4. 6. Spherical node = n -l- 1
\ Radial nodes = n -l- 1 = 6 - 4 - 1 = 1 and non spherical =l.
Angular nodes =l= 4 7. The dual nature of electrons is the premise on which
\ Total 5 nodes. this model is based.
2. The radius of maximum probability of 1s orbital of 8. i) Electron density in the XY plane in 3d x - y 2 2
is not zero
\ A is 1s and B is 2s iii) 2s orbital has one nodal surface-it is a spherical
4. Dumbell lies at 45o to x & y axis represents dxy node.
orbital. iv) For 2pz orbital, XY is the nodal plane
5. XZ is the nodal plane of px orbital 9. Factual.
10. n, l and m, are obtained from y.
EXERCISE - 1
16. E = - 13.6
Z2 34. E in L shell (n = 2) = - 3.4 ev. If it loses 10.2 eV then
n2 new energy = (- 3.4 - 10.2) eV
1
= - 13.6 × 9 = - 1.51 eV
= 13.6 eV.
17. rn = ron2 ⇒ r3 = 9ro 35.
E1 = - 54.4 eV
18. E at n = 1 = - 13.6 eV - 54.4
\ E2 = 4 =- 13.6 eV
E at n = 2 = - 3.4 eV
\ I. E. = 13.6 eV.
E at n 3 = - 1.51 eV 36. Theoretical.
1st excitation potential = 10.2 37. Free electron at rest has 0 energy. When the electron
2nd excitation potential = 12.09 eV is bound to an atom, its energy is therefore negative.
19. I.E. from n = 3 is 1.51 eV 38. Shortest line of Paschen ⇒ n = 3 $ n = 3
\ E3 = - 1.51 eV = R3 2 : 9 - 3 D
1 1 1
m
\ E1 = - 1.51 × 9 = - 13.6 eV
1
13.6 \ m= R
\ E2 = - 4 = - 3.4 eV
39. Z = 2
20. L shell —→ n = 2
n = 2 → n = 1 (Longest l for lowest DE)
E = -3.4 eV
= R × 4 :1 - 4 D = R × 4 : 4 D
1 1 3
P.E. = 2 × -3.4 eV = -6.8 eV m
- P.E.
1
\ m = 3R (b)
21. K.E. =- T.E. = 2
22. K.E. decreases and total energy increases. 40. Z = 1
23. The charge on the nucleus of atomic no. Z n = 3 $ n = 1 (Shortest l for highest DE)
1
24. -3.4 eV (When n = 2). The possible value of energy = R x 1[1] = R
m
13.6
are - 2 eV where ‘n’ is an integer.
1
\ m= R =x
n
25. Bohr said that electrons neither gain nor lose energy Z = 2
when they are at particular orbits and hence these
n = 3 → n = 2
orbits are called stationary states.
= x × 4 : 4 - 9 D
1 1 1 1
26. Emission spectra is diserect, unequally spaced with m
varying intensity.
= x × 4 : 36 D
1 1 5
m
27. Electrons reaching n = 4 from any state emits EM
1 1 5
waves in the Brackett series. = x × 9
m
28. The energy of the orbits keep changing with Z. Thus m= 5
9x
line spectra of no two elements are indetical.
2.6 Chemistry
41. Photo electric emission occurs when u > uo 61. spin Q.N. is not obtained from y.
42. Refer Q. 41 above 62. Theoretical
43.
V I B G Y OR 63. Degenerate orbitals are such orbitals which have
decreasing frequency same energy.
So only V, I, B, G can cause emission
64. For m = 2, l can be from - 2 to 2.
44. It establishes the existence of quantum of energy,
65. If n = 2 then l can be 0 or 1.
which is a packet of energy.
66. An orbital can have maximum 2 electrons.
45. h (u1 - u0) = K.E.
u1 then K.E. - 67. For principal Q.N. n, number of possible values of
l is also n. Hence, number of subshells = n.
1242
46. E =
m (nm) 68. No. of subshells = n = 3.
4=
1242
No. of orbitals in 3s, 3p, 3d = 1 + 3 + 5 = 9.
m (nm) o
69. d x - y orbitals are double dumbbell shaped with its
2 2
l (nm) = 310.5 nm = 3105 A
two lobes lying along the x and y axes.
47. KE1 = E1 - f 70. Since m = -1, therefore it cannot be s-orbital
KE2 = 2E1 - f becuase for s-orbital m = 0.
\ K.E.2 = 2K.E.1 + f 71. Orbital anular momentum = 2r , ], + 1g
h
48. Changing frequency changes the K.E. of the 72. m can be -lto +l. So no. of values possible
photoelectron, not the number of electrons ejected.
= 2l+ 1.
Photocurrent increases on increasing intensity to
and attains a maximum value. 73. 19th electron goes to 4s orbital in Chromium.
49. Theoretical. 74. Fe3+ : [Ar] 3d5
50. Definition of work function. Co2+ : [Ar] 3d7
55. For 2 electrons in same orbital, n, l, m are same but 77. s-orbital is spherically symmetric. The probability
s is different. distribution is uniform in all directions independent
of the angle.
56. No. of orbitals in a subshell = 2l+ 1. Since each
orbital can have a maximum of 2 electrons therefore, 78. No. of radial nodes = 4 - 2 - 1 = 1.
maximum no. of electrons = 2 (2l+ 1). Thus (d) is correct.
57. n = 2 may have one s and 3 p orbitals with a maximum 79. Radial nodes = 5 - 3 - 1 = 1
of 8 electrons. Node at infinity = 1
58. n = 2 l= 1 for 2 p orbitals. Angular node = 3
\ Total number of nodes = 5
59. f-subshell has 7 orbitals and can accomodate a
maximum of 14 electrons. 80. No. of radial nodes for 5d orbitals = 5 - 2 - 1 = 2
60. p orbital is dumbell shaped. Number of maxima in graph = no. of nodes + 1 = 3.
Atomic Structure 2.7
EXERCISE - 2
1. Isotopes have same atomic number and different 13. N shell ⇒ n = 4
mass number. - 13.6 × 4 2
\ E4 (Bi3+) = = - 13.6 eV
2. The a-particles (He2+ ions) get deflected by the 42
Now, P.E. = 2 T.E. = - 27.2 eV
positively charged nucleus due to the electrostatic
forces of repulsion. - 13.6
14. P.E. of n = 2 of H atom = 2 × 4 = - 6.8 eV
3. Rutherford discoverd the nucleus by this experiment.
6.8
Now, for He+ if K.E. = 2 , T.E. = - 3.4
4. rnu = 1.25 × 10-13 × 641/3 cm = 5 × 10-13 cm \
- 13.6×4
=- 3.4 & n = 4
n2
ratom = 10-8 cm
0.529×9 o 0.529×16 o
V r3 125×10 -39 15. r3 (He+) = A and r4 (He+) = A
\ V Nu = 3nu = = 1.25 × 10-13 2 2
atom r atom 10 -24 0.529 o o
\ r4 - r3 = 2 (16 - 9) A = 1.851 A
5. A = 39 ⇒ n + p = 39 and n = (p+1)
\ (p + 1) + p = 39 ⇒ p = 19 16. r4 (Z) =
0.529×16
Z
Also, e = 19 r1 (H) = 0.529
Now, n = (p + 1) = 20.
\ Z = 25 from the given options
6. In an element ZA X ,
Note: for Z = 16 it overlaps and doesn’t fit inside
no. of protons = electrons = Z the 1st Bohr orbit of H.
no. of neutrons = A - Z ro $ 4 RZ
28×60 + 29×30 + 30×20 17. r2 = R =
Z & ro - 4
Mavg = 110 RZ 9 9
= 28.64.
\ r3 = 4 × Z = 4 R = 2.25R
7. Atomic electrically neutral as well as nucleus n2
18. 0.529× 4 = 0.529
contains neutrons but neutrality is due toequal
number of protons and electrons. n ` =2
hc
8. Eabsorbed =
Ereleased =
hc hc
+ 19. rn \ n 2
^n 22 - n12h
m m1 m 2
\ Spacing is maximum when is
hc hc hc mm maximum.
\ = + &m= 1 2
m m1 m 2 m1 + m 2
1
9. Let no. of quanta absorbed and emitted be na and ne 20. E n \
n2
respectively.
\ spacing in terms of energy is maximum when
n a hc n e hc 1 1
\ Ea = 4500 and Ee = 5000 - is maximum.
n12 n 22
ne 1 na
Now, Ee = 0.5 Ea & 5000 = 2 × 4500 21. r \ n 2 and time period \ n3
n 5000 5
\ nea = 9000 = 9 = 0.55 r 1 T
since r12 = 4 & T1 = 8
1
2
10. Rest mass is not property of photons as they never 22. Bohr’s model cannot explain emission spectrum of
come to rest. multi electron species.
hc
11. E of quanta able to ionize Na = 23. More the energy of an electron, for ther a way from
2414 ×10 -10
the nucleus it can stay.
hc 6.02×10 23
\ I. E. of Na = -10 × kJ/mol
2414×10 103 24. E3 - E1 = 12.09 eV for H atoms.
. 497 kJ/mol.
Other permissible values of energy absorbed may be:
12. P.E. = 2 T.E. ⇒ T.E. = - 3.4 eV. Z = 2 : 12.09 × 4 = 48.36 eV
- 13.6
\ - 3.4 = Z = 3 : 12.09 × 9 = 108.81 eV
n2
⇒ n=2 and so on.
\ 1 excited state.
st
2.8 Chemistry
25. From III to I,
= R ×1 : 9 - 16 D
1 1 1
\
hc m
2 E - E = E = .....(1)
m 1 7R
From II to I =
m 144
4E E hc 144
3 - E = 3 = m1 ..... (2) m = 7R
Hence, potential should be dropped by 25 V. 18. 3 → 2, 2 → 1, 3 → 1.
19. 5.27 = f + 0.27 ⇒ f = 5
12400
5. 3 E = 6200 = 2 eV.
20. Cu+ has 3d10 configuration. So, no. of electrons with
bs =- 1 l = 5
2 × 1.6 × 10-19 × n = 40 × 60 × 0.5
n = 3.75 × 1021 2
6. n = 2, l= 0, 1, 2, 3 = 1.09677×10 +7 ×Z 2 :1 - 4 D
1 1 1
21.
\ for last subshell, n = 2 and l= 3. 3×10 -8
4
\ n + l= 5
or, Z 2 =
3×3×1.09677×10 -8 ×10 +7
7. 2nd line of Balmer series ⇒ 4 → 2
⇒ Z2 = 4 ⇒ Z =2
1st line of Lyman series ⇒ 2 → 1 22. Maximum m = + 3 ⇒ l= 3 ⇒ n = 4
= R : 4 - 16 D & m B = 3R \ No. of waves by the electron in the fourth orbit = 4
1 1 1 16
\
mB
23. n l = 2 p r ⇒ n 200 = 400 ⇒ n =2
= R :1 - 4 D & m L = 3R
1 1 4
mL R R
24. E =- 9H =- 2H & n = 3 .
m n
\ B =4
mL No. of electrons that can be accomodated in n = 3 is
8. 4d orbital has 1 radial node, as (n -l- 1) = 1 2 × 32 = 18.
\ No. of peaks = no. of radial nodes + 1 = 2
\ No. of orbitals presents in n = 3 is 9. All these
9. b ro n4 l = ]rogH & n = 2
2 orbitals are degenerate as of single electron
Be 3+ species E3s = E3p = E3d and so on.
]5 - 2g]5 - 2 - 1g 25. 4→2 in He+ has same energy difference as 2→1 of H.
10. No. of lines = 2 =6
Atomic Structure 2.11
EXERCISE - 4
10.
1. For He+ : x = R $ 4 ; - E & Rc 2 - 2 m = x
1 1 1 1 C contains 6 protons and 6 neutrons and weighs
12
6
n12 n 22 n1 n 2 4 12 amu. Mass of electron is negligible.
Now, if mass of neutrons is halved, total mass = 9
= R $ 16 ; 2 - 2 E & = 16× 4 = 4x
1 1 1 1 x
For Be3+ : amu.
m n1 n 2 m
3
2. Note that the question states that there is a single H
\ reduction in mass = 3 amu ⇒ 12 × 100 = 25%
atom. Thus, the maximum number of spectral lines 11. Factual.
emitted may be 3 for the transitions 5 → 4, 4 → 3
and 3 → 2. 12. Red end ⇒ we are talking about visible region of the
EM spectrum ⇒ Balmer series in an H atom.
3. The lowest value of ‘n’ for which d-orbital exists Thus, 3rd line from red end ⇒ 5 → 2
is 3.
13. Balmer series lines of only H atoms lies in the visible
\ Electronic configuration given is 3d6 4s2
region of the spectrum
⇒ 4th period.
14. K shell ⇒ n = 1
4. DE2→1=13.6 b 1 - 4 l eV and DE3→2=13.6× b 4 - 9 l eV
1 1 1 1
L shell ⇒ n = 2
3 5 M shell ⇒ n = 3 and so on
= 13.6× 4 eV = 13.6× 36 eV
Since electron makes transition into n = 2, therefore
\
3 E2 " 1 3/4 27 it is Balmer series.
3 E3 " 2 = 5/36 = 5
15. Lyman series is in UV region and Balmer series is in
5. Factural : K. E.max = huincident - f visible region in H atom.
6. Orbital angular momentum = 2r , ], + 1g = 2r
The 4 lines in uv region are : 2→1, 3→1, 4→1, 5→1
h 6h
3h
In the visible region we will have: 3→2, 4→2, 5→2
angular momentum in 3rd Bohr orbit = 2r
\ In the IR region: 5→4, 5→3, 4→3 ⇒ 3 lines
6 2
\ ratio = 3 = 3 16. Rest mass of photon =
h
cm
7. m = 1.73 = 3 = n ]n + 2g
= R :1 - 4 D = 4 R
1 1 3
For 1st line of Lyman:
\ no. of unpaired electrons, n = 1. m1
Now Vanadium has Z = 23 and E.C. of [Ar] 4s23d3 = R : 4 - 9 D = 36 R
1 1 1 5
For 1st line of Balmer:
m2
\ for 1 unpaired electron V must be in + 4 state
m m m 3 36 27
with an E.C. of [Ar] 3d1.
\ m12 = 2 & m12 = 4 × 5 = 5
m1
1
8. 4.25 - fA = TA and lA \ 17. Series limit of any series & 3 $ n1
TA
= R :1 - 3 D &
1 1 1 1
1 \ For Lyman series: =R
4.2 - fB = TB and lB \ mL mL
= R; 2 - 3 E &
TB 1 1 1 1 R
a lB = 2 lA For Balmer series: = 4
mB 2 mB
\ TA = 4 TB \ lL = 4 lB
Now, TB = TA - 1.5 ⇒ 3 TB = 1.5 18. Theoretical
⇒ TB = 0.5 eV and TA = 2 eV
19. Spectral lines of an element are unique and no 2
\ fA = 4.25 - TA = 2.25 eV lines of an element can have the same wavelength.
and fB = 4.2 - TB = 3.7 eV 20. y2 is the probability density i.e. probability per unit
9. 2.1 g ion of Cl- ⇒ 2.1 mole Cl- ions volume.
Now, 1 Cl- ion has 18 electrons 21. In H atom
\ 2.1 mole Cl contains 18 × 2.1 × NA electrons
- Elyman > Ebalmer > Epaschen ..........
\ llyman < lbalmer < lpaschen
\ l1 < l2 < l3 < l4
2.12 Chemistry
o o 36. In H atom, or any other H like species, the energy of
22. For n = 10, r = 0.529 × 102 A = 52.9 A
the electron depends only on the value of ‘n’. Thus,
\ 2 × p × 52.9 = 10 l we can say that for such species (E4s = E4p = E4d =
\ l = 33.22 A
o
E4f) > E3s = E3p = E3d and so on.
II : Zero radial nodes ⇒ 3d 38. Heisenberg’s uncertainty principle is valid for both
microscopic and macroscopic moving objects.
III : 2 radial nodes ⇒ 3s
However, it is significant only for microscopic
24. Longest wavelength of Paschen series ⇒ 4 → 3 objects.
\ R $ 1 2 $ : 9 - 16 D = R $ 2 2 $ ; 2 - 2 E
1 1 1 1
h
39. 3 x $3 p $ 4r : by definition.
n1 n 2
⇒ n1 = 6 and n2 = 8. dp
Now, dt = dF⇒ dp = dF.dt
25. y2 is maximum at nucleus and 3p r2 y2 is zero.
dE
hc And dF $ dx = dE & dx = dF
26. E = hu = = hc y
m dE
hc \ dp $ dx = dF $ dt $ dF
Also, Etot = n , but energy of 1 quantum is
m
= dE $ dt
independent of n.
27. \ -particles being much heavier than the electrons \ Heisenberg’s principle may be written as
have a high penetrating power, which is also because h
3 E $3 t $ 4r
of the high speed of \ -particles.
40. In option (c) if l= 2 then ‘m’ cannot be - 3.
28. All 4 statements were conclusions drawn from the
\ -scattering experiment. 41. a) s-orbital is spherically symmetric
29. Bohr’s model doesn’t talk about probabilities. Hence b) shape of orbital is given by ‘l’ not ‘m’.
statement (a) is incorrect. c) Since l= 0, therefore orbital angular momentum
30. Bohr derived that = 0 for 1s, 2s, 3s etc.
n2 Z Z2 d) Electrons in different orbitals have different
rn \ Z , v n \ n and freq \ 3 velocities.
n
Kq q KZe 2 Z3 42. For 3d orbitals: n = 3, l= 2, m = -2, -1, 0, 1, 2 and
]n /Zg
Now, Force = 2 & F \ 2 2 F \ 4
1 2
r n s = + 0.5
31. 2nd I.E. of He = 13.6 × 22 eV 43. If ‘l’ of two orbitals are same, then their orbital
3rd I.E. of Li = 13.6 × 32 eV angular momentum is also same.
1st I.E. of H = 13.6 eV 44. b) if n = 3 then l can be 0 or 1 or 2.
o o
9
r3 of H = 0.529 × 9 A and r3 of Li2+ = 0.529 × 3 A d) if l= 2 then m can be 0 or + 1 or + 2.
n,land m are the 3 Q.N. which can define an orbital. 45. All 3 statements are correct.
Z2 Z2 46. All 3 statements are correct.
32. K.E. K.E. \2 , P.E. \ - 2 , rn = ro $ n
2
n n
47. electron cloud density of px orbital
Energy levels or orbits are not equally spaced. The
distance between the orbits keeps increasing with n. 48. (2) is the excited state electronic configuration of (1)
33. Bohr’s model can be applied to all single electron 49. (b) For n = 2 we can have 4 orbitals but they all do
species. not have different energy levels. Out of the 4, 3
are degenerate and have different energy from
n3
34. Frequency \ the 4th.
Z2
(c) M ⇒ n = 3 and can accommodate a maximum
35. For electronic transition from n → 1, no. of spectral
n ]n - 1g
of 18 electrons.
lines is given by 1 + 2 + 3 + ..... (n - 1) = 2
Atomic Structure 2.13
50. Quantum numbers are derived by solving the 2.178×10 -11
Schroedinger’s wave equation. For a multi-electron 62. T.E.3 = - 9 ergs
species, the energy of an electron can be estimated a P.E. = 2 T.E.
by the value of (n +l). Azimuthal Q.N. does not 2
\ P.E. = - 9 ×2.18×10 -11 ergs
tell us anything about the motion of the electron.
= - 4.84 × 10-12 erts
51. Shape of orbital is given by azimuthal Q.N. Also,
h
electrons in an atom move with different velocities. 63. m =
2m ]K.E.g
52. Due to the presence of electrons in them the orbital
h
ex-orient themselves to minimize the energy in a 64. m =
2m qV
magnetic field.
6.625×10 -34
53. Spin of electron does not affect the angular 5 × 10-12 =
2×1.67×10 -27 ×1.6×10 -19 ×V
momentum and can be represented as clockwise and
Solving we get V = 32.8 V
anticlockwise.
65. m = 75 × 10-3 kg
54. Factual.
h 6.625×10 -34
55. E4s < E3d. If n = 2 the there are 4 orbitals which can Dx = l = mv ⇒ Dx =
75×10 -3 ×4
accommodate a maximum of 8 electrons. If n = 5 h 6.625×10 -34
then maximum no. of electrons in it is 2n2 = 50. \ Dv = 4rm 3 x =
4×3.14×75×10 -3 ×2.2×10 -33
56. If n = 4 and m = - 2, it may be a 4d or 4f orbital. The = 0.32 m/s
1 1
spin of the electron may be + 2 or - 2 . 66. No. of electrons possible in an orbital = 4
57.
l= 1 to (n + 1)
, ,
electron p q x y z
m = - 2 to + 2
n 3 3 3 3 3
For n = 1 ⇒ l= 1, 2 i.e. 1A, 1B
m 0 0 1 1 1
For n = 2 ⇒ l= 1, 2, 3 i.e. 2A, 2B, 2C
l 0 0 -1 +1 0
For n = 3 ⇒ l= 1, 2, 3, 4 i.e. 3A, 3B, 3C, 3D
s - 1
2 + 1
2 + 1
2 + 1
2 + 1
2
Now, for l= 1 : m = - 1 2 , + 1 2
58. K.E. of photo electron varies with u and l but is
l= 2 : m = -1, 0, 1
constant with intensity.
3 1 1 3
l= 3 : m = - 2 , - 2 , + 2 , + 2
59. A1 = p r12 An = p rn2 and rn = r1n2
l= 4 : m = -2, -1, 0, 1, 2
\ A subshell has 2 orbitals
\ b An l = & ln b An l = 4ln (n)
2 4
A rr n A
1
1 rr12 1 B subshell has 3 orbitals
\ Graph of ln b An l vs ln (n) is a straight line with
A
\ E.C. would be as follows:
1
1A 8
1B 12
2A 8
2B 12
3A 8
.....
slope = 4 and this line passes through the origin. 14444244443 14444244443
1st period 2 nd period
22
b) r2, 1 = ro 1 = 4 ro
12 r
and r1, 2 = ro 2 = 2o c) 5 degenerate orbitals ⇒ d-orbitals
When n = 2, Z = 4.