317THE p-BLOCK ELEMENTS
N≡N) and to other second row elements (e.g.,
C=O, C=N, C≡N, N=O). This type of
π
- bonding
is not particularly strong for the heavier
p-block elements. The heavier elements do form
π
bonds but this involves d orbitals (d
π
– p
π
or d
π
–d
π
). As the d orbitals are of higher
energy than the p orbitals, they contribute less
to the overall stability of molecules than does
p
π
- p
π
bonding of the second row elements.
However, the coordination number in species
of heavier elements may be higher than for
the first element in the same oxidation state.
For example, in +5 oxidation state both N and
P form oxoanions : NO
3
–
(three-coordination
with
π
– bond involving one nitrogen p-orbital)
and
3
4
PO
−
(four-coordination involving s, p and
d orbitals contributing to the
π
– bond). In
this unit we will study the chemistry of group
13 and 14 elements of the periodic table.
11.1 GROUP 13 ELEMENTS: THE BORON
FAMILY
This group elements show a wide variation in
properties. Boron is a typical non-metal,
aluminium is a metal but shows many
chemical similarities to boron, and gallium,
indium, thallium and nihonium are almost
exclusively metallic in character.
Boron is a fairly rare element, mainly
occurs as orthoboric acid, (H
3
BO
3
), borax,
Na
2
B
4
O
7
·10H
2
O, and kernite, Na
2
B
4
O
7
·4H
2
O.
In India borax occurs in Puga Valley (Ladakh)
and Sambhar Lake (Rajasthan). The
abundance of boron in earth crust is less than
0.0001% by mass. There are two isotopic
forms of boron
10
B (19%) and
11
B (81%).
Aluminium is the most abundant metal and
the third most abundant element in the earth’s
crust (8.3% by mass) after oxygen (45.5%) and
Si (27.7%). Bauxite, Al
2
O
3
. 2H
2
O and cryolite,
Na
3
AlF
6
are the important minerals of
aluminium. In India it is found as mica in
Madhya Pradesh, Karnataka, Orissa and
Jammu. Gallium, indium and thallium are less
abundant elements in nature. Nihonium has
symbol Nh, atomic number 113, atomic mass
286 g mol
-1
and electronic configuration [Rn]
5f
14
6d
10
7s
2
7p
2
.
So far it has been prepared
in small amount and half life of its most stable
isotope is 20 seconds. Due to these reasons its
chemistry has not been established.
Nihonium is a synthetically prepared
radioactive element. Here atomic, physical and
chemical properties of elements of this group
leaving nihonium are discussed below.
11.1.1 Electronic Configuration
The outer electronic configuration of these
elements is ns
2
np
1
. A close look at the
electronic configuration suggests that while
boron and aluminium have noble gas
core, gallium and indium have noble gas plus
10 d-electrons, and thallium has noble gas
plus 14 f- electrons plus 10 d-electron cores.
Thus, the electronic structures of these
elements are more complex than for the first
two groups of elements discussed in unit 10.
This difference in electronic structures affects
the other properties and consequently the
chemistry of all the elements of this group.
11.1.2 Atomic Radii
On moving down the group, for each successive
member one extra shell of electrons is added
and, therefore, atomic radius is expected to
increase. However, a deviation can be seen.
Atomic radius of Ga is less than that of Al. This
can be understood from the variation in the
inner core of the electronic configuration. The
presence of additional 10 d-electrons offer
only poor screening effect (Unit 2) for the outer
electrons from the increased nuclear charge in
gallium. Consequently, the atomic radius of
gallium (135 pm) is less than that of
aluminium (143 pm).
11.1.3 Ionization Enthalpy
The ionisation enthalpy values as expected
from the general trends do not decrease
smoothly down the group. The decrease from
B to Al is associated with increase in size. The
observed discontinuity in the ionisation
enthalpy values between Al and Ga, and
between In and Tl are due to inability of d- and
f-electrons ,which have low screening effect, to
compensate the increase in nuclear charge.
The order of ionisation enthalpies, as
expected, is ∆
i
H
1
<∆
i
H
2
<∆
i
H
3
. The sum of the
first three ionisation enthalpies for each of the