Each electron must move about the nucleus in
an electrical field generated by the positive charge of the nucleus
and the negative charges of the other electrons. Coulomb's
law determines the potential energy of attraction of each electron
to the nucleus:
Vr=((Z)e)(−e)r
V
r
Z
e
e
r
(1)where
(Z)e
Z
e
is the charge on the nucleus with
atomic number ZZ
and
−e
e
is the charge on the electron, and r is the
distance from the electron to the nucleus. The potential energy of
an electron in an atom is negative. This is because we take the
potential energy of the electron when removed to great distance
from the atom (very large rr)
to be zero, since the electron and the
nucleus do not interact at large distance. In order to remove an
electron from an atom, we have to raise the potential energy from
its negative value to zero. According to Coulomb's law, we
expect electrons closer to the nucleus to have a lower potential
energy and thus to require more energy to remove from the
atom.
We can directly measure how much energy is
required to remove an electron from an atom. Without concerning
ourselves with how this measurement is made, we simply measure the
minimum amount of energy required to carry out the following
"ionization reaction":
A
(g)
→
A
+
(g)
+
e
-
(g)
A
(g)
→
A
+
(g)
+
e
-
(g)
(2)Here, AA
is an atom in the gas phase, and
A
+
A
+
is
the same atom with one electron
e
-
e
-
removed and is thus an ion.
The minimum energy required to perform the ionization is called the
ionization energy. The values of the ionization energy
for each atom in Groups I through VIII of the periodic table are
shown as a function of the atomic number
here.
This figure is very reminiscent of the
Periodic Law, which states that chemical and physical properties of
the elements are periodic functions of the atomic number. Notice
that the elements with the largest ionization energies (in other
words, the most tightly bound electrons) are the inert gases. By
contrast, the alkali metals are the elements with the smallest
ionization energies. In a single period of the periodic table,
between each alkali metal atom and the next inert gas atom, the
ionization energy rises fairly steadily, falling dramatically from
the inert gas to the following alkali metal at the start of the
next period.
We need a model which accounts for these
variations in the ionization energy. A reasonable assumption from
Coulomb's law is that these variations are due to variations
in the nuclear charge (atomic number) and in the distance of the
electrons from the nucleus. To begin, we can make a very crude
approximation that the ionization energy is just the negative of
this attractive potential energy given by Coulomb's law. This
is crude because we have ignored the kinetic energy and because
each electron may not have fixed value of
rr.
Nevertheless, this approximation gives a way
to analyze this figure.
For example, from Coulomb's law it seems
to make sense that the ionization energy should increase with
increasing atomic number. It is easier to remove an electron from
Lithium than from Neon because the nuclear charge in Lithium is
much smaller than in Neon. But this cannot be the whole picture,
because this argument would imply that Sodium atoms should have
greater ionization energy than Neon atoms, when in fact Sodium
atoms have a very much lower ionization energy. Similarly, although
the ionization energy rises as we go from Sodium to Argon, the
ionization energy of Argon is still less than that of Neon, even
though the nuclear charge in an Argon atom is much greater than the
nuclear charge in a Neon atom. What have we omitted from our
analysis?
The answer is that we must consider also the
distance of the electrons from the nucleus. Since it requires much
less energy to ionize a Sodium atom than to ionize a Neon atom even
though Sodium's nuclear charge is greater, it must be that
the electron which we remove from a Sodium atom is much farther
from the nucleus than the electron in the Neon atom. We can make
the same comparison of the electrons removed during ionization of
Neon and Argon atoms: the Argon electron must be farther from the
nucleus than the Neon electron.
On the other hand, since the ionization energy
fairly smoothly increases as we move from Lithium to Neon in the
second period of elements, this reveals that the electrons are
increasingly attracted to the nucleus for greater nuclear charge
and suggests that the electrons' distance from the nucleus
might not be varying too greatly over the course of a single period
of the table.
If we follow this reasoning, we can even
estimate how far an electron might typically be from the nucleus by
using our crude approximation that the ionization energy is equal
to the negative of the Coulomb potential and solving for
rr for each
atom. This gives an estimate of distance of the electron from the
nucleus:
r
shell
=−((Z)e)(−e)ionization energy
r
shell
Z
e
e
ionization energy
(3)Values of
r
shell
r
shell
calculated in this way are
shown for the first 20 elements here. Also shown for
comparison is the ionization energy for these elements. Notice that
the approximate distance of the electrons from the nucleus
increases in steps exactly coinciding with the increases and dips
in the ionization energy.
Although these distances we have calculated do
not have a precise physical meaning, this
figure
suggests a significant
conclusion. The electrons in the elements are arranged into
"shells" of increasingly greater distance from the
nucleus. Hydrogen and Helium, with one and two electrons, have
ionization energies consistent with electrons at similar and close
distance from the nucleus. Then the second row elements lithium
through neon have virtually identical sizes, though larger than
that for the first two elements. The third row elements, sodium
argon, have an approximate electron-nuclear distance which
fluctuates a bit but is consistently larger than the second row
elements.
Because the sizes of the atoms appear to grow
in steps which correspond exactly to the periods of the Periodic
Table, it seems that the electrons in the atoms are grouped into
sets which are differing distances away from the nucleus. The first
two electrons, as in Helium, are close to the nucleus, whereas
additional electrons, as in Lithium to Neon, are farther from the
nucleus than the first two. The suggests that, for atoms Lithium to
Neon, the first two electrons are in an inner "shell",
and the remaining electrons are in an outer
"shell."
We can refine this shell model for the
electrons in an atom with further analysis of ionization energies.
We can remove any number of electrons in sequence, forming ions
with greater charge. We have been examining the first ionization
energy,
IE
1
IE
1
, but each successively removed electron has
successively greater ionization energy:
First ionization energy
IE
1
IE
1
:
A
(g)
→
A
+
(g)
+
e
-
(g)
A
(g)
→
A
+
(g)
+
e
-
(g)
(4)Second ionization energy
IE
2
IE
2
:
A
+
(g)
→
A
2+
(g)
+
e
-
(g)
A
+
(g)
→
A
2+
(g)
+
e
-
(g)
(5)Third ionization energy
IE
3
IE
3
:
A
2+
→
A
3+
(g)
+
e
-
(g)
A
2+
→
A
3+
(g)
+
e
-
(g)
(6)The sequential ionization energies for the
elements in the second row of the periodic table are shown
here.
Table 1: Successive Ionization Energies (kJ/mol)
| |
Na |
Mg |
Al |
Si |
P |
S |
Cl |
Ar |
|
IE
1
IE
1
|
496 |
738 |
578 |
787 |
1012 |
1000 |
1251 |
1520 |
|
IE
2
IE
2
|
4562 |
1451 |
1817 |
1577 |
1903 |
2251 |
2297 |
2665 |
|
IE
3
IE
3
|
6912 |
7733 |
2745 |
3231 |
2912 |
3361 |
3822 |
3931 |
|
IE
4
IE
4
|
9543 |
10540 |
11575 |
4356 |
4956 |
4564 |
5158 |
5770 |
|
IE
5
IE
5
|
13353 |
13630 |
14830 |
16091 |
6273 |
7013 |
6542 |
7238 |
|
IE
6
IE
6
|
16610 |
17995 |
18376 |
19784 |
22233 |
8495 |
9458 |
8781 |
|
IE
7
IE
7
|
20114 |
21703 |
23293 |
23783 |
25397 |
27106 |
11020 |
11995 |
Note that the second ionization energy is
always greater than the first, and the third is always greater than
the second, etc. This makes sense, since an electron should be more
strongly attracted to a positively charged atom than to a neutral
atom.
However, the data in the
table
show a surprising
feature. In most cases, the ionization energy increases a fairly
large amount for successive ionizations. But for each atom, there
is one much larger increase in ionization in the sequence. In Na
for example,
IE
2
IE
2
is nearly 10 times greater than
IE
1
IE
1
. Similarly,
IE
3
IE
3
is five times greater than
IE
2
IE
2
for Mg, although
IE
2
IE
2
is less
than twice
IE
1
IE
1
. The data for Na through S all show a single large
step in addition to the smaller increases in IE.
Looking closely and counting electrons, we see
that this unusually large increase always occurs for the ionization
where we have already removed all of the outer shell electrons and
are now removing an electron from the inner shell. This occurs
uniformly across the second row elements, indicating that our shell
model is in fact a very accurate predictor of the higher ionization
energies. We can now tell how many electrons there are in the outer
shell of each atom: it is equal to the number of electrons since
the last inert gas.
We can conclude that an inner shell is
"filled" once we have the number of electrons equal to
the number in an inert gas atom. The subsequent electrons are added
to a new outer shell. This is commonly referred to as the
valence shell of the atom.
However, we do not know why only a limited
number of electrons can reside in each shell. There is no obvious
reason at this point why all the electrons in an atom do not reside
in the shell closest to the nucleus. Similarly, there is no reason
given for why the number of electrons in an inert gas atom exactly
fills the outer shell, without room for even a single additional
electron. These questions must be addressed further.
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