Our Lewis model of bonding, as currently
developed, incorporates two extreme views of the distribution of
electrons in a bond. In a covalent bond, we have assumed up to this
point that the electron pair is shared perfectly. In complete
contrast, in ionic bonding we have assumed that the electrons are
not shared at all. Rather, one of the atoms is assumed to entirely
extract one or more electrons from the other. We might expect that
a more accurate description of the reality of chemical bonds falls
in general somewhere between these two extremes. To observe this
intermediate behavior, we can examine molecular dipole
moments.
An electric dipole is a spatial separation of
positive and negative charges. In the simplest case, a positive
charge
QQ
and a negative charge
−QQ
separated by a distance
RR produce a
measurable dipole moment,
μμ
equal to
Q×R×QR.
An electric field can interact with an electric dipole and can even
orient the dipole in the direction of the field.
We might initially expect that molecules do
not in general have dipole moments. Each atom entering into a
chemical bond is electrically neutral, with equal numbers of
positive and negative charges. Consequently, a molecule formed from
neutral atoms must also be electrically neutral. Although electron
pairs are shared between bonded nuclei, this does not affect the
total number of negative charges. We might from these simple
statements that molecules would be unaffected by electric or
magnetic fields, each molecule behaving as a single uncharged
particle.
This prediction is incorrect, however. To
illustrate, a stream of water can be deflected by an electrically
charged object near the stream, indicating that individual water
molecules exhibit a dipole moment. A water molecule is rather more
complicated than a simple separation of a positive and negative
charges, however. Recall though that a water molecule has equal
total numbers of positive and negative charges, consisting of three
positively charged nuclei surrounded by ten electrons.
Nevertheless, measurements reveal that water has a dipole moment of
6.17×10-30(Cm)=1.85debye6.17-30Cm1.85debye.
(The debye is a unit used to measure dipole moments:
1debye=3.33
×10-30(Cm)1debye3.33
-30Cm.)
Water is not unique: the molecules of most substances have dipole
moments. A sampling of molecules and their dipole moments is given
in Table 2.
Table 2: Dipole Moments of Specific Molecules
| |
μ (debye) |
| H2OH2O |
1.85 |
| HFHF |
1.91 |
| HClHCl |
1.08 |
| HBrHBr |
0.80 |
| HIHI |
0.42 |
| COCO |
0.12 |
| CO2CO2 |
0 |
| NH3NH3 |
1.47 |
| PH3PH3 |
0.58 |
| AsH3AsH3 |
0.20 |
| CH4CH4 |
0 |
| NaClNaCl |
9.00 |
Focusing again on the water molecule, how can
we account for the existence of a dipole moment in a neutral
molecule? The existence of the dipole moment reveals that a water
molecule must have an internal separation of positive partial
charge
δδ
and negative partial charge
−δδ.
Thus, it must be true that the electrons in the covalent bond
between hydrogen and oxygen are not
equally shared. Rather, the shared
electrons must spend more time in the vicinity of one nucleus than
the other. The molecule thus has one region where, on average,
there is a net surplus of negative charge and one region where, on
average, there is a compensating surplus of positive charge, thus
producing a molecular dipole. Additional observations reveal that
the oxygen "end" of the molecule holds the partial negative charge.
Hence, the covalently shared electrons spend more time near the
oxygen atom than near the hydrogen atoms. We conclude that oxygen
atoms have a greater ability to attract the shared electrons in the
bond than do hydrogen atoms.
We should not be surprised by the fact that
individual atoms of different elements have differing abilities to
attract electrons to themselves. We have previously seen that
different atoms have greatly varying ionization energies,
representing great variation in the extent to which atoms cling to
their electrons. We have also seen great variation in the electron
affinities of atoms, representing variation in the extent to which
atoms attract an added electron. We now define the
electronegativity of an atom as the
ability of the atom to attract electrons in a chemical bond. This
is different than either ionization energy or electron affinity,
because electronegativity is the attraction of electrons
in a chemical bond, whereas
ionization energy and electron affinity refer to removal and
attachment of electrons in free atoms. However, we can expect
electronegativity to be correlated with electron affinity and
ionization energy. In particular, the electronegativity of an atom
arises from a combination of properties of the atom, including the
size of the atom, the charge on the nucleus, the number of
electrons about the nuclei, and the number of electrons in the
valence shell.
Because electronegativity is an abstractly
defined property, it cannot be directly measured. In fact, there
are many definitions of electronegativity, resulting in many
different scales of electronegativities. However, relative
electronegativities can be observed indirectly by measuring
molecular dipole moments: in general, the greater the dipole
moment, the greater the separation of charges must be, and
therefore, the less equal the sharing of the bonding electrons must
be.
With this in mind, we refer back to the
dipoles given in Table 2. There
are several important trends in these data. Note that each hydrogen
halide
(HFHF,
HClHCl,
HBrHBr,
and
HIHI)
has a significant dipole moment. Moreover, the dipole moments
increase as we move up the
periodic table in the halogen group. We can conclude that fluorine
atoms have a greater electronegativity than do chlorine atoms,
etc. Note also that
HFHF
has a greater dipole moment than
H2OH2O,
which is in turn greater than that of
NH3NH3.
We can conclude that electronegativity increases as we move
across the periodic table from
left to right in a single period. These trends hold generally in
comparisons of the electronegativities of the individual elements.
One set of relative electronegativities of atoms in the first three
rows of the periodic table is given in Table 3.
Table 3: Electronegativities of Selected Atoms
| |
χ |
| H |
2.1 |
| He |
- |
| Li |
1.0 |
| Be |
1.5 |
| B |
2.0 |
| C |
2.5 |
| N |
3.0 |
| O |
3.5 |
| F |
4.0 |
| Ne |
- |
| Na |
0.9 |
| Mg |
1.2 |
| Al |
1.5 |
| Si |
1.8 |
| P |
2.1 |
| S |
2.5 |
| Cl |
3.0 |
| Ar |
- |
| K |
0.8 |
| Ca |
1.0 |
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