Quantum
Numbers and Electron Configurations
Quantum
Numbers
The Bohr model was a one-dimensional model that used one
quantum number to describe the distribution of electrons in
the atom. The only information that was important was the size
of the orbit, which was described by the n quantum
number. Schrödinger's model allowed the electron to occupy
three-dimensional space. It therefore required three
coordinates, or three quantum numbers, to describe the
orbitals in which electrons can be found.
The three coordinates that come from Schrödinger's wave
equations are the principal (n), angular (l),
and magnetic (m) quantum numbers. These quantum
numbers describe the size, shape, and orientation in space of
the orbitals on an atom.
The principal quantum number (n) describes
the size of the orbital. Orbitals for which n = 2 are
larger than those for which n = 1, for example.
Because they have opposite electrical charges, electrons are
attracted to the nucleus of the atom. Energy must therefore
be absorbed to excite an electron from an orbital in which
the electron is close to the nucleus (n = 1) into an
orbital in which it is further from the nucleus (n =
2). The principal quantum number therefore indirectly
describes the energy of an orbital.
The angular quantum number (l) describes the
shape of the orbital. Orbitals have shapes that are best
described as spherical (l = 0), polar (l = 1),
or cloverleaf (l = 2). They can even take on more
complex shapes as the value of the angular quantum number
becomes larger.

There is only one way in which a sphere (l = 0) can
be oriented in space. Orbitals that have polar (l = 1)
or cloverleaf (l = 2) shapes, however, can point in
different directions. We therefore need a third quantum
number, known as the magnetic quantum number (m),
to describe the orientation in space of a particular orbital.
(It is called the magnetic quantum number because the
effect of different orientations of orbitals was first
observed in the presence of a magnetic field.)

Rules Governing the
Allowed Combinations of Quantum Numbers
- The three quantum numbers (n, l, and m)
that describe an orbital are integers: 0, 1, 2, 3,
and so on.
- The principal quantum number (n) cannot be
zero. The allowed values of n are therefore 1,
2, 3, 4, and so on.
- The angular quantum number (l) can be any
integer between 0 and n - 1. If n = 3,
for example, l can be either 0, 1, or 2.
- The magnetic quantum number (m)
can be any integer between -l and +l.
If l = 2, m can be either -2, -1, 0,
+1, or +2.

Shells and
Subshells of Orbitals
Orbitals that have the same value of the principal quantum
number form a shell. Orbitals within a shell are
divided into subshells that have the same value of the
angular quantum number. Chemists describe the shell and
subshell in which an orbital belongs with a two-character
code such as 2p or 4f. The first character
indicates the shell (n = 2 or n = 4). The
second character identifies the subshell. By convention, the
following lowercase letters are used to indicate different
subshells.
s: |
|
l = 0 |
p: |
|
l = 1 |
d: |
|
l = 2 |
f: |
|
l = 3 |
Although there is no pattern in the first
four letters (s, p, d, f), the
letters progress alphabetically from that point (g, h,
and so on). Some of the allowed combinations of the n
and l quantum numbers are shown in the figure below.

The third rule limiting allowed combinations of the n,
l, and m quantum numbers has an important
consequence. It forces the number of subshells in a shell to
be equal to the principal quantum number for the shell. The n
= 3 shell, for example, contains three subshells: the 3s,
3p, and 3d orbitals.

Possible
Combinations of Quantum Numbers
There is only one orbital in the n = 1 shell
because there is only one way in which a sphere can be
oriented in space. The only allowed combination of quantum
numbers for which n = 1 is the following.
There are four orbitals in the n = 2
shell.
2 |
|
1 |
|
-1 |
|
|
2 |
|
1 |
|
0 |
2p |
2 |
|
1 |
|
1 |
|
There is only one orbital in the 2s
subshell. But, there are three orbitals in the 2p
subshell because there are three directions in which a p
orbital can point. One of these orbitals is oriented along
the X axis, another along the Y axis, and the
third along the Z axis of a coordinate system, as
shown in the figure below. These orbitals are therefore known
as the 2px, 2py,
and 2pz orbitals.

There are nine orbitals in the n = 3 shell.
n |
|
l |
|
m |
|
|
3 |
|
0 |
|
0 |
|
3s |
|
|
|
|
|
|
|
3 |
|
1 |
|
-1 |
 |
|
3 |
|
1 |
|
0 |
3p |
3 |
|
1 |
|
1 |
|
|
|
|
|
|
|
|
3 |
|
2 |
|
-2 |
 |
|
3 |
|
2 |
|
-1 |
3d |
3 |
|
2 |
|
0 |
3 |
|
2 |
|
1 |
3 |
|
2 |
|
2 |
|
There is one orbital in the 3s
subshell and three orbitals in the 3p subshell. The n
= 3 shell, however, also includes 3d orbitals.
The five different orientations of orbitals in the 3d
subshell are shown in the figure below. One of these orbitals
lies in the XY plane of an XYZ coordinate
system and is called the 3dxy orbital. The
3dxz and 3dyz orbitals
have the same shape, but they lie between the axes of the
coordinate system in the XZ and YZ planes. The
fourth orbital in this subshell lies along the X and Y
axes and is called the 3dx2-y2
orbital. Most of the space occupied by the fifth orbital lies
along the Z axis and this orbital is called the 3dz2
orbital.

The number of orbitals in a shell is the square of the
principal quantum number: 12 = 1, 22 =
4, 32 = 9. There is one orbital in an s
subshell (l = 0), three orbitals in a p
subshell (l = 1), and five orbitals in a d
subshell (l = 2). The number of orbitals in a subshell
is therefore 2(l) + 1.
Before we can use these orbitals we need to know the
number of electrons that can occupy an orbital and how they
can be distinguished from one another. Experimental evidence
suggests that an orbital can hold no more than two electrons.
To distinguish between the two electrons in an orbital, we
need a fourth quantum number. This is called the spin
quantum number (s) because electrons behave as if
they were spinning in either a clockwise or counterclockwise
fashion. One of the electrons in an orbital is arbitrarily
assigned an s quantum number of +1/2, the other is
assigned an s quantum number of -1/2. Thus, it takes
three quantum numbers to define an orbital but four quantum
numbers to identify one of the electrons that can occupy the
orbital.
The allowed combinations of n, l, and m
quantum numbers for the first four shells are given in the
table below. For each of these orbitals, there are two
allowed values of the spin quantum number, s.

Summary of Allowed
Combinations of Quantum Numbers
n |
|
|
l |
|
|
|
m |
Subshell Notation |
Number of Orbitals
in the Subshell |
Number of
Electrons Needed to Fill Subshell |
Total Number of
Electrons in Subshell |
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1 |
|
|
0 |
|
|
|
0 |
1s |
1 |
2 |
2 |
ŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻ |
2 |
|
|
0 |
|
|
|
0 |
2s |
1 |
2 |
|
2 |
|
|
1 |
|
|
|
1,0,-1 |
2p |
3 |
6 |
8 |
ŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻ |
3 |
|
|
0 |
|
|
|
0 |
3s |
1 |
2 |
|
3 |
|
|
1 |
|
|
|
1,0,-1 |
3p |
3 |
6 |
|
3 |
|
|
2 |
|
|
|
2,1,0,-1,-2 |
3d |
5 |
10 |
18 |
ŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻŻ |
4 |
|
|
0 |
|
|
|
0 |
4s |
1 |
2 |
|
4 |
|
|
1 |
|
|
|
1,0,-1 |
4p |
3 |
6 |
|
4 |
|
|
2 |
|
|
|
2,1,0,-1,-2 |
4d |
5 |
10 |
|
4 |
|
|
3 |
|
|
|
3,2,1,0,-1,-2,-3 |
4f |
7 |
14 |
32 |

The Relative
Energies of Atomic Orbitals
Because of the force of attraction between objects of
opposite charge, the most important factor influencing the
energy of an orbital is its size and therefore the value of
the principal quantum number, n. For an atom that
contains only one electron, there is no difference between
the energies of the different subshells within a shell. The 3s,
3p, and 3d orbitals, for example, have the same
energy in a hydrogen atom. The Bohr model, which specified
the energies of orbits in terms of nothing more than the
distance between the electron and the nucleus, therefore
works for this atom.
The hydrogen atom is unusual, however. As soon as an atom
contains more than one electron, the different subshells no
longer have the same energy. Within a given shell, the s
orbitals always have the lowest energy. The energy of the
subshells gradually becomes larger as the value of the
angular quantum number becomes larger.
Relative energies: s
< p < d < f
As a result, two factors control the
energy of an orbital for most atoms: the size of the orbital
and its shape, as shown in the figure below.

A very simple device can be
constructed to estimate the relative energies of atomic
orbitals. The allowed combinations of the n and l
quantum numbers are organized in a table, as shown in the
figure below and arrows are drawn at 45 degree angles
pointing toward the bottom left corner of the table.

The order of increasing energy of the orbitals is then
read off by following these arrows, starting at the top of
the first line and then proceeding on to the second, third,
fourth lines, and so on. This diagram predicts the following
order of increasing energy for atomic orbitals.
1s < 2s < 2p
< 3s < 3p <4s < 3d
<4p < 5s < 4d < 5p
< 6s < 4f < 5d < 6p
< 7s < 5f < 6d < 7p
< 8s ...

Electron
Configurations, the Aufbau Principle, Degenerate Orbitals,
and Hund's Rule
The electron configuration of an atom describes the
orbitals occupied by electrons on the atom. The basis of this
prediction is a rule known as the aufbau principle,
which assumes that electrons are added to an atom, one at a
time, starting with the lowest energy orbital, until all of
the electrons have been placed in an appropriate orbital.
A hydrogen atom (Z = 1) has only one electron,
which goes into the lowest energy orbital, the 1s
orbital. This is indicated by writing a superscript
"1" after the symbol for the orbital.
H (Z = 1): 1s1
The next element has two electrons and the second electron
fills the 1s orbital because there are only two
possible values for the spin quantum number used to
distinguish between the electrons in an orbital.
He (Z = 2): 1s2
The third electron goes into the next orbital in the
energy diagram, the 2s orbital.
Li (Z = 3): 1s2 2s1
The fourth electron fills this orbital.
Be (Z = 4): 1s2 2s2
After the 1s and 2s orbitals have been
filled, the next lowest energy orbitals are the three 2p
orbitals. The fifth electron therefore goes into one of these
orbitals.
B (Z = 5): 1s2 2s2
2p1
When the time comes to add a sixth electron, the electron
configuration is obvious.
C (Z = 6): 1s2 2s2
2p2
However, there are three orbitals in the 2p
subshell. Does the second electron go into the same orbital
as the first, or does it go into one of the other orbitals in
this subshell?
To answer this, we need to understand the concept of degenerate
orbitals. By definition, orbitals are degenerate
when they have the same energy. The energy of an orbital
depends on both its size and its shape because the electron
spends more of its time further from the nucleus of the atom
as the orbital becomes larger or the shape becomes more
complex. In an isolated atom, however, the energy of an
orbital doesn't depend on the direction in which it points in
space. Orbitals that differ only in their orientation in
space, such as the 2px, 2py,
and 2pz orbitals, are therefore
degenerate.
Electrons fill degenerate orbitals according to rules
first stated by Friedrich Hund. Hund's rules can be
summarized as follows.
- One electron is added to each of the degenerate
orbitals in a subshell before two electrons are added
to any orbital in the subshell.
- Electrons are added to a subshell with the same value
of the spin quantum number until each orbital in the
subshell has at least one electron.
When the time comes to place two electrons into the 2p
subshell we put one electron into each of two of these
orbitals. (The choice between the 2px,
2py, and 2pz
orbitals is purely arbitrary.)
C (Z = 6): 1s2 2s2
2px1
2py1
The fact that both of the electrons in the 2p
subshell have the same spin quantum number can be shown by
representing an electron for which s = +1/2 with an
arrow pointing up and an electron for which s =
-1/2 with an arrow pointing down.
The electrons in the 2p orbitals on carbon can
therefore be represented as follows.

When we get to N (Z = 7), we have to put one
electron into each of the three degenerate 2p
orbitals.
N (Z = 7): |
|
1s2 2s2 2p3
|
|
 |
Because each orbital in this subshell now
contains one electron, the next electron added to the
subshell must have the opposite spin quantum number, thereby
filling one of the 2p orbitals.
O (Z = 8): |
|
1s2 2s2 2p4
|
|
 |
The ninth electron fills a second orbital
in this subshell.
F (Z = 9): |
|
1s2 2s2 2p5
|
|
 |
The tenth electron completes the 2p
subshell.
Ne (Z = 10): |
|
1s2 2s2 2p6
|
|
 |
There is something unusually stable about
atoms, such as He and Ne, that have electron configurations
with filled shells of orbitals. By convention, we therefore
write abbreviated electron configurations in terms of the
number of electrons beyond the previous element with a
filled-shell electron configuration. Electron configurations
of the next two elements in the periodic table, for example,
could be written as follows.
Na (Z = 11):
[Ne] 3s1
Mg (Z = 12): [Ne] 3s2
The aufbau process can be used to predict
the electron configuration for an element. The actual
configuration used by the element has to be determined
experimentally. The experimentally determined electron
configurations for the elements in the first four rows of the
periodic table are given in the table in the following
section.

The Electron
Configurations of the Elements
(1st, 2nd, 3rd, and 4th Row Elements)
Atomic Number |
|
Symbol |
|
Electron Configuration |
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1 |
|
H |
|
1s1 |
2 |
|
He |
|
1s2 = [He] |
3 |
|
Li |
|
[He] 2s1 |
4 |
|
Be |
|
[He] 2s2 |
5 |
|
B |
|
[He] 2s2 2p1 |
6 |
|
C |
|
[He] 2s2 2p2 |
7 |
|
N |
|
[He] 2s2 2p3 |
8 |
|
O |
|
[He] 2s2 2p4 |
9 |
|
F |
|
[He] 2s2 2p5 |
10 |
|
Ne |
|
[He] 2s2 2p6
= [Ne] |
11 |
|
Na |
|
[Ne] 3s1 |
12 |
|
Mg |
|
[Ne] 3s2 |
13 |
|
Al |
|
[Ne] 3s2 3p1 |
14 |
|
Si |
|
[Ne] 3s2 3p2 |
15 |
|
P |
|
[Ne] 3s2 3p3 |
16 |
|
S |
|
[Ne] 3s2 3p4 |
17 |
|
Cl |
|
[Ne] 3s2 3p5 |
18 |
|
Ar |
|
[Ne] 3s2 3p6
= [Ar] |
19 |
|
K |
|
[Ar] 4s1 |
20 |
|
Ca |
|
[Ar] 4s2 |
21 |
|
Sc |
|
[Ar] 4s2 3d1 |
22 |
|
Ti |
|
[Ar] 4s2 3d2 |
23 |
|
V |
|
[Ar] 4s2 3d3 |
24 |
|
Cr |
|
[Ar] 4s1 3d5 |
25 |
|
Mn |
|
[Ar] 4s2 3d5 |
26 |
|
Fe |
|
[Ar] 4s2 3d6 |
27 |
|
Co |
|
[Ar] 4s2 3d7 |
28 |
|
Ni |
|
[Ar] 4s2 3d8 |
29 |
|
Cu |
|
[Ar] 4s1 3d10 |
30 |
|
Zn |
|
[Ar] 4s2 3d10 |
31 |
|
Ga |
|
[Ar] 4s2 3d10
4p1 |
32 |
|
Ge |
|
[Ar] 4s2 3d10
4p2 |
33 |
|
As |
|
[Ar] 4s2 3d10
4p3 |
34 |
|
Se |
|
[Ar] 4s2 3d10
4p4 |
35 |
|
Br |
|
[Ar] 4s2 3d10
4p5 |
36 |
|
Kr |
|
[Ar] 4s2 3d10
4p6 = [Kr] |

Exceptions to
Predicted Electron Configurations
There are several patterns in the electron configurations
listed in the table in the previous section. One of the most
striking is the remarkable level of agreement between these
configurations and the configurations we would predict. There
are only two exceptions among the first 40 elements: chromium
and copper.
Strict adherence to the rules of the aufbau process would
predict the following electron configurations for chromium
and copper.
predicted electron configurations: |
|
Cr (Z = 24): [Ar] 4s2 3d4
|
|
|
Cu (Z = 29): [Ar] 4s2 3d9
|
The experimentally determined electron
configurations for these elements are slightly different.
actual electron configurations: |
|
Cr (Z = 24): [Ar] 4s1 3d5
|
|
|
Cu (Z = 29): [Ar] 4s1 3d10
|
In each case, one electron has been
transferred from the 4s orbital to a 3d
orbital, even though the 3d orbitals are supposed to
be at a higher level than the 4s orbital.
Once we get beyond atomic number 40, the difference
between the energies of adjacent orbitals is small enough
that it becomes much easier to transfer an electron from one
orbital to another. Most of the exceptions to the electron
configuration predicted from the aufbau
diagram shown earlier therefore occur among elements with
atomic numbers larger than 40. Although it is tempting to
focus attention on the handful of elements that have electron
configurations that differ from those predicted with the
aufbau diagram, the amazing thing is that this simple diagram
works for so many elements.

Electron
Configurations and the Periodic Table
When electron configuration data are arranged so that we
can compare elements in one of the horizontal rows of the
periodic table, we find that these rows typically correspond
to the filling of a shell of orbitals. The second row, for
example, contains elements in which the orbitals in the n
= 2 shell are filled.
Li (Z = 3): |
|
[He] 2s1 |
Be (Z = 4): |
|
[He] 2s2 |
B (Z = 5): |
|
[He] 2s2 2p1 |
C (Z = 6): |
|
[He] 2s2 2p2 |
N (Z = 7): |
|
[He] 2s2 2p3 |
O (Z = 8): |
|
[He] 2s2 2p4 |
F (Z = 9): |
|
[He] 2s2 2p5 |
Ne (Z = 10): |
|
[He] 2s2 2p6 |
There is an obvious pattern within the
vertical columns, or groups, of the periodic table as well.
The elements in a group have similar configurations for their
outermost electrons. This relationship can be seen by looking
at the electron configurations of elements in columns on
either side of the periodic table.
Group IA |
|
|
|
Group VIIA |
|
|
H |
|
1s1 |
|
|
|
|
Li |
|
[He] 2s1 |
|
F |
|
[He] 2s2 2p5 |
Na |
|
[Ne] 3s1 |
|
Cl |
|
[Ne] 3s2 3p5 |
K |
|
[Ar] 4s1 |
|
Br |
|
[Ar] 4s2 3d10
4p5 |
Rb |
|
[Kr] 5s1 |
|
I |
|
[Kr] 5s2 4d10
5p5 |
Cs |
|
[Xe] 6s1 |
|
At |
|
[Xe] 6s2 4f14
5d10 6p5 |
The figure below shows the relationship
between the periodic table and the orbitals being filled
during the aufbau process. The two columns on the left side
of the periodic table correspond to the filling of an s
orbital. The next 10 columns include elements in which the
five orbitals in a d subshell are filled. The six
columns on the right represent the filling of the three
orbitals in a p subshell. Finally, the 14 columns at
the bottom of the table correspond to the filling of the
seven orbitals in an f subshell.


