1.8: Electron Configurations
-
- Last updated
- Save as PDF
Learning Objectives
- To understand the basics of adding electrons to atomic orbitals
- To understand the basics of the Aufbau principle
The electron configuration of an element is the arrangement of its electrons in its atomic orbitals. By knowing the electron configuration of an element, we can predict and explain a great deal of its chemistry.
The Aufbau Principle
We construct the periodic table by following the aufbau principle (from German, meaning “building up”). First we determine the number of electrons in the atom; then we add electrons one at a time to the lowest-energy orbital available without violating the Pauli principle . We use the orbital energy diagram of Figure \(\PageIndex{1}\), recognizing that each orbital can hold two electrons, one with spin up ↑, corresponding to m s = +½, which is arbitrarily written first, and one with spin down ↓, corresponding to m s = −½. A filled orbital is indicated by ↑↓, in which the electron spins are said to be paired . Here is a schematic orbital diagram for a hydrogen atom in its ground state:
From the orbital diagram, we can write the electron configuration in an abbreviated form in which the occupied orbitals are identified by their principal quantum number n and their value of l ( s , p , d , or f ), with the number of electrons in the subshell indicated by a superscript. For hydrogen, therefore, the single electron is placed in the 1 s orbital, which is the orbital lowest in energy (Figure \(\PageIndex{1}\)), and the electron configuration is written as 1 s 1 and read as “one-s-one.”
A neutral helium atom, with an atomic number of 2 ( Z = 2), has two electrons. We place one electron in the orbital that is lowest in energy, the 1 s orbital. From the Pauli exclusion principle , we know that an orbital can contain two electrons with opposite spin, so we place the second electron in the same orbital as the first but pointing down, so that the electrons are paired. The orbital diagram for the helium atom is therefore
written as 1 s 2 , where the superscript 2 implies the pairing of spins. Otherwise, our configuration would violate the Pauli principle.
The next element is lithium, with Z = 3 and three electrons in the neutral atom. We know that the 1 s orbital can hold two of the electrons with their spins paired; the third electron must enter a higher energy orbital. Figure 6.29 tells us that the next lowest energy orbital is 2 s , so the orbital diagram for lithium is
This electron configuration is written as 1 s 2 2 s 1 .
The next element is beryllium, with Z = 4 and four electrons. We fill both the 1 s and 2 s orbitals to achieve a 1 s 2 2 s 2 electron configuration:
When we reach boron, with Z = 5 and five electrons, we must place the fifth electron in one of the 2 p orbitals. Because all three 2 p orbitals are degenerate, it doesn’t matter which one we select. The electron configuration of boron is 1 s 2 2 s 2 2 p 1 :
At carbon, with Z = 6 and six electrons, we are faced with a choice. Should the sixth electron be placed in the same 2 p orbital that already has an electron, or should it go in one of the empty 2 p orbitals? If it goes in an empty 2 p orbital, will the sixth electron have its spin aligned with or be opposite to the spin of the fifth? In short, which of the following three orbital diagrams is correct for carbon, remembering that the 2 p orbitals are degenerate?
Because of electron-electron interactions, it is more favorable energetically for an electron to be in an unoccupied orbital than in one that is already occupied; hence we can eliminate choice a. Similarly, experiments have shown that choice b is slightly higher in energy (less stable) than choice c because electrons in degenerate orbitals prefer to line up with their spins parallel; thus, we can eliminate choice b. Choice c illustrates Hund’s rule (named after the German physicist Friedrich H. Hund, 1896–1997), which today says that the lowest-energy electron configuration for an atom is the one that has the maximum number of electrons with parallel spins in degenerate orbitals. By Hund’s rule, the electron configuration of carbon, which is 1 s 2 2 s 2 2 p 2 , is understood to correspond to the orbital diagram shown in c. Experimentally, it is found that the ground state of a neutral carbon atom does indeed contain two unpaired electrons.
When we get to nitrogen ( Z = 7, with seven electrons), Hund’s rule tells us that the lowest-energy arrangement is
with three unpaired electrons. The electron configuration of nitrogen is thus 1 s 2 2 s 2 2 p 3 .
At oxygen, with Z = 8 and eight electrons, we have no choice. One electron must be paired with another in one of the 2 p orbitals, which gives us two unpaired electrons and a 1 s 2 2 s 2 2 p 4 electron configuration. Because all the 2 p orbitals are degenerate, it doesn’t matter which one has the pair of electrons.
Similarly, fluorine has the electron configuration 1 s 2 2 s 2 2 p 5 :
When we reach neon, with Z = 10, we have filled the 2 p subshell, giving a 1 s 2 2 s 2 2 p 6 electron configuration:
Notice that for neon, as for helium, all the orbitals through the 2 p level are completely filled. This fact is very important in dictating both the chemical reactivity and the bonding of helium and neon, as you will see.
Electron Configuration of Atoms: Electron Configuration of Atoms, YouTube(opens in new window) [youtu.be]
Valence Electrons
As we continue through the periodic table in this way, writing the electron configurations of larger and larger atoms, it becomes tedious to keep copying the configurations of the filled inner subshells. In practice, chemists simplify the notation by using a bracketed noble gas symbol to represent the configuration of the noble gas from the preceding row because all the orbitals in a noble gas are filled. For example, [Ne] represents the 1 s 2 2 s 2 2 p 6 electron configuration of neon ( Z = 10), so the electron configuration of sodium, with Z = 11, which is 1 s 2 2 s 2 2 p 6 3 s 1 , is written as [Ne]3 s 1 :
| Neon | Z = 10 | 1 s 2 2 s 2 2 p 6 |
|---|---|---|
| Sodium | Z = 11 | 1 s 2 2 s 2 2 p 6 3 s 1 = [Ne] 3 s 1 |
Because electrons in filled inner orbitals are closer to the nucleus and more tightly bound to it, they are rarely involved in chemical reactions. This means that the chemistry of an atom depends mostly on the electrons in its outermost shell, which are called the valence electrons . The simplified notation allows us to see the valence-electron configuration more easily. Using this notation to compare the electron configurations of sodium and lithium, we have:
| Sodium | 1 s 2 2 s 2 2 p 6 3 s 1 = [Ne]3 s 1 |
|---|---|
| Lithium | 1 s 2 2 s 1 = [He]2 s 1 |
It is readily apparent that both sodium and lithium have one s electron in their valence shell. We would therefore predict that sodium and lithium have very similar chemistry, which is indeed the case.
As we continue to build the eight elements of period 3, the 3 s and 3 p orbitals are filled, one electron at a time. This row concludes with the noble gas argon, which has the electron configuration [Ne]3 s 2 3 p 6 , corresponding to a filled valence shell.
Example \(\PageIndex{1}\): Electronic Configuration of Phosphorus
Draw an orbital diagram and use it to derive the electron configuration of phosphorus, Z = 15. What is its valence electron configuration?
Given: atomic number
Asked for: orbital diagram and valence electron configuration for phosphorus
Strategy:
- Locate the nearest noble gas preceding phosphorus in the periodic table. Then subtract its number of electrons from those in phosphorus to obtain the number of valence electrons in phosphorus.
- Referring to Figure \(\PageIndex{1}\), draw an orbital diagram to represent those valence orbitals. Following Hund’s rule, place the valence electrons in the available orbitals, beginning with the orbital that is lowest in energy. Write the electron configuration from your orbital diagram.
- Ignore the inner orbitals (those that correspond to the electron configuration of the nearest noble gas) and write the valence electron configuration for phosphorus.
Solution:
A Because phosphorus is in the third row of the periodic table, we know that it has a [Ne] closed shell with 10 electrons. We begin by subtracting 10 electrons from the 15 in phosphorus.
B The additional five electrons are placed in the next available orbitals, which Figure \(\PageIndex{1}\) tells us are the 3 s and 3 p orbitals:
Because the 3 s orbital is lower in energy than the 3 p orbitals, we fill it first:
Hund’s rule tells us that the remaining three electrons will occupy the degenerate 3 p orbitals separately but with their spins aligned:
The electron configuration is [Ne]3 s 2 3 p 3 .
C We obtain the valence electron configuration by ignoring the inner orbitals, which for phosphorus means that we ignore the [Ne] closed shell. This gives a valence-electron configuration of 3 s 2 3 p 3 .
Exercise \(\PageIndex{1}\)
Draw an orbital diagram and use it to derive the electron configuration of chlorine, Z = 17. What is its valence electron configuration?
- Answer
-
[Ne]3 s 2 3 p 5 ; 3 s 2 3 p 5
Definition of Valence Electrons: Definition of Valence Electrons, YouTube(opens in new window) [youtu.be]
The general order in which orbitals are filled is depicted in Figure \(\PageIndex{2}\). Subshells corresponding to each value of n are written from left to right on successive horizontal lines, where each row represents a row in the periodic table. The order in which the orbitals are filled is indicated by the diagonal lines running from the upper right to the lower left. Accordingly, the 4 s orbital is filled prior to the 3 d orbital because of shielding and penetration effects. Consequently, the electron configuration of potassium, which begins the fourth period, is [Ar]4 s 1 , and the configuration of calcium is [Ar]4 s 2 . Five 3 d orbitals are filled by the next 10 elements, the transition metals, followed by three 4 p orbitals. Notice that the last member of this row is the noble gas krypton ( Z = 36), [Ar]4 s 2 3 d 10 4 p 6 = [Kr], which has filled 4 s , 3 d , and 4 p orbitals. The fifth row of the periodic table is essentially the same as the fourth, except that the 5 s , 4 d , and 5 p orbitals are filled sequentially.
The sixth row of the periodic table will be different from the preceding two because the 4 f orbitals, which can hold 14 electrons, are filled between the 6 s and the 5 d orbitals. The elements that contain 4 f orbitals in their valence shell are the lanthanides. When the 6 p orbitals are finally filled, we have reached the next noble gas, radon ( Z = 86), [Xe]6 s 2 4 f 14 5 d 10 6 p 6 = [Rn]. In the last row, the 5 f orbitals are filled between the 7 s and the 6 d orbitals, which gives the 14 actinide elements. Because the large number of protons makes their nuclei unstable, all the actinides are radioactive.
Example \(\PageIndex{2}\): Electron Configuration of Mercury
Write the electron configuration of mercury ( Z = 80), showing all the inner orbitals.
Given: atomic number
Asked for: complete electron configuration
Strategy:
Using the orbital diagram in Figure \(\PageIndex{1}\) and the periodic table as a guide, fill the orbitals until all 80 electrons have been placed.
Solution:
By placing the electrons in orbitals following the order shown in Figure \(\PageIndex{2}\) and using the periodic table as a guide, we obtain
| 1 s 2 | row 1 | 2 electrons |
|---|---|---|
| 2 s 2 2 p 6 | row 2 | 8 electrons |
| 3 s 2 3 p 6 | row 3 | 8 electrons |
| 4 s 2 3 d 10 4 p 6 | row 4 | 18 electrons |
| 5 s 2 4 d 10 5 p 6 | row 5 | 18 electrons |
| row 1–5 | 54 electrons |
After filling the first five rows, we still have 80 − 54 = 26 more electrons to accommodate. According to Figure \(\PageIndex{2}\), we need to fill the 6 s (2 electrons), 4 f (14 electrons), and 5 d (10 electrons) orbitals. The result is mercury’s electron configuration:
1 s 2 2 s 2 2 p 6 3 s 2 3 p 6 4 s 2 3 d 10 4 p 6 5 s 2 4 d 10 5 p 6 6 s 2 4 f 14 5 d 10 = Hg = [Xe]6 s 2 4 f 14 5 d 10
with a filled 5 d subshell, a 6 s 2 4 f 14 5 d 10 valence shell configuration, and a total of 80 electrons. (You should always check to be sure that the total number of electrons equals the atomic number.)
Exercise \(\PageIndex{2}\): Electron Configuration of Flerovium
Although element 114 is not stable enough to occur in nature, atoms of element 114 were created for the first time in a nuclear reactor in 1998 by a team of Russian and American scientists. The element is named after the Flerov Laboratory of Nuclear Reactions of the Joint Institute for Nuclear Research in Dubna, Russia, where the element was discovered. The name of the laboratory, in turn, honors the Russian physicist Georgy Flyorov. Write the complete electron configuration for element 114.
- Answer
-
s 2 2 s 2 2 p 6 3 s 2 3 p 6 4 s 2 3 d 10 4 p 6 5 s 2 4 d 10 5 p 6 6 s 2 4 f 14 5 d 10 6 p 6 7 s 2 5 f 14 6 d 10 7 p 2
The electron configurations of the elements are presented in Figure \(\PageIndex{2}\), which lists the orbitals in the order in which they are filled. In several cases, the ground state electron configurations are different from those predicted by Figure \(\PageIndex{1}\). Some of these anomalies occur as the 3 d orbitals are filled. For example, the observed ground state electron configuration of chromium is [Ar]4 s 1 3 d 5 rather than the predicted [Ar]4 s 2 3 d 4 . Similarly, the observed electron configuration of copper is [Ar]4 s 1 3 d 10 instead of [Ar] s 2 3 d 9 . The actual electron configuration may be rationalized in terms of an added stability associated with a half-filled ( ns 1 , np 3 , nd 5 , nf 7 ) or filled ( ns 2 , np 6 , nd 10 , nf 14 ) subshell. (In fact, this "special stability" is really another consequence of the instability caused by pairing an electron with another in the same orbital, as illustrated by Hund's rule.) Given the small differences between higher energy levels, this added stability is enough to shift an electron from one orbital to another. In heavier elements, other more complex effects can also be important, leading to many additional anomalies. For example, cerium has an electron configuration of [Xe]6 s 2 4 f 1 5 d 1 , which is impossible to rationalize in simple terms. In most cases, however, these apparent anomalies do not have important chemical consequences.
Additional stability is associated with half-filled or filled subshells.
Electron Configuration of Transition Metals: Electron Configuration of Transition Metals, YouTube(opens in new window) [youtu.be]
Summary
Based on the Pauli principle and a knowledge of orbital energies obtained using hydrogen-like orbitals, it is possible to construct the periodic table by filling up the available orbitals beginning with the lowest-energy orbitals (the aufbau principle ), which gives rise to a particular arrangement of electrons for each element (its electron configuration ). Hund’s rule says that the lowest-energy arrangement of electrons is the one that places them in degenerate orbitals with their spins parallel. For chemical purposes, the most important electrons are those in the outermost principal shell, the valence electrons .