Ionisation Energy Trends (Cambridge (CIE) AS Chemistry)
Revision Note
Trends in Ionisation Energy
Ionisation energies show periodicity - a trend across a period of the Periodic Table
As could be expected from their electronic configuration, the group I metals have a relatively low ionisation energy, whereas the noble gases have very high ionisation energies
The size of the first ionisation energy is affected by four factors:
Size of the nuclear charge
The nuclear charge increases with increasing atomic number, which means that there are greater attractive forces between the nucleus and electrons, so more energy is required to overcome these attractive forces when removing an electron
Distance of outer electrons from the nucleus
Electrons in shells that are further away from the nucleus are less attracted to the nucleus - the nuclear attraction is weaker - so the further the outer electron shell is from the nucleus, the lower the ionisation energy
Shielding effect of inner electrons
The shielding effect is when the electrons in full inner shells repel electrons in outer shells, preventing them from feeling the full nuclear charge, so the more shells an atom has, the greater the shielding effect, and the lower the ionisation energy
Spin-pair repulsion
Electrons in the same atomic orbital in a subshell repel each other more than electrons in different atomic orbitals which makes it easier to remove an electron (which is why the first ionisation energy is always the lowest)
Ionisation Energy & the Periodic Table
So, the first ionisation energy increases across a period and decreases down a group
Graph of first ionisation energies from H to Na
There are ionisation energy trends within periods and groups
Ionisation energy across a period
The ionisation energy over a period increases due to the following factors:
Across a period the nuclear charge increases
This causes the atomic radius of the atoms to decrease, as the outer shell is pulled closer to the nucleus, so the distance between the nucleus and the outer electrons decreases
The shielding by inner shell electrons remain reasonably constant as electrons are being added to the same shell
It becomes harder to remove an electron as you move across a period; more energy is needed
So, the ionisation energy increases
There is a rapid decrease in ionisation energy between the last element in one period, and the first element in the next period because:
There is increased distance between the nucleus and the outer electrons as you have added a new shell
There is increased shielding by inner electrons because of the added shell
These two factors outweigh the increased nuclear charge
There is a slight decrease in IE1 between beryllium and boron as the fifth electron in boron is in the 2p subshell, which is further away from the nucleus than the 2s subshell of beryllium
Beryllium has a first ionisation energy of 900 kJ mol-1 as its electron configuration is 1s2 2s2
Boron has a first ionisation energy of 800 kJ mol-1 as its electron configuration is 1s2 2s2 2px1
Nitrogen has a first ionisation energy of 1400 kJ mol-1 as its electron configuration is 1s2 2s2 2px1 2py1 2pz1
Oxygen has a first ionisation energy of 1310 kJ mol-1 as its electron configuration is 1s2 2s2 2px2 2py1 2pz1There is a slight decrease in IE1 between nitrogen and oxygen due to spin-pair repulsion in the 2px orbital of oxygen
Ionisation energy down a group
The ionisation energy down a group decreases due to the following factors:
The number of protons in the atom is increased, so the nuclear charge increases
But, the atomic radius of the atoms increases as you add more shells of electrons, making the atoms bigger
So, the distance between the nucleus and outer electron increases as you descend the group
The shielding by inner shell electrons increases as there are more shells of electrons
These factors outweigh the increased nuclear charge, meaning it becomes easier to remove the outer electron as you descend a group
So, the ionisation energy decreases
Table summarising ionisation energy trends across a period & down a group
Across a period: Ionisation energy increases | Down a group: Ionisation energy decreases |
---|---|
Increase in nuclear charge | Increase in nuclear charge |
The same number of shells | Increased number of shells |
Distance from the outer electron to the nucleus decreases | Distance from the outer electron to the nucleus increases |
Shielding remains relatively constant | Shielding increases |
Decreased atomic / ionic radius | Increased atomic / ionic radius |
The attraction between the outer electron and the nucleus gets stronger so the outer electron is harder to remove | The attraction between the outer electron and the nucleus gets weaker so the outer electron is easier to remove |
Successive Ionisation Energies of an Element
The successive ionisation energies of an element increase
This is because once you have removed the outer electron from an atom, you have formed a positive ion
Removing an electron from a positive ion is more difficult than from a neutral atom
As more electrons are removed, the attractive forces increase due to decreasing shielding and an increase in the proton to electron ratio
The increase in ionisation energy, however, is not constant and is dependent on the atom's electronic configuration
Taking calcium as an example:
Table Showing the Successive Ionisation Energies of Calcium Table
Electronic Configuration | 1s2 2s2 2p6 3s2 3p6 4s1 | 1s2 2s2 2p6 3s2 3p6 | 1s2 2s2 2p6 3s2 3p5 | 1s2 2s2 2p6 3s2 3p4 |
IE | First | Second | Third | Fourth |
IE (kJ mol-1) | 590 | 1150 | 4940 | 6480 |
Successive ionisation energies of an element
The ionisation energy increases as you remove more electrons from an element
The first electron removed has a low IE1 as it is easily removed from the atom due to the spin-pair repulsion of the electrons in the 4s orbital
The second electron is more difficult to remove than the first electron as there is no spin-pair repulsion
The third electron is much more difficult to remove than the second one corresponding to the fact that the third electron is in a principal quantum shell which is closer to the nucleus (3p)
Removal of the fourth electron is more difficult as the orbital is no longer full, and there is less spin-pair repulsion
Examiner Tips and Tricks
It is easy to remove electrons from a full subshell as they undergo spin-pair repulsion.
It gets more difficult to remove electrons from principal quantum shells that get closer to the nucleus as there is less shielding and an increase in attractive forces between the electrons and nuclear charge.
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