Q.Define ionisation enthalpy. Discuss the factors affecting ionisation enthalpy of the elements and its trends in the periodic table.
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Start your 14-day free trial to unlock the full solution →Ionisation enthalpy is the energy required to remove an electron from a gaseous atom. It increases across a period (stronger nuclear pull, smaller size) and decreases down a group (larger size, more shielding), with key exceptions arising from half-filled and fully-filled subshell stability.
What is Ionisation Enthalpy?
Ionisation enthalpy (or ionisation energy) is the minimum energy required to remove the most loosely bound electron from an isolated gaseous atom in its ground state, converting it into a gaseous cation:
The process is always endothermic because energy must be supplied to overcome the electrostatic attraction between the nucleus and the electron. The value is typically expressed in or .
Successive ionisation enthalpies () refer to the removal of the first, second, third electrons, and so on. Each successive ionisation requires more energy because you are removing an electron from an increasingly positive ion.
Factors Affecting Ionisation Enthalpy
Understanding why some atoms hold their electrons more tightly than others requires examining four interrelated factors:
1. Nuclear Charge ()
As the number of protons in the nucleus increases, the positive charge pulling on the electrons grows stronger. Higher nuclear charge means a tighter grip on the outermost electron, so ionisation enthalpy increases.
For example, across the second period from lithium to neon, the nuclear charge rises from to , and ionisation enthalpy climbs accordingly.
2. Atomic Radius
The farther an electron sits from the nucleus, the weaker the electrostatic attraction it experiences (Coulomb's law: force ). Larger atoms have their valence electrons at greater distances, making them easier to remove.
This is why ionisation enthalpy generally decreases as you move down a group: each successive element adds a new shell, dramatically increasing atomic size.
3. Shielding (Screening) Effect
Inner-shell electrons repel outer-shell electrons, partially canceling the nuclear attraction. This "shielding" reduces the effective nuclear charge () felt by valence electrons:
where is the shielding constant. More inner electrons mean greater shielding and lower ionisation enthalpy. Down a group, the addition of complete inner shells significantly increases shielding, contributing to the decrease in ionisation enthalpy.
4. Electronic Configuration (Subshell Stability)
Certain electron configurations are exceptionally stable and resist ionisation:
- Half-filled subshells (): Electrons occupy separate orbitals with parallel spins, minimizing electron-electron repulsion (exchange energy stabilization).
- Fully-filled subshells (): Maximum symmetry and stability.
Removing an electron from these stable arrangements requires extra energy, creating anomalies in otherwise smooth trends.
When comparing ionisation enthalpies, always check the electron configuration first. Stability from half-filled or fully-filled subshells often trumps the simple trend.
Periodic Trends in Ionisation Enthalpy
Across a Period (Left to Right)
Ionisation enthalpy generally increases across a period.
Why? Moving left to right:
- Nuclear charge increases (more protons).
- Atomic radius decreases (electrons added to the same shell, pulled closer).
- Shielding remains roughly constant (no new inner shells).
The net effect is a stronger hold on valence electrons.
Key exceptions arise from subshell stability:
| Element | Configuration | trend |
|---|---|---|
| Be → B | → | Drops (easier to remove a electron than disrupt the stable ) |
| N → O | → | Drops (removing one electron from relieves pairing repulsion; is half-filled and stable) |
These dips interrupt the overall upward trend but are entirely predictable from electronic structure.
Down a Group (Top to Bottom) …
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