Ionization energy is one of the most fundamental ideas in IB Chemistry. It explains how strongly an atom holds onto its electrons, why some elements form positive ions more easily than others, and how periodic trends arise from nuclear charge, electron shielding, and atomic radius. Understanding ionization energy helps students interpret reactivity trends, metallic behavior, and electron configurations.
What Is Ionization Energy?
Ionization energy is the energy required to remove one mole of electrons from one mole of gaseous atoms to form one mole of gaseous positive ions.
The definition used in IB Chemistry emphasizes:
- Gaseous atoms
- One mole of particles
- Formation of +1 ions
Example:
X(g) → X⁺(g) + e⁻
Ionization involves overcoming the attraction between the nucleus and the outer electron.
Why Energy Is Required
Electrons are attracted to the positively charged nucleus.
To remove one, energy must be supplied to overcome this electrostatic attraction.
If the attraction is strong:
- More energy is needed
- Ionization energy is high
If the attraction is weak:
- Less energy is needed
- Ionization energy is low
This explains why metals lose electrons easily while non-metals do not.
Factors Affecting Ionization Energy
Three main factors determine ionization energy:
1. Nuclear Charge (number of protons)
More protons → stronger attraction → higher ionization energy.
As nuclear charge increases, electrons are held more tightly.
