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2.3

Spectra and ionization energy as evidence

Your guide: Miss SanaCounts atoms the way you count rupees: carefully.

Spectra and ionization energy as evidence

How do we know electrons sit in shells? We never see them.

Two kinds of evidence answer this.

Smart Syllabus 2026 leaves out the atomic spectra part (2.3.1) for the 2026 exam. The ionization evidence part stays. Learn both, because they explain shells.

1 · Atomic spectra

Heat a gas or pass electric discharge through it. It gives out light of certain wavelengths.

This spectrum has coloured lines. It is the atomic emission spectrum.

Pass white light through a cold gas. Some wavelengths are absorbed. They show as dark lines. This is the atomic absorption spectrum.

The dark lines sit at exactly the same wavelengths as the coloured lines.

Each element has its own fixed energy levels. So each has its own spectrum. The book calls spectra the finger prints of elements.

2 · Successive ionization energies of magnesium

Remove the electrons of one atom one by one. The energies are the successive ionization energies.

The energy rises as we go from the valence shell to inner shells.

For magnesium, the first two electrons come from the outer shell. They need less energy.

A big jump comes at the third electron. It lies in a shell much closer to the nucleus.

A much bigger jump comes at the eleventh and twelfth electrons. They lie in the first shell.

Two big jumps show that electrons of magnesium sit in three shells.

3 · First ionization energies across elements

All ionization energies are strongly endothermic. It takes energy to remove an electron.

Down a group the energy falls. More shells weaken the hold on the valence electrons.

Across a period it rises. The shell number is the same, but the proton number grows.

Alkali metals have the lowest value in each period. Noble gases have the highest.

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Notes, short questions and MCQs

Read the full notes: key terms, model answers and MCQs with answers

Spectra and ionization energy as evidence

How do we know electrons sit in shells? We never see them.

Two kinds of evidence answer this.

Smart Syllabus 2026 leaves out the atomic spectra part (2.3.1) for the 2026 exam. The ionization evidence part stays. Learn both, because they explain shells.

1 · Atomic spectra

Heat a gas or pass electric discharge through it. It gives out light of certain wavelengths.

This spectrum has coloured lines. It is the atomic emission spectrum.

Pass white light through a cold gas. Some wavelengths are absorbed. They show as dark lines. This is the atomic absorption spectrum.

The dark lines sit at exactly the same wavelengths as the coloured lines.

Each element has its own fixed energy levels. So each has its own spectrum. The book calls spectra the finger prints of elements.

2 · Successive ionization energies of magnesium

Remove the electrons of one atom one by one. The energies are the successive ionization energies.

The energy rises as we go from the valence shell to inner shells.

For magnesium, the first two electrons come from the outer shell. They need less energy.

A big jump comes at the third electron. It lies in a shell much closer to the nucleus.

A much bigger jump comes at the eleventh and twelfth electrons. They lie in the first shell.

Two big jumps show that electrons of magnesium sit in three shells.

3 · First ionization energies across elements

All ionization energies are strongly endothermic. It takes energy to remove an electron.

Down a group the energy falls. More shells weaken the hold on the valence electrons.

Across a period it rises. The shell number is the same, but the proton number grows.

Alkali metals have the lowest value in each period. Noble gases have the highest.

Key terms

Emission spectrum
Coloured lines from a hot or excited gas.
Absorption spectrum
Dark lines where a cold gas takes light from white light.
Successive ionization energies
The energies to remove the 1st, 2nd, 3rd electron and so on.

Short questions with model answers

  1. Q1. Quick Check 2.2 (c): which element is a noble gas, and which is a metal giving AX2?

      Element I has the highest i1 = 2372, so it is the noble gas. Element III has i2 = 1760, about 2 × 900 = 1800, so two outer electrons: a metal for AX2.

    Common mistakes

    • ✗ “Every element has the same spectrum.”

      ✓ Each element has its own fixed energy levels, so its own spectrum.

    • ✗ “Ionization energy releases energy.”

      ✓ Removing an electron takes energy. It is endothermic.

    MCQs

    1. 1. In the magnesium plot, where does the first big jump come?

      1. (a) At the 1st electron.
      2. (b) At the 2nd electron.
      3. (c) At the 3rd electron.
      4. (d) At the 12th electron only.
      Show answer

      (c) Two electrons are in the outer shell. The third lies in the shell below.

    2. 2. Which group has the lowest ionization energy in each period?

      1. (a) Alkali metals
      2. (b) Halogens
      3. (c) Noble gases
      4. (d) Transition metals
      Show answer

      (a) The book says so.

    3. 3. Dark lines in an absorption spectrum sit at:

      1. (a) the same wavelengths as the emission lines
      2. (b) random wavelengths
      3. (c) only red wavelengths
      4. (d) no wavelength
      Show answer

      (a) The book says they match exactly.

    4. 4. The ionization energy goes down a group because:

      1. (a) the number of shells increases
      2. (b) the nucleus gets smaller
      3. (c) electrons get heavier
      4. (d) the shell number falls
      Show answer

      (a) More shells weaken the hold on valence electrons.

    Quick revision

    • Atomic spectra are fingerprints of elements.
    • Two big jumps in the magnesium data show three shells.
    • Ionization energy rises across a period and falls down a group.

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