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Reading Time: 6 min
Last Updated: January 23, 2026
Main Ideas: 5
Reading Time: 6 min
Last Updated: January 23, 2026
Main Ideas: 5

Topic 1.5 Notes – Atomic Structure and Electron Configuration

Verified for 2027 AP® Chemistry Exam
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Atomic structure explains how protons, neutrons, and electrons are arranged in an atom and how their charges interact. Electron configuration builds on that structure by showing where electrons are located in energy levels and subshells. Together, these ideas explain why atoms behave the way they do, especially when forming ions and during ionization.

1. Atomic Structure and Coulombic Attraction

Every atom contains three subatomic particles:

  • Protons
    • Charge = +1
    • Mass ≈ 1 amu
    • Located in the nucleus
  • Neutrons
    • Charge = 0
    • Mass ≈ 1 amu
    • Located in the nucleus
  • Electrons
    • Charge = -1
    • Mass ≈ 0 amu (very small)
    • Found outside the nucleus

The atomic number equals the number of protons. In a neutral atom, electrons = protons.

The key force holding electrons near the nucleus is electrostatic attraction. Opposite charges attract, and the strength of that attraction follows Coulomb’s law:

F∝q1q2r2 F \propto \frac{q_{1} q_{2}}{r^{2}}

  • Larger charges → stronger attraction
  • Smaller distance rr → much stronger attraction (because of r2r^{2})

This explains two big ideas you’ll use all year:

  • Electrons closer to the nucleus have lower energy.
  • Electrons farther away are easier to remove.

When you justify ionization energy on a test, your reasoning almost always traces back to charge and distance.

2. Energy Levels, Sublevels, and Electron Organization

Electrons don’t sit randomly. They occupy specific energy levels.

Shells (Principal Energy Levels)

  • Labeled n=1,2,3,4...n = 1, 2, 3, 4...
  • As nn increases:
    • Distance from nucleus increases
    • Energy increases

The outermost shell is the valence shell.

Subshells (Sublevels)

Each shell contains subshells:

  • s → max 2 electrons
  • p → max 6
  • d → max 10
  • f → max 14

These subshells correspond directly to the blocks of the periodic table.

Study guide illustration

Periodic table divided into s, p, d, and f blocks

The left two columns are the s-block, the right six columns are the p-block, the middle transition metals are the d-block, and the bottom rows are the f-block. If you can read these blocks, you can write electron configurations without memorizing a long energy chart.

Core vs Valence Electrons

  • Valence electrons = electrons in the highest nn level (for main-group elements, only s and p)
  • Core electrons = inner electrons

Example:
Phosphorus → 1s22s22p63s23p31s^{2} 2s^{2} 2p^{6} 3s^{2} 3p^{3}
Valence electrons are in n=3n=3: 3s23p33s^{2} 3p^{3} → 5 valence electrons.

3. The Rules for Writing Ground-State Electron Configurations

Three rules control how electrons fill orbitals.

Aufbau Principle

Electrons fill orbitals in order of increasing energy.

Order (follow periodic table layout):
1s → 2s → 2p → 3s → 3p → 4s → 3d → 4p → 5s → 4d → 5p → 6s → 4f → 5d → 6p

Notice 4s fills before 3d. That detail matters later for ions.

Pauli Exclusion Principle

  • Max 2 electrons per orbital
  • Must have opposite spins

No orbital can hold more than two electrons.

Hund’s Rule

In equal-energy orbitals (like the three p orbitals):

  • Fill singly first
  • Then pair
Study guide illustration

Orbital box diagrams illustrating Hund’s rule (N → Ne)

In the 2p orbitals for N, O, F, and Ne, notice how each box gets one electron before any pairing happens.

This reduces electron-electron repulsion.

Quantum numbers exist behind all this, but assigning them is not tested on the AP exam.

4. How to Write Electron Configurations

Example: Sulfur (atomic number 16)

  1. 16 electrons total
  2. Fill in order:

1s22s22p63s23p41s^{2} 2s^{2} 2p^{6} 3s^{2} 3p^{4}

Check: 2 + 2 + 6 + 2 + 4 = 16 ✔

Noble Gas Shortcut

Use the previous noble gas in brackets.

Sulfur becomes:
[Ne]3s23p4[Ne] 3s^{2} 3p^{4}

This saves time and reduces mistakes.

Writing Ions

Cations: remove electrons from the highest nn level first.

Example:
Fe = [Ar]4s23d6[Ar] 4s^{2} 3d^{6}

Fe²⁺: remove 4s electrons first →
[Ar]3d6[Ar] 3d^{6}

That 4s-before-3d removal shows up constantly on tests.

Anions: add electrons following Aufbau order.

5. Electron Configuration and Ionization Energy

Ionization energy = energy required to remove an electron.

Think Coulomb’s law every time.

Ionization energy increases when:

  • Nuclear charge increases (more protons)
  • Atomic radius decreases (smaller rr)
  • Effective nuclear charge increases (less shielding)

Ionization energy decreases when:

  • Electron is farther from nucleus
  • More core electrons shield the attraction

When comparing two atoms, your explanation should include words like:

  • “greater nuclear charge”
  • “smaller radius”
  • “stronger attraction between nucleus and valence electron”

If those ideas aren’t in your answer, you’re probably not scoring full credit.

Key Takeaways

Coulombic attraction depends on charge and distance, following F∝q1q2r2F \propto \frac{q_{1} q_{2}}{r^{2}}.
Electrons in higher nn levels are farther from the nucleus and easier to remove.
s, p, d, f subshell capacities are 2, 6, 10, and 14 electrons.
4s fills before 3d, but 4s electrons are removed first when forming transition metal cations.
Valence electrons for main-group elements are the outermost s and p electrons only.
Stronger nucleus–electron attraction means higher ionization energy.

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Notes

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