CHEMISTRY · LESSON 03 OF 12
Periodic table
Electron configurations follow from filling orbitals in order of energy. The periodic table groups elements with similar outer electrons, and effective nuclear charge explains the trends in size, ionisation energy and electronegativity.
What this lesson explains
The periodic table is chemistry’s map. From an element’s position you can predict its outer electrons, the ions it forms, how reactive it is, whether it is a metal, and what kind of bonds it makes. These predictions guide material selection, corrosion behaviour and reaction design in chemical engineering.
Before you begin
Quantum numbers and subshells
Shell n contains subshells s, p, d, … with 1, 3, 5, … orbitals (see Quantum theory). Each orbital holds two electrons.
Noble-gas shorthand
Write the preceding noble gas in brackets for the core: Na = [Ne]3s1.
The idea, made visible
Electrons fill orbitals from the lowest energy upward (the Aufbau principle): 1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 5s, 4d, … Each orbital holds at most two electrons with opposite spins (Pauli exclusion principle). Within a subshell of equal-energy orbitals, electrons occupy separate orbitals with parallel spins before pairing (Hund’s rule).
The valence electrons (outermost shell) govern chemistry. Elements in the same group have the same valence configuration — for example ns1 for the alkali metals — and therefore similar properties. The table’s blocks show which subshell is being filled: s, p, d or f.
The key to the trends is effective nuclear charge Zeff: the positive charge an outer electron actually feels, less than Z because inner electrons shield it. Across a period, Z increases while the added electrons are in the same shell and shield each other poorly, so Zeff increases: the atoms become smaller and hold their electrons more tightly. Down a group, a new, larger shell is added each period, so atoms get bigger and outer electrons are easier to remove.
So atomic radius decreases across a period and increases down a group; ionisation energy (energy to remove an electron) and electronegativity (pull on bonding electrons) increase across and decrease down. Small exceptions have clear reasons: ionisation energy drops from Be to B (the 2p electron is higher in energy than 2s) and from N to O (pairing repulsion in O’s 2p).
Ions: cations are smaller than their atoms (fewer electrons, sometimes a whole shell removed); anions are larger. When transition metals form ions they lose their 4s electrons before 3d: Fe is [Ar]3d64s2, Fe2+ is [Ar]3d6.
| element | configuration | IE₁ (kJ/mol) | radius (pm) |
|---|---|---|---|
| Na | [Ne]3s¹ | 496 | 186 |
| Mg | [Ne]3s² | 738 | 160 |
| Al | [Ne]3s²3p¹ | 578 | 143 |
| Si | [Ne]3s²3p² | 787 | 118 |
| P | [Ne]3s²3p³ | 1012 | 110 |
| S | [Ne]3s²3p⁴ | 1000 | 103 |
| Cl | [Ne]3s²3p⁵ | 1251 | 99 |
| Ar | [Ne]3s²3p⁶ | 1521 | 71 |
The general rise has two dips: Mg → Al (the 3p electron is higher in energy and slightly shielded by 3s) and P → S (the fourth 3p electron is paired and repelled). Radii are approximate and differ between sources depending on how they are defined.
Key terms
- Electron configuration
- The distribution of electrons among orbitals, e.g. O: 1s22s22p4.
- Valence electrons
- Electrons in the outermost shell (for main-group elements: the ns and np electrons).
- Effective nuclear charge Zeff
- The net positive charge felt by an electron after shielding by other electrons; roughly Z − (number of core electrons) for valence electrons.
- Ionisation energy (IE)
- Energy required to remove an electron from a gaseous atom or ion: X(g) → X+(g) + e−. Successive IEs increase.
- Electronegativity
- The ability of an atom in a molecule to attract bonding electrons (Pauling scale: F = 3.98 highest).
- Paramagnetic / diamagnetic
- Having unpaired electrons (attracted by a magnetic field) / all electrons paired (weakly repelled).
The formulas and what they mean
| Symbol | Meaning | Unit |
|---|---|---|
| nℓx | x electrons in subshell ℓ of shell n (e.g. 2p⁴) | — |
| Zeff | effective nuclear charge | proton charges |
| IE1, IE2 | first, second ionisation energies | kJ/mol |
| χ | electronegativity | no unit |
Filling order
1s 2s 2p 3s 3p 4s 3d 4p 5s 4d 5p 6s 4f 5d 6p …
Conditions and limits: Ground states of most atoms. Exceptions include Cr ([Ar]3d⁵4s¹) and Cu ([Ar]3d¹⁰4s¹).
Capacity
s: 2, p: 6, d: 10, f: 14 electrons
Conditions and limits: Each orbital holds 2 electrons of opposite spin (Pauli).
Valence effective charge (estimate)
Zeff ≈ Z − (core electrons)
Conditions and limits: A rough guide for comparing main-group atoms; refined models (Slater’s rules) are beyond this topic.
Ion formation, transition metals
remove ns before (n − 1)d
Conditions and limits: Fe → Fe2+: remove the two 4s electrons.
Why it works: Why a large jump in ionisation energy reveals the valence electrons
Magnesium ([Ne]3s²) has IE₁ = 738, IE₂ = 1451 and IE₃ = 7733 kJ/mol.
IE₁ and IE₂ remove the two 3s valence electrons.
Each removal is harder because the ion becomes more positive.
IE₃ must remove an electron from the 2p core, much closer to the nucleus with far less shielding.
A new, inner shell.
So IE₃ is about five times IE₂.
The jump marks the end of the valence shell.
This is why magnesium forms Mg²⁺ but never Mg³⁺ in chemical reactions.
A first worked example
Writing configurations and predicting trends
- Count the electrons (Z for a neutral atom; adjust for charge).
- Fill subshells in the Aufbau order, respecting capacities; use noble-gas shorthand.
- For orbital diagrams, apply Hund’s rule; count unpaired electrons.
- For cations of transition metals, remove the ns electrons first.
- For trends, compare positions: same period → Z_eff argument; same group → number of shells argument. Mention known exceptions.
Configuration and unpaired electrons of oxygen
Problem. Write the ground-state configuration of oxygen (Z = 8) and find the number of unpaired electrons.
1s2 2s2 2p4.
Fill 1s, 2s, then 2p with the remaining four electrons.
2p has three orbitals: put one electron in each, then pair the fourth: ↑↓ ↑ ↑.
Hund’s rule.
Result: 1s²2s²2p⁴, with 2 unpaired electrons (oxygen atoms are paramagnetic).
What it means: A 2p³ configuration (nitrogen) would have 3 unpaired electrons.
A different case
A transition-metal ion
Problem. Write configurations for Fe (Z = 26) and Fe3+.
Fe: [Ar]3d64s2.
18 core electrons + 8.
Fe3+: remove the two 4s electrons, then one 3d: [Ar]3d5.
Remove ns before (n − 1)d.
Result: Fe = [Ar]3d⁶4s²; Fe³⁺ = [Ar]3d⁵.
What it means: Writing Fe³⁺ as [Ar]3d³4s² is a common error; the 4s electrons go first.
More worked cases
Each case below uses a different skill. Every step and result is shown.
Electrons needed for a noble-gas configuration
Problem. An atom has shell arrangement 2, 8, 7. How many electrons must it gain to complete an octet? Which element and ion is it?
Outer shell has 7; an octet needs 8: gain 1.
Main-group atoms tend to reach 8 valence electrons.
Total electrons 17 ⇒ chlorine; ion Cl−.
Z = 17.
Result: Gains 1 electron to form Cl− (configuration of argon).
What it means: Halogens (group 17) form 1− ions; alkali metals (2, 8, 1 etc.) form 1+ ions.
Compare sizes and ionisation energies
Problem. Arrange Na, Mg and K in order of increasing atomic radius, and of increasing first ionisation energy.
Na and Mg are in period 3; Mg has higher Zeff, so Mg is smaller than Na.
Across a period.
K is below Na (an extra shell), so K is larger than Na.
Down a group.
Ionisation energy follows the reverse order.
Smaller atoms hold electrons more tightly.
Result: Radius: Mg < Na < K. First ionisation energy: K < Na < Mg (419 < 496 < 738 kJ/mol).
What it means: This is why potassium reacts with water more violently than sodium.
Isoelectronic ions
Problem. Order O2−, F−, Na+ and Mg2+ by size.
All have 10 electrons (the neon configuration).
Same electron count.
Their proton numbers are 8, 9, 11, 12: more protons pull the same electrons closer.
Higher nuclear charge, smaller ion.
Result: Mg²⁺ < Na⁺ < F⁻ < O²⁻ (smallest to largest).
What it means: For isoelectronic species, size decreases as Z increases.
Common misunderstandings
Misunderstanding: Filling 3d before 4s for neutral atoms, or removing 3d before 4s for ions.
Correct idea: Fill 4s before 3d; ionise 4s before 3d.
Misunderstanding: Pairing electrons before filling each orbital of a subshell singly.
Correct idea: Hund’s rule: singly first, parallel spins.
Misunderstanding: “Atoms get bigger across a period because they have more electrons.”
Correct idea: They get smaller: the added electrons are in the same shell while Z_eff increases.
Misunderstanding: Treating trends as rules with no exceptions.
Correct idea: Be/B and N/O ionisation dips, and Cr/Cu configurations, are the standard exceptions.
Keep in mind
- 1s 2s 2p 3s 3p 4s 3d 4p 5s 4d 5p 6s 4f 5d 6p …Filling order
- s: 2, p: 6, d: 10, f: 14 electronsCapacity
- Zeff ≈ Z − (core electrons)Valence effective charge (estimate)
- remove ns before (n − 1)dIon formation, transition metals
Scope of this lesson
- Quantitative shielding (Slater’s rules), lanthanides and actinides, and detailed transition-metal chemistry are beyond this topic.
Next: Chemical bonding. Atoms bond by transferring electrons (ionic) or sharing them (covalent). Lewis structures count the electrons; VSEPR turns electron domains into shapes; shape and electronegativity decide polarity.
Original study text. Sources and credits.