Periodic table and periodicity

Class 11 · Updated 2026-10-02. Published for practice.

Why classify

Too many elements to learn one by one. Put similar outer configurations in the same column so one member teaches you the family.

Periodic table: arrangement where similar properties fall under the same group.

Short history path

Dobereiner’s triads: groups of three; middle atomic weight ≈ average of the other two. Only a few sets fit.

Newlands’ octaves: every eighth element echoed the first (noble gases were unknown then, so modern counting looks like 1st and 9th).

Mendeleev: properties are a periodic function of atomic weight. Groups I–VIII with A/B subgroups; left gaps that later filled with real elements.

Mendeleev’s pain points: hydrogen’s place, isotopes sharing one box, Te before I by mass, and no clear “why” behind the periodicity.

Modern law (Moseley): properties are a periodic function of atomic number. Long form: 7 periods, 18 IUPAC groups.

Reading the long form

Period number ≈ highest principal quantum number n for that row. Period lengths: 2, 8, 8, 18, 18, 32… (7th still filling out in textbooks).

Lanthanoids and actinoids sit in panels at the bottom so the table stays usable.

Elements with Z > 100 get systematic IUPAC names built from digit roots + “ium”. You mainly need the idea, not every name memorised.

s, p, d, f blocks

s-block: Groups 1–2. Outer config ns1–2. Soft, reactive metals; low IE; often colour flames (Be, Mg exceptions). Strongly electropositive.

p-block: Groups 13–18. Outer ns2 np1–6. With s-block → representative / main-group elements. End of each period: noble gas ns2 np6.

d-block: Groups 3–12. (n−1)d1–10 ns0–2. Transition metals: coloured ions, variable oxidation states, often catalysts, high melting points.

f-block: lanthanoids Ce–Lu, actinoids Th–Lr. Inner transition. (n−2)f filling. Actinoids radioactive; post-U = transuranium.

Atomic and ionic size

Atomic radius: nucleus centre → outermost electron cloud (definitions differ: covalent, van der Waals, metallic — know which your question means).

Across a period: nuclear charge up, same shell filling → size generally shrinks.

Down a group: new shells → size grows.

Cation < parent atom (less e-, same Z pulls harder). Anion > parent atom (extra e-, more repulsion).

Isoelectronic ions (same e- count): higher nuclear charge → smaller ion. Classic set: N3- > O2- > F- > Na+ > Mg2+ > Al3+.

IE, electron gain enthalpy, electronegativity

Ionisation enthalpy ΔᵢH: energy to remove the outermost e- from gaseous atom. Across period: generally up. Down group: generally down.

Exceptions students must flag: Be, Mg, N, P, noble gases look “high” because of stable configs. He is extreme. Second IE of Na is huge (you’re ripping from Ne-like Na+).

Electron gain enthalpy Δ_egH: enthalpy when gaseous atom gains an e-. More negative = easier anion formation. Cl is the classic “most negative” in many tables; F is less negative than Cl because of small-size repulsion.

Successive electron gains are endothermic (you’re charging a negative ion further).

Electronegativity: pull on a shared pair in a bond. F highest, Cs among the lowest. Not the same thing as IE — you’re in a molecule, not an isolated atom.

Used in these practicals