Periodic trends explorer: atomic radius, ionisation energy and electronegativity across a period and down a group, with the exceptions explained

Colour the periodic table by atomic radius, first ionisation energy or electronegativity, tap any element, and graph the trend across its period or down its group. The exceptions to each trend (beryllium to boron, nitrogen to oxygen, aluminium to gallium) are flagged in red with the reason.

Keep it one tap away for everyday use.

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  1. Pick element
  2. Property
  3. Trend
  4. Check
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Tap an element to choose its period and group. Lanthanoids and actinoids are left out. Radii are approximate covalent radii rounded to 5 pm, for s- and p-block elements only; ionisation energies (NIST) and electronegativities (Pauling scale) are rounded textbook values.

Try this

  • Pick atomic radius and go across period 2. Each step adds a proton that pulls the same shell in tighter.
  • Switch to ionisation energy across period 2. It rises, except at boron and oxygen: read why underneath.
  • Go down group 1. The atoms grow and the outer electron is easier to remove, which is why caesium is so reactive.
  • Look at group 13. Gallium is no bigger than aluminium: the ten d electrons in between change the pattern.

Check yourself

What it does

The periodic table is not just a list: its rows (periods) and columns (groups) show smooth patterns in how big atoms are, how tightly they hold their electrons, and how strongly they pull on shared electrons in a bond. This tool colours the table by one of three properties at a time: atomic radius, first ionisation energy and electronegativity. Tap any element and a bar graph shows the trend across its period or down its group.

Trends have exceptions, and exam questions love them. Where a value breaks the usual direction, its bar turns red and a short reason appears underneath: why boron is easier to ionise than beryllium, why oxygen is easier than nitrogen, and why gallium is no bigger than aluminium.

It follows the school topics on the modern periodic table and periodic trends in properties (Class 11 Chemistry, classification of elements and periodicity), and the periodic table in Class 10. For every element’s full data see interactive periodic table, for how electrons fill the shells behind these trends electron configuration filler, and for how the table was first built mendeleev's predictions.

How to use it

  1. Pick the property: atomic radius, ionisation energy or electronegativity. The table recolours: pale is low, dark is high.
  2. Tap an element. Its period (or group) is outlined and graphed below.
  3. Switch between Across the period and Down the group.
  4. Read the element’s values and the explanation of the trend and any exceptions under the graph.

Worked example

Open the page: carbon is chosen and the graph shows atomic radius across period 2: lithium about 130 pm, beryllium 95, boron 85, carbon 75, nitrogen 70, oxygen 65 and fluorine 55. Each step adds a proton that pulls the same second shell in tighter. Neon has no bar: noble gases form almost no bonds, so their size is measured differently.

Switch to ionisation energy: the bars rise from lithium (520 kJ/mol) to neon (2080 kJ/mol), but two are red. Boron (801) is below beryllium (899) because its electron sits alone in a 2p orbital, and oxygen (1314) is below nitrogen (1402) because its fourth p electron has to pair up. Carbon’s own value is 1086 kJ/mol (11.26 eV per atom).

Tap aluminium, choose Down the group with atomic radius: gallium (about 120 pm) is flagged, no bigger than aluminium, because of the ten poorly shielding 3d electrons added in between.

Tips

  • Size and ionisation energy usually move in opposite directions: big atoms lose electrons easily.
  • Fluorine is the most electronegative element; caesium and francium the least.
  • Exceptions to ionisation energy come at half-full and full subshells.

FAQ

Why are some radii missing? Radii are shown only for the s- and p-block elements, where the trend is clearest and the values agree best between sources. Noble gases are left out on purpose.

Why kJ/mol and not eV? Textbooks give ionisation enthalpy per mole; the facts also show eV per atom. Multiply eV by 96.485 to get kJ/mol.

Is anything stored? No. It all runs in your browser.

Where the numbers come from

  • First ionisation energies: NIST Atomic Spectra Database values (public domain), rounded to 0.01 eV and converted with 1 eV per atom = 96.485 kJ/mol. Electronegativities: the Pauling scale values most textbooks print, rounded. Both from the site's periodic table data (src/lib/sci/ptable.ts).
  • Atomic radii: approximate single-bond covalent radii rounded to the nearest 5 pm, for the s- and p-block elements of periods 1 to 6; published sets differ by 5 to 10 pm, so the tool is for reading trends, not for exact values.
  • The trends and their exceptions (Be → B and N → O in ionisation energy; Al ≈ Ga in size) are general chemistry found in any textbook. Checked: radius falls across periods 2 and 3 and grows down groups 1 and 2; the exceptions are flagged exactly where expected.

Standard scientific values, such as constants, atomic weights and melting points, are facts found in every textbook; we name where ours were checked. If you are an author or publisher and want a value, a credit or a table changed or removed, tell us and we will act quickly.

Last updated 2026-11-09.

Change log for Periodic trends

  1. Add #1356 Periodic trends Details on GitHub

Every change to fibub

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