Learn

Learning preferences

Make learning more comfortable. Changes apply immediately.

Enlarges page content, including diagrams and their labels. You can also use your browser’s zoom.

Choose the colours that are easiest for you to distinguish. Applies to lesson diagrams and lab plots. Labels, shapes, hatching and line patterns also distinguish meanings. Source photographs and raw image brightness stay unchanged; mask-only views are available for image overlays.

ExampleComparisonSample link

Saved in this browser on this device. Preferences are separate from progress backups.

SCIENCE · INVESTIGATE AND EXPLAIN

Test periodic explanations with ionization evidence

Compare evaluated reference data, explain departures from smooth trends and identify successive-removal shell changes.

Learning outcome: Calculate a signed energy difference and ratio, distinguish first from successive removal and defend a structural explanation with source provenance.

Starting recap

Ionization energy removes one electron from an isolated gaseous ground-state atom or ion. The next removal starts with a different ion; its energy is not the cumulative energy already spent.

All lessons are open directly. Your saved experiments remain when you leave and return.

Try

Al has more protons than Mg, yet its first removal energy is smaller. Magnesium’s third removal also costs far more than its second. Can one smooth arrow on a periodic table explain both?

Open the experiment

Predict

Predict the sign of Al minus Mg before inspecting the reference rows. Predict where a large jump should appear in sodium and magnesium successive removals.

Experiment

Capture both adjacent comparisons for Na/Mg/Al and C/N/O. Then compare sodium and magnesium successive removals, checking starting configurations and cumulative sums. Use Li/Na/K to test a down-group explanation.

Test an ionization-energy explanation against evidence

Frozen NIST reference inputs · calculated comparisons · Frozen NIST ASD 5.12 reference rows inspected 2026-10-28. Isolated gaseous ground-state species, not bulk reaction energy or complete PES. Source uncertainty is reported separately and is not an invented hard bound.

Reset keeps your prediction, captures and practice history.

First removal: Na, Mg, Al

Each row starts with a different neutral gaseous atom. These rows are not consecutive removals from one atom. Values are a frozen NIST ASD 5.12 reference excerpt, inspected 2026-10-28, not newly collected observations.

RemovalStarting configurationEnergy (eV)Source uncertainty (eV)Source references
Na[Ne] 3s^15.139076962.5e-7L10921,L9648
Mg[Ne] 3s^27.6462360.000004L10635,L6969
Al[Ne] 3s^2 3p^15.9857690.000003L7215,L10321
04812165.1391Na7.6462Mg5.9858AlRemoval energy (eV) — fixed zero baselineFirst-removal panels: 0–16 eV. Successive-removal panels: 0–90 eV.

Selected comparison: (Mg) versus (Al). Difference (second minus first) = 5.985769 − 7.646236 = -1.660467 eV. Ratio = 5.985769/7.646236 ≈ 0.7828. Al is lower than Mg despite its higher nuclear charge: its removed electron occupies 3p rather than 3s. Subshell energy and penetration matter.

Bracketed [71.6200] is NIST’s semiempirical sodium third-removal value; brackets are a provenance label, not an uncertainty interval. Listed uncertainties retain the source convention. Do not replace them with arbitrary absolute bounds or infer that every row is a direct measurement. No fitted electron-force model produced these energies.

Inspect this NIST data query and bibliography identifiers · Read the definitions, brackets and uncertainty documentation.

Selected change: -1.660467 eV; ratio 0.7828.

Al is lower than Mg despite its higher nuclear charge: its removed electron occupies 3p rather than 3s. Subshell energy and penetration matter.

Captures preserve the selected frozen NIST packet and comparison. Replay recomputes differences and ratios from the same reference inputs; it creates no new measurement or independent replicate.

Understand

Let a reference observation challenge the rule

A first-ionization plot often rises across a period, but “more protons always means a larger first ionization energy” is too strong. Magnesium’s evaluated value is 7.646236 eV, while aluminum’s is 5.985769 eV. Their difference, aluminum minus magnesium, is −1.660467 eV. An explanation that cannot accommodate this pair needs revision.

Select the Na/Mg/Al packet and compare its first pair, then its second pair. Keep the starting configurations beside the energy values. Na to Mg follows the broad rise. Mg to Al reverses it: aluminum’s removed electron is in 3p rather than 3s. Subshell energy, penetration and shielding matter alongside nuclear charge. The numerical values come from an evaluated reference; the qualitative explanation does not calculate those values.

The packets are selected rows from NIST Atomic Spectra Database version 5.12, inspected 28 October 2026. They are not invented detector readings, a complete photoelectron spectrum or new measurements performed in this browser. Each row preserves its source bibliography identifiers and reported uncertainty. Source links are in the live table.

Define the comparison before calculating

An electron volt, eV, is an energy unit for an individual particle-scale event. The listed ionization energy is the minimum energy to remove one electron from an isolated gaseous ground-state atom or ion. It is not the heat released when a solid reacts, a reaction rate, or the energy needed to remove every electron.

For two rows with energies E₁ and E₂, calculate ΔE = E₂ − E₁ and the ratio E₂/E₁. The signed difference answers which is larger and by how much; the ratio answers how many times as large. The table retains the source values; displayed calculations are rounded. A ratio and a difference are distinct summaries, not independent new observations.

In a first-removal packet, each row begins with a different neutral atom. Adding Li’s removal energy to Na’s does not give a successive ionization energy of either species. In a successive-removal packet, each row begins with the progressively charged ion named before the arrow. Its ground state changes, while proton count remains fixed.

Pairing is another reason to inspect structure

Compare carbon, nitrogen and oxygen. Nitrogen has three singly occupied 2p orbitals in the reference description. Oxygen has a paired 2p electron and a smaller first removal energy: 13.618055 eV versus nitrogen’s 14.53413 eV, a difference of −0.916075 eV. Electron repulsion and the energies of the initial and resulting states help explain the departure from a smooth trend.

Avoid the shortcut “a half-filled shell is stable, so no explanation is needed.” State what changes in the electron arrangement, and acknowledge that a qualitative account is not a quantitative many-electron solution. The source uncertainty is not a freely chosen error bar or a claim that the true value must lie inside a hard interval. This exercise does not perform a statistical significance test.

Read a shell transition in successive removals

Neutral Mg starts with [Ne] 3s². The first removal costs 7.646236 eV and leaves Mg+ with one 3s electron. The second costs 15.035271 eV and leaves Mg2+ with the ten-electron closed-shell arrangement. The third costs 80.1436 eV and removes an electron from what was the neutral atom’s n=2 core.

The much larger third cost is consistent with two outer 3s electrons before reaching that core. Reaching charge +2 requires both earlier steps: 7.646236 + 15.035271 = 22.681507 eV. The second-step energy alone is not that sum. The cumulative column adds central values; it does not invent a combined uncertainty from potentially related source errors.

Compare sodium. It begins with only one 3s electron, so the large jump occurs at the second removal. The third sodium entry appears in brackets because NIST identifies it as semiempirical. The NIST quantity documentation explains that distinction. Keep the bracket visible; do not present every number as a directly measured experimental value.

Use a trend within its conditions

Li, Na and K each begin with one outer s electron, but in different shells. Their first removal energies decrease down this group even though nuclear charge rises. Additional shell extent and shielding help explain that comparison. It does not establish how quickly bulk samples react under unspecified conditions.

For practice, consider an original, deliberately synthetic main-group packet: successive removal energies 6, 12, 25 and 120 arbitrary energy units. Predict the likely number of outer electrons before the pronounced jump, and calculate the cumulative energy of the first three steps. Do not identify an element from this information alone.

Check the changed packet

The pronounced fourth-step jump supports three outer electrons under the stated main-group shell interpretation. The first three steps sum to 43 units. That does not uniquely identify an element or prove a particular compound will form. The synthetic values are not additional NIST rows.

Return to configuration checks if the initial species is unclear. Next use controlled charge and distance comparisons to distinguish an explanatory model from a measured atomic property.

Apply

The first three Mg removal energies are about 7.65, 15.04 and 80.14 eV. The strongest supported shell interpretation is:

Public practice checks a specific claim. It does not establish independent mastery.

Explain one trend and one exception without inventing a measured effective charge. Distinguish central values, source uncertainties and bracketed semiempirical entries. Give a changed-case valence inference from a supplied jump.

Continue

Completion requires a saved prediction, at least one capture and a reflection. Presence checks do not grade your reasoning.

Skipping retains experiments and awards no mastery.

Save a science backup or import one

Science work is stored locally in this browser, separately from mathematics and AI. It does not sync automatically. Use this science-only backup; this checkout's older all-subject export does not include science.

A legacy file is available only when the complete snapshot fits the 36 MB limit. For larger snapshots, prepare a complete file set below; never discard notebooks to make a smaller file.

Matching imported notebook drafts replace their current drafts. Omitted lessons and known first attempts remain. Export your current work first if you want to retain both drafts.

Complete file sets and course backups

A file set can hold more work than one science file. Keep its manifest and every part together. Each file is limited to 36 MB. This format needs this version of LearnAI or a compatible newer version; older versions can use only the legacy single-file backup above.

The set includes every saved science course and global continuation at this moment. Later edits need a new export. A conflicting tab exports its own visible work, which may differ from saved work in another tab.

0 file(s) selected. File order and filenames do not determine identity. Missing, changed or conflicting parts block the entire restore; no good part is applied by itself.

Science storage: loading. No account or remote computation is required.