Visual walkthrough — Modern periodic law — based on atomic number
Prerequisites we lean on (all built here as we go): Bohr Model of the Atom, Atomic Number and Atomic Mass, Effective Nuclear Charge and Shielding, and the experiment itself, Moseley's X-ray Experiment. This page is the visual companion to the parent topic.
Step 1 — What is inside an atom, drawn to scale of idea
WHAT we did: Named the pieces and the one number we care about, .
WHY: Everything that follows is about how hard the nucleus pulls an electron. That pull is set by the charge . So is the hero of the whole story.
WHAT IT LOOKS LIKE: A red central charge , with electrons parked on rings labelled by their shell number (the innermost ring is ).

Recall What does
physically count? The number of protons in the nucleus. ::: The number of protons in the nucleus.
Step 2 — Why an X-ray is born: an electron falls
WHAT we did: Turned "X-ray emission" into a concrete motion — an electron dropping from ring to ring .
WHY: Energy is never destroyed. The energy the electron loses by falling has to go somewhere; it comes out as the X-ray. So the X-ray's energy = the energy gap between the two rings. If we can compute that gap, we know the X-ray.
WHAT IT LOOKS LIKE: A red arrow diving from the outer ring to the inner hole, with a wavy red X-ray shooting off.

Step 3 — The screen: electrons hide part of the nucleus
WHAT we did: Replaced the full charge with the smaller, honest charge .
WHY THIS TOOL and not just ? Because a real atom has many electrons, and they get in each other's way. Using alone would over-count the pull. The single correction is the simplest honest fix — see Effective Nuclear Charge and Shielding.
WHAT IT LOOKS LIKE: The bright red at the centre, partly greyed out by a shield, leaving a smaller effective red core labelled .

Step 4 — The energy of a fall depends on charge squared
WHAT we did: Wrote the X-ray energy in terms of the felt charge, and reminded ourselves that energy .
WHY the square? Two effects both grow with charge: a bigger charge pulls the rings closer and pulls harder. Multiply two charge-effects together and you get charge. That is why appears to the power 2, not 1.
WHAT IT LOOKS LIKE: A curve of versus that bends upward — a parabola — because of the squaring. Not a line yet.

Step 5 — Take the square root to straighten the curve
WHAT we did: Undid the square with a square root, turning the parabola into .
WHY THIS TOOL (the square root)? A square root is exactly the operation that undoes a square. We chose it precisely because it converts the awkward into a clean first-power , which draws a line.
WHAT IT LOOKS LIKE: The bent parabola of Step 4 pulled straight — a red line rising steadily, crossing the -axis a little to the right of zero (at ).

Step 6 — Why the line crosses at , not at zero
WHAT we did: Located the exact crossing point of the line.
WHY: This is the degenerate case — what happens when the frequency drops to zero. It pins down the meaning of : it is the atomic number at which the felt charge would vanish.
WHAT IT LOOKS LIKE: A zoom on the bottom of the line, red dot sitting at , clearly to the right of the origin.

Step 7 — The whole point: gives a line, mass does not
WHAT we did: Ran the experiment's logic side by side — versus mass.
WHY: Ordering elements needs a quantity that changes smoothly and by exactly one from element to element. The straight line shows does; the crooked plot shows mass does not.
WHAT IT LOOKS LIKE: Two panels — left, a clean red line ( vs ); right, the same points scattered off a line ( vs mass).

The one-picture summary
Everything above, in one flow: an electron falls (), it feels charge , we take a root, and out comes the straight line that fingerprints atomic number.

Recall Feynman: the whole walkthrough in plain words
Picture an atom as a tiny red ball of "pull" (that's the protons, of them) with electrons circling it. Kick out an inner electron; an outer one dives in to fill the gap and spits out a flash of X-ray light. How energetic that flash is depends on how strong the pull feels — but other electrons shade the ball a little, so the felt pull is minus a small hider-number . Bohr tells us the flash energy grows like that felt pull squared, which draws a curved line versus . Take the square root — the exact undo of squaring — and the curve snaps into a perfectly straight ruler line. Do the same trick against atomic mass and you get a messy zig-zag. The straight line is nature shouting: "count the protons, not the weight." That is Moseley's law, and it is why the modern periodic table is built on atomic number.
Active Recall
Why does the X-ray energy depend on and not ?
Why take the square root of at all?
At what does the Moseley line cross the horizontal axis?
What does the slope contain?
Why does mass fail to give a straight line?
Connections
- Bohr Model of the Atom — source of the energy dependence (Step 4)
- Effective Nuclear Charge and Shielding — origin of and the constant (Step 3)
- Atomic Number and Atomic Mass — meaning of (Step 1)
- Moseley's X-ray Experiment — the experiment we reconstructed
- Mendeleev's Periodic Table — the mass-based law this replaced (Step 7)
- Periodic Trends — the repeating properties that riding on makes regular