Visual walkthrough — Formulae — Σ1, Σn, Σn², Σn³ — proofs
Before line one, here is the entire vocabulary we will use, each earned with a picture as we go. If a word looks scary, wait for its step — it gets a drawing.
Step 1 — What "square a number" looks like
WHAT. means a grid of unit boxes. So box, boxes, boxes.
WHY. Our whole sum is literally the total number of little boxes in a growing family of square tiles. Seeing it as area makes the "shortcut" believable — there really is a pattern to count, not just symbols to push.
PICTURE. Look at the growing squares: each new term is a bigger solid square of chalk boxes.

Step 2 — The one idea: a difference that cancels itself
WHAT. Pick any function . Look at the chain of differences Every middle value appears once with a plus and once with a minus, so it dies. Only the outermost survivors remain:
WHY. This is the engine. It turns a long sum into just two numbers — but only if the thing we are summing can be written as a difference . So our job becomes: find an whose difference secretly contains .
PICTURE. Watch the pluses and minuses annihilate down the ladder; only the top and bottom rungs light up.

Here each symbol's job:
- — the rung difference we add up.
- — the top survivor (the very last plus).
- — the bottom survivor (the very first minus).
Step 3 — Choose the right : why
WHAT. We try and compute its rung difference:
WHY and not something else? We want a to fall out. Expanding a cube produces a square term automatically. Cubing is one power above squaring, and taking a difference of consecutive cubes drops the leading (it cancels), leaving the we hunt for on top. That is the whole reason for the choice — not magic, just "one power up, then difference."
PICTURE. The cube is a solid block of side ; carving out the inner block leaves an L-shaped shell. The shell's pieces are exactly .

Expanding with the Binomial Theorem (or just multiplying out): Each term is a physical piece of that shell — the three slabs are the , the three bars are the , the single corner is the .
Step 4 — Sum both sides and let the left telescope
WHAT. Apply to both sides of Step 3:
WHY. The left side is exactly the telescoping shape from Step 2 with , so it collapses instantly. The right side we will break apart in the next step. We are trading a hard sum for an easy end minus start.
PICTURE. The ladder of cube-shells stacks; interiors cancel; only at the top and at the bottom survive.

- — the top survivor, the biggest cube.
- — the bottom survivor, since .
Step 5 — Split the right side using known sums
WHAT. Break the right side apart:
WHY. A sum of a sum is the sum of the parts, and a constant multiplier slides out front — this is linearity of . Doing this exposes our unknown plus two sums we already know, so we can solve for the unknown.
PICTURE. The mixed pile of chalk boxes sorts into three colour-coded bins: the bin (what we want), the bin (known), and the bin (known).

The two known building blocks (proven on the parent note and via Arithmetic Progressions for the linear one):
- — a triangular number (see Triangular Numbers): stack into a triangle.
- — just ones added, giving .
Step 6 — Set the two sides equal and solve
WHAT. Equate Step 4 and Step 5, then isolate :
WHY. The left is a plain polynomial in ; the right holds our target. One rearrangement frees , then divide by .
PICTURE. A balance scale: the cube-difference on the left, the three bins on the right; we slide the known bins across to leave alone.

Expand the left, , then move the known terms over: Put over a common denominator of : Factor the top: . So
Step 7 — The degenerate and edge cases (never skipped)
WHAT. Check the boundary values so the formula is trustworthy everywhere.
WHY. A formula that only works for "nice" is a trap. We test the smallest, the empty case, and the growth for huge .
PICTURE. Three quick chalk panels: (nothing), (one box), and the large- cubic curve the sum hugs.

- : formula gives . Direct: . ✔
- (empty sum): the sum has no terms, so it is by convention. Formula: . ✔ The empty sum equalling is why the startstop bookkeeping stays consistent.
- : formula . Direct: . ✔
- Large : the top is dominated by , so . This matches — the sum is a discrete area, the seed of Definite Integrals as Limits of Sums.
The one-picture summary
Everything compressed: choose → its shell difference is → summing telescopes the left to → split the right into the known → solve for the last bin .

Recall Feynman retelling — say it to a friend
We wanted to add up all the square tiles without adding them one at a time. Trick: think about cubes instead. Take a cube of side and peel off the smaller cube of side inside it — the leftover shell is made of three flat squares (), three thin bars (), and one tiny corner (). Now stack these shells for every from up to . Because each shell's inside exactly matches the previous shell's outside, almost everything cancels — like a telescope folding shut — and we're left with just the big cube minus the tiny starting . That leftover equals three times our square-sum plus stuff we already know (the plain sum and ). Move the known stuff aside, divide by three, and out drops . We never added a single square directly — we let the cubes do the counting.
Recall
Which do we telescope for , and why?
What does the left side collapse to after summing ?
State .
Check the formula at .
Why is the empty sum () equal to here?
Large- size of ?
Connections
- Telescoping Series — the collapse in Steps 2 and 4 is exactly this trick.
- Binomial Theorem — expands in Step 3.
- Arithmetic Progressions — supplies used in Step 5.
- Triangular Numbers — the shape of we borrow.
- Definite Integrals as Limits of Sums — the large- cubic match in Step 7.
- Mathematical Induction — an alternative way to verify this same formula.
- Hinglish version of the parent note