1.2.19 · D2Newton's Laws & Dynamics

Visual walkthrough — Newton's law of gravitation — universal, action at distance

2,146 words10 min readBack to topic

We only ever use words you already know: stuff (matter), pull, distance, and area. Every symbol below is introduced the moment it is needed and not one step earlier.


Step 1 — Two lumps of stuff, one invisible pull

WHAT. Put two objects in empty space. Call the amount of "stuff" in each one its mass. Write the first mass as and the second as . The little "1" and "2" are just name-tags — they say which lump we mean, nothing more.

WHY. Before any formula, we must agree on the cast of characters. The whole law is a sentence about these two lumps and the empty gap between them. That gap — the straight-line distance from the centre of one to the centre of the other — we name (for range).

PICTURE. Look at the figure: two orange dots, a dotted teal line joining their centres labelled , and two arrows (one on each lump) pointing along that line, toward each other. The arrows are the pull. Notice they lie exactly on the joining line — never sideways. That is the first fact of gravity: the pull is always along the line of centres.

Figure — Newton's law of gravitation — universal, action at distance

Step 2 — More stuff means more pull

WHAT. Ask: if I double the stuff in lump 1, what happens to the pull? Imagine lump 1 as two identical half-lumps glued together. Each half pulls lump 2 on its own. Two halves side by side pull twice as hard. So doubling doubles the force.

WHY. Every tiny bit of matter does its own pulling, and the pulls add up. Twice the matter = twice as many pulling bits = twice the pull. In symbols we write this as The wiggly sign means "grows in step with" — if the right side doubles, so does . Here is the size (magnitude) of the pull.

The same argument works for lump 2. Doubling doubles the pull too, so . Putting both together:

WHY the product, not the sum? The figure shows it: stacking copies of lump 1 multiplies the force from lump 1's side, and independently stacking lump 2 multiplies it from the other side. Two independent doublings multiply to a four-fold pull — that is exactly what gives (), while would only add. (The 3rd-law symmetry in the parent note is the deeper reason the two masses must enter the same way.)

PICTURE. Left panel: one lump 1 → one bundle of pull-lines to lump 2. Right panel: lump 1 doubled → the bundle of pull-lines is visibly doubled. Count the teal lines: they scale with the stuff.

Figure — Newton's law of gravitation — universal, action at distance

Step 3 — Why the pull fades, and fades like

WHAT. Now move the lumps apart and ask how fast the pull weakens. Picture the pull leaving lump 1 as a fixed number of straight "influence lines" spraying outward in every direction — like paint sprayed from a point.

WHY. Those lines spread over the surface of an imaginary sphere centred on lump 1. A sphere of radius has surface area Here is just a fixed number () that comes with spheres; means . The same fixed spray of lines is now smeared over this area. So the concentration of lines — the strength you feel — is

WHY squared and not just ? Because a sphere's skin grows with , not . Go twice as far and the same lines cover times the area, so the pull is four times weaker — not two times. That is the meaning of inverse-square.

PICTURE. Two nested spheres. The near one (small radius) has the lines packed tight — strong pull. The far one (double radius) has the same lines spread thin over 4× the skin — weak pull. Watch the shaded patch: same number of lines, four times the area.

Figure — Newton's law of gravitation — universal, action at distance

Step 4 — Turning "" into "" with the constant

WHAT. The symbol tells us the shape of the law but not the scale. To get real numbers (newtons of force), we multiply by one fixed number, called :

WHY. Nature does not tell us how strong one kilogram's pull is — we must measure it. Henry Cavendish did exactly this by watching two masses gently twist a delicate rod. The number he found is tiny: That (a decimal point followed by ten zeros) is why gravity feels so weak between everyday objects — the whole formula is multiplied by an almost-nothing number.

Term-by-term, right where each lives:

PICTURE. A "dial" figure: the relationship is a fixed curve shape; is the knob that sets its height. Big → tall curve (strong gravity); the real, tiny → a curve pressed almost flat near the axis. The shape is fixed; only scales it.

Figure — Newton's law of gravitation — universal, action at distance

Step 5 — Giving the pull a direction (making it a vector)

WHAT. So far is just a size — a number of newtons. But a pull also has a direction. We attach an arrow of length 1 that points from lump 1 straight toward lump 2, and name it (the little hat "^" means "length exactly one — a pure direction, no size"). Then the full pull on lump 1 is

WHY. The arrow over says "this is a full arrow, size and direction." Multiplying the size by the unit arrow glues the correct direction onto the correct size. The plus sign combined with pointing toward the other mass is what makes gravity attractive — the force points the way the arrow points, i.e. toward lump 2.

WHY not just leave it as a number? Because if a third lump appeared, we would need to add the pulls, and you can only add arrows correctly when each carries its direction. The vector form is future-proof.

PICTURE. The joining line with the little unit arrow drawn on it (length exactly 1), then the full force arrow drawn along the same line but scaled to the force's true size. Same direction; different length.

Figure — Newton's law of gravitation — universal, action at distance

Step 6 — Edge case: what happens at the extremes?

WHAT. A good law must behave sensibly in the corners. Check three:

  1. (lumps infinitely far). The bottom explodes, so . Gravity never becomes exactly zero at any finite distance — it only fades — but it dies fast.
  2. (lumps merge). The bottom shrinks to zero, so the formula screams . This is a warning sign: the law is written for point masses (or centre-to-centre for spheres). Real objects have size, so you never actually put — for a real planet the closest meaningful is its radius (the shell theorem guarantees a solid sphere acts as if all its stuff sits at its centre).
  3. One mass zero (). The top becomes , so . No stuff, no pull — exactly right.

WHY it matters. These checks are how you trust a formula: it must give zero when there's nothing to pull, and it must flag (with infinity) the one place it isn't allowed to be used. The everyday lives on this curve too — it is just the value of evaluated at (Earth's surface):

PICTURE. The full -versus- curve: a steep wall near (the forbidden ), a smooth downhill that flattens toward as grows, with a marker dropped at showing where "surface gravity " sits on the very same curve.

Figure — Newton's law of gravitation — universal, action at distance

The one-picture summary

Everything above collapses into a single labelled diagram: two masses, the joining line , the inward attraction arrows, and the assembled formula with each piece coloured to match where it came from — from Step 2 (stuff), from Step 3 (spreading over a sphere), from Step 4 (measured scale), the arrow from Step 5 (direction).

Figure — Newton's law of gravitation — universal, action at distance
Recall Feynman retelling — the whole walkthrough in plain words

Two blobs of stuff sit in empty space (Step 1). Each blob is really a crowd of tiny pulling grains, so more stuff means proportionally more pull — and because both blobs multiply their pull independently, the force follows the product , not the sum (Step 2). Now imagine that pull sprayed outward like paint from a point; it smears over the skin of a growing sphere whose area is , so twice as far means four times thinner means four times weaker — inverse-square (Step 3). That gives us the shape of the law, and one measured knob sets its true, absurdly-tiny height (Step 4). Glue on an arrow pointing blob-to-blob and it becomes a proper pulling vector (Step 5). Finally we sanity-check the corners: far away the pull fades to nothing, at zero separation the formula (correctly) refuses to answer because that's where point-mass thinking breaks, and no stuff means no pull — and the everyday is just this same curve read off at Earth's surface (Step 6).

Recall Rebuild it yourself (cover the answers)

Why product not sum ::: Two independent doublings multiply; and each scale the force on their own side. Why not ::: Pull spreads over a sphere's skin, area ; area grows as . What does do ::: Sets the true scale (height) of the fixed proportional shape; measured by Cavendish. What does the hat in mean ::: A pure direction — an arrow of length exactly one, pointing from mass 1 toward mass 2. What breaks at ::: The formula gives infinity; it's built for point masses / centre-to-centre, so never use for a real body.


Connections

  • Parent topic — the full statement this page derives.
  • Newton's Third Law — the deep reason both masses enter symmetrically (Step 2).
  • Shell Theorem — why is centre-to-centre and why is forbidden (Step 6).
  • Gravitational Field & Potential — the field view that grows out of the vector form (Step 5).
  • Weight vs Mass read straight off the Step 6 curve.
  • Circular Motion & Centripetal Force & Kepler's Laws — where this force does its orbital work.
  • General Relativity — what replaces the "instant" arrow at cosmic scale.