Moment of a force about a point
Push on a door far from its hinge and it swings open with almost no effort; push the same way right next to the hinge and nothing happens, no matter how hard you shove. The force is identical — what changed is its turning effect, and statics gives that effect a precise name and a precise number: the moment of a force about a point. A moment is not the force itself; it is how much that force wants to rotate a rigid body about some chosen point , and it depends on both how big the force is and how far its line of action passes from . This article builds the moment two equivalent ways — the vector cross product , which handles any 3-D geometry in one stroke, and the scalar force-times-perpendicular-distance method used for quick 2-D sketches — and shows how Varignon's theorem lets you swap an awkward geometry problem for an easy one by resolving the force into components first.
The moment of a force about a point is , with magnitude where is the perpendicular distance from to the force's line of action, and it changes with the choice of because a single force (unlike a couple) has no reference-point-independent moment.
The core idea
A rigid body resists rotation about a point the same way it resists translation under a net force — the measure of "how hard a given force is trying to spin it about " is the moment, and geometry alone decides the answer: same force, same body, but push near the axis and the moment is tiny; push far from it and the moment is large.
The vector definition. Pick any point on the force's line of action and draw the position vector from to . The moment is the cross product
where: is the position vector from to any point on the line of action of , and is the force vector. Because of transmissibility (a force can slide along its own line of action without changing its external effect), the answer does not depend on which point along the line you pick for — a convenient freedom worth using to choose the simplest available.
Magnitude and the scalar shortcut. Expanding the cross product's magnitude gives
where: is the angle between and , , , and is the perpendicular (moment-arm) distance from to the line of action. In 2-D problems this scalar version is usually all you need: find by inspection or trigonometry, multiply by , and fix the sign by the right-hand rule — curl your fingers from toward and your thumb gives the direction of , which in the plane reduces to counterclockwise-positive by the usual sign convention.
Component (determinant) form. Writing and , the cross product expands to
where: each bracketed term is a determinant obtained by crossing out the row and column of that unit vector in the array . For a purely 2-D problem (, ) only the term survives, giving the handy scalar .
Varignon's theorem. The moment of a force about a point equals the sum of the moments of its components about that same point. Instead of hunting for one awkward perpendicular distance to a tilted line of action, resolve into and , find each component's (usually trivial) moment arm, and add the two scalar moments algebraically. This is the single biggest time-saver in moment problems.
The goal is to show, starting only from the geometric definition of the cross product, that the vector rule collapses to the scalar rule "moment equals force times perpendicular distance," so that the right-hand rule, the scalar formula, and the component determinant are provably three routes to the same number and a mismatch between them signals an arithmetic slip.
Step 1. By definition, is a vector of magnitude , where is the angle between (from to any point on the force's line of action) and , directed perpendicular to their plane with sense fixed by the right-hand rule.
Step 2. Interpret geometrically. Drop a perpendicular from onto the line of action; call its length . In the right triangle formed by , the foot of that perpendicular, and the point used for , the side opposite has length — exactly the perpendicular distance . So regardless of which point on the line was chosen, which is transmissibility appearing algebraically.
Step 3. Substitute back: . The moment is simply the force multiplied by how far its line of action misses .
Step 4. Expanding and in Cartesian components and evaluating the determinant gives , algebraically the same object as Step 1. In 2-D only the term survives, and its coefficient must equal from Step 3 — the standard self-check in a moment problem.
Worked example
A force acts at point , directed above the horizontal. Find its moment about the origin , then use the result to also find the moment of the same force about the point .
Step 1. Resolve the force into components: and .
Step 2. Moment about using the 2-D component formula with : , positive so counterclockwise.
Step 3. Cross-check with Varignon's theorem: lies along , so its moment arm about is zero, contributing ; acts at , giving moment CCW. The two components sum to the same , confirming Step 2.
Step 4. Now shift the reference point to . The new position vector is . Using the same 2-D formula, , negative, so clockwise — sharply different from , confirming a single force's moment is reference-point dependent. Final answers: counterclockwise; clockwise.
Competitive stretch
For a 3-D check, at has , giving about the origin. Recomputing with for gives — only the component changes, again confirming the moment tracks the reference point.
Common traps
- Treating a single force's moment as reference-point-independent — that property belongs only to a couple; always recompute freshly when the reference point changes, as the worked example above shows.
- Measuring to a point that is not on the force's line of action — any point on the line works by transmissibility, but a point off the line gives a wrong moment.
- Losing track of the sign convention in the scalar method — fix counterclockwise-positive (or whichever convention the problem states) before assigning or to , and apply it consistently across every force in the problem.
- Searching for one awkward perpendicular distance by trigonometry when Varignon's theorem would let you resolve the force into simple components first.
Ask the tutor: If setting up the cross-product determinant or tracking the sign when the reference point changes feels error-prone, ask the AI tutor to walk through a moment calculation with you step by step.
Why does the moment of a single force change when I pick a different point O, but a couple's moment does not?
A single force's moment depends on the perpendicular distance from to its one line of action, and moving almost always changes that distance, so changes too — as seen when the worked example switched from to and the answer flipped sign and size. A couple (two equal, opposite, parallel forces) has a combined moment about any point that depends only on the distance between the two forces, because the position-vector terms for the two forces cancel identically. That cancellation is special to a force pair and does not happen for a lone force.
Do I have to use the cross product every time, even for a simple 2-D sketch?
No — in 2-D the scalar method is usually faster: identify the perpendicular distance from to the line of action, multiply by the force magnitude, and fix the sign with a chosen positive-rotation convention. The cross product and its determinant form are what you reach for in 3-D, where there is no single obvious "perpendicular distance" to eyeball, or in 2-D when you want a guaranteed-correct sign without reasoning about rotation sense by inspection.
How do I know which point on the line of action to use for r?
Any point works, and that is the content of transmissibility: sliding a force along its own line does not change its external turning effect, so gives the same answer no matter which point on the line you chose for . In practice, pick whichever point makes the coordinates simplest — often where the line of action crosses an axis — since that minimizes arithmetic without changing the result.