Before you can trust that one-line law, you must earn every symbol inside it. Below, each piece is built from nothing — plain words first, then the picture, then why the topic can't live without it. Read top to bottom: each block uses only things defined above it.
This page is the ground floor for the parent topic. Nothing here is assumed — we start from an arrow on a page.
A plain number (like "5 kg") is a scalar — size only, no direction. But "moving 5 m/s to the east" needs a direction too, so it's a vector.
Look at the figure below. On the left, the blue arrow's length is the size and where it points is the direction — that single arrow carries two pieces of information at once. On the right, the yellow dot labelled "5 kg" is a scalar: a bare number with nowhere to point.
The key subtlety: r only means something once you name O. Move the origin, and r changes. That is why the parent note keeps shouting "about the same point" — every rotational quantity is measured relative to a chosen O.
In the figure below, the blue arrow r runs from the yellow origin O to the green object. Now watch the red dashed arrow r′: it reaches the same object but starts from a different origin O′ — so it has a different length and direction. Same object, different r, purely because we moved the reference point.
This is the one genuinely new tool, so we build it carefully. See Cross Product for more.
Why sinθ and not, say, cosθ? Because sinθ measures how perpendicular the two arrows are:
If the arrows point the same way (θ=0°): sin0°=0 → the cross product is zero.
If the arrows are at right angles (θ=90°): sin90°=1 → the cross product is biggest.
If they point opposite ways (θ=180°): sin180°=0 → zero again.
The figure below shows exactly this: three panels of the same two arrows at 0°, 90°, 180°, with sinθ printed under each — 0, then 1, then 0 again. Watch how the "twisting power" peaks when the arrows are square to each other.
Everything funnels into the single boxed law, then branches out to the rigid-body special case and to Conservation of Angular Momentum (what happens when the twist is zero).
Cover the right side; can you answer each before moving on?
What does the little arrow on r tell you that a plain number cannot?
A direction — r carries both a length (distance) and a direction; a scalar has size only.
What does the origin O have to do with r?
r is measured fromO; change O and r changes — so every rotational quantity is "about a point."
Momentum p in symbols and which way it points?
p=mv; same direction as v since mass is a positive scalar.
What does dtd(⋅) mean, and how do you differentiate a vector?
The rate of change per second — steepness of the graph for a scalar; for a vector, differentiate each component, giving a new arrow that can be nonzero even when the length is fixed.
Newton's second law in momentum form?
F=dp/dt.
The size of a×b, and why sinθ?
absinθ; sinθ keeps only the perpendicular (twisting) part and vanishes when the arrows are parallel.
Which way does a×b point, and what's our 2D sign convention?
Right-hand rule — perpendicular to both; in-plane arrows give out-of-page = counterclockwise = positive, into-page = clockwise = negative.
Why is v×v=0?
A vector makes a 0° angle with itself, and sin0°=0.
Angular momentum and torque as cross products?
L=r×p and τ=r×F.
What is a radian, and why prefer it to degrees?
The angle whose arc equals one radius; a full turn is 2π rad; it makes arc=rθ and spin formulas clean.
Does a particle on a straight path have angular momentum about an off-line point?
Yes — L=pd where d is the perpendicular distance from the point to the path.