Andromeda
Note

Lines in Space

Definition

A line in three-dimensional space is the set of all points that can be reached by starting at a point P0P_0 and moving any distance along a fixed direction vector v\mathbf{v}.

Why It Matters

Precise 3D line modeling is the difference between a successful rendezvous in orbit and a collision; it provides the coordinate-free framework needed to navigate and build in the complex three-dimensional reality of our universe.

Core Concepts

  • Vector Equation: r(t)=r0+tv\mathbf{r}(t) = \mathbf{r}_0 + t\mathbf{v}, where r0\mathbf{r}_0 is the position vector of the fixed point and tt is a scalar parameter.

    • How to read: “The vector function r of t equals the vector r zero plus t times the vector v.”

    • Meaning: Start at r0\mathbf{r}_0, move along direction v\mathbf{v} scaled by parameter tt—all points on the line.

    • Parametric Equations: x=x0+tv1,y=y0+tv2,z=z0+tv3x = x_0 + tv_1, y = y_0 + tv_2, z = z_0 + tv_3. These describe the coordinates individually as functions of the parameter tt.

    • How to read: “The coordinate x equals x zero plus t v one, with similar linear forms for y and z.”

    • Meaning: Component form of the vector equation—each coordinate changes linearly with tt.

  • Distance from Point to Line: The distance dd from a point SS to a line passing through PP with direction v\mathbf{v} is given by: d=PS×vvd = \frac{|\vec{PS} \times \mathbf{v}|}{|\mathbf{v}|}

    • How to read: “The distance d equals the magnitude of the cross product of vector P S and vector v, all divided by the magnitude of vector v.”
    • Meaning / when to use: Cross product gives parallelogram area; dividing by v|\mathbf{v}| yields perpendicular distance from point to line.

Connected Concepts