Normal Vector — Definition, Formula & Examples
A normal vector is a vector that points perpendicular (at a right angle) to a surface or curve at a specific point. It tells you which direction is 'straight out' from the surface at that location.
Given a surface defined by , the normal vector at a point on the surface is , which is orthogonal to every tangent vector at that point. For a plane with equation , the normal vector is .
Key Formula
Where:
- = The normal vector to the surface
- = A scalar function whose level surface F = 0 defines the surface
- = The gradient of F, computed via partial derivatives
How It Works
For a plane, you can read the normal vector directly from the coefficients of , , and in the plane equation. For a general surface , compute the gradient and evaluate it at the point of interest. If you have two tangent vectors lying in a plane or on a surface, their cross product gives a normal vector. The normal vector is not unique in direction — you can scale it by any nonzero scalar, and both and are valid normals pointing in opposite directions.
Worked Example
Problem: Find a normal vector to the plane 3x − 2y + 5z = 10.
Identify coefficients: For a plane ax + by + cz = d, the normal vector is simply the vector of coefficients.
Read off the normal: From the equation 3x − 2y + 5z = 10, extract a = 3, b = −2, c = 5.
Answer: A normal vector to the plane is .
Why It Matters
Normal vectors are essential in multivariable calculus for computing surface integrals and flux. In computer graphics, normal vectors at each point on a surface determine how light reflects, controlling shading and rendering. Physics uses them to define forces on surfaces, such as the normal force in mechanics.
Common Mistakes
Mistake: Confusing a normal vector with a normalized (unit) vector.
Correction: A normal vector is perpendicular to a surface and can have any magnitude. A normalized vector has magnitude 1. To get a unit normal, divide the normal vector by its magnitude: .
