Normal Vector -- From Wolfram MathWorld
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The normal vector, often simply called the "normal," to a surface is a vector which is perpendicular to the surface at a given point. When normals are considered on closed surfaces, the inward-pointing normal (pointing towards the interior of the surface) and outward-pointing normal are usually distinguished.
The unit vector obtained by normalizing the normal vector (i.e., dividing a nonzero normal vector by its vector norm) is the unit normal vector, often known simply as the "unit normal." Care should be taken to not confuse the terms "vector norm" (length of vector), "normal vector" (perpendicular vector) and "normalized vector" (unit-length vector).
The normal vector is commonly denoted or
, with a hat sometimes (but not always) added (i.e.,
and
) to explicitly indicate a unit normal vector.
The normal vector at a point on a surface
is given by
| (1) |
where and
are partial derivatives.
A normal vector to a plane specified by
| (2) |
is given by
| (3) |
where denotes the gradient. The equation of a plane with normal vector
passing through the point
is given by
| (4) |
For a plane curve, the unit normal vector can be defined by
| (5) |
where is the unit tangent vector and
is the polar angle. Given a unit tangent vector
| (6) |
with , the normal is
| (7) |
For a plane curve given parametrically, the normal vector relative to the point is given by
| (8) | |||
| (9) |
To actually place the vector normal to the curve, it must be displaced by .
For a space curve, the unit normal is given by
| (10) | |||
| (11) | |||
| (12) |
where is the tangent vector,
is the arc length, and
is the curvature. It is also given by
| (13) |
where is the binormal vector (Gray 1997, p. 192).
For a surface with parametrization , the normal vector is given by
| (14) |
Given a three-dimensional surface defined implicitly by ,
| (15) |
If the surface is defined parametrically in the form
| (16) | |||
| (17) | |||
| (18) |
define the vectors
| (19) |
| (20) |
Then the unit normal vector is
| (21) |
Let be the discriminant of the metric tensor. Then
| (22) |
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