Section Objectives
In this section, we will use our knowledge of vectors to help us describe and work with lines and planes in 3-dimensional space. Let's start with lines.
Consider the line in space that passes through the point and is parallel to the vector . Let be another point on the line.
The vector must be parallel to . Therefore , for some scalar . It follows that
or
These equations are the parametric equations for the line. If we solve each for , we find the symmetric equations for the line:
In the symmetric equations, if one of the direction numbers (, , or ) is zero, then the corresponding fraction is not defined. In such a case, we will not write that fraction as part of the symmetric equations, rather we will simply write of value of the coordinate in its place. For example, parametric equations for the line through and parallel to are
and we will write the symmetric equations as
To describe a plane in space, let's suppose we are given a point on the plane and a vector that is normal (perpendicular) to the plane. Then the plane is the collections of all points such that is orthogonal to .
In other words,
This vector equation can be expanded by writing the vectors in component form and computing the dot product:
or
If we further expand the equation, we get the general form of the equation of a plane:
where .
Suppose is a point on the plane , which has normal vector . Also suppose that is a point that is not on the plane. Then the distance from the plane to the point is given by (see the figure).
Is it easy to find a more convenient formula for by using the formula for the projection:
Now let's use the fact that satisfies that equation of the plane to say that
or
Therefore we have the following point-to-plane distance formula:
Suppose is a point on the line parallel to , and is a point not on the line. By referring to the figure below, it is easy to derive the following point-to-line distance formula: