STRAIGHT LINES IN SPACE
The Vector, Parametric, Canonical, and General Equations of a Straight Line
The position of a straight line in space is determined by a point on this line and a vector parallel to the line. Let us write an
equation of such a line in space.
To this end, we take an arbitrary point on the line, join Ì0 and Ì to the origin, and find the coordinates of the radius-vectors
It is seen from the figure, that .
If the point Ì belongs to the straight line, then the vectors and are collinear.
Consequently, these vectors meet the collinearity condition
where t is a parameter.
Let us write the collinearity condition in the form
equation (*) is the vector equation of the given line.
Suppose given the coordinates of the point M0(x0,y0,z0) and the direction vector . Let us write the left-hand side of equation (*) in the vector form
the direction vector is
Let us represent equation (*) in the form
Equating the respective coefficients of the unit vectors on the right- and left- sides, we obtain parametric equations of the straight line:
Eliminating the parameter t, we obtain the canonical equations of a straight line:
Example. Write the canonical equations of the straight line passing through the point parallel to the vector . We compose the canonical equation by formula (28):
Equating each fraction to a parameter t, we obtain the parametric equations of the line:
The general equation of a straight line in space. Since a straight line in space is represented as the intersection of two planes, the general equation of a straight line in space has the form of a system
where the first and the second equations are the equations of the corresponding planes.
It is always possible to transform the general equation of a straight line into a canonical equation and vice versa.
Since the direction of is perpendicular to those of the vectors and , it follows that
i.e., the canonical equation is
The angle between straight lines in space. The parallelism and perpendicularity conditions for straight lines. Let us find the angle between intersecting right lines given by their canonical equations
The angle between these two lines is equal to the angle between their direction vectors
The parallelism and perpendicularity conditions for right lines coincide with the collinearity and perpendicularity conditions of their direction vectors and .
If straight lines are perpendicular, then , i.e., , and the perpendicularity condition is
If straight lines are parallel, then the vector is collinear to , i.e., their coordinates are proportional, and the proportionality condition is
Date: 2015-01-02; view: 2040