where λis a scalar parameter. Note that as λvaries from 0 to 1 the position vector
r moves from r 1 to r 2 .An alternative form for the equation of the line is given by
r =r 2 +λ∗(r 1 −r 2 ) −∞ < λ ∗<∞
where λ∗ is some other scalar parameter. This second form for the line has the
position vector r moving from r 2 to r 1 as λ∗varies from 0 to 1. The vector ±(r 2 −r 1 )
is called the direction vector of the line. Equating the coefficients of the unit vectors
in the equation (6.41) there results the scalar parametric equations representing the
line. These parametric equations have the form
x=x 1 +λ(x 2 −x 1 ), y =y 1 +λ(y 2 −y 1 ), z =z 1 +λ(z 1 −z 2 ) −∞ < λ < ∞
If the quantities x 2 −x 1 ,y 2 −y 1 and z 2 −z 1 are different from zero, then the equation
for the line can be represented in the symmetric form
x−x 1
x 2 −x 1 =
y−y 1
y 2 −y 1 =
z−z 1
z 2 −z 1 =λ (6 .42)
Note that the equation of a line can also be represented as the intersection of
two planes
N 1 x+N 2 y+N 3 z+D 1 =0
M 1 x+M 2 y+M 3 z+D 2 =0
or
N ·(r −r 0 ) =0
M ·(r −r 1 ) =0
provided the planes are not parallel or N =kM, for ka nonzero constant.
Example 6-13. Show the perpendicular distance from a point (x 0 , y 0 , z 0 )to a
given line defined by x=x 1 +α 1 t, y =y 1 +α 2 t, z =z 1 +α 3 tis given by
d=
∣∣
∣∣(r 0 −r 1 )× α
|α|
∣∣