Position vectors

We can use vectors to represent positions in space. By definition, (geometric) vectors don't have positions in space (or their positions are irrelevant). Nevertheless, we can always choose a representative vector from its equivalence class such that the source is nailed down to the origin. Such a vector is called a position vector, as its target corresponds to a point in space.



Example. Let us find the equation of the straight line in R2 that goes through the two points (1,2) and (3,4). The position vectors are a=(1,2) and b=(3,4). ba is a vector which is the direction of the line from =(\mathbf{a}\) to b. Let r be the position vector of any point on the desired line. Then ra is a vector which is the direction of the line from a to r, which also goes through the point b. Thus we should have

ra=λ(ba)

for some λR. Thus we have

r=a+λ(ba)

as the general equation for the points on the line that goes through a and b.

If λ=0, then r=a. If λ=1, then r=b. If 0<λ<1, then r is somewhere between a and b. □

Example. Let cRn be a constant vector. The set of position vectors defined by

P={rRn|rc,c=0}

represents the ``plane'' that contains the point c and is perpendicular to the vector c. In R2, this ``plane'' is actually a line. In R3, this is indeed a plane. In Rn with n>3, this ``plane'' is usually called a hyperplane. Find out why this is so named. □

Example. Let cRn be a fixed position vector and rR a positive constant. The set of position vectors defined by
S={xRnxc=r}
defines an n-sphere centered at c with radius r. If n=2, this ``sphere'' is a circle. If n=3, this is indeed a sphere. If n>3, we just call it an n-sphere or a hypersphere
Similarly,
B={xRnxcr}
defines an n-ball centered at c with radius r. If n=2, this is a disk. If n=3, this is indeed a ball. Balls play an important role in topology (a study of shapes based on the ``closeness'' of points). □

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