Previously, we learned to calculate the length of vectors in Rn, and thus the distance between points in An. It's often useful to express a vector in terms of its length and its direction.
Let's start by defining direction.
If v∈Rn is any nonzero vector, its direction is
v:=∥v∥v
This is also called the normalization of v. By definition, we have
v=∥v∥v,
which expresses v as its direction times its length. The 0 vector has no direction.
We can now give a formal definition of one of the most important spaces in geometry: the n-sphere. This is defined to be the set of unit vectors in Rn+1:
Note the shift in indexing: S1⊂R2 is the usual unit circle in 2d, while S2⊂R3 is the usual unit sphere in 3d.
It's worth looking at the edge case
S0={v∈R1∣∥v∥=1}={±1}⊂R
That is, the 0-sphere consists of exactly two points! While this may seem strange, it fits nicely into a pattern about spheres in general:
every "slice" or "cross-section" of S2 is a 1-sphere, except for the "north and south poles" (0,0,±1).
every "slice" or "cross-section" of S1 is a 0-sphere, except for the "north and south poles" (0,±1);
Let's prove this in general! This is a nice example of how we can use mathematical formalism to prove statements in n dimensions based on our intuition in ≤3 dimensions.
We can use the defining equation of Sn to find a parametrization of it. Let's start with the case of S1. Its defining equation is
x2+y2=1
Let's rearrange this to solve for y in terms of x:
x2+y2y2y2=1=1−x2=±1−x2
So we can take x=t as our parameter variable. We also need to find the domain of t (equivalently x). Remember that we can only take square roots of non-negative numbers. So we need to have