The previous article showed that, even in the plane, the notion of a "ball" gives rise to some surprising shapes. What happens in space?
Balls that grow… ---------------------------
Let p be a strictly positive real number. In ordinary space—that is, ℝ3 equipped with an orthonormal coordinate system—we define the norm N*p* of the vector in ℝ3 with coordinates (x, y, z) by Np(x,y,z)=(xp+yp+zp)1/p,\text{N}_p (x, y, z) = ( | x |^p + | y |^p + | z |^p ) ^{1/p}, just as for vectors in the plane (see page 36). This then allows us to define the distance associated with N*p*.
As in the plane, N*p is a norm only when p ≥ 1. When p = 2, we recover Euclidean distance, for which the shortest path between two points is a straight line. When p = 1, the distance from the origin O(0, 0, 0) to the point with coordinates (x, y, z*) is attained by a path consisting of three line segments parallel to the axes, generalizing the "Manhattan" distance.
The unit ball B*p(O, 1) in space, or simply Bp, is defined in the same way as in the plane; its boundary* is the surface with equation xp+yp+zp=1.| x |^p + | y |^p + | z |^p = 1.