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…
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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)=(∣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 ∣x∣p+∣y∣p+∣z∣p=1.