N-sphere

In mathematics, an n-sphere or hypersphere is an ⁠${\displaystyle n}$⁠-dimensional generalization of the ⁠${\displaystyle 1}$⁠-dimensional circle and ⁠${\displaystyle 2}$⁠-dimensional sphere to any non-negative integer ⁠${\displaystyle n}$⁠. The circle is considered 1-dimensional, and the sphere 2-dimensional, because the surfaces themselves are 1- and 2-dimensional respectively, not because they exist as shapes in 1- and 2-dimensional space. As such, the ⁠${\displaystyle n}$⁠-sphere is the setting for ⁠${\displaystyle n}$⁠-dimensional spherical geometry.

Considered extrinsically, as a hypersurface embedded in ⁠${\displaystyle (n+1)}$⁠-dimensional Euclidean space, an ⁠${\displaystyle n}$⁠-sphere is the locus of points at equal distance (the radius) from a given center point. Its interior, consisting of all points closer to the center than the radius, is an ⁠${\displaystyle (n+1)}$⁠-dimensional ball. In particular:

• The ⁠${\displaystyle 0}$⁠-sphere is the pair of points at the ends of a line segment (⁠${\displaystyle 1}$⁠-ball).
• The ⁠${\displaystyle 1}$⁠-sphere is a circle, the circumference of a disk (⁠${\displaystyle 2}$⁠-ball) in the two-dimensional plane.
• The ⁠${\displaystyle 2}$⁠-sphere, often simply called a sphere, is the boundary of a ⁠${\displaystyle 3}$⁠-ball in three-dimensional space.
• The 3-sphere is the boundary of a ⁠${\displaystyle 4}$⁠-ball in four-dimensional space.
• The ⁠${\displaystyle (n-1)}$⁠-sphere is the boundary of an ⁠${\displaystyle n}$⁠-ball.

Given a Cartesian coordinate system, the unit ⁠${\displaystyle n}$⁠-sphere of radius ⁠${\displaystyle 1}$⁠ can be defined as:

${\displaystyle S^{n}=\left\{x\in \mathbb {R} ^{n+1}:\left\|x\right\|=1\right\}.}$

Considered intrinsically, when ⁠${\displaystyle n\geq 1}$⁠, the ⁠${\displaystyle n}$⁠-sphere is a Riemannian manifold of positive constant curvature, and is orientable. The geodesics of the ⁠${\displaystyle n}$⁠-sphere are called great circles.

The stereographic projection maps the ⁠${\displaystyle n}$⁠-sphere onto ⁠${\displaystyle n}$⁠-space with a single adjoined point at infinity; under the metric thereby defined, ${\displaystyle \mathbb {R} ^{n}\cup \{\infty \}}$ is a model for the ⁠${\displaystyle n}$⁠-sphere.

In the more general setting of topology, any topological space that is homeomorphic to the unit ⁠${\displaystyle n}$⁠-sphere is called an ⁠${\displaystyle n}$⁠-sphere. Under inverse stereographic projection, the ⁠${\displaystyle n}$⁠-sphere is the one-point compactification of ⁠${\displaystyle n}$⁠-space. The ⁠${\displaystyle n}$⁠-spheres admit several other topological descriptions: for example, they can be constructed by gluing two ⁠${\displaystyle n}$⁠-dimensional spaces together, by identifying the boundary of an ⁠${\displaystyle n}$⁠-cube with a point, or (inductively) by forming the suspension of an ⁠${\displaystyle (n-1)}$⁠-sphere. When ⁠${\displaystyle n\geq 2}$⁠ it is simply connected; the ⁠${\displaystyle 1}$⁠-sphere (circle) is not simply connected; the ⁠${\displaystyle 0}$⁠-sphere is not even connected, consisting of two discrete points.