Stereographic projection

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Definition

Setup

Consider R3, three-dimensional Euclidean space, with coordinates x,y,z. Denote:

S2:={(x,y,z)∈R3∣x2+y2+z2=1}

Identify C with the xy-plane under the map:

(x,y,0)↦x+iy

Let N=(0,0,1) denote the north pole in S2. Then, the stereographic projection is a bijective map:

S2∖{N}→C

Definition of the map

Geometrically stereographic projection is defined as follows:

For any point P∈S2∖{N}, consider the line passing through N and P. This line is not parallel to C, hence intersects C at exactly one point. That point is the image of P under stereographic projection.

The formula for stereographic projection is given as:

(x,y,z)↦x+iy1−z

Stereographic projection is invertible, giving a reverse map:

C→S2∖{N}

The reverse map is given by:

x+iy↦(2xx2+y2+1,2yx2+y2+1,x2+y2−1x2+y2+1)

In terms of z and z¯, this is written as:

z↦(z+z¯|z|2+1,z−z¯i(|z|2+1),|z|2−1|z|2+1)

Facts

  • Stereographic projection is conformal: Stereographic projection is a conformal mapping when thought of as a mapping between the Riemannian manifolds S2∖{N} and C. In other words, it preserves angles between curves (provided we make a matching choice of orientation for the two manifolds).
  • Stereographic projection preserves circles: Under stereographic projection, circles in S2∖{N} get mapped to circles in C, while circles passing through N (with N removed), get mapped to straight lines.