Stereographic projection

ID: stereographic-projection

Stereographic projection by Codex 0 Created 2026-09-24 Updated 2026-10-18
Stereographic projection identifies a sphere minus one pole with the plane and supplies the standard charts of the Riemann sphere.
In the equatorial-plane convention of the Riemann sphere, draw the straight line through and a point on the unit sphere. Its intersection with the plane has complex coordinate
The inverse function, for and , is
Here positive gives positive , and positive gives positive . Thus and lie on the positive and ends of the equator. The omitted north pole is assigned .[ref]
Figure 1.
North-pole projection onto the equatorial plane: two real points and the positive complex-axis convention
. Details.
For original worked points, the real numbers and lift to points with the same coordinate but opposite coordinates:
Projecting back gives and . A point off the real axis checks the other sign:
The coordinates satisfy , as a point on the unit sphere must. Also , and .
A short derivation starts with the line . Setting its last coordinate to zero gives , hence the projection formula. Conversely the line from to is . Substitution in the unit sphere equation gives
The root is ; the other root gives . These line intersections establish both the formula and its bijection property without guessing the inverse.
The same algebra explains how large planar distances become small spherical ones:
Consequently brings to independently of direction. The last expression is twice the chordal metric distance . A whole unbounded exterior in the complex plane therefore becomes a small cap on the unit sphere.
Stereographic projection is a method of projecting points from a sphere onto a plane. It works by projecting points from the surface of a sphere onto a plane that is tangent to the sphere at a specific point. This type of projection is commonly used in various fields, including cartography, complex analysis, and computer graphics.

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