For north-pole stereographic projection on the unit sphere, the antipodal pair point has coordinate . Since , this gives when both coordinates are finite. On the whole Riemann sphere, write , pairing zero with infinity. The two axis endpoints fixed by a sphere rotation obey this relation.
Use the north-pole stereographic projection and the cross-ratio convention . Antipodes have coordinates . Rotate the first point to the south pole, whose coordinate is zero: its antipode becomes infinity, while a point at spherical distance has projected modulus . Möbius invariance of the cross-ratio then gives the displayed identity. Antipodal endpoints require the extended-value interpretation.

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