The curvature-minus-one Poincaré disk model has Riemannian metric
The geodesics through zero are Euclidean diameters. Indeed, for a path written in polar coordinates, its length is at least , and hence at least between zero and a point of modulus . The radial segment attains this lower bound. By uniqueness of a geodesic with given initial tangent, these radial paths describe all geodesics through the origin. The radial hyperbolic distance is
Thus a hyperbolic circle in the Poincare disc is the indicated Euclidean circle.
An isometry from the Poincaré half-plane model to the Poincaré disk model is the Cayley transform between the half-plane and disk,
Writing , one has and . Substitution into the disk Riemannian metric gives , the half-plane metric, and maps to zero.
Put . The inverse image of obeys
Since , completing the square yields
This proves that the hyperbolic circle in the upper half-plane has Euclidean centre and radius .

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