# Horosphere

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{{Short description|Hypersurface in hyperbolic space}}
[[File:633 honeycomb one cell horosphere.png|220px|right|thumb|A horosphere within the [Poincaré disk model](/source/Poincar%C3%A9_disk_model) tangent to the edges of a [hexagonal tiling](/source/hexagonal_tiling) cell of a [hexagonal tiling honeycomb](/source/hexagonal_tiling_honeycomb)]]
[[File:Apollonian spheres.jpg|thumb|[Apollonian sphere packing](/source/Apollonian_sphere_packing) can be seen as showing horospheres that are tangent to an outer sphere of a [Poincaré disk model](/source/Poincar%C3%A9_disk_model)]]
In [hyperbolic geometry](/source/hyperbolic_geometry), a '''horosphere''' (or '''parasphere''') is a specific [hypersurface](/source/hypersurface) in [hyperbolic ''n''-space](/source/hyperbolic_space). It is the boundary of a '''horoball''', the limit of a sequence of increasing balls sharing (on one side) a tangent hyperplane and its point of tangency.  For ''n'' = 2 a horosphere is called a [horocycle](/source/horocycle).

A horosphere can also be described as the limit of the hyperspheres that share a tangent hyperplane at a given point, as their radii go towards infinity. In Euclidean geometry, such a "hypersphere of infinite radius" would be a hyperplane, but in hyperbolic geometry it is a horosphere (a curved surface).

==History==
The concept has its roots in a notion expressed by [F. L. Wachter](/source/Friedrich_Ludwig_Wachter) in 1816 in a letter to his teacher [Gauss](/source/Carl_Friedrich_Gauss). Noting that in Euclidean geometry the limit of a sphere as its radius tends to infinity is a plane, Wachter affirmed that even if the [fifth postulate](/source/Euclid's_fifth_postulate) were false, there would nevertheless be a geometry on the surface identical with that of the ordinary plane.<ref>Roberto Bonola (1906), ''Non-Euclidean Geometry'', translated by [H.S. Carslaw](/source/Horatio_Scott_Carslaw), Dover, 1955; p. 63</ref>  The terms ''horosphere'' and ''horocycle'' are due to [Lobachevsky](/source/Nikolai_Lobachevsky), who established various results showing that the geometry of horocycles and the horosphere in hyperbolic space were equivalent to those of lines and the plane in Euclidean space.<ref>Roberto Bonola (1906), ''Non-Euclidean Geometry'', translated by H.S. Carslaw, Dover, 1955; p. 88</ref>  The term "horoball" is  due to [William Thurston](/source/William_Thurston), who used it in his work on [hyperbolic 3-manifold](/source/hyperbolic_3-manifold)s.  The terms horosphere and horoball are often used in 3-dimensional hyperbolic geometry.

==Models==
In the [conformal ball model](/source/Poincar%C3%A9_disc), a horosphere is represented by a sphere tangent to the horizon sphere.  In the [upper half-space model](/source/Poincar%C3%A9_half-plane_model), a horosphere can appear either as a sphere tangent to the horizon plane, or as a plane parallel to the horizon plane.  In the [hyperboloid model](/source/hyperboloid_model), a horosphere is represented by a plane whose normal lies in the asymptotic cone.

==Curvature==
A horosphere has a critical amount of (isotropic) curvature: if the curvature were any greater, the surface would close, yielding a sphere, and if the curvature were any less, the surface would be an (''N''&nbsp;−&nbsp;1)-dimensional [hypercycle](/source/hypercycle_(geometry)).

==References==
{{reflist}}

* ''Appendix, the theory of space'' Janos Bolyai, 1987, p.143

{{Manifolds}}

Category:3-manifolds
Category:Curves
Category:Hyperbolic geometry

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Adapted from the Wikipedia article [Horosphere](https://en.wikipedia.org/wiki/Horosphere) by Wikipedia contributors ([contributor history](https://en.wikipedia.org/wiki/Horosphere?action=history)). Available under [Creative Commons Attribution-ShareAlike 4.0 International](https://creativecommons.org/licenses/by-sa/4.0/). Changes may have been made.
