# Difference between revisions of "Hyperbolic Geometry"

The McDonnell Planetarium at the St. Louis Science Center.

## Explorations

You may begin exploring hyperbolic geometry with the following explorations. We recommend doing some or all of the basic explorations before reading the section. Gaining some intuition about the nature of hyperbolic space before reading this section will be more effective in the long run.

Basic Explorations

Further explorations that help give a better understanding of hyperbolic geometry.

## Hyperbolic Space

We have seen two different geometries so far: Euclidean and spherical geometry. Geometry is meant to describe the world around us, and the geometry then depends on some fundamental properties of the world we are describing. Objects that live in a flat world are described by Euclidean (or flat) geometry, while objects that live on a spherical world will need to be described by spherical geometry.

In two dimensions there is a third geometry. This geometry is called hyperbolic geometry. If Euclidean geometry describes objects in a flat world or a plane, and spherical geometry describes objects on the sphere, what world does hyperbolic geometry describe? Like spherical geometry, which takes place on a sphere, hyperbolic geometry takes place on a curved two dimensional surface called hyperbolic space.

We will describe hyperbolic space in several different ways. In Escher's work, hyperbolic space is a distorted disk. All of the angels in Circle Limit IV (Heaven and Hell) live in hyperbolic space, where they are actually the same size, as do the devil figures. The image that Escher presents is a distorted map of the hyperbolic world.

You can explore Escher's hyperbolic Circle Limit prints and get an introduction to hyperbolic geometry in the Escher's Circle Limit Exploration

## Models of Hyperbolic Space

On a sphere, a small neighborhood of a point looks like a cap. In hyperbolic space, every point looks like a saddle:

A piece of a sphere A piece of hyperbolic space

Unfortunately, while you can piece caps together to make a sphere, piecing saddles together quickly runs out of space. Try this yourself with the Hyperbolic Paper Exploration.

Hyperbolic paper

Hyperbolic paper is a floppy, saddle like object. Eventually, it contains too many triangles in too small a space to continue any further, although most people and run out of patience before running out of room. It's also possible to crochet models of hyperbolic space.

Because globes are unwieldy, navigators use flat maps of the spherical earth. Maps of the Earth are necessarily distorted, for example Greenland appears extremely large on the common Mercator map of the Earth, shown with red dots to indicate the distortion of area.

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Mercator projection map with equal area dots.

### Poincare Disk Model

Because models of hyperbolic space are unwieldy (not to mention infinite), we will do all of our work with a map of hyperbolic space called the Poincaré disk. The Poincaré disk is the inside of a circle (although the circle is not included) and is badly distorted near its edge.

Objects near the edge of the Poincaré disk are larger than they appear.

Hyperbolic man takes a walk

The picture shows a stick man as he walks towards the edge of the disk. He appears to shrink, as does the distance he moves with each step. But this disk is a distorted map, and in the actual hyperbolic space his steps are all the same length and he stays the same size. The man will never reach the edge of the disk, because it is infinitely far away. The edge is drawn dashed because it is not actually part of hyperbolic space.

The geodesics in hyperbolic space play the role of straight lines. Geodesics appear straight to an inhabitant of hyperbolic space, and they are the shortest paths between points. In the Poincaré disk model, geodesics appear curved. They are arcs of circles. Specifically:

Geodesics are arcs of circles which meet the edge of the disk at 90°.

Geodesics which pass through the center of the disk appear straight.

Geodesics in the Poincaré disk

Practice drawing geodesics in the Poincaré disk with Hyperbolic Geometry Exploration.

### Upper Half Space Model

Hyperbolic triangle in Upper Half Space Model. From a Roman mosaic, Real Alcazar, Cordoba, Spain

Another commonly used model for Hyperbolic space in the Upper Half Space Model. Hyperbolic 2-space for instance can be thought of as lying in the plane. The model includes all points (x,y) where y>0. The geodesics in this pace are lines perpendicular to the x-axis and semi-circles perpendicular to the x-axis.

Non-Euclid also allows the user to experiment with this model of hyperbolic space.

### Other Models

There are several other models that can be used to represent hyperbolic space. The Pseudo-sphere for instance is often used as a model to illustrate a 2-dimensional space with negative curvature.

The Beltrami-Klein Model represent hyperbolic space as the interior of a disk, just as the Poincare disk model, but geodesics are different.

There are more models besides the ones mentioned here, but we will not list all of them.

## Polygons and Defect

Polygon
A polygon in hyperbolic geometry is a sequence of points and geodesic segments joining those points. The geodesic segments are called the sides of the polygon.

A triangle in hyperbolic geometry is a polygon with three sides, a quadrilateral is a polygon with four sides, and so on, as in Euclidean geometry. Here are some triangles in hyperbolic space:

From these pictures, you can see that:

The sum of the angles in any hyperbolic triangle is less than 180°.

Defect
The defect of a hyperbolic triangle is 180° – (angle sum of the triangle).

By cutting other polygons into triangles, we see that a hyperbolic polygon has angle sum less than that of the corresponding Euclidean polygon.

Define the defect for a hyperbolic polygon with $n$ sides to be $(n - 2)\times180^\circ - (angle sum of the polygon)$.

Putting this together with the defect in spherical geometry:

The defect of a polygon is the difference between its angle sum and the angle sum for a Euclidean polygon with the same number of sides.

This statement works in spherical and hyperbolic geometry, for polygons with any number of sides. It even works for biangles, because a biangle in Euclidean geometry must have two 0° angles. The area of a hyperbolic polygon is still proportional to its defect:

Area of a hyperbolic polygon = $\frac{\pi}{180^\circ}\times defect$.

This equality is a special case of the Gauss-Bonnet theorem.

In spherical geometry, we had a formula relating the defect of a polygon to the fraction of the sphere's area covered by the polygon. For a sphere of radius 1, the total surface area of the sphere is $4\pi$, and so the area of a polygon is $4\pi \times \frac{defect}{720^\circ}$ which (after a little simplification) is exactly the same formula as in hyperbolic space!

### Ideal Polygons

Ideal Triangle
An ideal triangle consists of three geodesics that touch at the boundary of the Poincaré disk.

The three geodesics are called the sides of the ideal triangle. Since the boundary of the disk isn’t part of hyperbolic space, the sides of an ideal triangle are infintely long and never actually meet. However, the do get closer together as they head towards the edge. The three points on the boundary are called the ideal vertices of the ideal triangle, and play a similar role as the vertices of an ordinary triangle. Since the sides are all perpendicular to the Poincaré disk boundary, they make an angle of 0° with each other.

You can create other ideal polygons in a similar manner:

 Ideal triangles and an ideal hexagon

The area formula implies that any ideal triangle has area $\pi$, because the angle sum is zero and its defect is 180°. Both ideal triangles shown above have the same area even though the distortion of the Poincaré disk makes one look much smaller than the other. The ideal hexagon shown has angle sum zero, so it’s defect is 720° and its area is $4\pi$.

## Hyperbolic Tessellations

A hyperbolic tessellation is a covering of hyperbolic space by tiles, with no overlapping tiles and no gaps. Escher’s Circle Limit prints are examples of hyperbolic tessellations. Like his other tessellations, Escher began with a geometric tessellation by polygons and worked from there.

Consider Escher’s Circle Limit I, shown with geometric scaffolding consisting of geodesics drawn in red:

The spines of the fish, emphasized with red lines, form a tessellation of hyperbolic space by quadrilaterals. Since these quadrilaterals meet four or six at a vertex, they have corner angles 90°-60°-90°-60°. They are not regular polygons because regular polygons have all sides and all angles equal.

There are plenty of other tessellations of hyperbolic space, including regular tessellations. In fact, there are infinitely many regular tessellations of hyperbolic space. This stands in sharp contrast to Euclidean space, which has only three, and to spherical geometry, where there are only five non-degenerate possibilities (corresponding to the Platonic solids). Hyperbolic space is easy to tessellate because the corner angles of polygons want to be small, and small angles fit nicely around a vertex.

As in the other two geometries, we describe regular tessellations by the number of sides in each polygon and the number of polygons that meet at a vertex.

Schläfli Symbol
The Schläfli symbol $\{n,k\}$ describes the regular tessellation by $n$-gons where $k$ meet at each vertex.

### Examples

This tessellation has seven triangles at each vertex, and so its Schläfli symbol is {3,7}.

The triangles have

360°/7 ≈51.4°

angles and angle sums of approximately

3×51.4°=154.3°

This gives a defect of approximately 180°–154.3° = 25.7° and an area of approximately 0.45.

This tessellation has four pentagons at each vertex, and so its Schläfli symbol is {5,4}.

Each pentagon has five 90° angles.

The angle sum for each pentagon is 450°.

Since Euclidean pentagons have angle sum 540°, these pentagons have a defect of 540°-450° = 90° and an area of approximately 1.57.

### Escher's Circle Limit III

M.C. Escher, Circle Limit III, 1959.

Escher's Circle Limit III is his most accomplished print based on hyperbolic space. It is also his most subtle.

Looking at the white spines of the fish, it appears to be a tessellation of hyperbolic space by triangles and squares, with three triangles and three squares coming together at each vertex. This would mean that the corner angles of both polygons are 60° each, but this gives the triangle an angle sum of 180°, which cannot happen in hyperbolic space!

However, Circle Limit III clearly has the flavor of a hyperbolic tessellation. H.S.M Coxeter, a mathematician and friend of Escher’s analyzed the print[1], and discovered that the white circular arcs along the spines meet the boundary of the disk at 80° each, rather than the 90° required to be geodesic. Since the white lines are not geodesics, neither the “triangle” or the “square” is really a polygon at all! Even Escher does not seem to have realized this, although most probably he would not have cared, as he was very satisfied with the print and the suggestion of infinity it presents.

A natural underlying tessellation for Circle Limit III is the {8,3} tessellation by octagons:

A re-creation of Circle Limit III[2]
A geodesic and two (non-geodesic) curves at equal distance from the geodesic.

The image on the right shows a hyperbolic geodesic that runs through the midpoints of the sides of the octagons, surrounded by two curves (not geodesics) at a fixed distance from the geodesic. The rightmost of these curves forms the spines of one row of fish in Circle Limit III.

In general hyperbolic tessellations would take quite a bit of work. There is a special type of tesseallation - those made up of ideal polygons - that are easier to construct. These tessellations are introduce in the Ideal Hyperbolic Tessellations Exploration.

## Notes

1. Coxeter, H.S.M. "The Non-Euclidean Symmetry of Escher's Picture 'Circle Limit III'". Leonardo Vol. 12 No. 1, 1979, pg 19-25.
2. Dunham, D. "More 'Circle Limit III' patterns". Proceedings of Bridges 2006 pg 451.
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