Stellation is a process of constructing new polygons (in two dimensions), new polyhedra in three dimensions, or, in general, new polytopes in n dimensions. The process consists of extending elements such as edges or face planes, usually in a symmetrical way, until they meet each other again. The new figure is a stellation of the original.


Kepler's definition

In 1619 Kepler defined stellation for polygons and polyhedra, as the process of extending edges or faces until they meet to form a new polygon or polyhedron. He stellated the dodecahedron to obtain two of the regular star polyhedra (two of the Kepler-Poinsot polyhedra).

Stellated polygons

A stellation of a regular polygon is a regular star polygon or polygonal compound.

A regular star polygon is represented by its Schläfli symbol {n/m}, where n is the number of vertices, m is the step used in sequencing the edges around it, and m and n are co-prime (i.e. have no common divisor). Making m = 1 gives the convex {n}.

If n and m do have a common divisor, then a regular compound can be made. For example {6/2} leads to the regular compound of two triangles {3} or hexagram, while {10/4} leads to a compound of two pentagrams {5/2}.

Some authors use the Schläfli symbol for such regular compounds. Others regard the symbol as indicating a single path which is wound m times around n/m vertex points, such that one edge is superimposed upon another and each vertex point is visited m times. In this case a modified symbol may be used for the compound, for example 2{3} for the hexagram and 2{5/2) for the regular compound of two pentagrams.

A regular n-gon has (n-4)/2 stellations if n is even, and (n-3)/2 stellations if n is odd.

Pentagram green.svg
The pentagram, {5/2}, is the only stellation of a pentagon
The hexagram, {6/2}, the stellation of a hexagon and a compound of two triangles.
Enneagon stellations.png
The enneagon (nonagon) has 3 enneagrammic forms:
{9/2}, {9/3}, {9/4}, with {9/3} being 3 triangles.
Obtuse heptagram.svgAcute heptagram.svg

The heptagon has two heptagrammic forms:
{7/2}, {7/3}

Like the heptagon, the octagon also has two octagrammic stellations, one, {8/3} being a star polygon, and the other, {8/2}, being the compound of two squares.

Stellated polyhedra

First stellation of octahedron.png First stellation of dodecahedron.png Second stellation of dodecahedron.png Third stellation of dodecahedron.png Sixteenth stellation of icosahedron.png First stellation of icosahedron.png Seventeenth stellation of icosahedron.png

The face planes of a polyhedron divide space into many discrete cells. For a symmetrical polyhedron, these cells will fall into groups, or sets, of congruent cells - we say that the cells in such a congruent set are of the same type. A common method of finding stellations involves selecting one or more cell types.

This can lead to a huge number of possible forms, so further criteria are often imposed to reduce the set to those stellations that are significant and unique in some way.

A set of cells forming a closed layer around its core is called a shell. For a symmetrical polyhedron, a shell may be made up of one or more cell types.

Based on such ideas, several restrictive categories of interest have been identified.

  • Main-line stellations. Adding successive shells to the core polyhedron leads to the set of main-line stellations.
  • Fully supported stellations. The underside faces of a cell can appear externally as an "overhang." In a fully supported stellation there are no such overhangs, and all visible parts of a face are seen from the same side.
  • Monoacral stellations. Literally "single-peaked." Where there is only one kind of peak, or vertex, in a stellation (i.e. all vertices are congruent within a single symmetry orbit), the stellation is monoacral. All such stellations are fully supported.
  • Primary stellations. Where a polyhedron has planes of mirror symmetry, edges falling in these planes are said to lie in primary lines. If all edges lie in primary lines, the stellation is primary. All primary stellations are fully supported.
  • Miller stellations. In "The Fifty-Nine Icosahedra" Coxeter, Du Val, Flather and Petrie record five rules suggested by Miller. Although these rules refer specifically to the icosahedron's geometry, they can easily be adapted to work for arbitrary polyhedra. They ensure, among other things, that the rotational symmetry of the original polyhedron is preserved, and that each stellation is different in outward appearance. The four kinds of stellation just defined are all subsets of the Miller stellations.

We can also identify some other categories:

  • A partial stellation is one where not all elements of a given dimensionality are extended.
  • A sub-symmetric stellation is one where not all elements are extended symmetrically.

The Archimedean solids and their duals can also be stellated. Here we usually add the rule that all of the original face planes must be present in the stellation, i.e. we do not consider partial stellations. For example the cube is not considered a stellation of the cuboctahedron. There are:

Seventeen of the nonconvex uniform polyhedra are stellations of Archimedean solids.

Miller's rules

In the book The fifty nine icosahedra, J.C.P. Miller proposed a set of rules for defining which stellation forms should be considered "properly significant and distinct".

These rules have been adapted for use with stellations of many other polyhedra. Under Miller's rules we find:

Many "Miller stellations" cannot be obtained directly by using Kepler's method. For example many have hollow centres where the original faces and edges of the core polyhedron are entirely missing: there is nothing left to be stellated. On the other hand, Kepler's method also yields stellations which are forbidden by Miller's rules since their cells are edge- or vertex-connected, even though their faces are single polygons. This discrepancy received no real attention until Inchbald (2002).

A stellation of the triakis icosahedron

To the right is an example of a stellation. This one is a stellation of a Catalan solid, the triakis icosahedron.

Other rules for stellation

Miller's rules by no means represent the "correct" way to enumerate stellations. They are based on combining parts within the stellation diagram in certain ways, and don't take into account the topology of the resulting faces. As such there are some quite reasonable stellations of the icosahedron that are not part of their list - one was identified by James Bridge in 1974, while some "Miller stellations" are questionable as to whether they should be regarded as stellations at all - one of the icosahedral set comprises several quite disconnected cells floating symmetrically in space.

As yet an alternative set of rules that takes this into account has not been fully developed. Most progress has been made based on the notion that stellation is the reciprocal process to facetting, whereby parts are removed from a polyhedron without creating any new vertices. For every stellation of some polyhedron, there is a dual facetting of the dual polyhedron, and vice versa. By studying facettings of the dual, we gain insights into the stellations of the original. Bridge found his new stellation of the icosahedron by studying the facettings of its dual, the dodecahedron.

Some polyhedronists take the view that stellation is a two-way process, such that any two polyhedra sharing the same face planes are stellations of each other. This is understandable if one is devising a general algorithm suitable for use in a computer program, but is otherwise not particularly helpful.

Many examples of stellations can be found in the list of Wenninger's stellation models.

Stellated polytopes

The stellation process applies to higher dimensional polytopes as well. A stellation diagram of an n-polytope exists in an (n-1)-dimensional hyperplane of a given facet.

For example, in 4-space, the great grand stellated 120-cell is the final stellation of the Regular 4-polytope 120-cell.

Naming stellations

The first systematic naming of stellated polyhedra was Cayley's naming of the regular star polyhedra (nowadays known as the Kepler-Poinsot polyhedra). This system was widely, but not always systematically, adopted for other polyhedra and higher polytopes.

John Conway devised a terminology for stellated polygons, polyhedra and polychora (Coxeter 1974). In this system the process of extending edges to create a new figure is called stellation, that of extending faces is called greatening and that of extending cells is called aggrandizement (this last does not apply to polyhedra). This allows a systematic use of words such as 'stellated', 'great, and 'grand' in devising names for the resulting figures. For example Conway proposed some minor variations to the names of the Kepler-Poinsot polyhedra.

Stellation to infinity

Wenninger noticed that some polyhedra, such as the cube, do not have any finite stellations. The stellation cells are prisms which extend to infinity. The figure comprising these prisms is a stellation to infinity. By most definitions of a polyhedron, these stellations are not strictly polyhedra. They occur as dual polyhedra of the uniform hemipolyhedra.

See also


  • Bridge, N. J.; Facetting the dodecahedron, Acta Crystallographica A30 (1974), pp. 548-552.
  • Coxeter, H.S.M.; Regular complex polytopes (1974).
  • Coxeter, H.S.M.; Du Val, P.; Flather, H. T.; and Petrie, J. F. The Fifty-Nine Icosahedra. Stradbroke, England: Tarquin Publications (1999).
  • Inchbald, G.; In search of the lost icosahedra, The Mathematical Gazette 86 (2002), p.p. 208-215.
  • Messer, P.; Stellations of the rhombic triacontahedron and beyond, Symmetry: culture and science, 11 (2000), pp 201-230.
  • Wenninger, Magnus (1974). Polyhedron Models. Cambridge University Press. ISBN 0-521-09859-9. 
  • Wenninger, Magnus (1983). Dual Models. Cambridge University Press. ISBN 0-521-24524-9. 

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