Kepler–Poinsot polyhedron
Template:Short description Script error: No such module "Multiple image". In geometry, a Kepler–Poinsot polyhedron is any of four regular star polyhedra.[1]
They may be obtained by stellating and faceting the regular convex dodecahedron and icosahedron, and differ from these in having regular pentagrammic faces or vertex figures. They can all be seen as three-dimensional analogues of the pentagram in one way or another.
Characteristics
The Kepler–Poinsot polyhedra are the regular star polyhedra, obtained by extending both regular icosahedron and regular dodecahedron, an operation named stellation. This operation results in four different polyhedra:[2]Template:R/superscript
- Great dodecahedron: constructed from attaching twelve pentagonal pyramids (with regular polygonal faces) onto the face of a regular dodecahedron, and attached again with thirty wedges.[3]Template:R/superscript However, this can be constructed alternatively by removing its polygonal faces without changing or creating new vertices of a regular icosahedron.[4]Template:R/superscript
- Small stellated dodecahedron: attaching twelve pentagonal pyramids onto a regular dodecahedron's faces.[5]Template:R/superscript Topologically, this shares the same surface as the pentakis dodecahedron.
- Great icosahedron; and
- Great stellated dodecahedron: constructed from a great dodecahedron with twenty asymmetric triangular bipyramids, attaching to the hollow between the wedges.Template:Sfnp
John Conway introduces operators for the Kepler–Poinsot polyhedra known as greatenings—(gScript error: No such module "Check for unknown parameters".), maintaining the type of faces, shifting and resizing them into parallel planes—and stellations—(sScript error: No such module "Check for unknown parameters".), changing pentagonal faces into pentagrams—of the convex solids. In his naming convention, the small stellated dodecahedron is just the stellated dodecahedron.[6]Template:R/superscript
By the construction above, these figures have pentagrams (star pentagons) as faces or vertex figures.[2]Template:R/superscript The dual polyhedron of a great dodecahedron is the small stellated dodecahedron, and the dual of a great icosahedron is the great stellated dodecahedron.[7]Template:R/superscript The four share the symmetry as both regular icosahedron and regular dodecahedron, the icosahedral symmetry.[8]Template:R/superscript
Euler characteristic
A Kepler–Poinsot polyhedron covers its circumscribed sphere more than once, with the centers of faces acting as winding points in the figures which have pentagrammic faces, and the vertices in the others. Because of this, they are not necessarily topologically equivalent to the sphere as Platonic solids are, and in particular, the Euler relation does not always hold. Schläfli held that all polyhedra must have χ = 2Script error: No such module "Check for unknown parameters"., and he rejected the small stellated dodecahedron and great dodecahedron as proper polyhedra. This view was never widely held.[9]
A modified form of Euler's formula, using density (Template:Mvar) of the vertex figures (Template:Mvar) and faces (Template:Mvar) was given by Arthur Cayley, and holds both for convex polyhedra (where the correction factors are all 1), and the Kepler–Poinsot polyhedra:[10]Template:R/superscript and by this calculation, the density of the great icosahedron and the great stellated dodecahedron are 7, whereas the great dodecahedron and the small stellated dodecahedron are 3.Template:Sfnp
Duality and Petrie polygons
The Kepler–Poinsot polyhedra exist in dual pairs. Duals have the same Petrie polygon, or more precisely, Petrie polygons with the same two-dimensional projection.
The following images show the two dual compounds with the same edge radius. They also show that the Petrie polygons are skew. Two relationships described in the article below are also easily seen in the images: That the violet edges are the same, and that the green faces lie in the same planes.
| horizontal edge in front | vertical edge in front | Petrie polygon |
|---|---|---|
| small stellated dodecahedron | great dodecahedron | hexagon |
| great icosahedron | great stellated dodecahedron | decagram |
|
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Summary
| Name (Conway's abbreviation) |
Picture | Spherical tiling |
Stellation diagram |
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Vertex figure (config.) |
Petrie polygon | χ | Density | Symmetry | Dual |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| great dodecahedron (gDScript error: No such module "Check for unknown parameters".) |
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| small stellated dodecahedron (sDScript error: No such module "Check for unknown parameters".) |
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| great icosahedron (gIScript error: No such module "Check for unknown parameters".) |
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| great stellated dodecahedron (sgD = gsDScript error: No such module "Check for unknown parameters".) |
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History
Script error: No such module "Multiple image". Most, if not all, of the Kepler–Poinsot polyhedra were known of in some form or other before Kepler. A small stellated dodecahedron appears in a marble tarsia (inlay panel) on the floor of St. Mark's Basilica, Venice, Italy. It dates from the 15th century and is sometimes attributed to Paolo Uccello.[11]Template:R/superscript
In his Perspectiva corporum regularium, a book of woodcuts published in 1568, Wenzel Jamnitzer depicts the great stellated dodecahedron and a great dodecahedron. It is clear from the general arrangement of the book that he regarded only the five Platonic solids as regular.[12]Template:R/superscript[13]Template:R/superscript
The small and great stellated dodecahedra, sometimes called the Kepler polyhedra, were first recognized as regular by Johannes Kepler around 1619.[14]Template:R/superscript He obtained them by stellating the regular convex dodecahedron, for the first time treating it as a surface rather than a solid. He noticed that by extending the edges or faces of the convex dodecahedron until they met again, he could obtain star pentagons. Further, he recognized that these star pentagons are also regular. In this way, he constructed the two stellated dodecahedra. Each has the central convex region of each face "hidden" within the interior, with only the triangular arms visible. Kepler's final step was to recognize that these polyhedra fit the definition of regularity, even though they were not convex, as the traditional Platonic solids were.
In 1809, Louis Poinsot rediscovered Kepler's figures by assembling star pentagons around each vertex. He also assembled convex polygons around star vertices to discover two more regular stars, the great icosahedron and great dodecahedron. Some people call these two the Poinsot polyhedra. Poinsot did not know if he had discovered all the regular star polyhedra. Three years later, Augustin Cauchy proved the list complete by stellating the Platonic solids,[15]Template:R/superscript and almost half a century after that, in 1858, Bertrand provided a more elegant proof by faceting them.[16]Template:R/superscript The following year, Arthur Cayley gave the Kepler–Poinsot polyhedra the names by which they are generally known today.[17]Template:R/superscript A hundred years later, John Conway developed a systematic terminology for stellations in up to four dimensions. Within this scheme, the small stellated dodecahedron is just the stellated dodecahedron.[6]Template:R/superscript
Artist M. C. Escher's interest in geometric forms often led to works based on or including regular solids; Gravitation is based on a small stellated dodecahedron.[2]Template:R/superscript A dissection of the great dodecahedron was used for the 1980s puzzle Alexander's Star.[18]Template:R/superscript Norwegian artist Vebjørn Sand's sculpture The Kepler Star is displayed near Oslo Airport, Gardermoen. The star spans 14 meters and consists of both a regular icosahedron and a regular dodecahedron inside a great stellated dodecahedron.
See also
- Regular polytope
- Regular polyhedron
- List of regular polytopes
- Uniform polyhedron
- Uniform star polyhedron
- Polyhedral compound
- Regular star 4-polytope – the ten regular star 4-polytopes, 4-dimensional analogues of the Kepler–Poinsot polyhedra
References
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- ↑ Coxeter, Star polytopes and the Schläfli function f(α,β,γ) p. 121 1. The Kepler–Poinsot polyhedra
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- ↑ a b c Script error: No such module "citation/CS1". See Figure 26.1, Relationships among the three-dimensional star-polytopes.
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- Kaleidoscopes: Selected Writings of H. S. M. Coxeter, edited by F. Arthur Sherk, Peter McMullen, Anthony C. Thompson, Asia Ivic Weiss, Wiley-Interscience Publication, 1995, Template:Isbn [1] Script error: No such module "webarchive".
- (Paper 1) H.S.M. Coxeter, The Nine Regular Solids [Proc. Can. Math. Congress 1 (1947), 252–264, MR 8, 482]
- (Paper 10) H.S.M. Coxeter, Star Polytopes and the Schlafli Function f(α,β,γ) [Elemente der Mathematik 44 (2) (1989) 25–36]
- Theoni Pappas, (The Kepler–Poinsot Solids) The Joy of Mathematics. San Carlos, CA: Wide World Publ./Tetra, p. 113, 1989.
- Louis Poinsot, Memoire sur les polygones et polyèdres. J. de l'École Polytechnique 9, pp. 16–48, 1810.
- Lakatos, Imre; Proofs and Refutations, Cambridge University Press (1976) - discussion of proof of Euler characteristic
- Script error: No such module "citation/CS1". Chapter 8: Kepler Poisot polyhedra
External links
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- Paper models of Kepler–Poinsot polyhedra
- Free paper models (nets) of Kepler–Poinsot polyhedra
- The Uniform Polyhedra
- Kepler-Poinsot Solids in Visual Polyhedra
- VRML models of the Kepler–Poinsot polyhedra
- Stellation and facetting - a brief history
- Stella: Polyhedron Navigator: Software used to create many of the images on this page.
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