Kepler–Poinsot polyhedron: Difference between revisions
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== Characteristics == | == 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:{{r|barnes}} | |||
* [[Great dodecahedron]]: constructed from attaching twelve [[pentagonal pyramid]]s (with [[regular polygon]]al faces) onto the face of a regular dodecahedron, and attached again with thirty [[Wedge (geometry)|wedge]]s.{{r|cromwell}} However, this can be constructed alternatively by [[Faceting|removing its polygonal faces without changing or creating new vertices]] of a regular icosahedron.{{r|inchbald}} | |||
* [[Small stellated dodecahedron]]: attaching twelve pentagonal pyramids onto a regular dodecahedron's faces.{{r|kappraff}} [[Topology|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.{{sfnp|Cromwell|1997|p=[https://books.google.com/books?id=OJowej1QWpoC&pg=PA266 266–267]}} | |||
= | [[File:Relationship among regular star polyhedra (direction colors).png|thumb|upright=1.5|Conway's system of relations between the six polyhedra (ordered vertically by [[Density (polytope)|density]]). Here, the green arrow represents the connection of [[Dual polyhedron|duality]], blue represents the greatening (g), and orange represents the stellation (s).{{r|conway-2008}}]] | ||
[[John Horton Conway|John Conway]] introduces operators for the Kepler–Poinsot polyhedra known as ''greatenings''—(g), maintaining the type of faces, shifting and resizing them into parallel planes—and ''stellations''—(s), changing pentagonal faces into pentagrams—of the convex solids. In his [[Stellation#Naming stellations|naming convention]], the small stellated dodecahedron is just the ''stellated dodecahedron''.{{r|conway-2008}} | |||
By the construction above, these figures have [[pentagram]]s (star pentagons) as faces or vertex figures.{{r|barnes}} The [[dual polyhedron]] of a great dodecahedron is the small stellated dodecahedron, and the dual of a great icosahedron is the great stellated dodecahedron.{{r|wenninger}} The four share the symmetry as both regular icosahedron and regular dodecahedron, the [[icosahedral symmetry]].{{r|dubrovin}} | |||
=== 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 characteristic|Euler relation]] | |||
<math display="block">\chi=V-E+F=2\ </math> | |||
does not always hold. Schläfli held that all polyhedra must have χ = 2, and he rejected the small stellated dodecahedron and great dodecahedron as proper polyhedra. This view was never widely held.<ref>{{cite book| first = H. S. M. | last = Coxeter | author-link = Harold Scott MacDonald Coxeter|title=Regular Polytopes|title-link=Regular Polytopes (book)|publisher=Methuen|year=1947|page=[https://books.google.com/books?id=iWvXsVInpgMC&pg=PA114 114]}}</ref> | |||
A modified form of Euler's formula, using [[Density (polytope)|density]] (<math>D</math>) of the [[vertex figure]]s (<math>d_v</math>) and faces (<math>d_f</math>) was given by [[Arthur Cayley]], and holds both for convex polyhedra (where the correction factors are all 1), and the Kepler–Poinsot polyhedra:{{r|huylebrouck}} | |||
<math display="block"> d_v V - E + d_f F = 2D,</math> | |||
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.{{sfnp|Barnes|2012|p=[https://books.google.com/books?id=7YCUBUd-4BQC&pg=PA47 47]}} | |||
A modified form of Euler's formula, using [[Density (polytope)|density]] ( | |||
=== Duality and Petrie polygons === | === Duality and Petrie polygons === | ||
The Kepler–Poinsot polyhedra exist in [[dual polyhedron|dual]] pairs. Duals have the same [[Petrie polygon]], or more precisely, Petrie polygons with the same two dimensional projection. | The Kepler–Poinsot polyhedra exist in [[dual polyhedron|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 compound]]s with the same [[midsphere|edge radius]]. They also show that the Petrie polygons are [[skew polygon|skew]]. | The following images show the two [[dual compound]]s with the same [[midsphere|edge radius]]. They also show that the Petrie polygons are [[skew polygon|skew]]. | ||
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|{5/2, 3}<br />{{CDD|node|3|node|5|rat|d2|node_1}} | |{5/2, 3}<br />{{CDD|node|3|node|5|rat|d2|node_1}} | ||
|12<br />{5/2} | |12<br />{5/2} | ||
|30||20<br />{3}||[[File:Great stellated dodecahedron vertfig. | |30||20<br />{3}||[[File:Great stellated dodecahedron vertfig.svg|80px]]<BR>(5/2)<sup>3</sup> | ||
|[[File:Skeleton GrSt12, Petrie, stick, size m, 5-fold.png|80px]]<br>{10/3} | |[[File:Skeleton GrSt12, Petrie, stick, size m, 5-fold.png|80px]]<br>{10/3} | ||
|2||7||I<sub>h</sub>||great icosahedron | |2||7||I<sub>h</sub>||great icosahedron | ||
|} | |} | ||
== | == History == | ||
{{multiple image | {{multiple image | ||
| | | perrow = 2 | ||
| image1 = | | total_width = 400 | ||
| | | image1 = Marble floor mosaic Basilica of St Mark Vencice.jpg | ||
| image2 = Perspectiva Corporum Regularium 22c.jpg | |||
| image3 = Perspectiva Corporum Regularium MET DP239933, great stellated dodecahedron.jpg | |||
| image4 = Stellated dodecahedra Harmonices Mundi.jpg | |||
| image5 = Sternpolyeder.jpg | |||
| image6 = Alexander's Star.jpg|thumb|Alexander's Star | |||
| footer = Top left to bottom right: floor [[mosaic]] in [[St Mark's Basilica|St Mark's]], [[Venice]], possibly by [[Paolo Uccello]]; [[great dodecahedron]] and [[great stellated dodecahedron]] in ''[[Perspectiva Corporum Regularium]]'' (1568); stellated dodecahedra, ''[[Harmonices Mundi]]'' by [[Johannes Kepler]] (1619); cardboard model of a [[great icosahedron]] from [[University of Tübingen|Tübingen University]] (around 1860); and the [[Alexander's Star]]. | |||
}} | }} | ||
|} | 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]].{{r|coxeter-2013}} | ||
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.{{r|innocenzi|ss}} | |||
|} | |||
The small and great stellated dodecahedra, sometimes called the '''Kepler polyhedra''', were first recognized as regular by [[Johannes Kepler]] around 1619.{{r|coxeter-1999}} He obtained them by [[stellation|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 polyhedron|convex]], as the traditional [[Platonic solid]]s 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 [[stellation|stellating]] the [[Platonic solid]]s,{{r|cauchy}} and almost half a century after that, in 1858, [[Joseph Bertrand|Bertrand]] provided a more elegant proof by [[faceting]] them.{{r|bertrand}} The following year, [[Arthur Cayley]] gave the Kepler–Poinsot polyhedra the names by which they are generally known today.{{r|cayley}} A hundred years later, [[John Horton Conway|John Conway]] developed a [[Stellation#Naming stellations|systematic terminology]] for stellations in up to four dimensions. Within this scheme, the [[small stellated dodecahedron]] is just the ''stellated dodecahedron''.{{r|conway-2008}} | ||
Artist [[M. C. Escher]]'s interest in geometric forms often led to works based on or including regular solids; ''[[Gravitation (M. C. Escher)|Gravitation]]'' is based on a small stellated dodecahedron.{{r|barnes}} A [[Dissection (geometry)|dissection]] of the great dodecahedron was used for the 1980s puzzle [[Alexander's Star]].{{r|alexander's}} Norwegian artist [[Vebjørn Sand#Kepler Star|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#Finite Non-Convex Polytopes - star-polytopes|List of regular polytopes]] | |||
* [[Uniform polyhedron]] | |||
* [[Uniform star polyhedron]] | |||
* [[Polyhedral compound]] | |||
* [[Regular star 4-polytope]] – the ten regular star [[4-polytope]]s, 4-dimensional analogues of the Kepler–Poinsot polyhedra | |||
== References == | |||
{{Reflist|refs= | |||
<ref name=alexander's>{{cite magazine | |||
| url = https://archive.org/details/games-32-1982-October/page/n57/mode/2up | |||
| title = Alexander's star | |||
| magazine = Games | |||
| issue = 32 | |||
| date = October 1982 | |||
| page = 56 | |||
}}</ref> | |||
| | |||
| | |||
| | |||
| | |||
| | |||
| | |||
=== | <ref name=barnes>{{cite book | ||
| last = Barnes | first = John | |||
| year = 2012 | |||
| title = Gems of Geometry | |||
| edition = 2nd | |||
| url = https://books.google.com/books?id=7YCUBUd-4BQC&pg=PA46 | |||
| page = 46 | |||
| publisher = Springer | |||
| doi = 10.1007/978-3-642-30964-9 | |||
| isbn = 978-3-642-30964-9 | |||
}}</ref> | |||
<ref name=bertrand>{{cite journal | |||
| last = Bertrand | first = Joseph | author-link = Joseph Bertrand | |||
| title = Note sur la théorie des polyèdres réguliers | |||
| journal = {{ill|Comptes rendus des séances de l'Académie des Sciences|fr|Comptes rendus des séances de l'Académie des Sciences}} | |||
| volume = 46 | |||
| year = 1858 | |||
| pages = 79–82, 117 | |||
}}</ref> | |||
<ref name=cauchy>{{cite journal | |||
| last = Cauchy | first = Augustin-Louis | author-link = Augustin-Louis Cauchy | |||
| title = Recherches sur les polyèdres | |||
| journal = Journal de l'École polytechnique | |||
| volume = 9 | |||
| pages = 68–86 | |||
| year = 1813 | |||
}}</ref> | |||
{{ | <ref name=cayley>{{cite journal | ||
| last = Cayley | first = Arthur | author-link = Arthur Cayley | |||
| title = On Poinsot's Four New Regular Solids | |||
| journal = Philosophical Magazine | |||
| volume = 17 | |||
| pages = 123–127, 209 | |||
| year = 1859 | |||
}}</ref> | |||
<ref name=conway-2008>{{cite book | |||
| last1 = Conway | first1 = John Horton | |||
| last2 = Burgiel | first2 = Heidi | |||
| last3 = Goodman-Strauss | first3 = Chaim | author-link3 = Chaim Goodman-Strauss | |||
| title = The Symmetry of Things | |||
| isbn = 978-1-56881-220-5 | |||
| year = 2008 | |||
| page = 405 | |||
| publisher = CRC Press | |||
| url = https://books.google.com/books?id=Drj1CwAAQBAJ&pg=PA405 | |||
}} See Figure 26.1, Relationships among the three-dimensional star-polytopes.</ref> | |||
{{ | <ref name=coxeter-1999>{{cite book | ||
| last1 = Coxeter | first1 = H.S.M. | author-link1 = Harold Scott MacDonald Coxeter | |||
| last2 = du Val | first2 = P. | |||
| last3 = Flather | first3 = H.T. | |||
| last4 = Petrie | first4 = J.F. | |||
| title = The Fifty-Nine Icosahedra | |||
| title-link = The Fifty-Nine Icosahedra | |||
| edition = 3rd | |||
| publisher = Tarquin | |||
| year = 1999 | |||
| page = [http://books.google.com/books?id=k13lBwAAQBAJ&pg=PA11 11] | |||
}}</ref> | |||
{| | <ref name=coxeter-2013>{{cite book | ||
| contribution = Regular and semiregular polyhedra | |||
|- | | last = Coxeter | first = H. S. M. | author-link = Harold Scott MacDonald Coxeter | ||
| pages = 41–52 | |||
| title = Shaping Space: Exploring Polyhedra in Nature, Art, and the Geometrical Imagination | |||
| edition = 2nd | |||
| | | editor-first = Marjorie | editor-last = Senechal | editor-link = Marjorie Senechal | ||
| | | publisher = Springer | ||
| | | year = 2013 | ||
| | | doi = 10.1007/978-0-387-92714-5 | ||
|- | | isbn = 978-0-387-92713-8 | ||
| | }} See in particular p. 42.</ref> | ||
| | |||
| | |||
== | <ref name=cromwell>{{cite book | ||
| last = Cromwell | first = Peter | |||
| year = 1997 | |||
| title = Polyhedra | |||
| url = https://books.google.com/books?id=OJowej1QWpoC&pg=PA265 | |||
| page = 265 | |||
| publisher = [[Cambridge University Press]] | |||
| isbn = 978-0-521-66405-9 | |||
}}</ref> | |||
<ref name=dubrovin>{{cite book | |||
| last = Dubrovin | first = Boris | |||
| editor-last = Conte | editor-first = Robert | |||
| year = 1999 | |||
| title = The Painlevé Property: One Century Later | |||
| contribution = Painlevé Transcendents in Two-Dimensional Topological Field Theory | |||
| contribution-url = https://books.google.com/books?id=nBznBwAAQBAJ&pg=PA403 | |||
| page = 403 | |||
| doi = 10.1007/978-1-4612-1532-5 | |||
| isbn = 978-1-4612-1532-5 | |||
}}</ref> | |||
<ref name=huylebrouck>{{cite book | |||
| last = Huylebrouck | first = Dirk | |||
| editor-first1 = Eve | editor-last1 = Torrence | |||
| editor-first2 = Bruce | editor-last2 = Torrence | |||
| editor-first3 = Carlo H. | editor-last3 = Séquin | |||
| editor-first4 = Douglas | editor-last4 = McKenna | |||
| editor-first5 = Kristóf | editor-last5 = Fenyvesi | |||
| editor-first6 = Reza | editor-last6 = Sarhangi | |||
| publisher = Tessellations Publishing | |||
| location = [[Phoenix, Arizona]] | |||
| year = 2016 | |||
| title = Bridges Finland: Mathematics, Music, Art, Architecture, Education, Culture | |||
| contribution-url = https://archive.bridgesmathart.org/2016/bridges2016-263.pdf | |||
| contribution = Euler-Cayley Formula for ‘Unusual’ Polyhedra | |||
}}</ref> | |||
<ref name=inchbald>{{cite journal | |||
| last = Inchbald | first = Guy | |||
| year = 2006 | |||
| title = Facetting Diagrams | |||
| journal = [[The Mathematical Gazette]] | |||
| volume = 90 | issue = 518 | pages = 253–261 | |||
| doi = 10.1017/S0025557200179653 | |||
| jstor = 40378613 | |||
}}</ref> | |||
The | <ref name=innocenzi>{{cite book | ||
| last = Innocenzi | first = Plinio | |||
| year = 2019 | |||
| title = The Innovators Behind Leonardo: The True Story of the Scientific and Technological Renaissance | |||
| url = https://books.google.com/books?id=61diDwAAQBAJ&pg=PA257 | |||
| page = 256–257 | |||
| doi = 10.1007/978-3-319-90449-8 | |||
| isbn = 978-3-319-90449-8 | |||
}}</ref> | |||
{| | <ref name=kappraff>{{cite book | ||
| | | last = Kappraff | first = Jay | ||
| year = 2001 | |||
| title = Connections: The Geometric Bridge Between Art and Science | |||
| edition = 2nd | |||
| | | publisher = [[World Scientific]] | ||
| url = https://books.google.com/books?id=twF7pOYXSTcC&pg=PA309 | |||
| page = 309 | |||
| isbn = 981-02-4585-8 | |||
}}</ref> | |||
| | |||
|- | |||
{| | <ref name=ss>{{cite book | ||
| last1 = Scriba | first1 = Christoph | |||
| | | last2 = Schreiber | first2 = Peter | ||
| | | year = 2015 | ||
| title = 5000 Years of Geometry: Mathematics in History and Culture | |||
| url = https://books.google.com/books?id=6Kp9CAAAQBAJ&pg=PA305 | |||
| page = 305 | |||
| publisher = Springer | |||
| | | doi = 10.1007/978-3-0348-0898-9 | ||
| isbn = 978-3-0348-0898-9 | |||
| | }}</ref> | ||
| | |||
|- | |||
== | <ref name=wenninger>{{cite book | ||
| last = Wenninger | first = Magnus | author-link = Magnus Wenninger | |||
| title = Dual Models | |||
| publisher = [[Cambridge University Press]] | |||
| year = 1983 | |||
| isbn = 0-521-54325-8 | |||
| pages = 39–41 | |||
| url = https://books.google.com/books?id=mfmzUjhs-_8C&pg=PA39 | |||
}}</ref> | |||
}} | }} | ||
* ''Kaleidoscopes: Selected Writings of [[Harold Scott MacDonald Coxeter|H. S. M. Coxeter]]'', edited by F. Arthur Sherk, Peter McMullen, Anthony C. Thompson, Asia Ivic Weiss, Wiley-Interscience Publication, 1995, {{isbn|978-0-471-01003-6}} [http://www.wiley.com/WileyCDA/WileyTitle/productCd-0471010030.html] {{Webarchive|url=https://web.archive.org/web/20160711140441/http://www.wiley.com/WileyCDA/WileyTitle/productCd-0471010030.html |date=2016-07-11 }} | * ''Kaleidoscopes: Selected Writings of [[Harold Scott MacDonald Coxeter|H. S. M. Coxeter]]'', edited by F. Arthur Sherk, Peter McMullen, Anthony C. Thompson, Asia Ivic Weiss, Wiley-Interscience Publication, 1995, {{isbn|978-0-471-01003-6}} [http://www.wiley.com/WileyCDA/WileyTitle/productCd-0471010030.html] {{Webarchive|url=https://web.archive.org/web/20160711140441/http://www.wiley.com/WileyCDA/WileyTitle/productCd-0471010030.html |date=2016-07-11 }} | ||
** (Paper 1) H.S.M. Coxeter, ''The Nine Regular Solids'' [Proc. Can. Math. Congress 1 (1947), 252–264, MR 8, 482] | ** (Paper 1) H.S.M. Coxeter, ''The Nine Regular Solids'' [Proc. Can. Math. Congress 1 (1947), 252–264, MR 8, 482] | ||
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* [[Louis Poinsot]], Memoire sur les polygones et polyèdres. ''J. de l'École Polytechnique'' '''9''', pp. 16–48, 1810. | * [[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 | * Lakatos, Imre; ''Proofs and Refutations'', Cambridge University Press (1976) - discussion of proof of Euler characteristic | ||
* {{cite book | author= Anthony Pugh | date= 1976 | title= Polyhedra: A Visual Approach | publisher= University of California Press Berkeley | location= California | isbn= 0-520-03056-7 }} Chapter 8: Kepler Poisot polyhedra | * {{cite book | author= Anthony Pugh | date= 1976 | title= Polyhedra: A Visual Approach | publisher= University of California Press Berkeley | location= California | isbn= 0-520-03056-7 }} Chapter 8: Kepler Poisot polyhedra | ||
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{{Commons category|Kepler-Poinsot solids}} | {{Commons category|Kepler-Poinsot solids}} | ||
*{{Mathworld | urlname=Kepler-PoinsotSolid | title=Kepler–Poinsot solid }} | *{{Mathworld | urlname=Kepler-PoinsotSolid | title=Kepler–Poinsot solid }} | ||
*[ | *[https://www.software3d.com/Kepler.php Paper models of Kepler–Poinsot polyhedra] | ||
*[ | *[https://www.korthalsaltes.com/cuadros.php?type=k Free paper models (nets) of Kepler–Poinsot polyhedra] | ||
*[ | *[https://www.mathconsult.ch/showroom/unipoly/ The Uniform Polyhedra] | ||
*[http://dmccooey.com/polyhedra/KeplerPoinsot.html Kepler-Poinsot Solids] in Visual Polyhedra | *[http://dmccooey.com/polyhedra/KeplerPoinsot.html Kepler-Poinsot Solids] in Visual Polyhedra | ||
*[http://www.georgehart.com/virtual-polyhedra/kepler-poinsot-info.html VRML models of the Kepler–Poinsot polyhedra] | *[http://www.georgehart.com/virtual-polyhedra/kepler-poinsot-info.html VRML models of the Kepler–Poinsot polyhedra] | ||
*[ | *[https://www.steelpillow.com/polyhedra/StelFacet/history.html Stellation and facetting - a brief history] | ||
*[ | *[https://www.software3d.com/Stella.php Stella: Polyhedron Navigator]: Software used to create many of the images on this page. | ||
{{Nonconvex polyhedron navigator}} | {{Nonconvex polyhedron navigator}} | ||
Latest revision as of 07:19, 14 October 2025
Template:Short description Template:Multiple image In geometry, a Kepler–Poinsot polyhedron is any of four regular star polyhedra.[1]
They may be obtained by stellating 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:Template:R
- 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.Template:R However, this can be constructed alternatively by removing its polygonal faces without changing or creating new vertices of a regular icosahedron.Template:R
- Small stellated dodecahedron: attaching twelve pentagonal pyramids onto a regular dodecahedron's faces.Template:R 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—(g), maintaining the type of faces, shifting and resizing them into parallel planes—and stellations—(s), changing pentagonal faces into pentagrams—of the convex solids. In his naming convention, the small stellated dodecahedron is just the stellated dodecahedron.Template:R
By the construction above, these figures have pentagrams (star pentagons) as faces or vertex figures.Template:R The dual polyhedron of a great dodecahedron is the small stellated dodecahedron, and the dual of a great icosahedron is the great stellated dodecahedron.Template:R The four share the symmetry as both regular icosahedron and regular dodecahedron, the icosahedral symmetry.Template:R
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 = 2, and he rejected the small stellated dodecahedron and great dodecahedron as proper polyhedra. This view was never widely held.[2]
A modified form of Euler's formula, using density () of the vertex figures () and faces () was given by Arthur Cayley, and holds both for convex polyhedra (where the correction factors are all 1), and the Kepler–Poinsot polyhedra:Template:R 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 |
Summary
History
Template: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.Template:R
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.Template:R
The small and great stellated dodecahedra, sometimes called the Kepler polyhedra, were first recognized as regular by Johannes Kepler around 1619.Template:R 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,Template:R and almost half a century after that, in 1858, Bertrand provided a more elegant proof by faceting them.Template:R The following year, Arthur Cayley gave the Kepler–Poinsot polyhedra the names by which they are generally known today.Template:R 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.Template:R
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.Template:R A dissection of the great dodecahedron was used for the 1980s puzzle Alexander's Star.Template:R 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
- 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] Template: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.