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Face (geometry)
Face (geometry)
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In solid geometry, a face is a flat surface (a planar region) that forms part of the boundary of a solid object. For example, a cube has six faces in this sense.

In more modern treatments of the geometry of polyhedra and higher-dimensional polytopes, a "face" is defined in such a way that it may have any dimension. The vertices, edges, and (2-dimensional) faces of a polyhedron are all faces in this more general sense.[1]

Polygonal face

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In elementary geometry, a face is a polygon[2] on the boundary of a polyhedron.[1][3] (Here a "polygon" should be viewed as including the 2-dimensional region inside it.) Other names for a polygonal face include polyhedron side and Euclidean plane tile.

For example, any of the six squares that bound a cube is a face of the cube. Sometimes "face" is also used to refer to the 2-dimensional features of a 4-polytope. With this meaning, the 4-dimensional tesseract has 24 square faces, each sharing two of 8 cubic cells.

Regular examples by Schläfli symbol
Polyhedron Star polyhedron Euclidean tiling Hyperbolic tiling 4-polytope
{4,3} {5/2,5} {4,4} {4,5} {4,3,3}

The cube has 3 square faces per vertex.

The small stellated dodecahedron has 5 pentagrammic faces per vertex.

The square tiling in the Euclidean plane has 4 square faces per vertex.

The order-5 square tiling has 5 square faces per vertex.

The tesseract has 3 square faces per edge.

Number of polygonal faces of a polyhedron

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Any convex polyhedron's surface has Euler characteristic

where V is the number of vertices, E is the number of edges, and F is the number of faces. This equation is known as Euler's polyhedron formula. Thus the number of faces is 2 more than the excess of the number of edges over the number of vertices. For example, a cube has 12 edges and 8 vertices, and hence 6 faces.

k-face

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In higher-dimensional geometry, the faces of a polytope are features of all dimensions.[4][5] A face of dimension k is sometimes called a k-face. For example, the polygonal faces of an ordinary polyhedron are 2-faces. The word "face" is defined differently in different areas of mathematics. For example, many but not all authors allow the polytope itself and the empty set as faces of a polytope, where the empty set is for consistency given a "dimension" of −1. For any n-dimensional polytope, faces have dimension with .

For example, with this meaning, the faces of a cube comprise the cube itself (a 3-face), its (square) facets (2-faces), its (line segment) edges (1-faces), its (point) vertices (0-faces), and the empty set.

In some areas of mathematics, such as polyhedral combinatorics, a polytope is by definition convex. In this setting, there is a precise definition: a face of a polytope P in Euclidean space is the intersection of P with any closed halfspace whose boundary is disjoint from the relative interior of P.[6] According to this definition, the set of faces of a polytope includes the polytope itself and the empty set.[4][5] For convex polytopes, this definition is equivalent to the general definition of a face of a convex set, given below.

In other areas of mathematics, such as the theories of abstract polytopes and star polytopes, the requirement of convexity is relaxed. One precise combinatorial concept that generalizes some earlier types of polyhedra is the notion of a simplicial complex. More generally, there is the notion of a polytopal complex.

An n-dimensional simplex (line segment (n = 1), triangle (n = 2), tetrahedron (n = 3), etc.), defined by n + 1 vertices, has a face for each subset of the vertices, from the empty set up through the set of all vertices. In particular, there are 2n + 1 faces in total. The number of k-faces, for k ∈ {−1, 0, ..., n}, is the binomial coefficient .

There are specific names for k-faces depending on the value of k and, in some cases, how close k is to the dimension n of the polytope.

Vertex or 0-face

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Vertex is the common name for a 0-face.

Edge or 1-face

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Edge is the common name for a 1-face.

Face or 2-face

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The use of face in a context where a specific k is meant for a k-face but is not explicitly specified is commonly a 2-face.

Cell or 3-face

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A cell is a polyhedral element (3-face) of a 4-dimensional polytope or 3-dimensional tessellation, or higher. Cells are facets for 4-polytopes and 3-honeycombs.

Examples:

Regular examples by Schläfli symbol
4-polytopes 3-honeycombs
{4,3,3} {5,3,3} {4,3,4} {5,3,4}

The tesseract has 3 cubic cells (3-faces) per edge.

The 120-cell has 3 dodecahedral cells (3-faces) per edge.

The cubic honeycomb fills Euclidean 3-space with cubes, with 4 cells (3-faces) per edge.

The order-4 dodecahedral honeycomb fills 3-dimensional hyperbolic space with dodecahedra, 4 cells (3-faces) per edge.

Facet or (n − 1)-face

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In higher-dimensional geometry, the facets of a n-polytope are the (n − 1)-faces (faces of dimension one less than the polytope itself).[7] A polytope is bounded by its facets.

For example:

Ridge or (n − 2)-face

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In related terminology, the (n − 2)-faces of an n-polytope are called ridges (also subfacets).[8] A ridge is seen as the boundary between exactly two facets of a polytope or honeycomb.

For example:

Peak or (n − 3)-face

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The (n − 3)-faces of an n-polytope are called peaks. A peak contains a rotational axis of facets and ridges in a regular polytope or honeycomb.

For example:

Face of a convex set

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The two distinguished points are examples of extreme points of a convex set that are not exposed points. Therefore, not every face of a convex set is an exposed face.

The notion of a face can be generalized from convex polytopes to all convex sets, as follows. Let be a convex set in a real vector space . A face of is a convex subset such that whenever a point lies strictly between two points and in , both and must be in . Equivalently, for any and any real number such that is in , and must be in .[9]

According to this definition, itself and the empty set are faces of ; these are sometimes called the trivial faces of .

An extreme point of is a point such that is a face of .[9] That is, if lies between two points , then .

For example:

  • A triangle in the plane (including the region inside) is a convex set. Its nontrivial faces are the three vertices and the three edges. (So the only extreme points are the three vertices.)
  • The only nontrivial faces of the closed unit disk are its extreme points, namely the points on the unit circle .

Let be a convex set in that is compact (or equivalently, closed and bounded). Then is the convex hull of its extreme points.[10] More generally, each compact convex set in a locally convex topological vector space is the closed convex hull of its extreme points (the Krein–Milman theorem).

An exposed face of is the subset of points of where a linear functional achieves its minimum on . Thus, if is a linear functional on and , then is an exposed face of .

An exposed point of is a point such that is an exposed face of . That is, for all . See the figure for examples of extreme points that are not exposed.

Competing definitions

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Some authors do not include and/or as faces of . Some authors require a face to be a closed subset; this is automatic for a compact convex set in a vector space of finite dimension, but not in infinite dimensions.[11] In infinite dimensions, the functional is usually assumed to be continuous in a given vector topology.

Properties

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An exposed face of a convex set is a face. In particular, it is a convex subset.

If is a face of a convex set , then a subset is a face of if and only if is a face of .

See also

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References

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Bibliography

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
In , a face of a is a flat, two-dimensional polygonal surface that forms part of the boundary of a three-dimensional solid figure. In the context of , which are three-dimensional shapes composed of polygonal faces joined along edges, each face is itself a —typically a , , , or higher-sided figure—bounded by straight line segments. These faces intersect pairwise along edges and meet at vertices, where at least three edges converge, defining the overall structure of the solid. The number of faces, edges, and vertices in a polyhedron are interrelated through Euler's formula, which states that for any convex polyhedron, the quantity V - E + F = 2, where V is the number of vertices, E the number of edges, and F the number of faces. This relation, discovered by Leonhard Euler in 1752, applies to simple convex polyhedra and highlights the topological consistency of such shapes, excluding more complex cases like those with holes. Faces can be regular (equilateral and equiangular polygons) in symmetric polyhedra, such as the Platonic solids, or regular but of multiple types in more general polyhedra like Archimedean solids, where they meet at each vertex. The concept of faces in geometry traces back to ancient Greek mathematicians, with providing the first systematic classification of polyhedra in his Elements (circa 300 BCE), where he demonstrated that only five regular polyhedra—, , , , and —exist, each with identical regular polygonal faces. These Platonic solids, named after who associated them with the classical elements, laid the foundation for later studies in convexity, , and combinatorial . In modern , the concept of faces extends beyond strict polyhedra to include curved surfaces in solids like cylinders (with circular bases and a curved as faces) and cones, though traditional polyhedral definitions emphasize planarity. The notion generalizes to higher-dimensional polytopes, where faces are lower-dimensional facets known as k-faces.

Faces in Polyhedra

Definition of Polygonal Faces

In , a face of a is defined as a flat, two-dimensional polygonal surface that bounds the solid, typically convex and enclosed by straight edges connecting vertices. These faces form the boundary components of the , ensuring it is a closed three-dimensional without gaps or overlaps. Faces possess specific geometric and topological properties: they are planar, meaning all points lie in a single plane, and constitute simple polygons—closed chains of at least three edges that are connected and free of self-intersections. Each edge of a face is shared precisely by two adjacent faces, maintaining the 's , while every vertex on a face connects to at least three faces to prevent collapse into a lower-dimensional form. Common face types include triangles, quadrilaterals, and pentagons, which must satisfy convexity to ensure the overall remains convex. Representative examples illustrate these properties. In a , each of the four faces is an , providing a minimal convex enclosure. The features twelve regular pentagonal faces, where each is bounded by five equal edges and angles, demonstrating how polygonal faces can vary while adhering to planarity and simplicity. Faces play a central role in for convex polyhedra, which relates the number of vertices VV, edges EE, and faces FF via VE+F=2V - E + F = 2, capturing the topological structure where faces contribute directly to the characteristic count. Historically, the concept of polygonal faces originated with the study of Platonic solids in , where associated these regular polyhedra—each with identical regular polygonal faces—with the classical elements, a framework later formalized by in his Elements.

Enumeration and Formulas for Faces

Euler's polyhedron formula provides a fundamental relation for counting the faces FF of a convex , stating that for any convex , the number of vertices VV, edges EE, and faces FF satisfy VE+F=2V - E + F = 2. This equation holds for simply connected polyhedra of genus 0, equivalent to those topologically equivalent to a . The formula originates from Euler's work in and can be derived using by considering the polyhedron's skeleton as a connected embedded on a , where the χ=VE+F=2\chi = V - E + F = 2 reflects the topology of the surface; each face, including the infinite outer face in the planar embedding, contributes to the count. In topological terms, this generalizes to the for surfaces, as extended by Poincaré, confirming the invariant value of 2 for spherical topology. Specific examples illustrate the formula's application in enumerating faces for regular polyhedra, known as Platonic solids. The has 4 triangular faces, the has 6 square faces, the has 8 triangular faces, the has 12 pentagonal faces, and the has 20 triangular faces. These counts satisfy ; for instance, the icosahedron has V=12V = 12, E=30E = 30, and F=20F = 20, yielding 1230+20=212 - 30 + 20 = 2. The following table summarizes the face counts for the five Platonic solids: For convex polyhedra, inequalities provide bounds on the number of faces relative to other elements. The simplest convex polyhedron is the , establishing a lower bound of F4F \geq 4. Assuming each face is a with at least 3 edges, the for faces implies that the total number of face-edge incidences is at least 3F3F, but since each edge bounds exactly 2 faces, 2E3F2E \geq 3F. Combining this with yields further constraints, such as E3V6E \leq 3V - 6 for planar graphs underlying the , which indirectly limits FF. Schläfli symbols offer a compact notation for classifying regular polyhedra by encoding the structure of their faces and vertex figures. For a regular polyhedron, the symbol {p,q}\{p, q\} indicates that each face is a regular pp-gon and exactly qq faces meet at each vertex. This notation determines the total number of faces; for example, the icosahedron has Schläfli symbol {3,5}\{3, 5\}, signifying triangular faces (p=3p=3) with 5 meeting at each vertex, resulting in 20 faces overall. The symbol facilitates enumeration: the number of faces F=2EpF = \frac{2E}{p}, where EE is derived from vertex and edge relations in the symbol. In dual polyhedra, the faces of one polyhedron correspond directly to the vertices of its dual, preserving combinatorial structure while interchanging these elements. For instance, the , with 6 square faces, is dual to the , which has 6 vertices; conversely, the octahedron's 8 triangular faces correspond to the cube's 8 vertices. This duality, formalized by the principle that vertices and faces trade roles, allows face counts of the original to predict vertex counts of the dual, aiding in and enumeration across pairs like the dodecahedron-icosahedron duality.

k-Faces in Polytopes

General Concept of k-Faces

In the study of polytopes, the of a face generalizes from the polygonal boundaries of three-dimensional polyhedra to higher dimensions. A k-face of an n-dimensional PP is a k-dimensional subpolytope that is the of PP with a , where the touches PP at exactly that subpolytope and PP lies entirely on one side of the . This definition includes the as the (-1)-face and the full as the n-face, ensuring a comprehensive structure for all dimensional elements. In three dimensions, polygonal faces correspond to 2-faces under this framework. The collection of all faces of a , ordered by inclusion, forms a known as the face lattice. This lattice is ranked, with the rank function typically defined as the of the face (or plus one, depending on convention), providing a measure of the hierarchical depth from vertices (0-faces) to the full . Every k-face is contained in some (k+1)-face, establishing an inclusion chain that reflects the polytope's combinatorial ; the face lattice thus captures the incidence relations among all subpolytopes. Examples illustrate this generalization vividly in higher dimensions. Consider the , or 4-cube, a with 8 cubic 3-faces; its 2-faces consist of 24 squares, each serving as the boundary intersection analogous to the faces of a 3D . These 2-faces arise from supporting hyperplanes that slice the tesseract perpendicular to specific directions, yielding square polytopes of dimension 2. Such structures highlight how k-faces maintain the geometric and combinatorial properties of lower-dimensional analogs while embedding in higher-dimensional space. The enumeration of k-faces is quantified by the f-vector of the , defined as (f0,f1,,fn1)(f_0, f_1, \dots, f_{n-1}), where fkf_k denotes the number of k-faces. This vector encodes the polytope's face counts and satisfies certain linear relations; for simplicial polytopes, where all faces are simplices, the Dehn-Sommerville relations impose symmetries on the f-vector components, such as equating the h-numbers hi=hnih_i = h_{n-i} derived from it via inclusion-exclusion transformations. These relations, originally for 3D polyhedra, extend to higher dimensions and constrain possible face configurations.

Dimensional Terminology for Faces

In the context of polytopes, the faces are classified by their dimension kk, where a kk-face is a face of dimension kk in an nn-dimensional . This dimensional terminology provides standard names for these elements, facilitating precise description of polytope structure. A 0-face is termed a vertex, representing the 0-dimensional boundary points of the polytope. These are the discrete points where multiple higher-dimensional faces intersect. A 1-face is called an edge, consisting of line segments that connect pairs of vertices and form the 1-dimensional boundaries between adjacent 2-faces. The 2-face is commonly referred to as a face or surface, denoting the polygonal areas that bound the in three dimensions, as seen in where these are the familiar 2D polygons. In four dimensions, a 3-face is known as a cell or , representing the 3-dimensional components that fill the , analogous to how faces fill a polyhedron. For higher codimensions, the (n1)(n-1)-face is designated a facet, which are the highest-dimensional proper faces that directly bound the nn-polytope, forming its outermost layer. The (n2)(n-2)-face is a ridge, defined as the codimension-2 elements shared by exactly two facets, serving as the intersection lines or surfaces between them. Similarly, the (n3)(n-3)-face is termed a peak, corresponding to codimension-3 elements that lie at the intersections of three or more facets in higher dimensions. As an illustrative example, consider the 4-simplex, the simplest 4-dimensional . Its facets are five tetrahedra, each a 3-face or cell, while its ridges are the ten triangular 2-faces shared between these cells.

Faces in Convex Sets

Definitions and Competing Views

In , a face of a CC is defined as a FCF \subseteq C such that whenever a [x,y]C[x, y] \subseteq C has a point in the relative interior of [x,y][x, y] belonging to FF, the entire segment [x,y][x, y] lies in FF. This condition ensures that FF is "extremal" in the sense that it cannot be crossed by segments interior to CC without fully containing them, generalizing the notion of boundary components in lower-dimensional convex objects. An alternative formulation emphasizes exposed faces, where FF is the intersection of CC with a , meaning there exists a hyperplane HH such that CC lies entirely on one side of HH and F=CHF = C \cap H. Exposed faces are always faces under the primary definition, but the converse does not hold in general, as some faces may not arise from any . The study of convex bodies originated with Hermann Minkowski's foundational work in 1896, in the context of lattice-point problems and volume estimates for bounded convex sets. The modern topological definitions of faces, developed through the mid-20th century in , broaden the notion to include non-exposed faces using relative interior conditions, accommodating infinite-dimensional spaces and non-compact sets. The concept of faces in convex sets was formalized in during the 20th century, with systematic treatments emphasizing the role of faces in optimization and duality theory, building on Minkowski's 1896 monograph Geometrie der Zahlen. Representative examples include extreme points, which serve as 0-dimensional faces (vertices in finite dimensions), as no non-degenerate segment can have its relative interior at such a point without coinciding with it. In unbounded convex sets, such as a closed half-space, the bounding itself acts as a facet (a maximal proper face). These notions specialize to kk-faces in polytopes, where faces are themselves polytopes of kk.

Key Properties and Theorems

Faces of convex sets inherit convexity from the parent set, meaning that any face FF of a convex set CC is itself convex. The of a face FF is defined as the of its affine hull, and faces are categorized by their ranging from 0 (extreme points) to the nn of CC itself, with CC serving as the unique nn-dimensional face. The relative boundary of a face FF consists entirely of lower-dimensional faces of CC, ensuring a hierarchical structure in the facial . The collection of all faces of a CC, ordered by inclusion, forms a lattice known as the face lattice. In this lattice, the meet operation is the of two faces, while the join is the of their union, providing a complete that captures the inclusion relations among faces. Not all faces are exposed; an exposed face is the of CC with a , but pathological convex sets in infinite-dimensional spaces can have non-exposed faces that are not obtainable this way. In finite dimensions, non-exposed faces can still exist. The Krein-Milman theorem states that a compact in a locally convex is the closed of its extreme points, which are precisely the 0-dimensional faces. This theorem underscores the foundational role of extreme points in representing the entire set. Carathéodory's theorem asserts that if CC is a in Rd\mathbb{R}^d, then every point in CC lies in the of at most d+1d+1 points from CC, directly linking the of faces to the minimal number of affinely independent points needed to span them. For example, in the as a 3-dimensional , the 0-faces are the 8 vertices, the 1-faces are the 12 edges, the 2-faces are the 6 square facets, and the full 3-face is the itself, illustrating the dimensional and lattice structure.

References

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