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Parallelepiped

A parallelepiped is a three-dimensional formed by six faces, where opposite faces are congruent and parallel, analogous to a in two dimensions. It can be conceptualized as the set of all points obtained by linear combinations of three linearly independent vectors originating from a common , thus spanning a in . This geometric figure generalizes the rectangular box (or ) and appears in classical as described in Euclid's Elements, Book XI, where it serves as a fundamental prism-like solid with parallelogram bases. Parallelepipeds are classified into several types based on the shapes of their faces and the angles between edges. A rectangular parallelepiped, also known as a cuboid or rectangular prism, has all six faces as rectangles, with edges meeting at right angles. In contrast, a rhombohedron features six congruent rhombic faces, where all edges are of equal length, and a general parallelepiped (or oblique parallelepiped) has arbitrary parallelogram faces without such symmetries. Special cases include the cube, a rectangular parallelepiped with square faces, and the right parallelepiped, where lateral edges are perpendicular to the base. These variations highlight the parallelepiped's flexibility in modeling skewed or sheared three-dimensional structures. Key properties of a parallelepiped include its , which for vectors \vec{u}, \vec{v}, \vec{w} defining its edges from one is the of the scalar |\vec{u} \cdot (\vec{v} \times \vec{w})|, equivalent to the of the matrix formed by these vectors as columns. This underscores its role in linear algebra, where the parallelepiped represents the "unit cell" spanned by basis , and in applications such as for describing lattice structures. Additionally, the surface area consists of the sum of the areas of its six faces, each computed as base times height or via vector cross products. Parallelepipeds also exhibit along their edges, making them essential in geometry and for integrals over oriented volumes.

Definition and Fundamentals

Definition

A parallelepiped is a three-dimensional geometric figure formed by six parallelogram faces, consisting of three pairs of identical and parallel faces. This structure arises as a prism with parallelogrammatic bases, where opposite faces are congruent and parallel, ensuring the figure maintains along its defining directions. The extends the concept of a two-dimensional into three dimensions, much like a generalizes a square. In this analogy, just as a is bounded by two pairs of parallel sides, the parallelepiped is delimited by three such pairs of faces, creating a solid that can be generated by translating a along a third direction not coplanar with the first two. It possesses 6 faces, all parallelograms; 12 edges, with four edges meeting at each in a consistent manner; and 8 vertices, where three edges converge. As a fundamental , the parallelepiped is inherently , meaning that the line segment connecting any two points within the figure lies entirely inside it, and it qualifies as a polyhedral solid with planar faces and straight edges. This underpins its role as a basic building block in three-dimensional , serving as a prerequisite for exploring more advanced properties and constructions.

Vector Representation

A parallelepiped can be formally constructed in three-dimensional using vector geometry, starting from a fixed point O and three emanating \mathbf{a}, \mathbf{b}, and \mathbf{c} that are not coplanar. These define the edges originating from O, and the parallelepiped is the of the eight points formed by their linear combinations with coefficients 0 or 1. The vertices of the parallelepiped are precisely: O, \mathbf{a}, \mathbf{b}, \mathbf{c}, \mathbf{a} + \mathbf{b}, \mathbf{a} + \mathbf{c}, \mathbf{b} + \mathbf{c}, and \mathbf{a} + \mathbf{b} + \mathbf{c}. This set of points ensures that opposite faces are identical parallelograms, with edges parallel to the defining vectors. Any point within or on the of the parallelepiped can be represented parametrically as a position vector \mathbf{r} = u \mathbf{a} + v \mathbf{b} + w \mathbf{c}, where the parameters satisfy $0 \leq u, v, w \leq 1. This parameterization describes the solid as the image of the unit under the linear with columns \mathbf{a}, \mathbf{b}, and \mathbf{c}. The edges of the parallelepiped consist of three sets of four edges each, with lengths given by the magnitudes |\mathbf{a}|, |\mathbf{b}|, and |\mathbf{c}|, corresponding to the directions of the defining vectors. The six faces are pairwise parallelograms, each spanned by a pair of the defining vectors: one pair by \mathbf{a} and \mathbf{b}, another by \mathbf{a} and \mathbf{c}, and the third by \mathbf{b} and \mathbf{c}. These faces meet at the vertices, forming the closed surface of the parallelepiped.

Properties

Geometric Properties

A parallelepiped has six faces, each a , twelve edges, and eight vertices. Opposite faces are congruent and parallel, forming three pairs of identical faces. It is a type of zonohedron, generated as the Minkowski sum of three line segments in different directions.

Symmetry and Tessellation

A general parallelepiped possesses symmetry C_i, which consists solely of the and inversion operations through its . This inversion arises because the parallelepiped's opposite faces are equal parallelograms, ensuring that the figure maps onto itself under central inversion. In special cases, such as when edges are orthogonal or faces are regular polygons, the symmetry elevates to higher point groups, but the generic form retains only this minimal symmetry. The parallelepiped admits translations along its edge directions, allowing identical copies to be shifted uniformly along the three directions defined by its edge vectors to form a periodic structure. These translations form the basis of periodic repetition in three dimensions, where each shift corresponds to one of the primitive vectors spanning the figure. This translational property enables the parallelepiped to tessellate three-dimensional completely, filling it without gaps or overlaps through successive translations along its edge directions. Such space-filling behavior is fundamental to periodic arrangements, as congruent parallelepipeds can replicate indefinitely to cover the entire volume. In , the parallelepiped serves as the unit cell for crystal , particularly in the triclinic system, where it encapsulates the minimal repeating volume that generates the full via translations. All 14 Bravais can be described using parallelepiped unit cells, with the general form corresponding to the lowest-symmetry triclinic .

Geometric Quantities

Volume

The volume of a parallelepiped, defined by three vectors \mathbf{a}, \mathbf{b}, and \mathbf{c} emanating from a common , is given by the of the :
V = |\mathbf{a} \cdot (\mathbf{b} \times \mathbf{c})|.
This formula arises from the geometric interpretation of the parallelepiped as a prism with a parallelogram base spanned by \mathbf{b} and \mathbf{c}, extruded along \mathbf{a}. The area of the base parallelogram is the magnitude of the cross product \|\mathbf{b} \times \mathbf{c}\|, which provides a vector normal to the base plane. The height is then the projection of \mathbf{a} onto this normal direction, computed as the of the dot product \mathbf{a} \cdot (\mathbf{b} \times \mathbf{c}) / \|\mathbf{b} \times \mathbf{c}\|. Multiplying the base area by this height yields V = |\mathbf{a} \cdot (\mathbf{b} \times \mathbf{c})|, where the ensures a positive volume regardless of the vectors' orientation.
An equivalent expression uses the determinant of the matrix M formed by \mathbf{a}, \mathbf{b}, and \mathbf{c} as its columns:
V = |\det(M)|.
The scalar triple product equals the \det(M), linking the volume directly to linear algebra properties; the absolute value again accounts for signed , with the magnitude representing the unsigned volume. This formulation generalizes to higher dimensions via the determinant's role in computing the volume of parallelotopes.
If the vectors are measured in units of (e.g., meters), the volume V has units of cubic (e.g., cubic meters). Furthermore, under uniform of all linear dimensions by a factor k > 0, the volume scales by k^3, as the of the scaled is k^3 \det(M).

Surface Area

The total surface area of a parallelepiped is the sum of the areas of its six parallelogram faces, with opposite faces being congruent and parallel. Given three edge vectors \mathbf{a}, \mathbf{b}, and \mathbf{c} emanating from a common , the three pairs of opposite faces are spanned by (\mathbf{a}, \mathbf{b}), (\mathbf{a}, \mathbf{c}), and (\mathbf{b}, \mathbf{c}), respectively. The area of each parallelogram face is the of the of its spanning vectors, as this equals the area of the parallelogram they form. Thus, the total surface area A is given by A = 2 \left( |\mathbf{a} \times \mathbf{b}| + |\mathbf{a} \times \mathbf{c}| + |\mathbf{b} \times \mathbf{c}| \right), where the factor of 2 accounts for the two faces in each pair. Equivalently, in terms of the edge lengths a = |\mathbf{a}|, b = |\mathbf{b}|, c = |\mathbf{c}| and the angles between them—denoted \gamma as the angle between \mathbf{a} and \mathbf{b}, \beta as the angle between \mathbf{a} and \mathbf{c}, and \alpha as the angle between \mathbf{b} and \mathbf{c}—the formula becomes A = 2 \left( ab \sin \gamma + ac \sin \beta + bc \sin \alpha \right). This follows directly from the cross product magnitude |\mathbf{u} \times \mathbf{v}| = uv \sin \theta, where \theta is the angle between \mathbf{u} and \mathbf{v}. These angles \alpha, \beta, and \gamma are the angles at the vertex between the respective pairs of edges.

Special Cases

Special Cases by Symmetry

Special cases of parallelepipeds with higher symmetry include the rectangular parallelepiped (or ), where all faces are rectangles and edges meet at right angles; the , with all six faces congruent rhombi and equal edge lengths; and the , a special rhombohedron with square faces and 90-degree angles. These cases exhibit increased symmetry compared to the general parallelepiped.

Perfect Parallelepiped

A perfect parallelepiped is defined as a parallelepiped with integer edge lengths a, b, and c, where the face diagonals—such as \sqrt{a^2 + b^2 + 2ab \cos \gamma} for the face formed by edges a and b with included angle \gamma, and analogous expressions for the other faces—are integers, and the space diagonals—such as \sqrt{a^2 + b^2 + c^2 + 2ab \cos \gamma + 2ac \cos \beta + 2bc \cos \alpha}, with \alpha, \beta, \gamma the angles between the respective edges—are also integers. This condition requires solving a system of Diophantine equations derived from the vector representations of the edges, ensuring all relevant norms and sums/differences of edge vectors yield integer lengths. The smallest known perfect parallelepiped has edge lengths 103, 106, and 271, with all face and space diagonals integers, including minor face diagonals of 101, 266, and 255, major face diagonals of 183, 312, and 323, and space diagonals of 272, 278, 300, and 374. This example, which is (with coprime edge lengths), was discovered in 2009 through computational brute-force searches by Jorge Sawyer and Clifford Reiter, resolving an open question posed by Richard Guy. Their work identified dozens of primitive perfect parallelepipeds, some with up to two rectangular faces. Subsequent has established the of an of dissimilar perfect parallelepipeds, each with two nonparallel rectangular faces, further expanding the known solutions to these Diophantine systems. Despite extensive computational searches since 2009, no smaller perfect parallelepiped than the one with edges 103, 106, and 271 has been found as of November 2025, leaving open questions about the minimal possible edge lengths and potential additional constraints like integer volumes.

Generalizations and Applications

Parallelotope

A parallelotope is the n-dimensional analogue of a parallelepiped, defined as the set of all points that are linear combinations of n linearly independent vectors in n-dimensional Euclidean space.

Applications

Rectangular parallelepipeds are prevalent in everyday objects, including matchboxes, bricks, shoeboxes, books, and mobile phones, where their right-angled edges facilitate efficient packaging and construction. In physics and , the scalar triple product of vectors defining a parallelepiped's edges is used to compute volumes in applications such as simulations and material stress analysis, providing a measure of enclosed space for modeling deformations or flow rates. In , the unit cell of crystals with low symmetry, such as triclinic and monoclinic systems, is modeled as an oblique parallelepiped, where the three non-coplanar edges represent vectors that tile the . In , oriented bounding parallelepipeds serve as efficient bounding volumes for complex 3D models, accelerating ray-tracing and by enclosing objects with minimal overlap. In , the parallelepiped classifier segments multispectral image data by defining class boundaries as multidimensional boxes in spectral space, enabling supervised categorization of types. Recent advances in the 2020s have applied parallelepiped-based lattice designs in optimization, where AI-driven methods predict and refine geometries to enhance mechanical properties like strength-to-weight ratios in additive manufacturing. These approaches, while promising, remain an emerging area with ongoing research into scalable implementations.

History and Etymology

Historical Development

The concept of the parallelepiped traces its origins to , where it was implicitly described through discussions of solid figures in 's Elements, composed around 300 BCE. In Book XI, Euclid examines "parallelepipedal solids" in several propositions, such as Proposition 29, which equates volumes of such solids on the same base and height with extremities aligned on straight lines, and Proposition 32, which establishes their ratios based on bases when heights are equal. These treatments laid foundational principles for three-dimensional extensions of parallelograms, focusing on properties like equality and proportion without explicit modern . The term "parallelepipedon," derived from roots meaning "parallel planes," emerged in as a descriptor for these figures, reflecting Hellenistic advancements in . Its first recorded use in English appeared in 1570 within Billingsley's translation of Euclid's Elements, where it rendered Greek descriptions of the solid as "parallelipipedon," marking the introduction of the concept into English mathematical . In the late , advanced the study through descriptive , developed around 1765 for military applications, which enabled precise two-dimensional representations of three-dimensional objects like parallelepipeds via orthogonal projections. This method facilitated engineering visualizations of such solids, emphasizing their projection onto perpendicular planes to capture spatial relations. By the mid-19th century, the parallelepiped was formalized within emerging vector geometry; Hermann Grassmann's 1844 Ausdehnungslehre introduced linear extensions where the volume of a parallelepiped spanned by vectors corresponds to the magnitude of their exterior product, providing an algebraic framework for multidimensional geometry. William Rowan Hamilton's concurrent work on quaternions (1843–1844) complemented this by extending scalar and vector operations to three dimensions, indirectly supporting parallelepiped analyses in spatial calculations. The 19th century also saw applications in , where Auguste Bravais identified 14 types in 1850, each definable by a primitive parallelepiped unit cell with edges a, b, c and angles α, β, γ, forming the basis for classifying symmetries. In the , this evolved into Bravais lattices as infinite arrays of such cells, essential for understanding atomic arrangements in solids. Computational explorations intensified in the , particularly for "perfect" parallelepipeds—those with integer edge, face-diagonal, and body-diagonal lengths—yielding the first examples in 2009 via brute-force searches satisfying Diophantine conditions. Subsequent work in 2014 established an infinite family of such figures using parametric vector generations.

Etymology

The term "parallelepiped" derives from the παραλληλεπίπεδον (parallēlepípedon), which translates to "a body with parallel plane surfaces." This compound word combines παράλληλος (parallēlos), meaning "parallel," with ἐπίπεδον (epipedon), denoting "plane" or "level surface," the latter formed from ἐπί (epi), "upon" or "on," and πέδον (pedon), "ground" or "soil." The concept of the parallelepiped is described in Euclid's Elements around the 3rd century BCE, with the Greek term parallēlepípedon emerging later in Hellenistic mathematical literature to denote a three-dimensional figure bounded by parallelograms. It entered Latin as parallelepipedum in post-classical texts, notably in Boethius's works from the 5th–6th centuries , and persisted through mathematics. In English, it was introduced as "parallelepipedon" in Henry Billingsley's 1570 translation of Euclid's Elements, later shortening to "parallelepiped" by 1663. An archaic English spelling, "parallelopiped," appears in early 19th-century sources such as Webster's 1828 dictionary. The related term "parallelotope" shares these roots, referring to higher-dimensional generalizations bounded by parallel hyperplanes.

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