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   » » Wiki: Parallelepiped
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Prism
6
12
8
, 2+,2+, (×), order 2
convex,

In , a parallelepiped is a three-dimensional figure formed by six (the term is also sometimes used with this meaning). By analogy, it relates to a just as a relates to a .

Three equivalent definitions of parallelepiped are

The rectangular cuboid (six faces), (six faces), and the (six faces) are all special cases of parallelepiped.

"Parallelepiped" is now usually pronounced or ; traditionally it was Oxford English Dictionary 1904; Webster's Second International 1947 because of its etymology in παραλληλεπίπεδον parallelepipedon (with short -i-), a body "having ".

Parallelepipeds are a subclass of the .


Properties
Any of the three pairs of parallel faces can be viewed as the base planes of the prism. A parallelepiped has three sets of four parallel edges; the edges within each set are of equal length.

Parallelepipeds result from linear transformations of a (for the non-degenerate cases: the bijective linear transformations).

Since each face has , a parallelepiped is a . Also the whole parallelepiped has point symmetry (see also ). Each face is, seen from the outside, the mirror image of the opposite face. The faces are in general chiral, but the parallelepiped is not.

A space-filling tessellation is possible with congruent copies of any parallelepiped.


Volume
A parallelepiped is a prism with a as base. Hence the volume V of a parallelepiped is the product of the base area B and the height h (see diagram). With
  • B = \left|\mathbf a\right| \cdot \left|\mathbf b\right| \cdot \sin \gamma = \left|\mathbf a \times \mathbf b\right| (where \gamma is the angle between vectors \mathbf a and \mathbf b), and
  • h = \left|\mathbf c\right| \cdot \left|\cos \theta\right| (where \theta is the angle between vector \mathbf c and the normal to the base), one gets:
V = B\cdot h = \left(\left|\mathbf a\right| \left|\mathbf b\right| \sin \gamma\right) \cdot \left|\mathbf c\right| \left|\cos \theta\right| = \left|\mathbf a \times \mathbf b\right| \left|\mathbf c\right| \left|\cos \theta\right| = \left|\left(\mathbf{a} \times \mathbf{b}\right) \cdot \mathbf{c}\right|. The mixed product of three vectors is called . It can be described by a . Hence for \mathbf a=(a_1,a_2,a_3)^\mathsf{T}, ~\mathbf b=(b_1,b_2,b_3)^\mathsf{T}, ~\mathbf c=(c_1,c_2,c_3)^\mathsf{T}, the volume is:

Another way to prove () is to use the scalar component in the direction of \mathbf a\times\mathbf b of vector \mathbf c: \begin{align} V = \left|\mathbf a\times\mathbf b\right| \left|\operatorname{scal}_{\mathbf a \times \mathbf b} \mathbf c\right| = \left|\mathbf a\times\mathbf b\right| \frac{\left|\left(\mathbf a\times \mathbf b\right) \cdot \mathbf c\right|}{\left|\mathbf a\times \mathbf b\right|} = \left|\left(\mathbf a\times \mathbf b\right) \cdot \mathbf c\right|. \end{align} The result follows.

An alternative representation of the volume uses geometric properties (angles and edge lengths) only:

where \alpha = \angle(\mathbf b, \mathbf c), \beta = \angle(\mathbf a,\mathbf c), \gamma = \angle(\mathbf a,\mathbf b) , and a,b,c are the edge lengths.

Corresponding tetrahedron

The volume of any that shares three converging edges of a parallelepiped is equal to one sixth of the volume of that parallelepiped (see proof).


Surface area
The surface area of a parallelepiped is the sum of the areas of the bounding parallelograms: \begin{align} A &= 2 \cdot \left(|\mathbf a \times \mathbf b| + |\mathbf a \times \mathbf c| + |\mathbf b \times \mathbf c|\right) \\ &= 2\left(ab\sin\gamma+ bc\sin\alpha+ca\sin\beta\right). \end{align} (For labeling: see previous section.)


Special cases by symmetry

Octahedral symmetry subgroup relations with

Special cases of the parallelepiped
  • The parallelepiped with Oh symmetry is known as a , which has six congruent square faces.
  • The parallelepiped with D4h symmetry is known as a , which has two square faces and four congruent rectangular faces.
  • The parallelepiped with D3d symmetry is known as a trigonal trapezohedron, which has six congruent faces (also called an isohedral rhombohedron).
  • For parallelepipeds with D2h symmetry, there are two cases:
    • Rectangular cuboid: it has six rectangular faces (also called a rectangular parallelepiped, or sometimes simply a cuboid).
    • Right rhombic prism: it has two rhombic faces and four congruent rectangular faces.
    • :Note: the fully rhombic special case, with two rhombic faces and four congruent square faces (a=b=c), has the same name, and the same symmetry group (D2h , order 8).
  • For parallelepipeds with C2h symmetry, there are two cases:
    • Right parallelogrammic prism: it has four rectangular faces and two parallelogrammic faces.
    • Oblique rhombic prism: it has two rhombic faces, while of the other faces, two adjacent ones are equal and the other two also (the two pairs are each other's mirror image).


Perfect parallelepiped
A perfect parallelepiped is a parallelepiped with integer-length edges, face diagonals, and . In 2009, dozens of perfect parallelepipeds were shown to exist,. answering an open question of Richard Guy. One example has edges 271, 106, and 103, minor face diagonals 101, 266, and 255, major face diagonals 183, 312, and 323, and space diagonals 374, 300, 278, and 272.

Some perfect parallelepipeds having two rectangular faces are known. But it is not known whether there exist any with all faces rectangular; such a case would be called a perfect .


Parallelotope
called the generalization of a parallelepiped in higher dimensions a parallelotope Https://doi.org/10.1007/bf01954540< /ref>

Specifically in n-dimensional space it is called n-dimensional parallelotope, or simply -parallelotope (or -parallelepiped). Thus a is a 2-parallelotope and a parallelepiped is a 3-parallelotope.

The of an n-parallelotope intersect at one point and are bisected by this point. Inversion in this point leaves the n-parallelotope unchanged. See also Fixed points of isometry groups in Euclidean space.

The edges radiating from one vertex of a k-parallelotope form a (v_1,\ldots, v_n) of the vector space, and the parallelotope can be recovered from these vectors, by taking linear combinations of the vectors, with weights between 0 and 1.

The n-volume of an n-parallelotope embedded in \R^m where m \geq n can be computed by means of the . Alternatively, the volume is the norm of the of the vectors: V = \left\| v_1 \wedge \cdots \wedge v_n \right\| .

If , this amounts to the absolute value of the determinant of matrix formed by the components of the vectors.

A formula to compute the volume of an -parallelotope in \R^n, whose vertices are V_0,V_1, \ldots, V_n, is \mathrm{Vol}(P) = \left|\det \left(\leftV_0\^\mathsf{T}, \leftV_1\^\mathsf{T}, \ldots, \leftV_n\^\mathsf{T}\right)\right|, where V_i\ is the row vector formed by the concatenation of the components of V_i and 1.

Similarly, the volume of any n- that shares n converging edges of a parallelotope has a volume equal to one 1/ of the volume of that parallelotope.


Etymology
The term parallelepiped stems from ( parallēlepípedon, "body with parallel plane surfaces"), from parallēl ("parallel") + epípedon ("plane surface"), from epí- ("on") + pedon ("ground"). Thus the faces of a parallelepiped are planar, with opposite faces being parallel..

In English, the term parallelipipedon is attested in a 1570 translation of Euclid's Elements by Henry Billingsley. The spelling parallelepipedum is used in the 1644 edition of Pierre Hérigone's Cursus mathematicus. In 1663, the present-day parallelepiped is attested in Chorea gigantum.

Dictionary (1795) shows parallelopiped and parallelopipedon, showing the influence of the combining form parallelo-, as if the second element were pipedon rather than epipedon. (1806) includes the spelling parallelopiped. The 1989 edition of the Oxford English Dictionary describes parallelopiped (and parallelipiped) explicitly as incorrect forms, but these are listed without comment in the 2004 edition, and only pronunciations with the emphasis on the fifth syllable pi () are given.


See also
  • Lists of shapes


Notes
  • Coxeter, H. S. M. Regular Polytopes, 3rd ed. New York: Dover, p. 122, 1973. (He defines parallelotope as a generalization of a parallelogram and parallelepiped in n-dimensions.)


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