Descriptions
By equations
A flat can be described by a system of linear equations. For example, a line in two-dimensional space can be described by a single linear equation involving and : : In three-dimensional space, a single linear equation involving , , and defines a plane, while a pair of linear equations can be used to describe a line. In general, a linear equation in variables describes a hyperplane, and a system of linear equations describes the intersection of those hyperplanes. Assuming the equations are consistent and linearly independent, a system of equations describes a flat of dimension .Parametric
A flat can also be described by a system of linear parametric equations. A line can be described by equations involving one parameter: : while the description of a plane would require two parameters: : In general, a parameterization of a flat of dimension would require parameters, e.g. .Operations and relations on flats
Intersecting, parallel, and skew flats
An intersection of flats is either a flat or theJoin
For two flats of dimensions and there exists the minimal flat which contains them, of dimension at most . If two flats intersect, then the dimension of the containing flat equals to minus the dimension of the intersection.Properties of operations
These two operations (referred to as ''meet'' and ''join'') make the set of all flats in the Euclidean -space a lattice and can build systematic coordinates for flats in any dimension, leading to Grassmann coordinates or dual Grassmann coordinates. For example, a line in three-dimensional space is determined by two distinct points or by two distinct planes. However, the lattice of all flats is not a distributive lattice. If two lines and intersect, then is a point. If is a point not lying on the same plane, then , both representing a line. But when and are parallel, this distributivity fails, giving on the left-hand side and a third parallel line on the right-hand side.Euclidean geometry
The aforementioned facts do not depend on the structure being that of Euclidean space (namely, involving Euclidean distance) and are correct in any affine space. In a Euclidean space: * There is the distance between a flat and a point. (See for example '' Distance from a point to a plane'' and '' Distance from a point to a line''.) * There is the distance between two flats, equal to 0 if they intersect. (See for example '' Distance between two parallel lines'' (in the same plane) and '.) * There is theSee also
* Matroid * Coplanarity * IsometryNotes
References
* Heinrich Guggenheimer (1977), ''Applicable Geometry'', Krieger, New York, page 7. *External links
* *{{MathWorld, urlname=Flat, title=Flat Euclidean geometry Affine geometry Linear algebra fr:Hyperplan