
A representation of one line

Three lines — the red and blue lines have same slope, while the red and green ones have same y-intercept.
A 'line' can be described as an ideal zero-width, infinitely long, perfectly straight
curve (the term curve in mathematics includes "straight curves") containing an
infinite number of points. In
Euclidean geometry, exactly one line can be found that passes through any two
points. The line provides the shortest connection between the points.
In two dimensions, two different lines can either be
parallel, meaning they never meet, or may
intersect at one and only one point. In three or more dimensions, lines may also be
skew, meaning they don't meet, but also don't define a plane. Two distinct
planes intersect in at most one line. Three or more points that lie on the same line are called ''collinear''.
Examples
Lines in a
Cartesian plane can be described algebraically by
linear equations and
linear functions. In two dimensions, the characteristic equation is often given by the ''
slope-intercept form'':
:
where:
: ''m'' is the
slope of the line.
: ''b'' is the
y-intercept of the line.
: ''x'' is the
independent variable of the function ''y''.
In three dimensions, a line is often described by
parametric equations:
:
:
:
where:
: ''x'', ''y'', and ''z'' are all functions of the independent variable ''t''.
:
,
, and
are the initial values of each respective variable.
: ''a'', ''b'', and ''c'' are related to the slope of the line, such that the
vector (''a'', ''b'', ''c'') is a parallel to the line.
Formal definitions
This intuitive concept of a line can be formalized in various ways. If
geometry is developed axiomatically (as in
Euclid's
''Elements'' and later in
David Hilbert's ''
Foundations of Geometry''), then lines are not defined at all, but characterized axiomatically by their properties. While Euclid did define a line as "length without breadth", he did not use this rather obscure definition in his later development.
In
Euclidean space 'R'
''n'' (and analogously in all other
vector spaces), we define a line ''L'' as a subset of the form
:
where ''a'' and ''b'' are given
vectors in 'R'
''n'' with ''b'' non-zero. The vector ''b'' describes the direction of the line, and ''a'' is a point on the line. Different choices of ''a'' and ''b'' can yield the same line.
Properties
In a two-dimensional space, such as the plane, two different lines must either be
parallel lines or must intersect at one point. In higher-dimensional spaces however, two lines may do neither, and two such lines are called
skew lines.
In 'R'
2, every line ''L'' is described by a linear equation of the form
:
with fixed real
coefficients ''a'', ''b'' and ''c'' such that ''a'' and ''b'' are not both zero (see
Linear equation for other forms). Important properties of these lines are their
slope,
x-intercept and
y-intercept. The
eccentricity of a straight line is
infinity.
More abstractly, one usually thinks of the
real line as the prototype of a line, and assumes that the points on a line stand in a one-to-one correspondence with the
real numbers. However, one could also use the
hyperreal numbers for this purpose, or even the
long line of
topology.
The "straightness" of a line, interpreted as the property that it minimizes distances between its points, can be generalized and leads to the concept of
geodesics on differentiable
manifolds.
Ray
In
Euclidean geometry, a ray, or half-line, given two distinct
points A (the origin) and B on the ray, is the set of points C on the line containing points A and B such that A is not strictly between C and B. In
geometry, a ray starts at one
point, then goes on forever in one direction.
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Ray
See also
★
Line segment
★
Affine function
★
Diffraction
★
Glossary of Riemannian and metric geometry#R for its meaning in
Riemannian geometry.
★
Incidence (geometry)
★
Minimal line representation
External links
★
Detailed explanation of the line at MathWorld Encyclopedia
★
Equations of the Straight Line at
cut-the-knot