Line (geometry)
Straight figure with zero width and depth

In geometry, a straight line, usually abbreviated line, is an infinitely long object with no width, depth, or curvature. It is a special case of a curve and an idealisation of such physical objects as a straightedge, a taut string, or a ray of light. Lines are spaces of dimension one, which may be embedded in spaces of dimension two, three, or higher. The word line may also refer, in everyday life, to a line segment, which is a part of a line delimited by two points (its endpoints).
Euclid's Elements defines a straight line as a "breadthless length" that "lies evenly with respect to the points on itself", and introduced several postulates as basic unprovable properties on which the rest of geometry was established. Euclidean line and Euclidean geometry are terms introduced to avoid confusion with generalizations introduced since the end of the 19th century, such as non-Euclidean, projective, and affine geometry.
01Properties
In the Greek deductive geometry of Euclid's Elements, a general line (now called a curve) is defined as a "breadthless length", and a straight line (now called a line segment) was defined as a line "which lies evenly with the points on itself". These definitions appeal to readers' physical experience, relying on terms that are not themselves defined, and the definitions are never explicitly referenced in the remainder of the text. In modern geometry, a line is usually either taken as a primitive notion with properties given by axioms, or else defined as a set of points obeying a linear relationship, for instance when real numbers are taken to be primitive and geometry is established analytically in terms of numerical coordinates.
In an axiomatic formulation of Euclidean geometry, such as that of Hilbert (modern mathematicians added to Euclid's original axioms to fill perceived logical gaps), a line is stated to have certain properties that relate it to other lines and points. For example, for any two distinct points, there is a unique line containing them, and any two distinct lines intersect at most at one point. In two dimensions (i.e., the Euclidean plane), two lines that do not intersect are called parallel. In higher dimensions, two lines that do not intersect are parallel if they are contained in a plane, or skew if they are not.
On a Euclidean plane, a line can be represented as a boundary between two regions. Any collection of finitely many lines partitions the plane into convex polygons (possibly unbounded); this partition is known as an arrangement of lines.
In higher dimensions
In three-dimensional space, a first degree equation in the variables x, y, and z defines a plane, so two such equations, provided the planes they give rise to are not parallel, define a line which is the intersection of the planes. More generally, in n-dimensional space n − 1 first-degree equations in the n coordinate variables define a line under suitable conditions.
In more general Euclidean space, (and analogously in every other affine space), the line L passing through two different points a and b is the subset
The orientation or direction of the oriented line (or directed line) above is from a reference point a (t = 0) to a target point b (t = 1), or in other words, in the direction of the relative vector b − a. A directed line is also called an axis, especially if it plays a distinctive role (e.g., an axis of rotation). Swapping points a and b yields the opposite directed line.
Collinear points
Three or more points are said to be collinear if they lie on the same line. If three points are not collinear, there is exactly one plane that contains them.
In affine coordinates, in n-dimensional space the points
are collinear if the matrix
has a rank less than 3. In particular, for three points in the plane (n = 2), the above matrix is square and the points are collinear if and only if its determinant is zero.
Equivalently for three points in a plane, the points are collinear if and only if the slope between one pair of points equals the slope between any other pair of points (in which case the slope between the remaining pair of points will equal the other slopes). By extension, k points in a plane are collinear if and only if any (k, 1) pairs of points have the same pairwise slopes.
In Euclidean geometry, the Euclidean distance d(a,b) between two points a and b may be used to express the collinearity between three points by:
- The points a, b and c are collinear if and only if d(x,a) = d(c,a) and d(x,b) = d(c,b) implies x = c.
However, there are other notions of distance (such as the Manhattan distance) for which this property is not true.
In the geometries where the concept of a line is a primitive notion, as may be the case in some synthetic geometries, other methods of determining collinearity are needed.
Relationship with other figures
In Euclidean geometry, all lines are congruent, meaning that every line can be obtained by moving a specific line. However, lines may play special roles with respect to other geometric objects and can be classified according to that relationship.
For instance, with respect to a conic (a circle, ellipse, parabola, or hyperbola), lines can be:
- tangent lines, which touch the conic at a single point;
- secant lines, which intersect the conic at two points and pass through its interior;
- exterior lines, which do not meet the conic at any point of the Euclidean plane; or
- a directrix, whose distance from a point helps to establish whether the point is on the conic.
- a coordinate line, a linear coordinate dimension
In the context of determining parallelism in Euclidean geometry, a transversal is a line that intersects two other lines that may or not be parallel to each other.
For more general algebraic curves, lines could also be:
- i-secant lines, meeting the curve in i points counted without multiplicity, or
- asymptotes, which a curve approaches arbitrarily closely without touching it.
With respect to triangles we have:
- the Euler line,
- the Simson lines, and
- central lines.
For a convex quadrilateral with at most two parallel sides, the Newton line is the line that connects the midpoints of the two diagonals.
For a hexagon with vertices lying on a conic we have the Pascal line and, in the special case where the conic is a pair of lines, we have the Pappus line.
Parallel lines are lines in the same plane that never cross. Intersecting lines share a single point in common. Coincidental lines coincide with each other, every point that is on either one of them is also on the other.
Perpendicular lines are lines that intersect at right angles.
In three-dimensional space, skew lines are lines that are not in the same plane and thus do not intersect each other.
In axiomatic systems
In synthetic geometry, the concept of a line is often considered as a primitive notion, meaning it is not being defined by using other concepts, but it is defined by the properties, called axioms, that it must satisfy.
However, the axiomatic definition of a line does not explain the relevance of the concept and is often too abstract for beginners. So, the definition is often replaced or completed by a mental image or intuitive description that allows understanding of what a line is. Such descriptions are sometimes referred to as definitions, but are not true definitions since they cannot be used in mathematical proofs. The "definition" of a line in Euclid's Elements falls into this category; and is never used in proofs of theorems.


02Definition
Linear equation
Lines in a Cartesian plane or, more generally, in affine coordinates, are characterized by linear equations. More precisely, every line L (including vertical lines) is the set of all points whose coordinates (x, y) satisfy a linear equation; that is,
where a, b and c are fixed real numbers (called coefficients) such that a and b are not both zero. Using this form, vertical lines correspond to equations with b = 0.
One can further suppose either c = 1 or c = 0, by dividing everything by c if it is not zero.
There are many variant ways to write the equation of a line, which can all be converted from one to another by algebraic manipulation. The above form is sometimes called the standard form. If the constant term is put on the left, the equation becomes
and this is sometimes called the general form of the equation. However, this terminology is not universally accepted, and many authors do not distinguish these two forms.
These forms are generally named by the type of information (data) about the line that is needed to write down the form. Some of the important data of a line is its slope, x-intercept, known points on the line and y-intercept.
The equation of the line passing through two different points P0(x0, y0) and P1(x1, y1) may be written as
If x0 ≠ x1, this equation may be rewritten as
In two dimensions, the equation for non-vertical lines is often given in the slope-intercept form:
where
- m is the slope or gradient of the line.
- b is the y-intercept of the line.
- x is the independent variable of the function y = f(x).
The slope of the line through points A(xa, ya) and B(xb, yb), when xa ≠ xb, is given by
and the equation of this line can be written
As a note, lines in three dimensions may also be described as the simultaneous solutions of two linear equations
such that (a1, b1, c1) and (a2, b2, c2) are not proportional (the relations a1 = ta2, b1 = tb2, c1 = tc2 imply t = 0). This follows since in three dimensions a single linear equation typically describes a plane and a line is what is common to two distinct intersecting planes.
Parametric equation
Parametric equations are also used to specify lines, particularly in those in three dimensions or more, because in more than two dimensions lines cannot be described by a single linear equation.
In three dimensions, lines are frequently described by parametric equations:
where:
- x, y, and z are all functions of the independent variable t which ranges over the real numbers.
- (x0, y0, z0) is any point on the line.
- a, b, and c are related to the slope of the line, such that the direction vector (a, b, c) is parallel to the line.
Parametric equations for lines in higher dimensions are similar in that they are based on the specification of one point on the line and a direction vector.
Hesse normal form
The normal form (also called the Hesse normal form, after the German mathematician Ludwig Otto Hesse), is based on the normal segment for a given line, which is defined to be the line segment drawn from the origin perpendicular to the line. This segment joins the origin with the closest point on the line to the origin. The normal form of the equation of a straight line on the plane is given by:
where φ is the angle of inclination of the normal segment (the oriented angle from the unit vector of the x-axis to this segment), and p is the (positive) length of the normal segment. The normal form can be derived from the standard form
by dividing all of the coefficients by
and also multiplying through by , 1 if c < 0.
Unlike the slope-intercept and intercept forms, this form can represent any line but also requires only two finite parameters, φ and p, to be specified. If p > 0, then φ is uniquely defined modulo 2π. On the other hand, if the line is through the origin (c = p = 0), one drops the c/|c| term to compute sin φ and cos φ, and it follows that φ is only defined modulo π.

03Other representations
Vectors
The vector equation of the line through points A and B is given by (where λ is a scalar).
If a is vector OA and b is vector OB, then the equation of the line can be written:
A ray starting at point A is described by limiting λ. One ray is obtained if λ ≥ 0, and the opposite ray comes from λ ≤ 0.
Polar coordinates
In a Cartesian plane, polar coordinates (r, θ) are related to Cartesian coordinates by the parametric equations:
In polar coordinates, the equation of a line not passing through the origin, the point with coordinates (0, 0), can be written
with r > 0 and
Here, p is the (positive) length of the line segment perpendicular to the line and delimited by the origin and the line, and φ is the (oriented) angle from the x-axis to this segment.
It may be useful to express the equation in terms of the angle between the x-axis and the line. In this case, the equation becomes
with r > 0 and 0 < θ < α + π.
These equations can be derived from the normal form of the line equation by setting
and then applying the angle difference identity for sine or cosine.
These equations can also be proven geometrically by applying right triangle definitions of sine and cosine to the right triangle that has a point of the line and the origin as vertices, and the line and its perpendicular through the origin as sides.
The previous forms do not apply for a line passing through the origin, but a simpler formula can be written: the polar coordinates (r, θ) of the points of a line passing through the origin and making an angle of with the x-axis, are the pairs
such that


04Generalizations
In modern mathematics, given the multitude of geometries, the concept of a line is closely tied to the way the geometry is described. For instance, in analytic geometry, a line in the plane is often defined as the set of points whose coordinates satisfy a given linear equation, but in a more abstract setting, such as incidence geometry, a line may be an independent object, distinct from the set of points which lie on it.
When a geometry is described by a set of axioms, the notion of a line is usually left undefined (a so-called primitive object). The properties of lines are then determined by the axioms which refer to them. One advantage to this approach is the flexibility it gives to users of the geometry. Thus in differential geometry, a line may be interpreted as a geodesic (shortest path between points), while in some projective geometries, a line is a 2-dimensional vector space (all linear combinations of two independent vectors). This flexibility also extends beyond mathematics and, for example, permits physicists to think of the path of a light ray as being a line.
Projective geometry
In many models of projective geometry, the representation of a line rarely conforms to the notion of the "straight curve" as it is visualised in Euclidean geometry. In elliptic geometry we see a typical example of this. In the spherical representation of elliptic geometry, lines are represented by great circles of a sphere with diametrically opposite points identified. In a different model of elliptic geometry, lines are represented by Euclidean planes passing through the origin. Even though these representations are visually distinct, they satisfy all the properties (such as, two points determining a unique line) that make them suitable representations for lines in this geometry.
The "shortness" and "straightness" of a line, interpreted as the property that the distance along the line between any two of its points is minimized (see triangle inequality), can be generalized and leads to the concept of geodesics in metric spaces.

Sources and credits
This article is adapted from the Wikipedia article “Line (geometry)”, written by its contributors and licensed under CC BY-SA 4.0. Fathomly has changed the layout, removed citation markers, navigation and maintenance notices, and adjusted punctuation. This adapted version is shared under the same license. For references, see the original article.
Images, from Wikimedia Commons:
- Gerade.svg by Adrian Neumann, CC BY-SA 3.0
- Tangent to a curve.svg by Jacj at English Wikipedia / Later versions were uploaded by Oleg Alexandrov at en.wikipedia., Public domain
- Linear Function Graph.svg by Jim.belk, Public domain
- Hesse normalenform.svg by Kmhkmh, CC BY 4.0
- Parametres polaires droite.svg by Cdang, CC BY-SA 4.0
- Great circle hemispheres.png by Jhbdel at en.wikipedia, CC BY-SA 3.0
- Ray (A, B, C).svg by Unknown author, Public domain
- Number line with x smaller than y.svg by Stephan Kulla (User:Stephan Kulla), CC BY 3.0
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