In mathematics, the parabola (pronounced /pəˈræbələ/, from the Greek παραβολή) is a conic section, the intersection of a right circular conical surface and a plane to a generating straight line of that surface. Given a point (the focus) and a corresponding line (the directrix) on the plane, the locus of points in that plane that are equidistant from them is a parabola.
The parabola has many important applications, from automobile headlight reflectors to the design of ballistic missiles. They are frequently used in physics, engineering, and many other areas.
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The earliest known work on conic sections was by Menaechmus in the fourth century B.C.. He discovered a way to solve the problem of doubling the cube using parabolae. (The solution, however, does not meet the requirements imposed by compass and straightedge construction.) The name "parabola" is due to Apollonius, who discovered many properties of conic sections. The focus–directrix property of the parabola and other conics is due to Pappus.
Galileo showed that the path of a projectile follows a parabola, a consequence of uniform acceleration due to gravity.
The idea of using a paraboloid in a reflecting telescope is due to James Gregory in 1663 and the first to be constructed was by Isaac Newton in 1668. The same principle is used in satellite dishes and radar receivers.
Let the directrix be the line x = −p and let the focus be the point (p, 0). If (x, y) is a point on the parabola then, by Pappus' definition of a parabola, it is the same distance from the directrix as the focus; in other words:
Squaring both sides and simplifying produces
as the equation of the parabola.
By translation, the general equation of a parabola with a horizontal axis is
and interchanging the roles of x and y gives the corresponding equation of a parabola with a vertical axis as
The last equation can be rewritten
so the graph of any function which is a polynomial of degree 2 in x is a parabola with a vertical axis.
More generally, a parabola is a curve in the Cartesian plane defined by an irreducible equation of the form
such that
where all of the coefficients are real, neither A nor B is zero and more than one solution exists, defining a pair of points (x, y) on the parabola. That the equation is irreducible means it does not factor as a product of two not necessarily distinct linear equations.It is very difficult to solve.
A parabola may also be characterized as a conic section with an eccentricity of 1. As a consequence of this, all parabolae are similar, meaning that while they can be different sizes, they are all the same shape. A parabola can also be obtained as the limit of a sequence of ellipses where one focus is kept fixed as the other is allowed to move arbitrarily far away in one direction. In this sense, a parabola may be considered an ellipse that has one focus at infinity. The parabola is an inverse transform of a cardioid.
A parabola has a single axis of reflective symmetry, which passes through its focus and is perpendicular to its directrix. The point of intersection of this axis and the parabola is called the vertex. A parabola spun about this axis in three dimensions traces out a shape known as a paraboloid of revolution.
The parabola is found in numerous situations in the physical world (see below).
(with vertex (h, k) and distance p between vertex and focus  note that if the vertex is below the focus, or equivalently above the directrix, p is positive, otherwise p is negative; similarly with horizontal axis of symmetry p is positive if vertex is to the left of the focus, or equivalently to the right of the directrix)
The general form for a parabola is
This result is derived from the general conic equation given above:
and the fact that, for a parabola,
In polar coordinates, a parabola with the focus at the origin and the directrix parallel to the yaxis, is given by the equation
where l is the semilatus rectum: the distance from the focus to the parabola itself, measured along a line perpendicular to the axis. Note that this is twice the distance from the focus to the vertex of the parabola or the perpendicular distance from the focus to the latus rectum.
The latus rectum is the chord that passes through the focus and is perpendicular to the axis. It has a length of 2l.
A Gaussmapped form: (tan^{2}φ,2tanφ) has normal (cosφ,sinφ).
To derive the focus of a simple parabola, where the axis of symmetry is parallel to the yaxis with the vertex at (0,0), such as
then there is a point (0,f)—the focus, F—such that any point P on the parabola will be equidistant from both the focus and the linea directrix, L. The linea directrix is a line perpendicular to the axis of symmetry of the parabola (in this case parallel to the x axis) and passes through the point (0,f). So any point P=(x,y) on the parabola will be equidistant both to (0,f) and (x,f).
FP, a line from the focus to a point on the parabola, has the same length as QP, a line drawn from that point on the parabola perpendicular to the linea directrix, intersecting at point Q.
Imagine a right triangle with two legs, x and fy (the vertical distance between F and P). The length of the hypotenuse, FP, is given by
(Note that (fy) and (yf) produce the same result because it is squared.)
The line QP is given by adding y (the vertical distance between the point P and the xaxis) and f (the vertical distance between the xaxis and the linea directrix).
These two line segments are equal, and, as indicated above, y=ax², thus
Square both sides,
Cancel out terms from both sides,
Divide out the x² from both sides (we assume that x is not zero),
So, for a parabola such as f(x)=x², the a coefficient is 1, so the focus F is (0,¼)
As stated above, this is the derivation of the focus for a simple parabola, one centered at the origin and with symmetry around the yaxis. For any generalized parabola, with its equation given in the standard form
the focus is located at the point
which may also be written as
and the directrix is designated by the equation
which may also be written as
The tangent of the parabola described by equation y=ax^{2} has slope
This line intersects the yaxis at the point (0,y) = (0,  a x²), and the xaxis at the point (x/2,0). Let this point be called G. Point G is also the midpoint of points F and Q:
Since G is the midpoint of line FQ, this means that
and it is already known that P is equidistant from both F and Q:
and, thirdly, line GP is equal to itself, therefore:
It follows that .
Line QP can be extended beyond P to some point T, and line GP can be extended beyond P to some point R. Then and are vertical, so they are equal (congruent). But is equal to . Therefore is equal to .
The line RG is tangent to the parabola at P, so any light beam bouncing off point P will behave as if line RG were a mirror and it were bouncing off that mirror.
Let a light beam travel down the vertical line TP and bounce off from P. The beam's angle of inclination from the mirror is , so when it bounces off, its angle of inclination must be equal to . But has been shown to be equal to . Therefore the beam bounces off along the line FP: directly towards the focus.
Conclusion: Any light beam moving vertically downwards in the concavity of the parabola (parallel to the axis of symmetry) will bounce off the parabola moving directly towards the focus. (See parabolic reflector.)
The same reasoning can be applied to a parabola whose axis is vertical, so that it can be specified by the equation
The tangent has then a generic slope of
Reflection derivation, together with trigonometric angle addition rules, leads to the result that the reflected ray has a slope of
The xcoordinate at the vertex is , so substitute it into the equation y = ax^{2} + bx + c
Simplifying:
Thus, the vertex is at point
In nature, approximations of parabolae and paraboloids are found in many diverse situations. The bestknown instance of the parabola in the history of physics is the trajectory of a particle or body in motion under the influence of a uniform gravitational field without air resistance (for instance, a baseball flying through the air, neglecting air friction).
The parabolic trajectory of projectiles was discovered experimentally by Galileo in the early 17th century, who performed experiments with balls rolling on inclined planes. He also later proved this mathematically in his book Dialogue Concerning Two New Sciences.^{[1]}^{[2]} For objects extended in space, such as a diver jumping from a diving board, the object itself follows a complex motion as it rotates, but the center of mass of the object nevertheless forms a parabola. As in all cases in the physical world, the trajectory is always an approximation of a parabola. The presence of air resistance, for example, always distorts the shape, although at low speeds, the shape is a good approximation of a parabola. At higher speeds, such as in ballistics, the shape is highly distorted and does not resemble a parabola.
Another situation in which parabolae may arise in nature is in twobody orbits, for example, of a small planetoid or other object under the influence of the gravitation of the sun. Such parabolic orbits are a special case that are rarely found in nature. Orbits that form a hyperbola or an ellipse are much more common. In fact, the parabolic orbit is the borderline case between those two types of orbit. An object following a parabolic orbit moves at the exact escape velocity of the object it is orbiting, while elliptical orbits are slower and hyperbolic orbits are faster.
Approximations of parabolae are also found in the shape of the main cables on a typical suspension bridge. Freely hanging cables as seen on a simple suspension bridge do not describe parabolic curves, but rather hyperbolic catenary curves. Under the influence of a uniform load (such as a horizontal suspended deck), the otherwise hyperbolic cable is deformed toward a parabola. Unlike an inelastic chain, a freelyhanging spring of zero rest length takes the shape of a parabola.
Paraboloids arise in several physical situations as well. The bestknown instance is the parabolic reflector, which is a mirror or similar reflective device that concentrates light or other forms of electromagnetic radiation to a common focal point. The principle of the parabolic reflector may have been discovered in the 3rd century BC by the geometer Archimedes, who, according to a legend of debatable veracity,^{[3]} constructed parabolic mirrors to defend Syracuse against the Roman fleet, by concentrating the sun's rays to set fire to the decks of the Roman ships. The principle was applied to telescopes in the 17th century. Today, paraboloid reflectors can be commonly observed throughout much of the world in microwave and satellite dish antennas.
Paraboloids are also observed in the surface of a liquid confined to a container and rotated around the central axis. In this case, the centrifugal force causes the liquid to climb the walls of the container, forming a parabolic surface. This is the principle behind the liquid mirror telescope.
Aircraft used to create a weightless state for purposes of experimentation, such as NASA's “Vomit Comet,” follow a vertically parabolic trajectory for brief periods in order to trace the course of an object in free fall, which produces the same effect as zero gravity for most purposes.
In algebraic geometry, the parabola is generalized by the rational normal curves, which have coordinates the standard parabola is the case n = 2, and the case n = 3 is known as the twisted cubic. A further generalization is given by the Veronese variety, when there are more than one input variable.
In the theory of quadratic forms, the parabola is the graph of the quadratic form x^{2} (or other scalings), while the elliptic paraboloid is the graph of the positivedefinite quadratic form x^{2} + y^{2} (or scalings) and the hyperbolic paraboloid is the graph of the indefinite quadratic form x^{2} − y^{2}. Generalizations to more variables yield further such objects.
