Hyperbola
- This article isn't about hyperbole, a figure of speech. For that article, see hyperbole.
a graph of a hyperbola, where h = k = 0 and a = b = 2 A
hyperbola is a type of
conic section.
- Geometrically, it is defined as the intersection between a cone and a plane which cuts through both halves of the cone.
- Analytically, it is defined as the set of all points for which the difference in the distance to two fixed points (called the foci) is constant.
For a simple geometric proof that the two characterizations above are equivalent to each other, see Dandelin spheres.
- It can also be defined as the locus of points for which the ratio of the distances to one focus and to a line (called the directrix) is a constant larger than 1. This constant is the eccentricity of the hyperbola. These foci lie on the transverse axis and their midpoint is called the center.
A hyperbola comprises two disconnected curves called its arms which separate the foci.
At large distances from the foci the hyperbola begins to approximate two lines, known as asymptotes.
A hyperbola has the property that a ray originating at one of the foci is reflected in such a way as to appear to have originated at the other focus.
A special case of the hyperbola is the equilateral or rectangular hyperbola, in which the asymptotes intersect at right angles. The rectangular hyperbola with the co-ordinate axes as its asymptotes is given by the equation xy=c, where c is a constant.
Just as the sine and cosine functions give a parametric equation for the ellipse, so the hyperbolic sine and hyperbolic cosine give a parametric equation for the hyperbola.
A body that has sufficient energy to escape the gravitational field of a massive body moves in a hyperbolic trajectory with the massive body at one of the foci.
Equations (Cartesian):
(center (
h,
k) )
- <math>\frac{\left( x-h \right)^2}{a^2} - \frac{\left( y-k \right)^2}{b^2} = 1<math>
- <math>\frac{\left( y-k \right)^2}{a^2} - \frac{\left( x-h \right)^2}{b^2} = 1<math>
- <math>(x-h)(y-k) = c \,<math>
Equations (polar):
- <math>r^2 =\ \ \, a\,\sec 2t<math>
- <math>r^2 = -a\,\sec 2t<math>
- <math>r^2 =\ \ \, a\,\csc 2t<math>
- <math>r^2 = -a\,\csc 2t<math>
Equations (parametric):
- <math>x = a\,\cosh \theta;\; y = b\,\sinh \theta<math>
- <math>x = a\,\tan \theta;\ \ y = b\,\sec \theta<math>
See also