Ellipse

It generalizes a circle, which is the special type of ellipse in which the two focal points are the same. The elongation of an ellipse is measured by its eccentricity ${\displaystyle e}$, a number ranging from ${\displaystyle e=0}$ (the limiting case of a circle) to ${\displaystyle e=1}$ (the limiting case of infinite elongation, no longer an ellipse but a parabola).

An ellipse has a simple algebraic solution for its area, but only approximations for its perimeter (also known as circumference), for which integration is required to obtain an exact solution.

Analytically, the equation of a standard ellipse centered at the origin with width ${\displaystyle 2a}$ and height ${\displaystyle 2b}$ is:

$${\displaystyle {\frac {x^{2}}{a^{2}}}+{\frac {y^{2}}{b^{2}}}=1.}$$

Assuming ${\displaystyle a\geq b}$, the foci are ${\displaystyle (\pm c,0)}$ for ${\textstyle c={\sqrt {a^{2}-b^{2}}}}$. The standard parametric equation is:

$${\displaystyle (x,y)=(a\cos(t),b\sin(t))\quad {\text{for}}\quad 0\leq t\leq 2\pi .}$$

Ellipses are the closed type of conic section: a plane curve tracing the intersection of a cone with a plane (see figure). Ellipses have many similarities with the other two forms of conic sections, parabolas and hyperbolas, both of which are open and unbounded. An angled cross section of a right circular cylinder is also an ellipse.

An ellipse may also be defined in terms of one focal point and a line outside the ellipse called the directrix: for all points on the ellipse, the ratio between the distance to the focus and the distance to the directrix is a constant. This constant ratio is the above-mentioned eccentricity:

$${\displaystyle e={\frac {c}{a}}={\sqrt {1-{\frac {b^{2}}{a^{2}}}}}.}$$

Ellipses are common in physics, astronomy and engineering. For example, the orbit of each planet in the Solar System is approximately an ellipse with the Sun at one focus point (more precisely, the focus is the barycenter of the Sun–planet pair). The same is true for moons orbiting planets and all other systems of two astronomical bodies. The shapes of planets and stars are often well described by ellipsoids. A circle viewed from a side angle looks like an ellipse: that is, the ellipse is the image of a circle under parallel or perspective projection. The ellipse is also the simplest Lissajous figure formed when the horizontal and vertical motions are sinusoids with the same frequency: a similar effect leads to elliptical polarization of light in optics.

The name, ἔλλειψις (élleipsis, "omission"), was given by Apollonius of Perga in his Conics.

 

 

An ellipse can be defined geometrically as a set or locus of points in the Euclidean plane:

Given two fixed points ${\displaystyle F_{1},F_{2}}$  called the foci and a distance ${\displaystyle 2a}$  which is greater than the distance between the foci, the ellipse is the set of points ${\displaystyle P}$  such that the sum of the distances ${\displaystyle |PF_{1}|,\ |PF_{2}|}$  is equal to ${\displaystyle 2a}$ :

$${\displaystyle E=\left\{P\in \mathbb {R} ^{2}\,\mid \,\left|PF_{2}\right|+\left|PF_{1}\right|=2a\right\}.}$$

 

The midpoint ${\displaystyle C}$  of the line segment joining the foci is called the center of the ellipse. The line through the foci is called the major axis, and the line perpendicular to it through the center is the minor axis. The major axis intersects the ellipse at two vertices ${\displaystyle V_{1},V_{2}}$ , which have distance ${\displaystyle a}$  to the center. The distance ${\displaystyle c}$  of the foci to the center is called the focal distance or linear eccentricity. The quotient ${\displaystyle e={\tfrac {c}{a}}}$  is the eccentricity.

The case ${\displaystyle F_{1}=F_{2}}$  yields a circle and is included as a special type of ellipse.

The equation ${\displaystyle \left|PF_{2}\right|+\left|PF_{1}\right|=2a}$  can be viewed in a different way (see figure):

If ${\displaystyle c_{2}}$  is the circle with center ${\displaystyle F_{2}}$  and radius ${\displaystyle 2a}$ , then the distance of a point ${\displaystyle P}$  to the circle ${\displaystyle c_{2}}$  equals the distance to the focus ${\displaystyle F_{1}}$ :

$${\displaystyle \left|PF_{1}\right|=\left|Pc_{2}\right|.}$$

 

${\displaystyle c_{2}}$  is called the circular directrix (related to focus ${\displaystyle F_{2}}$ ) of the ellipse. This property should not be confused with the definition of an ellipse using a directrix line below.

Using Dandelin spheres, one can prove that any section of a cone with a plane is an ellipse, assuming the plane does not contain the apex and has slope less than that of the lines on the cone.

 

Standard equation

The standard form of an ellipse in Cartesian coordinates assumes that the origin is the center of the ellipse, the x-axis is the major axis, and:

For an arbitrary point ${\displaystyle (x,y)}$  the distance to the focus ${\displaystyle (c,0)}$  is ${\textstyle {\sqrt {(x-c)^{2}+y^{2}}}}$  and to the other focus ${\textstyle {\sqrt {(x+c)^{2}+y^{2}}}}$ . Hence the point ${\displaystyle (x,\,y)}$  is on the ellipse whenever:

$${\displaystyle {\sqrt {(x-c)^{2}+y^{2}}}+{\sqrt {(x+c)^{2}+y^{2}}}=2a\ .}$$

 

Removing the radicals by suitable squarings and using ${\displaystyle b^{2}=a^{2}-c^{2}}$  (see diagram) produces the standard equation of the ellipse:

$${\displaystyle {\frac {x^{2}}{a^{2}}}+{\frac {y^{2}}{b^{2}}}=1,}$$

 

$${\displaystyle y=\pm {\frac {b}{a}}{\sqrt {a^{2}-x^{2}}}=\pm {\sqrt {\left(a^{2}-x^{2}\right)\left(1-e^{2}\right)}}.}$$

 

The width and height parameters ${\displaystyle a,\;b}$  are called the semi-major and semi-minor axes. The top and bottom points ${\displaystyle V_{3}=(0,\,b),\;V_{4}=(0,\,-b)}$  are the co-vertices. The distances from a point ${\displaystyle (x,\,y)}$  on the ellipse to the left and right foci are ${\displaystyle a+ex}$  and ${\displaystyle a-ex}$ .

It follows from the equation that the ellipse is symmetric with respect to the coordinate axes and hence with respect to the origin.

Parameters

Principal axes

Throughout this article, the semi-major and semi-minor axes are denoted ${\displaystyle a}$  and ${\displaystyle b}$ , respectively, i.e. ${\displaystyle a\geq b>0\ .}$ 

In principle, the canonical ellipse equation ${\displaystyle {\tfrac {x^{2}}{a^{2}}}+{\tfrac {y^{2}}{b^{2}}}=1}$  may have ${\displaystyle a$  (and hence the ellipse would be taller than it is wide). This form can be converted to the standard form by transposing the variable names ${\displaystyle x}$  and ${\displaystyle y}$  and the parameter names ${\displaystyle a}$  and ${\displaystyle b.}$ 

Linear eccentricity

This is the distance from the center to a focus: ${\displaystyle c={\sqrt {a^{2}-b^{2}}}}$ .

Eccentricity

The eccentricity can be expressed as:

$${\displaystyle e={\frac {c}{a}}={\sqrt {1-\left({\frac {b}{a}}\right)^{2}}},}$$

 

assuming ${\displaystyle a>b.}$  An ellipse with equal axes (${\displaystyle a=b}$ ) has zero eccentricity, and is a circle.

Semi-latus rectum

The length of the chord through one focus, perpendicular to the major axis, is called the latus rectum. One half of it is the semi-latus rectum ${\displaystyle \ell }$ . A calculation shows:

$${\displaystyle \ell ={\frac {b^{2}}{a}}=a\left(1-e^{2}\right).}$$

 

The semi-latus rectum ${\displaystyle \ell }$  is equal to the radius of curvature at the vertices (see section curvature).

Tangent

An arbitrary line ${\displaystyle g}$  intersects an ellipse at 0, 1, or 2 points, respectively called an exterior line, tangent and secant. Through any point of an ellipse there is a unique tangent. The tangent at a point ${\displaystyle (x_{1},\,y_{1})}$  of the ellipse ${\displaystyle {\tfrac {x^{2}}{a^{2}}}+{\tfrac {y^{2}}{b^{2}}}=1}$  has the coordinate equation:

$${\displaystyle {\frac {x_{1}}{a^{2}}}x+{\frac {y_{1}}{b^{2}}}y=1.}$$

 

A vector parametric equation of the tangent is:

$${\displaystyle {\vec {x}}={\begin{pmatrix}x_{1}\\y_{1}\end{pmatrix}}+s\left({\begin{array}{r}-y_{1}a^{2}\\x_{1}b^{2}\end{array}}\right),\quad s\in \mathbb {R} .}$$

 

Proof: Let ${\displaystyle (x_{1},\,y_{1})}$  be a point on an ellipse and ${\textstyle {\vec {x}}={\begin{pmatrix}x_{1}\\y_{1}\end{pmatrix}}+s{\begin{pmatrix}u\\v\end{pmatrix}}}$  be the equation of any line ${\displaystyle g}$  containing ${\displaystyle (x_{1},\,y_{1})}$ . Inserting the line's equation into the ellipse equation and respecting ${\textstyle {\frac {x_{1}^{2}}{a^{2}}}+{\frac {y_{1}^{2}}{b^{2}}}=1}$  yields:

$${\displaystyle {\frac {\left(x_{1}+su\right)^{2}}{a^{2}}}+{\frac {\left(y_{1}+sv\right)^{2}}{b^{2}}}=1\ \quad \Longrightarrow \quad 2s\left({\frac {x_{1}u}{a^{2}}}+{\frac {y_{1}v}{b^{2}}}\right)+s^{2}\left({\frac {u^{2}}{a^{2}}}+{\frac {v^{2}}{b^{2}}}\right)=0\ .}$$

 

1. ${\displaystyle {\frac {x_{1}}{a^{2}}}u+{\frac {y_{1}}{b^{2}}}v=0.}$  Then line ${\displaystyle g}$  and the ellipse have only point ${\displaystyle (x_{1},\,y_{1})}$  in common, and ${\displaystyle g}$  is a tangent. The tangent direction has perpendicular vector ${\displaystyle {\begin{pmatrix}{\frac {x_{1}}{a^{2}}}&{\frac {y_{1}}{b^{2}}}\end{pmatrix}}}$ , so the tangent line has equation ${\textstyle {\frac {x_{1}}{a^{2}}}x+{\tfrac {y_{1}}{b^{2}}}y=k}$  for some ${\displaystyle k}$ . Because ${\displaystyle (x_{1},\,y_{1})}$  is on the tangent and the ellipse, one obtains ${\displaystyle k=1}$ .
2. ${\displaystyle {\frac {x_{1}}{a^{2}}}u+{\frac {y_{1}}{b^{2}}}v\neq 0.}$  Then line ${\displaystyle g}$  has a second point in common with the ellipse, and is a secant.

Using (1) one finds that ${\displaystyle {\begin{pmatrix}-y_{1}a^{2}&x_{1}b^{2}\end{pmatrix}}}$  is a tangent vector at point ${\displaystyle (x_{1},\,y_{1})}$ , which proves the vector equation.

If ${\displaystyle (x_{1},y_{1})}$  and ${\displaystyle (u,v)}$  are two points of the ellipse such that ${\textstyle {\frac {x_{1}u}{a^{2}}}+{\tfrac {y_{1}v}{b^{2}}}=0}$ , then the points lie on two conjugate diameters (see below). (If ${\displaystyle a=b}$ , the ellipse is a circle and "conjugate" means "orthogonal".)

Shifted ellipse

If the standard ellipse is shifted to have center ${\displaystyle \left(x_{\circ },\,y_{\circ }\right)}$ , its equation is

$${\displaystyle {\frac {\left(x-x_{\circ }\right)^{2}}{a^{2}}}+{\frac {\left(y-y_{\circ }\right)^{2}}{b^{2}}}=1\ .}$$

 

The axes are still parallel to the x- and y-axes.

General ellipse

 

In analytic geometry, the ellipse is defined as a quadric: the set of points ${\displaystyle (x,\,y)}$  of the Cartesian plane that, in non-degenerate cases, satisfy the implicit equation

$${\displaystyle Ax^{2}+Bxy+Cy^{2}+Dx+Ey+F=0}$$

 

${\displaystyle B^{2}-4AC<0.}$ 

To distinguish the degenerate cases from the non-degenerate case, let ∆ be the determinant

$${\displaystyle \Delta ={\begin{vmatrix}A&{\frac {1}{2}}B&{\frac {1}{2}}D\\{\frac {1}{2}}B&C&{\frac {1}{2}}E\\{\frac {1}{2}}D&{\frac {1}{2}}E&F\end{vmatrix}}=ACF+{\tfrac {1}{4}}BDE-{\tfrac {1}{4}}(AE^{2}+CD^{2}+FB^{2}).}$$

 

Then the ellipse is a non-degenerate real ellipse if and only if C∆ < 0. If C∆ > 0, we have an imaginary ellipse, and if ∆ = 0, we have a point ellipse.^: 63

The general equation's coefficients can be obtained from known semi-major axis ${\displaystyle a}$ , semi-minor axis ${\displaystyle b}$ , center coordinates ${\displaystyle \left(x_{\circ },\,y_{\circ }\right)}$ , and rotation angle ${\displaystyle \theta }$  (the angle from the positive horizontal axis to the ellipse's major axis) using the formulae:

$${\displaystyle {\begin{aligned}A&=a^{2}\sin ^{2}\theta +b^{2}\cos ^{2}\theta &B&=2\left(b^{2}-a^{2}\right)\sin \theta \cos \theta \\[1ex]C&=a^{2}\cos ^{2}\theta +b^{2}\sin ^{2}\theta &D&=-2Ax_{\circ }-By_{\circ }\\[1ex]E&=-Bx_{\circ }-2Cy_{\circ }&F&=Ax_{\circ }^{2}+Bx_{\circ }y_{\circ }+Cy_{\circ }^{2}-a^{2}b^{2}.\end{aligned}}}$$

 

These expressions can be derived from the canonical equation

$${\displaystyle {\frac {X^{2}}{a^{2}}}+{\frac {Y^{2}}{b^{2}}}=1}$$

 

${\displaystyle (X,\,Y)}$ 

$${\displaystyle {\begin{aligned}X&=\left(x-x_{\circ }\right)\cos \theta +\left(y-y_{\circ }\right)\sin \theta ,\\Y&=-\left(x-x_{\circ }\right)\sin \theta +\left(y-y_{\circ }\right)\cos \theta .\end{aligned}}}$$

 

Conversely, the canonical form parameters can be obtained from the general-form coefficients by the equations:

$${\displaystyle {\begin{aligned}a,b&={\frac {-{\sqrt {2{\big (}AE^{2}+CD^{2}-BDE+(B^{2}-4AC)F{\big )}{\big (}(A+C)\pm {\sqrt {(A-C)^{2}+B^{2}}}{\big )}}}}{B^{2}-4AC}},\\x_{\circ }&={\frac {2CD-BE}{B^{2}-4AC}},\\[5mu]y_{\circ }&={\frac {2AE-BD}{B^{2}-4AC}},\\[5mu]\theta &={\tfrac {1}{2}}\operatorname {atan2} (-B,\,C-A),\end{aligned}}}$$

 

where atan2 is the 2-argument arctangent function.

 

 

Standard parametric representation

Using trigonometric functions, a parametric representation of the standard ellipse ${\displaystyle {\tfrac {x^{2}}{a^{2}}}+{\tfrac {y^{2}}{b^{2}}}=1}$  is:

$${\displaystyle (x,\,y)=(a\cos t,\,b\sin t),\ 0\leq t<2\pi \,.}$$

 

The parameter t (called the eccentric anomaly in astronomy) is not the angle of ${\displaystyle (x(t),y(t))}$  with the x-axis, but has a geometric meaning due to Philippe de La Hire (see § Drawing ellipses below).

Rational representation

With the substitution ${\textstyle u=\tan \left({\frac {t}{2}}\right)}$  and trigonometric formulae one obtains

$${\displaystyle \cos t={\frac {1-u^{2}}{1+u^{2}}}\ ,\quad \sin t={\frac {2u}{1+u^{2}}}}$$

 

and the rational parametric equation of an ellipse

$${\displaystyle {\begin{cases}x(u)=a\,{\dfrac {1-u^{2}}{1+u^{2}}}\\[10mu]y(u)=b\,{\dfrac {2u}{1+u^{2}}}\\[10mu]-\infty$$

 

which covers any point of the ellipse ${\displaystyle {\tfrac {x^{2}}{a^{2}}}+{\tfrac {y^{2}}{b^{2}}}=1}$  except the left vertex ${\displaystyle (-a,\,0)}$ .

For ${\displaystyle u\in [0,\,1],}$  this formula represents the right upper quarter of the ellipse moving counter-clockwise with increasing ${\displaystyle u.}$  The left vertex is the limit ${\textstyle \lim _{u\to \pm \infty }(x(u),\,y(u))=(-a,\,0)\;.}$ 

Alternately, if the parameter ${\displaystyle [u:v]}$  is considered to be a point on the real projective line ${\textstyle \mathbf {P} (\mathbf {R} )}$ , then the corresponding rational parametrization is

$${\displaystyle [u:v]\mapsto \left(a{\frac {v^{2}-u^{2}}{v^{2}+u^{2}}},b{\frac {2uv}{v^{2}+u^{2}}}\right).}$$

 

Then ${\textstyle [1:0]\mapsto (-a,\,0).}$ 

Rational representations of conic sections are commonly used in computer-aided design (see Bezier curve).

Tangent slope as parameter

A parametric representation, which uses the slope ${\displaystyle m}$  of the tangent at a point of the ellipse can be obtained from the derivative of the standard representation ${\displaystyle {\vec {x}}(t)=(a\cos t,\,b\sin t)^{\mathsf {T}}}$ :

$${\displaystyle {\vec {x}}'(t)=(-a\sin t,\,b\cos t)^{\mathsf {T}}\quad \rightarrow \quad m=-{\frac {b}{a}}\cot t\quad \rightarrow \quad \cot t=-{\frac {ma}{b}}.}$$

 

With help of trigonometric formulae one obtains:

$${\displaystyle \cos t={\frac {\cot t}{\pm {\sqrt {1+\cot ^{2}t}}}}={\frac {-ma}{\pm {\sqrt {m^{2}a^{2}+b^{2}}}}}\ ,\quad \quad \sin t={\frac {1}{\pm {\sqrt {1+\cot ^{2}t}}}}={\frac {b}{\pm {\sqrt {m^{2}a^{2}+b^{2}}}}}.}$$

 

Replacing ${\displaystyle \cos t}$  and ${\displaystyle \sin t}$  of the standard representation yields:

$${\displaystyle {\vec {c}}_{\pm }(m)=\left(-{\frac {ma^{2}}{\pm {\sqrt {m^{2}a^{2}+b^{2}}}}},\;{\frac {b^{2}}{\pm {\sqrt {m^{2}a^{2}+b^{2}}}}}\right),\,m\in \mathbb {R} .}$$

 

Here ${\displaystyle m}$  is the slope of the tangent at the corresponding ellipse point, ${\displaystyle {\vec {c}}_{+}}$  is the upper and ${\displaystyle {\vec {c}}_{-}}$  the lower half of the ellipse. The vertices${\displaystyle (\pm a,\,0)}$ , having vertical tangents, are not covered by the representation.

The equation of the tangent at point ${\displaystyle {\vec {c}}_{\pm }(m)}$  has the form ${\displaystyle y=mx+n}$ . The still unknown ${\displaystyle n}$  can be determined by inserting the coordinates of the corresponding ellipse point ${\displaystyle {\vec {c}}_{\pm }(m)}$ :

$${\displaystyle y=mx\pm {\sqrt {m^{2}a^{2}+b^{2}}}\,.}$$

 

This description of the tangents of an ellipse is an essential tool for the determination of the orthoptic of an ellipse. The orthoptic article contains another proof, without differential calculus and trigonometric formulae.

General ellipse

 

Another definition of an ellipse uses affine transformations:

Any ellipse is an affine image of the unit circle with equation ${\displaystyle x^{2}+y^{2}=1}$ .

Parametric representation

An affine transformation of the Euclidean plane has the form ${\displaystyle {\vec {x}}\mapsto {\vec {f}}\!_{0}+A{\vec {x}}}$ , where ${\displaystyle A}$  is a regular matrix (with non-zero determinant) and ${\displaystyle {\vec {f}}\!_{0}}$  is an arbitrary vector. If ${\displaystyle {\vec {f}}\!_{1},{\vec {f}}\!_{2}}$  are the column vectors of the matrix ${\displaystyle A}$ , the unit circle ${\displaystyle (\cos(t),\sin(t))}$ , ${\displaystyle 0\leq t\leq 2\pi }$ , is mapped onto the ellipse:

$${\displaystyle {\vec {x}}={\vec {p}}(t)={\vec {f}}\!_{0}+{\vec {f}}\!_{1}\cos t+{\vec {f}}\!_{2}\sin t\,.}$$

 

Here ${\displaystyle {\vec {f}}\!_{0}}$  is the center and ${\displaystyle {\vec {f}}\!_{1},\;{\vec {f}}\!_{2}}$  are the directions of two conjugate diameters, in general not perpendicular.

Vertices

The four vertices of the ellipse are ${\displaystyle {\vec {p}}(t_{0}),\;{\vec {p}}\left(t_{0}\pm {\tfrac {\pi }{2}}\right),\;{\vec {p}}\left(t_{0}+\pi \right)}$ , for a parameter ${\displaystyle t=t_{0}}$  defined by:

$${\displaystyle \cot(2t_{0})={\frac {{\vec {f}}\!_{1}^{\,2}-{\vec {f}}\!_{2}^{\,2}}{2{\vec {f}}\!_{1}\cdot {\vec {f}}\!_{2}}}.}$$

 

(If ${\displaystyle {\vec {f}}\!_{1}\cdot {\vec {f}}\!_{2}=0}$ , then ${\displaystyle t_{0}=0}$ .) This is derived as follows. The tangent vector at point ${\displaystyle {\vec {p}}(t)}$  is:

$${\displaystyle {\vec {p}}\,'(t)=-{\vec {f}}\!_{1}\sin t+{\vec {f}}\!_{2}\cos t\ .}$$

 

At a vertex parameter ${\displaystyle t=t_{0}}$ , the tangent is perpendicular to the major/minor axes, so:

$${\displaystyle 0={\vec {p}}'(t)\cdot \left({\vec {p}}(t)-{\vec {f}}\!_{0}\right)=\left(-{\vec {f}}\!_{1}\sin t+{\vec {f}}\!_{2}\cos t\right)\cdot \left({\vec {f}}\!_{1}\cos t+{\vec {f}}\!_{2}\sin t\right).}$$

 

Expanding and applying the identities ${\displaystyle \;\cos ^{2}t-\sin ^{2}t=\cos 2t,\ \ 2\sin t\cos t=\sin 2t\;}$  gives the equation for ${\displaystyle t=t_{0}\;.}$ 

Area

From Apollonios theorem (see below) one obtains:
The area of an ellipse ${\displaystyle \;{\vec {x}}={\vec {f}}_{0}+{\vec {f}}_{1}\cos t+{\vec {f}}_{2}\sin t\;}$  is

$${\displaystyle A=\pi \left|\det({\vec {f}}_{1},{\vec {f}}_{2})\right|.}$$

 

Semiaxes

With the abbreviations ${\displaystyle \;M={\vec {f}}_{1}^{2}+{\vec {f}}_{2}^{2},\ N=\left|\det({\vec {f}}_{1},{\vec {f}}_{2})\right|}$  the statements of Apollonios's theorem can be written as:

$${\displaystyle a^{2}+b^{2}=M,\quad ab=N\ .}$$

 

${\displaystyle a,b}$ 

$${\displaystyle {\begin{aligned}a&={\frac {1}{2}}({\sqrt {M+2N}}+{\sqrt {M-2N}})\\[1ex]b&={\frac {1}{2}}({\sqrt {M+2N}}-{\sqrt {M-2N}})\,.\end{aligned}}}$$

 

Implicit representation

Solving the parametric representation for ${\displaystyle \;\cos t,\sin t\;}$  by Cramer's rule and using ${\displaystyle \;\cos ^{2}t+\sin ^{2}t-1=0\;}$ , one obtains the implicit representation

$${\displaystyle \det {\left({\vec {x}}\!-\!{\vec {f}}\!_{0},{\vec {f}}\!_{2}\right)^{2}}+\det {\left({\vec {f}}\!_{1},{\vec {x}}\!-\!{\vec {f}}\!_{0}\right)^{2}}-\det {\left({\vec {f}}\!_{1},{\vec {f}}\!_{2}\right)^{2}}=0.}$$

 

Conversely: If the equation

${\displaystyle x^{2}+2cxy+d^{2}y^{2}-e^{2}=0\ ,}$  with ${\displaystyle \;d^{2}-c^{2}>0\;,}$ 

of an ellipse centered at the origin is given, then the two vectors

$${\displaystyle {\vec {f}}_{1}={e \choose 0},\quad {\vec {f}}_{2}={\frac {e}{\sqrt {d^{2}-c^{2}}}}{-c \choose 1}}$$

 

Example: For the ellipse with equation ${\displaystyle \;x^{2}+2xy+3y^{2}-1=0\;}$  the vectors are

$${\displaystyle {\vec {f}}_{1}={1 \choose 0},\quad {\vec {f}}_{2}={\frac {1}{\sqrt {2}}}{-1 \choose 1}.}$$

 

 

Rotated Standard ellipse

For ${\displaystyle {\vec {f}}_{0}={0 \choose 0},\;{\vec {f}}_{1}=a{\cos \theta \choose \sin \theta },\;{\vec {f}}_{2}=b{-\sin \theta \choose \;\cos \theta }}$  one obtains a parametric representation of the standard ellipse rotated by angle ${\displaystyle \theta }$ :

$${\displaystyle {\begin{aligned}x&=x_{\theta }(t)=a\cos \theta \cos t-b\sin \theta \sin t\,,\\y&=y_{\theta }(t)=a\sin \theta \cos t+b\cos \theta \sin t\,.\end{aligned}}}$$

 

Ellipse in space

The definition of an ellipse in this section gives a parametric representation of an arbitrary ellipse, even in space, if one allows ${\displaystyle {\vec {f}}\!_{0},{\vec {f}}\!_{1},{\vec {f}}\!_{2}}$  to be vectors in space.

Polar form relative to center

 

In polar coordinates, with the origin at the center of the ellipse and with the angular coordinate ${\displaystyle \theta }$  measured from the major axis, the ellipse's equation is^: 75

$${\displaystyle r(\theta )={\frac {ab}{\sqrt {(b\cos \theta )^{2}+(a\sin \theta )^{2}}}}={\frac {b}{\sqrt {1-(e\cos \theta )^{2}}}}}$$

 

${\displaystyle e}$ 

Polar form relative to focus

 

If instead we use polar coordinates with the origin at one focus, with the angular coordinate ${\displaystyle \theta =0}$  still measured from the major axis, the ellipse's equation is

$${\displaystyle r(\theta )={\frac {a(1-e^{2})}{1\pm e\cos \theta }}}$$

 

where the sign in the denominator is negative if the reference direction ${\displaystyle \theta =0}$  points towards the center (as illustrated on the right), and positive if that direction points away from the center.

The angle ${\displaystyle \theta }$  is called the true anomaly of the point. The numerator ${\displaystyle \ell =a(1-e^{2})}$  is the semi-latus rectum.

 

Each of the two lines parallel to the minor axis, and at a distance of ${\textstyle d={\frac {a^{2}}{c}}={\frac {a}{e}}}$  from it, is called a directrix of the ellipse (see diagram).

For an arbitrary point ${\displaystyle P}$  of the ellipse, the quotient of the distance to one focus and to the corresponding directrix (see diagram) is equal to the eccentricity:
$${\displaystyle {\frac {\left|PF_{1}\right|}{\left|Pl_{1}\right|}}={\frac {\left|PF_{2}\right|}{\left|Pl_{2}\right|}}=e={\frac {c}{a}}\ .}$$
 

The proof for the pair ${\displaystyle F_{1},l_{1}}$  follows from the fact that ${\textstyle \left|PF_{1}\right|^{2}=(x-c)^{2}+y^{2},\ \left|Pl_{1}\right|^{2}=\left(x-{\tfrac {a^{2}}{c}}\right)^{2}}$  and ${\displaystyle y^{2}=b^{2}-{\tfrac {b^{2}}{a^{2}}}x^{2}}$  satisfy the equation

$${\displaystyle \left|PF_{1}\right|^{2}-{\frac {c^{2}}{a^{2}}}\left|Pl_{1}\right|^{2}=0\,.}$$

 

The second case is proven analogously.

The converse is also true and can be used to define an ellipse (in a manner similar to the definition of a parabola):

For any point ${\displaystyle F}$  (focus), any line ${\displaystyle l}$  (directrix) not through ${\displaystyle F}$ , and any real number ${\displaystyle e}$  with ${\displaystyle 0$  the ellipse is the locus of points for which the quotient of the distances to the point and to the line is ${\displaystyle e,}$  that is:
$${\displaystyle E=\left\{P\ \left|\ {\frac {|PF|}{|Pl|}}=e\right.\right\}.}$$
 

The extension to ${\displaystyle e=0}$ , which is the eccentricity of a circle, is not allowed in this context in the Euclidean plane. However, one may consider the directrix of a circle to be the line at infinity in the projective plane.

(The choice ${\displaystyle e=1}$  yields a parabola, and if ${\displaystyle e>1}$ , a hyperbola.)

 

Proof

Let ${\displaystyle F=(f,\,0),\ e>0}$ , and assume ${\displaystyle (0,\,0)}$  is a point on the curve. The directrix ${\displaystyle l}$  has equation ${\displaystyle x=-{\tfrac {f}{e}}}$ . With ${\displaystyle P=(x,\,y)}$ , the relation ${\displaystyle |PF|^{2}=e^{2}|Pl|^{2}}$  produces the equations

${\displaystyle (x-f)^{2}+y^{2}=e^{2}\left(x+{\frac {f}{e}}\right)^{2}=(ex+f)^{2}}$  and ${\displaystyle x^{2}\left(e^{2}-1\right)+2xf(1+e)-y^{2}=0.}$ 

The substitution ${\displaystyle p=f(1+e)}$  yields

$${\displaystyle x^{2}\left(e^{2}-1\right)+2px-y^{2}=0.}$$

 

This is the equation of an ellipse (${\displaystyle e<1}$ ), or a parabola (${\displaystyle e=1}$ ), or a hyperbola (${\displaystyle e>1}$ ). All of these non-degenerate conics have, in common, the origin as a vertex (see diagram).

If ${\displaystyle e<1}$ , introduce new parameters ${\displaystyle a,\,b}$  so that ${\displaystyle 1-e^{2}={\tfrac {b^{2}}{a^{2}}},{\text{ and }}\ p={\tfrac {b^{2}}{a}}}$ , and then the equation above becomes

$${\displaystyle {\frac {(x-a)^{2}}{a^{2}}}+{\frac {y^{2}}{b^{2}}}=1\,,}$$

 

which is the equation of an ellipse with center ${\displaystyle (a,\,0)}$ , the x-axis as major axis, and the major/minor semi axis ${\displaystyle a,\,b}$ .

 

Construction of a directrix

Because of ${\displaystyle c\cdot {\tfrac {a^{2}}{c}}=a^{2}}$  point ${\displaystyle L_{1}}$  of directrix ${\displaystyle l_{1}}$  (see diagram) and focus ${\displaystyle F_{1}}$  are inverse with respect to the circle inversion at circle ${\displaystyle x^{2}+y^{2}=a^{2}}$  (in diagram green). Hence ${\displaystyle L_{1}}$  can be constructed as shown in the diagram. Directrix ${\displaystyle l_{1}}$  is the perpendicular to the main axis at point ${\displaystyle L_{1}}$ .

General ellipse

If the focus is ${\displaystyle F=\left(f_{1},\,f_{2}\right)}$  and the directrix ${\displaystyle ux+vy+w=0}$ , one obtains the equation

$${\displaystyle \left(x-f_{1}\right)^{2}+\left(y-f_{2}\right)^{2}=e^{2}{\frac {\left(ux+vy+w\right)^{2}}{u^{2}+v^{2}}}\ .}$$

 

(The right side of the equation uses the Hesse normal form of a line to calculate the distance ${\displaystyle |Pl|}$ .)

 

 

An ellipse possesses the following property:

The normal at a point ${\displaystyle P}$  bisects the angle between the lines ${\displaystyle {\overline {PF_{1}}},\,{\overline {PF_{2}}}}$ .

Proof

Because the tangent line is perpendicular to the normal, an equivalent statement is that the tangent is the external angle bisector of the lines to the foci (see diagram). Let ${\displaystyle L}$  be the point on the line ${\displaystyle {\overline {PF_{2}}}}$  with distance ${\displaystyle 2a}$  to the focus ${\displaystyle F_{2}}$ , where ${\displaystyle a}$  is the semi-major axis of the ellipse. Let line ${\displaystyle w}$  be the external angle bisector of the lines ${\displaystyle {\overline {PF_{1}}}}$  and ${\displaystyle {\overline {PF_{2}}}.}$  Take any other point ${\displaystyle Q}$  on ${\displaystyle w.}$  By the triangle inequality and the angle bisector theorem, ${\displaystyle 2a=\left|LF_{2}\right|<{}}$ ${\displaystyle \left|QF_{2}\right|+\left|QL\right|={}}$ ${\displaystyle \left|QF_{2}\right|+\left|QF_{1}\right|,}$  therefore ${\displaystyle Q}$  must be outside the ellipse. As this is true for every choice of ${\displaystyle Q,}$  ${\displaystyle w}$  only intersects the ellipse at the single point ${\displaystyle P}$  so must be the tangent line.

Application

The rays from one focus are reflected by the ellipse to the second focus. This property has optical and acoustic applications similar to the reflective property of a parabola (see whispering gallery).

Definition of conjugate diameters

 

A circle has the following property:

The midpoints of parallel chords lie on a diameter.

An affine transformation preserves parallelism and midpoints of line segments, so this property is true for any ellipse. (Note that the parallel chords and the diameter are no longer orthogonal.)

Definition

Two diameters ${\displaystyle d_{1},\,d_{2}}$  of an ellipse are conjugate if the midpoints of chords parallel to ${\displaystyle d_{1}}$  lie on ${\displaystyle d_{2}\ .}$ 

From the diagram one finds:

Two diameters ${\displaystyle {\overline {P_{1}Q_{1}}},\,{\overline {P_{2}Q_{2}}}}$  of an ellipse are conjugate whenever the tangents at ${\displaystyle P_{1}}$  and ${\displaystyle Q_{1}}$  are parallel to ${\displaystyle {\overline {P_{2}Q_{2}}}}$ .

Conjugate diameters in an ellipse generalize orthogonal diameters in a circle.

In the parametric equation for a general ellipse given above,

$${\displaystyle {\vec {x}}={\vec {p}}(t)={\vec {f}}\!_{0}+{\vec {f}}\!_{1}\cos t+{\vec {f}}\!_{2}\sin t,}$$

 

any pair of points ${\displaystyle {\vec {p}}(t),\ {\vec {p}}(t+\pi )}$  belong to a diameter, and the pair ${\displaystyle {\vec {p}}\left(t+{\tfrac {\pi }{2}}\right),\ {\vec {p}}\left(t-{\tfrac {\pi }{2}}\right)}$  belong to its conjugate diameter.

For the common parametric representation ${\displaystyle (a\cos t,b\sin t)}$  of the ellipse with equation ${\displaystyle {\tfrac {x^{2}}{a^{2}}}+{\tfrac {y^{2}}{b^{2}}}=1}$  one gets: The points

${\displaystyle (x_{1},y_{1})=(\pm a\cos t,\pm b\sin t)\quad }$  (signs: (+,+) or (−,−) )
${\displaystyle (x_{2},y_{2})=({\color {red}{\mp }}a\sin t,\pm b\cos t)\quad }$  (signs: (−,+) or (+,−) )
are conjugate and
${\displaystyle {\frac {x_{1}x_{2}}{a^{2}}}+{\frac {y_{1}y_{2}}{b^{2}}}=0\ .}$ 

In case of a circle the last equation collapses to ${\displaystyle x_{1}x_{2}+y_{1}y_{2}=0\ .}$ 

Theorem of Apollonios on conjugate diameters

 

 

For an ellipse with semi-axes ${\displaystyle a,\,b}$  the following is true:

Let ${\displaystyle c_{1}}$  and ${\displaystyle c_{2}}$  be halves of two conjugate diameters (see diagram) then
1. ${\displaystyle c_{1}^{2}+c_{2}^{2}=a^{2}+b^{2}}$ .
2. The triangle ${\displaystyle O,P_{1},P_{2}}$  with sides ${\displaystyle c_{1},\,c_{2}}$  (see diagram) has the constant area ${\textstyle A_{\Delta }={\frac {1}{2}}ab}$ , which can be expressed by ${\displaystyle A_{\Delta }={\tfrac {1}{2}}c_{2}d_{1}={\tfrac {1}{2}}c_{1}c_{2}\sin \alpha }$ , too. ${\displaystyle d_{1}}$  is the altitude of point ${\displaystyle P_{1}}$  and ${\displaystyle \alpha }$  the angle between the half diameters. Hence the area of the ellipse (see section metric properties) can be written as ${\displaystyle A_{el}=\pi ab=\pi c_{2}d_{1}=\pi c_{1}c_{2}\sin \alpha }$ .
3. The parallelogram of tangents adjacent to the given conjugate diameters has the ${\displaystyle {\text{Area}}_{12}=4ab\ .}$ 

Proof

Let the ellipse be in the canonical form with parametric equation

$${\displaystyle {\vec {p}}(t)=(a\cos t,\,b\sin t).}$$

 

The two points ${\textstyle {\vec {c}}_{1}={\vec {p}}(t),\ {\vec {c}}_{2}={\vec {p}}\left(t+{\frac {\pi }{2}}\right)}$  are on conjugate diameters (see previous section). From trigonometric formulae one obtains ${\displaystyle {\vec {c}}_{2}=(-a\sin t,\,b\cos t)^{\mathsf {T}}}$  and

$${\displaystyle \left|{\vec {c}}_{1}\right|^{2}+\left|{\vec {c}}_{2}\right|^{2}=\cdots =a^{2}+b^{2}\,.}$$

 

The area of the triangle generated by ${\displaystyle {\vec {c}}_{1},\,{\vec {c}}_{2}}$  is

$${\displaystyle A_{\Delta }={\tfrac {1}{2}}\det \left({\vec {c}}_{1},\,{\vec {c}}_{2}\right)=\cdots ={\tfrac {1}{2}}ab}$$

 

and from the diagram it can be seen that the area of the parallelogram is 8 times that of ${\displaystyle A_{\Delta }}$ . Hence

$${\displaystyle {\text{Area}}_{12}=4ab\,.}$$

 

 

For the ellipse ${\displaystyle {\tfrac {x^{2}}{a^{2}}}+{\tfrac {y^{2}}{b^{2}}}=1}$  the intersection points of orthogonal tangents lie on the circle ${\displaystyle x^{2}+y^{2}=a^{2}+b^{2}}$ .

This circle is called orthoptic or director circle of the ellipse (not to be confused with the circular directrix defined above).

 

Ellipses appear in descriptive geometry as images (parallel or central projection) of circles. There exist various tools to draw an ellipse. Computers provide the fastest and most accurate method for drawing an ellipse. However, technical tools (ellipsographs) to draw an ellipse without a computer exist. The principle of ellipsographs were known to Greek mathematicians such as Archimedes and Proklos.

If there is no ellipsograph available, one can draw an ellipse using an approximation by the four osculating circles at the vertices.

For any method described below, knowledge of the axes and the semi-axes is necessary (or equivalently: the foci and the semi-major axis). If this presumption is not fulfilled one has to know at least two conjugate diameters. With help of Rytz's construction the axes and semi-axes can be retrieved.

de La Hire's point construction

The following construction of single points of an ellipse is due to de La Hire. It is based on the standard parametric representation ${\displaystyle (a\cos t,\,b\sin t)}$  of an ellipse:

1. Draw the two circles centered at the center of the ellipse with radii ${\displaystyle a,b}$  and the axes of the ellipse.
2. Draw a line through the center, which intersects the two circles at point ${\displaystyle A}$  and ${\displaystyle B}$ , respectively.
3. Draw a line through ${\displaystyle A}$  that is parallel to the minor axis and a line through ${\displaystyle B}$  that is parallel to the major axis. These lines meet at an ellipse point (see diagram).
4. Repeat steps (2) and (3) with different lines through the center.